Diff for "ProposalList"

Differences between revisions 25 and 26

Observing proposals for 2013

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 / HETG	X-ray monitoring of Sgr A* during outburst	280ksec	ToO: If SgrA* gets brighter than Lx = 10^36 erg/s
Haggard	X-ray	Chandra	Joint Chandra/XMM/EVLA Monitoring of the Gas Cloud G2 as it Encounters Sgr A*	6 x 50ksec	Roughly monthly sampling around pericenter time
public NRAO	radio	VLA	Continuum monitoring	13 x 2hrs x 8 bands	initially bimonthly, then monthly monitoring	link to eNews letter will follow
public NRAO	radio	VLBA	Angular size measurements and astrometry of SgrA*	13 x 2hrs x 8 bands	single, pre-encounter, baseline measurement	beginning of semester 2013A, link to eNews letter will follow

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
Ponti	X-ray	XMM	Capturing a major accretion event of Sgr A*	230ks	ToO: If Sgr A* becomes brighter than 10^35 erg/s	late 12-12
Ponti	X-ray	XMM	Monitoring Sgr A*	200ks	Monitoring the cloud-SgrA* interaction	late 12-12
Boller	X-ray	XMM	Testing GR with XMM-Newton observations in the Galactic Centre	50ks	Selection of observable tests of GR with luminous features close to the GC, ToO	late December 2012
Haggard	X-ray	Swift	Swift Monitoring of the Encounter Between Sgr A* and the Gas Cloud G2	68ks	Monitoring weekly, then twice weekly, then daily (near pericenter)	late 2012 or early 2013

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+||public NRAO || radio || VLA || Continuum monitoring ||  13 x 2hrs x 8 bands || initially bimonthly, then monthly monitoring || link to eNews letter will follow ||
||public NRAO || radio || VLBA || Angular size measurements and astrometry of SgrA* || 13 x 2hrs x 8 bands || single, pre-encounter, baseline measurement  || beginning of semester 2013A, link to eNews letter will follow ||