Optical Identification of the ISOPHOTFIR Sources

Details Optical Identification of the ISOPHOTFIR Sources Optical Identification of the ISOPHOTFIR Sources

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sgyu.conf..129k&link_type=abstract

Studies of Galaxies in the Young Universe with New Generation Telescope, Proceedings of Japan-German Seminar, held in Sendai, Ja

Physics

Scientific paper

We present the optical follow up observations of the ISOPHOTFIR sources found in our 175 micron deep survey in the Lockman Hole using ISOPHOT on board ISO (Kawara et al. 1998, AA, 328, L9). Optical and NIR observations were made using ESI and NIRSPEC on the Keck II, IRCS on the Subaru, the 8k mosaic CCD camera on the UH88, and VLA. We have identified optical counterparts of 35 ISOPHOT FIR sources with redshift between 0.03 and 1.6. We discuss their observational properties.

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