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Title: Observations of the lensed quasar Q2237+0305 with Canaricam at GTC

Journal Article · · Astrophysical Journal
;  [1];  [2];  [3];  [4]
  1. Departamento de Astronomía y Astrofísica, Universidad de Valencia, E-46100 Burjassot, Valencia (Spain)
  2. Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States)
  3. Instituto de Astrofísica de Canarias, E-38200 La Laguna, Santa Cruz de Tenerife (Spain)
  4. Departamento de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada (Spain)

We present new mid-IR observations of the quadruply lensed quasar Q2237+0305 taken with CanariCam on the Gran Telescopio Canarias. Mid-IR emission by hot dust, unlike the optical and near-IR emission from the accretion disk, is unaffected by the interstellar medium (extinction/scattering) or stellar microlensing. We compare these “true” ratios to the (stellar) microlensed flux ratios observed in the optical/near-IR to constrain the structure of the quasar accretion disk. We find a half-light radius of R{sub 1/2}=3.4{sub −2.1}{sup +5.3}√(〈M〉/0.3M{sub ⊙}) lt-day at λ{sub rest}=1736 A-ring and an exponent for the temperature profile R∝λ{sup p} of p=0.79±0.55, where p=4/3 for a standard thin-disk model. If we assume that the differences in the mid-IR flux ratios measured over the years are due to microlensing variability, we find a lower limit for the size of the mid-IR-emitting region of R{sub 1/2}≳200 √(〈M〉/0.3M{sub ⊙}) lt-day. We also test for the presence of substructure/satellites by comparing the observed mid-IR flux ratios with those predicted from smooth lens models. We can explain the differences if the surface density fraction in satellites near the lensed images is α=0.033{sub −0.019}{sup +0.046} for a singular isothermal ellipsoid plus external shear mass model or α=0.013{sub −0.008}{sup +0.019} for a mass model combining ellipsoidal NFW and de Vaucouleurs profiles in an external shear.

OSTI ID:
22868537
Journal Information:
Astrophysical Journal, Vol. 831, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English