The X-ray Multi-mirror Mission (XMM-Newton) is the second cornerstone of ESA's Horizon 2000 Science Programme, providing an observatory-class X-ray facility. XMM-Newton was launched by an Ariane 5 on 10 December 1999 and has an expected lifetime of at least 18 years. The observatory provides simultaneous non-dispersive spectroscopic imaging and timing (European Photon Imaging Camera; EPIC), medium resolution dispersive spectroscopy (Reflection Grating Spectrometer; RGS) and optical/UV imaging, spectroscopy and timing from a co-aligned telescope (Optical Monitor; OM).
In combination the three cameras of EPIC offer a large effective
area over the energy range from 300 eV to 12 keV, up to
2500 cm
at 1.5 keV and
1800 cm
at 5 keV.
Each of the two modules of the RGS cover the energy range from
0.4 keV
to 2.2 keV with an effective area of up to 60 cm
at 15 Å.
Thus, XMM-Newton offers a unique opportunity for a wide
variety of sensitive X-ray observations accompanied by simultaneous
optical/UV measurements.
The majority of XMM-Newton's observing time is made available
to the astronomical community by the traditional route of
Announcements of Opportunity (AO), followed by peer review.
These Announcements are open to the worldwide scientific community
and the observing time they offer is referred to as ``Open Time''.
This eighth Announcement, AO-8, solicits proposals for observations
to be carried out in the period between (approximately)
May 2009 and April 2010.
Electronic submission of proposals will be required in response to
this Announcement.
For all matters relating to the proposal the Principal
Investigator (PI) is the single point of contact for ESA.
After peer review by the XMM-Newton Observing Time Allocation
Committee (OTAC), every PI will be
informed about OTAC's decision.
The following schedule has been established:
| Announcement of Opportunity | 26 August 2008 |
| Due date for proposals | 10 October 2008 (12:00 UT) |
| Final OTAC approved programme | late December 2008 |
| Definition of observation details | 12 January to 30 January 2009 |
As soon as the technical details of successful proposals
are confirmed, the
observations will be made available for scheduling.
Thus, execution of observations resulting from the
Announcement of Opportunity could start four to five months
after OTAC's decision, or in individual cases a few weeks to months
earlier, depending on the visibility of a target and on the science aimed.