6533b85bfe1ef96bd12bb4cd
RESEARCH PRODUCT
Revealing the structure of the lensed quasar Q 0957+561. I. Accretion disk size
C. FianEvencio MediavillaEvencio MediavillaP. Goméz-alvarezJ. A. MuñozArnold HanslmeierD. CheloucheVeronica MottaK. RojasJ. Jiménez-vicentesubject
Brightnessmagnificationtime-delayFOS: Physical sciencesAstrophysicsgravitational lensing: microAstrophysics::Cosmology and Extragalactic AstrophysicsGravitational microlensingvlbi observationsmicro [Gravitational lensing]accretionpeculiar velocityindividual: Q 0957+561 [Quasars]Astrophysics::Galaxy AstrophysicsPhysicsquasars: individual: q 0957+561robust determinationaccretion disksvelocity dispersionq0957+561Astronomy and AstrophysicsQuasarAccretion accretion disksLight curveAstrophysics - Astrophysics of GalaxiesGalaxyAccretion (astrophysics)StarsGravitational lensdark-matterx-raySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary Astrophysicsoptical continuum emissiondescription
We thank the anonymous referee for the helpful comments, and constructive remarks on this manuscript. We thank the GLENDAMA project for making publicly available the monitoring data of Q 0957+561. C.F. gratefully acknowledges the financial support from Tel Aviv University and University of Haifa through a DFG grant HA3555-14/1. E.M. and J.A.M are supported by the Spanish MINECO with the grants AYA2016- 79104-C3-1-P and AYA2016-79104-C3-3-P. J.A.M. is also supported from the Generalitat Valenciana project of excellence Prometeo/2020/085. J.J.V. is supported by the project AYA2017-84897-P financed by the Spanish Ministerio de Economia y Competividad and by the Fondo Europeo de Desarrollo Regional (FEDER), and by project FQM-108 financed by Junta de Andalucia. K. R. acknowledges support from the Swiss National Science Foundation (SNSF). V.M. acknowledges the support of Centro de Astrofisica de Valparaiso.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2021-01-01 |