TEXES Demo Science Plan |
The call for TEXES Demonstration Science proposals was made on May 15, 2006, with a deadline for receiving proposals of June 7, 2006. The PIs of successful SV applications have now been notified.
The table below summarizes the pool of observations which have been selected and approved by the Gemini Science Committee. The total available time for TEXES-DS is 36.67 hours. The observations are scheduled for July 8-11, 2006. As usual the presence of a proposed observation in the DS plan does not by any means guarantee that the observation will be executed.
DS Program # |
PI Name |
Title |
Time Awarded (hrs) |
Band |
Modes |
RA (hrs) |
Obs conditions1 |
||
Point-source Spectroscopy |
Slit-scanning |
IQ |
CC |
||||||
GN-2006A-DS-1 | Knez | The warm, dense ISM in the nucleus of the ULIRG NGC 4418 | 4.67 | 1 | 8.0 and 13.1 microns |
12.4 |
85 |
90 |
|
GN-2006A-DS-2 | Lacy | Mid-Infrared Spectroscopy of High Mass Star-forming Regions | 14.0 | 2 | 12.8, 12.8-13.7 microns |
9.0, 10.5, 12.4, 12.8, 18.7 microns | 18-23 |
any |
70 |
GN-2006A-DS-3 | Richter | Mid-Infrared Spectroscopy of Protoplanetary Disk Gas | 18.0 | 1 | 8.0, 11.6, 11.8, 12.0, 12.3, 12.8, 13.2, 13.4, 17.0 microns |
16-02 |
~70 (varies) |
~50 (varies) |
1 See the detailed observing condition constraints for the precise meaning of the %-ile categories.
Last update June 29, 2006; T. Geballe