The definitive schedule will always be the long term and short term schedules found on the Chandra web pages:

 

.

The Chandra schedule is always subject to change, so please consult the schedules near the time of any multi-wavelength observation to check on the status of the Chandra observation.


As of today, July 8, 2012, the following is the *long term* schedule. Observations are “week of” and year 2012.  Specific dates are subject to change as the Chandra schedule evolves:


ObsID     Exposure          Week (UT)         Best Chandra Orbits* 

                                                  for IR AO


13850      180 ks       06-Feb to 13-Feb            None

13854       40 ks       26-Mar to 02-Apr            None

13855       40 ks                                  

13847      180 ks       30-Apr to 07-May            1760

13856       40 ks                                  

13857       40 ks                                  

13849      180 ks       07-May to 14-May            None

13848      180 ks                                  

13846      180 ks       14-May to 21-May            1764-1766

13845      180 ks                                  

14460       24 ks       09-Jul to 16-Jul            1787

13844       20 ks                                  

14461       76 ks                                  

14462       32 ks                                  

13853      160 ks                                  

13841      180 ks       16-Jul to 23-Jul            1788-1790

13842      180 ks                                  

13839      180 ks       23-Jul to 30-Jul            1791

13840      180 ks                                  

13838      180 ks       30-Jul to 06-Aug            None

13852      160 ks                                  

13851      180 ks       15-Oct to 22-Oct            1822

13843      180 ks       22-Oct to 29-Oct            None


*Our preference - the actual Chandra orbits for the observations may differ.  Again, always check the short term schedules to find the specific times of the Chandra observations.

Simulated 3 Msec, 0th Order Image