NGC 1068

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Source Name:NGC 1068

Type Seyfert 2/ Starburst

Source Parameters[edit]

Position: RA = 40.66962153 deg, Dec:-0.01329436 deg

Zenith = 29-70 deg

Cycle I[edit]

Analysis by Sweta Menon(sweta.menon@inaf.it)

Data from /fefs/aswg/data/real/DL1/YYYYMMDD/v0.10/tailcut84

MC files : dec_min_413


MC Model NGC 1068.jpg



E threshold 20 40 zenith.jpgE threshold 20 50 zenith.jpgE threshold 20 70 zenith.jpg


Energy threshold is quite high(~ 500 GeV) if I include all the data. So as balance between including as much events as possible, I am doing my analysis with a zenith cut of 50 deg, with a threshold of about 180 GeV. ~ 70% of events and observation time of total "good" data taken.

Low Zenith[edit]

Zenith < 50 deg

Datacheck[edit]

Verification for malfunctioning pixel clusters


20230923:[14696 14697 14698 14699]: OK Some bright pixels

20231007:[14929]: OK

20231113:[15474 15475 15476]: OK

20231116:[15615 15615 15618]: OK

20231117:[15656 15657 15658 15659]: OK

20231118:[15672]:OK?

20231119:[15706]:OK

20231208:[15883 15884 15886 15887]:OK

20231209:[15917 15918 15920]:OK (little problem with one-ish pixels)

20231214:[16085 16086 16087]: OK really good

20231217:[16195 16198]: OK

20240129:[16427 16428 16429]: VERY PROBLEMATIC PIXEL CLUSTER UNFLAGGED request put in for Cat b interleaved events calibration

20240131:[16445 16446 16447 16448]: OK

20240210:[16660, 16661]: OK

Data Quality Checks[edit]

Standard latest version of the data quality selection notebook.

Standard configuration

Cut of max_diffuse_nsb_std = 2.3

Run selection.jpg Subrun cuts.png

Theta-square Plots[edit]

Theta sqr 20 50 zenith.jpg file:///home/sweta-work/Documents/NGC_1068/LST-1_comparison_2024.jpg

=== Light-curve ===file:///home/sweta-work/Documents/NGC_1068/LST-1_comparison_2024.jpg

Lightcurve 20 50 zenith.jpg File:LST-1 comparison 2024.jpg

Spectrum[edit]

Spectrum 20 50 zenith.jpg LST-1 comparison 2024.png

High Zenith[edit]