Determination of the cosmic far-infrared background level with the ISOPHOT instrument (Research Note)

Astronomy and Astrophysics

Volumn 500, Issue 2, 2009, Pages 763-768

  Juvela, M ^a   Mattila, K ^a   Lemke, D ^b   Klaas, U ^b   Leinert, C ^b   Kiss, Cs ^c  

^a UNIVERSITY OF HELSINKI   (Finland)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c KONKOLY OBSERVATORY   (Hungary)

Author keywords

Cosmology, observations ; Galaxies, evolution ; Infrared, galaxies

Indexed keywords

COSMIC FAR-INFRARED BACKGROUNDS; CURRENT ESTIMATES; FAR-INFRARED; HYDROGEN COLUMN DENSITY; INFRARED BACKGROUND; INFRARED, GALAXIES; ISOPHOT; LINE DATA; SHORTER WAVELENGTH; SURFACE BRIGHTNESS; UPPER LIMITS; ZODIACAL LIGHT;

APPROXIMATION THEORY; COSMOLOGY; HYDROGEN; RADIO TELESCOPES; SATELLITE OBSERVATORIES; SYSTEMATIC ERRORS; TELESCOPES; TROPICAL ENGINEERING;

GALAXIES;

EID: 67649541416     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811351     Document Type: Article

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