NAME HS 1549 Protocluster , the SIMBAD biblio

NAME HS 1549 Protocluster , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:08:18


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Title First 3 Authors
2011ApJ...736..160S 106           X         2 5 305 Diffuse Lyα emitting halos: a generic property of high-redshift star-forming galaxies. STEIDEL C.C., BOGOSAVLJEVIC M., SHAPLEY A.E., et al.
2019MNRAS.488.1790L 146     A     X         4 72 7 Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity. LACAILLE K.M., CHAPMAN S.C., SMAIL I., 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.
2021A&A...654A.121P 42           X         1 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.
2023ApJ...947...75K 261           X         6 4 2 UV and Lyα Halos of Lyα Emitters across Environments at z = 2.84. KIKUTA S., MATSUDA Y., INOUE S., et al.
2024A&A...692A..22Z 90             C       1 21 ~ ASW2DF: Census of the obscured star formation in a galaxy cluster in formation at z = 2.2. ZHANG Y.H., DANNERBAUER H., PEREZ-MARTINEZ J.M., et al.
2025ApJ...983...69W 3807 T   A S   X C       79 13 ~ A 100 Mpc2 Structure Traced by Hyperluminous Galaxies around a Massive z = 2.85 Protocluster. WANG G.C.P., CHAPMAN S.C., SULZENAUER N., 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.
2025ApJ...993..111W 140           X C       2 17 ~ A Multiwavelength Study of ELAN Environments (AMUSE2): The Impact of Dense Environment on Massive Dusty Star-forming Galaxies at Cosmic Noon. WANG Y.-J., CHEN C.-C., ARRIGONI BATTAIA F., et al.

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