J/A+A/596/A77       SDSS J1339+1310 spectra and light curves (Goicoechea+, 2016)

Gravitational lens system SDSS J1339+1310: microlensing factory and time delay. Goicoechea L.J., Shalyapin V.N. <Astron. Astrophys. 596, A77 (2016)> =2016A&A...596A..77G 2016A&A...596A..77G (SIMBAD/NED BibCode)
ADC_Keywords: Gravitational lensing ; QSOs ; Spectroscopy ; Photometry Keywords: gravitational lensing: strong - gravitational lensing: micro - quasars: individual (SDSS J1339+1310) - cosmological parameters Abstract: We spectroscopically re-observed the gravitational lens system SDSS J1339+1310 using OSIRIS on the GTC. We also monitored the r-band variability of the two quasar images (A and B) with the LT over 143 epochs in the period 2009-2016. These new data in both the wavelength and time domains have confirmed that the system is an unusual microlensing factory. The CIV emission line is remarkably microlensed, since the microlensing magnification of B relative to that for A,µBA, reaches a value of 1.4 (∼0.4mag) for its core. Moreover, the B image shows a red wing enhancement of CIV flux (relative to A), and µBA=2 (0.75mag) for the CIV broad-line emission. Regarding the nuclear continuum, we find a chromatic behaviour of µBA, which roughly varies from ∼5 (1.75mag) at 7000Å to ∼6 (1.95mag) at 4000Å. We also detect significant microlensing variability in the r band, and this includes a number of microlensing events on timescales of 50-100d. Fortunately, the presence of an intrinsic 0.7 mag dip in the light curves of A and B, permitted us to measure the time delay between both quasar images. This delay is ΔtAB=47+5-6d (1σ confidence interval; A is leading), in good agreement with predictions of lens models. Description: We carried out long-slit spectroscopy of the lens system SDSS J1339+1310 (Inada et al., 2009AJ....137.4118I 2009AJ....137.4118I) in 2014 using the OSIRIS instrument on the 10.4m Gran Telescopio Canarias (GTC). We then extracted the optical spectra of the two quasar images (A and B) and the main lensing galaxy (G) on 27 March 2014 (R500R grism; Table 1) and 20 May 2014 (R500B grism; Table 2), i.e., at two epochs separated by approximately the time delay of the system. Previous GTC spectra (13 April 2013) were presented in Shalyapin et al. (2014A&A...568A.116S 2014A&A...568A.116S, Cat. J/A+A/586/A116). In addition, we conducted a monitoring campaign in 2009, 2012-2015 and early 2016 with the 2.0m Liverpool Telescope in the SDSS-r passband. This allowed us to construct an optical variability database of the two images of the gravitationally lensed quasar (Table 3). While Table 3 contains r-band magnitudes for 143 observation nights, an extended (updated) version is also available at the Glendama website (http://grupos.unican.es/glendama/q1339.htm) Objects: ------------------------------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------------------------------- 13 39 07.14 +13 10 39.7 SDSS J1339+1310 = [IOS2009] SDSS J1339+1310 ------------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 28 916 Red grism spectra (485.0-925.7nm) table2.dat 28 979 Blue grism spectra (360.1-720.2nm) table3.dat 47 143 Light curves in the r band (622.5nm) -------------------------------------------------------------------------------- See also: J/A+A/586/A116 : HD50138 time-dependent spectral variations (Jerabkova+, 2016) http://grupos.unican.es/glendama/ : Glendama website Byte-by-byte Description of file: table1.dat table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.3 0.1nm lambda Observed wavelength in Angstroms 10- 15 F6.3 0.1nW/m3 FA Flux of SDSS J1339+1310A 17- 22 F6.3 0.1nW/m3 FB Flux of SDSS J1339+1310B 24- 28 F5.3 0.1nW/m3 FG Flux of SDSS J1339+1310G -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.3 d MJD Modified Julian Date (MJD-50000) 10- 15 F6.3 mag rmagA r magnitude of SDSS J1339+1310A 17- 21 F5.3 mag e_rmagA Error in r magnitude of SDSS J1339+1310A 23- 28 F6.3 mag rmagB r magnitude of SDSS J1339+1310B 30- 34 F5.3 mag e_rmagB Error in r magnitude of SDSS J1339+1310B 36- 41 F6.3 mag rmagS r magnitude of the control star S 43- 47 F5.3 mag e_rmagS Error in r magnitude of S -------------------------------------------------------------------------------- Acknowledgements: Luis J. Goicoechea, luis.goicoechea(at)unican.es
(End) L.J. Goicoechea [Univ. de Cantabria, Spain], P. Vannier [CDS] 26-Sep-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line