SDSS J022550.67-042142.0 , the SIMBAD biblio

SDSS J022550.67-042142.0 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:39:03


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Title First 3 Authors
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2011A&A...533A..20P 2425     A D   O X C       64 16 24 Disk, merger, or outflow? Molecular gas kinematics in two powerful obscured QSOs at z≥3.4. POLLETTA M., NESVADBA N.P.H., NERI R., et al.
2013MNRAS.428.1281J viz 15       D               1 209883 256 The VISTA Deep Extragalactic Observations (VIDEO) survey. JARVIS M.J., BONFIELD D.G., BRUCE V.A., et al.
2013A&A...559A..14L viz 15       D               1 37850 306 The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z ∼ 6.7 selected with 17.5 ≤ iAB≤ 24.75. LE FEVRE O., CASSATA P., CUCCIATI O., et al.
2014A&A...572A..90L viz 15       D               1 4063 24 Hidden starbursts and active galactic nuclei at 0<z<4 from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback. LEMAUX B.C., LE FLOC'H E., LE FEVRE O., et al.
2018A&A...619A..90P 257       D     X C       6 23 12 Molecular gas content in obscured AGN at z > 1. PERNA M., SARGENT M.T., BRUSA M., et al.
2018PASJ...70S..10O viz 16       D               1 365 182 Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4-7 derived with the half-million dropouts on the 100 deg2 sky. ONO Y., OUCHI M., HARIKANE Y., et al.
2019ApJ...879....9S 16       D               1 98 24 How do galaxies trace a large-scale structure? A case study around a massive protocluster at z = 3.13. SHI K., HUANG Y., LEE K.-S., et al.
2022ApJS..259...20H viz 17       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., et al.

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