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Time Domain and Multi-Messenger Astrophysics

The Astro2020 Decadal Survey recommended an investment in Time Domain and Multi-Messenger Astrophysics (TDAMM) as the top-priority sustaining activity in space for the coming decade. TDAMM SIG is open to the scientific community.

About TDAMM SIG

Covering a Wide Range of Time-Varying and Multi-Messenger Phenomena

This relatively new field burst onto the scene with the detection of neutrinos and photons from SN 1987A, and entered a new era in 2017, with the first detection of a binary neutron star merger, GW 170817 / GRB 170817A, in both gravitational waves and across the electromagnetic spectrum, and the second strong association between an astrophysical neutrino, IceCube-170922A, and a known source, the blazar TXS 0506+056. 

The field’s potential continues to grow as searches for electromagnetic counterparts to GW events continue and with the high-significance detection of neutrino emission from the galaxy NGC 1068.

This image depicts a gamma-ray burst caused by the merger of two neutron stars.
This image depicts phenomena observed over the course of nine days following the neutron star merger known as GW170817, detected on Aug. 17, 2017. They include gravitational waves (pale arcs), a near-light-speed jet that produced gamma rays (magenta), expanding debris from a kilonova that produced ultraviolet (violet), optical and infrared (blue-white to red) emission, and, once the jet directed toward us expanded into our view from Earth, X-rays (blue)..
Credit: NASA Goddard Space Flight Center/CI Lab

TDAMM observations cover a wide range of time-varying and multi-messenger phenomena that, expanding on the examples mentioned above, include characterization of exoplanet host stars, variable stars, fast radio bursts, and the regions closely surrounding supermassive black holes, to mention just a few.

TDAMM SIG Tasks

Tasks for the TDAMM SIG may include any of the following:

  1. Provide analysis and feedback to NASA on the impact of the Astronomy & Astrophysics Decadal Survey on the subfield.
  2. Identify and articulate “science gaps”: gaps between the current state of knowledge in the subfield and the goals outlined by the Decadal Survey that require new data in order to fully define new missions (precursor gaps), prepare for approved missions that are in development (preparatory gaps), and maximize the science return from current missions (follow-up gaps).
  3. Serve as ambassadors to facilitate communications between NASA and the science community. In particular, act as the interface to relevant TDAMM communities outside NASA’s immediate sphere, e.g., ground-based observers, physics facilities.
  4. Engage in scientific discussions and exchange of ideas through meetings and seminars to make best use of NASA assets for current research and to assist NASA in strategic planning in TDAMM activities.
  5. Propose and organize TDAMM sessions at conferences and arrange other public meetings as appropriate.
  6. Establish and disseminate best practices for conducting TDAMM science, for missions both in development and in operations, and for observers and investigators, including in regards to sharing and citing data in an era of open data.

TDAMM SIG Chairs

NameInstitution
Rebekah HounsellUMBC / GSFC
Brad CenkoNASA / GSFC
Brian GrefenstetteCaltech
Christos PanagiotouMIT

News & Events

Fourth TDAMM Workshop

Advancing Community Observing Plans for Rapid Follow-Up of Explosive Transients We are pleased to announce the 4th TDAMM Workshop to be held October 27-30, 2025 in Huntsville, Alabama. Location: Embassy Suites by Hilton For more information, including registration and connection information: https://sti.usra.edu/4th-tdamm/

Sep 30, 2025
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Time Domain and Multi-Messenger SIG Meeting 15 Sept 2025

Transient Science with Euclid — Early Results and Prospects Speaker Chris Duffy Abstract Euclid is a ESA mission launched in 2023 which began survey operations in 2024 using red visible and near infrared observations to explore dark matter and dark…

Sep 15, 2025
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Time Domain and Multi-Messenger Astrophysics Science Interest Group (TDAMM SIG)

TDAMM observations cover a wide range of time-varying and multi-messenger phenomena that, expanding on the examples mentioned above, include characterization of exoplanet host stars, variable stars, fast radio bursts, and the regions closely surrounding supermassive black holes, to mention just…

Sep 9, 2025
Topic
Time Domain and Multi-Messenger SIG Meeting 12 Aug 2025

Swift and TDAMM: New Tricks for the Old Dog Speaker Prof. Jamie Kennea, Penn State University Abstract In this talk, I will discuss NASA’s Neil Gehrels Swift Observatory, which is now 20 years old. It is an epochal mission for…

Aug 12, 2025
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Time Domain and Multi-Messenger SIG Meeting 21 May 2025

Exploring the Changing Sky with the Vera C. Rubin Observatory LSST Speaker Michael Wood-Vasey Abstract The Vera C. Rubin Observatory is an 8.4-m telescope with a 10 square degree field of view camera that will observe the visible southern sky…

May 21, 2025
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AAS Meeting 245 (Jan 2025)

Physics of the Cosmos and Joint Program Analysis Group activities will be scheduled from 9am to 6pm Eastern on Sunday, 12 January 2025. Sunday, 12 January 2025 Physics of the Cosmos & Physics of the Cosmos Program Analysis Group Sessions Room: Maryland Ballroom…

Jan 12, 2025
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