[HOO2019] HSC-z6PCC1 , the SIMBAD biblio

[HOO2019] HSC-z6PCC1 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST22:44:05


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2018NatAs...2..962J 2569       S   X C       62 47 40 A giant protocluster of galaxies at redshift 5.7. JIANG L., WU J., BIAN F., et al.
2019ApJ...879...28H 1 46 57 SILVERRUSH. VII. Subaru/HSC identifications of protocluster candidates at z ∼ 6-7: implications for cosmic reionization. HIGUCHI R., OUCHI M., ONO Y., et al.
2019ApJ...883..142H 2640     A D S   X C       64 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.497.5220C 66     A     X         2 1 ~ Protoclusters at z = 5.7: a view from the MultiDark galaxies. CUI W., QIAO J., DAVE R., et al.
2022ApJ...926..114O 85       S             1 24 8 Conditions for Direct Black Hole Seed Collapse near a Radio-loud Quasar 1 Gyr after the Big Bang. OVERZIER R.A.
2023ApJ...950..191R 87             C       1 15 8 The Young and the Wild: What Happens to Protoclusters Forming at Redshift z ≈ 4? REMUS R.-S., DOLAG K. and DANNERBAUER H.
2024MNRAS.532.4551L 45           X         1 25 ~ The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST. LIM S., TACCHELLA S., SCHAYE J., et al.
2025MNRAS.539.1834M 327           X C F     5 13 ~ FOREVER22: insights into star formation and clustering properties of protoclusters from simulations and JWST. MOROKUMA-MATSUI K., YAJIMA H. and ABE M.
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.

goto View the references in ADS