We present the results of our analysis of cosmic-ray electrons using about 8 x 10(6) electron candidates detected in the first 12 months on-orbit by the Fermi Large Area Telescope. This work extends our previously published cosmic-ray electron spectrum down to 7 GeV, giving a spectral range of approximately 2.5 decades up to 1 TeV. We describe in detail the analysis and its validation using beam-test and on-orbit data. In addition, we describe the spectrum measured via a subset of events selected for the best energy resolution as a cross-check on the measurement using the full event sample. Our electron spectrum can be described with a power law proportional to E(-3.08+/-0.05) with no prominent spectral features within systematic uncertainties. Within the limits of our uncertainties, we can accommodate a slight spectral hardening at around 100 GeV and a slight softening above 500 GeV.

Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV / Ackermann, M., Ajello, M., Atwood, W.b., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Baughman, B.m., Bechtol, K., Bellardi, F., Bellazzini, R., Belli, F., Berenji, B., Blandford, R.d., Bloom, E.d., Bogart, J.r., Bonamente, E., Borgland, A.w., Brandt, T.j., Bregeon, J., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - STAMPA. - 82:9(2010). [10.1103/PhysRevD.82.092004]

Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV

FAVUZZI, Cecilia;GIGLIETTO, Nicola;
2010

Abstract

We present the results of our analysis of cosmic-ray electrons using about 8 x 10(6) electron candidates detected in the first 12 months on-orbit by the Fermi Large Area Telescope. This work extends our previously published cosmic-ray electron spectrum down to 7 GeV, giving a spectral range of approximately 2.5 decades up to 1 TeV. We describe in detail the analysis and its validation using beam-test and on-orbit data. In addition, we describe the spectrum measured via a subset of events selected for the best energy resolution as a cross-check on the measurement using the full event sample. Our electron spectrum can be described with a power law proportional to E(-3.08+/-0.05) with no prominent spectral features within systematic uncertainties. Within the limits of our uncertainties, we can accommodate a slight spectral hardening at around 100 GeV and a slight softening above 500 GeV.
2010
Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV / Ackermann, M., Ajello, M., Atwood, W.b., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Baughman, B.m., Bechtol, K., Bellardi, F., Bellazzini, R., Belli, F., Berenji, B., Blandford, R.d., Bloom, E.d., Bogart, J.r., Bonamente, E., Borgland, A.w., Brandt, T.j., Bregeon, J., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - STAMPA. - 82:9(2010). [10.1103/PhysRevD.82.092004]
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/6268
Citazioni
  • Scopus 387
  • ???jsp.display-item.citation.isi??? 307
social impact