QSO B0105+1619 , the SIMBAD biblio

QSO B0105+1619 , the SIMBAD biblio (59 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.13CEST01:25:36


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Title First 3 Authors
1999A&AS..134..483H viz 274 35 The Hamburg Quasar Survey. III. Further new bright quasars. HAGEN H.-J., ENGELS D. and REIMERS D.
2001A&A...376..751P 2 2 13 Deuterium at high redshift: Primordial or evolved? PRANTZOS N. and ISHIMARU Y.
2001AJ....121.2843B viz 6250 77 Quasars in the 2MASS second incremental data release. BARKHOUSE W.A. and HALL P.B.
2001ApJ...552..718O 132 T K                 5 353 The deuterium to hydrogen abundance ratio toward a fourth QSO: HS 0105+1619. O'MEARA J.M., TYTLER D., KIRKMAN D., et al.
2001ApJ...560...41P 10 6 193 A new measurement of the primordial abundance of deuterium: toward convergence with the baryon density from the cosmic microwave background? PETTINI M. and BOWEN D.V.
2002A&A...395..789C 2 7 56 Evolution of deuterium, 3He and 4He in the Galaxy. CHIAPPINI C., RENDA A. and MATTEUCCI F.
2002ApJS..140....3M 2 22 156 Abundances of deuterium, nitrogen, and oxygen in the local interstellar medium: overview of first results from the FUSE mission. MOOS H.W., SEMBACH K.R., VIDAL-MADJAR A., et al.
2002PASA...19..238R 9 1 Big Bang nucleosynthesis, population III, and stellar genetics in the galactic halo. RYAN S.G.
2003ApJ...599..297H 31 68 The deuterium-to-oxygen ratio in the interstellar medium. HEBRARD G. and MOOS H.W.
2003ApJS..148..175S 204 16 9815 First-year Wilkinson microwave anisotropy probe (WMAP)(1) observations: determination of cosmological parameters. SPERGEL D.N., VERDE L., PEIRIS H.V., et al.
2003ApJS..149....1K 19 7 402 The cosmological baryon density from the Deuterium-to-Hydrogen ratio in QSO absorption systems: D/H toward Q1243+3047. KIRKMAN D., TYTLER D., SUZUKI N., et al.
2003MNRAS.339.1183P 57 67 The SCUBA Bright Quasar Survey (SBQS) - II. Unveiling the quasar epoch at submillimetre wavelengths. PRIDDEY R.S., ISAAK K.G., McMAHON R.G., et al.
2004ApJ...617...29O 3 21 207 A realistic determination of the error on the primordial helium abundance: steps toward nonparametric nebular helium abundances. OLIVE K.A. and SKILLMAN E.D.
2004ApJS..150..387S 24 67 The Deuterium-to-Hydrogen ratio in a low-metallicity cloud falling onto the Milky Way. SEMBACH K.R., WAKKER B.P., TRIPP T.M., et al.
2004MNRAS.355.1042C 1 11 47 Deuterium/hydrogen in a new Lyman limit absorption system at z= 3.256 towards PKS1937-1009. CRIGHTON N.H.M., WEBB J.K., ORTIZ-GIL A., et al.
2005MNRAS.360.1373K 1 24 72 The HI opacity of the intergalactic medium at redshifts 1.6 < z < 3.2. KIRKMAN D., TYTLER D., SUZUKI N., et al.
2006A&A...455..773V viz 108224 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2006MNRAS.369..295R 2 11 46 Deuterium astration in the local disc and beyond. ROMANO D., TOSI M., CHIAPPINI C., et al.
2007MNRAS.374..867P 22 17 A sensitive submillimetre survey of broad absorption-line quasars. PRIDDEY R.S., GALLAGHER S.C., ISAAK K.G., et al.
2008MNRAS.391.1499P 27       D               1 7 178 Deuterium abundance in the most metal-poor damped Lyman alpha system: converging on Ωb,0h2. PETTINI M., ZYCH B.J., MURPHY M.T., 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.
2010MNRAS.404.1583I 16       D               1 10 39 HD molecules at high redshift: the absorption system at z = 2.3377 towards Q 1232+082. IVANCHIK A.V., PETITJEAN P., BALASHEV S.A., et al.
2011MNRAS.415.1105S viz 284       D     X         8 392 10 Distance limits to intermediate- and high-velocity clouds. SMOKER J.V., FOX A.J. and KEENAN F.P.
2009PhR...472....1I 199           X C       4 19 401 Primordial nucleosynthesis: from precision cosmology to fundamental physics. IOCCO F., MANGANO G., MIELE G., et al.
2012ApJ...750...67R 22       D               1 17 270 The gaseous environment of high-z galaxies: precision measurements of neutral hydrogen in the circumgalactic medium of z ∼ 2-3 galaxies in the Keck baryonic structure survey. RUDIE G.C., STEIDEL C.C., TRAINOR R.F., 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.422.1700C 80           X         2 3 20 The kinetic temperature in a damped Lyman α absorption system in Q2206-199 - an example of the warm neutral medium. CARSWELL R.F., BECKER G.D., JORGENSON R.A., et al.
2012ApJ...752...39T 18       D               2 16 108 The halo masses and galaxy environments of hyperluminous QSOs at z ≃ 2.7 in the Keck baryonic structure survey. TRAINOR R.F. and STEIDEL C.C.
2012MNRAS.425.2477P 22       D               1 10 140 A new, precise measurement of the primordial abundance of deuterium. PETTINI M. and COOKE R.
2012ApJ...757L..30R 16       D               1 16 57 The temperature-density relation in the intergalactic medium at redshift $ < z$ > = 2.4. RUDIE G.C., STEIDEL C.C. and PETTINI M.
2011Sci...334.1245F 8 9 153 Detection of pristine gas two billion years after the Big Bang. FUMAGALLI M., O'MEARA J.M. and PROCHASKA J.X.
2013ApJ...769..146R 19       D               1 15 111 The column density distribution and continuum opacity of the intergalactic and circumgalactic medium at redshift $ < z$ > = 2.4. RUDIE G.C., STEIDEL C.C., SHAPLEY A.E., et al.
2013ApJ...775L...3T 17       D               1 8 31 Constraints on hyperluminous QSO lifetimes via fluorescent Lyα emitters at z ≃ 2.7. TRAINOR R. and STEIDEL C.C.
2014ApJ...781...31C 242       D S   X C       4 5 301 Precision measures of the primordial abundance of deuterium. COOKE R.J., PETTINI M., JORGENSON R.A., et al.
2014A&A...563A..54P viz 16       D               1 168926 217 The Sloan Digital Sky Survey quasar catalog: tenth data release. PARIS I., PETITJEAN P., AUBOURG E., et al.
2015ApJ...800...12C 254       D     X C       6 35 48 The most metal-poor damped Lyα systems: an insight into dwarf galaxies at high-redshift. COOKE R.J., PETTINI M. and JORGENSON R.A.
2015ApJ...804..110W 40           X         1 16 6 The chemical evolution of very metal-poor damped Lyα systems. WEBSTER D., BLAND-HAWTHORN J. and SUTHERLAND R.S.
2015ApJ...809...89T 17       D               1 40 125 The spectroscopic properties of Lyα-emitters at z ∼2.7: escaping gas and photons from faint galaxies. TRAINOR R.F., STEIDEL C.C., STROM A.L., et al.
2015AJ....150..111O viz 16       D               1 171 71 The first data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2016MNRAS.457..487Y 80               F     3 10 2 The physical nature of the most metal-poor damped Lyman α systems. YUAN S. and CEN R.
2016MNRAS.458.2188B 17       D               1 15 18 The primordial deuterium abundance: subDLA system at zabs = 2.437 towards the QSO J 1444+2919. BALASHEV S.A., ZAVARYGIN E.O., IVANCHIK A.V., et al.
2016ApJ...830..148C 32       D               1 6 98 The primordial deuterium abundance of the most metal-poor damped Lyman-α system. COOKE R.J., PETTINI M., NOLLETT K.M., 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.
2017MNRAS.467..802C 17       D               1 21 29 Discovery of the most metal-poor damped Lyman α system. COOKE R.J., PETTINI M. and STEIDEL C.C.
2017AJ....154..114O viz 16       D               4 298 26 The second data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2018ApJ...855..102C 62       D               1 7 322 One percent determination of the primordial deuterium abundance. COOKE R.J., PETTINI M. and STEIDEL C.C.
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.477.5536Z 16       D               1 14 12 The primordial deuterium abundance at zabs = 2.504 from a high signal-to-noise spectrum of Q1009+2956. ZAVARYGIN E.O., WEBB J.K., DUMONT V., et al.
2018PASP..130k4001P 16       D               1 15 ~ Median statistics analysis of deuterium abundance measurements and spatial curvature constraints. PENTON J., PEYTON J., ZAHOOR A., et al.
2019MNRAS.485..753H 602       D     X C       14 17 4 The SCUBA-2 web survey: I. Observations of CO(3-2) in hyper-luminous QSO fields. HILL R., CHAPMAN S.C., SCOTT D., et al.
2019ApJ...882...77C 17       D               2 73 40 Heavy element absorption systems at 5.0 < z < 6.8: metal-poor neutral gas and a diminishing signature of highly ionized circumgalactic matter. COOPER T.J., SIMCOE R.A., COOKSEY K.L., et al.
2019MNRAS.489.2536D 17       D               1 66 ~ Power spectrum of the flux in the Lyman-alpha forest from high-resolution spectra of 87 QSOs. DAY A., TYTLER D. and KAMBALUR B.
2019ApJ...887..205T 17       D               1 47 ~ Thermal state of the intergalactic medium at z ∼ 2-4. TELIKOVA K.N., SHTERNIN P.S. and BALASHEV S.A.
2020ApJ...888...85F viz 17       D               1 145239 ~ Ghostly strong Lyα absorbers: tracers of gas flows in the close vicinity of quasars? FATHIVAVSARI H.
2020ApJ...894....3O 17       D               3 49 28 The FLASHES survey. I. Integral field spectroscopy of the CGM around 48 z ≃ 2.3-3.1 QSOs. O'SULLIVAN D.B., MARTIN C., MATUSZEWSKI M., et al.
2020ApJS..249...17R viz 17       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 17       D               1 750060 219 The Sloan Digital Sky Survey quasar catalog: Sixteenth Data Release. LYKE B.W., HIGLEY A.N., McLANE J.N., et al.
2021A&A...651A..78N 17       D               1 12 9 Sharpening quasar absorption lines with ESPRESSO. Temperature of warm gas at z ∼ 2, constraints on the Mg isotopic ratio, and structure of cold gas at z ∼ 0.5. NOTERDAEME P., BALASHEV S., LEDOUX C., et al.
2022ApJ...929..158W 18       D               1 29 9 Oxygen-enhanced Extremely Metal-poor Damped Lyα Systems: A Signpost of the First Stars?. WELSH L., COOKE R., FUMAGALLI M., et al.

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