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||<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 || X-ray monitoring of Sgr A* during outburst || || ToO: If SgrA* gets brighter than Lx = 10^38 erg/s || ||		 ||<rowstyle="background-color: #E0E0FF;"> 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 || ||
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||<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 ||		 ||<rowstyle="background-color: #E0E0FF;"> PI || Band || Instrument || Title || Time Applied For || Strategy || Expected decision ||
|| 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 ||

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

Submitted observing proposals

PI

Band

Instrument

Title

Time Applied For

Strategy

Expected decision

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

GASCLOUDwiki: ProposalList (last edited 2014-04-01 15:02:56 by AnthonyRushton)