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The Large Array Survey Telescope-Pipeline. I. Basic Image Reduction and Visit Coaddition
DOI: 10.1088/1538-3873/ad0977 Bibcode: 2023PASP..135l4502O

Fallah Ramazani, V.; Ofek, E. O.; Ben-Ami, S. +18 more

The Large Array Survey Telescope (LAST) is a wide-field telescope designed to explore the variable and transient sky with a high cadence and to be a test-bed for cost-effective telescope design. A LAST node is composed of 48 (32 already deployed), 28 cm f/2.2 telescopes. A single telescope has a 7.4 deg2 field of view and reaches a 5σ l…

2023 Publications of the Astronomical Society of the Pacific
Gaia XMM-Newton 7
Broadband X-Ray Spectral Analysis of the ULX NGC 1313 X-1 Using JeTCAF: Origin of the ULX Bubble
DOI: 10.1088/1538-3873/accf35 Bibcode: 2023PASP..135e4101P

Mondal, Santanu; Palit, Biswaraj

NGC 1313 X-1 is a mysterious ultraluminous X-ray (ULX) source whose X-ray-powering mechanism and bubble-like structure surrounding the source are topics of intense study. Here, we perform an X-ray spectroscopic study of the source using joint XMM-Newton and NuSTAR observations taken during 2012-2017. The combined spectra cover the energy band 0.3-…

2023 Publications of the Astronomical Society of the Pacific
XMM-Newton 4
A Census of Archival X-Ray Spectra for Modeling Tidal Disruption Events
DOI: 10.1088/1538-3873/acb9bc Bibcode: 2023PASP..135c4101G

Wen, Sixiang; Jonker, Peter G.; Stone, Nicholas C. +3 more

Tidal disruption events (TDEs) are highly energetic phenomena that occur when a star is tidally disrupted by the central massive black hole in a galaxy. Fitting the observed X-ray spectra of TDEs with a first-principles, general-relativistic slim-disk model for the emission from the inner accretion disk can constrain the black hole mass M

2023 Publications of the Astronomical Society of the Pacific
XMM-Newton 4
Multiwavelength Analysis of a Nearby Heavily Obscured AGN in NGC 449
DOI: 10.1088/1538-3873/acb294 Bibcode: 2023PASP..135a4102G

Fang, Guanwen; Gu, Qiusheng; Xu, Jun +5 more

We present the multiwavelength analysis of a heavily obscured active galactic nucleus (AGN) in NGC 449. We first constructed a broadband X-ray spectrum using the latest NuSTAR and XMM-Newton data. Its column density (≃1024 cm-2) and photon index (Γ ≃ 2.4) were reliably obtained by analyzing the broadband X-ray spectrum. Howev…

2023 Publications of the Astronomical Society of the Pacific
AKARI XMM-Newton 1