Phase B Preparation Workshop
Introduction | Logistics | Preparation | Programme | Upload slides
Introduction
We are planning to hold a workshop in late April to kick-start the preparation of the science cases for Level 3 development effort in the Phase B proposal. As you know, Phase B is due to run from April 2019 to March 2023, thereby spanning LSST Commissioning and the start of survey operations. The DEV side of the Phase B proposal should, therefore, focus on what we could do (R&D tasks, not exploitation) with the commissioning data and what is needed for early science with LSST. The intention is that this workshop should inform the development of those cases by providing a more detailed description of what we can expect from the Project - in terms of data products, software and computing infrastructure - and comparing that with the requirements for some of our high priority science cases, thereby yielding a better idea of what we must provide ourselves, funded through the Phase B award.
From initial discussion with Mario Juric and Andy Connolly in the LSST Project team, we have come up with the following initial plan.
Logistics
Registration: Please add your name and details on the Phase B Prep W/shop Participants page to help us coordinate catering, venue, etc.
Dates: 26th—28th April 2017
Location: Royal Observatory Edinburgh
Accommodation: Accommodation options in the vicinity of the Royal Observatory are listed on the ROE website. Of particular note, the Travel Lodge at Cameron Toll is conveniently located on major public transport links to/ from city, around a 15-minutes walk from the observatory.
Social events: We have not arranged any group dinners, to enable you to explore Edinburgh a little, but here are some suggested restaurants.
Pre-meeting preparation
- The recommended Wi-Fi network for use during the meeting is Eduroam. You may wish to check you have your current Eduroam credentials, before travelling.
- Read the Data Products Definition Document.
- Read the Juric et al paper on The LSST Data Management System from ADASS XXV [https://arxiv.org/abs/1512.07914]
- Install some Python software on laptop — LSST Software Tutorial Notes
Final Programme:
Slides from talks are (will be) available from here, as well as being linked from the programme below.
Day One: What to expect from the LSST Project
- 09.00: Workshop Introduction (Bob Mann)
- 09.30: Session 1 (1.5hr): Level 1 (Eric Bellm)
- Difference Image Analysis pipeline data products
- Alert stream and Level 1 database: what to do with which and how
- Brokers - what will the Project deliver? What are the constraints on developments by others (e.g. LSST:UK)?
- 11.00: coffee
- 11.30: Session 2 (1.5 hr): Level 2 (Robert Lupton)
- Outline of direct imaging pipeline, highlighting key algorithms
- Specification of direct imaging data products
- Availability of data products (policies and practicalities) - e.g. which images and how soon?
- Data Release production and Data Access Centre capabilities
- 13.00: lunch
- 14.00: Session 3 (1.5 hr): Level 3 (Mario Juric and Simon Krughoff)
- DAC concepts and plans
- Availability of LSST software stack to use in Level 3 re-reductions and analysis
- Data access software
- Environment to support development of Level 3 software (and constraints on that software)
- Standards-compliance - e.g. how easy to use astropy, VO tools, etc.
- Video of Simon K's Juptyer Lab demos are available from https://github.com/lsst-dm/sciplat-examples; the notebooks and instructions will be added there soon. The videos may also be viewed on YouTube: https://www.youtube.com/playlist?list=PLOVYFNUhDEm_gTJXLFhxgh1bgu-pCI0s1
- 15.30: tea
- 16.00: Session 4 (1 hr): LSST Simulations (Lynne Jones, remotely)
Introduction to scope and aims of different packages - PhoSim, CatSim, AlertSim, OpSim, MAF, GalSim.
- More detailed descriptions of use of some: i.e. MAF, GalSim/PhoSim, CatSim (possibly also AlertSim?)
- 17.00: Session 5 (0.5 hr): LSSTC and Science Collaborations (Pat Eliason, remotely, with slides from Lucianne Walkowicz)
- Role of LSSTC in operations and before - e.g. supporting scientific activities
- Science Collaborations: roles
- 17.30: close
Day Two: Requirements from high-priority UK science cases
This will be a walk-through of a number of high-priority UK science cases, describing the requirements on data (quality and quantity), software and hardware, so that we could contrast those with what had been described on Day One. The cases should be drawn from a range of science areas, so as to span the range of dependencies on the Project deliverables. Since the goal is identifying gaps for development in Phase B, the focus should be on “early science”, but it will be left to each speaker to decide whether that means use of commissioning data, first year survey data, etc
The format for these will be as follows*:
- 20 min talk:
- What is the science?
- What data is required?
- What is the computational scale of the analysis? - e.g. workstation v small cluster v supercomputer/grid
- 10 min discussion:
- Feedback from Project staff: what will and will not be available
- Identification of gaps - what might be developed into a case for the Phase B proposal?
*N.B. the stellar talks have a different timing, but the same split between talk and discussion.
- 09.00: Introduction (Bob Mann)
- 09.15: AGN (Carole Mundell)
- 09.45: Strong lensing (Aprajita Verma)
- 10.15: Weak lensing and clustering (Benjamin Joachimi)
- 10.45: Coffee
- 11.30: Extracting supernovae, variables and transients from LSST streams (Stephen Smartt)
- 12.00: Spectroscopic follow-up of transients (Mark Sullivan)
- 12.30: Supernova classification (Hiranya Peiris)
- 13.00: Lunch
- 13.45: Galactic stellar halo (Vasily Belokurov)
- 14.09: Resolved stellar populations in nearby galaxies (Vicky Scowcroft)
- 14.33: Solar neighbourhood (Ben Burningham)
- 14.57: YSO variability and main sequence clusters (Tim Naylor)
- 15.08: Stellar variability (Aleks Scholz)
- 15.19: Discussion of Naylor and Scholz talks
- 15.30: Tea
- 16.00: Solar System science: Activity, collisions and extreme objects (Alan Fitzsimmons)
- 16.30: Solar system requirements (Wes Fraser)
- 17.00: Exoplanets (Eamonn Kerins)
- 17.30: Close
Day Three: Requirements for high-priority UK science cases (cont'd) and hands-on sessions
Before participating in this tutorial, you need to install a copy of the LSST pipeline software on your laptop.
- 09.00: Multi-wavelength data fusion in the LSST fields (Manda Banerji)
- 09.30: UK participation in LSST Galaxies science: key themes (Sugata Kaviraj)
- 10.00: Clusters of galaxies (Graham Smith)
- 10.30: Coffee
- (Details from here TBC)
- 11.00: Demo of Prototype DAC using Stripe 82 data
- 11.15: UK DAC planning (Bob Mann)
- 12.00: Walk through some iPython notebooks with realistic data and simulation tools
- 13.00: Lunch
- 13.45: Walk through some iPython notebooks with realistic data and simulation tools (cont'd)
- 15.30: Tea
- 16.00: Walk through some iPython notebooks with realistic data and simulation tools (cont'd?) and other discussion (TBD)
- 17.00: Close
Attendance (deprecated, see Participant page)
- Likely to attend: Bob Mann, Sugata Kaviraj, Mark Sullivan, Benjamin Joachimi, Wes Fraser, David Bacon, Stephen Smartt, Aprajita Verma, Carole Mundell Manda Banerji, Tim Naylor, Vicky Scowcroft, Philip Lucas, Graham Smith, Nicholas Walton, WIll Hartley, Aleks Scholz, Ben Burningham, Andy Lawrence Richard McMahon, Isobel Hook
- Unlikely to attend: John Veitch (timing conflict), Jon Loveday (teaching), Annette Ferguson (away)
If you require this document in an alternative format, please contact the LSST:UK Project Managers lusc_pm@mlist.is.ed.ac.uk or phone +44 131 651 3577