QSO J2346+1247 , the SIMBAD biblio

QSO J2346+1247 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST11:02:33


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Title First 3 Authors
2005ApJ...629..636A 1 53 254 The connection between galaxies and intergalactic absorption lines at redshift 2≲z≲3. ADELBERGER K.L., SHAPLEY A.E., STEIDEL C.C., et al.
2007A&A...469..319N 61 135 Sulphur and zinc abundances in Galactic halo stars revisited. NISSEN P.E., AKERMAN C., ASPLUND M., et al.
2007ApJ...670...15R 111 T K                 19 16 The sightline to
Q2343-BX415: clues to galaxy formation in a quasar environment.
RIX S.A., PETTINI M., STEIDEL C.C., et al.
2009ApJ...697.2057L 79             C       1 43 347 The kiloparsec-scale kinematics of high-redshift star-forming galaxies. LAW D.R., STEIDEL C.C., ERB D.K., et al.
2010MNRAS.406.1435E 39           X         1 28 57 The nature of proximate damped Lyman α systems. ELLISON S.L., PROCHASKA J.X., HENNAWI J., et al.
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.
2012ApJ...745...85L 78             C       1 27 151 An HST/WFC3-IR morphological survey of galaxies at z = 1.5-3.6. I. Survey description and morphological properties of star-forming galaxies. LAW D.R., STEIDEL C.C., SHAPLEY A.E., et al.
2012ApJ...751...94R 16       D               1 15 46 Neutral hydrogen optical depth near star-forming galaxies at z ~ 2.4 in the Keck baryonic structure survey. RAKIC O., SCHAYE J., STEIDEL C.C., et al.
2012MNRAS.422.3370K viz 15       D               2 127 227 Spatial variation in the fine-structure constant - new results from VLT/UVES. KING J.A., WEBB J.K., MURPHY M.T., et al.
2013A&A...556A.140Z 54       D     X         2 249 20 The ESO UVES advanced data products quasar sample. I. Dataset and new NHI measurements of damped absorbers. ZAFAR T., POPPING A. and PEROUX C.
2013A&A...556A.141Z viz 54       D     X         2 252 158 The ESO UVES advanced data products quasar sample. II. Cosmological evolution of the neutral gas mass density. ZAFAR T., PEROUX C., POPPING A., et al.
2016MNRAS.458.4074Q viz 16       D               1 368 72 The ESO UVES advanced data products quasar sample - VI. Sub-damped Lyman α metallicity measurements and the circumgalactic medium. QUIRET S., PEROUX C., ZAFAR T., et al.
2017A&A...597A..79P viz 16       D               1 302147 367 The Sloan Digital Sky Survey Quasar Catalog: Twelfth data release. PARIS I., PETITJEAN P., ROSS N.P., et al.
2018A&A...613A..51P viz 16       D               1 525784 350 The Sloan Digital Sky Survey Quasar Catalog: Fourteenth data release. PARIS I., PETITJEAN P., AUBOURG E., et al.
2018MNRAS.477.5625F viz 16       D               1 605 5 Eclipsing damped Ly α systems in the Sloan Digital Sky Survey Data Release 12. FATHIVAVSARI H., PETITJEAN P., JAMIALAHMADI N., et al.
2018ApJ...866..119L 1341       D S   X C       32 11 4 Imaging spectroscopy of ionized gaseous nebulae around optically faint AGNs at redshift z ∼ 2. LAW D.R., STEIDEL C.C., CHEN Y., et al.
2019MNRAS.482.3458M viz 16       D               1 472 60 The UVES Spectral Quasar Absorption Database (SQUAD) data release 1: the first 10 million seconds. MURPHY M.T., KACPRZAK G.G., SAVORGNAN G.A.D., et al.
2020ApJ...888...85F viz 16       D               1 145239 ~ Ghostly strong Lyα absorbers: tracers of gas flows in the close vicinity of quasars? FATHIVAVSARI H.
2020ApJS..249...17R viz 16       D               1 525797 112 Spectral properties of quasars from Sloan Digital Sky Survey data release 14: the catalog. RAKSHIT S., STALIN C.S. and KOTILAINEN J.
2020ApJS..250....8L viz 16       D               1 750061 219 The Sloan Digital Sky Survey quasar catalog: Sixteenth Data Release. LYKE B.W., HIGLEY A.N., McLANE J.N., et al.
2020ApJ...904...28C viz 16       D               1 247 9 Mg II absorbers in high-resolution quasar spectra. I. Voigt profile models. CHURCHILL C.W., EVANS J.L., STEMOCK B., et al.
2026A&A...707A.178C 120       D       C       2 21 ~ The multiple coherence scales of C IV at cosmic noon. CORTES-MUNOZ H., LOPEZ S., TEJOS N., et al.

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