Wine and Cheese Fall 2016: Difference between revisions

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== Massimo Robberto ==
== Massimo Robberto ==
'''GMOX and SAMOS''' <br>
'''GMOX and SAMOS''' <br>
Abstract to be added
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