Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift
- 1 July 1998
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 394 (6690) , 248-251
- https://doi.org/10.1038/28338
Abstract
No abstract availableKeywords
All Related Versions
This publication has 19 references indexed in Scilit:
- The Spectrum of the Extragalactic Far‐Infrared Background from theCOBEFIRAS ObservationsThe Astrophysical Journal, 1998
- The Ultraviolet Spectroscopic Properties of Local Starbursts: Implications at High RedshiftThe Astrophysical Journal, 1998
- Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation ForegroundsThe Astrophysical Journal, 1998
- High-[CLC][ITAL]z[/ITAL][/CLC] L[CLC]y[/CLC]α Emitters. I. A Blank-Field Search for Objects near Redshift [CLC][ITAL]z[/ITAL][/CLC] = 3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA 22The Astronomical Journal, 1998
- The Evolution of the Distribution of Star Formation Rates in GalaxiesThe Astrophysical Journal, 1997
- LUMINOUS INFRARED GALAXIESAnnual Review of Astronomy and Astrophysics, 1996
- The Keck Low-Resolution Imaging SpectrometerPublications of the Astronomical Society of the Pacific, 1995
- Galaxy formation and the origin of the ionizing flux at large redshiftThe Astrophysical Journal, 1990
- Star formation in active dwarf galaxiesThe Astrophysical Journal, 1986
- The molecular gas distribution in M51The Astrophysical Journal, 1983