Fermi-LAT detection of enhanced gamma-ray activity from the FSRQ PKS 0227-369
ATel #16224; Adithiya Dinesh (Universidad Complutense de Madrid) , on behalf of the Fermi Large Area Telescope Collaboration
on 2 Sep 2023; 08:58 UT
Credential Certification: Denis Bernard (Denis.bernard@in2p3.fr)
Subjects: Gamma Ray, >GeV, Request for Observations, AGN, Blazar, Quasar
The Large Area Telescope (LAT), one of the two instruments on the Fermi Gamma-ray Space Telescope, has observed enhanced gamma-ray activity from a source positionally consistent with the flat-spectrum radio quasar PKS 0227-369, also known as 4FGL J0229.5-3644 (The Fermi-LAT collaboration 2020, ApJS, 247, 33), with coordinates R.A. = 37.368 deg, Decl. = -36.732 deg (J2000; Fomalont et al. 2003, AJ, 126, 2562), and redshift z=2.115 (Hook et al. 2003, A&A, 399, 469).
Preliminary analysis indicates that this source was in an elevated gamma-ray emission state on August 31, 2023, with a daily averaged gamma-ray flux (E>100MeV) of (0.55 +/- 0.16) X 10^-6 photons cm^-2 s^-1 (statistical uncertainty only). This corresponds to a flux increase of a factor of 20 relative to the average flux reported in the fourth Fermi-LAT catalog (4FGL). This is comparable to the highest daily flux ever observed with the LAT for this source. The corresponding photon index is 2.39 +/- 0.27, and is consistent with the 4FGL value of 2.60 +/- 0.034 within the uncertainties.
Because Fermi normally operates in an all-sky scanning mode, regular gamma-ray monitoring of this source will continue. We encourage multifrequency observations of this source. For this source, the Fermi-LAT contact person is Adithiya Dinesh (adinesh@ucm.es).
The Fermi-LAT is a pair conversion telescope designed to cover the energy band from 20 MeV to greater than 300 GeV. It is the product of an international collaboration between NASA and DOE in the U.S. and many scientific institutions across France, Italy, Japan and Sweden.
