A survey for DLA galaxies with integral field spectroscopy

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Using integral field spectroscopy (ifs) we have observed QSOs which were previously known to have intervening DLAs, to search for emission lines in the field surrounding the QSOs. The sample consists of 13 DLAs plus 7 sub-DLAs at z>2, from which we find emission line candidates at the expected wavelengths for 8 systems, implying a detection frequency of 40%. Emission lines detected at the DLA redshifts are interpreted as being due to Lyα lines from galaxies associated with the DLA clouds. Candidates are detected at 3-4σ levels in both narrow-band images and spectra created from the data cubes. We find no preference for candidate detection associated with either high or low metallicity DLAs. In comparison with the properties of previously known DLA galaxies, the candidates show similar distributions of line fluxes and line widths, but their impact parameters are slightly different, suggesting H I cross sections larger than 10 kpc.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

A survey for DLA galaxies with integral field spectroscopy 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 A survey for DLA galaxies with integral field spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A survey for DLA galaxies with integral field spectroscopy will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1566709

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.