Difference between revisions of "NGC 1275"
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=== Related analysis pages === | === Related analysis pages === | ||
| − | [[ Analysis_NGC1275_Dec_2022_w_IRF_interpolation_Priyadarshi ]] (Dec | + | [[ 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 ) | [[ 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 == | == Preliminary results == | ||
Revision as of 13:13, 26 December 2022
Contents
General information
- Name of the source: NGC 1275
- Brief description of the source:
- - Object type : Seyfert 2 Galaxy
- - RA: 3 19 48.16 (hh mm ss), Dec: +41 30 42.1088 (dd mm ss)
NGC 1275 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 )
