Difference between revisions of "NGC 1275"
(→Related analysis pages) |
|||
| Line 13: | Line 13: | ||
[[ 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 ) | ||
| + | |||
| + | = Cycle I (including major flare Dec 2022) = | ||
| + | |||
| + | === Data selection === | ||
| + | |||
| + | * Zenith distance / AZ distributions (before cuts) | ||
| + | |||
| + | [[File:NGC1275_CycleI_ZD_AZ_hist_mnievas.jpg]] | ||
| + | |||
| + | |||
| + | |||
== Preliminary results == | == Preliminary results == | ||
Revision as of 16:24, 6 February 2024
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 )
Cycle I (including major flare Dec 2022)
Data selection
- Zenith distance / AZ distributions (before cuts)
File:NGC1275 CycleI ZD AZ hist mnievas.jpg
