Difference between revisions of "Analysis BLLac Oct 2022"
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− | =BL Lacertae flare | + | =BL Lacertae flare Oct 2022= |
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** RA: 22 02 43.3 (hh mm ss), Dec: +42 16 40 (dd mm ss) | ** RA: 22 02 43.3 (hh mm ss), Dec: +42 16 40 (dd mm ss) | ||
** RA, Dec in deg (ICRS): 330.68038, 42.277772 | ** RA, Dec in deg (ICRS): 330.68038, 42.277772 | ||
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==Data-taking information== | ==Data-taking information== | ||
* '''Dates of data-taking''': | * '''Dates of data-taking''': | ||
− | ** 2022-10-20 ( | + | ** overview |
− | ***ZD: | + | *** https://docs.google.com/presentation/d/1tJyPyoCCOmWm1kS6j4ao_CmNMPDAIQqDWK7uRIpDNUA/edit?usp=sharing |
− | ***Transmission9km: | + | ** 2022-10-20 (2.6 h) |
− | ***Runs: | + | ***ZD: 16 - 42 deg |
+ | ***Transmission9km: n/a | ||
+ | ***Runs: 9753, 9754, 9755, 9756, 9757, 9758, 9759, 9760, 9761 | ||
***Joint observations with MAGIC | ***Joint observations with MAGIC | ||
+ | ***https://www.lst1.iac.es/datacheck/observation_overview/2022/10/CameraDailyCheck20221020.pdf | ||
− | + | ==DL1 data== | |
− | == | ||
Standard run-wise data files produced by LSTOSA. | Standard run-wise data files produced by LSTOSA. | ||
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* tailcut 8-4 (with cleaning based on pedestal RMS) | * tailcut 8-4 (with cleaning based on pedestal RMS) | ||
− | /fefs/aswg/data/real/ | + | /fefs/aswg/data/real/DL1/20221020/v0.9/tailcut84/ |
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− | + | ==Fast analysis by Seiya Nozaki (source-dependent analysis)== | |
− | == | + | ===DL2 data=== |
− | + | * lstchain v0.9.6 | |
+ | * source-dependent | ||
− | + | ===Significance of the detection=== | |
+ | * 1 Off reflected position | ||
+ | * cut | ||
+ | ** intensity > 100 | ||
+ | ** gammaness > 0.7 | ||
+ | ** alpha < 10 | ||
− | + | * statistics | |
+ | ** Number of ON events: 128864 | ||
+ | ** Number of OFF events: 113599 | ||
+ | ** Excess: 15265 | ||
+ | ** Li&Ma significance: 31 sigma | ||
− | [[File: | + | [[File:Alpha_BLLac_20221020_SNozaki.png|400px]] |
+ | ===DL3 analysis=== | ||
− | * | + | *gammapy 0.20.1 |
− | [[ | + | *cut |
+ | **intensity > 0 | ||
+ | **r: [0, 1] | ||
+ | **wl: [0.01, 1] | ||
+ | ** event_type = 32 | ||
+ | **70% efficiency gammaness cut (min_gh_cut=0.1, max_gh_cut=0.95 | ||
+ | **70% efficiency gammaness cut (min_alpha_cut=1, min_alpha_cut=20) | ||
− | * | + | * 2022-10-20 (SED) |
− | + | [[File:SED_BLLac_20221020_SNozaki.png|400px]] | |
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− | [[File: | + | * 2022-10-20 (LC) |
+ | ** > 100 GeV: (6.29 +/- 0.20) x 1E-10 / (cm2 s) | ||
+ | [[File:LC_BLLac_20221020_SNozaki.png|400px]] | ||
+ | ==Fast analysis by Chaitanya Priyadarshi (source-independent analysis)== | ||
+ | https://www.lst1.iac.es/wiki/index.php/Analysis_BLLac_Oct_2022_w_IRF_interpolation_Priyadarshi | ||
[[Data analysis | Back to the Data analysis page]] | [[Data analysis | Back to the Data analysis page]] |
Latest revision as of 12:40, 28 October 2022
Contents
BL Lacertae flare Oct 2022[edit]
General information[edit]
- Name of the source: BL Lacertae
- Brief description of the source:
- IBL / LBL
- highly variable
- z = 0.069
- RA: 22 02 43.3 (hh mm ss), Dec: +42 16 40 (dd mm ss)
- RA, Dec in deg (ICRS): 330.68038, 42.277772
Data-taking information[edit]
- Dates of data-taking:
- overview
- 2022-10-20 (2.6 h)
- ZD: 16 - 42 deg
- Transmission9km: n/a
- Runs: 9753, 9754, 9755, 9756, 9757, 9758, 9759, 9760, 9761
- Joint observations with MAGIC
- https://www.lst1.iac.es/datacheck/observation_overview/2022/10/CameraDailyCheck20221020.pdf
DL1 data[edit]
Standard run-wise data files produced by LSTOSA.
- tailcut 8-4 (with cleaning based on pedestal RMS)
/fefs/aswg/data/real/DL1/20221020/v0.9/tailcut84/
Fast analysis by Seiya Nozaki (source-dependent analysis)[edit]
DL2 data[edit]
- lstchain v0.9.6
- source-dependent
Significance of the detection[edit]
- 1 Off reflected position
- cut
- intensity > 100
- gammaness > 0.7
- alpha < 10
- statistics
- Number of ON events: 128864
- Number of OFF events: 113599
- Excess: 15265
- Li&Ma significance: 31 sigma
DL3 analysis[edit]
- gammapy 0.20.1
- cut
- intensity > 0
- r: [0, 1]
- wl: [0.01, 1]
- event_type = 32
- 70% efficiency gammaness cut (min_gh_cut=0.1, max_gh_cut=0.95
- 70% efficiency gammaness cut (min_alpha_cut=1, min_alpha_cut=20)
- 2022-10-20 (SED)
- 2022-10-20 (LC)
- > 100 GeV: (6.29 +/- 0.20) x 1E-10 / (cm2 s)
Fast analysis by Chaitanya Priyadarshi (source-independent analysis)[edit]
https://www.lst1.iac.es/wiki/index.php/Analysis_BLLac_Oct_2022_w_IRF_interpolation_Priyadarshi