Opportunity Information: Apply for PD 18 5115

The National Science Foundation (NSF) grant opportunity "Windows on the Universe: The Era of Multi-Messenger Astrophysics" (WoU-MMA; Funding Opportunity Number PD 18-5115) is designed to accelerate a new style of astronomy where researchers study the same cosmic events using multiple kinds of signals, or "messengers." Instead of relying on only light (electromagnetic radiation), this program emphasizes the combined use of three complementary windows on the universe: electromagnetic waves across the spectrum (radio through gamma rays), high-energy particles (especially neutrinos and cosmic rays), and gravitational waves. The basic premise is that each messenger reveals different physics, and that coordinated, interoperable observing and analysis across these channels can unlock discoveries that would be difficult or impossible using any single messenger alone. WoU-MMA is the NSF implementation of its broader "Windows on the Universe" Big Idea, and it aims to build shared capability and tighter integration across communities that have historically operated somewhat separately (astronomy, particle astrophysics, gravitational-wave science, theory and computation, and supporting cyberinfrastructure).

At its core, the program invites proposals that meaningfully advance multi-messenger astrophysics by addressing at least one of three qualifying tracks. The first is Coordination, which covers the hardware, software, and other infrastructure needed to coordinate observations involving more than one messenger. This can include systems for event alerts, scheduling and follow-up networks, data pipelines that link observatories, interoperable standards, and tools that help different facilities respond rapidly and consistently to transient events. The second is Observations, which supports observational campaigns or projects targeting objects and phenomena that can produce more than one messenger, such as neutron star mergers, core-collapse supernovae, active galactic nuclei, tidal disruption events, or other transients and energetic sources. Observations can involve using existing observatories and experiments, working with data archives, or developing and constructing new capabilities that specifically push multi-messenger astronomy forward (for example, improved sensitivity, wider sky coverage, better timing, or better event localization). The third is Interpretation, which supports theory, simulations, and related efforts that help explain and extract physics from multi-messenger datasets, including modeling source populations, emission mechanisms, particle acceleration, gravitational-wave signatures, and the coupling between what is seen in light, particles, and spacetime signals.

WoU-MMA also lays out three broader investment themes that describe what NSF is trying to build over time. One major focus is enhancing and accelerating theory, computation, and observational activity across the community. This includes efforts that strengthen observational and analysis capabilities within each messenger domain while also building the "glue" that makes them work together: shared methods, interoperable tools, cross-disciplinary collaboration, and a workforce trained to operate in this integrated paradigm. Within this theme, NSF emphasizes expansion of ongoing activities and notes a priority for PI-led and small-group awards that directly advance multi-messenger goals and speed progress. Another investment theme is building dedicated midscale experiments and instrumentation in the midscale project range, aimed at making critical contributions to the multi-messenger infrastructure. These projects might enable new energy coverage, improved sensitivity, broader sky coverage, or new computational capabilities that change what can be detected and how quickly and reliably signals can be connected across messengers. The third theme is exploiting current facilities and developing next-generation observatories, including modest upgrades and infrastructure improvements that allow the current suite of facilities to be used to their full potential for multi-messenger work, as well as planning and development activities that position the field for significantly greater capabilities in the future.

Administratively, WoU-MMA is structured as a cross-cutting initiative rather than a standalone replacement for existing NSF programs. Proposals are generally submitted to the relevant existing NSF program area depending on the scientific and technical emphasis, but flagged for WoU-MMA consideration when they have a substantial multi-messenger component. The solicitation explicitly states that WoU-MMA is not intended to replace the standard programs that fund electromagnetic astronomy, particle astrophysics, gravitational physics, or theory on their own; instead, it is meant to support work that genuinely integrates multiple messengers or builds the coordination and interpretive capability needed for integrated studies. If a proposal does not actually meet at least one of the three WoU-MMA criteria (coordination, observations of multi-messenger sources, or interpretation of multi-messenger sources), it will be reviewed within the normal context of the individual program rather than within WoU-MMA.

In terms of where proposals can land, the opportunity spans NSF’s participating divisions and program lines, including Astronomy (AST), Physics (PHY), and the Office of Polar Programs (OPP) where relevant. Examples of referenced programs include Astronomy and Astrophysics Postdoctoral Fellowships (AAPF), Astronomy and Astrophysics Research Grants (AAG), and Advanced Technologies and Instrumentation (ATI) within AST, along with multiple PHY programs such as Nuclear Physics (theory and experiment), Particle Astrophysics (experiment), Particle Astrophysics and Cosmology (theory), Gravitational Physics (theory), LIGO Research Support, and Plasma Physics. Midscale projects that are primarily electromagnetic and within AST are directed to the Mid-Scale Innovations Program (MSIP), while midscale projects primarily focused on high-energy particles or gravitational waves are directed to relevant PHY programs. Projects that involve facilities in Antarctica must list OPP’s Antarctic Astrophysics and Geospace Sciences (AAGS) program as a secondary program, reflecting the logistical and oversight requirements for polar research infrastructure.

The eligibility is broad (listed as unrestricted, subject to any clarifications in the solicitation), the funding instrument is a grant, and the activity category is science and technology research and development. The source data lists CFDA numbers 47.049 and 47.050, an expected number of awards of around 200, and no specific award ceiling (shown as 0, which typically indicates that budgets depend on the underlying program and project scope rather than a single cap across the entire WoU-MMA umbrella). For proposals seeking WoU-MMA consideration, NSF requires that the proposal title begin with the acronym "WoU-MMA," and it also notes that supplement requests to existing awards may be considered if they address the WoU-MMA goals. Overall, the opportunity is best understood as NSF’s mechanism for funding the connective tissue of modern astrophysics: the coordinated observing, shared infrastructure, and integrated modeling that turn separate detections in light, particles, and gravitational waves into a unified physical story about the most extreme events in the universe.

  • The National Science Foundation in the science and technology and other research and development sector is offering a public funding opportunity titled "WINDOWS ON THE UNIVERSE: THE ERA OF MULTI-MESSENGER ASTROPHYSICS" and is now available to receive applicants.
  • Interested and eligible applicants and submit their applications by referencing the CFDA number(s): 47.049, 47.050.
  • This funding opportunity was created on Aug 01, 2018.
  • Applicants must submit their applications by Dec 11, 2018 Nuclear Physics - Theory and Experiment Particle Astrophysics - Experiment Particle Astrophysics and Cosmology - Theory Gravitational Physics - Theory LIGO Research Support Plasma Physics Astronomy and Astrophysics Postdoctoral Fellowships Astronomy and Astrophysics Research Grants Advanced Technologies and Instrumentation. (Agency may still review applications by suitable applicants for the remaining/unused allocated funding in 2026.)
  • The number of recipients for this funding is limited to 200 candidate(s).
  • Eligible applicants include: Unrestricted (i.e., open to any type of entity above), subject to any clarification in text field entitled Additional Information on Eligibility.
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