Friday 2 March 2018 9.00am EST
During the last week Chandra completed the observing schedule as planned. A Chandra image release was issued on Mar 1 describing observations of an ultraluminous X-ray (ULX) source in M51. Using data from Chandra, observers discovered an unusual dip in the X-ray spectrum which they attribute to cyclotron resonance scattering due to charged particles circling in a strong magnetic field. This implies that the ULX is a neutron star rather than a black hole and may provide insight into the mechanism by which these sources shine so brightly. For details see: http://chandra.harvard.edu/photo/2018/m51/ The schedule of targets for the next week is shown below and includes an observation of PSR J1622-4950 coordinated with NuSTAR, and an observation of MAXI J1813-095, which was accepted as a Target of Opportunity on Feb 21 and is coordinated with NuSTAR. |
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SDSSJ092023.84+0034 ACIS-S Mar 5
SDSSJ022556.08+0030 ACIS-S
J0224-4711 ACIS-S
Abell1300 ACIS-I Mar 6
SPT-CLJ2355-5259 ACIS-I
MAXIJ1813-095 ACIS-S
Radiation Belts Mar 7
Mrk59 ACIS-S
PSRJ1622-4950 ACIS-S
Abell1300 ACIS-I Mar 8
CentaurusA ACIS-I
SPT-CLJ2328-5533 ACIS-I
PSRJ1622-4950 ACIS-S
Abell1300 ACIS-I
PSS0926+3055 ACIS-S Mar 9
J0300+2654 ACIS-S
VHSJ2227-5203 ACIS-S
Radiation Belts Mar 10
VHSJ2130-4930 ACIS-S
Abell1300 ACIS-I
NGC4242 ACIS-S
NGC3726 ACIS-S
PS12dm ACIS-S
NGC5448 ACIS-S
PS12kn ACIS-S Mar 11
NGC5473 ACIS-S
Mrk59 ACIS-S
Radiation Belts Mar 12------------------------------------------
All spacecraft subsystems continued to support nominal operations.
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