File(s) not publicly available
What we learn from the comparison between ISOCAM 15-micron & Spitzer 24-micron source counts.
presentation
posted on 2023-06-08, 05:45 authored by Francesca Pozzi, C Gruppioni, C Lari, Seb OliverSeb Oliver, G. RodighieroThe Spitzer Space Telescope is now providing new insights into the IR population contributing to the CIRB, in particular with the MIPS 24-µm band. The question raises on how to compare them with the previous ISOCAM counts at 15-µm. In this work, we present the 24-µm predictions, inferred accurately from a phenomenological 15-µm based model. We will show how extrapolating the ISOCAM populations at higher z, we can explain almost all the 24-µm sources.
History
Publication status
- Published
Publisher
Ed. by A. Wilson. ESA SP-577, Noordwijk, Netherlands: ESA Publications Division,Publisher URL
Volume
557Page range
315-316Presentation Type
- paper
Event name
Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004Event location
Paris, FranceEvent type
conferenceEvent date
27-29 October 2004.ISBN
92-9092-855-7Department affiliated with
- Physics and Astronomy Publications
Notes
Published in: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A. Wilson. ESA SP-577, Noordwijk, Netherlands: ESA Publications Division, ISBN 92-9092-855-7, 2005, p. 315 - 316Full text available
- No
Peer reviewed?
- Yes
Legacy Posted Date
2012-02-06Usage metrics
Categories
No categories selectedKeywords
Licence
Exports
RefWorks
BibTeX
Ref. manager
Endnote
DataCite
NLM
DC