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Time delay and lens redshift for the doubly imaged BAL quasar SBS 1520+530

Burud, I. and Hjorth, J. and Courbin, F. and Cohen, J. G. and Magain, P. and Jaunsen, A. O. and Kaas, A. A. and Faure, C. and Letawe, G. (2002) Time delay and lens redshift for the doubly imaged BAL quasar SBS 1520+530. Astronomy & Astrophysics, 391 (2). pp. 481-486. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20180207-101035264

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Abstract

We present optical R-band light curves of the gravitationally lensed quasar SBS 1520+530 derived from data obtained at the Nordic Optical Telescope. A time delay of 130 ± 3 days (1σ) is determined from the light curves. In addition, spectra of SBS 1520+530 obtained at the Keck Observatory are spatially deconvolved in order to extract the spectrum of the faint lensing galaxy, free of any contamination by the light from the bright quasar images. This spectrum indicates a lens redshift z = 0.717, in agreement with one of the absorption systems found in the quasar spectra. The best mass model of the system includes a second nearby galaxy and a cluster of galaxies in addition to the main lensing galaxy. Adopting this model and an Ω = 0.3, Λ = 0.7 cosmology, our time-delay measurement yields a Hubble constant of H_0 = 51 ± 9 km s^(-1) Mpc^(-1) (1σ error).


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/0004-6361:20020856DOIArticle
https://arxiv.org/abs/astro-ph/0206084arXivDiscussion Paper
ORCID:
AuthorORCID
Hjorth, J.0000-0002-4571-2306
Cohen, J. G.0000-0002-8039-4673
Additional Information:© 2002 ESO. Received: 23 April 2002. Accepted: 4 June 2002. We thank the NOT Director Vilppu Piirola for granting us observing time for this project on a flexible basis. We are especially grateful to the many visiting observers at NOT who have contributed to this project by performing the scheduled observations. This project was conceived in 1997 while JH and AOJ were visiting scientists at the Center for Advanced Study in Oslo. We thank Rolf Stabell and Sjur Refsdal for inviting us in their center and for their kind hospitality. JH appreciates the hospitality of the OMP where some of this work was conducted. The project was supported by the Danish Natural Science Research Council (SNF). IB was supported in part by contract ARC94/99-178 "Action de Recherche Concertée de la Communauté Française (Belgium)'' and Pôle d'Attraction Interuniversitaire, P4/05 (SSTC, Belgium). FC acknowledges financial support through Chilean grant FONDECYT/3990024 and through Marie Curie grant MCFI-2001-0242. Additional support from the European Southern Observatory and ECOS/CONICYT CU00U05 grant is also gratefully acknowledged.
Funders:
Funding AgencyGrant Number
Danish Natural Science Research CouncilUNSPECIFIED
Communauté française de Belgique - Actions de recherche concertéeARC94/99-178
Pôle d'Attraction Interuniversitaire P4/05 (Belgium)UNSPECIFIED
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)3990024
Marie Curie FellowshipMCFI-2001-0242
European Southern ObservatoryUNSPECIFIED
ECOS/CONICYTCU00U05
Comisión Nacional de Investigación Científica y Tecnológica (CONICYT)UNSPECIFIED
Subject Keywords:gravitational lensing - quasars: individual: SBS 1520+530 - cosmology: cosmological parameters
Issue or Number:2
Record Number:CaltechAUTHORS:20180207-101035264
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180207-101035264
Official Citation:Time delay and lens redshift for the doubly imaged BAL quasar SBS 1520+530 I. Burud, J. Hjorth, F. Courbin, J. G. Cohen, P. Magain, A. O. Jaunsen, A. A. Kaas, C. Faure and G. Letawe A&A, 391 2 (2002) 481-486 DOI: https://doi.org/10.1051/0004-6361:20020856
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84714
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:08 Feb 2018 21:15
Last Modified:09 Mar 2020 13:18

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