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events section


Meet IXO scientists at Explore@NASA Goddard on Saturday, May 14, 11am – 5pm rain or shine.


IXO Science Team Meeting, March 14—16, 2011, Rome, Italy »


IXO will take part in the AAS # 217 meeting held on January 9—13, 2011 in Seattle, WA. Please come by to see us at our booth # 218.


The IXO team will make an initial presentation on October 6th to the ESA Cosmic Vision review


Several members of the IXO Team will be giving presentations at the SPIE meeting in San Diego this week, June 28 – July 2, 2010


The First Galaxies, Quasars & Gamma-Ray Bursts, Pennsylvania State University. Niel Brandt will give a talk about IXO.

Read more »


IXO Science Team Meeting, Paris, France

Meeting page »


HEAD 2010

The 11th HEAD meeting will be held on Kailua-Kona coast of Big Island, Hawaii»


215 AAS meeting, Washington, DC

Meeting program and schedule »

09.07—09.11 2009

X-ray astronomy 2009: Present status, multi-wavelength approach and future perspectives, Bologna, Italy

Nicholas E. White´s talk about IXO, [.pdf]


AIAA SPACE 2009 Conference & Exposition

Ann Hornschemeier´s talk about IXO is available for download.


Presentations for the IXO Science Team Meeting held on July 3rd, 2009, in Otaru, Japan available for download


214th Meeting of the American Astronomical Society (AAS)

Sunday, 7 June 2009–Thursday, 11 June 2009, Pasadena, CA. The IXO Team is giving a requested presentation to the Astro2010 Program Prioritization Panel.


Astro2010 March meeting agenda

is available for download

More »

+ Image credits

The International X-ray Observatory (IXO) combines a large X-ray mirror with powerful new instrumentation that will explore the high energy Universe.

An Update on IXO

From Nick White and Jay Bookbinder

April 8, 2011

US IXO Team,

This is an update on the discussions with the European Space Agency (ESA) at the recent ESA-NASA bilateral meeting. This was reported by Jon Morse (HQ Astrophysics Division Director), first, to the IXO and LISA teams on Tuesday, and then, at the Astrophysics NASA Advisory Committee (NAC) sub-committee meeting on Thursday afternoon.

IXO was one of three candidates competing for the L1 opportunity in ESA´s Cosmic Vision Program (2015-2025). The Astrophysics and Planetary decadal rankings and NASA´s constrained out-year resources projected in the President's FY12 budget request led ESA to conclude that none of the three mission concepts were feasible within the Cosmic Vision L1 schedule. Consequently, ESA has ended consideration of IXO and the other concepts as partnerships at the scale proposed in the New Worlds New Horizons decadal survey (NWNH) and EJSM/Laplace in Visions and Voyages for Planetary Science.

Instead, ESA has begun a rapid definition effort that includes the formation of a new science team (to be announced shortly). That effort will identify science goals and a mission concept that can be implemented as part of an ESA-led mission launching in the early 2020´s for a cost to ESA of about 800M Euro. Revised mission concepts from the three science areas will be considered in a selection process tentatively foreseen in February 2012.

A future minor role for NASA in the new ESA-led X-ray mission, in particular contributions at the instrument level, has not been ruled out. NASA will participate in the new ESA science team through a "NASA HQ-empowered scientist." This will be a NASA civil servant scientist who will be the conduit for any engagement with the new ESA team.

Currently the decadal survey recommendations are centered on the IXO (and LISA) concept and partnerships. NASA HQ will NOT disband the current NASA IXO (and LISA) teams immediately, but will follow a deliberate path towards redirecting the NASA efforts in the context of the decadal survey recommendations. Read more »

Former IXO concept and science performance requirements

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IXO Science Team Meeting, March 14—16, 2011, Rome, Italy


IXO Astro2010 Decadal submissions available here.

Recent Technology Milestones

The XPOL team is continuing to investigate how different gas mixtures impact on the sensitivity of the X-ray polarimeter on-board of IXO. Read more »


Spectrum of monochromatic photons at 2.6, 5.2 and 7.8 keV. The energy resolution is 32.1% at 2.6 keV, 24.5% at 5.2 keV and 23.5% at 7.8 keV (Muleri et al., 2010). Read more »

Recent Publications

Delphine Porquet, Jacques Dubau, Nicolas Grosso, "He-like ions as practical astrophysical plasma diagnostics: From stellar coronae to active galactic nuclei." More publications »