NAME USS 1558-003 Protocluster , the SIMBAD biblio

NAME USS 1558-003 Protocluster , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST14:45:23

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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
2012ApJ...757...15H 444 T   A     X C       10 13 76 A starbursting proto-cluster in making associated with a radio galaxy at z = 2.53 discovered by Hα imaging. HAYASHI M., KODAMA T., TADAKI K.-I., et al.
2014ApJ...788L..23T 371 T   A S   X C       7 8 15 Evidence for a gas-rich major merger in a
proto-cluster at z = 2.5. 		TADAKI K.-I., KODAMA T., TAMURA Y., et al.
2014MNRAS.441L...1S 932     A D S   X C F     22 5 33 Identification of the progenitors of rich clusters and member galaxies in rapid formation at z > 2. SHIMAKAWA R., KODAMA T., TADAKI K.-I., et al.
2016ApJ...826L..28H 103     A       C       2 3 9 Enhanced star formation of less massive galaxies in a protocluster at z = 2.5. HAYASHI M., KODAMA T., TANAKA I., et al.
2017MNRAS.468L..21S 466     A     X C F     10 1 11 Direct evidence for Ly{alpha } depletion in the protocluster core. SHIMAKAWA R., KODAMA T., HAYASHI M., et al.
2017A&A...608A..48D viz 159           X C       3 33 61 The implications of the surprising existence of a large, massive CO disk in a distant protocluster. DANNERBAUER H., LEHNERT M.D., EMONTS B., et al.
2018MNRAS.473.1977S viz 1332     A D S   X C F     31 6 42 MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z = 2.5. SHIMAKAWA R., KODAMA T., HAYASHI M., et al.
2018MNRAS.481.5630S viz 1325           X C F     31 75 33 MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z = 2.2. SHIMAKAWA R., KOYAMA Y., ROTTGERING H.J.A., et al.
2019ApJ...874...54M viz 390 T   A     X C       8 14 11 The fraction of active galactic nuclei in the
USS 1558-003 Protocluster at z = 2.53. 		MACUGA M., MARTINI P., MILLER E.D., et al.
2019ApJ...883..142H 16       D               1 89 67 SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ∼ 6-7: strong associations of dusty star-forming galaxies. HARIKANE Y., OUCHI M., ONO Y., et al.
2019PASJ...71...40T 66     A     X         2 26 42 Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2. TADAKI K., KODAMA T. and HAYASHI M.
2020A&A...635A..32C 16       D               1 127 ~ Molecular gas in distant brightest cluster galaxies. CASTIGNANI G., COMBES F., SALOME P., et al.
2020ApJ...899....5I 165           X         4 4 ~ The UV luminosity function of protocluster galaxies at z ∼ 4: the bright-end excess and the enhanced star formation rate density. ITO K., KASHIKAWA N., TOSHIKAWA J., et al.
2020MNRAS.499.2104H 988     A D     X C F     23 3 ~ Are Ly α emitters segregated in protoclusters regions? HOUGH T., GURUNG-LOPEZ S., ORSI A., et al.
2021ApJ...915...32S 100       D     X         3 111 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...654A.121P 59       D     X         2 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 1643     A S   X C       37 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...70W 17       D               1 48 14 The Mass-Metallicity Relation at Cosmic Noon in Overdense Environments: First Results from the MAMMOTH-Grism HST Slitless Spectroscopic Survey. WANG X., LI Z., CAI Z., et al.
2023ApJ...958..170N 566     A D S   X         13 6 ~ Environmental Impacts on the Rest-frame UV Size and Morphology of Star-forming Galaxies at z ∼ 2. NAUFAL A., KOYAMA Y., SHIMAKAWA R., et al.
2024MNRAS.52710221P 1102 T   A S   X C F     21 3 ~ Enhanced star formation and metallicity deficit in the
USS 1558-003 forming protocluster at z = 2.53. 		PEREZ-MARTINEZ J.M., KODAMA T., KOYAMA Y., et al.
2024A&A...682A.186L 45           X         1 20 ~ Feeding and feedback processes in the Spiderweb proto-intracluster medium. LEPORE M., DI MASCOLO L., TOZZI P., et al.
2024MNRAS.531.2335D 4614   K A D S   X C F     101 4 ~ Star-formation activity of low-mass galaxies at the peak epoch of galaxy formation probed by deep narrow-band imaging. DAIKUHARA K., KODAMA T., PEREZ-MARTINEZ J.M., 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.
2025A&A...696A.236P 47           X         1 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.
2025A&A...697A.142E 140           X C       2 6 ~ Galaxy populations of protoclusters in cosmological hydrodynamical simulations. ESPOSITO M., BORGANI S., STRAZZULLO V., et al.
2025ApJ...990..225B 19       D               1 30 ~ Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation. BAXTER D.C., COIL A.L., NADLER E.O., et al.

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