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[LLC2018] PCl J1001+0220 , the SIMBAD biblio

[LLC2018] PCl J1001+0220 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.09.27CEST07:59:46

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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...615A..77L 12534 T   A S   X C       297 5 55 The VIMOS Ultra-Deep Survey: Emerging from the dark, a massive
proto-cluster at z ∼ 4.57. 		LEMAUX B.C., LE FEVRE O., CUCCIATI O., et al.
2019ApJ...883..142H 17       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.491L..18J 44           X         1 9 ~ The ALPINE-ALMA [C II] Survey: a triple merger at z 4.56. JONES G.C., BETHERMIN M., FUDAMOTO Y., et al.
2020MNRAS.496..875R 87           X         2 11 ~ The ALPINE-ALMA [C II] Survey: on the nature of an extremely obscured serendipitous galaxy. ROMANO M., CASSATA P., MORSELLI L., et al.
2020A&A...643A...7G 440           X C       9 5 27 The ALPINE-ALMA [CII] survey. Circumgalactic medium pollution and gas mixing by tidal stripping in a merging system at z ∼ 4.57. GINOLFI M., JONES G.C., BETHERMIN M., et al.
2021A&A...646A..76L 235           X C       4 4 44 The ALPINE-ALMA [C II] survey. Luminosity function of serendipitous [C II] line emitters at z ∼ 5. LOIACONO F., DECARLI R., GRUPPIONI C., et al.
2021MNRAS.502.1797R 45           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.
2021A&A...653A.111R 48           X         1 6 21 The ALPINE-ALMA [CII] survey. The contribution of major mergers to the galaxy mass assembly at z ∼ 5. ROMANO M., CASSATA P., MORSELLI L., et al.
2021ApJ...921....4H 49           X         1 1 4 The role of dust, UV luminosity and large-scale environment on the escape of Lyα photons: a case study of a protocluster field at z = 3.1. HUANG Y., LEE K.-S., SHI K., et al.
2022MNRAS.511.1303V 47           X         1 13 6 The ALPINE-ALMA [C II] survey: Investigation of 10 galaxies at z ∼ 4.5 with [O II] and [C II] line emission - ISM properties and [O II]-SFR relation. VANDERHOOF B.N., FAISST A.L., SHEN L., et al.
2022ApJ...926...37M 47           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.
2022A&A...662A..33L 941           X C       19 3 26 The VIMOS Ultra Deep Survey: The reversal of the star-formation rate - density relation at 2 < z < 5. LEMAUX B.C., CUCCIATI O., LE FEVRE O., et al.
2022ApJ...935..177S 47           X         1 5 ~ The ALPINE-ALMA [C II] Survey: The Infrared-Radio Correlation and Active Galactic Nucleus Fraction of Star-forming Galaxies at z ∼ 4.4-5.9. SHEN L., LEMAUX B.C., LUBIN L.M., et al.

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2023.09.27-07:59:46

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