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arxiv: 2606.18229 · v1 · pith:XI5X4R77new · submitted 2026-06-16 · 🌌 astro-ph.GA

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

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

Pith reviewed 2026-06-27 00:01 UTC · model grok-4.3

classification 🌌 astro-ph.GA
keywords ram-pressure strippingprotoclustergalaxy quenchinghigh-redshift galaxiescold gasenvironmental effectsALMAJWST
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The pith

Ram-pressure stripping removes more than half the cold gas from a massive galaxy in a protocluster at redshift 4.3.

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

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.

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.

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.

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.

Where Pith is reading between the lines

These are 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.

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.

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.

read the original 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 $z>4$.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

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

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.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

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

axioms (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.

pith-pipeline@v0.9.1-grok · 5935 in / 1249 out tokens · 45562 ms · 2026-06-27T00:01:06.647936+00:00 · methodology

discussion (0)

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Works this paper leans on

82 extracted references · 74 canonical work pages · 35 internal anchors

  1. [1]

    PASP118(842), 517–559 (2006) https://doi.org/10.1086/ 500691 arXiv:astro-ph/0601108 [astro-ph]

    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]

    Pith/arXiv 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 internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/721/1/193 2010

  3. [3]

    , keywords =

    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]

    MNRAS488(4), 5370–5389 (2019) https://doi.org/10.1093/mnras/stz2070 arXiv:1810.02382 [astro-ph.GA]

    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 internal anchor Pith review Pith/arXiv 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 internal anchor Pith review Pith/arXiv arXiv doi:10.1086/523034 2007

  8. [8]

    A&A Rv30(1), 3 (2022) https://doi.org/10.1007/s00159-022-00140-3 arXiv:2109.13614 [astro-ph.GA]

    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

  9. [9]

    The kinematic imprinting of environmental quenching in $z<0.2$ galaxies

    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/10.48550/arXiv.2603.03432 arXiv:2603.03432 [astro-ph.GA]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.2603.03432 2026

  10. [10]

    Ram-Pressure Stripping of Galaxies in High-Redshift Clusters and Influence of ICM Heating

    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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/319811 2001

  11. [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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stu2293 2015

  12. [13]

    The implications of the surprising existence of a large, massive CO disk in a distant protocluster

    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., Wylezalek, D.: The implications of the 29 surprising existence of a large, massive...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201730449 2017

  13. [14]

    Revealing environmental dependence of molecular gas content in a distant X-ray cluster at z=2.51

    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 Cluster at z = 2.51. ApJL867(2), 29 (2018) https://doi.org/10.3847/2041-8213/aaeb...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/2041-8213/aaeb2c 2018

  14. [15]

    Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing

    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) https://doi.org/10.1093/mnras/ stz361 arXiv:1901.03336 [astro-ph.GA]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/ 2019

  15. [16]

    Ram-pressure stripping caught in action in a young cluster at $z = 2.51$

    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 Big Bang. arXiv e-prints, 2503–21724 (2025) https://doi.org/10.48550/arXiv.2503....

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.2503.21724 2025

  16. [17]

    A Post-starburst Galaxy Undergoing Ram-pressure Stripping at Redshift 3.06

    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 at Redshift 3.06. arXiv e-prints, 2604–11892 (2026) https://doi.org/10.48550/arX...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.2604.11892 2026

  17. [18]

    Extragalactic millimeter-wave sources in South Pole Telescope survey data: source counts, catalog, and statistics for an 87 square-degree field

    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., High, F.W., Holder, G.P., Holzapfel, W.L., Hrubes, J.D., Joy, M., Keisler, R., K...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/ 2010

  18. [19]

    A massive core for a cluster of galaxies at a redshift of 4.3

    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., Lacaille, K., Litke, K.C., Ma, J., Malkan, M., Marrone, D.P., Morningstar, W., ...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1038/s41586-018-0025-2 2018

  19. [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., Spilker, J., Vieira, J.D., Weiß, A.: Megaparsec-scale structure around the protoclust...

    work page doi:10.1093/mnras/staa1275 2020

  20. [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.: Bright [CII]158µm Streamers as a Beacon for Giant Galaxy Formation in SPT2349−56 at...

    work page doi:10.48550/arxiv.2509.08035 2025

  21. [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., Vieira, J.D., Vizgan, D., Wang, G., Weiss, A.: An Overabundance of Radio-AGN ...

    work page doi:10.48550/arxiv.2511.17814 2025

  22. [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, J.D., Vizgan, D., Wang, G.C.P., Weiß, A.: Sunyaev-Zeldovich detection of hot in...

    work page doi:10.1038/s41586-025-09901-3 2026

  23. [24]

    The Evolution of Galaxies in and around Clusters at High-Redshift

    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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/pasj/56.4.621 2004

  24. [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]

    work page doi:10.1051/0004-6361/201935394 2019

  25. [26]

    The effect of ram pressure on the star formation, mass distribution and morphology of galaxies

    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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/200811551 2009

  26. [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-Zavadsky, M., Fujimoto, S., Gruppioni, C., Hathi, N.P., Hemmati, S., Ibar, E., J...

    work page doi:10.3847/1538-4365/ 2020

  27. [29]

    The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift

    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., Coogan, R.T.: The [C II] emission as a molecular gas mass tracer in galaxies at lo...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/sty2394 1976

  28. [30]

    Cool Gas in High Redshift Galaxies

    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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1146/annurev-astro-082812-140953 2013

  29. [31]

    A survey of the cold molecular gas in gravitationally lensed star-forming galaxies at z>2

    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., Collier, J.D.: A survey of the cold molecular gas in gravitationally lensed star...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stw275 2016

  30. [32]

    , keywords =

    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/10.1111/j.1365-2966.2010. 18028.x arXiv:1009.0749 [astro-ph.CO]

    work page doi:10.1111/j.1365-2966.2010 1913

  31. [33]

    ISM masses and the star formation law at Z = 1 to 6 // ALMA observations of dust continuum in 145 galaxies in the COSMOS survey field

    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 and the Star formation Law at Z = 1 to 6: ALMA Observations of Dust Continuum in 1...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/0004-637x/820/2/83 2016

  32. [34]

    GASP. X: APEX detection of molecular gas in the tails and in the disks 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(2), 2508–2520 (2018) https: //doi.org/10.1093/mnras/sty2021 arXiv:1803.06183 [a...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/sty2021 2018

  33. [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: Does Ram Pressure Promote Molecular Gas Formation? ApJ889(1), 9 (2020) https://doi...

    work page doi:10.3847/1538-4357/ab616a 2020

  34. [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., Omizzolo, A.: GASP XXIII: A Jellyfish Galaxy as an Astrophysical Laboratory of...

    work page doi:10.3847/1538-4357/ab5224 2019

  35. [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/s41550-021-01516-8 arXiv:2103.09205 [astro-ph.GA]

    work page doi:10.1038/s41550-021-01516-8 2021

  36. [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 Abell 2465. ApJ908(2), 228 (2021) https: //doi.org/10.3847/1538-4357/abd71e arXiv:...

    work page doi:10.3847/1538-4357/abd71e 2021

  37. [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) https://doi.org/10.3847/ 1538-4357/ab3e6c arXiv:1905.13249 [astro-ph.GA]

    arXiv 2019

  38. [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), 5029–5043 (2020) https://doi.org/10.1093/ mnras/staa968 arXiv:2004.04754 [astro-ph.GA]

    arXiv 2020

  39. [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]

    work page doi:10.1093/pasj/psae076 2024

  40. [43]

    Ackermann et al

    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]

    work page doi:10.3847/1538-4357/ 2024

  41. [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., Koyama, Y., Lehnert, M.D., Macgregor, P., Miley, G., Naufal, A., R¨ ottgering, H....

    work page doi:10.1051/0004-6361/202450785 2025

  42. [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]

    Pith/arXiv arXiv 2026

  43. [46]

    The Effects of Ram Pressure on the Cold Clouds in the Centers of Galaxy Clusters

    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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aaa843 2018

  44. [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

    work page doi:10.3847/1538-4357/ae4226 2026

  45. [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, K.M., Scott, D., Spilker, J., Vieira, J.D., Wang, G., Weiß, A.: Rapid build-up...

    work page doi:10.1093/mnras/stab3539 2022

  46. [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 effects in thez= 4.3 protocluster core SPT2349−56. arXiv e-prints, 2412–03790 (2024) h...

    work page doi:10.48550/arxiv.2412.03790 2024

  47. [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 at z = 4.3. ApJL982(1), 17 (2025) https://doi.org/10.3847/2041-8213/adb8d8 arXiv...

    work page doi:10.3847/2041-8213/adb8d8 2025

  48. [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 arXiv:2507.22826 [astro-ph.GA]

    work page doi:10.1051/0004-6361/202555071 2025

  49. [52]

    Enrichment of the ICM of galaxy clusters due to ram-pressure stripping

    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:astro-ph/0507605 [astro-ph]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361:20053921 2006

  50. [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., Drouart, G., Kodama, T., Koyama, Y., Lagos, C.D.P., Macgregor, P., Miley, G., Rodr´ ı...

    work page doi:10.1093/mnras/stad3128 2024

  51. [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]

    work page doi:10.3847/1538-4357/ae3824 2026

  52. [55]

    Metal enrichment of galaxies in a massive node of the Cosmic Web at $z \sim 3$

    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/arXiv.2511.19608 arXiv:2511.19608 [astro-ph.GA]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.2511.19608 2025

  53. [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]

    work page doi:10.3847/2041-8213/add1d4 2025

  54. [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, B.R.D., Robertson, B., Parlanti, E., Perna, M., ¨Ubler, H., Venturi, G., Witst...

    work page doi:10.1038/s41550-025-02751-z 2026

  55. [59]

    A first [CII] view of high-z quiescent galaxies

    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.2604.09347 arXiv:2604.09347 [astro-ph.GA]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.2604.09347 2026

  56. [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, M., Cimatti, A., Gruppioni, C., Hathi, N.P., Ibar, E., Koekemoer, A.M., Lemaux...

    arXiv 2020

  57. [61]

    PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

    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., Cox, P., Feruglio, C., Freundlich, J., Herrera-Camus, R., Juneau, S., Lippa, M.,...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aaa4b4 2018

  58. [62]

    Planck Collaboration et al.Astron

    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]

    work page doi:10.1051/0004-6361/ 2021

  59. [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, P., Bock, J.J., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F....

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201525830 2015

  60. [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., MacDonald, K., Bradley, L., Shanahan, C., Jamieson, W., Teodoro, M., Williams...

    work page doi:10.5281/zenodo.6984365

  61. [65]

    Gaia Data Release 3

    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., Panem, C., Pourbaix, D., Randich, S., Sartoretti, P., Soubiran, C., Tanga, P.,...

    work page doi:10.1051/0004-6361/202243940 2023

  62. [66]

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

  63. [67]

    CASA, the Common Astronomy Software Applications for Radio Astronomy

    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, J., McNichols, A., Mehringer, D., Miel, R., Moellenbrock, G., Montesino, F., Na...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1538-3873/ 2022

  64. [68]

    Bias-free Measurement of Giant Molecular Cloud Properties

    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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/502982 2006

  65. [69]

    , keywords =

    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., Belfiore, F., Beˇ sli´ c, I., Bigiel, F., Blanc, G.A., Bolatto, A.D., Boquien, M., Cao,...

    work page doi:10.3847/1538-4365/abec80 2021

  66. [70]

    2024, astropy/photutils: 2.0.2, 2.0.2 Zenodo, 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., Ginsburg, A., Jamieson, W., Barentsen, G., Craig, M., Morris, B.M., Perrin, M., Rathi...

    work page doi:10.5281/zenodo.13989456

  67. [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]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/316632 2000

  68. [72]

    , keywords =

    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

    work page doi:10.1111/j.1365-2966.2008.13535.x 2008

  69. [73]

    An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling

    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-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties D...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/806/1/ 2015

  70. [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]

    work page doi:10.3847/1538-4357/ab5fdd 2020

  71. [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]

    work page doi:10.48550/arxiv.2603.22945 2026

  72. [76]

    Gone with the heat: A fundamental constraint on the imaging of dust and molecular gas in the early Universe

    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.160025 arXiv:1605.03885 [astro- ph.GA]

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1098/rsos.160025 2016

  73. [77]

    Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift

    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, A., Toft, S., Masters, D.: Evolution of Interstellar Medium, Star Formation, an...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aa61a0 2017

  74. [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, C., Masters, D.: Cosmic Evolution of Gas and Star Formation. ApJ943(2), 82 (20...

    work page doi:10.3847/1538-4357/aca1bc 2023

  75. [79]

    , keywords =

    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.R., Mortier, A.M.J., Oliver, S., Papovich, C., P´ erez-Gonz´ alez, P.G., Pope, ...

    work page doi:10.1111/j.1365-2966.2007 2007

  76. [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: Kinematics of the Jellyfish Galaxy JO201. ApJ 844(1), 49 (2017) https://doi.org/1...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aa7875 2017

  77. [81]

    The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

    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 Kerkwijk, M.H., Robitaille, T.P., Merry, B., Bachetti, M., G¨ unther, H.M., Aldcroft, ...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/ac7c74 2022

  78. [82]

    astroquery: An Astronomical Web-Querying Package in Python

    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., Tollerud, E.J., de Val-Borro, M., Valtchanov, I., Woillez, J., Astroquery Collabor...

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-3881/aafc33 2019

  79. [83]

    Computing in Science and Engineering , keywords =

    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

    work page doi:10.1109/mcse.2007.55 2007

  80. [84]

    Harris and K

    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., Reddy, T., Weckesser, W., Abbasi, H., Gohlke, C., Oliphant, T.E.: Array program...

    work page doi:10.1038/s41586-020-2649-2 2020

Showing first 80 references.