Open AccessGLITP optical monitoring of QSO 0957+561: VR light curves and variability
Author(s) -
Ullán A.,
Goicoechea L. J.,
Muñoz J. A.,
Mediavilla E.,
SerraRicart M.,
Puga E.,
Alcalde D.,
Oscoz A.,
Barrena R.
Publication year - 2003
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-2966.2003.07091.x
Subject(s) - physics , quasar , astrophysics , observatory , redshift , astronomy , supernova remnant , gravitational lens , light curve , supernova , telescope , galaxy
ABSTRACT The Gravitational Lenses International Time Project (GLITP) collaboration observed the first gravitational lens system (QSO 0957+561) from 2000 February 3 to March 31. The daily VR observations were made with the 2.56‐m Nordic Optical Telescope at Roque de los Muchachos Observatory, La Palma, Spain. We have derived detailed and robust VR light curves of the two components Q0957+561A and Q0957+561B. In spite of the excellent sampling rate, we have not found evidence in favour of true daily variability. With respect to variability on time‐scales of several weeks, we measure VR gradients of about −0.8 mmag d −1 in Q0957+561A and +0.3 mmag d −1 in Q0957+561B. The gradients are very probably originated in the far source. Thus, adopting this reasonable hypothesis (intrinsic variability), we compare them to the expected gradients during the evolution of a compact supernova remnant at the redshift of the source quasar. The starburst scenario is roughly consistent with some former events, but the new gradients do not seem to be caused by supernova remnant activity.