ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations

Details ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...336l...9k&link_type=abstract

Astronomy and Astrophysics, v.336, p.L9-L12 (1998)

Astronomy and Astrophysics

Astrophysics

126

Galaxies: Evolution, Galaxies: Starburst, Cosmology: Observations, Infrared: Galaxies

Scientific paper

Two 44arcmin x 44arcmin fields in the Lockman Hole were mapped at 95 mu m and 175 mu m using ISOPHOT. A simple program code combined with PIA works well to correct for drift in the detector responsivity. The number density of 175 mu m sources is 3-10 times higher than expected from the no-evolution model. Based on observations with ISO, an ESA project with instruments funded by ESA member states (especially the PI countries: France, Germany, the Netherlands, and the United Kingdom) and with the participation of ISAS and NASA. The ISOPHOT data presented in this paper was reduced using PIA, which is a joint development by the ESA Astrophysics Division and the ISOPHOT consortium led by the Max Plank Institute for Astronomy (MPIA), Heidelberg.

Affiliated with

Also associated with

No associations

Rating

ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ISO deep far-infrared survey in the ``Lockman Hole''. A search for obscured objects at high redshift. I. Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1574377