Published 1999
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Photometric Redshifts Applied to WFPC2 and NICMOS HDF Data
- Other:
- Weymann, Ray J.
Chicago
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Abstract
A photometric redshift analysis of optical and infrared images of the Northern Hubble Deep Field indicate a constant star formation rate for redshifts between 1 and 6. The small size of the field and small number of high redshift objects limits this finding to just the area of the NICMOS image. The photometric redshift technique is a modified version of chi square fits to observed and calculated galaxy spectral energy distribution templates.
Additional Information
© 1999 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System. This work is supported in part by NASA grant NAG 5-3042. This work utilized observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy under NASA contract NAS5-26555.Attached Files
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Additional details
- Eprint ID
- 75484
- Resolver ID
- CaltechAUTHORS:20170328-135939327
- NASA
- NAG 5-3042
- NASA
- NAS5-26555
- Created
-
2017-03-28Created from EPrint's datestamp field
- Updated
-
2019-10-03Created from EPrint's last_modified field
- Series Name
- Astronomical Society of the Pacific Conference Series
- Series Volume or Issue Number
- 191