Astrophysics around 100 GeV with STACEE

Details Astrophysics around 100 GeV with STACEE Astrophysics around 100 GeV with STACEE

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newar..48..359w&link_type=abstract

New Astronomy Reviews, Volume 48, Issue 5-6, p. 359-366.

Astronomy and Astrophysics

Astronomy

3

Bl Lacertae Objects: Individual (H1426+428, Markarian 421, W Comae), Galaxies: Active, Γ-Rays: Observations, Instrumentation: Detectors, Ism: Individual (Crab Nebula), Pulsars: Individual (Crab Pulsar)

Scientific paper

STACEE is an atmospheric Cherenkov detector using the large mirror area of a solar research facility to obtain an energy threshold around 100 GeV. STACEE has been used to study the Crab and several AGN: Markarian 421, W Comae, H1426+428. The STACEE observing program is coordinated with the high-energy astrophysics community both by participation in multiwavelength campaigns and by follow-up observations of γ-ray burst alerts. Analysis methods under development using pulse height information from flash ADCs installed on each channel are expected to substantially improve the experiment's sensitivity. A summary of the performance is given.

Affiliated with

Also associated with

No associations

Rating

Astrophysics around 100 GeV with STACEE 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 Astrophysics around 100 GeV with STACEE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Astrophysics around 100 GeV with STACEE will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-738843