UCSD/Keck Damped Ly{alpha} Abundance Database (Prochaska+, 2007)

Details UCSD/Keck Damped Ly{alpha} Abundance Database (Prochaska+, 2007) UCSD/Keck Damped Ly{alpha} Abundance Database (Prochaska+, 2007)

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..21710029p&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/171/29. Originally published in: 2007ApJS..171...29P

Physics

H I Data, Qsos, Spectroscopy, Abundances

Scientific paper

For nearly all observations, the HIRES spectra were acquired using either a 0.8" or 1.1" wide decker (FWHM about 6 and 8km/s, respectively) and the ESI observations were carried out with the 0.5" or 0.75" slit (FWHM about 33 and 44km/s, respectively). All of the HIRES spectra were acquired with the original Tektronix 2048*2048CCD. In general we strove to achieve a final signal-to-noise ratio (S/N) of >15pixel-1^ (2km/s/pix for HIRES, 11km/s/pix for ESI). ESI has a fixed format that covers the spectral region {lambda}=4000 to 10000{AA}.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

UCSD/Keck Damped Ly{alpha} Abundance Database (Prochaska+, 2007) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with UCSD/Keck Damped Ly{alpha} Abundance Database (Prochaska+, 2007), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UCSD/Keck Damped Ly{alpha} Abundance Database (Prochaska+, 2007) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1866898