CTA Top Level Use Cases F2F meeting #2

Europe/Berlin
409 (Bologna (Italy))

409

Bologna (Italy)

INAF/IASF Bologna Via Gobetti 101
Andrea Bulgarelli (INAF/IASF Bologna), Fabian Schüssler (IRFU), Sera Markoff (Astronomical Institute 'Anton Pannekoek', University of Amsterdam)
Description
Discussion on CTA Top Level Use Cases. First day: discussion on science-related use cases Second day: discussion on observatory-related use cases LOC: Valentina Fioretti, Vito Conforti, Andrea Bulgarelli The CTA Observatory is an open Observatory serving multiple types of scientific users, including Guest Observers, Archive Users, and members of the CTA Consortium. The Use Cases are divided into two categories: • Science-related use cases: the goal is to understand how to perform an observation with a specific scientific objective. The focus of each Use Case is the science and the operations to perform science. The purpose is to find an agreement between scientists and engineers in term of content and language and to understand the workflow to realize scientific objectives. The starting point of this work is the main scientific requirements of CTA. • Observatory-related use cases: the goal is to understand how to serve scientific users and ToO observations with conflicting scientific objectives; The Observatory-related use cases will describe how to perform observations with the CTA Observatory from a user point of view, with conflicting scientific objectives. (e.g. Submit a proposal, Review a proposal, Prepare an Observation Programme, Execute a Programme, Manage ToOs, etc.) The main purpose is to discuss the new science-related use cases (with respect to the Paris meeting), include comment on already existing science-related use cases and discuss on observatory-related use cases. For this meeting the following steps need to happen: 1) People need to let Sera, Andrea and Fabian know if they are interested in participating in this new round of UC’s. If you cannot attend Bologna please try to participate remotely. 2) Register to the Indico page for Bologna 3) Once we know who is interested we will ask who wants to work on each UC, and form small working groups under a coordinator. Ideally ~5 UC’s chosen for the exercise. 4) The coordinator of each group will make sure work on the UC (see template and older UC’s for guidance) 5) Interim progress telecon where coordinators report to the group 6) Bologna: 1 hour per UC, 10 minute presentation of UC by coordinator followed by general discussion. Sharepoint page: https://portal.cta-observatory.org/WG/obs/tluc/SitePages/Home.aspx The first 8 science-related use-cases are now on Jama: 1. UC-SCI-001: Long Term Monitoring of AGN 2. UC-SCI-002: Perform an AGN Snapshots 3. UC-SCI-003: Observe a transient discovered with RTA (Real- Time Analysis) 4. UC-SCI-004: Observe a ToO following an alert from gravitational wave observatories 5. UC-SCI-005: Observe a ToO following an alert from high-energy neutrino telescopes 6. UC-SCI-006: Observe a GRB after external alerts 7. UC-SCI-007: Observe an XRB/gamma binary from external alert 8. UC-SCI-008: Perform a Survey of a region Hotel and transportation information, here: https://www.cta-observatory.org/indico/getFile.py/access?resId=0&materialId=0&confId=1139
document
live broadcast
more information
Participants
  • Alessandro Carosi
  • Andrea Bulgarelli
  • Andreas Zech
  • Antonio Stamerra
  • Catherine Boisson
  • Claudio Melioli
  • Daniel Mazin
  • Elena Moretti
  • Eleonora Torresi
  • Elisabete de Gouveia Dal Pino
  • Emma de Ona Wilhelmi
  • Fabian Schüssler
  • Fabrizio Lucarelli
  • Felicia Krauss
  • Filippo D'Ammando
  • Francesco Longo
  • Gabriele Giovannini
  • Garret Cotter
  • Gavin Rowell
  • Gino Tosti
  • Giovanni De Cesare
  • Giulia Stratta
  • Holder Jamie
  • Jerome Rodriguez
  • Jürgen Knödlseder
  • Karl Kosack
  • Marcello Giroletti
  • Markoff Sera
  • Paolo Goldoni
  • pierre-olivier petrucci
  • Saverio Lombardi
  • stefano Vercellone
  • Valentina Fioretti
  • Wednesday 22 June
    • 09:00 09:30
      Observe a GRB after external alerts 30m
      Speaker: Dr Jerome Rodriguez (CEA/DSM-IRFU/SAp)
    • 09:30 10:00
      Observe an XRB/gamma binary from external alert 30m
      Speaker: Dr Jerome Rodriguez (CEA/DSM-IRFU/SAp)
    • 10:00 10:30
      Observe a transient discovered with RTA (Real-Time Analysis) 30m
      Speakers: Dr Andrea Bulgarelli (INAF/IASF Bologna), Dr Sera Markoff (Astronomical Institute 'Anton Pannekoek', University of Amsterdam)
    • 10:30 11:00
      Observe a ToO following an alert from gravitational wave observatories 30m
      Speaker: Dr Fabian Schüssler (IRFU)
      Slides
    • 11:00 11:20
      Break 20m
    • 11:20 11:50
      Observe a ToO following an alert from high-energy neutrino telescopes 30m
      Speaker: Dr Fabian Schüssler (IRFU)
      Slides
    • 11:50 12:20
      Perform a long term Monitoring of AGN 30m
      Speaker: Prof. Catherine Boisson (LUTH - Observatoire de Paris)
    • 12:20 12:50
      Perform an AGN Snapshots 30m
      Speaker: Dr Andreas Zech (LUTH, Observatoire de Paris)
    • 13:30 14:30
      Launch 1h
    • 14:30 15:00
      Perform a Survey of a region of the sky 30m
      Speaker: Dr Karl Kosack (CEA Saclay)
      Slides
    • 15:00 16:00
      identification of new use cases 1h
      Speaker: Dr Daniel Mazin (MPI for Physics, Munich & ICRR, University of Tokyo)
      Slides
    • 16:00 17:00
      Discussion on Observing modes 1h
      Speaker: Dr Jamie Holder (University of Delaware)
      document
    • 17:00 18:00
      Tools: discussion on requirements 1h
  • Thursday 23 June
    • 09:00 11:00
      Observatory-level use cases: presentation of workflow, actors and observing objects. 2h
      Slides
    • 11:00 11:30
      CTA global scheduler discussion 30m
      Speaker: Dr Emma de Ona Wilhelmi (IEEC-CSIC)
      Slides
    • 11:30 11:50
      Break 20m
    • 11:50 13:20
      Discussion on “Observe with CTA” use case 1h 30m
    • 13:30 14:30
      Launch 1h
    • 14:30 17:00
      Discussion on detailed observatory-level use cases and link with science-related use cases 2h 30m