AGN paper LST1

People involved

• Chaitanya Priyadarshi
• Daniel Morcuende
• David Sanchez
• Estelle Pons
• Andres Baquero
• Ryuji Takeishi
• Joshua Baxter
• Gaetano Di Marco
• Mireia Nievas
• Monica Vazquez Acosta

Slack channel

https://cta-north.slack.com/archives/C031QEQ3YDP

List of AGNs

Analysis by Chaitanya Priyadarshi using v0.7.x data and MC

Using MC with 2 different sky pointing, where the RF model was trained using the corresponding MC DL1 files

• For zenith < 30 deg, MC (point-gamma, proton and electron) and RF models used -

/fefs/aswg/data/mc/DL2/20200629_prod5_trans_80/gamma/zenith_20deg/south_pointing/20210923_v0.7.5_prod5_trans_80_dynamic_cleaning/ /fefs/aswg/data/models/20200629_prod5_trans_80/zenith_20deg/south_pointing/20210923_v0.7.5_prod5_trans_80_dynamic_cleaning/

• For zenith > 30 deg, MC (point-gamma, proton and electron) and RF models used -

/fefs/aswg/data/mc/DL2/20200629_prod5_trans_80/gamma/zenith_40deg/south_pointing/20210506_v0.7.3_prod5_trans_80_zen40deg_local_tailcut_8_4/ /fefs/aswg/data/models/20200629_prod5_trans_80/zenith_40deg/south_pointing/20210506_v0.7.3_prod5_trans_80_zen40deg_local_tailcut_8_4/

For DL3 cuts, energy-dependent cuts with an efficiency of 80% were used for gammaness and theta(only for point-like IRFs) Using the DL3 Tools of lstchain v0.9.2 and with gammapy developer build after the stable release of v0.19 (to extract signal from energy-dependent theta regions)

Mrk 421

Mrk421 coordinates:

• RA = 11h 04m 27.314s
• DEC = 38deg 12m 31.80s
• z = 0.0308

Wobble (0.4 deg), Zd < 30

Mrk421 Wobble (0.4 deg)
Date	Runs (Zd < 30, 17.23 hrs)	Runs (Zd > 30, 11 hrs)
20201212	3222-3227	3216-3221
20201213	3238, 3239
20201214	3247-3250
20210214	3661-3665	3666-3668
20210215	3687, 3688
20210216	3715, 3716	3717-3721
20210217	3732-3736
20210219	3800
20210313	4016	4017-4019
20210316	4097-4100
20210317	4131-4134	4135-4138
20210318		4479
20210320	4184, 4185	4186-4188
20210321		4208
20210412		4386-4388
20210416	4441
20210417	4457-4459
20210418		4479
20210430	4568-4572
20210505	4612-4614
20210508	4612-4614
20210509	4667-4670	4671
20210531		4852, 4853
20210601		48668, 4869
20210606		4939
20210608		4962

Wobble (0.8 or 0.5 deg)

Mrk421 Wobble (0.8 or 0.5 deg)
Date	Runs, Zd < 30, 1.76 hrs	Runs, Zd > 30, 2.18 hrs
20210212	3617-3619	3620-3624
20210213	3641	3642-3646
20210416	4442, 4443

Data analysis

Analysis by Chaitanya Priyadarshi using v0.7.x data and MC

A total of 27 hrs of data was analyzed

For DL3 data reduction to DL4 dataset,

• OFF regions selected - 1 Wobble
• Safe Energy mask for systematics - No
• Energy axes -
  • True: 10 GeV to 100 TeV with 10 bins per decade
  • Reco: 10 GeV to 40 TeV with 5 bins per decade

For spectral analysis,

• Model used - Log Parabola
• Reference energy used by calculating the decorrelation energy with a Power Law fit, ~340 GeV
• Spectral Fit energy range - 10 GeV to 40 TeV with 5 bins per decade
• Spectral fit with gammapy default optimization - minuit

Main Results

Analysis by Chaitanya Priyadarshi using v0.7.x data and MC

Preliminary LC and SED, for the full dataset-

Mrk 501

Mrk501 coordinates:

• RA = 16h 53m 52.21s
• DEC = 39deg 45m 37.6s
• z = 0.033640

Wobble observations

Mrk501 Wobble observations
Date	Runs, Zd < 30, 19.8 hrs	Runs (Zd > 30, 5.24 hrs)
20200710	2177-2180
20200909		2606-2607
20210317	4139, 4140
20210319		4167-4170
20210320	4191-4193
20210321	4212-4215
20210416	4452, 4455
20210417	4473-4476
20210418	4480	4483
20210419	4496-4498
20210503	4586-4590
20210504	4600-4602	4597-4599
20210506	4625-4628
20210507	4643-4645
20210508	4656, 4657
20210509	4673-4677	4672
20210605	4921-4933	4934
20210606	4944-4947
20210608	4977
20210612	5011
20210613	5039, 5040	5038
20210702		5095-5096
20210708	5202-5205
20210710	5227, 5228
20210801	5438	5439
20210805	5489, 5490
20210808	5550	5551
20210906	6076	6077, 6078

Data analysis

Analysis by Chaitanya Priyadarshi using v0.7.x data and MC

A total of 24.5 hrs of data was analyzed

For DL3 data reduction to DL4 dataset,

• OFF regions selected - 1 Wobble
• Safe Energy mask for systematics - No
• Energy axes -
  • True: 10 GeV to 100 TeV with 10 bins per decade
  • Reco: 10 GeV to 40 TeV with 5 bins per decade

For spectral analysis,

• Model used - Log Parabola
• Reference energy used by calculating the decorrelation energy with a Power Law fit, ~490 GeV
• Spectral Fit energy range - 10 GeV to 40 TeV with 5 bins per decade
• Spectral fit with gammapy default optimization - minuit

Main Results

Analysis by Chaitanya Priyadarshi using v0.7.x data and MC

Preliminary LC and SED, for the full dataset-

PG 1553+113

Data available

In total there is 35 runs analysed

Date	Runs
20210322	4207
20210408	4333-4334-4335-4336
20210409	4343-4344
20210411	4363-4364-4365-4366-4367-4368-4369-4370
20210421	4514-4515-4516
20210508	4652-4653-4654
20210604	4902-4903-4904-4905
20210606	4930-4931-4932-4940-4941-4942-4943
20210609	4987-4988-4989

2 runs might be removed at the end

Data analysis

We used the V0.7.3 and V0.7.1 data and used the corresponding IRFs (there is a wide spread of zenith angle) for each run. The background model was computed using the tool of Mathieu de Bony presented at the analysis call

Main Results

Livetime : 8.07 h

Significance : 13.5

Excess : 1624.9

S/B : 0.145

Rate : 3.36 per min

Count map of PG 1553

Theta2 plot

Excess and Significance map

Zd<30	Zd>30
Livetime : 6.34 h Significance : 13.8 Excess : 1462.83 S/B : 0.18	Livetime : 2.33 h Significance : 2.68 Excess : 181.6 S/B : 1.30