Quasar lenses and pairs in the VST-ATLAS and Gaia

被引:32
作者
Agnello, A. [1 ]
Schechter, P. L. [2 ]
Morgan, N. D. [3 ]
Treu, T. [4 ]
Grillo, C. [5 ,6 ]
Malesani, D. [6 ]
Anguita, T. [7 ,8 ]
Apostolovski, Y. [7 ]
Rusu, C. E. [9 ,10 ]
Motta, V. [11 ]
Rojas, K. [11 ]
Chehade, B. [12 ]
Shanks, T. [12 ]
机构
[1] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[2] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[3] Staples High Sch, Westport, CT 06880 USA
[4] PAB, Dept Phys & Astron, 430 Portola Plaza,Box 951547, Los Angeles, CA 90095 USA
[5] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy
[6] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark
[7] Univ Andres Bello, Dept Ciencias Fis, Fernandez Concha 700, Santiago, Chile
[8] Millennium Inst Astrophys, Santiago, Chile
[9] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[10] Subaru Telescope, Hilo, HI 96720 USA
[11] Univ Valparaso, Inst Fs & Astronoma, Avda Gran Bretana 1111, Playa Ancha 2360102, Valparaso, Chile
[12] Univ Durham, Ctr Extragalact Astron, Dept Phys, Durham DH1 3LE, England
关键词
gravitational lensing: strong; methods: statistical; techniques: image processing; surveys; quasars: general; DARK ENERGY SURVEY; GRAVITATIONAL LENS; GALAXIES; TELESCOPE; CANDIDATE; SELECTION; PROGRAM; SIZE;
D O I
10.1093/mnras/stx3226
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on discovery results from a quasar lens search in the ATLAS-DR3 public footprint. Spectroscopic follow-up campaigns, conducted at the 2.6 m Nordic Optical Telescope (La Palma) and 3.6 m New Technology Telescope (La Silla) in 2016, yielded seven pairs of quasars exhibiting the same lines at the same redshift and monotonic flux ratios with wavelength (hereafter NIQs, nearly identical quasar pairs). Magellan spectra of A0140-1152 (01(h)40(m)03(s).0-11(d)52(m)19(s).0, z(s) = 1.807) confirm it as a lens with deflector at zl = 0.277 and Einstein radius theta(E) = (0.73 +/- 0.02) arcsec. Follow-up imaging of the NIQ A2213-2652 (22(h)13(m)38(s).4-26(d)52(m)27(s).1) reveals the deflector galaxy and confirms it as a lens. We show the use of spatial resolution from the Gaia mission to select lenses and list additional systems from a WISEGaia- ATLAS search, yielding three additional lenses (02(h)35(m)27(s)4-24(d)33(m)13(s).2, 02(h)59(m)33(s)-23(d)38(m)01(s).8 , 01(h)46(m)32(s).9-11(d)33(m)39(s).0). The overall sample consists of 11 lenses/NIQs, plus three lenses known before 2016, over the ATLAS-DR3 footprint (approximate to 3500 deg(2)). Finally, we discuss future prospects for objective classification of pair/NIQ/contaminant spectra.
引用
收藏
页码:2086 / 2096
页数:11
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