Massimo Moscetti
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View article: Stripe 82-XL: The ∼54.8 deg<sup>2</sup> and ∼18.8 Ms Chandra and XMM-Newton Point-source Catalog and Number of Counts
Stripe 82-XL: The ∼54.8 deg<sup>2</sup> and ∼18.8 Ms Chandra and XMM-Newton Point-source Catalog and Number of Counts Open
We present an enhanced version of the publicly available Stripe 82X catalog (S82-XL), featuring a comprehensive set of 22,737 unique X-ray point sources identified with a significance ≳4 σ . This catalog is four times larger than the origi…
View article: Stripe 82-XL: the $\sim$54.8 deg$^2$ and $\sim$18.8 Ms Chandra and XMM-Newton point source catalog and number of counts
Stripe 82-XL: the $\sim$54.8 deg$^2$ and $\sim$18.8 Ms Chandra and XMM-Newton point source catalog and number of counts Open
We present an enhanced version of the publicly-available Stripe 82X catalog (S82-XL), featuring a comprehensive set of 22,737 unique X-ray point sources identified with a significance $\gtrsim 4σ$. This catalog is four times larger than th…
View article: Constraining Sterile Neutrino Dark Matter in the Milky Way Halo with Swift-XRT
Constraining Sterile Neutrino Dark Matter in the Milky Way Halo with Swift-XRT Open
We present a search for sterile neutrino dark matter decay signals in the Milky Way’s dark matter halo by considering the entirety of the Swift X-ray Telescope (Swift-XRT) data archive. After filtering the raw archive, we analyze a ∼77 Ms …
View article: Constraining Sterile Neutrino Dark Matter in the Milky Way Halo with Swift-XRT
Constraining Sterile Neutrino Dark Matter in the Milky Way Halo with Swift-XRT Open
We present a search for sterile neutrino dark matter decay signals in the Milky Way's dark matter halo by considering the entirety of the Swift-XRT data archive. After filtering the raw archive, we analyze a $\sim$77 Ms data set containing…
View article: Probing the Milky Way’s Dark Matter Halo for the 3.5 keV Line
Probing the Milky Way’s Dark Matter Halo for the 3.5 keV Line Open
We present a comprehensive search for the 3.5 keV line using ∼51 Ms of archival Chandra observations peering through the Milky Way’s dark matter halo from across the entirety of the sky, gathered via the Chandra Source Catalog Release 2.0.…