[ZCA2021] BOSS1542 , the SIMBAD biblio

[ZCA2021] BOSS1542 , the SIMBAD biblio (17 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST01:45:27


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Title First 3 Authors
2021MNRAS.500.4354Z 2576   K A     X C       61 7 12 MAMMOTH: confirmation of two massive galaxy overdensities at z = 2.24 with Hα emitters. ZHENG X.Z., CAI Z., AN F.X., et al.
2021ApJ...915...32S 5935 T   A D S   X C       140 111 12 Spectroscopic confirmation of two extremely massive protoclusters, BOSS1244 and
BOSS1542, at z = 2.24.
SHI D.D., CAI Z., FAN X., et al.
2022ApJ...926...70W 43           X         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.
2022MNRAS.512.4893Z 5023     A D     X C F     117 8 7 Submillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks. ZHANG Y., ZHENG X.Z., SHI D.D., et al.
2022ApJ...929L...8L 68     A     X         2 24 7 First Census of Gas-phase Metallicity Gradients of Star-forming Galaxies in Overdense Environments at Cosmic Noon. LI Z., WANG X., CAI Z., et al.
2023MNRAS.523.2422L 3482   K A D S   X C F     78 4 ~ What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24? LIU S., ZHENG X.Z., SHI D.D., et al.
2024MNRAS.533.2399C 45           X         1 22 ~ An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: an unbiased study of SMG environments measured with narrow-band imaging. CORNISH T.M., WARDLOW J., WADE H., et al.
2024ApJ...972...51L 45           X         1 4 ~ Lyα Imaging around the Hyperluminous Dust-obscured Quasar W2246-0526 at z = 4.6. LUO Y., FAN L., LIANG Y., et al.
2024ApJS..275...27L viz 45           X         1 4 ~ MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Lyα Nebulae at Cosmic Noon. LI M., ZHANG H., CAI Z., et al.
2025MNRAS.536.2000L 513       S   X         10 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.
2025PASJ...77...21S 187           X         4 13 ~ Galaxy morphologies revealed with Subaru HSC and super-resolution techniques. II. Environmental dependence of galaxy mergers at z ∼ 2-5. SHIBUYA T., ITO Y., ASAI K., et al.
2025ApJ...988...47N 47           X         1 9 ~ LATIS: A Sample of IGM-selected Protoclusters and Protogroups at z ∼ 2.5. NEWMAN A.B., QEZLOU M., RUDIE G.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.
2025ApJ...991..183W 93           X         2 9 ~ Active Galactic Nuclei in the Extremely Overdense Galaxy Region BOSS 1441: A Chandra Observation. WU J., DOU L., CAI Z., et al.
2025ApJ...993..231Z 1045       D     X C       22 6 ~ MAMMOTH-MOSFIRE: Environmental Effects on Galaxy Interstellar Medium at z ∼ 2. ZHOU H., WANG X., MALKAN M.A., et al.
2026ApJ...997...95Y 670       D     X C       13 69 ~ MAMMOTH-Grism: Revisiting the Mass-Metallicity Relation in Protocluster Environments at Cosmic Noon. YANG Y., WANG X., HE X., et al.
2026A&A...706A..55G 70       D     X         2 5 ~ The HST-Hyperion Survey: Companion fraction and overdensity in a z ∼ 2.5 proto-supercluster. GIDDINGS F., LEMAUX B.C., FORREST B., et al.

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