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=== Approved observing proposals === ||<rowstyle="background-color: #E0E0FF;"> PI || Instrument || Title || Allocated Time || Strategy || UT observing dates || ||Baganoff || Chandra || Monitoring the Tidal Disruption of a Gas Cloud Approaching Sgr A* || 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 === ||<rowstyle="background-color: #E0E0FF;"> 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 || |
Observing proposals for 2013
Approved observing proposals
PI |
Instrument |
Title |
Allocated Time |
Strategy |
UT observing dates |
Baganoff |
Chandra |
Monitoring the Tidal Disruption of a Gas Cloud Approaching Sgr A* |
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 |