Fermi-LAT observations of the Geminga pulsar
2010 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 720, no 1, 272-283 p.Article in journal (Refereed) Published
We report on the Fermi-LAT observations of the Geminga pulsar, the second brightest non-variable GeV source in the gamma-ray sky and the first example of a radio-quiet gamma-ray pulsar. The observations cover one year, from the launch of the Fermi satellite through 2009 June 15. A data sample of over 60,000 photons enabled us to build a timing solution based solely on gamma-rays. Timing analysis shows two prominent peaks, separated by Delta phi = 0.497 +/- 0.004 in phase, which narrow with increasing energy. Pulsed gamma-rays are observed beyond 18 GeV, precluding emission below 2.7 stellar radii because of magnetic absorption. The phase-averaged spectrum was fitted with a power law with exponential cutoff of spectral index Gamma = (1.30 +/- 0.01 +/- 0.04), cutoff energy E-0 = (2.46 +/- 0.04 +/- 0.17) GeV, and an integral photon flux above 0.1 GeV of (4.14 +/- 0.02 +/- 0.32) x 10(-6) cm(-2) s(-1). The first uncertainties are statistical and the second ones are systematic. The phase-resolved spectroscopy shows a clear evolution of the spectral parameters, with the spectral index reaching a minimum value just before the leading peak and the cutoff energy having maxima around the peaks. The phase-resolved spectroscopy reveals that pulsar emission is present at all rotational phases. The spectral shape, broad pulse profile, and maximum photon energy favor the outer magnetospheric emission scenarios.
Place, publisher, year, edition, pages
2010. Vol. 720, no 1, 272-283 p.
gamma rays: stars, pulsars: general, pulsars: individual (PSR J0633+1746, Geminga)
Astronomy, Astrophysics and Cosmology
IdentifiersURN: urn:nbn:se:kth:diva-26711DOI: 10.1088/0004-637X/720/1/272ISI: 000281596000025ScopusID: 2-s2.0-78149242219OAI: oai:DiVA.org:kth-26711DiVA: diva2:372698
QC 201011262010-11-262010-11-262010-11-26Bibliographically approved