Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20717020s&link_type=abstract
American Astronomical Society Meeting 207, #170.20; Bulletin of the American Astronomical Society, Vol. 37, p.1430
Astronomy and Astrophysics
Astronomy
Scientific paper
We use deep multi-wavelength imaging in the optical and near infrared to identify bright high redshift candidates in a widefield region surrounding the Hubble Deep Field North.
The faint galaxy population at high redshift (z>5) has recently been the subject of intensive research, largely based on Hubble Space Telescope imaging. However many of the galaxy candidates thus identified are inaccessible to the current generation of spectrographs and ground based telescopes. Ground based imaging presents the opportunity to identify brighter high redshift candidates, but has its own complications - notably the difficulty of distinguishing lower redshift contaminants from high redshift sources.
The long wavelength baseline of our imaging, and in particular our new near-infrared J and H band observations (reaching HAB=23.5, 3 sigma), enable effective seperation of high redshift galaxies and AGN from galactic class M, L and T stars. We find that samples of sources with extreme colours are dominated by Galactic stars at the relatively bright magnitudes accessible to widefield imaging. The large area of our field, combined with our clean selection, enable us to place constraints on the bright end of the ultraviolet-luminous galaxy luminosity function and the abundance of low luminosity AGN at z>5.
Barger Amy. J.
Cowie Lennox L.
Stanway Elizabeth R.
Trouille Laura
No associations
LandOfFree
A High Redshift Survey Using Deep Near-Infrared Imaging 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 High Redshift Survey Using Deep Near-Infrared Imaging, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A High Redshift Survey Using Deep Near-Infrared Imaging will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1287930