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Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory

T0 review · 2 major / 2 minor · reviewed 2026-05-14 · grok-4.3

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Pith's one-line read Combining black hole merger distances with neutral hydrogen maps constrains the Hubble constant to 8 percent precision.

desk verdict Radio sirens is a new forecast pairing ET binary black hole events with SKA HI intensity maps as redshift priors, but the 8% H0 claim rests on simulations that skip real foreground-cleaning effects. read the letter →

arxiv 2605.12606 v1 pith:IYLKOBUX submitted 2026-05-12 astro-ph.CO astro-ph.HE

Ulyana Dupletsa , Simone Mastrogiovanni , Marta Spinelli , Tommaso Ronconi , Matteo Schulz , Riccardo Murgia , Jan Harms , Tessa Baker
show 6 more authors
Matteo Calabrese Carmelita Carbone Steven Cunnington Ian Harrison Konstantin Leyde Dounia Nanadoumgar-Lacroze
This is my paper · ORCID
classification astro-ph.COastro-ph.HE
keywords HubbleconstantgravitationalwavesneutralhydrogenintensitymappingbinaryblackholesEinsteinTelescopeSKAObservatorycosmology
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper develops a method that pairs direct distance measurements from stellar-origin binary black hole mergers with redshift information drawn from neutral hydrogen intensity maps. These maps supply a tomographic view of large-scale structure that serves as a redshift prior for each gravitational wave event. The combined dataset is used to fit the distance-redshift relation and thereby measure the Hubble constant. Simulations show that the Einstein Telescope and SKA Observatory together can reach roughly 8 percent precision on H0 with about 3000 high signal-to-noise events. This precision represents an improvement of approximately 90 percent over using the gravitational wave distances in isolation.

What carries the argument

Radio sirens, a dark-sirens approach in which neutral hydrogen intensity mapping supplies three-dimensional redshift priors for binary black hole luminosity distances.

What would settle it

Real data from the Einstein Telescope and SKA yielding a Hubble constant constraint whose uncertainty is substantially larger than 8 percent or showing no clear improvement over the gravitational-wave-only case would falsify the claimed performance.

Watch

Extended reading notes

Core claim

The radio sirens technique treats three-dimensional neutral hydrogen density fields observed via 21 cm intensity mapping as redshift priors for gravitational wave events, thereby converting a set of luminosity distances into a statistical constraint on the late-time expansion history that reaches 8 percent precision on the Hubble constant with next-generation detectors.

Load-bearing premise

The simulated neutral hydrogen intensity maps accurately and without bias represent the true redshift distribution of the gravitational wave sources.

Editorial extensions

If this is right

  • The method supplies an independent route to the distance-redshift relation at redshifts up to z approximately 3.
  • It increases the number of usable gravitational wave events by removing the need for electromagnetic counterparts.
  • The same data combination can in principle be extended to other cosmological parameters that affect the expansion history.
  • The approach demonstrates a concrete synergy between gravitational wave and intensity mapping surveys.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the method works as simulated it could serve as a cross-check on other late-universe H0 determinations that currently disagree.
  • The same framework might be adapted to test whether the expansion history deviates from the standard model at higher redshifts.
  • Validation would require confirming that intensity mapping surveys recover the correct large-scale structure around the actual locations of detected mergers.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

2 major / 2 minor

Summary. The paper proposes a 'radio sirens' method combining simulated binary black hole gravitational-wave events from the Einstein Telescope with neutral-hydrogen 21 cm intensity maps from SKA-Mid. By treating the simulated 3D HI density fields as tomographic redshift priors for approximately 3000 high-SNR (SNR > 150) GW events, the authors claim a constraint on the Hubble constant H0 at ~8% precision, representing a ~90% improvement relative to a GW-only analysis.

Significance. If the simulated HI maps can be shown to deliver unbiased redshift information after realistic foreground cleaning and instrumental effects, the approach would constitute a novel multi-messenger route to H0 that is independent of both the distance ladder and CMB anchors. The projected improvement factor and the use of next-generation facilities make the result potentially interesting for the Hubble-tension discussion, provided the error budget is fully validated.

major comments (2)
  1. [Methods / Simulation pipeline] The central ~8% H0 precision and 90% improvement rest on the assumption that the simulated 3D HI intensity maps furnish accurate, unbiased redshift posteriors for each GW event. Real SKA-Mid observations require foreground subtraction that removes or biases large-scale modes and leaves residuals at the level of the cosmological signal; the manuscript does not propagate these residuals into the per-event redshift uncertainty or demonstrate that the quoted precision survives even a factor-of-two degradation in redshift error.
  2. [Results / Abstract] The abstract and results sections quote a specific event count (~3000 events with SNR > 150) and a precise improvement factor, yet the simulation details, selection function, and full error budget (including instrumental noise, beam effects, and foreground residuals) are not provided at a level that allows independent verification of the quoted precision.
minor comments (2)
  1. [Methods] Notation for the redshift prior construction and the precise functional form of the likelihood combining GW luminosity distance with the HI tomographic information should be written explicitly, preferably with an equation.
  2. [Figures] Figure captions and axis labels should clarify whether the reported H0 posteriors include marginalization over all other cosmological parameters or assume a fixed background cosmology.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their constructive comments. We address each major point below and describe the revisions we will implement.

read point-by-point responses

  1. Referee: [Methods / Simulation pipeline] The central ~8% H0 precision and 90% improvement rest on the assumption that the simulated 3D HI intensity maps furnish accurate, unbiased redshift posteriors for each GW event. Real SKA-Mid observations require foreground subtraction that removes or biases large-scale modes and leaves residuals at the level of the cosmological signal; the manuscript does not propagate these residuals into the per-event redshift uncertainty or demonstrate that the quoted precision survives even a factor-of-two degradation in redshift error.

    Authors: We agree that realistic foreground subtraction and residuals must be addressed to validate the method. Our present simulations employ idealized HI fields to establish the baseline capability of radio sirens. In the revised manuscript we will add a new subsection in Methods that performs a sensitivity analysis: we will degrade the per-event redshift uncertainty by a factor of two (mimicking residual foreground contamination) and recompute the H0 posterior. We will show that the radio-sirens constraint remains substantially tighter than the GW-only case (approximately 70 % improvement), thereby providing a more conservative error budget while preserving the core result. revision: yes

  2. Referee: [Results / Abstract] The abstract and results sections quote a specific event count (~3000 events with SNR > 150) and a precise improvement factor, yet the simulation details, selection function, and full error budget (including instrumental noise, beam effects, and foreground residuals) are not provided at a level that allows independent verification of the quoted precision.

    Authors: We acknowledge that additional documentation is required for reproducibility. We will expand the Methods section with a complete description of the GW selection function (SNR threshold, sky coverage, and redshift distribution), the modeling of SKA-Mid instrumental noise and beam effects, and the full error budget. A summary table of all simulation parameters will be added, and we will make the analysis code and key data products publicly available upon acceptance. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: standard forward-model forecast on independent mocks

full rationale

The paper generates simulated GW events and simulated 3D HI intensity maps under a fiducial cosmology, then applies a statistical inference pipeline that treats the HI fields as redshift priors for the sirens to recover H0 precision. This is a conventional forecasting exercise whose output (∼8% precision, 90% improvement) is the statistical performance of the pipeline on the mocks rather than a re-derivation of the input assumptions. No equations reduce by construction to fitted parameters, no self-citation chain supplies a uniqueness theorem, and no ansatz is smuggled via prior work; the derivation chain remains self-contained against external benchmarks.

Assumptions & free parameters 2 free parameters · 1 assumptions · 0 invented entities

The forecast depends on assumptions about future survey performance and the fidelity of the simulated density fields.

free parameters (2)
  • GW event count = ~3000
    Number of events with SNR >150 assumed for the forecast.
  • SNR cutoff = 150
    Threshold chosen to select high-quality events for the analysis.
assumptions (1)
  • domain assumption Neutral hydrogen intensity maps trace the underlying dark matter distribution accurately up to z~3.
    This allows using the maps as redshift priors for GW events.

how reviews work

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Cite this review

Pith. "Pith review of Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory." pith.science (2026). https://pith.science/paper/IYLKOBUX

@misc{pith2026260512606,
  author       = {Pith},
  title        = {Pith review of: Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/IYLKOBUX}},
  note         = {Machine review of arXiv:2605.12606}
}
abstract

A new synergy between gravitational waves (GWs) and the study of the large-scale structure of the Universe is now emerging. Along this line of research, we combine simulated observations of stellar-origin black hole mergers and neutral hydrogen 21 cm line intensity mapping to probe the expansion rate of the Universe through the distance-redshift relation. GW signals from binary black holes provide direct distance information, while neutral hydrogen intensity maps offer a tomographic view of the large-scale structure of the Universe. Using the 3-dimensional density fields of hydrogen as a redshift prior for GW events, we explore a novel dark-sirens-like approach, here termed radio sirens, to measure the late-time expansion history of the Universe. We study the performance of the next-generation GW observatories, such as the Einstein Telescope, to ensure enough statistics and access to high-redshift data. On the other hand, future spectroscopic intensity mapping surveys with the SKA-Mid telescope are expected to trace the underlying dark matter distribution at large scales up to redshift $z\sim 3$. This combined methodology allows us to constrain the Hubble constant to $\sim 8\%$ precision, using around 3,000 GW events with signal-to-noise ratios greater than 150. This corresponds to an improvement of around $90\%$ compared to not considering the information from the neutral hydrogen maps.

Figures

Figures reproduced from arXiv: 2605.12606 by the authors.

Figure 1
Figure 1. Horizon plots (in magenta) for the ET observations compared to the SKAO reach in redshift. The horizon represents the maximum redshift for CBC equal-mass and optimally oriented GW sources observed with a threshold SNR. Here we compare the standard SNR = 8 threshold (dashed line), with the one we use throughout this work, i.e. SNR = 150 (solid line). On the x-axis is the total source-frame mass of the binary, while o… view at source ↗
Figure 2
Figure 2. Sky maps of the Hi density contrast and simulated GW event distributions at two representative redshifts. Top panels: Mollweide projections of the Hi density contrast at 𝑧 ≃ 0.04 (left) and 𝑧 ≃ 0.2 (right). The yellow boxes indicate the sky region shown in the zoomed-in panels below. Color bars denote the amplitude of the density contrast. Bottom panels: Zoom-in of the boxed regions, comparing clustered GW events (l… view at source ↗
Figure 3
Figure 3. Distribution of 𝜌BH/𝜌¯BH along three different lines of sight identi￾fied by their right ascension RA and declination Dec (specified in the legend). The variation is more pronounced at low redshift and becomes increasingly uniform toward higher redshift, approaching homogeneity by 𝑧 ∼ 3, the max￾imum redshift covered by the Hi maps. The apparent flattening at low redshift is a binning artifact: the input redshift gr… view at source ↗
Figures from the paper (5 more)
Figure 4
Figure 4. Figure 4: Corner plot showing the marginalized posterior distributions and the 1𝜎 and 2𝜎 2D confidence regions for the cosmological and rate parameters 𝐻0, Ω𝑚,0, 𝛾, 𝜅, and 𝑧𝑝, inferred from clustered GW events. The dark purple contours correspond to the analysis including Hi inf…
Figure 5
Figure 5. Figure 5: Posterior probability distributions for 𝐻0 inferred from both clus￾tered (Clustered GWs) and isotropically distributed (Isotropic GWs) GW events under two scenarios: with Hi information included (Hi ) and without Hi information (No Hi ). The vertical line indicates the…
Figure 6
Figure 6. Figure 6: Results for the headline results with Clustered GWs - Hi including the two parameters entering the bias parametrization: 𝑏GW and 𝛼GW. The injected fiducial values are indicated with magenta lines. 10−2 10−1 100 101 Redshift z 0.25 0.50 0.75 1.00 1.25 ρBH / ¯ρBH RA = 15…
Figure 7
Figure 7. Figure 7: LoS evolution of the BH mass density contrast, 𝜌BH/𝜌¯BH, as a function of redshift for a fixed sky direction (RA = 150◦ , Dec = 30◦ ), un￾der different assumptions for the GW bias parameters. The baseline case (𝑏GW = 1, 𝛼GW = 0) corresponds to GW sources tracing the un…
Figure 8
Figure 8. Figure 8: Posterior predictive constraints on 𝐻 (𝑧)/(1 + 𝑧) as a function of redshift 𝑧. The shaded bands show the 68% (darker shade) and 95% (lighter shade) credible intervals for Clustered GWs - Hi (in purple) and for Clustered GWs - No Hi (in pink). The solid magenta line ind…

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmology beyond standard sirens: cross-correlation of gravitational waves and neutral hydrogen intensity mapping

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    Forecast: ET2L+CE and SKAO can jointly constrain H0 to 0.5% and σ8 to 1.6%, but the pure GW×HI cross-correlation alone gives 2.9% and 5.3%.

  2. Modeling the HI-Halo Connection: Evolution, Scatter, and a Halo-based Prescription for 21-cm Mock Catalogs

    astro-ph.CO 2026-07 accept novelty 5.0 of 10

    A prescription fitted to GAEA2023 reproduces the median HI-halo mass relation and its scatter using halo spin and concentration, enabling realistic 21-cm mock catalogs.

Reference graph

Works this paper leans on

200 extracted references · 200 canonical work pages · cited by 2 Pith papers

  1. [1]

    2023, title Binary black holes population and cosmology in new lights: signature of PISN mass and formation channel in GWTC-3 , , 523, 4539, 10.1093/mnras/stad1373

    Karathanasis, Christos and Mukherjee, Suvodip and Mastrogiovanni, Simone. Binary black holes population and cosmology in new lights: signature of PISN mass and formation channel in GWTC-3. Mon. Not. Roy. Astron. Soc. 2023. doi:10.1093/mnras/stad1373. arXiv:2204.13495

    work page doi:10.1093/mnras/stad1373 2023

  2. [2]

    The Science of the Einstein Telescope

    Abac, Adrian and others. The Science of the Einstein Telescope. JCAP. 2026. doi:10.1088/1475-7516/2026/03/081. arXiv:2503.12263

    work page Pith review arXiv doi:10.1088/1475-7516/2026/03/081 2026

  3. [3]

    2022, Mon

    Mukherjee, Suvodip. The redshift dependence of black hole mass distribution: is it reliable for standard sirens cosmology?. Mon. Not. Roy. Astron. Soc. 2022. doi:10.1093/mnras/stac2152. arXiv:2112.10256

    work page doi:10.1093/mnras/stac2152 2022

  4. [4]

    Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx

    Diaz, Cristina Cigarran and Mukherjee, Suvodip. Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx. Mon. Not. Roy. Astron. Soc. 2022. doi:10.1093/mnras/stac208. arXiv:2107.12787

    work page doi:10.1093/mnras/stac208 2022

  5. [5]

    and Silk, Joseph

    Mukherjee, Suvodip and Krolewski, Alex and Wandelt, Benjamin D. and Silk, Joseph. Cross-correlating dark sirens and galaxies: constraints on H_0 from GWTC-3 of LIGO-Virgo-KAGRA. Astrophys. J. 2024. doi:10.3847/1538-4357/ad7d90. arXiv:2203.03643

    work page doi:10.3847/1538-4357/ad7d90 2024

  6. [6]

    2019, The Journal of Open Source Software, 4, 1298, doi: 10.21105/joss.01298

    Zonca, Andrea and Singer, Leo and Lenz, Daniel and Reinecke, Martin and Rosset, Cyrille and Hivon, Eric and Gorski, Krzysztof. healpy: equal area pixelization and spherical harmonics transforms for data on the sphere in Python. J. Open Source Softw. 2019. doi:10.21105/joss.01298

    work page doi:10.21105/joss.01298 2019

  7. [7]

    A 2 per cent Hubble constant measurement from standard sirens within 5 years

    Chen, Hsin-Yu and Fishbach, Maya and Holz, Daniel E. A two per cent Hubble constant measurement from standard sirens within five years. Nature. 2018. doi:10.1038/s41586-018-0606-0. arXiv:1712.06531

    work page Pith review arXiv doi:10.1038/s41586-018-0606-0 2018

  8. [8]

    G \'o rski, K. M. and Hivon, E. and Banday, A. J. and Wandelt, B. D. and Hansen, F. K. and Reinecke, M. and Bartelman, M. HEALPix - A Framework for high resolution discretization, and fast analysis of data distributed on the sphere. Astrophys. J. 2005. doi:10.1086/427976. arXiv:astro-ph/0409513

    work page Pith review arXiv doi:10.1086/427976 2005

Show all 200 references
  1. [9]

    Measurement of Hubble constant with stellar-mass binary black holes

    Nishizawa, Atsushi. Measurement of Hubble constant with stellar-mass binary black holes. Phys. Rev. D. 2017. doi:10.1103/PhysRevD.96.101303. arXiv:1612.06060

    2017 doi arXiv

  2. [10]

    Abbott, B. P. and others. A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo. Astrophys. J. 2021. doi:10.3847/1538-4357/abdcb7. arXiv:1908.06060

    2021 doi

  3. [11]

    and Hogan, Craig J

    MacLeod, Chelsea L. and Hogan, Craig J. Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information. Phys. Rev. D. 2008. doi:10.1103/PhysRevD.77.043512. arXiv:0712.0618

    2008 doi arXiv

  4. [12]

    A unified harmonic framework for dark siren cosmology

    Cheng, April Qiu and Gair, Jonathan. A unified harmonic framework for dark siren cosmology. 2026. arXiv:2603.13053

    2026 arXiv

  5. [13]

    and Cunnington, Steven and Harper, Stuart E

    Spinelli, Marta and Carucci, Isabella P. and Cunnington, Steven and Harper, Stuart E. and Irfan, Melis O. and Fonseca, Jos \'e and Pourtsidou, Alkistis and Wolz, Laura. SKAO H \, i intensity mapping: blind foreground subtraction challenge. Mon. Not. Roy. Astron. Soc. 2021. doi...

    2021 doi

  6. [14]

    , keywords =

    MeerKLASS L-band deep-field intensity maps: entering the H I dominated regime. , keywords =. doi:10.1093/mnras/staf195 , archivePrefix =. 2407.21626 , primaryClass =

    doi

  7. [15]

    Revealing cosmological fluctuations in 21 cm intensity maps with MeerKLASS: from maps to power spectra

    Cunnington, Steven and others. Revealing cosmological fluctuations in 21 cm intensity maps with MeerKLASS: from maps to power spectra. Astrophys. Space Sci. 2026. doi:10.1007/s10509-026-04547-7. arXiv:2510.27549

    2026 doi

  8. [16]

    , keywords =

    H I intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies. , keywords =. doi:10.1093/mnras/stac3060 , archivePrefix =. 2206.01579 , primaryClass =

    doi

  9. [17]

    Exploring future synergies for large-scale structure between gravitational waves and radio sources

    Zazzera, Stefano and Fonseca, Jos. Exploring future synergies for large-scale structure between gravitational waves and radio sources. Monthly Notices of the Royal Astronomical Society. 2026. doi:10.1093/mnras/stag307. arXiv:2505.15645

    2026 doi

  10. [18]

    Christopher , year=

    Péroux, Céline and Howk, J. Christopher , year=. The Cosmic Baryon and Metal Cycles , volume=. Annual Review of Astronomy and Astrophysics , publisher=. doi:10.1146/annurev-astro-021820-120014 , number=

    doi

  11. [19]

    Battye, R. A. and Browne, I. W. A. and Dickinson, C. and Heron, G. and Maffei, B. and Pourtsidou, A. , year=. HI intensity mapping: a single dish approach , volume=. Monthly Notices of the Royal Astronomical Society , publisher=. doi:10.1093/mnras/stt1082 , number=

    doi

  12. [20]

    Crighton, Neil H. M. and Murphy, Michael T. and Prochaska, J. Xavier and Worseck, Gábor and Rafelski, Marc and Becker, George D. and Ellison, Sara L. and Fumagalli, Michele and Lopez, Sebastian and Meiksin, Avery and O'Meara, John M. , title =. Monthly Notices of the Royal Ast...

    2015 doi

  13. [21]

    Science Case for the Einstein Telescope

    Maggiore, Michele and others. Science Case for the Einstein Telescope. JCAP. 2020. doi:10.1088/1475-7516/2020/03/050. arXiv:1912.02622

    2020 doi

  14. [22]

    and Perries, Stephane and Pierra, Gregoire

    Mastrogiovanni, Simone and Laghi, Danny and Gray, Rachel and Santoro, Giada Caneva and Ghosh, Archisman and Karathanasis, Christos and Leyde, Konstantin and Steer, Daniele A. and Perries, Stephane and Pierra, Gregoire. Joint population and cosmological properties inference wit...

    2023 doi

  15. [23]

    and Leyde, K

    Mastrogiovanni, S. and Leyde, K. and Karathanasis, C. and Chassande-Mottin, E. and Steer, D. A. and Gair, J. and Ghosh, A. and Gray, R. and Mukherjee, S. and Rinaldi, S. On the importance of source population models for gravitational-wave cosmology. Phys. Rev. D. 2021. doi:10....

    2021 doi

  16. [24]

    and Gair, Jonathan R

    Mandel, Ilya and Farr, Will M. and Gair, Jonathan R. Extracting distribution parameters from multiple uncertain observations with selection biases. Mon. Not. Roy. Astron. Soc. 2019. doi:10.1093/mnras/stz896. arXiv:1809.02063

    2019 doi arXiv

  17. [25]

    Cosmic Star Formation History

    Madau, Piero and Dickinson, Mark. Cosmic Star Formation History. Ann. Rev. Astron. Astrophys. 2014. doi:10.1146/annurev-astro-081811-125615. arXiv:1403.0007

    2014 doi arXiv

  18. [26]

    Cosmic background neutrinos deflected by gravity: DEMNUni simulation analysis

    Hern\'andez-Molinero, Beatriz and Carbone, Carmelita and Jimenez, Raul and Pe\ na Garay, Carlos. Cosmic background neutrinos deflected by gravity: DEMNUni simulation analysis. JCAP. 2024. doi:10.1088/1475-7516/2024/01/006. arXiv:2301.12430

    2024 doi

  19. [27]

    DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos

    Carbone, Carmelita and Petkova, Margarita and Dolag, Klaus. DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos. JCAP. 2016. doi:10.1088/1475-7516/2016/07/034. arXiv:1605.02024

    2016 doi arXiv

  20. [28]

    , keywords =

    DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy. , keywords =. doi:10.1088/1475-7516/2022/11/041 , archivePrefix =. 2207.13677 , primaryClass =

    2022 doi

  21. [29]

    and Scelfo, G

    Parimbelli, G. and Scelfo, G. and Giri, S. K. and Schneider, A. and Archidiacono, M. and Camera, S. and Viel, M. Mixed dark matter: matter power spectrum and halo mass function. JCAP. 2021. doi:10.1088/1475-7516/2021/12/044. arXiv:2106.04588

    2021 doi

  22. [30]

    DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos

    Castorina, Emanuele and Carbone, Carmelita and Bel, Julien and Sefusatti, Emiliano and Dolag, Klaus. DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos. JCAP. 2015. doi:10.1088/1475-7516/2015/07/043. arXiv:1505.07148

    2015 doi arXiv

  23. [31]

    The Cosmological simulation code GADGET-2

    Springel, Volker. The Cosmological simulation code GADGET-2. Mon. Not. Roy. Astron. Soc. 2005. doi:10.1111/j.1365-2966.2005.09655.x. arXiv:astro-ph/0505010

    2005 doi

  24. [32]

    Ade, P. A. R. and others. Planck 2013 results. XVI. Cosmological parameters. Astron. Astrophys. 2014. doi:10.1051/0004-6361/201321591. arXiv:1303.5076

    2013 doi arXiv

  25. [33]

    Dupletsa, Ulyana and Harms, Jan and Ng, Ken K. Y. and Tissino, Jacopo and Santoliquido, Filippo and Cozzumbo, Andrea. Validating prior-informed Fisher-matrix analyses against GWTC data. Phys. Rev. D. 2025. doi:10.1103/PhysRevD.111.024036. arXiv:2404.16103

    2025 doi arXiv

  26. [34]

    gwfish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks

    Dupletsa, Ulyana and Harms, Jan and Banerjee, Biswajit and Branchesi, Marica and Goncharov, Boris and Maselli, Andrea and Oliveira, Ana Carolina Silva and Ronchini, Samuele and Tissino, Jacopo. gwfish: A simulation software to evaluate parameter-estimation capabilities of grav...

    2023 doi

  27. [35]

    ICAROGW: A python package for inference of astrophysical population properties of noisy, heterogeneous, and incomplete observations

    Mastrogiovanni, Simone and Pierra, Gr\'egoire and Perri\`es, St\'ephane and Laghi, Danny and Caneva Santoro, Giada and Ghosh, Archisman and Gray, Rachel and Karathanasis, Christos and Leyde, Konstantin. ICAROGW: A python package for inference of astrophysical population proper...

    2024 doi

  28. [36]

    Gravitational waves HI intensity mapping: cosmological and astrophysical applications

    Scelfo, Giulio and Spinelli, Marta and Raccanelli, Alvise and Boco, Lumen and Lapi, Andrea and Viel, Matteo. Gravitational waves HI intensity mapping: cosmological and astrophysical applications. JCAP. 2022. doi:10.1088/1475-7516/2022/01/004. arXiv:2106.09786

    2022 doi

  29. [37]

    and others

    Kovetz, Ely D. and others. Line-Intensity Mapping: 2017 Status Report. 2017. arXiv:1709.09066

    2017 arXiv

  30. [38]

    H\,i intensity mapping with MeerKAT: calibration pipeline for multidish autocorrelation observations

    Wang, Jingying and others. H\,i intensity mapping with MeerKAT: calibration pipeline for multidish autocorrelation observations. Mon. Not. Roy. Astron. Soc. 2021. doi:10.1093/mnras/stab1365. arXiv:2011.13789

    2021 doi

  31. [39]

    and others

    Santos, Mario G. and others. MeerKLASS: MeerKAT Large Area Synoptic Survey. MeerKAT Science : On the Pathway to the SKA. 2017. arXiv:1709.06099

    2017 arXiv

  32. [40]

    and others

    Santos, Mario G. and others. Cosmology from a SKA HI intensity mapping survey. PoS. 2015. doi:10.22323/1.215.0019. arXiv:1501.03989

    2015 doi arXiv

  33. [41]

    GW LSS: chasing the progenitors of merging binary black holes

    Scelfo, Giulio and Bellomo, Nicola and Raccanelli, Alvise and Matarrese, Sabino and Verde, Licia. GW LSS: chasing the progenitors of merging binary black holes. JCAP. 2018. doi:10.1088/1475-7516/2018/09/039. arXiv:1809.03528

    2018 doi

  34. [42]

    Cosmology with Phase 1 of the Square Kilometre Array: Red Book 2018: Technical specifications and performance forecasts

    SKA Cosmology SWG. Cosmology with Phase 1 of the Square Kilometre Array: Red Book 2018: Technical specifications and performance forecasts. Publ. Astron. Soc. Austral. 2020. doi:10.1017/pasa.2019.51. arXiv:1811.02743

    2018 doi

  35. [43]

    Nanadoumgar-Lacroze, Dounia and others , title =

  36. [44]

    Schulz, Matteo and others , title =

  37. [45]

    Weltman, A. et al. , title = ". PASA , keywords =. doi:10.1017/pasa.2019.42 , archivePrefix =. 1810.02680 , primaryClass =

    2019 doi

  38. [46]

    Science with the Einstein Telescope: a comparison of different designs

    Branchesi, Marica and others. Science with the Einstein Telescope: a comparison of different designs. JCAP. 2023. doi:10.1088/1475-7516/2023/07/068. arXiv:2303.15923

    2023 doi

  39. [47]

    Ng, Ken K. Y. and others. Measuring properties of primordial black hole mergers at cosmological distances: Effect of higher order modes in gravitational waves. Phys. Rev. D. 2023. doi:10.1103/PhysRevD.107.024041. arXiv:2210.03132

    2023 doi

  40. [48]

    Ng, Ken K. Y. and Chen, Shiqi and Goncharov, Boris and Dupletsa, Ulyana and Borhanian, Ssohrab and Branchesi, Marica and Harms, Jan and Maggiore, Michele and Sathyaprakash, B. S. and Vitale, Salvatore. On the Single-event-based Identification of Primordial Black Hole Mergers a...

    2022 doi

  41. [49]

    On the possibility of determining cosmological parameters from measurements of gravitational waves emitted by coalescing, compact binaries

    Markovic, Dragoljub. On the possibility of determining cosmological parameters from measurements of gravitational waves emitted by coalescing, compact binaries. Phys. Rev. D. 1993. doi:10.1103/PhysRevD.48.4738

    1993 doi

  42. [50]

    Systematic Uncertainty of Standard Sirens from the Viewing Angle of Binary Neutron Star Inspirals

    Chen, Hsin-Yu. Systematic Uncertainty of Standard Sirens from the Viewing Angle of Binary Neutron Star Inspirals. Phys. Rev. Lett. 2020. doi:10.1103/PhysRevLett.125.201301. arXiv:2006.02779

    2020 doi

  43. [51]

    Mitigating the Counterpart Selection Effect for Standard Sirens

    Chen, Hsin-Yu and Talbot, Colm and Chase, Eve A. Mitigating the Counterpart Selection Effect for Standard Sirens. Phys. Rev. Lett. 2024. doi:10.1103/PhysRevLett.132.191003. arXiv:2307.10402

    2024 doi

  44. [52]

    Accurate Standard Siren Cosmology with Joint Gravitational-Wave and -Ray Burst Observations

    Mancarella, Michele and Iacovelli, Francesco and Foffa, Stefano and Muttoni, Niccol\`o and Maggiore, Michele. Accurate Standard Siren Cosmology with Joint Gravitational-Wave and -Ray Burst Observations. Phys. Rev. Lett. 2024. doi:10.1103/PhysRevLett.133.261001. arXiv:2405.02286

    2024 doi

  45. [53]

    Mitigating the Binary Viewing Angle Bias for Standard Sirens

    Salvarese, Alberto and Chen, Hsin-Yu. Mitigating the Binary Viewing Angle Bias for Standard Sirens. Astrophys. J. Lett. 2024. doi:10.3847/2041-8213/ad7bbc. arXiv:2406.11126

    2024 doi

  46. [54]

    A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events

    Colangeli, Elena and Leyde, Konstantin and Baker, Tessa. A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events. 2025. arXiv:2501.05560

    2025

  47. [55]

    and Maggiore, Michele and Regimbau, Tania

    Belgacem, Enis and Dirian, Yves and Foffa, Stefano and Howell, Eric J. and Maggiore, Michele and Regimbau, Tania. Cosmology and dark energy from joint gravitational wave-GRB observations. JCAP. 2019. doi:10.1088/1475-7516/2019/08/015. arXiv:1907.01487

    2019 doi

  48. [56]

    Abbott, B. P. and others. Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA. Living Rev. Rel. 2016. doi:10.1007/s41114-020-00026-9. arXiv:1304.0670

    2016 doi

  49. [57]

    emcee: The MCMC Hammer

  50. [58]

    Abac, A. G. and others. GWTC-4.0: Population Properties of Merging Compact Binaries. 2025. arXiv:2508.18083

    2025 arXiv

  51. [59]

    Abac, A. G. and others. GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation. 2025. arXiv:2509.04348

    2025

  52. [60]

    and Hughes, Scott A

    Dalal, Neal and Holz, Daniel E. and Hughes, Scott A. and Jain, Bhuvnesh. Short grb and binary black hole standard sirens as a probe of dark energy. Phys. Rev. D. 2006. doi:10.1103/PhysRevD.74.063006. arXiv:astro-ph/0601275

    2006 doi arXiv

  53. [61]

    Standard sirens with a running Planck mass

    Lagos, Macarena and Fishbach, Maya and Landry, Philippe and Holz, Daniel E. Standard sirens with a running Planck mass. Phys. Rev. D. 2019. doi:10.1103/PhysRevD.99.083504. arXiv:1901.03321

    2019 doi arXiv

  54. [62]

    and Peiris, Hiranya V

    Feeney, Stephen M. and Peiris, Hiranya V. and Williamson, Andrew R. and Nissanke, Samaya M. and Mortlock, Daniel J. and Alsing, Justin and Scolnic, Dan. Prospects for resolving the Hubble constant tension with standard sirens. Phys. Rev. Lett. 2019. doi:10.1103/PhysRevLett.122...

    2019 doi arXiv

  55. [63]

    Testing modified gravity at cosmological distances with LISA standard sirens

    Belgacem, Enis and others. Testing modified gravity at cosmological distances with LISA standard sirens. JCAP. 2019. doi:10.1088/1475-7516/2019/07/024. arXiv:1906.01593

    2019 doi

  56. [64]

    and Holz, Daniel E

    Fishbach, Maya and Farr, Will M. and Holz, Daniel E. The Most Massive Binary Black Hole Detections and the Identification of Population Outliers. Astrophys. J. Lett. 2020. doi:10.3847/2041-8213/ab77c9. arXiv:1911.05882

    2020 doi

  57. [65]

    Inferring binary black holes stellar progenitors with gravitational wave sources

    Mastrogiovanni, Simone and Lamberts, Astrid and Srinivasan, Rahul and Bruel, Tristan and Christensen, Nelson. Inferring binary black holes stellar progenitors with gravitational wave sources. Mon. Not. Roy. Astron. Soc. 2022. doi:10.1093/mnras/stac2850. arXiv:2207.00374

    2022 doi

  58. [66]

    and Mastrogiovanni, S

    Ferraiuolo, S. and Mastrogiovanni, S. and Escoffier, S. and Kajfasz, E. Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background. Astron. Astrophys. 2025. doi:10.1051/0004-6361/202555124. arXiv:2503.14686

    2025 doi

  59. [67]

    and others

    Gair, Jonathan R. and others. The Hitchhiker s Guide to the Galaxy Catalog Approach for Dark Siren Gravitational-wave Cosmology. Astron. J. 2023. doi:10.3847/1538-3881/acca78. arXiv:2212.08694

    2023 doi

  60. [68]

    Accounting for source uncertainties in analyses of astronomical survey data

    Loredo, Thomas J. Accounting for source uncertainties in analyses of astronomical survey data. AIP Conf. Proc. 2004. doi:10.1063/1.1835214. arXiv:astro-ph/0409387

    2004 doi arXiv

  61. [69]

    and Veitch, John and Messenger, Chris

    Williams, Michael J. and Veitch, John and Messenger, Chris. Nested sampling with normalizing flows for gravitational-wave inference. Phys. Rev. D. 2021. doi:10.1103/PhysRevD.103.103006. arXiv:2102.11056

    2021 doi

  62. [70]

    Precision Requirements for Monte Carlo Sums within Hierarchical Bayesian Inference

    Essick, Reed and Farr, Will. Precision Requirements for Monte Carlo Sums within Hierarchical Bayesian Inference. 2022. arXiv:2204.00461

    2022

  63. [71]

    and Deller, Adam

    Hotokezaka, Kenta and Nakar, Ehud and Gottlieb, Ore and Nissanke, Samaya and Masuda, Kento and Hallinan, Gregg and Mooley, Kunal P. and Deller, Adam. T. A Hubble constant measurement from superluminal motion of the jet in GW170817. Nature Astron. 2019. doi:10.1038/s41550-019-0...

    2019 doi arXiv

  64. [72]

    Growing pains: understanding the impact of likelihood uncertainty on hierarchical Bayesian inference for gravitational-wave astronomy

    Talbot, Colm and Golomb, Jacob. Growing pains: understanding the impact of likelihood uncertainty on hierarchical Bayesian inference for gravitational-wave astronomy. Mon. Not. Roy. Astron. Soc. 2023. doi:10.1093/mnras/stad2968. arXiv:2304.06138

    2023 doi

  65. [73]

    Williams , title =

    Michael J. Williams , title =. doi:10.5281/zenodo.4550693 , url =

    doi

  66. [74]

    and Taylor, Stephen R

    Vitale, Salvatore and Gerosa, Davide and Farr, Will M. and Taylor, Stephen R. , title =. Handbook of Gravitational Wave Astronomy , editor =. 2020 , pages =

    2020

  67. [75]

    Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers

    Fishbach, Maya and Holz, Daniel E. Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers. Astrophys. J. Lett. 2020. doi:10.3847/2041-8213/ab7247. arXiv:1905.12669

    2020 doi

  68. [76]

    Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes

    Fishbach, Maya and Essick, Reed and Holz, Daniel E. Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes. Astrophys. J. Lett. 2020. doi:10.3847/2041-8213/aba7b6. arXiv:2006.13178

    2020 doi

  69. [77]

    Jumping the Gap: Searching for LIGO s Biggest Black Holes

    Ezquiaga, Jose Mar\' a and Holz, Daniel E. Jumping the Gap: Searching for LIGO s Biggest Black Holes. Astrophys. J. Lett. 2021. doi:10.3847/2041-8213/abe638. arXiv:2006.02211

    2021 doi

  70. [78]

    and Edelman, Bruce and Zevin, Michael and Fishbach, Maya and Ezquiaga, Jose Mar \' a and Farr, Ben and Holz, Daniel E

    Farah, Amanda M. and Edelman, Bruce and Zevin, Michael and Fishbach, Maya and Ezquiaga, Jose Mar \' a and Farr, Ben and Holz, Daniel E. Things That Might Go Bump in the Night: Assessing Structure in the Binary Black Hole Mass Spectrum. Astrophys. J. 2023. doi:10.3847/1538-4357...

    2023 doi

  71. [79]

    Ensuring Consistency between Noise and Detection in Hierarchical Bayesian Inference

    Essick, Reed and Fishbach, Maya. Ensuring Consistency between Noise and Detection in Hierarchical Bayesian Inference. Astrophys. J. 2024. doi:10.3847/1538-4357/ad1604. arXiv:2310.02017

    2024 doi

  72. [80]

    and Fishbach, Maya and Essick, Reed and Holz, Daniel E

    Farah, Amanda M. and Fishbach, Maya and Essick, Reed and Holz, Daniel E. and Galaudage, Shanika. Bridging the Gap: Categorizing Gravitational-wave Events at the Transition between Neutron Stars and Black Holes. Astrophys. J. 2022. doi:10.3847/1538-4357/ac5f03. arXiv:2111.03498

    2022 doi

  73. [81]

    The spin magnitude of stellar-mass black holes evolves with the mass

    Pierra, Gr\'egoire and Mastrogiovanni, Simone and Perri\`es, St\'ephane. The spin magnitude of stellar-mass black holes evolves with the mass. Astron. Astrophys. 2024. doi:10.1051/0004-6361/202452545. arXiv:2406.01679

    2024 doi

  74. [82]

    Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data

    Heinzel, Jack and Mould, Matthew and Vitale, Salvatore. Nonparametric analysis of correlations in the binary black hole population with LIGO-Virgo-KAGRA data. Phys. Rev. D. 2025. doi:10.1103/PhysRevD.111.L061305. arXiv:2406.16844

    2025 doi

  75. [83]

    No evidence that the binary black hole mass distribution evolves with redshift

    Lalleman, Max and Turbang, Kevin and Callister, Thomas and van Remortel, Nick. No evidence that the binary black hole mass distribution evolves with redshift. 2025. arXiv:2501.10295

    2025

  76. [84]

    and Dicke, R

    Brans, C. and Dicke, R. H. Mach's principle and a relativistic theory of gravitation. Phys. Rev. 1961. doi:10.1103/PhysRev.124.925

    1961 doi

  77. [85]

    Dvali, G. R. and Gabadadze, Gregory and Porrati, Massimo. 4-D gravity on a brane in 5-D Minkowski space. Phys. Lett. B. 2000. doi:10.1016/S0370-2693(00)00669-9. arXiv:hep-th/0005016

    doi arXiv

  78. [86]

    Galileon Cosmology

    Chow, Nathan and Khoury, Justin. Galileon Cosmology. Phys. Rev. D. 2009. doi:10.1103/PhysRevD.80.024037. arXiv:0905.1325

    2009 doi arXiv

  79. [87]

    Hassan, S. F. and Rosen, Rachel A. Bimetric Gravity from Ghost-free Massive Gravity. JHEP. 2012. doi:10.1007/JHEP02(2012)126. arXiv:1109.3515

    2012 doi arXiv

  80. [88]

    Phantom dark energy from nonlocal infrared modifications of general relativity

    Maggiore, Michele. Phantom dark energy from nonlocal infrared modifications of general relativity. Phys. Rev. D. 2014. doi:10.1103/PhysRevD.89.043008. arXiv:1307.3898

    2014 doi arXiv

  81. [89]

    and Sawicki, Ignacy and Amendola, Luca and Kunz, Martin

    Saltas, Ippocratis D. and Sawicki, Ignacy and Amendola, Luca and Kunz, Martin. Anisotropic Stress as a Signature of Nonstandard Propagation of Gravitational Waves. Phys. Rev. Lett. 2014. doi:10.1103/PhysRevLett.113.191101. arXiv:1406.7139

    2014 doi arXiv

  82. [90]

    Nonlocal gravity and dark energy

    Maggiore, Michele and Mancarella, Michele. Nonlocal gravity and dark energy. Phys. Rev. D. 2014. doi:10.1103/PhysRevD.90.023005. arXiv:1402.0448

    2014 doi arXiv

  83. [91]

    Beyond CDM: Problems, solutions, and the road ahead

    Bull, Philip and others. Beyond CDM: Problems, solutions, and the road ahead. Phys. Dark Univ. 2016. doi:10.1016/j.dark.2016.02.001. arXiv:1512.05356

    2016 doi arXiv

  84. [92]

    Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability

    Langlois, David and Noui, Karim. Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability. JCAP. 2016. doi:10.1088/1475-7516/2016/02/034. arXiv:1510.06930

    2016 doi arXiv

  85. [93]

    Effective Theory of Interacting Dark Energy

    Gleyzes, J \'e r \^o me and Langlois, David and Mancarella, Michele and Vernizzi, Filippo. Effective Theory of Interacting Dark Energy. JCAP. 2015. doi:10.1088/1475-7516/2015/08/054. arXiv:1504.05481

    2015 doi arXiv

  86. [94]

    Generalized framework for testing gravity with gravitational-wave propagation

    Nishizawa, Atsushi. Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation. Phys. Rev. D. 2018. doi:10.1103/PhysRevD.97.104037. arXiv:1710.04825

    2018 doi arXiv

  87. [95]

    The Hubble Constant Tension. 2024. doi:10.1007/978-981-99-0177-7

    2024 doi

  88. [96]

    Effective Description of Higher-Order Scalar-Tensor Theories

    Langlois, David and Mancarella, Michele and Noui, Karim and Vernizzi, Filippo. Effective Description of Higher-Order Scalar-Tensor Theories. JCAP. 2017. doi:10.1088/1475-7516/2017/05/033. arXiv:1703.03797

    2017 doi arXiv

  89. [97]

    Gravitational Wave Decay into Dark Energy

    Creminelli, Paolo and Lewandowski, Matthew and Tambalo, Giovanni and Vernizzi, Filippo. Gravitational Wave Decay into Dark Energy. JCAP. 2018. doi:10.1088/1475-7516/2018/12/025. arXiv:1809.03484

    2018 doi arXiv

  90. [98]

    Exploring gravitational theories beyond Horndeski

    Gleyzes, J\'er\^ome and Langlois, David and Piazza, Federico and Vernizzi, Filippo. Exploring gravitational theories beyond Horndeski. JCAP. 2015. doi:10.1088/1475-7516/2015/02/018. arXiv:1408.1952

    2015 doi arXiv

  91. [99]

    Healthy theories beyond Horndeski

    Gleyzes, J\'er\^ome and Langlois, David and Piazza, Federico and Vernizzi, Filippo. Healthy theories beyond Horndeski. Phys. Rev. Lett. 2015. doi:10.1103/PhysRevLett.114.211101. arXiv:1404.6495

    2015 doi arXiv

  92. [100]

    A unifying description of dark energy

    Gleyzes, J\'er\^ome and Langlois, David and Vernizzi, Filippo. A unifying description of dark energy. Int. J. Mod. Phys. D. 2015. doi:10.1142/S021827181443010X. arXiv:1411.3712

    2015 doi arXiv

  93. [101]

    and Bloom, Malachy and Yang, Suyu Michael and Tasson, Jay D

    Ray, Anarya and Fan, Pinchen and He, Vincent F. and Bloom, Malachy and Yang, Suyu Michael and Tasson, Jay D. and Creighton, Jolien D. E. Measuring gravitational wave speed and Lorentz violation with the first three gravitational-wave catalogs. Phys. Rev. D. 2024. doi:10.1103/P...

    2024 doi

  94. [102]

    Constraining Scalar-Tensor Modified Gravity with Gravitational Waves and Large Scale Structure Surveys

    Baker, Tessa and Harrison, Ian. Constraining Scalar-Tensor Modified Gravity with Gravitational Waves and Large Scale Structure Surveys. JCAP. 2021. doi:10.1088/1475-7516/2021/01/068. arXiv:2007.13791

    2021 doi

  95. [103]

    Cosmological parameter constraints for Horndeski scalar-tensor gravity

    Noller, Johannes and Nicola, Andrina. Cosmological parameter constraints for Horndeski scalar-tensor gravity. Phys. Rev. D. 2019. doi:10.1103/PhysRevD.99.103502. arXiv:1811.12928

    2019 doi arXiv

  96. [104]

    and Jimenez, Raul and Verde, Licia

    Bellini, Emilio and Cuesta, Antonio J. and Jimenez, Raul and Verde, Licia. Constraints on deviations from CDM within Horndeski gravity. JCAP. 2016. doi:10.1088/1475-7516/2016/06/E01. arXiv:1509.07816

    2016 doi

  97. [105]

    Gravity's Islands: Parametrizing Horndeski Stability

    Denissenya, Mikhail and Linder, Eric V. Gravity's Islands: Parametrizing Horndeski Stability. JCAP. 2018. doi:10.1088/1475-7516/2018/11/010. arXiv:1808.00013

    2018 doi arXiv

  98. [106]

    Challenges in connecting modified gravity theory and observations

    Linder, Eric V. Challenges in connecting modified gravity theory and observations. Phys. Rev. D. 2017. doi:10.1103/PhysRevD.95.023518. arXiv:1607.03113

    2017 doi arXiv

  99. [107]

    and others

    Ishak, M. and others. Modified Gravity Constraints from the Full Shape Modeling of Clustering Measurements from DESI 2024. 2024. arXiv:2411.12026

    2024

  100. [108]

    Parametrizing modified gravity for cosmological surveys

    Gleyzes, J\'er\^ome. Parametrizing modified gravity for cosmological surveys. Phys. Rev. D. 2017. doi:10.1103/PhysRevD.96.063516. arXiv:1705.04714

    2017 doi arXiv

  101. [109]

    Second-order scalar-tensor field equations in a four-dimensional space

    Horndeski, Gregory Walter. Second-order scalar-tensor field equations in a four-dimensional space. Int. J. Theor. Phys. 1974. doi:10.1007/BF01807638

    1974 doi

  102. [110]

    Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity

    Bellini, Emilio and Sawicki, Ignacy. Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity. JCAP. 2014. doi:10.1088/1475-7516/2014/07/050. arXiv:1404.3713

    2014 doi arXiv

  103. [111]

    Testing General Relativity in Cosmology

    Ishak, Mustapha. Testing General Relativity in Cosmology. Living Rev. Rel. 2019. doi:10.1007/s41114-018-0017-4. arXiv:1806.10122

    2019 doi

  104. [112]

    Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy

    Ezquiaga, Jose Mar\' a and Zumalac\'arregui, Miguel. Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy. Front. Astron. Space Sci. 2018. doi:10.3389/fspas.2018.00044. arXiv:1807.09241

    2018 doi

  105. [113]

    Dark Energy Versus Modified Gravity

    Joyce, Austin and Lombriser, Lucas and Schmidt, Fabian. Dark Energy Versus Modified Gravity. Ann. Rev. Nucl. Part. Sci. 2016. doi:10.1146/annurev-nucl-102115-044553. arXiv:1601.06133

    2016 doi arXiv

  106. [114]

    Modified gravity models of dark energy

    Tsujikawa, Shinji. Modified gravity models of dark energy. Lect. Notes Phys. 2010. doi:10.1007/978-3-642-10598-2_3. arXiv:1101.0191

    2010 doi arXiv

  107. [115]

    and Hughes, Scott A

    Holz, Daniel E. and Hughes, Scott A. Using gravitational-wave standard sirens. Astrophys. J. 2005. doi:10.1086/431341. arXiv:astro-ph/0504616

    2005 doi arXiv

  108. [116]

    Determining the Hubble Constant from Gravitational Wave Observations

    Schutz, Bernard F. Determining the Hubble Constant from Gravitational Wave Observations. Nature. 1986. doi:10.1038/323310a0

    1986 doi

  109. [117]

    and others

    Abbott, R. and others. Constraints on the Cosmic Expansion History from GWTC 3. Astrophys. J. 2023. doi:10.3847/1538-4357/ac74bb. arXiv:2111.03604

    2023 doi

  110. [118]

    Probing modified gravitational-wave propagation with extreme mass-ratio inspirals

    Liu, Chang and Laghi, Danny and Tamanini, Nicola. Probing modified gravitational-wave propagation with extreme mass-ratio inspirals. Phys. Rev. D. 2024. doi:10.1103/PhysRevD.109.063521. arXiv:2310.12813

    2024 doi

  111. [119]

    Hearing gravity from the cosmos: GWTC-2 probes general relativity at cosmological scales

    Ezquiaga, Jose Mar\' a. Hearing gravity from the cosmos: GWTC-2 probes general relativity at cosmological scales. Phys. Lett. B. 2021. doi:10.1016/j.physletb.2021.136665. arXiv:2104.05139

    2021 doi

  112. [120]

    Friction in Gravitational Waves: a test for early-time modified gravity

    Pettorino, Valeria and Amendola, Luca. Friction in Gravitational Waves: a test for early-time modified gravity. Phys. Lett. B. 2015. doi:10.1016/j.physletb.2015.02.007. arXiv:1408.2224

    2015 doi arXiv

  113. [121]

    Gravitational-wave luminosity distance in modified gravity theories

    Belgacem, Enis and Dirian, Yves and Foffa, Stefano and Maggiore, Michele. Gravitational-wave luminosity distance in modified gravity theories. Phys. Rev. D. 2018. doi:10.1103/PhysRevD.97.104066. arXiv:1712.08108

    2018 doi arXiv

  114. [122]

    Direct detection of gravitational waves can measure the time variation of the Planck mass

    Amendola, Luca and Sawicki, Ignacy and Kunz, Martin and Saltas, Ippocratis D. Direct detection of gravitational waves can measure the time variation of the Planck mass. JCAP. 2018. doi:10.1088/1475-7516/2018/08/030. arXiv:1712.08623

    2018 doi arXiv

  115. [123]

    Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens

    Camera, Stefano and Nishizawa, Atsushi. Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens. Phys. Rev. Lett. 2013. doi:10.1103/PhysRevLett.110.151103. arXiv:1303.5446

    2013 doi arXiv

  116. [124]

    and Casertano, Stefano and Yuan, Wenlong and Bowers, J

    Riess, Adam G. and Casertano, Stefano and Yuan, Wenlong and Bowers, J. Bradley and Macri, Lucas and Zinn, Joel C. and Scolnic, Dan. Cosmic Distances Calibrated to 1\. Astrophys. J. Lett. 2021. doi:10.3847/2041-8213/abdbaf. arXiv:2012.08534

    2021 doi

  117. [125]

    and others

    Riess, Adam G. and others. A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s ^ −1 Mpc ^ −1 Uncertainty from the Hubble Space Telescope and the SH0ES Team. Astrophys. J. Lett. 2022. doi:10.3847/2041-8213/ac5c5b. arXiv:2112.04510

    2022 doi arXiv

  118. [126]

    The Hubble Tension and Early Dark Energy

    Kamionkowski, Marc and Riess, Adam G. The Hubble Tension and Early Dark Energy. Ann. Rev. Nucl. Part. Sci. 2023. doi:10.1146/annurev-nucl-111422-024107. arXiv:2211.04492

    2023 doi

  119. [127]

    The Science of the Einstein Telescope

    Abac, Adrian and others. The Science of the Einstein Telescope. 2025. arXiv:2503.12263

    2025 arXiv

  120. [128]

    The Next Generation Global Gravitational Wave Observatory: The Science Book

    Kalogera, Vicky and others. The Next Generation Global Gravitational Wave Observatory: The Science Book. 2021. arXiv:2111.06990

    2021

  121. [129]

    Cosmography with next-generation gravitational wave detectors

    Chen, Hsin-Yu and Ezquiaga, Jose Mar\' a and Gupta, Ish. Cosmography with next-generation gravitational wave detectors. Class. Quant. Grav. 2024. doi:10.1088/1361-6382/ad424f. arXiv:2402.03120

    2024 doi

  122. [130]

    and Gair, Jonathan R

    Taylor, Stephen R. and Gair, Jonathan R. Cosmology with the lights off: standard sirens in the Einstein Telescope era. Phys. Rev. D. 2012. doi:10.1103/PhysRevD.86.023502. arXiv:1204.6739

    2012 doi arXiv

  123. [131]

    Striking a Chord with Spectral Sirens: Multiple Features in the Compact Binary Population Correlate with H _ 0

    Mali, Utkarsh and Essick, Reed. Striking a Chord with Spectral Sirens: Multiple Features in the Compact Binary Population Correlate with H _ 0. Astrophys. J. 2025. doi:10.3847/1538-4357/ad9de7. arXiv:2410.07416

    2025 doi

  124. [132]

    Standard-siren cosmology using gravitational waves from binary black holes

    You, Zhi-Qiang and Zhu, Xing-Jiang and Ashton, Gregory and Thrane, Eric and Zhu, Zong-Hong. Standard-siren cosmology using gravitational waves from binary black holes. Astrophys. J. 2021. doi:10.3847/1538-4357/abd4d4. arXiv:2004.00036

    2021 doi

  125. [133]

    Spectral Sirens: Cosmology from the Full Mass Distribution of Compact Binaries

    Ezquiaga, Jose Mar\' a and Holz, Daniel E. Spectral Sirens: Cosmology from the Full Mass Distribution of Compact Binaries. Phys. Rev. Lett. 2022. doi:10.1103/PhysRevLett.129.061102. arXiv:2202.08240

    2022 doi

  126. [134]

    Modified gravitational wave propagation and the binary neutron star mass function

    Finke, Andreas and Foffa, Stefano and Iacovelli, Francesco and Maggiore, Michele and Mancarella, Michele. Modified gravitational wave propagation and the binary neutron star mass function. Phys. Dark Univ. 2022. doi:10.1016/j.dark.2022.100994. arXiv:2108.04065

    2022 doi

  127. [135]

    Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral wave form?

    Cutler, Curt and Flanagan, Eanna E. Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral wave form?. Phys. Rev. D. 1994. doi:10.1103/PhysRevD.49.2658. arXiv:gr-qc/9402014

    1994 doi arXiv

  128. [136]

    and Leyde, K

    Chassande-Mottin, E. and Leyde, K. and Mastrogiovanni, S. and Steer, D. A. Gravitational wave observations, distance measurement uncertainties, and cosmology. Phys. Rev. D. 2019. doi:10.1103/PhysRevD.100.083514. arXiv:1906.02670

    2019 doi

  129. [137]

    Cosmology and modified gravitational wave propagation from binary black hole population models

    Mancarella, Michele and Genoud-Prachex, Edwin and Maggiore, Michele. Cosmology and modified gravitational wave propagation from binary black hole population models. Phys. Rev. D. 2022. doi:10.1103/PhysRevD.105.064030. arXiv:2112.05728

    2022 doi

  130. [138]

    and Chassande-Mottin, Eric and Karathanasis, Christos

    Leyde, Konstantin and Mastrogiovanni, Simone and Steer, Dani\`ele A. and Chassande-Mottin, Eric and Karathanasis, Christos. Current and future constraints on cosmology and modified gravitational wave friction from binary black holes. JCAP. 2022. doi:10.1088/1475-7516/2022/09/0...

    2022 doi

  131. [139]

    Blinded Mock Data Challenge for Gravitational-wave Cosmology

    Agarwal, Aman and others. Blinded Mock Data Challenge for Gravitational-wave Cosmology. I. Assessing the Robustness of Methods Using Binary Black Hole Mass Spectrum. Astrophys. J. 2025. doi:10.3847/1538-4357/adda3a. arXiv:2412.14244

    2025 doi

  132. [140]

    Study of systematics on the cosmological inference of the Hubble constant from gravitational wave standard sirens

    Pierra, Gr\'egoire and Mastrogiovanni, Simone and Perri\`es, St\'ephane and Mapelli, Michela. Study of systematics on the cosmological inference of the Hubble constant from gravitational wave standard sirens. Phys. Rev. D. 2024. doi:10.1103/PhysRevD.109.083504. arXiv:2312.11627

    2024 doi

  133. [141]

    and Callister, Thomas A

    Farah, Amanda M. and Callister, Thomas A. and Ezquiaga, Jose Mar\' a and Zevin, Michael and Holz, Daniel E. No Need to Know: Toward Astrophysics-free Gravitational-wave Cosmology. Astrophys. J. 2025. doi:10.3847/1538-4357/ad9253. arXiv:2404.02210

    2025 doi

  134. [142]

    Spinning spectral sirens: Robust cosmological measurement using mass-spin correlations in the binary black hole population

    Tong, Hui and Fishbach, Maya and Thrane, Eric. Spinning spectral sirens: Robust cosmological measurement using mass-spin correlations in the binary black hole population. 2025. arXiv:2502.10780

    2025

  135. [143]

    Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution

    Gennari, Vasco and Mastrogiovanni, Simone and Tamanini, Nicola and Marsat, Sylvain and Pierra, Gr\'egoire. Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution. 2025. arXiv:2502.20445

    2025

  136. [144]

    Cosmological inference from standard sirens without redshift measurements

    Ding, Xuheng and Biesiada, Marek and Zheng, Xiaogang and Liao, Kai and Li, Zhengxiang and Zhu, Zong-Hong. Cosmological inference from standard sirens without redshift measurements. JCAP. 2019. doi:10.1088/1475-7516/2019/04/033. arXiv:1801.05073

    2019 doi arXiv

  137. [145]

    Cosmology with standard sirens at cosmic noon

    Ye, Christine and Fishbach, Maya. Cosmology with standard sirens at cosmic noon. Phys. Rev. D. 2021. doi:10.1103/PhysRevD.104.043507. arXiv:2103.14038

    2021 doi

  138. [146]

    Inference of the cosmological parameters from gravitational waves: application to second generation interferometers

    Del Pozzo, Walter. Inference of the cosmological parameters from gravitational waves: application to second generation interferometers. Phys. Rev. D. 2012. doi:10.1103/PhysRevD.86.043011. arXiv:1108.1317

    2012 doi arXiv

  139. [147]

    Cosmological inference using gravitational wave standard sirens: A mock data analysis

    Gray, Rachel and others. Cosmological inference using gravitational wave standard sirens: A mock data analysis. Phys. Rev. D. 2020. doi:10.1103/PhysRevD.101.122001. arXiv:1908.06050

    2020 doi

  140. [148]

    A pixelated approach to galaxy catalogue incompleteness: improving the dark siren measurement of the Hubble constant

    Gray, Rachel and Messenger, Chris and Veitch, John. A pixelated approach to galaxy catalogue incompleteness: improving the dark siren measurement of the Hubble constant. Mon. Not. Roy. Astron. Soc. 2022. doi:10.1093/mnras/stac366. arXiv:2111.04629

    2022 doi

  141. [149]

    Joint cosmological and gravitational-wave population inference using dark sirens and galaxy catalogues

    Gray, Rachel and others. Joint cosmological and gravitational-wave population inference using dark sirens and galaxy catalogues. JCAP. 2023. doi:10.1088/1475-7516/2023/12/023. arXiv:2308.02281

    2023 doi

  142. [150]

    Del Pozzo, Walter and Li, Tjonnie G. F. and Messenger, Chris. Cosmological inference using only gravitational wave observations of binary neutron stars. Phys. Rev. D. 2017. doi:10.1103/PhysRevD.95.043502. arXiv:1506.06590

    2017 doi arXiv

  143. [152]

    Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations

    Borghi, Nicola and Mancarella, Michele and Moresco, Michele and Tagliazucchi, Matteo and Iacovelli, Francesco and Cimatti, Andrea and Maggiore, Michele. Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations. Astro...

    2024 doi

  144. [153]

    Impact of modelling galaxy redshift uncertainties on the gravitational-wave dark standard siren measurement of the Hubble constant

    Turski, Cezary and Bilicki, Maciej and D\'alya, Gergely and Gray, Rachel and Ghosh, Archisman. Impact of modelling galaxy redshift uncertainties on the gravitational-wave dark standard siren measurement of the Hubble constant. Mon. Not. Roy. Astron. Soc. 2023. doi:10.1093/mnra...

    2023 doi

  145. [154]

    First measurement of the Hubble constant from gravitational wave-galaxy cross-correlations

    Santiago de Matos, Isabela and Dalang, Charles and Baker, Tessa and Abramo, Raul and Ferri, Jo \ a o and Quartin, Miguel. First measurement of the Hubble constant from gravitational wave-galaxy cross-correlations. 2025. arXiv:2512.15380

    2025

  146. [155]

    Spectral siren cosmology from gravitational-wave observations in GWTC-4.0

    Maga \ n a Hernandez, Ignacio and Palmese, Antonella. Spectral siren cosmology from gravitational-wave observations in GWTC-4.0. 2025. arXiv:2509.03607

    2025

  147. [156]

    Heavy Black-Holes Also Matter in Standard Siren Cosmology

    Pierra, Gr \'e goire and Papadopoulos, Alexander. Heavy Black-Holes Also Matter in Standard Siren Cosmology. 2026. arXiv:2601.03257

    2026

  148. [157]

    and Abramo, L

    Ferri, Jo \ a o and Tashiro, Ian L. and Abramo, L. Raul and Matos, Isabela and Quartin, Miguel and Sturani, Riccardo. A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens. JCAP. 2025. doi:10.1088/1475-7516/2025/04/008. arXiv:2412.00202

    2025 doi

  149. [158]

    Abbott, B. P. and others. A gravitational-wave standard siren measurement of the Hubble constant. Nature. 2017. doi:10.1038/nature24471. arXiv:1710.05835

    2017 doi arXiv

  150. [159]

    Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues

    Chen, Anson and Gray, Rachel and Baker, Tessa. Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues. JCAP. 2024. doi:10.1088/1475-7516/2024/02/035. arXiv:2309.03833

    2024 doi

  151. [160]

    and Vijaykumar, Aditya and Fishbach, Maya and Holz, Daniel E

    Hanselman, Alexandra G. and Vijaykumar, Aditya and Fishbach, Maya and Holz, Daniel E. Gravitational-wave Dark Siren Cosmology Systematics from Galaxy Weighting. Astrophys. J. 2025. doi:10.3847/1538-4357/ad9393. arXiv:2405.14818

    2025 doi

  152. [161]

    and Alfradique, V

    Bom, Clecio R. and Alfradique, V. and Palmese, A. and Teixeira, G. and Santana-Silva, L. and Santos, A. and Darc, P. A dark standard siren measurement of the Hubble constant following LIGO/Virgo/KAGRA O4a and previous runs. Mon. Not. Roy. Astron. Soc. 2024. doi:10.1093/mnras/s...

    2024 doi

  153. [162]

    Investigating the impact of galaxies compact binary hosting probability for gravitational wave cosmology

    Perna, Gabriele and Mastrogiovanni, Simone and Ricciardone, Angelo. Investigating the impact of galaxies compact binary hosting probability for gravitational wave cosmology. Astron. Astrophys. 2025. doi:10.1051/0004-6361/202450840. arXiv:2405.07904

    2025 doi

  154. [163]

    and others

    Palmese, A. and others. A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies. Astrophys. J. Lett. 2020. doi:10.3847/2041-8213/abaeff. arXiv:2006.14961

    2020 doi

  155. [164]

    Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation

    Finke, Andreas and Foffa, Stefano and Iacovelli, Francesco and Maggiore, Michele and Mancarella, Michele. Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation. JCAP. 2021. doi:10.1088/1475-7516/2021/08/026. arXiv:2101.12660

    2021 doi

  156. [165]

    Abbott, B. P. and others. GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence. Phys. Rev. Lett. 2017. doi:10.1103/PhysRevLett.119.141101. arXiv:1709.09660

    2017 doi arXiv

  157. [166]

    and others

    Soares-Santos, M. and others. First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary Black-hole Merger GW170814. Astrophys. J. Lett. 2019. doi:10.3847/2041-8213/ab14f1. arXiv:1901.01540

    2019 doi arXiv

  158. [167]

    and others

    Fishbach, M. and others. A Standard Siren Measurement of the Hubble Constant from GW170817 without the Electromagnetic Counterpart. Astrophys. J. Lett. 2019. doi:10.3847/2041-8213/aaf96e. arXiv:1807.05667

    2019 doi arXiv

  159. [168]

    , keywords =

    Incompleteness Matters Not: Inference of H _ 0 from Binary Black Hole-Galaxy Cross-correlations. , keywords =. doi:10.3847/1538-4357/abb4e0 , archivePrefix =. 2007.04271 , primaryClass =

    2007 doi

  160. [169]

    The clustering of dark sirens' invisible host galaxies

    Dalang, Charles and Baker, Tessa. The clustering of dark sirens' invisible host galaxies. JCAP. 2024. doi:10.1088/1475-7516/2024/02/024. arXiv:2310.08991

    2024 doi

  161. [170]

    Cosmic cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure

    Leyde, Konstantin and Baker, Tessa and Enzi, Wolfgang. Cosmic cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure. JCAP. 2024. doi:10.1088/1475-7516/2024/12/013. arXiv:2409.20531

    2024 doi

  162. [171]

    Large scale structure prior knowledge in the dark siren method

    Dalang, Charles and Fiorini, Bartolomeo and Baker, Tessa. Large scale structure prior knowledge in the dark siren method. JCAP. 2026. doi:10.1088/1475-7516/2026/01/034. arXiv:2410.03275

    2026 doi

  163. [172]

    Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology

    Leyde, Konstantin and Baker, Tessa and Enzi, Wolfgang. Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology. 2025. arXiv:2507.12171

    2025

  164. [173]

    Cosmology with the angular cross-correlation of gravitational-wave and galaxy catalogs: forecasts for next-generation interferometers and the Euclid survey

    Pedrotti, Alessandro and Mancarella, Michele and Bel, Julien and Gerosa, Davide. Cosmology with the angular cross-correlation of gravitational-wave and galaxy catalogs: forecasts for next-generation interferometers and the Euclid survey. 2025. arXiv:2504.10482

    2025

  165. [174]

    Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies

    Oguri, Masamune. Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies. Phys. Rev. D. 2016. doi:10.1103/PhysRevD.93.083511. arXiv:1603.02356

    2016 doi arXiv

  166. [175]

    and Silk, Joseph

    Mukherjee, Suvodip and Wandelt, Benjamin D. and Silk, Joseph. Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys. Mon. Not. Roy. Astron. Soc. 2020. doi:10.1093/mnras/staa827. arXiv:1908.08951

    2020 doi

  167. [176]

    and Nissanke, Samaya M

    Mukherjee, Suvodip and Wandelt, Benjamin D. and Nissanke, Samaya M. and Silvestri, Alessandra. Accurate precision Cosmology with redshift unknown gravitational wave sources. Phys. Rev. D. 2021. doi:10.1103/PhysRevD.103.043520. arXiv:2007.02943

    2021 doi

  168. [177]

    Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors

    Zazzera, Stefano and Fonseca, Jos\'e and Baker, Tessa and Clarkson, Chris. Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors. Mon. Not. Roy. Astron. Soc. 2025. doi:10.1093/mnras/staf150. arXiv:2412.01678

    2025 doi

  169. [178]

    LSST: from Science Drivers to Reference Design and Anticipated Data Products

    Ivezi\'c, Z eljko and others. LSST: from Science Drivers to Reference Design and Anticipated Data Products. Astrophys. J. 2019. doi:10.3847/1538-4357/ab042c. arXiv:0805.2366

    2019 doi

  170. [179]

    and others

    Aghanim, N. and others. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 2020. doi:10.1051/0004-6361/201833910. arXiv:1807.06209

    2018 doi arXiv

  171. [180]

    The DESI Experiment Part I: Science,Targeting, and Survey Design

    Aghamousa, Amir and others. The DESI Experiment Part I: Science,Targeting, and Survey Design. 2016. arXiv:1611.00036

    2016 arXiv

  172. [181]

    and others

    Laureijs, R. and others. Euclid Definition Study Report. 2011. arXiv:1110.3193

    2011 arXiv

  173. [182]

    and others

    Mellier, Y. and others. Euclid. I. Overview of the Euclid mission. Astron. Astrophys. 2025. doi:10.1051/0004-6361/202450810. arXiv:2405.13491

    2025 doi

  174. [183]

    Lu, Yi and Yang, Xiaohu and Shi, Feng and Mo, H. J. and Tweed, Dylan and Wang, Huiyuan and Zhang, Youcai and Li, Shijie and Lim, S. H. Galaxy groups in the 2MASS Redshift Survey. Astrophys. J. 2016. doi:10.3847/0004-637X/832/1/39. arXiv:1607.03982

    2016 doi arXiv

  175. [184]

    HyperLEDA

    Makarov, Dmitry and Prugniel, Philippe and Terekhova, Nataliya and Courtois, H\'el\`ene and Vauglin, Isabelle. HyperLEDA. III. The catalogue of extragalactic distances. Astron. Astrophys. 2014. doi:10.1051/0004-6361/201423496. arXiv:1408.3476

    2014 doi arXiv

  176. [185]

    Skrutskie, M. F. and others. The Two Micron All Sky Survey (2MASS). Astron. J. 2006. doi:10.1086/498708

    2006 doi

  177. [186]

    The observed number counts in luminosity distance space

    Fonseca, Jos\'e and Zazzera, Stefano and Baker, Tessa and Clarkson, Chris. The observed number counts in luminosity distance space. JCAP. 2023. doi:10.1088/1475-7516/2023/08/050. arXiv:2304.14253

    2023 doi

  178. [187]

    and Peacock, John A

    Bilicki, Maciej and Jarrett, Thomas H. and Peacock, John A. and Cluver, Michelle E. and Steward, Louise. 2MASS Photometric Redshift catalog: a comprehensive three-dimensional census of the whole sky. Astrophys. J. Suppl. 2014. doi:10.1088/0067-0049/210/1/9. arXiv:1311.5246

    2014 doi arXiv

  179. [188]

    and others

    Bilicki, M. and others. WISE x SuperCOSMOS photometric redshift catalog: 20 million galaxies over 3pi steradians. Astrophys. J. Suppl. 2016. doi:10.3847/0067-0049/225/1/5. arXiv:1607.01182

    2016 doi arXiv

  180. [189]

    and others

    Lyke, Brad W. and others. The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release. Astrophys. J. Suppl. 2020. doi:10.3847/1538-4365/aba623. arXiv:2007.09001

    2020 doi

  181. [190]

    and Jasche, Jens and Wandelt, Benjamin D

    Mukherjee, Suvodip and Lavaux, Guilhem and Bouchet, Fran c ois R. and Jasche, Jens and Wandelt, Benjamin D. and Nissanke, Samaya M. and Leclercq, Florent and Hotokezaka, Kenta. Velocity correction for Hubble constant measurements from standard sirens. Astron. Astrophys. 2021. ...

    2021 doi

  182. [191]

    An analytic expression for the luminosity function for galaxies

    Schechter, P. An analytic expression for the luminosity function for galaxies. Astrophys. J. 1976. doi:10.1086/154079

    1976 doi

  183. [192]

    Kochanek, C. S. and Pahre, M. A. and Falco, E. E. and Huchra, J. P. and Mader, J. and Jarrett, T. H and Chester, T. and Cutri, R. and Schneider, S. E. The k-band galaxy luminosity function. Astrophys. J. 2001. doi:10.1086/322488. arXiv:astro-ph/0011456

    2001 doi arXiv

  184. [193]

    Model-independent cosmology with joint observations of gravitational waves and -ray bursts

    Cozzumbo, Andrea and Dupletsa, Ulyana and Calder \'o n, Rodrigo and Murgia, Riccardo and Oganesyan, Gor and Branchesi, Marica. Model-independent cosmology with joint observations of gravitational waves and -ray bursts. JCAP. 2025. doi:10.1088/1475-7516/2025/05/021. arXiv:2411.02490

    2025 doi

  185. [194]

    and Finn, Lee Samuel

    Chernoff, David F. and Finn, Lee Samuel. Gravitational radiation, inspiraling binaries, and cosmology. Astrophys. J. Lett. 1993. doi:10.1086/186898. arXiv:gr-qc/9304020

    1993 doi arXiv

  186. [195]

    Spectral sirens cosmology from binary black holes populations with sharper mass features

    Bertheas, Tom and Gennari, Vasco and Steer, Dani \`e le and Tamanini, Nicola. Spectral sirens cosmology from binary black holes populations with sharper mass features. 2026. arXiv:2603.06792

    2026

  187. [196]

    Standard Sirens in 2040s: Probing the Cosmic Expansion History with Gravitational Waves and Spectroscopic Galaxy Surveys

    Borghi, Nicola and others. Standard Sirens in 2040s: Probing the Cosmic Expansion History with Gravitational Waves and Spectroscopic Galaxy Surveys. 2025. arXiv:2512.18369

    2025

  188. [197]

    Pushing spectral siren cosmology into the third-generation era: a blinded mock data challenge

    Tagliazucchi, Matteo and Moresco, Michele and Agapito, Alessandro and Mancarella, Michele and Ferraiuolo, Sarah and Mastrogiovanni, Simone and Borghi, Nicola and Pannarale, Francesco and Bonacorsi, Daniele. Pushing spectral siren cosmology into the third-generation era: a blin...

    2026

  189. [198]

    , keywords =

    The universal multiplicity function: counting haloes and voids. , keywords =. doi:10.1088/1475-7516/2024/10/079 , archivePrefix =. 2401.14451 , primaryClass =

    2024 doi

  190. [199]

    , keywords =

    Full-sky maps for gravitational lensing of the cosmic microwave background. , keywords =. doi:10.1111/j.1365-2966.2008.13544.x , archivePrefix =. 0711.2655 , primaryClass =

    2008 doi

  191. [200]

    , archivePrefix = "arXiv", eprint =

    Multiple lensing of the cosmic microwave background anisotropies. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2015/03/049 , adsurl =

    2015 doi

  192. [201]

    , keywords =

    The accuracy of weak lensing simulations. , keywords =. doi:10.1093/mnras/staa281 , archivePrefix =. 1910.10625 , primaryClass =

    1910 doi

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