1029
Comment:
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1166
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Deletions are marked like this. | Additions are marked like this. |
Line 8: | Line 8: |
||Haggards || X-ray || Chandra || Joint Chandra/XMM/EVLA Monitoring of the Gas Cloud G2 as it Encounters Sgr A* || || || || |
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Line 13: | Line 15: |
|| Gillessen || NIR || SINFONI || Watching a gas cloud disrupt [...] || 70h || Two epochs of deep integral field spectroscopy to follow evolution of line shape || 22.12.2012 || || Gillessen || NIR || NACO || Watching a gas cloud disrupt [...] || 20h || ToO: If SgrA* changes in 2013, get multi-band lightcurves || 22.12.2012 || |
|| Gillessen || NIR || SINFONI/VLT || Watching a gas cloud disrupt [...] || 70h || Two epochs of deep integral field spectroscopy to follow evolution of line shape || 22.12.2012 || || Gillessen || NIR || NACO/VLT || Watching a gas cloud disrupt [...] || 20h || ToO: If SgrA* changes in 2013, get multi-band lightcurves || 22.12.2012 || |
Observing proposals for 2013
Approved observing proposals
PI |
Band |
Instrument |
Title |
Allocated Time |
Strategy |
UT observing dates |
Baganoff |
X-ray |
Chandra |
Monitoring the Tidal Disruption of a Gas Cloud Approaching Sgr A* |
6 x 20ksec |
Roughly monthly sampling around pericenter time |
|
Ponti |
X-ray |
Chandra |
X-ray monitoring of Sgr A* during outburst |
|
ToO: If SgrA* gets brighter than Lx = 10^38 erg/s |
|
Haggards |
X-ray |
Chandra |
Joint Chandra/XMM/EVLA Monitoring of the Gas Cloud G2 as it Encounters Sgr A* |
|
|
|
Submitted observing proposals
PI |
Band |
Instrument |
Title |
Time Applied For |
Strategy |
Expected decision |
Gillessen |
NIR |
SINFONI/VLT |
Watching a gas cloud disrupt [...] |
70h |
Two epochs of deep integral field spectroscopy to follow evolution of line shape |
22.12.2012 |
Gillessen |
NIR |
NACO/VLT |
Watching a gas cloud disrupt [...] |
20h |
ToO: If SgrA* changes in 2013, get multi-band lightcurves |
22.12.2012 |