Welcome to the XMM-Newton Science Operations Centre

 

The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.

Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.

Read more about the spacecraft, mirrors and instruments and about the XMM-Newton SOC.

News and Highlights

AO-25 Closed 15-Oct-2025

XMM-Newton Announcement of Opportunity (AO-25) Closed

The Twenty-fifth Announcement of Opportunity (AO-25) for XMM-Newton closed on 10 October 2025.

A total of 463 valid proposals were received for this cycle, which covers a one-year period with 10 Ms of observing time available. In contrast, 85.6 Ms of science time were requested, resulting in an over-subscription factor of 8.6.

This marks a significant increase in over-subscription compared to recent years. The rise is primarily due to reduced available observing time in AO-25, driven by operational constraints such as increased expected radiation levels and the ongoing evolution of the spacecraft’s orbit.

Proposal breakdown:

  • Large Programmes: 45 proposals
  • Fulfil Programmes: 13 proposals
  • Anticipated Target of Opportunity observations: 81 proposals

Joint Programme submissions totalled 114 proposals:

XMM–NuSTAR: 43
XMM–HST: 15
XMM–SWIFT: 19
XMM–VLT: 10
XMM–Chandra: 10
XMM–JWST: 19
XMM–NRAO: 12
XMM–XRISM (new): 9

Proposals were submitted by 375 different Principal Investigators from 42 countries. Including co-investigators, approximately 1,700 individual scientists participated in the response the Twenty-fifth Announcement of Opportunity.

2025-10-nature-newly-faint-ray-transient 13-Oct-2025
Observations inspect the nature of a newly discovered very faint X-ray transient
Using various space telescopes, an international team of astronomers have observed a newly detected very faint X-ray transient designated 4XMM J174610.7–290020. Results of the observational campaign, published October 2 on the arXiv pre-print server, yield new insights into the nature of this transient.
Further details on our Phys.org web portal.

hot-gaseous-outflow 9-Oct-2025
Hot gaseous outflow detected in the galaxy NGC 5746
Using ESA's XMM-Newton satellite, astronomers have conducted deep observations of a massive galaxy known as NGC 5746. As a result, they detected a hot gaseous outflow in the galaxy. The new findings, presented Oct. 1 on the arXiv pre-print server, could shed more light on the nature of NGC 5746.
Further details on our Phys.org web portal.

Erik Kuulkers 16-Sep-2025

Erik Kuulkers appointed as new XMM-Newton Project Scientist

As of 8 September 2025, Erik Kuulkers is leading XMM-Newton as Project Scientist, taking this role over from Norbert Schartel. Since 2013, Erik has been Project or Study Scientist for various missions, including Einstein Probe, Theseus, NewAthena, and, for over 10 years, INTEGRAL. Erik's main research interests are in the realm of transient and explosive X-ray phenomena in the universe. Erik is looking forward to continue writing the success story that is X-ray astronomy with XMM-Newton, allowing scientific discoveries spanning many decades, back from Apollo 15 to the 2030s and beyond.

Further details on our XMM-Newton SOC web portal.

AO-25 Opening 19-Aug-2025

XMM-Newton Announcement of Opportunity (AO-25)

Letter of Invitation by the ESA Director of Science

Dear Colleague,

I am pleased to invite you to respond to the 25th “Announcement of Opportunity" to submit proposals for observations to be performed with the XMM-Newton observatory.

This Announcement solicits proposals to be carried out between May 2026 and April 2027. Proposers from institutes located worldwide are welcome to participate. All proposals will be subject to peer review by the XMM-Newton Observing Time Allocation Committee.

The detailed schedule of milestones of the announcement, the required software tools and the documentation are available from:

     https://www.cosmos.esa.int/web/xmm-newton/ao25

I would appreciate it if you would distribute this invitation to interested colleagues.

I wish you every success in using the XMM-Newton observatory.

Yours sincerely,
Professor Carole Mundell
Director of Science

Key milestones for this announcement

Announcement of Opportunity 19 August 2025
Due date for Proposals 10 October 2025 (12:00 UT)
Final OTAC approved program mid December 2025

 

Timeline for Phase II proposal submission

After the cycle of proposal submission and selection, the observation details for successful proposals must be entered into the observatory system. This is done during "Phase II" proposal submission.

Find below for your information the anticipated timeline for that eventual Phase II:

Start of Phase II proposal submission 13 January 2026
Closure of Phase II proposal submission 6 February 2026

 

Further details on the XMM-Newton SOC web portal.

X-ray Universe Symposium 19-August-2025
The X-ray Universe 2026, Elche, Spain
The seventh meeting in the series "The X-ray Universe" is planned to be held in the Mediterranean city of Elche, Spain, from 8 to 11 June 2026. This conference series is aimed at encompassing a broad range of high-energy astrophysics topics, from solar system studies to cosmology, and at providing a showcase for results and discoveries from XMM-Newton as well as from the variety of other current missions. The scientific potential of future mission projects and the evolution of the scientific analysis landscape will be further topics for discussion.
Further details on our XMM-Newton SOC web portal.

 

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