S. Hattori
New York University Abu Dhabi
5 Papers
11 Citations
S. Hattori is an academic researcher from New York University Abu Dhabi. The author has contributed to research in topics: Pulsar & Supernova. The author has an hindex of 2, co-authored 3 publications.
Chat about Author
Papers
Bridging the Gap—The Disappearance of the Intermediate Period Gap for Fully Convective Stars, Uncovered by New ZTF Rotation Periods
TL;DR: In this article , the authors present a period catalog containing 40,553 rotation periods (9535 periods > 10 days), measured using the Zwicky Transient Facility (ZTF).
23
The Nonstandard Properties of a "Standard" PWN: Unveiling the Mysteries of PWN G21.5-0.9 Using Its IR and X-Ray Emission
TL;DR: In this article, the evolution of a pulsar wind nebula (PWN) depends on properties of the progenitor star, supernova, and surrounding environment, and reproducing the observed dynamical properties and spectral energy distribution with an evolutionary model is often the best approach in estimating their values.
9
TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars
Samuel K. Grunblatt,Nicholas Saunders,Ashley Chontos,S. Hattori,Dimitri Veras,Daniel Huber,Ruth Angus,Malena Rice,Katelyn Breivik,Sarah Blunt,Steven Giacalone,Jack Lubin,Howard Isaacson,Andrew W. Howard,David R. Ciardi,Boris Safonov,I. Strakhov,David W. Latham,Allyson Bieryla,George R. Ricker,Jon M. Jenkins,Peter Tenenbaum,A. Shporer,Edward H. Morgan,Veselin B. Kostov,Hugh P. Osborn,Diana Dragomir,Sara Seager,Roland Vanderspek,Joshua N. Winn +29 more
TL;DR: In this article , the authors present the discovery of TOI-4582 b, a 0.05 M J planet orbiting an intermediate-mass subgiant star every 31.034 days.
6
MeV emission from pulsar wind nebulae
J. D. Gelfand,S. M. Straal,S. Hattori +2 more
- 01 Jan 2019
TL;DR: In this article, the MeV properties of pulsar wind nebulae (PWNs) have been investigated for understanding how PWNs are able to accelerate e± to PeV energies.
2
The Nonstandard Properties of a "Standard" PWN: Unveiling the Mysteries of PWN G21.5-0.9 Using its IR and X-ray emission
TL;DR: In this article, the evolution of a pulsar wind nebula (PWN) depends on properties of the progenitor star, supernova, and surrounding environment, and reproducing the observed dynamical properties and spectral energy distribution with an evolutionary model is often the best approach in estimating their values.