SDSS J1004+4112 AGN
- Type
- AGN
- Status
- Confirmed
- Lensing
- Multiply imaged
- Lensing cluster
- SDSS J1004+4112 (z = 0.68)
- Redshift
- 1.734
Quasar at z = 1.734 lensed into four images up to 14.6 arcsec apart, the first quasar known to be lensed by a cluster (Inada et al. 2003); a faint fifth image lies near the brightest cluster galaxy (Inada et al. 2005). All the time delays are measured, the longest from a 14.5-year campaign (Muñoz et al. 2022), and are used for H0 measurements and to constrain the cluster's substructure. Microlensing of the images probes the quasar's accretion disc and broad-line region.
Papers
- Inada et al. (2003)
A gravitationally lensed quasar with quadruple images separated by 14.62 arcseconds - Williams & Saha (2004)
Models of the giant quadruple quasar SDSS J1004+4112 - Oguri et al. (2004)
Observations and theoretical implications of the large-separation lensed quasar SDSS J1004+4112 - Richards et al. (2004)
Microlensing of the broad emission line region in the quadruple lens SDSS J1004+4112 - Sharon et al. (2005)
Discovery of multiply imaged galaxies behind the cluster and lensed quasar SDSS J1004+4112 - Inada et al. (2005)
Discovery of a fifth image of the large separation gravitationally lensed quasar SDSS J1004+4112 - Lamer et al. (2006)
Strange magnification pattern in the large separation lens SDSS J1004+4112 from optical to X-rays - Ota et al. (2006)
Chandra observations of SDSS J1004+4112: constraints on the lensing cluster and anomalous X-ray flux ratios of the quadruply imaged quasar - Kawano & Oguri (2006)
Time delays for the giant quadruple lensed quasar SDSS J1004+4112: prospects for determining the density profile of the lensing cluster - Fohlmeister et al. (2007)
A time delay for the cluster-lensed quasar SDSS J1004+4112 - Fohlmeister et al. (2008)
The rewards of patience: an 822 day time delay in the gravitational lens SDSS J1004+4112 - Inada et al. (2008)
Spectroscopic confirmation of the fifth image of SDSS J1004+4112 and implications for the M_BH_-{sigma}* relation at z = 0.68 - Liesenborgs et al. (2009)
Non-parametric strong lens inversion of SDSS J1004+4112 - Oguri (2010)
The mass distribution of SDSS J1004+4112 revisited - Jackson (2011)
The faintest radio source yet: expanded very large array observations of the gravitational lens SDSS J1004+4112 - Mohammed et al. (2015)
Lensing time delays as a substructure constraint: a case study with the cluster SDSS J1004+4112 - Fian et al. (2016)
Size of the accretion disk in the graviationally lensed quasar SDSS J1004+4112 from the statistics of microlensing magnifications - Popović et al. (2020)
Spectroscopy and polarimetry of the gravitationally lensed quasar SDSS J1004+4112 with the 6m SAO RAS telescope - Hawkins (2020)
SDSS J1004+4112: the case for a galaxy cluster dominated by primordial black holes - Muñoz et al. (2022)
The Longest Delay: A 14.5 yr Campaign to Determine the Third Time Delay in the Lensing Cluster SDSS J1004+4112 - Forés-Toribio et al. (2022)
A Mass Model for the Lensing Cluster SDSS J1004+4112: Constraints from the Third Time Delay - Hutsemékers et al. (2023)
Microlensing of the broad emission line region in the lensed quasar J1004+4112 - Napier et al. (2023b)
Hubble Constant Measurement from Three Large-separation Quasars Strongly Lensed by Galaxy Clusters - Fian et al. (2024)
Probing the structure of the lensed quasar SDSS J1004+4112 through microlensing analysis of spectroscopic data - Martínez-Arrizabalaga et al. (2024)
Parameter-free Hubble constant from the quadruply lensed quasar SDSS J1004+4112 - Forés-Toribio et al. (2024)
Microlensing analysis of 14.5-year light curves in SDSS J1004+4112: Quasar accretion disk size and intracluster stellar mass fraction - Perera et al. (2024)
Free-form and hybrid lens models for SDSS J1004+4112: substructure and central image time delay constraints - Mediavilla et al. (2026)
Evidence for Substructure on the Inner Broad Line Region of the Lensed Quasar SDSS J1004+4112 from the Recurrence of Microlensing in the C IV Emission Line