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CCF General Meeting

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Edifici Nexus, 2nd floor, c/ Gran Capità 2-4. To arrive from the airport, take the metro line 9 and exit at "Zona Universitària" (Barcelona, Spain)

Edifici Nexus, 2nd floor, c/ Gran Capità 2-4. To arrive from the airport, take the metro line 9 and exit at "Zona Universitària"

Barcelona, Spain

Institut d'Estudis Espacials de Catalunya - IEEC c/ Gran Capità, 2-4, Edifici Nexus, 2nd floor. 08034 Barcelona
Accomodiation
Instructions how to arrive
Location of the meeting (google maps)
SeeVogh_20171002_20171003.txt
SeeVogh_20171004_20171005.txt
Markus Gaug
Registration
Participants
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  • Monday 2 October
    • 14:00 → 18:00
      Site climatology
      • 14:00
        Chilean site characterization 30m
        Speaker: Tomasz Bulik (University of Warsaw)
        Talk.pdf
      • 14:30
        Prototype Weather Monitoring System for CTA-N 20m
        Speaker: Lluis Font (UAB)
        Weather monitoring system at CTA-N.pdf
      • 14:50
        Update on All-Sky-Cameras 20m

        running analysis on existing data LP ARM, news - software, hardware, scripts, OPC-UA

        Speaker: Dusan Mandat (Institute of Physics ASCR, v. v. i.)
        Update on All-Sky-Cameras.pdf
      • 15:10
        All-Sky-Cameras for CTA 20m

        Plans for IKC

        Speaker: Dusan Mandat (Institute of Physics ASCR, v. v. i.)
        All-Sky-Cameras for CTA.pdf
      • 15:30
        Update on Sun/Moon photometer for CTA 20m
        Speaker: Jakub Jurysek (Institute of Physics of the Czech Academy of Sciences)
        photometer_jurysek_barcelona.pdf
      • 15:50
        Experience from the installation of the FRAM at CTA-S 20m
        Speaker: Jakub Jurysek (Institute of Physics of the Czech Academy of Sciences)
        cta_fram_jurysek_barcelona.pdf
      • 16:10
        Tropospheric Ozone at the CTA sites 20m
        Speaker: Markus Gaug (UAB Barcelona, Spain)
        gaug_ozone.pdf
      • 16:30
        Update on radio sonde campaigns 25m
        Speaker: Julio Marin (UV)
        Marin_radiosondes.pdf
  • Tuesday 3 October
    • 09:30 → 11:00
      Atmospheric Calibration
      • 09:30
        Molecular profiles at the CTA sites 30m
        Speaker: Pere Munar-Adrover (INAF-IAPS)
        peremunar_molecular_profiles.pdf
      • 10:00
        Status of MC Simulations 15m
        Speakers: Johan Bregeon (CNRS IN2P3 LUPM), Markus Gaug (UAB Barcelona, Spain), Michael Prouza (Institute of Physics - Prague)
        AtmoSim_update_JB.pdf
        • Piping corsika output into more than 3 simtel_array is not efficient because Corsika allocates only 1 CPU core, while 3 simtel_array's (on 3 cores each) are waiting for input basically idle. Moreover, simtel_array allocates ~1 GB of memory, cannot run more than 3 because of that.
        • We will soon call for a meeting in cta-wp-ccf-atmosim@cta-observatory.org, to organize the required MODTRAN tables by Johan.
        • The -DEXTRACLOUD option seems to be an efficient solution for the clouds only.
        • A full proton simulation setup for CTC  is available by Stan Stefanik, he will provide all his input to Johan
        • Johan asks for a person running basic tests on first output. That person should ask Konrad for help (but also Johan is avaiable)

         

         

    • 11:00 → 11:30
      Coffee break 30m
    • 11:30 → 13:00
      Atmospheric Calibration
      • 11:30
        Update on the FRAM 30m
        Speaker: Jan Ebr (Institute of Physics, Prague)
        FRAM-Ebr-Barcelona-2017.pdf
      • 12:00
        CTC for atmospheric calibration 20m
        Speaker: Stanislav Stefanik (Charles University in Prague)
        ctc_1.pdf
    • 13:00 → 14:30
      Lunch 1h 30m
    • 14:30 → 17:30
      Atmospheric Calibration
      • 14:30
        General status of the atmospheric correction projects 15m
        Speaker: Markus Gaug (UAB Barcelona, Spain)
        CCF info for Infra Interfaces CTAN v3.xlsx
        gaug_generallidar.pdf
      • 14:45
        Update on the LUPM Raman LIDAR 20m
        Speaker: George Vasileiadis (LUPM)
        Raman-LUPM.pdf
      • 15:05
        Update on the IFAE/UAB Raman LIDAR 25m
        Speakers: Mrs Camilla Maggio (UAB), Markus Gaug (UAB Barcelona, Spain), Mrs Merve Colak (IFAE)
        CCF LIDAR Presentation.pdf
      • 15:30
        Update on the CEILAP LIDAR 25m
        Speaker: Pablo Roberto Ristori (División Lidar - CEILAP - (UNIDEF-CONICET))
      • 15:55
        Status of the ARCADE LIDAR Project 20m
        Speaker: Laura Valore (INFN and University of Naples)
        valore_CCFMeeting_BarcelonaOct2017.pdf
        • Local installation:
        • Installation place:
        • Cross-calibration with MAGIC and CTA LIDARs:
      • 16:15
        UVscope: an instrument for calibration support 20m
        Speaker: Giovanni La Rosa (INAF-IASF Palermo)
        UVscope BCN.pdf
  • Wednesday 4 October
    • 09:30 → 11:20
      Common issues
      • 09:30
        Status of EoIs and plans for In-kind-contributions 30m
        Speaker: Markus Gaug (UAB Barcelona, Spain)

        Array calibration:

        Instrumentation:   

        Illuminator:    full IKC from INAF, but need to be updated for current number of devices

        UAV:    should be part of a larger IKC, but cannot be incorporated in INAF IKC.

        Methods and Software:

        Should be a global package, led by some coordinating institute, but the rest are "small" contributions, Before, the relation between A&S WG and CTAO must be legally clarified. (Might be an IKC from CTAC) 

         

        Atmospheric Calibration:

        Site Characterization:

        a) Acquired data that can be "transferred" to CTAO wihtout any IKC

        b) Certain data products want to be an IKC: ARCADE, existing photometer not, but perhaps a new one for CTA-N

        c) Spftware not included so far in EoI

        Dynamic Scheduling:

        ASC+ Ceilometer: IKC of AS-CR, EoI needs be updated for ASC w.r.t. dyn. scheduling

        Software: Should at least be led by AS-CR

         

        Atmospheric Corrections:

        FRAM+CTC: EoI of AS-CR, check whether 3 are included in EoI

        LIDAR: 2 EoI's, but one inofficial from CEILAP

        Software: Can AS-CR lead this part ?? (discuss with Michael Prouza)

         

        Weather monitoring:

        CTA-Spain:   full IKC for CTA-N + software for CTA-S

        Hadrware for CTA-S: directly pruchase by CTAO ???

         

        UVScope: IKC of ASTRI, should one UVScope be included for CTA-N? (Support of the Illuminator)

         

      • 10:00
        CTA-N infrastructure for CCF equipment 20m
        Speaker: Carla Crovari
        CTAN Infrastructure for CCF equipment.pdf
        • Markus will send an updated excel spreadsheet for infrastructure questions to the corresponding parties. 
        • CTA-N phase 2 will probably need 3-4 years (e.g. the technical building probably complete in 2021)
        • Infrastructure is probably ready in Q2 of 2019
        • CTAO will produce all foundations at once
        • There is a parallel session dedicated to INFRA @ CTA-N on Tuesday afternoon, during the general meeting, also a visit to ORM is foreseen
        • Dusan comments on the need to have soon reliable power and internet connection in CTA-S, also maintenance of instruments is difficult
        • Plans are to use intially a power generator, however nothing major is expected to happen before 1-1.5 years from now.

         

         

      • 10:20
        Status of Use Cases 20m
        Speaker: Franca Cassol (CNRS/IN2P3/CPPM)
        CTA_UseCases_Cassol.pdf
      • 10:40
        Calibration data flow in ctapipe 20m
        Speakers: Franca Cassol (CNRS/IN2P3/CPPM), Markus Gaug (UAB Barcelona, Spain)
        CalibrationDataFlow_v0.3.pdf
        NewTerminology.pdf
      • 11:00
        Publications 20m
        Speaker: Maria Concetta Maccarone (IASF-Palermo/INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo/Istituto Nazionale di Astrofisica)
        CCF_Publications_20171003_MCM.pdf
    • 11:00 → 11:30
      Coffee break 30m
    • 11:30 → 12:05
      Common issues
      • 11:30
        Split between CTAO and CTAC Calibration activities 10m
        Speakers: Gernot Maier (DESY), Markus Gaug (UAB Barcelona, Spain)
      • 11:40
        Architecture, Requirements and Interfaces from CTAO 25m
        Speaker: Alison Mitchell (Max-Planck-Institut fuer Kernphysik)
        CalibOct17CTAO.pdf
    • 12:00 → 13:00
      Array Calibration
    • 13:00 → 14:30
      Lunch 1h 30m
    • 14:30 → 17:30
      Array Calibration
      • 14:30
        CTC for array calibration 20m
        Speaker: Stanislav Stefanik (Charles University in Prague)
        ctc_2.pdf
      • 14:50
        Muon analysis in ctapipe 25m
        Speaker: Alison Mitchell (Max-Planck-Institut fuer Kernphysik)
        MuonCalibCtapipeOct17.pdf
  • Thursday 5 October
    • 09:30 → 11:00
      Array Calibration
      • 09:30
        Towards the muon calibration paper 1h 30m
        Speakers: Maria Concetta Maccarone (IASF-Palermo/INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo/Istituto Nazionale di Astrofisica), Markus Gaug (UAB Barcelona, Spain)
        1. Introduction  - ready
        2. Review of muon spectra and fluxes: ready
        3. Review of the method: ready

        4 & 5: Merge, shorten and generalize:  Markus

        6: Intensity fitting: Update with log-likelihood (Alison's thesis):  Alison

        6.2, 6.3, 6.4: Shorten and move to Section 5: Markus

        7: Systematic Uncertainties:  core of the paper, perhaps shorten a bit, if possible: Markus

        8: Simulations: core of the paper

        • keep an introduction mentionning the CORSIKA flags, and used site (atmosphere)
        • remove all further group-specific information
        • redo all simulations with Prob3b, and ctapipe
        • ask Gernot about status for Prob3b (updates from telescopes such that MC corresponds to current designs): ready for LST, SST-1M, ASTRI, ongoing for GCT, FlashCam, NectarCam, MST structure and MST-SC.
        • Common plots for all telescopes:
          • Bias and Resolution of all parameters used to derive the muon efficiency: as a function of muon energy, and as a function of mirror degradation  (perhaps also as a function of impact parameter and inclination angle, have to see how big they are).
          • Gaussianity of distributions
          • Linearity of distributions
          • Further plots will be suggested by Alison in a list at the beginning of this section

        9: Muon flagging in camera server: Cettina

        • too much ASTRI focused
        • needs to get updated with latest results (shown at this meeting)
        • include speed of algorithms
        • include Q-factor (perhaps as function of muon energy?)
        • include additional data rate obtained if the flagging is active

        10: Trigger strategies and expected rates: Markus

        • need updated MC simulations

        11: Discussion: Markus

        • rewrite according to results obtained from simulations
        • table 6 can stay (slightly updated)
        • remove all internal new requirements

        12: Conclusions: all

        • write at the end, same for abstract

        Schedules:

        • full text w/o chapter 8: 27/11/2017
        • full simulation chain with ctapipe including plots: end of 2017

        Further topics:

        • Discuss effect of large square camera for MST (effects of inclination angle), plots from Steve Fegan
        • Appendix revisited formulae for 2M telescopes: will be revisited by Alison and Teresa
        • Technical comparison of algorithm for generic telescope: might go in a separate paper, Alison to decide

         

         

    • 11:00 → 11:30
      Coffee break 30m
    • 11:30 → 13:00
      Array Calibration
      • 11:30
        Towards the muon calibration paper 1h 30m
        Speakers: Maria Concetta Maccarone (IASF-Palermo/INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo/Istituto Nazionale di Astrofisica), Markus Gaug (UAB Barcelona, Spain)
    • 13:00 → 14:30
      Lunch 1h 30m
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