Difference between revisions of "OP313"

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(OP313 data analysis)
(Preliminary results)
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[[ 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 )
 
[[ 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
 
 
[[File:image.png]]
 
 
[[File:excess.png]]
 
 
[[File:Theta2_counts_OP313_6_wob_obs_Run_8099_to_8104_3_en_bins.png]]
 
 
 
No detection
 

Revision as of 22:21, 14 December 2023

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 )