OP313

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Revision as of 22:21, 14 December 2023 by Nozaki (talk | contribs) (OP313 data analysis)
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General information

  • Name of the source: OP 313
  • Brief description of the source:
- Object type : FSRQ
- RA: 3 19 48.16 (hh mm ss), Dec: +41 30 42.1088 (dd mm ss)

OP313 data analysis

Related analysis pages

Analysis_OP313_Spring_2022_ToO

Analysis_NGC1275_Dec_2022_w_IRF_interpolation_Priyadarshi (Dec 2022, source-independent, IRF interpolation, energy-dependent cuts. Dec 20 flare for ATel https://www.astronomerstelegram.org/?read=15819 )

Analysis_NGC1275_Dec_2022_source_dep_Nozaki (Dec 20 Flare, source-dependent, IRF interpolation, energy-dependent cuts for ATel https://www.astronomerstelegram.org/?read=15819 )

Preliminary results

We took some data last night on OP 313 since a fermi analysis showed it was in a high state (~ 0.5 1e-6 /cm^2/s):

https://fermi.gsfc.nasa.gov/ssc/data/access/lat/lcr/source.html?source_name=4FGL_J1310.5+3221#

http://simbad.u-strasbg.fr/simbad/sim-id?Ident=OP+313


Analysis made by Chaitanya Priyadarshi, seiya_nozaki and María Láinez

Image.png

Excess.png

Theta2 counts OP313 6 wob obs Run 8099 to 8104 3 en bins.png


No detection