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TDAMM SIG Seminar

Time Domain and Multi-Messenger Science Interest Group

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 about TDAMM SIG Seminar

Location

Virtual

Dates

12 August 2025

Community

TDAMM SIG

Type

Seminar

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 Time Domain and Multi-Messenger Astrophysics (TDAMM). Swift became involved in TDAMM in the early 2010s, performing follow-up observations of neutrino detections by the IceCube observatory. In addition, Swift has been involved in LIGO follow-up since before the current Advanced LIGO era, with follow-up observations of (fake) triggers detected in 2009-2010. I will demonstrate how the unique approach to Swift Operations and the capabilities of Swift have led to the development of new capabilities that have kept it at the cutting edge of TDAMM observing, despite its advanced age.

Meeting Connection

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2862 452 7732

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.