J/A+A/585/A87       Quasar composite made from bright QSOs      (Selsing+, 2016)

An X-shooter composite of bright 1 < z < 2 quasars from UV to infrared. Selsing J., Fynbo J. P. U, Christensen L., Krogager J.-K. <Astron. Astrophys. 585, A87 (2016)> =2016A&A...585A..87S 2016A&A...585A..87S (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; Spectra, ultraviolet ; Spectra, infrared Keywords: quasars: general - galaxies: ISM - methods: data analysis - techniques: spectroscopic Abstract: Quasi-stellar object (QSO) spectral templates are important both to QSO physics and for investigations that use QSOs as probes of intervening gas and dust. However, combinations of various QSO samples obtained at different times and with different instruments so as to expand a composite and to cover a wider rest frame wavelength region may create systematic effects, and the contribution from QSO hosts may contaminate the composite. We have constructed a composite spectrum from luminous blue QSOs at 1<z<2.1 selected from the Sloan Digital Sky Survey (SDSS). The observations with X-shooter simultaneously cover ultraviolet (UV) to near-infrared (NIR) light, which ensures that the composite spectrum covers the full rest-frame range from Lyβ to 11350Å without any significant host contamination. Assuming a power-law continuum for the composite we find a spectral slope of αλ=1.70±0.01, which is steeper than previously found in the literature. We attribute the differences to our broader spectral wavelength coverage, which allows us to effectively avoid fitting any regions that are affected either by strong QSO emissions lines (e.g., Balmer lines and complex [FeII] blends) or by intrinsic host galaxy emission. Finally, we demonstrate the application of the QSO composite spectrum for evaluating the reddening in other QSOs. Description: Quasar composite made from bright QSOs, as described in the paper. The composite consists of wavelength with corresponding arbitrarily normalized flux and error. The source code and composite is also made available at https://github.com/jselsing/QuasarComposite File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file spectrum.dat 22 25875 Quasar composite spectrum -------------------------------------------------------------------------------- Byte-by-byte Description of file: spectrum.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.1 0.1nm lambda Wavelength array for the composite 9- 15 F7.4 --- S Normalized flux density, normalized to unity at 6800Å (1) 17- 22 F6.4 --- e_S Error relative to the normalized flux density -------------------------------------------------------------------------------- Note (1): Constituent spectra are corrected for galactic extinction using their coordinates and the extinctions map from http://irsa.ipac.caltech.edu/applications/DUST/ -------------------------------------------------------------------------------- Acknowledgements: Jonatan Selsing, jselsing(at)dark-cosmology.dk
(End) Jonatan Selsing [DARK, NBI], Patricia Vannier [CDS] 26-Oct-2015
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