NGC 1275

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General information

  • Name of the source: NGC 1275
  • Brief description of the source:
- Object type : FR-I Radio Galaxy + Spiral galaxy (in interaction)
- 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

  • Producer: Mireia Nievas Rosillo <mnievas@iac.es>

Data acquisition

(below some key points from Abelardo's old datacheck selection notebook, only showing those relevant for data selection)

  • ZD and AZ distributions

NGC1275 CycleI ZD AZ hist mnievas.png

  • NSB vs moon altitude and vs run number

NGC1275 CycleI MoonConditions mnievas.png

NGC1275 CycleI MoonConditions2 mnievas.png

  • Rate of cosmics

NGC1275 CycleI RateOfCosmics mnievas.png

  • Rate of pulses above a given pulse size

NGC1275 CycleI RateAboveCharge mnievas.png

  • NSB after all cuts

NGC1275 CycleI NSB aftercuts mnievas.png

Data selection

  • 204 wobble runs for the selected source (out of 246)
  • Observation time: 53.56 hours (out of 65.53 hours)
  • (most data in Perseus-MA mode, shared with IC310, some runs in NGC1275 pointing mode)
  • (moon data is removed)
1 : 2022-12-20 : [11522, 11528, 11529, 11530, 11531, 11532, 11522, 11528, 11529, 11530, 11531, 11532]
2 : 2022-12-21 : [11546, 11547, 11548, 11549, 11550]
3 : 2022-12-22 : [11566, 11568, 11569, 11570, 11571, 11572, 11573, 11574, 11566, 11568, 11569, 11570, 11571, 11572, 11573, 11574]
4 : 2022-12-23 : [11595, 11596, 11597, 11598, 11599, 11600]
5 : 2023-01-13 : [11618, 11619]
6 : 2023-01-14 : [11641, 11642, 11643, 11644, 11641, 11642, 11643, 11644]
7 : 2023-01-15 : [11660, 11661, 11662, 11663, 11660, 11661, 11662, 11663]
8 : 2023-08-15 : [13935, 13936, 13937, 13938, 13939, 13940, 13941, 13942, 13943, 13944]
9 : 2023-08-17 : [13987, 13988, 13989, 13990, 13991, 13992, 13993, 13994, 13995, 13996]
10 : 2023-08-18 : [14020, 14021, 14022, 14023]
11 : 2023-08-20 : [14069, 14070, 14071, 14072, 14073]
12 : 2023-08-21 : [14093, 14094, 14095, 14096, 14097, 14098, 14099, 14100]
13 : 2023-09-11 : [14258]
14 : 2023-09-16 : [14456]
15 : 2023-09-18 : [14495]
16 : 2023-09-19 : [14590]
17 : 2023-09-20 : [14623, 14624, 14625, 14626]
18 : 2023-09-21 : [14668, 14669]
19 : 2023-09-22 : [14700, 14701, 14702, 14703, 14704]
20 : 2023-09-23 : [14712, 14713, 14715, 14718, 14719, 14720, 14721]
21 : 2023-09-24 : [14731, 14732, 14733, 14736, 14737, 14738]
22 : 2023-10-09 : [15010, 15011, 15012, 15013, 15014, 15015, 15016, 15017]
23 : 2023-10-10 : [15039, 15040]
24 : 2023-10-11 : [15070, 15071, 15072, 15073, 15074]
25 : 2023-10-12 : [15117, 15118, 15119, 15120]
26 : 2023-11-08 : [15321, 15322, 15323, 15324, 15325, 15326, 15327]
27 : 2023-11-10 : [15401, 15402, 15403, 15404, 15405, 15406, 15407]
28 : 2023-11-11 : [15436, 15437, 15438]
29 : 2023-11-12 : [15470, 15471, 15472, 15473]
30 : 2023-11-16 : [15627, 15628, 15629, 15630, 15631]
31 : 2023-11-17 : [15660, 15661, 15662, 15663, 15664]
32 : 2023-11-19 : [15739, 15740, 15741]
33 : 2023-12-01 : [15786, 15787, 15788]
34 : 2023-12-08 : [15889, 15890, 15891, 15892, 15893]
35 : 2024-01-29 : [16423, 16424, 16425, 16426]
36 : 2024-01-30 : [16438, 16439, 16440, 16441, 16442]
37 : 2024-02-02 : [16492, 16493, 16494, 16495, 16496, 16497, 16498, 16499, 16500, 16501, 16502, 16503]
 

Analysis details

Software and analysis notebook:

  • Files (inc. provence): /fefs/aswg/workspace/mireia.nievas/NGC1275
  • Pipeline: /fefs/aswg/workspace/mireia.nievas/NGC1275/NGC1275_to_DL3.ipynb
  • lstchain: v0.10.5 originally, v0.10.7 now.
  • gammapy: 1.1
  • ctapipe: 0.19.2
  • astropy: 5.3.4

Source:

  • Coordinates: RA=49.95066663, DEC=41.5116969 (solved with astropy's SkyCoord / CDS name resolver)
  • Closest (chosen) dec track: 48.22 deg.
  • Cleaning: default, tail-cuts 8-4.
  • Analysis type: source-independent
  • IRFs: point-like, energy-dependent gammaness/theta2 cuts

Starting points:

  • MC: DL2
  • Models
  • Data: DL1b (merged files with no images)

Results

Analysis details

  • Total significance (per energy bin)
  • December flare


  • January flare

(note that the highest flux night was with Moon, so not included for now)

720px

  • Post-flare

720px

  • Per bayesian block bin (from LC analysis, see below)
Theta2 plots for different bayesian blocks
BB0 BB1
NGC1275 CycleI Theta2 bb0 mnievas.png NGC1275 CycleI Theta2 bb1 mnievas.png
BB2 BB3
NGC1275 CycleI Theta2 bb3 mnievas.png NGC1275 CycleI Theta2 bb4 mnievas.png
BB4 BB5
NGC1275 CycleI Theta2 bb5 mnievas.png NGC1275 CycleI Theta2 bb6 mnievas.png
BB6
NGC1275 CycleI Theta2 bb7 mnievas.png

Light Curve

NGC1275 CycleI LightCurveWithBB mnievas.png

SED

(from the 2nd plot, I show also the previous state for comparison)

  • Average

NGC1275 CycleI AverageSED mnievas.png

  • Flux-Binned SED

NGC1275 CycleI SEDWithBB mnievas.png

  • December

720px

  • January

720px

Bayesian blocks from the flux in the run-wise Light Curve to define flux bins, then computing one SED per block.

  • Fermi+LST

MWL Campaign