Difference between revisions of "GRB221009A"
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==Multi-wavelength Observations== | ==Multi-wavelength Observations== | ||
+ | Some references useful to understand the multi-wavelength context: | ||
+ | |||
+ | * Swift: https://www.swift.ac.uk/burst_analyser/01126853/ | ||
+ | |||
+ | * Fermi-GBM: https://arxiv.org/pdf/2303.14172.pdf | ||
+ | |||
+ | * Fermi-LAT: https://agenda.infn.it/event/33457/contributions/204976/attachments/109809/156172/BISSALDI_TeVPa_BoatGRB_230913.pdf | ||
+ | |||
+ | * H.E.S.S. paper. (53 hours after) : https://arxiv.org/pdf/2303.10558.pdf | ||
+ | |||
+ | * LHAASO paper (last stage at 10^3s): https://arxiv.org/pdf/2306.06372.pdf | ||
+ | |||
+ | * AGILE paper: https://arxiv.org/pdf/2309.10515 | ||
+ | |||
+ | * Discussion on how to retrieve points in the non-detection case: | ||
+ | ** MAGIC sGRB https://arxiv.org/abs/2012.07193 | ||
+ | |||
+ | * Discussion on modelling/jet structure: | ||
+ | |||
+ | ** Clearest evidence of structure of a jet so far.Indirect evidence for structured jets in long GRBs has been around for a while: https://arxiv.org/abs/2206.11088 | ||
+ | ** HESS upper limits combined with radio measurements indeed already constrain parameters such as the circumburst density for the outer jet. https://arxiv.org/abs/2310.12856 | ||
+ | ** numerical simulations to study the structured jets e.g. Gottlieb et al. https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.4962G/abstract | ||
+ | ** structure evolution of the afterglow using VLBI observations. Giarratana, Salafia, Ghirlanda et al. https://arxiv.org/pdf/2311.05527.pdf | ||
+ | ** Model with late-time TeV emission in excess of the LHAASO light curve extrapolation: Zheng et al. https://arxiv.org/abs/2310.12856. They argue that the HESS upper limits provide strong constraints on the circumburst medium density at large radii (Fig. 1). | ||
+ | ** Model with late-time TeV emission consistent with LHAASO light curve extrapolation: Ren et al. https://arxiv.org/abs/2310.15886 See Fig. 3. | ||
+ | ** Two component jet model: https://arxiv.org/pdf/2212.09266 | ||
+ | |||
+ | |||
+ | == Publication status == | ||
+ | |||
+ | Targeted journal: | ||
+ | |||
+ | {| class="wikitable sortable" | ||
+ | |- | ||
+ | ! style="width: 80px;" | Section | ||
+ | ! style="width: 80px;" | Preliminary deadline | ||
+ | ! style="width: 80px;" | Status | ||
+ | ! style="width: 150px;" | Responsible (and main responsible) | ||
+ | |- style="text-align:center;" | ||
+ | | Introduction || || Ongoing || All (Monica) | ||
+ | |- style="text-align:center;" | ||
+ | | Observations || || Ongoing || All (Alice?) | ||
+ | |- style="text-align:center;" | ||
+ | | Data Analysis (Moon) || || Ongoing || Arnau, Kenta | ||
+ | |- style="text-align:center;" | ||
+ | | Data Analysis (Dark) || || Ongoing || Arnau, Kenta | ||
+ | |- style="text-align:center;" | ||
+ | | Results || || Ongoing || Arnau, Kenta | ||
+ | |- style="text-align:center;" | ||
+ | | Modelling || || Not started || Susumu | ||
+ | |- style="text-align:center;" | ||
+ | | Discussion || || Not started || All (Alessandro) | ||
+ | |- style="text-align:center;" | ||
+ | | Conclusion || || Not started || All | ||
+ | |- style="text-align:center;" | ||
+ | |} | ||
== LST Observations == | == LST Observations == | ||
Line 108: | Line 164: | ||
*** Runs: 9861 - 9863 | *** Runs: 9861 - 9863 | ||
*** Joint observations with MAGIC? : No | *** Joint observations with MAGIC? : No | ||
− | *** ELOG link: [https://www.lst1.iac.es/elog/LST+commissioning/ | + | *** ELOG link: [https://www.lst1.iac.es/elog/LST+commissioning/2456] |
*** Important comments: some clouds | *** Important comments: some clouds | ||
Line 238: | Line 294: | ||
=== Related analysis pages === | === Related analysis pages === | ||
− | :* [[ | + | :* [[ GRB221009A_calib_and_r0_to_dl1_steps | Low-level reprocessing: strong moon condition ]] |
==== Source-dependent analysis ==== | ==== Source-dependent analysis ==== |
Latest revision as of 10:58, 27 June 2024
Go back to Transient Working Group.
Go Back to Gamma-Ray Bursts (GRBs).
Contents
Alert Information[edit]
- Name/type of the alert:
- GCN notice: []
- Triggered by: Fermi GBM/Swift BAT
- Alert coordinates:
- RA: h m s, Dec: deg m s
- RA, Dec in deg (ICRS): 288.26452 deg, +19.77350 deg
- Alert arrival time:
- Other relevant information:
- Redshift (z): 0.151
Multi-wavelength Observations[edit]
Some references useful to understand the multi-wavelength context:
- Fermi-GBM: https://arxiv.org/pdf/2303.14172.pdf
- H.E.S.S. paper. (53 hours after) : https://arxiv.org/pdf/2303.10558.pdf
- LHAASO paper (last stage at 10^3s): https://arxiv.org/pdf/2306.06372.pdf
- AGILE paper: https://arxiv.org/pdf/2309.10515
- Discussion on how to retrieve points in the non-detection case:
- MAGIC sGRB https://arxiv.org/abs/2012.07193
- Discussion on modelling/jet structure:
- Clearest evidence of structure of a jet so far.Indirect evidence for structured jets in long GRBs has been around for a while: https://arxiv.org/abs/2206.11088
- HESS upper limits combined with radio measurements indeed already constrain parameters such as the circumburst density for the outer jet. https://arxiv.org/abs/2310.12856
- numerical simulations to study the structured jets e.g. Gottlieb et al. https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.4962G/abstract
- structure evolution of the afterglow using VLBI observations. Giarratana, Salafia, Ghirlanda et al. https://arxiv.org/pdf/2311.05527.pdf
- Model with late-time TeV emission in excess of the LHAASO light curve extrapolation: Zheng et al. https://arxiv.org/abs/2310.12856. They argue that the HESS upper limits provide strong constraints on the circumburst medium density at large radii (Fig. 1).
- Model with late-time TeV emission consistent with LHAASO light curve extrapolation: Ren et al. https://arxiv.org/abs/2310.15886 See Fig. 3.
- Two component jet model: https://arxiv.org/pdf/2212.09266
Publication status[edit]
Targeted journal:
Section | Preliminary deadline | Status | Responsible (and main responsible) |
---|---|---|---|
Introduction | Ongoing | All (Monica) | |
Observations | Ongoing | All (Alice?) | |
Data Analysis (Moon) | Ongoing | Arnau, Kenta | |
Data Analysis (Dark) | Ongoing | Arnau, Kenta | |
Results | Ongoing | Arnau, Kenta | |
Modelling | Not started | Susumu | |
Discussion | Not started | All (Alessandro) | |
Conclusion | Not started | All |
LST Observations[edit]
- Observation conditions
- camera summary plot [1]
- first night (Oct 10) of the GRB observation and moon Crab observation (Nov 3-5) superplots
- Dates of data-taking: 2022-10-10,12,15-18,21,23-26,28,31. 2022-11-13,16,17,20
- 2022-10-10
- Zenith range (deg): 38.8 -> 57.9
- Transmission9km: n/a
- Observation condition: moon
- Observation mode: std wobble, reduced HV
- Runs: 9604 - 9607
- Joint observations with MAGIC? : No
- ELOG link: [2]
- Important comments: Data were affected by timestamp issue. (Reprocessing is already done and results below are from reprocessed data)
- 2022-10-10
- 2022-10-12
- Zenith range (deg): 34.6 -> 50.5
- Transmission9km: n/a
- Observation condition: moon
- Observation mode: std wobble, reduced HV
- Runs: 9613 - 9617
- Joint observations with MAGIC? : Yes
- ELOG link: [3]
- Important comments: Data were affected by timestamp issue. (Reprocessing is already done and results below are from reprocessed data). Run 9613 taken with HV setting "set_hv_reduced_0.5", the others with "set_hv_reduced_0.3"
- 2022-10-12
- 2022-10-15
- Zenith range (deg): 23.8 -> 57.9
- Transmission9km: n/a
- Observation condition: dark and moon (9629,9630)
- Observation mode: std wobble
- Runs: 9625 - 9630
- Joint observations with MAGIC? : Yes, except the first 2 runs
- ELOG link: [4]
- Important comments: Data were affected by timestamp issue. (Reprocessing is already done and results below are from reprocessed data)
- 2022-10-15
- 2022-10-16
- Zenith range (deg): 32.1 -> 64.1
- Transmission9km: n/a
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9640 - 9647
- Joint observations with MAGIC? : No
- ELOG link: [5]
- Important comments: Data were affected by timestamp issue. (Reprocessing is already done and results below are from reprocessed data)
- 2022-10-16
- 2022-10-17
- Zenith range (deg): 25.9 -> 58.6
- Transmission9km: n/a
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9670 - 9677
- Joint observations with MAGIC? : Yes
- ELOG link: [6]
- Important comments: Data were affected by timestamp issue. (Reprocessing is already done and results below are from reprocessed data)
- 2022-10-17
- 2022-10-18
- Zenith range (deg): 23.1 -> 43.5
- Transmission9km: n/a
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9691 - 9696
- Joint observations with MAGIC? : No
- ELOG link: [7]
- Important comments: unstable rate in run 9691
- 2022-10-18
- 2022-10-21
- Zenith range (deg): 34.6 -> 55.6
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9802 - 9807
- Joint observations with MAGIC? : Yes
- ELOG link: [8]
- Important comments:
- 2022-10-21
- 2022-10-23
- Zenith range (deg): 32.07 -> 59.21
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9829 - 9835
- Joint observations with MAGIC? : Yes
- ELOG link: [9]
- Important comments:
- 2022-10-23
- 2022-10-24
- Zenith range (deg): 49.6 -> 58.8
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9861 - 9863
- Joint observations with MAGIC? : No
- ELOG link: [10]
- Important comments: some clouds
- 2022-10-24
- 2022-10-25
- Zenith range (deg): 43.6 -> 56
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9888 - 9891
- Joint observations with MAGIC? : Yes
- ELOG link: [11]
- Important comments:
- 2022-10-25
- 2022-10-26
- Zenith range (deg): 40 -> 56
- Observation condition: dark
- Observation mode: std wobble
- Runs: 9917 - 9920
- Joint observations with MAGIC? : Only run 9919
- ELOG link: [12]
- Important comments: run 9918,9919 are both in W2
- 2022-10-26
- 2022-10-28
- Zenith range (deg): 36.04 -> 50.09
- Observation condition: moon (first 3 runs) and dark
- Observation mode: std wobble
- Runs: 9956 - 9960
- Joint observations with MAGIC? : yes
- ELOG link: [13]
- Important comments:
- 2022-10-28
- 2022-10-31
- Zenith range (deg): 58
- Observation condition: moon
- Observation mode: std wobble
- Runs: 10021
- Joint observations with MAGIC? : yes
- ELOG link: [14]
- Important comments: calibration rate is zero, but Calibox is connected and firing
- 2022-10-31
- 2022-11-13
- Zenith range (deg): 41->58
- Observation condition: dark conditions
- Observation mode: std wobble
- Runs: 10501 - 10505
- Joint observations with MAGIC? : no
- ELOG link: [15]
- Important comments: Structure in FAULT, BUSY spikes.
- 2022-11-13
- 2022-11-16
- Zenith range (deg): 48->64
- Observation condition: dark conditions
- Observation mode: std wobble
- Runs: 10611 - 10614
- Joint observations with MAGIC? : yes
- ELOG link: [16]
- Important comments: Several spikes in rates. At 20:19, MAGIC stopped util 21:15.
- 2022-11-16
- 2022-11-17
- Zenith range (deg): 43->65
- Observation condition: dark conditions
- Observation mode: std wobble
- Runs: 10643 - 10650
- Joint observations with MAGIC? : no for 10643, yes for the rest
- ELOG link: [17]
- Important comments: Several spikes in rates.
- 2022-11-17
- 2022-11-20
- Zenith range (deg): 45->67
- Observation condition: dark conditions
- Observation mode: std wobble
- Runs: 10892 - 10899
- Joint observations with MAGIC? : yes
- ELOG link: [18]
- Important comments: Several car flashes (19:47, 19:58 and 20:58)
- 2022-11-20
Fast check: Src-indep analysis by Kenta (Kyoto)[edit]
- Email address of analyser: terauchi.kenta.74s@st.kyoto-u.ac.jp
Data info[edit]
- Overall selected observation time: min ( h)
- Selected runs: 9604 - 9607
- Position analyzed: RA 288.26452 deg, Dec +19.77350 deg
DL1 data[edit]
Used DL1b files produced by LSTOSA (lstchain v0.9.6)
/fefs/aswg/data/real/DL1/20221010/v0.9/tailcut84/
DL2 data[edit]
- Random forest:
/fefs/aswg/data/models/AllSky/20220511_allsky_std/dec_2276
- lstchain v0.9.6 with config file taken from the All Sky model
/fefs/aswg/data/models/AllSky/20220511_allsky_std/dec_2276/lstchain_84.json
Theta2 plot[edit]
- Cuts and parameters used:
- intensity > 100
- gammaness > 0.6, 0.3
- leakage < 0.2
- Eest range: 0.3 - 10 TeV
- th2 cut = 0.04
- background normalization range: 0.2 < th2 < 0.4
Significance evolution[edit]
Detailed analysis[edit]
Related analysis pages[edit]
Source-dependent analysis[edit]
Source-independent analysis[edit]