Published 2008
| Published
Book Section - Chapter
Open
Spitzer 70-micron Confusion Level
- Creators
-
Frayer, D. T.
- Huynh, M. T.
Chicago
An error occurred while generating the citation.
Abstract
Spitzer 70μm confusion measurements are presented based on ultra-deep MIPS-70μm observations of GOODS Hubble Deep Field North (HDFN). The instrument noise for the MIPS-70μm band integrates down with nearly t^(−0.5) for the low background HDF-N field. The estimated confusion level is σ_c = 0.30 ± 0.15mJy for a limiting flux density of 1.5mJy (q = 5).
Additional Information
© 2008 Astronomical Society of the Pacific. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under NASA contract 1407.Attached Files
Published - Frayer2008p8405Second_Annual_Spitzer_Science_Center_Conference_Infrared_Diagnostics_Of_Galaxy_Evolution.pdf
Files
Frayer2008p8405Second_Annual_Spitzer_Science_Center_Conference_Infrared_Diagnostics_Of_Galaxy_Evolution.pdf
Files
(165.3 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:e24dee554e39ac85fa23ebeb0d6a751e
|
165.3 kB | Preview Download |
Additional details
- Eprint ID
- 19425
- Resolver ID
- CaltechAUTHORS:20100813-094749717
- NASA
- 1407
- Created
-
2010-08-13Created from EPrint's datestamp field
- Updated
-
2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- ASP Conference Series
- Series Volume or Issue Number
- 381