ClG J1001+0220 , the SIMBAD biblio

ClG J1001+0220 , the SIMBAD biblio (54 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:35:32

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2015ApJ...812...43B viz 133       D     X         4 101 88 HerMES: ALMA imaging of Herschel-selected dusty star-forming galaxies. BUSSMANN R.S., RIECHERS D., FIALKOV A., et al.
2016ApJ...828...56W 1262 T     S   X C       29 24 157 Discovery of a galaxy cluster with a violently starbursting core at z = 2.506. WANG T., ELBAZ D., DADDI E., et al.
2016A&ARv..24...14O 83           X         2 19 176 The realm of the galaxy protoclusters. OVERZIER R.A.
2017ApJ...846L..31D 24     A               4 9 12 Radio selection of the most distant galaxy clusters. DADDI E., JIN S., STRAZZULLO V., et al.
2017MNRAS.469.2235K 238           X         6 20 5 Bimodal morphologies of massive galaxies at the core of a protocluster at z = 3.09 and the strong size growth of a brightest cluster galaxy. KUBO M., YAMADA T., ICHIKAWA T., et al.
2017ApJ...849..154S 40           X         1 24 20 ALMA pinpoints a strong overdensity of U/LIRGs in the massive cluster XCS J2215 at z = 1.46. STACH S.M., SWINBANK A.M., SMAIL I., et al.
2018Natur.556..469M 27     A               1 39 135 A massive core for a cluster of galaxies at a redshift of 4.3. MILLER T.B., CHAPMAN S.C., ARAVENA M., et al.
2018ApJ...862...64S 80           X         2 14 11 Deciphering the activity and quiescence of high-redshift cluster environments: ALMA observations of Cl J1449+0856 at z = 2. STRAZZULLO V., COOGAN R.T., DADDI E., et al.
2018ApJ...864...56J viz 47           X         1 14 98 "Super-deblended" dust emission in galaxies. II. Far-IR to (Sub)millimeter photometry and high-redshift galaxy candidates in the full COSMOS field. JIN S., DADDI E., LIU D., et al.
2018ApJ...867L..29W 628 T   A     X C       14 16 40 Revealing the environmental dependence of molecular gas content in a distant X-ray
Cluster at z = 2.51. 		WANG T., ELBAZ D., DADDI E., et al.
2018A&A...620A.198M 81             C       3 5 8 Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate. MARTINACHE C., RETTURA A., DOLE H., et al.
2019ApJ...870....7K 41           X         1 80 10 Spectroscopic confirmation of five galaxy clusters at z > 1.25 in the 2500 deg2 SPT-SZ survey. KHULLAR G., BLEEM L.E., BAYLISS M.B., et al.
2019ApJ...872..117G 1949     A D S   X C       47 52 44 Confirming Herschel candidate protoclusters from ALMA/VLA CO observations. GOMEZ-GUIJARRO C., RIECHERS D.A., PAVESI R., et al.
2019A&A...625A..96K 41           X         1 36 7 Using ALMA to resolve the nature of the early star-forming large-scale structure PLCK G073.4-57.5. KNEISSL R., POLLETTA M.D.C., MARTINACHE C., et al.
2019A&A...629A.104G 41           X         1 14 ~ Sunyaev-Zel'dovich detection of the galaxy cluster Cl J1449+0856 at z = 1.99: The pressure profile in uv space. GOBAT R., DADDI E., COOGAN R.T., et al.
2020A&A...635A..32C 16       D               1 127 ~ Molecular gas in distant brightest cluster galaxies. CASTIGNANI G., COMBES F., SALOME P., et al.
2020A&A...642A..37B 128           X         3 6 31 The DIANOGA simulations of galaxy clusters: characterising star formation in protoclusters. BASSINI L., RASIA E., BORGANI S., et al.
2020A&A...642A.155Z 124           X C       2 19 21 GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5. ZHOU L., ELBAZ D., FRANCO M., et al.
2021MNRAS.501.1803L 125           X C       2 18 15 Is there enough star formation in simulated protoclusters? LIM S., SCOTT D., BABUL A., et al.
2021ApJ...912...60S 43           X         1 5 8 Implications of the Environments of radio-detected active galactic nuclei in a complex protostructure at z ∼ 3.3. SHEN L., LEMAUX B.C., LUBIN L.M., et al.
2021A&A...649A..78D 169           X         4 15 44 Three Lyman-α-emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infall. DADDI E., VALENTINO F., RICH R.M., et al.
2021ApJ...915...32S 17       D               1 111 12 Spectroscopic confirmation of two extremely massive protoclusters, BOSS1244 and BOSS1542, at z = 2.24. SHI D.D., CAI Z., FAN X., et al.
2021A&A...652A..11J 142       D     X         4 23 12 COALAS. I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z = 2.16. JIN S., DANNERBAUER H., EMONTS B., et al.
2021A&A...654A.121P 476       D     X C       11 67 12 Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field. POLLETTA M., SOUCAIL G., DOLE H., et al.
2022ApJ...924...74A 85           X         2 17 7 The environmental dependence of gas properties in dense cores of a protocluster at z ∼ 2.5 revealed with ALMA. AOYAMA K., KODAMA T., SUZUKI T.L., et al.
2022ApJ...926...37M 43           X         1 29 27 Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent Galaxies. McCONACHIE I., WILSON G., FORREST B., et al.
2022ApJ...926L..21D 231       D     X         6 9 12 Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3. DADDI E., RICH R.M., VALENTINO F., et al.
2022A&A...662A..85P 145       D     X C       3 7 3 Molecular gas properties of Planck-selected protocluster candidates at z ≃ 1.3-3. POLLETTA M., DOLE H., MARTINACHE C., et al.
2022A&A...664A..63X 553 T         X C       11 8 5 Starbursts with suppressed velocity dispersion revealed in a forming
cluster at z = 2.51. 		XIAO M.-Y., WANG T., ELBAZ D., et al.
2022A&A...665L...7S 170           X C       3 23 4 A galaxy group candidate at z ≃ 3.7 in the COSMOS field. SILLASSEN N.B., JIN S., MAGDIS G.E., et al.
2022Natur.606..261W 33 3 X-ray astronomy comes of age. WILKES B.J., TUCKER W., SCHARTEL N., et al.
2023ApJ...950..191R 87             C       1 15 8 The Young and the Wild: What Happens to Protoclusters Forming at Redshift z ≈ 4? REMUS R.-S., DOLAG K. and DANNERBAUER H.
2023ApJ...951L..21X 897     A S   X C       19 1 ~ Accelerated Structural Evolution of Galaxies in a Starbursting Cluster at z = 2.51. XU C., WANG T., GU Q., et al.
2023A&A...678A..15C 44           X         1 18 ~ Bright submillimeter galaxies do trace galaxy protoclusters. CALVI R., CASTIGNANI G. and DANNERBAUER H.
2024MNRAS.528.6222B 18       D               2 104 ~ Characterization of Herschel-selected strong lens candidates through HST and sub-mm/mm observations. BORSATO E., MARCHETTI L., NEGRELLO M., et al.
2024A&A...683L...4J 90               F     1 14 ~ Cosmic Vine: A z = 3.44 large-scale structure hosting massive quiescent galaxies. JIN S., SILLASSEN N.B., MAGDIS G.E., et al.
2024A&A...684A.196Z 179           X C       3 9 ~ Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z = 3.95. ZHOU L., WANG T., DADDI E., et al.
2024ApJ...967L..34S 2625     A     X C       58 2 ~ JWST's First Glimpse of a z > 2 Forming Cluster Reveals a Top-heavy Stellar Mass Function. SUN H., WANG T., XU K., et al.
2024MNRAS.532.2842K 45           X         1 10 ~ MeerKAT observations of starburst galaxies and AGNs within the core of XMMXCS J2215.9-1738 at z = 1.46. KLUTSE D.Y., HILTON M., HEYWOOD I., et al.
2024MNRAS.532.4551L 45           X         1 25 ~ The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST. LIM S., TACCHELLA S., SCHAYE J., et al.
2024A&A...690A.285P 45           X         1 22 ~ JWST's PEARLS: Resolved study of the stellar and dust components in starburst galaxies at cosmic noon. POLLETTA M., FRYE B.L., GARUDA N., et al.
2025MNRAS.536.2000L 93           X         2 13 ~ A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon. LIU S., ZHENG X.Z., GONZALEZ V., et al.
2025A&A...693L...1G 93           X         2 6 ~ Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at z = 2.363 and CARLA-Ser J0950+2743 at z = 2.243. GRISHIN K.A., MEI S., CHILINGARIAN I.V., et al.
2024ApJ...977..204A 45           X         1 6 ~ Modeling the Multiwavelength Detection of Protoclusters. I. An Excess of Submillimeter Galaxies in Protocluster Cores. ARAYA-ARAYA P., COCHRANE R.K., HAYWARD C.C., et al.
2025ApJ...978...17M 47           X         1 22 ~ MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters. McCONACHIE I., WILSON G., FORREST B., et al.
2025A&A...696A.236P 112       D     X         3 55 ~ COALAS III. The ATCA CO(1-0) look at the growth and death of Hα emitters in the Spiderweb protocluster at z = 2.16. PEREZ-MARTINEZ J.M., DANNERBAUER H., EMONTS B.H.C., et al.
2025ApJ...985...61F 47           X         1 3 ~ The HST-Hyperion Survey: Grism Observations of a z ∼ 2.5 Protosupercluster. FORREST B., SHEN L., LEMAUX B.C., et al.
2025A&A...697A.142E 560           X C       11 6 ~ Galaxy populations of protoclusters in cosmological hydrodynamical simulations. ESPOSITO M., BORGANI S., STRAZZULLO V., et al.
2025A&A...697A.197T viz 19       D               1 3 ~ The COSMOS-Web deep galaxy group catalog up to z = 3.7. TONI G., GOZALIASL G., MATURI M., et al.
2025A&A...698A.204H 93             C       2 21 ~ An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclusters. HILL R., DEL CARMEN POLLETTA M., BETHERMIN M., et al.
2025ApJ...990L..24P 140           X         3 3 ~ UNCOVER/MegaScience: No Evidence of Environmental Quenching in a z ∼ 2.6 Protocluster. PAN R., SUESS K.A., MARCHESINI D., et al.
2025ApJ...993L..49S 513           X C       10 4 ~ The Bigfoot: A Footprint of a Coma Cluster Progenitor at z = 3.98. SUN H., WANG T., DADDI E., et al.
2026A&A...706A.344S 50           X         1 5 ~ Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z = 3.44. SILLASSEN N.B., JIN S., MAGDIS G.E., et al.
2026ApJ..1000L..10C 50           X         1 18 ~ An Overabundance of Radio Active Galactic Nuclei in the SPT2349-56 Protocluster: Preheating the Intracluster Medium. CHAPMAN S.C., DEANE R.P., ZHOU D., et al.

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