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Local Luminosity Function at 15 micro m and Galaxy Evolution Seen by ISOCAM 15 micro m SurveysA local luminosity function at 15 micro m is derived using the bivariate (15 micro m vs. 60 micro m luminosities) method, based on the newly published ISOCAM LW3-band (15 micro m) survey of the very deep IRAS 60 micro m sample in the north ecliptic pole region (NEPR).
Document ID
20060032633
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/14289
Authors
Xu, C.
Date Acquired
August 23, 2013
Publication Date
January 1, 2000
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
galaxies luminosity function mass functions photometry infrared

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