NAME PSC J1001+0218 , the SIMBAD biblio

NAME PSC J1001+0218 , the SIMBAD biblio (17 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:01:59

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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
2018A&A...619A..49C 879     A     X C       21 5 62 The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS. CUCCIATI O., LEMAUX B.C., ZAMORANI G., et al.
2020ApJ...892....8D 169           X         4 5 21 Spectroscopic confirmation of a Coma Cluster progenitor at z ∼ 2.2. DARVISH B., SCOVILLE N.Z., MARTIN C., et al.
2020ApJ...898..159N                   Z 2 ~ Discovery of a supercluster candidate at z ∼ 1.1. NARWAL T., GOTO T., HASHIMOTO T., et al.
2021MNRAS.502.1797R 42           X         1 88 13 Optical and near-infrared observations of the SPT2349-56 proto-cluster core at z = 4.3. ROTERMUND K.M., CHAPMAN S.C., PHADKE K.A., et al.
2022NatAs...6..857A 783       D S   X C       17 10 9 Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations. ATA M., LEE K.-G., DALLA VECCHIA C., et al.
2022ApJ...941..134H 2027     A S   X C       46 3 5 Evaluating Lyα Emission as a Tracer of the Largest Cosmic Structure at z ∼ 2.47. HUANG Y., LEE K.-S., CUCCIATI O., et al.
2023ApJ...945L..28D 87           X         2 3 2 Observational Evidence for Large-scale Gas Heating in a Galaxy Protocluster at z = 2.30. DONG C., LEE K.-G., ATA M., et al.
2023MNRAS.523.5248B 46           X         1 2 5 The cosmic web in Lyman-alpha emission. BYROHL C. and NELSON D.
2023MNRAS.526L..56F 200     A     X         5 7 ~ Elentári:a massive proto-supercluster atZ ∼ 3.3 in the COSMOS field. FORREST B., LEMAUX B.C., SHAH E., 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.
2024MNRAS.529..873S 90           X         2 10 ~ Identification and characterization of six spectroscopically confirmed massive protostructures at 2.5 < z < 4.5. SHAH E.A., LEMAUX B., FORREST B., et al.
2024ApJ...966...18T 134           X C       2 7 ~ Large-scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4. TAAMOLI S., MOBASHER B., CHARTAB N., et al.
2024ApJ...971..169F 108       D     X         3 6 ~ Environmental Effects on the Stellar Mass Function in a z ∼ 3.3 Overdensity of Galaxies in the COSMOS Field. FORREST B., LEMAUX B.C., SHAH E.A., et al.
2025MNRAS.536.2000L 47           X         1 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.
2025ApJ...978...17M 140           X         3 22 ~ MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters. McCONACHIE I., WILSON G., FORREST B., et al.
2025ApJ...980..155H 233           X         5 8 ~ Discovering Large-scale Structure at 2 < z < 5 in the C3VO Survey. HUNG D., LEMAUX B.C., CUCCIATI O., et al.
2025A&A...698A.312G 6671 T   A D S   X C       141 3 ~ Gas properties as a function of environment in the proto-supercluster
Hyperion at z ∼ 2.45. 		GURURAJAN G., CUCCIATI O., LEMAUX B.C., et al.

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