Reference : Spectra of 13 lensed quasars (Sluse+, 2012)
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Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/129201
Spectra of 13 lensed quasars (Sluse+, 2012)
English
Sluse, Dominique mailto [> >]
Hutsemekers, Damien mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Courbin, F. [> >]
Meylan, G. [> >]
Wambsganss, J. [> >]
1-May-2012
[en] Active gal. nuclei ; Gravitational lensing ; QSOs ; Spectroscopy
[en] Extracted flux calibrated spectra of 13 lensed quasars following the methodology described in Sect. 2.1. of the oaoer. The data were obtained with the FORS spectrograph at VLT in multi-object spectroscopy mode. The typical wavelength coverage is from 4200 to 8200Å. The data concern the following objects: HE0047-1756 (HE0047), Q0142-100 (Q0142), SDSSJ0246-0825 (SDSS0246), HE0435-1223 (HE0435), SDSSJ0806+2006 (SDSS0806), FBQ0951+2635 (FBQ0951), BRI0952-0115 (BRI0952), SDSSJ1138+0314 (J1138), J1226-0006 (J1226), SDSSJ1335+0118 (J1335), Q1355-2257 (Q1355), WFI2033-4723 (WFI2033), and HE2149-2745 (HE2149). For each object, we provide the 1D flux calibrated spectrum of the 2 individual images in the slit. In addition, we also provide the 2D reduced spectrum and corresponding 1σ error frame (corresponding files are named "objectname[SUB]data" and "objectname[/SUB]err"), and the 2D processed spectra associated to the deconvolution, as shown in Fig.1 of the paper. These processed 2D spectra are the deconvolved frame ("[SUB]dec"), the extended component of the flux emission ("[/SUB]ext") and the residual frame in σ units ("_res") corresponding to panel (b), (c) and (d) of Fig.1. A pdf file file similar to Fig.1 is also provided for each object. (4 data files).
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http://hdl.handle.net/2268/129201
http://adsabs.harvard.edu/abs/2012yCat..35449062S
mlqsos.dat 13x161 List of objects with available spectra; fits1/* 26. 1D spectra of the quasar images; (2 spectra per object, one for each lensed image) ; fits2/* 65. Bidimensional spectra the quasar images; pdf/* 13. PDF files of deconvolution, as Fig1 of the paper

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