Submillimetre detection of a high-redshift type 2 QSO
- Author
- MAINIERI, V1 ; RIGOPOULOU, D2 ; LEHMANN, I1 ; SCOTT, S3 ; MATUTE, I1 ; ALMAINI, O4 ; TOZZI, P5 ; HASINGER, G1 ; DUNLOP, J. S3
[1] Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, PF 1312, 85741 Garching, Germany
[2] Astrophysics, Department of Physics, Keble Road, Oxford OX1 3RH, United Kingdom
[3] Institut for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, United Kingdom
[4] School of Physics & Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD, United Kingdom
[5] INAF, Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 34131, Trieste, Italy - Source
Monthly Notices of the Royal Astronomical Society. 2005, Vol 356, Num 4, pp 1571-1575, 5 p ; ref : 35 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- galaxies: active galaxies: nuclei quasars: general submillimetre
- Keyword (fr)
- Cosmologie Densité spectrale énergie Déplacement vers le rouge Formation galaxies Formation stellaire Galaxies actives Galaxies à flambée Noyau galactique actif Noyau galaxies Phase initiale Photométrie Quasar Raie émission Spectre optique Taux formation Trou noir
- Keyword (en)
- Cosmology Spectral energy distribution Red shift Galaxy formation Star formation Active galaxies Starburst galaxies Active galaxy nuclei Galaxy nuclei Early phase Photometry Quasars Emission line Optical spectrum Formation rate Black holes
- Keyword (es)
- Densidad espectral energía Galaxias llamarada estelar Fase inicial Raya emisión Espectro óptico Grado formación
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16536638
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1111/j.1365-2966.2004.08600.x 
https://dx.doi.org/10.1111/j.1365-2966.2004.08600.x
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