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THE LYMAN-ALPHA FOREST IN THE QUASAR B2 1225+317 FROM 3140 Å TO 3940 Å
O. BOULADE, D. KUNTH, W. L. W. SARGENT and L. VIGROUX
Publications of the Astronomical Society of the Pacific
Vol. 98, No. 609 (November 1986), pp. 1140-1146
Published by: Astronomical Society of the Pacific
Stable URL: http://www.jstor.org/stable/40678826
Page Count: 7
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We have obtained a spectrum of the quasar B2 1225+317 from 3140 Å to 3940 Å using the new "UV prime" spectrograph at the 3.6-m CFH telescope. A signal-to-noise ratio larger than 25 was achieved with an exposure of only 90 minutes using an RCA CCD. We produce a new line list of the Lyman-alpha forest that is complete to about 0.15 Å rest equivalent width. We confirm that the number density of the Lα lines increases steeply for rest equivalent widths smaller than 0.20 Å as suggested by previous workers. The new equipment is very suited for quick quasar survey and in particular for a Mg ii search at z < 0.40.
Publications of the Astronomical Society of the Pacific © 1986 The University of Chicago Press