Search Publications

Resurrecting Hitomi for Decaying Dark Matter and Forecasting Leading Sensitivity for XRISM
DOI: 10.1103/PhysRevLett.132.211002 Bibcode: 2024PhRvL.132u1002D

Safdi, Benjamin R.; Dessert, Christopher; Rodd, Nicholas L. +1 more

The Hitomi x-ray satellite mission carried unique high-resolution spectrometers that were set to revolutionize the search for sterile neutrino dark matter (DM) by looking for narrow x-ray lines arising from DM decays. Unfortunately, the satellite was lost shortly after launch, and to date the only analysis using Hitomi for DM decay used data taken…

2024 Physical Review Letters
Hitomi XMM-Newton 13
Hitomi HXT deconvolution imaging of the Crab Nebula dazzled by the Crab pulsar
DOI: 10.1093/pasj/psae008 Bibcode: 2024PASJ...76..272M

Maeda, Yoshitomo; Ishida, Manabu; Awaki, Hisamitsu +3 more

We develop a new deconvolution method to recover the precise Crab Nebula image taken by the Hitomi HXT, suppressing the artifact due to the bright Crab pulsar. We extend the Richardson-Lucy method, introducing two components corresponding to the nebula and pulsar with regularization for smoothness and flux, respectively, and performing simultaneou…

2024 Publications of the Astronomical Society of Japan
Hitomi 3
Investigating the Impact of Atomic Data Uncertainties on the Measured Physical Parameters of the Perseus Galaxy Cluster
DOI: 10.3847/1538-4357/ad17be Bibcode: 2024ApJ...962..192C

Raymond, John; Foster, Adam R.; Smith, Randall +4 more

Accurate atomic data and plasma models are essential for interpreting the upcoming high-quality spectra from missions like XRISM and Athena. Estimating physical quantities, like temperature, abundance, turbulence, and the resonance scattering factor, is highly dependent on the underlying atomic data. We use the AtomDB tool variableapec to estimate…

2024 The Astrophysical Journal
Hitomi 0
Dark matter search in the Perseus cluster with simultaneous analysis of Hitomi and Suzaku data
DOI: 10.1093/pasj/psae027 Bibcode: 2024PASJ...76..512F

Kitamoto, Shunji; Sawada, Makoto; Tamura, Takayuki +1 more

The reported detection of a 3.5 keV emission line in the Perseus cluster, possibly originating from dark matter decay, is still under scrutiny. Despite extensive observations, the detection has not yet been confirmed, and its origin remains a topic of active debate. Most of the previous searches relied on spectroscopy with X-ray charge-coupled dev…

2024 Publications of the Astronomical Society of Japan
Hitomi Suzaku 0