Difference between revisions of "NGC 1275"
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[[File:NGC1275_CycleI_MoonConditions2_mnievas.png|720px]] | [[File:NGC1275_CycleI_MoonConditions2_mnievas.png|720px]] | ||
| − | == | + | * Rate of cosmics |
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| + | [[File:NGC1275_CycleI_RateOfCosmics_mnievas.png|720px]] | ||
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| + | * Rate of pulses above a given pulse size | ||
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| + | [[File:NGC1275_CycleI_RateAboveCharge_mnievas.png|720px]] | ||
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| + | === Analysis conditions === | ||
Revision as of 16:34, 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)
Mireia Nievas
Data acquisition
- ZD and AZ distributions
- NSB vs moon altitude and vs run number
- Rate of cosmics
- Rate of pulses above a given pulse size
