[KCH2000] L2 , the SIMBAD biblio

[KCH2000] L2 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.06CEST15:23:13

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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
1998ApJ...501L...5B 2 7 45 High-resolution optical and near-infrared imaging of the quadruple quasar RX J0911.4+0551. BURUD I., COURBIN F., LIDMAN C., et al.
1998Msngr..92...29B 6 2 RX J0911.4+0551: a complex quadruply imaged gravitationally lensed QSO. BURUD I., COURBIN F., LIDMAN C., et al.
2000ApJ...544L..35K 40 58 RX J0911+05: a massive cluster lens at z=0.769. KNEIB J.-P., COHEN J.G. and HJORTH J.
2001ApJ...555....1M 1 7 23 Chandra X-ray observations of the quadruply lensed quasar RX J0911.4+0551. MORGAN N.D., CHARTAS G., MALM M., et al.
2003MNRAS.344..924V 34 54 The Fundamental Plane and the evolution of the M/L ratio of early-type field galaxies up to z ∼ 1. VAN DE VEN G., VAN DOKKUM P.G. and FRANX M.
2005ApJ...632...58R 13 29 Expansion and collapse in the cosmic web. RAUCH M., BECKER G.D., VIEL M., et al.
2006ApJ...649..616P 3 60 362 Probing the coevolution of supermassive black holes and galaxies using gravitationally lensed quasar hosts. PENG C.Y., IMPEY C.D., RIX H.-W., et al.
2006ApJS..166..443E 45 43 Extinction curves of lensing galaxies out to z = 1. ELIASDOTTIR A., HJORTH J., TOFT S., et al.
2006ApJ...650L..17S 1 24 51 The Hubble time inferred from 10 time delay lenses. SAHA P., COLES J., MACCIO A.V., et al.
2007ApJ...660....1O 1 46 156 Gravitational lens time delays: a statistical assessment of lens model dependences and implications for the global Hubble constant. OGURI M.
2008A&A...478...95Y 108 21 Origin of chromatic features in multiple quasars. Variability, dust, or microlensing. YONEHARA A., HIRASHITA H. and RICHTER P.
2008A&A...481..615A 75               F     1 23 14 Integral field spectroscopy of four lensed quasars: analysis of their neighborhood and evidence for microlensing. ANGUITA T., FAURE C., YONEHARA A., et al.
2009ApJ...690..154S 38           X         1 41 23 The cluster lens ACO 1703: redshift contrast and the inner profile. SAHA P. and READ J.I.
2012A&A...538A..99S 77               F     1 72 70 COSMOGRAIL: the COSmological MOnitoring of GRAvItational lenses. X. Modeling based on high-precision astrometry of a sample of 25 lensed quasars: consequences for ellipticity, shear, and astrometric anomalies. SLUSE D., CHANTRY V., MAGAIN P., et al.
2012MNRAS.424..104L 93       D         F     2 22 8 Diagnostics of baryonic cooling in lensing galaxies. LEIER D., FERRERAS I. and SAHA P.
2012ApJ...755...31C viz 15       D               1 313 26 Testing the dark energy with gravitational lensing statistics. CAO S., COVONE G. and ZHU Z.-H.
2014MNRAS.437..600S 173       D     X         5 40 30 Hubble constant and dark energy inferred from free-form determined time delay distances. SERENO M. and PARAFICZ D.
2013RAA....13..803H 13 2 Gravitationally lensed extended sources : the case of QSO RX J0911. HOAI D.T., NHUNG P.T., ANH P.T., et al.
2015MNRAS.454..287J 16       D               2 45 23 Observations of radio-quiet quasars at 10-mas resolution by use of gravitational lensing. JACKSON N., TAGORE A.S., ROBERTS C., et al.
2016MNRAS.456..870B 177       D     X         5 26 8 Light versus dark in strong-lens galaxies: dark matter haloes that are rounder than their stars. BRUDERER C., READ J.I., COLES J.P., et al.
2018MNRAS.479.4796B 16       D               1 32 16 HST imaging of four gravitationally lensed quasars. BATE N.F., VERNARDOS G., O'DOWD M.J., et al.
2020MNRAS.491.6077G 21       D               1 35 163 Warm dark matter chills out: constraints on the halo mass function and the free-streaming length of dark matter with eight quadruple-image strong gravitational lenses. GILMAN D., BIRRER S., NIERENBERG A., et al.
2023MNRAS.522.1863P 19       D               1 17 ~ Constraints on the inner regions of lensing galaxies from central images using a recent AGN offset distribution. PERERA D., WILLIAMS L.L.R. and SCARLATA C.

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