VizieR Online Data Catalog 36 accreting YSOs emission lines (Alcala+, 2014)

With its three spectrograph arms, X-shooter provides simultaneous wavelength coverage from ~300 to ~2480nm. For most of the targets, slits of 10/09/09 were used in the UVB/VIS/NIR arms, respectively, yielding resolving powers of 5100/8800/5600. Only the two brightest objects in the sample (Sz 74 and Sz 83) were observed through the 0.5/0.4/0.4 arcsec slits in the UVB/VIS/NIR arms, respectively, yielding resolving powers of 9100/17400/10500. Table 1 includes the observation log. X-shooter@VLT spectra of 36 Young Stellar Objects (YSOs) in the Lupus star forming region are published. For most of the targets, slits of 1"/0.9"/0.9" were used in the UVB/VIS/NIR arms, respectively, yielding resolving powers of 5100/8800/5600. Only the two brightest objects in the sample (Sz74 and Sz83) were observed through the 0.5/0.4/0.4 arcsec slits in the UVB/VIS/NIR arms, respectively, yielding resolving powers of 9100/17400/10500. For every YSO the spectra in the UVB, VIS and NIR arms are given. The 1d wavelength-calibrated and flux-calibrated spectra are in fits format and are not corrected for extinction. The VIS and NIR spectra are corrected for telluric absorption lines. The wavelength units are nm and the flux units are erg/s/cm<SUP>2</SUP>/nm. (16 data files).