Wine and Cheese Fall 2016: Difference between revisions
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== Massimo Robberto == | == Massimo Robberto == | ||
'''GMOX and SAMOS''' <br> | '''GMOX and SAMOS''' <br> | ||
NSF has recently funded a JHU-led collaboration to build SAMOS, a novel multi-slit spectograph for the 4.1m SOAR telescope in Chile. SAMOS exploits the ground-layer AO system to take hundreds of faint spectra in parallel at R~2000 over a 3’x’3’ field of view. At the same time, Gemini has contracted us with the study of an expanded version of SAMOS, GMOX, to be installed at the Multi-Conjugate extreme-AO system of Gemini South. GMOX covers the full U to K bandpass at R~5000 and can synthetize slits as small as a single HST/WFC3-vis pixel (40mas), reaching unpredentented levels of sensitivity in the near-IR from the ground. I will present the main characteristics of the instruments, their current status, and an outline of the type of science programs that can be carried out in the substantial amount of GTO time. | |||
== Bram Ochsendorf == | == Bram Ochsendorf == | ||
'''TBD''' <br> | '''TBD''' <br> |
Revision as of 15:05, 2 September 2016
This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Fall 2016.
Wine and Cheese sessions with one talk will have a 50 minute talk with 10 minutes for questions. Sessions with two speakers will have two 25 minute talks, each with 5 minutes for questions.
Back to W&C Schedule
September 12th
Exoplanet Workshop at STScI
September 19th
Massimo Robberto
GMOX and SAMOS
NSF has recently funded a JHU-led collaboration to build SAMOS, a novel multi-slit spectograph for the 4.1m SOAR telescope in Chile. SAMOS exploits the ground-layer AO system to take hundreds of faint spectra in parallel at R~2000 over a 3’x’3’ field of view. At the same time, Gemini has contracted us with the study of an expanded version of SAMOS, GMOX, to be installed at the Multi-Conjugate extreme-AO system of Gemini South. GMOX covers the full U to K bandpass at R~5000 and can synthetize slits as small as a single HST/WFC3-vis pixel (40mas), reaching unpredentented levels of sensitivity in the near-IR from the ground. I will present the main characteristics of the instruments, their current status, and an outline of the type of science programs that can be carried out in the substantial amount of GTO time.
Bram Ochsendorf
TBD
Abstract to be added
September 26th
Speaker Name
Title
Abstract to be added
October 3rd
David Hogg
Chemical tagging of stars with a data-driven model
Abstract to be added
October 10th
Cole Miller
TBD
Abstract to be added
October 17th
JHU-GSFC Interaction Day
October 24th
Speaker Name
Title
Abstract to be added
October 31st
Special Halloween Speakers
Title
Attendance in costume is optional
November 7th
Anthony Pullen
Revealing Intensity Fluctuations with LSS Tracers
Abstract to be added
November 14th
High Contrast Imaging Workshop at STScI
November 21st
Thanksgiving Break
November 28th
Aki Roberge
Star-Grazing Exocomets Around Nearby Young Stars and Big Bang to Biosignatures: The LUVOIR Decadal Mission Concept
A double-barreled talk!
December 5th
Speaker Name
Title
Abstract to be added
December 12th
Subaru Meeting