Observations of the Crab Nebula at TeV energies.

Bibcode
1994AIPC..304..270W
Weekes, T. C.; Akerlof, C. W.; Chantell, M.; Colombo, E.; Cawley, M. F.; Connaughton, V.; Fegan, D. J.; Fennell, S.; Gaidos, J.; Hillas, A. M.; Kerrick, A. D.; Kwok, P.; Lewis, D. A.; Lamb, R. C.; Meyer, D. I.; Mohanty, G.; Rose, J.; Rovero, A.; Sembroski, G.; Schubnell, M. S.; Punch, M.; West, M.; Whitaker, T.; Wilson, C.
Bibliographical reference

AIP Conf. Proc., No. 304, p. 270 - 274

Advertised on:
0
1994
Number of authors
24
IAC number of authors
0
Citations
8
Refereed citations
8
Description
The results of four years of observation of the Crab Nebula at TeV energies by the Whipple group are discussed and the status of the Crab Nebula as a standard candle for TeV astronomy is reviewed.
Type
Non-refereed
Gamma rays
Supernova remnants

It may interest you

  • Non-refereed
    Workshop summary: Kaons@CERN 2023

    Kaon physics is at a turning point - while the rare-kaon experiments NA62 and KOTO are in full swing, the end of their lifetime is approaching and the future experimental landscape needs to be defined. With HIKE, KOTO-II and LHCb-Phase-II on the table and under scrutiny, it is a very good moment in time to take stock and contemplate about the

    Anzivino, G. et al.

    Advertised on:

    4
    2024
    Bibcode
    2024EPJC...84..377A
    Citations
    0
  • Non-refereed
    Finding Water Worlds with Transit Timing Variations

    Models predict that planets with water-rich compositions may be common around low-mass stars, but definitive evidence for the existence of water worlds has remained elusive. Precise mass and radius measurements for small planets allow us to identify candidate water worlds that have bulk densities too low to be consistent with a rocky composition

    Greklek-McKeon, Michael et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....560502G
    Citations
    0
  • Non-refereed
    First light and results for atmospheric characterization with The Near Infra-Red Planet Searcher (NIRPS)

    NIRPS is a new fiber-fed high spectral resolution (~80k) spectrograph assisted by adaptive optics installed on the 3.6m telescope of ESO at LaSilla, Chile. Operated simultaneously with HARPS, NIRPS covers the Y, J, and H bands. The commissioning phase demonstrated high stability for time-series observations along precise radial velocities reaching

    Allart, Romain et al.

    Advertised on:

    4
    2024
    Bibcode
    2024ESS.....562419A
    Citations
    0