A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
ESO very large telescope optical spectroscopy of BL Lacertae objects. I. New redshifts
Tekijät: Sbarufatti B, Treves A, Falomo R, Heidt J, Kotilainen J, Scarpa R
Kustantaja: IOP PUBLISHING LTD
Julkaisuvuosi: 2005
Lehti:: Bulletin of the American Astronomical Society
Tietokannassa oleva lehden nimi: ASTRONOMICAL JOURNAL
Lehden akronyymi: ASTRON J
Vuosikerta: 129
Numero: 2
Aloitussivu: 559
Lopetussivu: 566
Sivujen määrä: 8
ISSN: 0004-6256
DOI: https://doi.org/10.1086/427138
Tiivistelmä
We report redshift measurements for 12 BL Lacertae objects from a program aimed at obtaining high signal-to-noise ratio (up to similar to500) optical spectroscopy of a mixed sample of objects. The new observations, gathered with the 8 m ESO Very Large Telescope, allowed us to detect weak spectral features down to a line equivalent width as small as similar to1 Angstrom. The new redshifts fall in the 0.2-1.3 interval. For nine objects we observe emission lines from the active nucleus. In the remaining three cases absorption lines from the host galaxy are found. For two objects we also detect absorption lines from intervening systems.
We report redshift measurements for 12 BL Lacertae objects from a program aimed at obtaining high signal-to-noise ratio (up to similar to500) optical spectroscopy of a mixed sample of objects. The new observations, gathered with the 8 m ESO Very Large Telescope, allowed us to detect weak spectral features down to a line equivalent width as small as similar to1 Angstrom. The new redshifts fall in the 0.2-1.3 interval. For nine objects we observe emission lines from the active nucleus. In the remaining three cases absorption lines from the host galaxy are found. For two objects we also detect absorption lines from intervening systems.
Turun yliopiston Tutkimustietojärjestelmän portaali