Pith. sign in

REVIEW 2 major objections 2 minor 82 references

An extreme ram-pressure stripping event in a protocluster at redshift 4.3

T0 review · 2 major / 2 minor · reviewed 2026-06-27 · grok-4.3

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

Pith's one-line read Ram-pressure stripping removes more than half the cold gas from a massive galaxy in a protocluster at redshift 4.3.

desk verdict The paper reports a 6-kpc gas-star offset and >50% displaced gas in a z=4.3 protocluster galaxy, but the case that this is ram-pressure stripping rather than a merger or projection effect is not yet solid. read the letter →

arxiv 2606.18229 v1 pith:XI5X4R77 submitted 2026-06-16 astro-ph.GA

Dazhi Zhou , Scott C. Chapman , Manuel Aravena , Roger Deane , Anthony H. Gonzalez , Ryley Hill , Nicholas LeVar , Matthew A. Malkan
show 11 more authors
Adam Muzzin Nan Zhang Kedar A. Phadke Vismaya R. Pillai Manuel Solimano Justin S. Spilker Nikolaus Sulzenauer Joaquin D. Vieira David Vizgan George C. P. Wang Axel Weiss
This is my paper · ORCID
classification astro-ph.GA
keywords ram-pressurestrippingprotoclustergalaxyquenchinghigh-redshiftgalaxiescoldgasenvironmentaleffectsALMAJWST
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 reports ALMA and JWST observations of galaxy C26 inside the SPT2349-56 protocluster at z=4.30. It shows a 6-kpc spatial offset between the peak of the gas emission and the stellar body, with the displaced gas amounting to more than half of the observed cold-gas reservoir. This is presented as evidence that ram-pressure stripping can operate efficiently enough to remove most cold gas from massive galaxies even in the dynamically young cores of protoclusters at z>4. A sympathetic reader would care because the result supplies a concrete hydrodynamic mechanism for environmental quenching at epochs when such effects were previously thought to be negligible compared with gravitational interactions.

What carries the argument

Ram-pressure stripping (RPS), the hydrodynamic process in which a galaxy moving through a dense hot medium experiences pressure that removes its interstellar gas and leaves trailing wakes.

What would settle it

High-resolution kinematic maps or deeper imaging that show the displaced gas remains gravitationally bound to the stellar body or exhibits merger-driven velocity gradients would falsify the ram-pressure interpretation.

Watch

Extended reading notes

Core claim

The central claim is that SPT2349-56-C26 exhibits an extreme active-stripping phase in which ram-pressure stripping has displaced more than half of the galaxy's cold-gas reservoir and produced a 6-kpc offset between the gas-emission peak and the stellar body. The observations therefore demonstrate that hydrodynamic stripping can remove most of the cold gas from massive galaxies inside dense protocluster cores as early as z=4.3, supplying a direct pathway for environmental quenching at z>4.

Load-bearing premise

The observed 6-kpc offset and the large displaced gas fraction are produced by ram-pressure stripping rather than by gravitational interactions, mergers, or projection effects inside the protocluster.

Editorial extensions

If this is right

  • Ram-pressure stripping supplies a viable hydrodynamic route for quenching star formation in massive galaxies at z>4.
  • Environmental quenching mechanisms can already operate inside protocluster cores before the hot atmospheres of mature clusters have fully assembled.
  • The fraction of cold gas that can be removed by RPS at z=4.3 is large enough to affect the subsequent star-formation history of the galaxy.
  • Similar extreme stripping events may be detectable in other high-redshift protoclusters with current ALMA and JWST sensitivity.

Reading between the lines

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

  • If RPS operates this efficiently at z=4.3, models of galaxy evolution may need to include hydrodynamic gas removal in dense environments at earlier epochs than previously assumed.
  • The same mechanism could produce observable gas tails or offsets in other massive galaxies within the same protocluster or in comparable structures at z>4.
  • Repeated stripping events over cosmic time could contribute to the buildup of the intracluster medium at high redshift.
Share X Bluesky LinkedIn Reddit HN

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 manuscript reports ALMA and JWST observations of galaxy SPT2349-56-C26 in the SPT2349-56 protocluster at z=4.30. It identifies a 6-kpc spatial offset between the gas-emission peak and stellar body together with a displaced gas mass fraction exceeding 50% of the cold-gas reservoir, which the authors interpret as an extreme ram-pressure stripping event. The central claim is that RPS can remove most of the cold gas from massive galaxies in dense protocluster cores as early as z=4.3, thereby supplying a direct hydrodynamic pathway for environmental quenching at z>4.

Significance. If the RPS interpretation is substantiated, the result would establish that hydrodynamic stripping can operate efficiently in dynamically immature protoclusters at z>4, extending the redshift range of known environmental quenching mechanisms and providing morphological evidence that challenges the prevailing view that gravitational interactions dominate at these epochs.

major comments (2)
  1. [Abstract] Abstract (final paragraph): The assertion that the 6-kpc offset and >50% displaced gas fraction demonstrate RPS (rather than mergers, gravitational encounters, or line-of-sight projection within the protocluster) is load-bearing for the hydrodynamic-quenching conclusion, yet the text supplies no kinematic modeling, tail-morphology diagnostics, or quantitative comparison to z=4.3 merger simulations that would exclude the alternatives.
  2. [Abstract] Abstract: The claim of an 'extreme active-stripping phase' rests on the offset and mass fraction alone; without reported velocity-field data, error budgets on the offset measurement, or explicit tests against projection effects, the distinction from non-RPS scenarios remains unaddressed.
minor comments (2)
  1. [Abstract] The abstract would be strengthened by inclusion of basic observational parameters (ALMA band, JWST filter or mode) and a short statement of the uncertainty on the reported 6-kpc offset and gas-mass fraction.
  2. A methods section detailing data reduction, source extraction, and how the displaced-gas fraction was calculated is needed for reproducibility and to allow readers to assess measurement robustness.

Simulated Author's Rebuttal

2 responses · 1 unresolved

We thank the referee for their careful reading and constructive comments on the abstract. We agree that the current wording in the abstract overstates the conclusiveness of the RPS interpretation without sufficient caveats or supporting diagnostics. We will revise the abstract and add targeted discussion in the main text to address the concerns while preserving the core observational result.

read point-by-point responses

  1. Referee: [Abstract] Abstract (final paragraph): The assertion that the 6-kpc offset and >50% displaced gas fraction demonstrate RPS (rather than mergers, gravitational encounters, or line-of-sight projection within the protocluster) is load-bearing for the hydrodynamic-quenching conclusion, yet the text supplies no kinematic modeling, tail-morphology diagnostics, or quantitative comparison to z=4.3 merger simulations that would exclude the alternatives.

    Authors: We accept this criticism. The abstract is a summary and does not contain the requested modeling or comparisons. The main text presents the offset measurement and gas-mass fraction but does not include explicit kinematic modeling, tail diagnostics, or simulation comparisons. We will revise the abstract to state the observations more cautiously and add a short discussion section paragraph that qualitatively addresses why mergers are less favored given the environment and gas fraction, while acknowledging the absence of quantitative z=4.3 merger simulations. revision: yes

  2. Referee: [Abstract] Abstract: The claim of an 'extreme active-stripping phase' rests on the offset and mass fraction alone; without reported velocity-field data, error budgets on the offset measurement, or explicit tests against projection effects, the distinction from non-RPS scenarios remains unaddressed.

    Authors: We agree that the abstract does not report velocity-field data, error budgets, or projection tests. These elements are partially present in the results section of the full manuscript (ALMA moment maps and positional uncertainties), but they are not summarized in the abstract and no explicit projection-effect test is performed. We will revise the abstract to remove the unqualified 'extreme active-stripping phase' phrasing and include a brief statement of the measured offset uncertainty. A new sentence will be added noting that line-of-sight projection cannot be fully excluded with the current data. revision: yes

standing simulated objections not resolved
  • Quantitative comparison to z=4.3 merger simulations cannot be performed because no such simulations exist in the current literature.

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity: purely observational report with no derivations or self-referential predictions

full rationale

The paper presents ALMA and JWST observations of SPT2349-56-C26, reporting a 6-kpc spatial offset and >50% displaced cold gas as evidence for extreme ram-pressure stripping at z=4.3. No equations, fitted parameters, model derivations, or predictions appear in the abstract or described content. The central interpretation (RPS vs. alternatives) is an inference from data products, not a reduction of any claimed result to its own inputs by construction. No self-citations are invoked as load-bearing uniqueness theorems or ansatzes. The derivation chain is empty; the work is self-contained as an observational report.

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

Observational discovery paper; relies on standard distance-redshift conversion and morphological interpretation of gas displacement as RPS.

assumptions (2)
  • standard math Standard flat Lambda-CDM cosmology for converting redshift to physical distances and look-back time
    Invoked to place the event at z=4.3 and interpret the 6-kpc offset as physical.
  • domain assumption Gas morphology and offset indicate ram-pressure stripping rather than tidal or merger-driven displacement
    Central interpretive step in the final sentence of the abstract.

how reviews work

0 comments
Cite this review

Pith. "Pith review of An extreme ram-pressure stripping event in a protocluster at redshift 4.3." pith.science (2026). https://pith.science/paper/XI5X4R77

@misc{pith2026260618229,
  author       = {Pith},
  title        = {Pith review of: An extreme ram-pressure stripping event in a protocluster at redshift 4.3},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/XI5X4R77}},
  note         = {Machine review of arXiv:2606.18229}
}
abstract

In the nearby Universe, the environment plays a crucial role in suppressing star formation in dense regions. In particular, ram-pressure stripping (RPS) is a major mechanism for removing gas from galaxies in clusters, occurring when galaxies travel through a dense hot atmosphere and leave trailing gaseous wakes. By depleting the cold gas reservoir, RPS can drive outside-in quenching and is therefore thought to be an important route for transforming cluster galaxies. At earlier times, however, protoclusters are dynamically young and their hot atmospheres are expected to be immature, so environmental effects are commonly assumed to be dominated by gravitational interactions rather than hydrodynamic stripping. Recent observations have begun to show that RPS can already operate before mature cluster assembly, including extended gas tails in a forming cluster at $z=2.51$ and in a galaxy group at $z=3.06$. These studies demonstrate that hydrodynamic stripping is possible at earlier times, but whether RPS can become sufficient enough to quench massive galaxies at $z>2$ remains unclear. Here we report ALMA and JWST observations of SPT2349$-$56-C26, a massive galaxy experiencing an extreme RPS event in the SPT2349$-$56 protocluster at $z=4.30$. C26 appears to exhibit a particularly severe active-stripping phase: the displaced gas contains more than half of the observed cold-gas reservoir, with the gas-emission peak showing a large 6-kpc offset from the stellar body. These observations show that RPS can remove most of the cold gas from massive galaxies in dense protocluster cores as early as $z=4.3$, providing a direct hydrodynamic pathway for environmental quenching at $z>4$.

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

82 extracted references · 79 canonical work pages

  1. [1]

    Environmental Effects on Late-Type Galaxies in Nearby Clusters

    Boselli, A., Gavazzi, G.: Environmental Effects on Late-Type Galaxies in Nearby Clusters. PASP118(842), 517–559 (2006) https://doi.org/10.1086/ 500691 arXiv:astro-ph/0601108 [astro-ph]

    work page Pith review arXiv 2006

  2. [2]

    Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Peng, Y.-j., Lilly, S.J., Kovaˇ c, K., Bolzonella, M., Pozzetti, L., Renzini, A., Zamorani, G., Ilbert, O., Knobel, C., Iovino, A., Maier, C., Cucciati, O., Tasca, L., Carollo, C.M., Silverman, J., Kampczyk, P., de Ravel, L., Sanders, D., Scoville, N., Contini, T., Mainieri, V., Scodeggio, M., Kneib, J.-P., Le F` evre, O., Bardelli, S., Bongiorno, A., Cap...

    work page Pith review arXiv doi:10.1088/0004-637x/721/1/193 2010

  3. [3]

    MNRAS , author =

    Wetzel, A.R., Tinker, J.L., Conroy, C.: Galaxy evolution in groups and clus- ters: star formation rates, red sequence fractions and the persistent bimodal- ity. MNRAS424(1), 232–243 (2012) https://doi.org/10.1111/j.1365-2966.2012. 21188.x arXiv:1107.5311 [astro-ph.CO]

    work page doi:10.1111/j.1365-2966.2012 2012

  4. [4]

    Gone after One Orbit:

    Lotz, M., Remus, R.-S., Dolag, K., Biviano, A., Burkert, A.: Gone after one orbit: How cluster environments quench galaxies. MNRAS488(4), 5370–5389 (2019) https://doi.org/10.1093/mnras/stz2070 arXiv:1810.02382 [astro-ph.GA]

    work page doi:10.1093/mnras/stz2070 2019

  5. [5]

    III: On the Infall of Matter Into Clusters of Galaxies and Some Effects on Their Evolution

    Gunn, J.E., Gott, J.R. III: On the Infall of Matter Into Clusters of Galaxies and Some Effects on Their Evolution. ApJ176, 1 (1972) https://doi.org/10.1086/ 151605

    1972

  6. [6]

    Ram Pressure Stripping in Clusters and Groups

    Hester, J.A.: Ram Pressure Stripping in Clusters and Groups. ApJ647(2), 910– 921 (2006) https://doi.org/10.1086/505614 arXiv:astro-ph/0610088 [astro-ph]

    work page Pith review arXiv doi:10.1086/505614 2006

  7. [7]

    Environmentally-Driven Evolution of Simulated Cluster Galaxies

    Tonnesen, S., Bryan, G.L., van Gorkom, J.H.: Environmentally Driven Evolution of Simulated Cluster Galaxies. ApJ671(2), 1434–1445 (2007) https://doi.org/ 10.1086/523034 arXiv:0709.1720 [astro-ph]

    work page Pith review arXiv doi:10.1086/523034 2007

  8. [8]

    A&AR , volume =

    Boselli, A., Fossati, M., Sun, M.: Ram pressure stripping in high-density envi- ronments. A&A Rv30(1), 3 (2022) https://doi.org/10.1007/s00159-022-00140-3 arXiv:2109.13614 [astro-ph.GA]

    work page doi:10.1007/s00159-022-00140-3 2022

Show all 82 references
  1. [9]

    arXiv e-prints, 2603–03432 (2026) https://doi.org/10.48550/arXiv.2603.03432 arXiv:2603.03432 [astro-ph.GA]

    de Is´ ıdio, N., Popesso, P., Bah´ e, Y., Vulcani, B., Toptun, V., Marini, I., Pog- gianti, B., Biffi, V., Belfiore, F., Lagos, C., Dolag, K., Mazengo, D.: The kinematic imprinting of environmental quenching inz <0.2 galaxies. arXiv e-prints, 2603–03432 (2026) https://doi.org/...

    2026 doi arXiv

  2. [10]

    ApJ550(2), 612–621 (2001) https: //doi.org/10.1086/319811 arXiv:astro-ph/0012252 [astro-ph]

    Fujita, Y.: Ram-Pressure Stripping of Galaxies in High-Redshift Clusters and the Influence of Intracluster Medium Heating. ApJ550(2), 612–621 (2001) https: //doi.org/10.1086/319811 arXiv:astro-ph/0012252 [astro-ph]

    2001 doi arXiv

  3. [12]

    Bah´ e, Y.M., McCarthy, I.G.: Star formation quenching in simulated group and cluster galaxies: when, how, and why? MNRAS447(1), 969–992 (2015) https: //doi.org/10.1093/mnras/stu2293 arXiv:1410.8161 [astro-ph.GA]

    2015 doi arXiv

  4. [13]

    A&A 608, 48 (2017) https://doi.org/10.1051/0004-6361/201730449 arXiv:1701.05250 [astro-ph.GA]

    Dannerbauer, H., Lehnert, M.D., Emonts, B., Ziegler, B., Altieri, B., De Breuck, C., Hatch, N., Kodama, T., Koyama, Y., Kurk, J.D., Matiz, T., Miley, G., Narayanan, D., Norris, R.P., Overzier, R., R¨ ottgering, H.J.A., Sargent, M., Sey- mour, N., Tanaka, M., Valtchanov, I., Wy...

    2017 doi arXiv

  5. [14]

    ApJL867(2), 29 (2018) https://doi.org/10.3847/2041-8213/aaeb2c arXiv:1810.10558 [astro-ph.GA]

    Wang, T., Elbaz, D., Daddi, E., Liu, D., Kodama, T., Tanaka, I., Schreiber, C., Zanella, A., Valentino, F., Sargent, M., Kohno, K., Xiao, M., Pannella, M., Ciesla, L., Gobat, R., Koyama, Y.: Revealing the Environmental Dependence of Molecu- lar Gas Content in a Distant X-Ray C...

    2018 doi arXiv

  6. [15]

    MNRAS485(2), 2287–2311 (2019) https://doi.org/10.1093/mnras/ stz361 arXiv:1901.03336 [astro-ph.GA]

    Bah´ e, Y.M., Schaye, J., Barnes, D.J., Dalla Vecchia, C., Kay, S.T., Bower, R.G., Hoekstra, H., McGee, S.L., Theuns, T.: Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre- processing. MNRAS485(2), 2287–2311 (2019)...

    2019 doi arXiv

  7. [16]

    arXiv e-prints, 2503–21724 (2025) https://doi.org/10.48550/arXiv.2503.21724 arXiv:2503.21724 [astro-ph.GA]

    Xu, K., Wang, T., Daddi, E., Elbaz, D., Sun, H., Chen, L., Gobat, R., Zanella, A., Liu, D., Xiao, M., Cen, R., Kodama, T., Kohno, K., Yang, T., Zhang, Z.-Y., Zhou, L., Valentino, F.: Ram-pressure stripping caught in action in a forming galaxy cluster 3 billion years after the ...

    2025 doi arXiv

  8. [17]

    arXiv e-prints, 2604–11892 (2026) https://doi.org/10.48550/arXiv.2604.11892 arXiv:2604.11892 [astro-ph.GA]

    Li, M., Cai, Z., Emonts, B.H.C., Sun, F., Sun, M., Bian, F., Li, Z., Lin, X., Wu, Y., Bauer, F.E., Fujimoto, S., Koekemoer, A.M., Kokorev, V., Willmer, C.N.A., Egami, E., Fan, X., Xaiver Prochaska, J., Sun, Z., Yu, F.: A Post-starburst Galaxy Undergoing Ram-pressure Stripping ...

    2026 doi arXiv

  9. [18]

    ApJ719(1), 763–783 (2010) https://doi.org/10.1088/0004-637X/ 719/1/763 arXiv:0912.2338 [astro-ph.CO]

    Vieira, J.D., Crawford, T.M., Switzer, E.R., Ade, P.A.R., Aird, K.A., Ashby, M.L.N., Benson, B.A., Bleem, L.E., Brodwin, M., Carlstrom, J.E., Chang, C.L., Cho, H.-M., Crites, A.T., de Haan, T., Dobbs, M.A., Everett, W., George, E.M., Gladders, M., Hall, N.R., Halverson, N.W., ...

    2010 doi arXiv

  10. [19]

    Nature556(7702), 469–472 (2018) https://doi.org/10.1038/s41586-018-0025-2 arXiv:1804.09231 [astro-ph.GA]

    Miller, T.B., Chapman, S.C., Aravena, M., Ashby, M.L.N., Hayward, C.C., Vieira, J.D., Weiß, A., Babul, A., B´ ethermin, M., Bradford, C.M., Brodwin, M., Carl- strom, J.E., Chen, C.-C., Cunningham, D.J.M., De Breuck, C., Gonzalez, A.H., 30 Greve, T.R., Harnett, J., Hezaveh, Y.,...

    2018 doi arXiv

  11. [20]

    MNRAS495(3), 3124–3159 (2020) https://doi.org/10.1093/mnras/staa1275 arXiv:2002.11600 [astro-ph.GA]

    Hill, R., Chapman, S., Scott, D., Apostolovski, Y., Aravena, M., B´ ethermin, M., Bradford, C.M., Canning, R.E.A., De Breuck, C., Dong, C., Gonzalez, A., Greve, T.R., Hayward, C.C., Hezaveh, Y., Litke, K., Malkan, M., Marrone, D.P., Phadke, K., Reuter, C., Rotermund, K., Spilk...

    2020 doi

  12. [21]

    arXiv e-prints, 2509–08035 (2025) https://doi.org/10.48550/arXiv.2509.08035 arXiv:2509.08035 [astro-ph.GA]

    Sulzenauer, N., Weiß, A., Hill, R., Chapman, S.C., Aravena, M., Dike, V.J., Gon- zalez, A., MacIntyre, D., Narayanan, D., Phadke, K.A., Pillai, V.R., Posses, A.C., Rennehan, D., Saintonge, A., Spilker, J.S., Solimano, M., Tsuchitori, J., Vieira, J.D., Vizgan, D., Zhou, D.: Bri...

    2025 doi

  13. [22]

    arXiv e-prints, 2511–17814 (2025) https: //doi.org/10.48550/arXiv.2511.17814 arXiv:2511.17814 [astro-ph.GA]

    Chapman, S.C., Deane, R.P., Zhou, D., Aravena, M., Rasakanya, W., Archipley, M., Burgoyne, J., Cathey, J., Gonzalez, A.H., Hill, R., Hughes, C., Isla Llave, M.N., Malkan, M., Phadke, K.A., Pillai, V., Posses, A., Slocombe, B., Solimano, M., Spilker, J., Sulzenauer, N., Vito, F...

    2025 doi

  14. [23]

    Nature 649(8099), 1130–1133 (2026) https://doi.org/10.1038/s41586-025-09901-3

    Zhou, D., Chapman, S.C., Aravena, M., Araya-Araya, P., Archipley, M., Cathey, J., Deane, R.P., Di Mascolo, L., Gobat, R., Greve, T.R., Hill, R., Kim, S., Phadke, K.A., Pillai, V.R., Posses, A.C., Reichardt, C.L., Solimano, M., Spilker, J.S., Sulzenauer, N., Dike, V.J., Vieira,...

    2026 doi

  15. [24]

    PASJ56, 621–631 (2004) https://doi.org/10.1093/pasj/56.4.621 arXiv:astro-ph/0406637 [astro-ph]

    Fujita, Y., Goto, T.: The Evolution of Galaxies in and around Clusters at High-Redshift. PASJ56, 621–631 (2004) https://doi.org/10.1093/pasj/56.4.621 arXiv:astro-ph/0406637 [astro-ph]

    2004 doi arXiv

  16. [25]

    A&A632, 49 (2019) https: //doi.org/10.1051/0004-6361/201935394 arXiv:1903.02879 [astro-ph.GA]

    Sarron, F., Adami, C., Durret, F., Laigle, C.: Pre-processing of galaxies in cosmic filaments around AMASCFI clusters in the CFHTLS. A&A632, 49 (2019) https: //doi.org/10.1051/0004-6361/201935394 arXiv:1903.02879 [astro-ph.GA]

    2019 doi

  17. [26]

    A&A499(1), 87–102 (2009) https://doi.org/10.1051/0004-6361/200811551 arXiv:0903.3818 [astro-ph.CO]

    Kapferer, W., Sluka, C., Schindler, S., Ferrari, C., Ziegler, B.: The effect of 31 ram pressure on the star formation, mass distribution and morphology of galax- ies. A&A499(1), 87–102 (2009) https://doi.org/10.1051/0004-6361/200811551 arXiv:0903.3818 [astro-ph.CO]

    2009 doi arXiv

  18. [27]

    ApJS247(2), 61 (2020) https://doi.org/10.3847/1538-4365/ ab7ccd arXiv:1912.01621 [astro-ph.GA]

    Faisst, A.L., Schaerer, D., Lemaux, B.C., Oesch, P.A., Fudamoto, Y., Cassata, P., B´ ethermin, M., Capak, P.L., Le F` evre, O., Silverman, J.D., Yan, L., Ginolfi, M., Koekemoer, A.M., Morselli, L., Amor´ ın, R., Bardelli, S., Boquien, M., Bram- mer, G., Cimatti, A., Dessauges-...

    2020 doi

  19. [29]

    MNRAS481(2), 1976–1999 (2018) https://doi.org/10.1093/mnras/sty2394 arXiv:1808.10331 [astro-ph.GA]

    Zanella, A., Daddi, E., Magdis, G., Diaz Santos, T., Cormier, D., Liu, D., Cibinel, A., Gobat, R., Dickinson, M., Sargent, M., Popping, G., Madden, S.C., Bethermin, M., Hughes, T.M., Valentino, F., Rujopakarn, W., Pannella, M., Bournaud, F., Walter, F., Wang, T., Elbaz, D., Co...

    1976 doi arXiv

  20. [30]

    ARA&A 51(1), 105–161 (2013) https://doi.org/10.1146/annurev-astro-082812-140953 arXiv:1301.0371 [astro-ph.CO]

    Carilli, C.L., Walter, F.: Cool Gas in High-Redshift Galaxies. ARA&A 51(1), 105–161 (2013) https://doi.org/10.1146/annurev-astro-082812-140953 arXiv:1301.0371 [astro-ph.CO]

    2013 doi arXiv

  21. [31]

    MNRAS457(4), 4406–4420 (2016) https://doi.org/10.1093/mnras/stw275 arXiv:1602.00652 [astro-ph.GA]

    Aravena, M., Spilker, J.S., Bethermin, M., Bothwell, M., Chapman, S.C., de Breuck, C., Furstenau, R.M., G´ onzalez-L´ opez, J., Greve, T.R., Litke, K., Ma, J., Malkan, M., Marrone, D.P., Murphy, E.J., Stark, A., Strandet, M., Vieira, J.D., Weiss, A., Welikala, N., Wong, G.F., ...

    2016 doi arXiv

  22. [32]

    MNRAS412(3), 1913–1925 (2011) https://doi.org/10.1111/j.1365-2966.2010

    Ivison, R.J., Papadopoulos, P.P., Smail, I., Greve, T.R., Thomson, A.P., 32 Xilouris, E.M., Chapman, S.C.: Tracing the molecular gas in distant submil- limetre galaxies via CO(1-0) imaging with the Expanded Very Large Array. MNRAS412(3), 1913–1925 (2011) https://doi.org/10.111...

    1913 doi

  23. [33]

    ApJ820(2), 83 (2016) https://doi.org/10.3847/0004-637X/820/2/83 arXiv:1511.05149 [astro-ph.GA]

    Scoville, N., Sheth, K., Aussel, H., Vanden Bout, P., Capak, P., Bongiorno, A., Casey, C.M., Murchikova, L., Koda, J., ´Alvarez-M´ arquez, J., Lee, N., Laigle, C., McCracken, H.J., Ilbert, O., Pope, A., Sanders, D., Chu, J., Toft, S., Ivi- son, R.J., Manohar, S.: ISM Masses an...

    2016 doi arXiv

  24. [34]

    APEX observations of molecular gas in the discs and in the tails of ram-pressure stripped galaxies

    Moretti, A., Paladino, R., Poggianti, B.M., D’Onofrio, M., Bettoni, D., Gul- lieuszik, M., Jaff´ e, Y.L., Vulcani, B., Fasano, G., Fritz, J., Torstensson, K.: GASP - X. APEX observations of molecular gas in the discs and in the tails of ram-pressure stripped galaxies. MNRAS480...

    2018 doi arXiv

  25. [35]

    Moretti, A., Paladino, R., Poggianti, B.M., Serra, P., Roediger, E., Gullieuszik, M., Tomiˇ ci´ c, N., Radovich, M., Vulcani, B., Jaff´ e, Y.L., Fritz, J., Bettoni, D., Ramatsoku, M., Wolter, A.: GASP. XXII. The Molecular Gas Content of the JW100 Jellyfish Galaxy at z∼0.05: Do...

    2020 doi

  26. [36]

    ApJ887(2), 155 (2019) https: //doi.org/10.3847/1538-4357/ab5224 arXiv:1910.11622 [astro-ph.GA]

    Poggianti, B.M., Ignesti, A., Gitti, M., Wolter, A., Brighenti, F., Biviano, A., George, K., Vulcani, B., Gullieuszik, M., Moretti, A., Paladino, R., Bettoni, D., Franchetto, A., Jaff´ e, Y.L., Radovich, M., Roediger, E., Tomiˇ ci´ c, N., Tonnesen, S., Bellhouse, C., Fritz, J....

    2019 doi

  27. [37]

    Nature Astronomy6, 270–274 (2021) https://doi.org/10.1038/s41550-021-01516-8 arXiv:2103.09205 [astro-ph.GA]

    Sun, M., Ge, C., Luo, R., Yagi, M., J´ achym, P., Boselli, A., Fossati, M., Nulsen, P.E.J., Yoshida, M., Gavazzi, G.: A universal correlation between warm and hot gas in the stripped tails of cluster galaxies. Nature Astronomy6, 270–274 (2021) https://doi.org/10.1038/s41550-02...

    2021 doi

  28. [38]

    ApJ908(2), 228 (2021) https: //doi.org/10.3847/1538-4357/abd71e arXiv:2101.01887 [astro-ph.GA]

    Liu, Q., Yee, H.K.C., Drissen, L., Sivanandam, S., Pintos-Castro, I., Alcorn, L.Y., Hsieh, B.-C., Lin, L., Lin, Y.-T., Muzzin, A., Noble, A., Old, L.: SITELLE Hα Imaging Spectroscopy of z∼0.25 Clusters: Emission-line Galaxy Detection and Ionized Gas Offset in Abell 2390 and Ab...

    2021 doi

  29. [39]

    ApJ883(2), 145 (2019) https://doi.org/10.3847/ 1538-4357/ab3e6c arXiv:1905.13249 [astro-ph.GA]

    J´ achym, P., Kenney, J.D.P., Sun, M., Combes, F., Cortese, L., Scott, T.C., Sivanandam, S., Brinks, E., Roediger, E., Palouˇ s, J., Fumagalli, M.: ALMA Unveils Widespread Molecular Gas Clumps in the Ram Pressure Stripped Tail 33 of the Norma Jellyfish Galaxy. ApJ883(2), 145 (...

    2019

  30. [41]

    MNRAS494(4), 5029–5043 (2020) https://doi.org/10.1093/ mnras/staa968 arXiv:2004.04754 [astro-ph.GA]

    Deb, T., Verheijen, M.A.W., Gullieuszik, M., Poggianti, B.M., van Gorkom, J.H., Ramatsoku, M., Serra, P., Moretti, A., Vulcani, B., Bettoni, D., Jaff´ e, L.Y., Tonnesen, S., Fritz, J.: GASP XXV: neutral hydrogen gas in the striking jelly- fish galaxy JO204. MNRAS494(4), 5029–5...

    2020

  31. [42]

    PASJ76(6), 1143–1157 (2024) https://doi.org/10.1093/pasj/psae076 arXiv:2212.05984 [astro-ph.GA]

    Momose, R., Lee, K.-G., Ata, M., Horowitz, B., Kartaltepe, J.S.: The dependence of galaxy properties on the underlying three-dimensional matter density field at 2.0 ¡ z ¡ 2.5. PASJ76(6), 1143–1157 (2024) https://doi.org/10.1093/pasj/psae076 arXiv:2212.05984 [astro-ph.GA]

    2024 doi

  32. [43]

    ApJ970(1), 59 (2024) https://doi.org/10.3847/1538-4357/ ad5316 arXiv:2311.11569 [astro-ph.GA]

    Tanaka, M., Onodera, M., Shimakawa, R., Ito, K., Kakimoto, T., Kubo, M., Mor- ishita, T., Toft, S., Valentino, F., Wu, P.-F.: A Protocluster of Massive Quiescent Galaxies at z = 4. ApJ970(1), 59 (2024) https://doi.org/10.3847/1538-4357/ ad5316 arXiv:2311.11569 [astro-ph.GA]

    2024 doi

  33. [44]

    The ATCA CO(1-0) look at the growth and death of Hαemitters in the Spiderweb protocluster at z = 2.16

    P´ erez-Mart´ ınez, J.M., Dannerbauer, H., Emonts, B.H.C., Allison, J.R., Cham- pagne, J.B., Indermuehle, B., Norris, R.P., Serra, P., Seymour, N., Thomson, A.P., Casey, C.M., Chen, Z., Daikuhara, K., De Breuck, C., D’Eugenio, C., Drouart, G., Hatch, N., Jin, S., Kodama, T., K...

    2025 doi

  34. [45]

    turbulent motions at the centres of galaxy clusters: Agn-driven turbulence according to tng-cluster (2026) arXiv:2606.05355 [astro-ph.GA]

    Saha, B., Pillepich, A., Braspenning, J., Prunier, M., Chatzigiannakis, D., Nel- son, D.: Bulk vs. turbulent motions at the centres of galaxy clusters: Agn-driven turbulence according to tng-cluster (2026) arXiv:2606.05355 [astro-ph.GA]

    2026 arXiv

  35. [46]

    ApJ854(2), 91 (2018) https://doi.org/ 10.3847/1538-4357/aaa843 arXiv:1703.06954 [astro-ph.GA]

    Li, Y., Ruszkowski, M., Tremblay, G.: The Effects of Ram Pressure on the Cold Clouds in the Centers of Galaxy Clusters. ApJ854(2), 91 (2018) https://doi.org/ 10.3847/1538-4357/aaa843 arXiv:1703.06954 [astro-ph.GA]

    2018 doi arXiv

  36. [47]

    ApJ1000(1), 67 (2026) https://doi.org/10.3847/1538-4357/ae4226 arXiv:2603.12082 [astro-ph.GA] 34

    Ge, C., Sun, M., Ramatsoku, M., Nolting, C., Koribalski, B.S.: The Shocking Features in the Closest Rich Galaxy Cluster Norma. ApJ1000(1), 67 (2026) https://doi.org/10.3847/1538-4357/ae4226 arXiv:2603.12082 [astro-ph.GA] 34

    2026 doi

  37. [48]

    MNRAS512(3), 4352–4377 (2022) https: //doi.org/10.1093/mnras/stab3539 arXiv:2109.04534 [astro-ph.GA]

    Hill, R., Chapman, S., Phadke, K.A., Aravena, M., Archipley, M., Ashby, M.L.N., B´ ethermin, M., Canning, R.E.A., Gonzalez, A., Greve, T.R., Gururajan, G., Hay- ward, C.C., Hezaveh, Y., Jarugula, S., MacIntyre, D., Marrone, D.P., Miller, T., Rennehan, D., Reuter, C., Rotermund...

    2022 doi

  38. [49]

    arXiv e-prints, 2412–03790 (2024) https://doi.org/10.48550/arXiv.2412.03790 arXiv:2412.03790 [astro-ph.GA]

    Hughes, C., Hill, R., Chapman, S., Aravena, M., Archipley, M., Dike, V.J., Gonza- lez, A., Greve, T.R., Gururajan, G., Hayward, C., Phadke, K., Reuter, C., Spilker, J., Sulzenauer, N., Vieira, J.D., Vizgan, D., Wang, G., Weiss, A., Zhou, D.: Evi- dence for environmental effect...

    2024 doi

  39. [50]

    ApJL982(1), 17 (2025) https://doi.org/10.3847/2041-8213/adb8d8 arXiv:2412.17980 [astro-ph.GA]

    Zhou, D., Chapman, S.C., Sulzenauer, N., Hill, R., Aravena, M., Araya-Araya, P., Cathey, J., Marrone, D.P., Phadke, K.A., Reuter, C., Solimano, M., Spilker, J.S., Vieira, J.D., Vizgan, D., Wang, G.C.P., Weiss, A.: A Large Molecular Gas Reservoir in the Protocluster SPT2349-56 ...

    2025 doi

  40. [51]

    Harrington, K.C., Vishwas, A., Man, A.W.S., De Breuck, C., Papadopoulos, P.P., Andreani, P., Bisbas, T.G.: Extended multi-phase gas reservoirs in the z = 4.3 protocluster SPT2349-56: Non-stellar ionisation sources? A&A701, 298 (2025) https://doi.org/10.1051/0004-6361/202555071...

    2025 doi

  41. [52]

    A&A452(3), 795– 802 (2006) https://doi.org/10.1051/0004-6361:20053921 arXiv:astro-ph/0507605 [astro-ph]

    Domainko, W., Mair, M., Kapferer, W., van Kampen, E., Kronberger, T., Schindler, S., Kimeswenger, S., Ruffert, M., Mangete, O.E.: Enrichment of the ICM of galaxy clusters due to ram-pressure stripping. A&A452(3), 795– 802 (2006) https://doi.org/10.1051/0004-6361:20053921 arXiv...

    2006 doi arXiv

  42. [53]

    Extended molecular gas reservoirs are common in a distant, forming galaxy cluster

    Chen, Z., Dannerbauer, H., Lehnert, M.D., Emonts, B.H.C., Gu, Q., Allison, J.R., Champagne, J.B., Hatch, N., Inderm¨ uehle, B., Norris, R.P., P´ erez-Mart´ ınez, J.M., R¨ ottgering, H.J.A., Serra, P., Seymour, N., Shimakawa, R., Thomson, A.P., Casey, C.M., De Breuck, C., Droua...

    2024 doi

  43. [54]

    ApJ998(2), 285 (2026) https://doi.org/10.3847/1538-4357/ae3824 arXiv:2506.14117 [astro-ph.GA]

    Roberts, I.D., Balogh, M.L., Sok, V., Muzzin, A., Hudson, M.J., Jablonka, P.: JWST Reveals a Candidate Jellyfish Galaxy at z = 1.156. ApJ998(2), 285 (2026) https://doi.org/10.3847/1538-4357/ae3824 arXiv:2506.14117 [astro-ph.GA]

    2026 doi

  44. [55]

    arXiv e-prints, 2511–19608 (2025) https://doi.org/10.48550/arXiv.2511.19608 arXiv:2511.19608 [astro-ph.GA]

    Wang, X., Cantalupo, S., Wang, W., Galbiati, M., Steidel, C.C., Pensabene, 35 A., Mao, S., Travascio, A., Lazeyras, T., Ledos, N., Quadri, G.: Metal enrich- ment of galaxies in a massive node of the Cosmic Web atz∼3. arXiv e-prints, 2511–19608 (2025) https://doi.org/10.48550/a...

    2025 doi arXiv

  45. [56]

    ApJL985(1), 8 (2025) https://doi.org/10.3847/2041-8213/add1d4 arXiv:2502.06538 [astro-ph.GA]

    Umehata, H., Kubo, M., Nakanishi, K.: ADF22-WEB: Detection of a Molecular Gas Reservoir in a Massive Quiescent Galaxy Located in a z = 3 Proto- cluster Core. ApJL985(1), 8 (2025) https://doi.org/10.3847/2041-8213/add1d4 arXiv:2502.06538 [astro-ph.GA]

    2025 doi

  46. [57]

    Nature Astronomy10, 431–439 (2026) https://doi.org/10.1038/s41550-025-02751-z arXiv:2405.19401 [astro-ph.GA]

    Scholtz, J., D’Eugenio, F., Maiolino, R., P´ erez-Gonz´ alez, P.G., Circosta, C., Tac- chella, S., Williams, C.C., Alberts, S., Arribas, S., Baker, W.M., Bertola, E., Bunker, A.J., Carniani, S., Charlot, S., Cresci, G., Jones, G.C., Kumari, N., Lamperti, I., Looser, T.J., Pino...

    2026 doi

  47. [59]

    arXiv e-prints, 2604–09347 (2026) https://doi.org/10.48550/arXiv.2604.09347 arXiv:2604.09347 [astro-ph.GA]

    D’Eugenio, C., Daddi, E., Gobat, R., Jin, S., Liu, D., Sun, H., Gentile, F., Bruckmann, F., Liu, Z., Delvecchio, I., Vallini, L., Magnelli, B., Zanella, A.: A first [CII] view of high-z quiescent galaxies. arXiv e-prints, 2604–09347 (2026) https://doi.org/10.48550/arXiv.2604.0...

    2026 doi arXiv

  48. [60]

    Molecular gas budget in the early Universe as traced by [C II]

    Dessauges-Zavadsky, M., Ginolfi, M., Pozzi, F., B´ ethermin, M., Le F` evre, O., Fujimoto, S., Silverman, J.D., Jones, G.C., Vallini, L., Schaerer, D., Faisst, A.L., Khusanova, Y., Fudamoto, Y., Cassata, P., Loiacono, F., Capak, P.L., Yan, L., Amorin, R., Bardelli, S., Boquien...

    2020

  49. [61]

    ApJ853(2), 179 (2018) https://doi.org/10.3847/1538-4357/aaa4b4 arXiv:1702.01140 [astro-ph.GA] 36

    Tacconi, L.J., Genzel, R., Saintonge, A., Combes, F., Garc´ ıa-Burillo, S., Neri, R., Bolatto, A., Contini, T., F¨ orster Schreiber, N.M., Lilly, S., Lutz, D., Wuyts, S., Accurso, G., Boissier, J., Boone, F., Bouch´ e, N., Bournaud, F., Burkert, A., Car- ollo, M., Cooper, M., ...

    2018 doi arXiv

  50. [62]

    A&A647, 33 (2021) https://doi.org/10.1051/0004-6361/ 202039280 arXiv:2101.04700 [astro-ph.GA]

    Magdis, G.E., Gobat, R., Valentino, F., Daddi, E., Zanella, A., Kokorev, V., Toft, S., Jin, S., Whitaker, K.E.: The interstellar medium of quiescent galaxies and its evolution with time. A&A647, 33 (2021) https://doi.org/10.1051/0004-6361/ 202039280 arXiv:2101.04700 [astro-ph.GA]

    2021 doi

  51. [63]

    Planck Collaboration, Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartlett, J.G., Bar- tolo, N., Battaner, E., Battye, R., Benabed, K., Benoˆ ıt, A., Benoit-L´ evy, A., Bernard, J.-P., Bersanelli, M., Bielewicz,...

    2015 doi arXiv

  52. [64]

    https://doi.org/10.5281/zenodo.6984365

    Bushouse, H., Eisenhamer, J., Dencheva, N., Davies, J., Greenfield, P., Morrison, J., Hodge, P., Simon, B., Grumm, D., Droettboom, M., Slavich, E., Sosey, M., Pauly, T., Miller, T., Jedrzejewski, R., Hack, W., Davis, D., Crawford, S., Law, 37 D., Gordon, K., Regan, M., Cara, M...

    doi

  53. [65]

    Summary of the content and survey properties

    Gaia Collaboration, Vallenari, A., Brown, A.G.A., Prusti, T., de Bruijne, J.H.J., Arenou, F., Babusiaux, C., Biermann, M., Creevey, O.L., Ducourant, C., Evans, D.W., Eyer, L., Guerra, R., Hutton, A., Jordi, C., Klioner, S.A., Lammers, U.L., Lindegren, L., Luri, X., Mignard, F....

    2023 doi

  54. [66]

    Robitaille, T., Deil, C., Ginsburg, A.: reproject: Python-based Astronomical Image Reprojection 38

  55. [67]

    PASP134(1041), 114501 (2022) https://doi.org/10.1088/1538-3873/ ac9642 arXiv:2210.02276 [astro-ph.IM]

    CASA Team, Bean, B., Bhatnagar, S., Castro, S., Donovan Meyer, J., Emonts, B., Garcia, E., Garwood, R., Golap, K., Gonzalez Villalba, J., Harris, P., Hayashi, Y., Hoskins, J., Hsieh, M., Jagannathan, P., Kawasaki, W., Keimpema, A., Kettenis, M., Lopez, J., Marvil, J., Masters,...

    2022 doi arXiv

  56. [68]

    PASP118(842), 590–610 (2006) https://doi.org/10.1086/502982 arXiv:astro-ph/0601706 [astro-ph]

    Rosolowsky, E., Leroy, A.: Bias-free Measurement of Giant Molecular Cloud Properties. PASP118(842), 590–610 (2006) https://doi.org/10.1086/502982 arXiv:astro-ph/0601706 [astro-ph]

    2006 doi arXiv

  57. [69]

    ApJS255(1), 19 (2021) https://doi.org/10.3847/1538-4365/abec80 arXiv:2104.07665 [astro-ph.IM]

    Leroy, A.K., Hughes, A., Liu, D., Pety, J., Rosolowsky, E., Saito, T., Schinnerer, E., Schruba, A., Usero, A., Faesi, C.M., Herrera, C.N., Chevance, M., Hygate, A.P.S., Kepley, A.A., Koch, E.W., Querejeta, M., Sliwa, K., Will, D., Wilson, C.D., Anand, G.S., Barnes, A., Belfior...

    2021 doi

  58. [70]

    https://doi.org/10.5281/zenodo.13989456

    Bradley, L., Sip˝ ocz, B., Robitaille, T., Tollerud, E., Vin´ ıcius, Z., Deil, C., Bar- bary, K., Wilson, T.J., Busko, I., Donath, A., G¨ unther, H.M., Cara, M., Lim, P.L., Meßlinger, S., Conseil, S., Burnett, Z., Bostroem, A., Droettboom, M., Bray, E.M., Bratholm, L.A., Ginsb...

    doi

  59. [71]

    Anderson, J., King, I.R.: Toward High-Precision Astrometry with WFPC2. I. Deriving an Accurate Point-Spread Function. PASP112(776), 1360–1382 (2000) https://doi.org/10.1086/316632 arXiv:astro-ph/0006325 [astro-ph]

    2000 doi arXiv

  60. [72]

    MNRAS388(4), 1595–1617 (2008) https://doi.org/10.1111/j.1365-2966.2008.13535.x arXiv:0806.1020 [astro-ph] 39

    da Cunha, E., Charlot, S., Elbaz, D.: A simple model to interpret the ultraviolet, optical and infrared emission from galaxies. MNRAS388(4), 1595–1617 (2008) https://doi.org/10.1111/j.1365-2966.2008.13535.x arXiv:0806.1020 [astro-ph] 39

    2008 doi

  61. [73]

    ApJ806(1), 110 (2015) https://doi.org/10.1088/0004-637X/806/1/ 110 arXiv:1504.04376 [astro-ph.GA]

    da Cunha, E., Walter, F., Smail, I.R., Swinbank, A.M., Simpson, J.M., Decarli, R., Hodge, J.A., Weiss, A., van der Werf, P.P., Bertoldi, F., Chapman, S.C., Cox, P., Danielson, A.L.R., Dannerbauer, H., Greve, T.R., Ivison, R.J., Karim, A., Thomson, A.: An ALMA Survey of Sub-mil...

    2015 doi arXiv

  62. [74]

    ApJ888(2), 108 (2020) https://doi.org/10.3847/1538-4357/ab5fdd arXiv:1912.05206 [astro- ph.GA]

    Battisti, A.J., Cunha, E.d., Shivaei, I., Calzetti, D.: The Strength of the 2175 ˚A Feature in the Attenuation Curves of Galaxies at 0.1 ¡ z≲3. ApJ888(2), 108 (2020) https://doi.org/10.3847/1538-4357/ab5fdd arXiv:1912.05206 [astro- ph.GA]

    2020 doi

  63. [75]

    arXiv e-prints, 2603–22945 (2026) https://doi.org/10.48550/arXiv.2603.22945 arXiv:2603.22945 [astro-ph.GA]

    Jones, Z.R., da Cunha, E., Battisti, A.: How well does MAGPHYS recover galaxy properties? A test using EAGLE simulated star-forming galaxies. arXiv e-prints, 2603–22945 (2026) https://doi.org/10.48550/arXiv.2603.22945 arXiv:2603.22945 [astro-ph.GA]

    2026 doi

  64. [76]

    Royal Society Open Science 3(6), 160025 (2016) https://doi.org/10.1098/rsos.160025 arXiv:1605.03885 [astro- ph.GA]

    Zhang, Z.-Y., Papadopoulos, P.P., Ivison, R.J., Galametz, M., Smith, M.W.L., Xilouris, E.M.: Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe. Royal Society Open Science 3(6), 160025 (2016) https://doi.org/10.1098/rsos...

    2016 doi arXiv

  65. [77]

    ApJ 837(2), 150 (2017) https://doi.org/10.3847/1538-4357/aa61a0 arXiv:1702.04729 [astro-ph.GA]

    Scoville, N., Lee, N., Vanden Bout, P., Diaz-Santos, T., Sanders, D., Darvish, B., Bongiorno, A., Casey, C.M., Murchikova, L., Koda, J., Capak, P., Vlahakis, C., Ilbert, O., Sheth, K., Morokuma-Matsui, K., Ivison, R.J., Aussel, H., Laigle, C., McCracken, H.J., Armus, L., Pope,...

    2017 doi arXiv

  66. [78]

    ApJ943(2), 82 (2023) https://doi.org/10.3847/1538-4357/aca1bc arXiv:2211.07836 [astro-ph.GA]

    Scoville, N., Faisst, A., Weaver, J., Toft, S., McCracken, H.J., Ilbert, O., Diaz- Santos, T., Staguhn, J., Koda, J., Casey, C., Sanders, D., Mobasher, B., Chartab, N., Sattari, Z., Capak, P., Vanden Bout, P., Bongiorno, A., Vlahakis, C., Sheth, K., Yun, M., Aussel, H., Laigle...

    2023 doi

  67. [79]

    Identification of radio and mid-infrared counterparts to submillimetre galax- ies

    Ivison, R.J., Greve, T.R., Dunlop, J.S., Peacock, J.A., Egami, E., Smail, I., Ibar, E., van Kampen, E., Aretxaga, I., Babbedge, T., Biggs, A.D., Blain, A.W., Chap- man, S.C., Clements, D.L., Coppin, K., Farrah, D., Halpern, M., Hughes, D.H., Jarvis, M.J., Jenness, T., Jones, J...

    2007 doi

  68. [80]

    Bellhouse, C., Jaff´ e, Y.L., Hau, G.K.T., McGee, S.L., Poggianti, B.M., Moretti, A., Gullieuszik, M., Bettoni, D., Fasano, G., D’Onofrio, M., Fritz, J., Omizzolo, A., Sheen, Y.-K., Vulcani, B.: GASP. II. A MUSE View of Extreme Ram-Pressure Stripping along the Line of Sight: K...

    2017 doi arXiv

  69. [81]

    ApJ935(2), 167 (2022) https://doi.org/10.3847/1538-4357/ac7c74 arXiv:2206.14220 [astro-ph.IM]

    Astropy Collaboration, Price-Whelan, A.M., Lim, P.L., Earl, N., Starkman, N., Bradley, L., Shupe, D.L., Patil, A.A., Corrales, L., Brasseur, C.E., N¨ othe, M., Donath, A., Tollerud, E., Morris, B.M., Ginsburg, A., Vaher, E., Weaver, B.A., Tocknell, J., Jamieson, W., van Kerkwi...

    2022 doi arXiv

  70. [82]

    AJ157(3), 98 (2019) 41 https://doi.org/10.3847/1538-3881/aafc33 arXiv:1901.04520 [astro-ph.IM]

    Ginsburg, A., Sip˝ ocz, B.M., Brasseur, C.E., Cowperthwaite, P.S., Craig, M.W., Deil, C., Guillochon, J., Guzman, G., Liedtke, S., Lian Lim, P., Lockhart, K.E., Mommert, M., Morris, B.M., Norman, H., Parikh, M., Persson, M.V., Robitaille, T.P., Segovia, J.-C., Singer, L.P., To...

    2019 doi arXiv

  71. [83]

    Computing in Science and Engineering9(3), 90–95 (2007) https://doi.org/10.1109/MCSE.2007.55

    Hunter, J.D.: Matplotlib: A 2D Graphics Environment. Computing in Science and Engineering9(3), 90–95 (2007) https://doi.org/10.1109/MCSE.2007.55

    2007 doi

  72. [84]

    Nature585(7825), 357–362 (2020) https://doi.org/10.1038/s41586-020-2649-2

    Harris, C.R., Millman, K.J., Walt, S.J., Gommers, R., Virtanen, P., Cournapeau, D., Wieser, E., Taylor, J., Berg, S., Smith, N.J., Kern, R., Picus, M., Hoyer, S., Kerkwijk, M.H., Brett, M., Haldane, A., R´ ıo, J.F., Wiebe, M., Peterson, P., G´ erard-Marchant, P., Sheppard, K.,...

    2020 doi

  73. [85]

    https://doi.org/10

    The pandas development Team: pandas-dev/pandas: Pandas. https://doi.org/10. 5281/zenodo.3509134

  74. [86]

    https://doi.org/10.5281/zenodo.2573901 42

    Ginsburg, A., Koch, E., Robitaille, T., Beaumont, C., Adamginsburg, ZuHone, J., Sipocz, B., Patra, S., Jones, C., Lim, P.L., Rosolowsky, E., Stern, K., Earl, N., De Val-Borro, M., Jrobbfed, Shuokong, Kepley, A., Sokolov, V., Badger, T.G., Maret, S., Garrido, J., Booker, J., To...

    doi

Pith tools

Reviewed June 27, 2026 · model on record in the stance chip above.