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ClG J1004+4112 , the SIMBAD biblio

ClG J1004+4112 , the SIMBAD biblio (45 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.10.03CEST15:45:48

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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
2003Natur.426..810I 9 6 167 A gravitationally lensed quasar with quadruple images separated by 14.62 arcseconds. INADA N., OGURI M., PINDOR B., et al.
2004ApJ...605...78O 3 9 100 Observations and theoretical implications of the large-separation lensed quasar SDSS J1004+4112. OGURI M., INADA N., KEETON C.R., et al.
2005ApJ...629L..73S 1 19 44 Discovery of multiply imaged galaxies behind the cluster and lensed quasar SDSS J1004+4112. SHARON K., OFEK E.O., SMITH G.P., et al.
2005PASJ...57L...7I 1 14 44 Discovery of a fifth image of the large separation gravitationally lensed quasar SDSS J1004+4112. INADA N., OGURI M., KEETON C.R., et al.
2006A&A...454..493L 1 7 18 Strange magnification pattern in the large separation lens SDSS J1004+4112 from optical to X-rays. LAMER G., SCHWOPE A., WISOTZKI L., et al.
2006ApJ...644..733G 28 20 Lens-Aided Multi-Angle Spectroscopy (LAMAS) reveals small-scale outflow structure in quasars. GREEN P.J.
2006ApJ...647..215O 2 7 28 Chandra observations of SDSS J1004+4112: constraints on the lensing cluster and anomalous X-ray flux ratios of the quadruply imaged quasar. OTA N., INADA N., OGURI M., et al.
2006PASJ...58..271K 7 11 Time delays for the giant quadruple lensed quasar SDSS J1004+4112: prospects for determining the density profile of the lensing cluster. KAWANO Y. and OGURI M.
2006ApJ...652L...5S 2 5 24 Two strong-lensing clusters confront universal dark matter profiles. SAHA P., READ J.I. and WILLIAMS L.L.R.
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.
2007ApJ...662...62F viz 2 8 32 A time delay for the cluster-lensed quasar SDSS J1004+4112. FOHLMEISTER J., KOCHANEK C.S., FALCO E.E., et al.
2007ApJ...663...29S 38   K                 15 25 Meso-structure in three strong-lensing systems. SAHA P., WILLIAMS L.L.R. and FERRERAS I.
2007MNRAS.379..190C 15       D               1 113 151 The observed concentration-mass relation for galaxy clusters. COMERFORD J.M. and NATARAJAN P.
2008MNRAS.388.1279I 18       D               1 6 43 A new independent limit on the cosmological constant/dark energy from the relativistic bending of light by Galaxies and clusters of Galaxies. ISHAK M., RINDLER W., DOSSETT J., et al.
2009ApJ...690..154S 114           X         3 41 23 The cluster lens ACO 1703: redshift contrast and the inner profile. SAHA P. and READ J.I.
2009MNRAS.396.1985Z 45           X         1 11 165 New multiply-lensed galaxies identified in ACS/NIC3 observations of Cl0024+1654 using an improved mass model. ZITRIN A., BROADHURST T., UMETSU K., et al.
2009ApJ...702..472R 38           X         1 9 8 The UV-Mid-IR spectral energy distribution of a z = 1.7 quasar host galaxy. ROSS N.R., ASSEF R.J., KOCHANEK C.S., et al.
2008PASJ...60L..27I 11 13 Spectroscopic confirmation of the fifth image of SDSS J1004+4112 and implications for the MBH-σ* relation at z = 0.68. INADA N., OGURI M., FALCO E.E., et al.
2010AJ....139.1935S 38           X         1 8 0 The optimal gravitational lens telescope. SURDEJ J., DELACROIX C., COLEMAN P., et al.
2010ApJ...718..876S 284       D     X   F     7 81 30 The type Ia supernova rate in redshift 0.5-0.9 galaxy clusters. SHARON K., GAL-YAM A., MAOZ D., et al.
2010MNRAS.408.1916Z 38           X         1 66 42 Full lensing analysis of Abell 1703: comparison of independent lens-modelling techniques. ZITRIN A., BROADHURST T., UMETSU K., et al.
2011MNRAS.414.1840M 40           X         1 6 23 A weak lensing detection of the cosmological distance–redshift relation behind three massive clusters. MEDEZINSKI E., BROADHURST T., UMETSU K., et al.
2011ApJ...739L..28J 15 8 The faintest radio source yet: expanded very large array observations of the gravitational lens SDSS J1004+4112. JACKSON N.
2012MNRAS.420.3213O 174       D       C F     6 34 203 Combined strong and weak lensing analysis of 28 clusters from the Sloan giant arcs survey. OGURI M., BAYLISS M.B., DAHLE H., et al.
2012ApJ...755...82M 27 21 Measuring microlensing using spectra of multiply lensed quasars. MOTTA V., MEDIAVILLA E., FALCO E., et al.
2012MNRAS.425.1215K viz 796       D S   X         20 18 9 A multiwavelength survey of AGN in massive clusters: AGN detection and cluster AGN fraction. KLESMAN A.J. and SARAJEDINI V.L.
2013ApJ...774...70M 39           X         1 5 9 Tangential velocity of the dark matter in the Bullet cluster from precise lensed image redshifts. MOLNAR S.M., BROADHURST T., UMETSU K., et al.
2014MNRAS.437..600S 95       D     X         3 40 30 Hubble constant and dark energy inferred from free-form determined time delay distances. SERENO M. and PARAFICZ D.
2014MNRAS.442..314K 16       D               2 14 4 A multi-wavelength survey of AGN in massive clusters: AGN distribution and host galaxy properties. KLESMAN A.J. and SARAJEDINI V.L.
2015PASJ...67...21M 963 T     S   X C       21 19 5 Lensing time delays as a substructure constraint: a case study with the
cluster SDSS J1004+4112. 		MOHAMMED I., SAHA P. and LIESENBORGS J.
2015MNRAS.449.2024S 16       D               1 105 30 The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects. SERENO M., GIOCOLI C., ETTORI S., et al.
2015MNRAS.450.3665S viz 16       D               1 429 35 CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). SERENO M.
2015MNRAS.454..287J 16       D               1 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.455..892G viz 16       D               4 351 14 The galaxy cluster concentration-mass scaling relation. GROENER A.M., GOLDBERG D.M. and SERENO M.
2016ApJ...830..149F 81           X         2 6 4 Size of the accretion disk in the graviationally lensed quasar SDSS J1004+4112 from the statistics of microlensing magnifications. FIAN C., MEDIAVILLA E., HANSLMEIER A., et al.
2018ApJ...859...65Y 17       D               2 23 15 X-ray properties of AGN in brightest cluster galaxies. I. A systematic study of the Chandra archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 redshift range. YANG L., TOZZI P., YU H., et al.
2018MNRAS.480.2236A 1689       D S   X C       39 16 4 The rise and fall of the UV upturn: z = 0.3, 0.55, and 0.7. ALI S.S., BREMER M.N., PHILLIPPS S., et al.
2019ApJ...879...35D 29 ~ Constraining quasar relativistic reflection regions and spins with microlensing. DAI X., STEELE S., GUERRAS E., et al.
2021ApJ...911...82C viz 18       D               1 387 ~ Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. CORASANITI P.-S., SERENO M. and ETTORI S.
2021AJ....162..175O 108       D     X         3 7 ~ Multiple Mg II absorption systems in the lines of sight to quadruply lensed quasar H1413+1143. OKOSHI K., MINOWA Y., KASHIKAWA N., et al.
2021ApJ...923...12A 376       D     X C       8 21 2 Evolution of the ultraviolet upturn at 0.3 < z < 1: exploring helium-rich stellar populations. ALI S.S., DE PROPRIS R., CHUNG C., et al.
2022ApJ...937...34M 467 T         X C       8 9 6 The Longest Delay: A 14.5 yr Campaign to Determine the Third Time Delay in the Lensing Cluster
SDSS J1004+4112. 		MUNOZ J.A., KOCHANEK C.S., FOHLMEISTER J., et al.
2022ApJ...937...35F 261 T   A     X         5 8 5 A Mass Model for the Lensing Cluster
SDSS J1004+4112: Constraints from the Third Time Delay. 		FORES-TORIBIO R., MUNOZ J.A., KOCHANEK C.S., et al.
2023ApJ...946...63M 70       D     X         2 12 6 COOL-LAMPS. III. Discovery of a 25.″9 Separation Quasar Lensed by a Merging Galaxy Cluster. MARTINEZ M.N., NAPIER K.A., CLOONAN A.P., et al.
2023A&A...672A..45H 50           X         1 6 1 Microlensing of the broad emission line region in the lensed quasar J1004+4112. HUTSEMEKERS D., SLUSE D., SAVIC D., et al.

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2023.10.03-15:45:49

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