Published 1999
| Published
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The HDF, The Arizona View
Chicago
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Abstract
We present an initial analysis of the star formation rates in the deep NICMOS field of the Hubble Deep Field. The analysis utilizes template photometric redshift and extinction techniques on the combination of six optical and near infrared fluxes available for this region from observations with both NICMOS and WFPC2. Our results are consistent with a constant star formation rate for a redshift range of 1 to 6.
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
Published - 1999ASPC__193__271T.pdf
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Additional details
- Eprint ID
- 75481
- Resolver ID
- CaltechAUTHORS:20170328-132025945
- 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
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- Astronomical Society of the Pacific Conference Series
- Series Volume or Issue Number
- 193