Difference between revisions of "OP313"

From my_wiki
Jump to: navigation, search
(Created page with "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.h...")
 
(Related analysis pages)
 
(4 intermediate revisions by the same user not shown)
Line 1: Line 1:
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#
+
==General information==
 +
* '''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
  
http://simbad.u-strasbg.fr/simbad/sim-id?Ident=OP+313
+
== OP313 data analysis ==
  
 +
=== Related analysis pages ===
  
 +
[[ Analysis_OP313_Spring_2022_ToO ]]
  
Analysis made by Chaitanya Priyadarshi, seiya_nozaki  and  María Láinez
+
[[ Analysis_OP313_Dec_2023_ToO ]] (Fast analysis by Daniel, Jorge, Seiya)
 
 
[[File:image.png]]
 
 
 
[[File:excess.png]]
 
 
 
[[File:Theta2_counts_OP313_6_wob_obs_Run_8099_to_8104_3_en_bins.png]]
 
 
 
 
 
No detection
 

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)