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Jack M. M. Neustadt

Physics and Astronomy · The Ohio State University

OpenAlex ORCID
Mid career · publishing since 2016Rising activity
Astrophysical Phenomena and ObservationsGamma-ray bursts and supernovaeAstrophysics and Cosmic PhenomenaGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical Research

Publications

49

Citations

714

Est. group size

~2

Recurring co-author estimate

Active years

11

Publishing since 2016

Research summary
AI-generated

Jack M. M. Neustadt works in observational astrophysics, studying active galactic nuclei (supermassive black holes actively pulling in surrounding gas), quasars, supernovae, and supernova remnants (the expanding debris left behind after a star explodes). Much of the recent work involves monitoring how light from these objects changes over time, using ground- and space-based telescopes including JWST, to map the structure and behavior of accretion disks and outflows around black holes.

Active galactic nuclei and quasar variabilityAccretion disk reverberation mappingSupernovae and their progenitor starsSupernova remnants and Galactic distance measurementsTime-domain and multi-wavelength astronomical monitoring

Publication output has generally grown over the last decade, rising from about 2 papers per year in 2017 to a peak of 10 in 2024, though with some year-to-year variation.

Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026

Publication cadence
Publications per year over the last 10 years — averaging 6.0/year recently
2017: 2 publications172018: 3 publications182019: 2 publications192020: 4 publications202021: 6 publications212022: 5 publications222023: 7 publications232024: 10 publications10242025: 3 publications252026: 5 publications26
Recent publications
Publishes in
  • arXiv (Cornell University)×16
  • Monthly Notices of the Royal Astronomical Society×12
  • The Astrophysical Journal×9
  • Repository of the Academy's Library (Library of the Hungarian Academy of Sciences)×1
  • Science Advances×1
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This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.

Last updated Jul 19, 2026.

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