Difference between revisions of "Workshop2010:agenda"
From Gaia Science Alerts Working Group
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | ||
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 |
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O'Brien | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O'Brien | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 |
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 |
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
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| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 |
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley | ||
| + | |- | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | ||
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo |
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | ||
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | ||
| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke | ||
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| + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | ||
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Burgon | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:05 |
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up |
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:30 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | ||
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | ||
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| style="border-width: 0px 1px 1px 0px; border-style: solid;" | Walton?? | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Walton?? | ||
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| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14: | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | ||
| − | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''' | + | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' |
| style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG | ||
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Revision as of 16:27, 9 June 2010
Workshop's agenda
This agenda is still in its draft form and it still might change. Please contact us if you have any comments.
The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop.
It is very likely we will record all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We might also be able to stream the talks live. Details soon.
| Wednesday 23 June 2010 | ||||
| time | session | title | speaker | |
| 10:30 | Coffee and registration | |||
| 11:00 | Welcome and update on GREAT | Nick Walton | ||
| 11:15 | Gaia | Gaia status | Timo Prusti | |
| 11:35 | The Gaia mission: a primer | Francois Mignard | ||
| 12:00 | Science Alerts | LW/STH | ||
| 12:25 | Asteroid Alerts | Paolo Tanga | ||
| 12:45 | Q+A/Discussion | |||
| 13:00 | Lunch | |||
| 14:00 | Surveys | Transient and Supernovae searches with PS1 | Stephen Smartt | |
| 14:25 | High energy transients | Paul O'Brien | ||
| 14:45 | Explosive Transient Detection in the Era of Synoptic Sky Surveys | Przemek Wozniak | ||
| 15:10 | The Palomar Transient Factory | Eran Ofek | ||
| 15:30 | Tea | |||
| 16:00 | PTF - The reduction, subtraction, detection, and classification pipelines + some results | Dovi Poznanski | ||
| 16:20 | Optical transients detected by the Wide Angle Search for Planets (WASP) | Peter Wheatley | ||
| 16:40 | Real-time Transient classification, follow-up and the way forward | Ashish Mahabal | ||
| 17:05 | Q+A/Discussion | |||
| 17:30 | end of day 1 | |||
| 18:30(TBC) | Reception and dinner in Churchill College | |||
| Thursday 24 June 2010 | ||||
| time | session | title | speaker | |
| 09:30 | Surveys | Gaia in the context of low-redshift transient surveys | Mark Sullivan | |
| 10:00 | The PTF core-collapse supernova key project | Avishay Gal-Yam | ||
| 10:20 | Supernova monitor programs | Massimo Turatto | ||
| 10:40 | Variability, outbursts and mass loss amongst massive evolved stars | Simon Clark | ||
| 11:00 | Coffee | |||
| 11:30 | Science | GRB science with GAIA | Nial Tanvir | |
| 11:50 | Orphan GRB afterglows with GAIA | Andrew Levan | ||
| 12:10 | Gaia Microlensing Alerts | Andrew Gould | ||
| 12:40 | Microlensing live and in colour | Martin Dominik | ||
| 13:00 | Lunch | |||
| 14:00 | Science | Workshop photo | ||
| 14:10 | Accretion-driven transients in the Galaxy | Danny Steeghs | ||
| 14:30 | The galactic population of cataclysmic variables. | Boris Gaensicke | ||
| 14:50 | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | Agnes Kospal | ||
| 15:10 | R Coronae Borealis variability and Galactic distribution | Patrick Tisserand | ||
| 15:30 | Tea | |||
| 16:00 | Science | Q+A/Discussion/Summary | ||
| 16:30 | Outreach | Outreach possibilties with Gaia and Hands-On-Universe | Roger Ferlet | |
| 16:55 | Outreach/Citizen's Science potential of GAIA Science Alert System. | Lech Mankiewicz | ||
| 17:20 | Q+A/Discussion | |||
| 17:30 | end of day 2 | |||
| Friday 25 June 2010 | ||||
| time | session | title | speaker | |
| 09:30 | Gaia | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | Elena Pancino | |
| 09:55 | Ground Based Optical Tracking of Gaia | Martin Altmann | ||
| 10:15 | Gaia and variable stars ; Ground based follow-up | Laurent Eyer | ||
| 10:35 | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | Rene Hudec | ||
| 11:00 | Coffee | |||
| 11:30 | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | George Seabroke | ||
| 11:50 | Alerts distributions possibilities | Ross Burgon | ||
| 12:05 | Follow-up | Follow-up opportunities with robotic telescopes | Sarah Roberts | |
| 12:30 | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | Iain Steele | ||
| 13:00 | Lunch | |||
| 14:00 | Discussion | Discussion - towards the Road Map | Walton?? | |
| 14:45 | Concluding summary | NAW/LW/STH/FvL/GG | ||
| 15:00 | end of day 3 | |||
