Difference between revisions of "OP313"
Davidsanchez (talk | contribs) (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...") |
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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_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): | 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): | ||
Revision as of 22:19, 14 December 2023
Contents
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_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
No detection
