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ROSES-25 D.3 AGIGO: New Joint program with XMM-Newton added to IXPE GO Cycle 4

27 May 2026

The IXPE (Imaging X-ray Polarimetry Explorer) GO (General Observer) Program solicits proposals for investigations in any area of astrophysics (not constrained to IXPE’s prime science areas). IXPE Cycle 4 observations will commence on or about 1 February 2027, and continue for a nominal period of 12 months. Individuals may submit proposals for observations that will advance the IXPE mission science return. Observing proposals may be for "standard", "Target-of-Opportunity (ToO)", “Large Program (LP)” or “Multi-cycle” observations. For ToO observations, IXPE anticipates executing approximately 1 high (observations begin within 9 days of trigger) and 7 medium (observations begin between 9 days and 4 weeks of trigger) priority triggers in this GO cycle, hence proposers must strongly justify the response time required to meet the scientific objectives.

A new joint observing program with the European Space Agency’s (ESA)/NASA X-ray Multi-Mirror Mission (XMM)-Newton X-ray observatory was added to IXPE GO Cycle 4. New Text is in bold. See Section 9 of D.3 Combined General Investigator General Observer Program. The due date for IXPE Cycle 4 Phase-1 Proposals (submitted via the Astrophysics Research Knowledgebase Remote Proposal System (ARK RPS)) remains 17 September 2026.

Please direct programmatic questions concerning IXPE to Hashima Hasan at hhasan@nasa.gov, and technical questions to Kavitha Arur at kavitha.arur@nasa.gov.

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This cropped horizontal image has layers of semi-opaque rusty red colored gas and dust that starts at the bottom right and goes toward the top left. There are three prominent pillars rising toward the top left. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of brown and have red outlines.