Results of the Mount Hopkins sky survey for sources of 100-1000 GeV gamma rays

Details Results of the Mount Hopkins sky survey for sources of 100-1000 GeV gamma rays Results of the Mount Hopkins sky survey for sources of 100-1000 GeV gamma rays

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977esasp.124...55w&link_type=abstract

In ESA Recent Advan. in Gamma-Ray Astronomy p 55-58 (SEE N78-11899 02-88)

Astronomy and Astrophysics

Astronomy

1

Astronomical Observatories, Cerenkov Radiation, Gamma Rays, Point Sources, Sky Surveys (Astronomy), Atmospheric Radiation, Galactic Radiation, Reflecting Telescopes, Scanning

Scientific paper

The 10 m reflector at the Mt. Hopkins Observatory (altitude 2.3 km) has been used in a multiple beam configuration to scan the celestial sphere for point sources of 100 to 1000 GeV gamma rays. During the period December 1974 to September 1976, almost the entire sky between declinations (-10 deg) and (+70 deg) has been surveyed at least once. Results of some 800 hrs of observations are reported; the emphasis was on a search for discrete sources at the lowest energies.

Affiliated with

Also associated with

No associations

Rating

Results of the Mount Hopkins sky survey for sources of 100-1000 GeV gamma rays 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 Results of the Mount Hopkins sky survey for sources of 100-1000 GeV gamma rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Results of the Mount Hopkins sky survey for sources of 100-1000 GeV gamma rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1560168