Difference between revisions of "OP313"

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(Preliminary results)
(Related analysis pages)
 
(One intermediate revision by the same user not shown)
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* '''Brief description of the source''':  
 
* '''Brief description of the source''':  
 
:- Object type : FSRQ
 
:- Object type : FSRQ
:- RA: 3 19 48.16 (hh mm ss), Dec: +41 30 42.1088 (dd mm ss)
+
:- RA: 13 10 28.66 (hh mm ss), Dec: +32 20 43.78 (dd mm ss)
 +
:- redshift: z=0.99591
  
 
== OP313 data analysis ==
 
== OP313 data analysis ==
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[[ Analysis_OP313_Spring_2022_ToO ]]
 
[[ 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_OP313_Dec_2023_ToO ]] (Fast analysis by Daniel, Jorge, Seiya)
 
 
[[ 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 )
 

Latest revision as of 23:17, 14 December 2023

General information[edit]

  • Name of the source: OP 313
  • Brief description of the source:
- Object type : FSRQ
- RA: 13 10 28.66 (hh mm ss), Dec: +32 20 43.78 (dd mm ss)
- redshift: z=0.99591

OP313 data analysis[edit]

Related analysis pages[edit]

Analysis_OP313_Spring_2022_ToO

Analysis_OP313_Dec_2023_ToO (Fast analysis by Daniel, Jorge, Seiya)