Observations of the Hubble Deep Field with the Infrared Space Observatory - V. Spectral energy distributions, starburst models and star formation history

Monthly Notices of the Royal Astronomical Society

Volumn 289, Issue 2, 1997, Pages 490-496

  Rowan Robinson, M ^a   Mann, R G ^a   Oliver, S J ^a   Efstathiou, A ^a   Eaton, N ^a   Goldschmidt, P ^a   Mobasher, B ^a   Serjeant, S B G ^a   Sumner, T J ^a   Danese, L ^b   Elbaz, D ^c   Franceschini, A ^d   Egami, E ^e   Kontizas, M ^f   Lawrence, A ^g   McMahon, R ^h   Norgaard Nielsen, H U ⁱ   Perez Fournon, I ^j   Gonzalez Serrano, J I ^k  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b SISSA   (Italy)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^f NATIONAL OBSERVATORY OF ATHENS   (Greece)

^g UNIVERSITY OF EDINBURGH   (United Kingdom)

^h UNIVERSITY OF CAMBRIDGE   (United Kingdom)

ⁱ TECHNICAL UNIVERSITY OF DENMARK   (Denmark)

^j INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^k INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

more..

Author keywords

Cosmology: Observations; Galaxies: Evolution; Galaxies: Starburst; Infrared: Galaxies; Stars: Formation

Indexed keywords

CHEMICAL ELEMENTS; DUST; SPECTROSCOPY; STARS;

COSMOLOGY OBSERVATIONS; GALAXIES: STARBURSTS; GALAXY EVOLUTION; INFRARED GALAXIES; INFRARED SPACE; SPECTRAL ENERGY DISTRIBUTION; STAR FORMATION RATES; STARBURST MODELS; STARS FORMATION; UNCERTAINTY;

GALAXIES;

EID: 0040293986     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/289.2.490     Document Type: Article

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