FBQ1633+3134*

Pan-STARRS
gri
riz
izY
g
r
i
z
Y

HST

F160W

Gaia DR2
ImageGBPRPBP-RPparallax (mas)pmra (mas)pmdec (mas)PMSIGAENAEN sigSource ID
117.421 17.427 16.814 0.613 -0.096 ±0.102 0.456 ±0.177 0.681 ±0.199 4.284 0.465 4.565 1324266274238816256
219.123 nan nan nan nan ±nan nan ±nan nan ±nan nan 0.816 1.057 1324266274240202240
Gaia DR1
ImageGAENAEN sigSource ID
117.378 0.800 8.928 1324266274238816256
NameRADECbW1-W2z qsoz lenssep.NGaia densityGDR1 countGDR2 countNEDSDSS DR14PanSTARRSDECaLSGaia cutoutWISE modelWISEFIRSTNVSSSUMSSGaiaCFHT cutoutCFHT searchDiscovery
FBQ1633+3134*248.4540831.5699741.1.4931.5180.684?0.662825012NED LinkSDSS DR14 LinkPanSTARRS LinkDECaLSGDR2 cutoutWISE modelWISEFIRST
GaiaCFHT cutoutCFHT searchMorgan et al. 2001



Relevant Publications

Nov 2000: The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low-Density Environments, Kochanek et al. 2000

Feb 2001: The Gravitational Lens Candidate FBQ 1633+3134, Morgan et al. 2001

00 2002: New optical surveys for gravitationally lensed quasars, Morgan 2002

00 2002: Quasar Lensing, Courbin, Saha & Schechter 2002

Jan 2002: Annual Reports of Astronomical Observatories and Departments: Lawrence Livermore National Laboratory, Physics and Advanced Technologies Directorate, Institute of Geophysics and Planetary Physics, 2002

May 2003: A catalog of secondary photometric standard stars around gravitational lenses, Nakos et al. 2003

Dec 2007: How robust are the constraints on cosmology and galaxy evolution from the lens-redshift test?, Capelo & Natarajan 2007

Jan 2008: Origin of chromatic features in multiple quasars. Variability, dust, or microlensing, Yonehara, Hirashita & Richter 2008

Feb 2008: The Sloan Digital Sky Survey Quasar Lens Search. II. Statistical Lens Sample from the Third Data Release, Inada et al. 2008

May 2011: Cusped mass density profiles and magnification ratios of double-image gravitational lenses, Mutka 2011

Dec 2011: Black Hole Mass Estimates Based on C IV are Consistent with Those Based on the Balmer Lines, Assef et al. 2011

Mar 2019: Microlensing flux ratio predictions for Euclid, Vernardos 2019

Jun 2019: Testing dark energy models with a new sample ofstrong-lensing systems, Amante et al. 2019