PSS J1058+1245 , the SIMBAD biblio

PSS J1058+1245 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:44:23


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Title First 3 Authors
2001A&A...374..371O 70 164 A 1.2 mm MAMBO/IRAM-30 m survey of dust emission from the highest redshift PSS quasars. OMONT A., COX P., BERTOLDI F., et al.
2002MNRAS.329..149I 68 91 The SCUBA Bright Quasar Survey (SBQS): 850-µm observations of the z ≳ 4 sample. ISAAK K.G., PRIDDEY R.S., McMAHON R.G., et al.
2005AJ....129.2519V 24 70 X-ray lighthouses of the high-redshift universe. II. Further snapshot observations of the most luminous z≳4 quasars with Chandra. VIGNALI C., BRANDT W.N., SCHNEIDER D.P., 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.
2007MNRAS.377..657G 90       D         F     2 45 42 Evidence for overdensity around zem> 4 quasars from the proximity effect. GUIMARAES R., PETITJEAN P., ROLLINDE E., et al.
2007ApJ...665.1004J 2 61 301 The X-ray properties of the most luminous quasars from the Sloan Digital Sky Survey. JUST D.W., BRANDT W.N., SHEMMER O., et al.
2009ApJ...690..644G viz 15       D               1 1491 54 A full year's Chandra exposure on Sloan Digital Sky Survey quasars from the Chandra multiwavelength project. GREEN P.J., ALDCROFT T.L., RICHARDS G.T., et al.
2009A&A...508..133G viz 91       D       C       3 99 19 Damped and sub-damped Lyman-α absorbers in z > 4 QSOs. GUIMARAES R., PETITJEAN P., DE CARVALHO R.R., 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.
2015ApJ...815...33R viz 16       D               1 814 170 A Hubble diagram for quasars. RISALITI G. and LUSSO E.
2016MNRAS.462.3285P viz 16       D               1 100 20 Nature and statistical properties of quasar associated absorption systems in the XQ-100 Legacy Survey. PERROTTA S., D'ODORICO V., PROCHASKA J.X., et al.
2016A&A...594A..91L 80           X         2 98 78 XQ-100: A legacy survey of one hundred 3.5 ≤ z ≤ 4.5 quasars observed with VLT/X-shooter. LOPEZ S., D'ODORICO V., ELLISON S.L., et al.
2016MNRAS.463.3021B 16       D               3 33 15 Chemical abundances of the damped Lyman α systems in the XQ-100 survey. BERG T.A.M., ELLISON S.L., SANCHEZ-RAMIREZ R., et al.
2017MNRAS.464L..56B viz 16       D               1 30 7 On the selection of damped Lyman α systems using Mg II absorption at 2 < zabs < 4. BERG T.A.M., ELLISON S.L., PROCHASKA J.X., et al.
2017A&A...608A..84C 41           X         1 87 6 Solving the conundrum of intervening strong Mg II absorbers towards gamma-ray bursts and quasars. CHRISTENSEN L., VERGANI S.D., SCHULZE S., et al.
2019MNRAS.487.3305M viz 17       D               1 230 47 New constraints on quasar evolution: broad-line velocity shifts over 1.5 <= z <= 7.5. MEYER R.A., BOSMAN S.E.I. and ELLIS R.S.
2019ApJ...883..163B viz 17       D               1 199 41 The evolution of O I over 3.2 < z < 6.5: reionization of the circumgalactic medium. BECKER G.D., PETTINI M., RAFELSKI M., et al.
2019MNRAS.490.2542P viz 17       D               1 2245 ~ Unveiling the weak radio quasar population at z≥4. PERGER K., FREY S., GABANYI K.E., et al.
2021MNRAS.502.4009B viz 17       D               1 74 10 Sub-damped Lyman α systems in the XQ-100 survey - II. Chemical evolution at 2.4 <= z <= 4.3. BERG T.A.M., FUMAGALLI M., D'ODORICO V., et al.
2021MNRAS.505..689J 17       D               1 100 ~ Constraining the ratio of median pixel optical depth profile around z ∼ 4 quasars using the longitudinal proximity effect. JALAN P., CHAND H. and SRIANAND R.
2022MNRAS.512.2389D 18       D               1 143 10 The evolution of the Si IV content in the Universe from the epoch of reionization to cosmic noon. D'ODORICO V., FINLATOR K., CRISTIANI S., et al.
2023ApJ...948...35S 19       D               1 101 3 Evidence of First Stars-enriched Gas in High-redshift Absorbers. SACCARDI A., SALVADORI S., D'ODORICO V., et al.
2023MNRAS.526.3230L 99 ~ Virial black hole mass estimates of quasars in the XQ-100 legacy survey. LAI S., ONKEN C.A., WOLF C., et al.

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