Pith. sign in

REVIEW

VERITAS: Very LArge Energetic Radiation Imaging Telescope Array System

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/9706143 v1 pith:PQY5QDXC submitted 1997-06-15 astro-ph

VERITAS: Very LArge Energetic Radiation Imaging Telescope Array System

T.C.Weekes , C.Akerlof , S.Biller , A.C.Breslin , J.H.Buckley , D.A.Carter-Lewis , M.Catanese , M.F.Cawley
show 32 more authors
B.Dingus G.G.Fazio D.J.Fegan J.Finley G.Fishman J.Gaidos G.H.Gillanders P.Gorham J.E.Grindlay A.M.Hillas J.Huchra P.Kaaret M.Kertzman D.Kieda F.Krennrich R.C.Lamb M.J.Lang A.P.Marscher S.Matz T.McKay D.Muller R.Ong W.Purcell J.Rose G.Sembroski F.D.Seward P.Slane S.Swordy T.Tumer M.Ulmer M.Urban B.J.Wilkes
This is my paper
classification astro-ph
keywords arrayimagingmaximumobservatorysensitivitytelescopewillatmospheric
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

A next generation atmospheric Cherenkov observatory is described based on the Whipple Observatory $\gamma$-ray telescope. A total of nine such imaging telescopes will be deployed in an array that will permit the maximum versatility and give high sensitivity in the 50 GeV - 50 TeV band (with maximum sensitivity from 100 GeV to 10 TeV).

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.