Unraveling the Nature of Unidentified High Galactic Latitude Fermi/LAT Gamma-ray Sources with Suzaku
arXiv:1101.2379 · doi:10.1088/0004-637X/729/2/103
Abstract
We report on the results of deep X-ray follow-up observations of four unidentified Fermi/LAT gamma-ray sources at high Galactic latitudes using Suzaku. The studied objects were detected with high significance during the first 3 months of Fermi/LAT operation, and subsequently better localized in the Fermi/LAT 1 year catalog (1FGL). Possible associations with pulsars and active galaxies have subsequently been discussed, and our observations provide an important contribution to this debate. In particular, an X-ray point source was found within the 95% confidence error circle of 1FGL J1231.1-1410. X-ray spectrum is well-fitted by a blackbody with an additional power-law. This supports the recently claimed identification of this source with a millisecond pulsar (MSP) PSR J1231-1411. Concerning 1FGL J1311.7-3429, two X-ray sources were found within the LAT error circle. Even though the X-ray spectral and variability properties were accessed, their nature and relationship with the gamma-ray source remain uncertain. We found several weak X-ray sources in the field of 1FGL J1333.2+5056, one coinciding with CLASS J1333+5057. We argue the available data are consistent with the association between these two objects. Finally, we have detected an X-ray source in the vicinity of 1FGL J2017.3+0603. This object was recently suggested to be associated with a newly discovered MSP PSR J2017+0603, because of the spatial-coincidence and the gamma-ray pulse detection. We have only detected the X-ray counterpart of the CLASS J2017+0603, while we determined an X-ray flux upper limit at the pulsar position. All in all, our studies indicate while a significant fraction of unidentified high Galactic latitude gamma-ray sources is related to the pulsar and blazar phenomena, associations with other classes of astrophysical objects are still valid options.
Accepted for publication in the ApJ
References in corpus (11)
- Fermi Large Area Telescope Bright Gamma-ray Source List
- Bright AGN Source List from the First Three Months of the Fermi Large Area Telescope All-Sky Survey
- Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT
- The Fermi-LAT high-latitude Survey: Source Count Distributions and the Origin of the Extragalactic Diffuse Background
- Fermi Large Area Telescope Observations of Misaligned AGN
- On the relation between AGN gamma-ray emission and parsec-scale radio jets
- Three Millisecond Pulsars in FERMI LAT Unassociated Bright Sources
- A revised catalogue of EGRET gamma-ray sources
- Pulsed Gamma-rays from PSR J2021+3651 with the Fermi Large Area Telescope
- Discovery of High-Energy Gamma-Ray Pulsations from PSR J2021+3651 with AGILE
- Gamma-Ray Emission from the Broad-Line Radio Galaxy 3C111
Cited by in corpus (13)
- Fermi Large Area Telescope Fourth Source Catalog
- The Extragalactic Gamma-ray Sky in the Fermi era
- Characterizing the Optical Variability of Bright Blazars: Variability-Based Selection of Fermi AGN
- Unveiling the nature of the unidentified gamma-ray sources IV: the catalog of potential X-ray counterparts
- The Gamma-ray Blazar Quest: new optical spectra, state of art and future perspectives
- Refining the associations of the Fermi Large Area Telescope Source Catalogs
- Multiband Diagnostics of Unidentified 1FGL Sources with Suzaku and Swift X-ray Observations
- Chandra X-ray Observations of the Two Brightest Unidentified High Galactic Latitude Fermi-LAT gamma-ray Sources
- Toward Identifying the Unassociated Gamma-ray Source 1FGL J1311.7-3429 with X-ray and Optical Observations
- Optical spectroscopic observations of gamma-ray blazar candidates. IX. Optical archival spectra and further observations from SOAR and OAGH
- Suzaku X-ray Follow-up Observations of Seven Unassociated Fermi-LAT Gamma-ray Sources at High Galactic Latitudes
- Quasi-star jets as unidentified gamma-ray sources
- Suzaku Observation of Abell 1555 and Abell 1558: Searching for Non-thermal Emission from Large Scale Structure Formation