[DLR2016] PC 217.96+32.3 , the SIMBAD biblio

[DLR2016] PC 217.96+32.3 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:36:32


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Title First 3 Authors
2014ApJ...796..126L 3                   Z 4 24 Discovery of a very large structure at z = 3.78. LEE K.-S., DEY A., HONG S., et al.
2016ApJ...823...11D viz 1361     A S   X C       33 174 25 Spectroscopic confirmation of a protocluster at z∼3.786. DEY A., LEE K.-S., REDDY N., et al.
2017ApJ...837..172X 200       S   X         4 6 23 The diversity of diffuse Lyα nebulae around star-forming galaxies at high redshift. XUE R., LEE K.-S., DEY A., et al.
2018ApJ...862...24L 482           X C       11 12 3 Discovery of a very large (≃20 kpc) galaxy at z = 3.72. LEE K.-S., DEY A., MATHESON T., et al.
2019ApJ...871...83S 1121     A     X C       27 6 4 A census of galaxy constituents in a Coma progenitor observed at z > 3. SHI K., LEE K.-S., DEY A., 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.
2020MNRAS.493.3223F 46           X         1 2 11 The faint host galaxies of C IV absorbers at z > 5. FINLATOR K., DOUGHTY C., CAI Z., et al.
2021MNRAS.501.1803L 42           X         1 18 15 Is there enough star formation in simulated protoclusters? LIM S., SCOTT D., BABUL A., 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.
2024ApJ...962...36L 45           X         1 7 ~ The One-hundred-deg2 DECam Imaging in Narrowbands (ODIN): Survey Design and Science Goals. LEE K.-S., GAWISER E., PARK C., 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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