784
Comment:
|
872
|
Deletions are marked like this. | Additions are marked like this. |
Line 7: | Line 7: |
||Ponti || Chandra || || || ToO: If SgrA* gets brighter than Lx = 10^38 erg/s || || |
|
Line 11: | Line 13: |
|| Gillessen || SINFONI || Watching a gas cloud disrupt [...] || 70h || two epochs of deep integral field spectroscopy to follow evolution of line shape || 22.12.2012 || | || Gillessen || SINFONI || Watching a gas cloud disrupt [...] || 70h || Two epochs of deep integral field spectroscopy to follow evolution of line shape || 22.12.2012 || |
Observing proposals for 2013
Approved observing proposals
PI |
Instrument |
Title |
Allocated Time |
Strategy |
UT observing dates |
Baganoff |
Chandra |
|
6 x 20ksec |
Roughly monthly sampling around pericenter time |
|
Ponti |
Chandra |
|
|
ToO: If SgrA* gets brighter than Lx = 10^38 erg/s |
|
Submitted observing proposals
PI |
Instrument |
Title |
Time Applied For |
Strategy |
Expected decision |
Gillessen |
SINFONI |
Watching a gas cloud disrupt [...] |
70h |
Two epochs of deep integral field spectroscopy to follow evolution of line shape |
22.12.2012 |
Gillessen |
NACO |
Watching a gas cloud disrupt [...] |
20h |
ToO: If SgrA* changes in 2013, get multi-band lightcurves |
22.12.2012 |