Diff for "ProposalList"

Differences between revisions 1 and 13 (spanning 12 versions)

Observing proposals for 2013

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

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

-  ⇤ ← Revision 1 as of 2012-09-29 00:02:42 → 
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+   ← Revision 13 as of 2012-09-29 00:51:12 → ⇥
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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 || X-ray monitoring of Sgr A* during outburst ||  || 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 ||