Fermi Establishes Classical Novae as a Distinct Class of Gamma-Ray Sources

The Fermi-LAT Collaboration†

†To whom correspondence should be addressed. E-mail: Teddy.Cheung@nrl.navy.mil (C.C.C.); E-mail: Pierre.Jean@irap.omp.eu (P.J.); E-mail: shore@df.unipi.it (S.N.S.)

Ackermann, M., et al. Science, Volume 345, pp. 554-558 (2014)

Provided are Fermi-LAT spectra of the four novae in ascii format.

- Energies in units of MeV at bin centers E, and minimum and maximum bin widths dEmin and dEmax, respectively
- E^2 F(E) fluxes (E2F) and 1 sigma uncertainties in units of 10^-11 erg s^-1 cm^-2; when error = 0.00, values are 2 sigma upper limits
- TS = test statistic