Difference between revisions of "Template"

Latest revision as of 15:01, 7 March 2022

Alert Information[edit]

Name/type of the alert: Name
GCN notice: link
Triggered by: e.g., Swift, Fermi/LAT...
Alert coordinates:
- RA: XX XX XX.XX (hh mm ss), Dec: +/-YY YY YY.YY (dd mm ss)
- RA, Dec in deg (ICRS): XX.XX, YY.YY
Alert arrival time: UTC
Other relevant information:
- Redshift (z):

Multi-wavelength Observations[edit]

Timeline
T0+	Instrument	Outcome	Outcome specific value (flux/UL/...)	Comment	Link
-		Initial detection
		UL
		Detection

LST Observations[edit]

Dates of data-taking:
- Date (time of observation h)
  - Zenith range (deg):
  - Transmission9km:
  - Observation condition: dark, moonlight, twilight, mixed, calima, ...
  - Observation mode: e.g., ON, std or custom wobbles
  - Runs:
  - Joint observations with MAGIC? : Yes/No
  - ELOG link:
  - Important comments: delay, ...

Analysis by Name (Institute - email)[edit]

Data-taking information[edit]

Overall selected observation time:
Selected runs:
Position analyzed: RA, Dec

Monte Carlo information[edit]

Link to MC files used:
- Particle types:

DL1 data[edit]

Please include your settings to produce your DL1a and DL1b files. This includes whether you use LSTOSA, specific versions of lstchain, dllab scripts, cleaning levels, and calibration information.

Example :

Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)

original DL1a files

/fefs/aswg/data/real/DL1/20210808/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5
/fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/XXX/zenith_20deg/south_pointing/20210416_v0.7.3_prod5_trans_80_local_taicut_8_4/

real data: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning

 /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/lstchain_standard_config.json

MC: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning, PSF+NSB tuning

 "image_modifier": {
   "increase_nsb": true,
   "extra_noise_in_dim_pixels": 0.74,
   "extra_bias_in_dim_pixels": 0.38,
   "transition_charge": 8,
   "extra_noise_in_bright_pixels": 0.052,
   "increase_psf": true,
   "smeared_light_fraction": 0.125
 },

 /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/lstchain_dl1ab_tune_MC_to_BLLac_config.json

Produced DL1b files

/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/data/
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/Run0XXXX

Random forest[edit]

Please include the path to the RF files used or your specific .json files used in producing your RFs and for which source analysis (source dependent or independent), and variables used in the RF.

Example

lstchain-0.7.6.dev242+g2086cb9

source-indep (diffuse gamma, src_r<3deg, disp_norm)

/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/RF/lstchain_standard_config.json

source-dep

/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/RF/lstchain_src_dep_config.json

DL2 data[edit]

Information about your DL2 data and settings such as: specifc versions of lstchain, specfic .json version used.

Example:

lstchain-0.7.6.dev242+g2086cb9

source-indep

/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/DL2/data/
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcindep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5

source-dep

/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/DL2/data/ 
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcdep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5

DL3 data selection[edit]

Information about your DL3 data selection.

Example

intensity > 50
r: [0, 1 ]
wl: [0.1, 1 ]
leakage_intensity_width_2: [0, 0.2 ]

source-indep
- fixed_gh_cut: 0.3
- fixed_theta_cut: 0.2

source-dep
- fixed_gh_cut: 0.7
- fixed_alpha_cut: 10

High-level analysis[edit]

Please put any information about the production of higher level analysis here.

Example

Science Tool: gammapy 0.18.2
Point-like IRF, 1D analysis

Analysis Results[edit]

Please place higher-level analysis results (Spectra, SkyMaps, Lightcurves, etc) here. If the alert was observed for several nights please add plots for each night separately and all data together.

@@ Line 1: / Line 1: @@
-Go back to [[Transient observation logbook]].
+Go back to [[Transient Working Group]].
-==Status==
-{|class="wikitable"
-!Step
-!Status
-!Comment
-|-
-|DL2 Production
-|style="background-color:#FF8000" | Ongoing
-|
-|-
-|Low Level Check
-|style="background-color:#FF8000" |To do
-|
-|-
-|DL3 Production
-|style="background-color:#FF8000" |To do
-|
-|-
-|High Level Analysis
-|style="background-color:#FF8000" |To do
-|
-|}
-Green color code : 00BA00
+== Alert Information ==
-Red Color code : FF0000
+* '''Name/type of the alert''': Name
+* '''GCN notice''': ''link''
+* '''Triggered by''': ''e.g., Swift, Fermi/LAT...''
+* '''Alert coordinates''':
+** ''RA: XX XX XX.XX (hh mm ss), Dec: +/-YY YY YY.YY (dd mm ss)''
+** ''RA, Dec in deg (ICRS): XX.XX, YY.YY''
+* '''Alert arrival time''': ''UTC''
+* '''Other relevant information''':
+** Redshift (z):
 ==Multi-wavelength Observations==
@@ Line 60: / Line 47: @@
 |}
-== Alert ==
-* '''Name/type of the alert''':
+== LST Observations ==
+* '''Dates of data-taking''':
+** Date (time of observation h)
+*** Zenith range (deg):
+*** Transmission9km:
+*** Observation condition: ''dark, moonlight, twilight, mixed, calima, ...''
+*** Observation mode: ''e.g., ON, std or custom wobbles''
+*** Runs:
+*** Joint observations with MAGIC? : ''Yes/No''
+*** ELOG link:
+*** Important comments: ''delay, ...''
+== Analysis by Name (Institute - email) ==
+=== Data-taking information ===
-* '''Triggered by''': ''e.g., Swift, Fermi/LAT...''
+* Overall selected observation time:
+* Selected runs:
+* Position analyzed: ''RA, Dec''
+=== Monte Carlo information ===
+* Link to MC files used:
+** Particle types:
+=== DL1 data ===
+Please include your settings to produce your DL1a and DL1b files.  This includes whether you use LSTOSA, specific versions of lstchain, dllab scripts, cleaning levels, and calibration information.
+'''Example''' :
+Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)
+* original DL1a files
-* '''Alert coordinates''': ''RA, Dec (J2000)''
+ /fefs/aswg/data/real/DL1/20210808/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5
+ /fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/XXX/zenith_20deg/south_pointing/20210416_v0.7.3_prod5_trans_80_local_taicut_8_4/
-* '''Alert arrival time''': ''UTC''
+* real data: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning
-* '''Additional info''': ''e.g., redshift, signalness...''
+  /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/lstchain_standard_config.json
-== LST Observations ==
+* MC: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning, PSF+NSB tuning
+  "image_modifier": {
+    "increase_nsb": true,
+    "extra_noise_in_dim_pixels": 0.74,
+    "extra_bias_in_dim_pixels": 0.38,
+    "transition_charge": 8,
+    "extra_noise_in_bright_pixels": 0.052,
+    "increase_psf": true,
+    "smeared_light_fraction": 0.125
+  },
-* '''Time and date of start/stop of data-taking''':  ''e.g., 00:10:00 2021-11-18 to 02:22:20 2021-11-18''
+  /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/lstchain_dl1ab_tune_MC_to_BLLac_config.json
-* '''Delay''':
+* Produced DL1b files
-* '''Overall observation time''':
+ /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/data/
+ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/Run0XXXX
-* '''Observation mode''': ''e.g., ON, std or custom wobbles''
+=== Random forest ===
-* '''Observed source position''':
+Please include the path to the RF files used or your specific .json files used in producing your RFs and for which source analysis (source dependent or independent), and variables used in the RF.
-* '''Observation condition''': ''dark, moonlight, twilight, mixed, calima, ...''
+'''Example'''
-* '''Zenith range''':
+* lstchain-0.7.6.dev242+g2086cb9
-* '''ELOG link''':
+* source-indep (diffuse gamma, src_r<3deg, disp_norm)
+ /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/RF/lstchain_standard_config.json
-* '''Important comments''':
+* source-dep
+ /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/RF/lstchain_src_dep_config.json
-* '''Run list''' :
+=== DL2 data ===
-{|class="wikitable"
+Information about your DL2 data and settings such as: specifc versions of lstchain, specfic .json version used.
-!Run number
-!Start date
-!Stop date
-!Drive target name
-!RA
-!Dec
-!Observation condition
-|-- style="text-align:center;"
-|3314 || 2020-12-17 20:31 || 2020-12-17 20:50 ||Crab || 83.633080 || 22.014500 || Moon
-|-- style="text-align:center;"
-| || || || || || ||
-|-
-|}
-==Low level check==
+'''Example''':
-Run xxxxxx : pdf file low level check
+* lstchain-0.7.6.dev242+g2086cb9
-Run xxxxxx : pdf file low level check
+* source-indep
+ /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/DL2/data/
+ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcindep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5
-Run xxxxxx : pdf file low level check
+* source-dep
+ /fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcdep/DL2/data/
+ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcdep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5
-Run xxxxxx : pdf file low level check
+=== DL3 data selection ===
-Upload low level check plots and comment possible issue and action taken
+Information about your DL3 data selection.
-== High Level Analysis ==
+'''Example'''
+*intensity > 50
+*r: [0,  1 ]
+*wl: [0.1, 1 ]
+*leakage_intensity_width_2: [0, 0.2 ]
-=== Analysis configuration ===
+* source-indep
+**fixed_gh_cut: 0.3
+**fixed_theta_cut: 0.2
-* '''Name and contact info of the analyzer''':
+* source-dep
+**fixed_gh_cut: 0.7
+**fixed_alpha_cut: 10
-* '''Software versions''':
+=== High-level analysis ===
-* '''Cuts and parameters used''':
+Please put any information about the production of higher level analysis here.
-* '''DL2 MC data used''':
+'''Example'''
-* '''Overall selected observation time''':
+* Science Tool: gammapy 0.18.2
+* Point-like IRF, 1D analysis
-* '''Position analyzed''': ''e.g., RA, DEC''
+== Analysis Results ==
-* '''Analysis/data problems''':
+Please place higher-level analysis results (Spectra, SkyMaps, Lightcurves, etc) here.
+If the alert was observed for several nights please add plots for each night separately and all data together.
 === Theta2 plot ===
-''If the alert was observed for several nights please add plots for each night separately and all data together.''
 === Significance map ===
-''If the alert was observed for several nights please add plots for each night separately and all data together.''
 === Excess map ===
-''If the alert was observed for several nights please add plots for each night separately and all data together.''
 === Spectral results ===

Difference between revisions of "Template"

Latest revision as of 15:01, 7 March 2022

Contents

Alert Information[edit]

Multi-wavelength Observations[edit]

LST Observations[edit]

Analysis by Name (Institute - email)[edit]

Data-taking information[edit]

Monte Carlo information[edit]

DL1 data[edit]

Random forest[edit]

DL2 data[edit]

DL3 data selection[edit]

High-level analysis[edit]

Analysis Results[edit]

Theta2 plot[edit]

Significance map[edit]

Excess map[edit]

Spectral results[edit]

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