Fermi Large Area Telescope Observation of a Gamma-ray Source at the Position of Eta Carinae
The Fermi LAT collaboration

TL;DR
The Fermi LAT detected a persistent gamma-ray source at Eta Carinae's position, with a stable flux and spectrum, but no clear variability or flare correlation, leaving the association unconfirmed.
Contribution
This study provides detailed gamma-ray observations of Eta Carinae, characterizing its spectrum and flux stability, and discusses the challenges in confirming its gamma-ray emission origin.
Findings
Gamma-ray source detected at Eta Carinae's position
Flux and spectrum are stable over the observation period
No gamma-ray flare or variability correlated with X-ray activity
Abstract
The Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope detected a gamma-ray source that is spatially consistent with the location of Eta Carinae. This source has been persistently bright since the beginning of the LAT survey observations (from 2008 August to 2009 July, the time interval considered here). The gamma-ray signal is detected significantly throughout the LAT energy band (i.e., up to ~100 GeV). The 0.1-100 GeV energy spectrum is well represented by a combination of a cutoff power-law model (< 10 GeV) and a hard power-law component (> 10 GeV). The total flux (> 100 MeV) is photons s cm, with additional systematic uncertainties of 10%, and consistent with the average flux measured by AGILE (Tavani et al. 2009). The light curve obtained by Fermi is consistent with steady emission. Our observations do not confirm…
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