Search Publications

From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources
DOI: 10.1088/1538-3873/ad357c Bibcode: 2024PASP..136e4201R

Rodriguez, Antonio C.

Galactic X-ray sources are diverse, ranging from active M dwarfs to compact object binaries, and everything in between. The X-ray landscape of today is rich, with point source catalogs such as those from XMM-Newton, Chandra, and Swift, each with ≳105 sources and growing. Furthermore, X-ray astronomy is on the verge of being transformed …

2024 Publications of the Astronomical Society of the Pacific
Gaia XMM-Newton 7
A Serendipitous Observation of the Recently Discovered Cataclysmic Variable TUVO-21acq
DOI: 10.1088/1538-3873/ad4592 Bibcode: 2024PASP..136e4203V

Kuntz, K. D.; Pfeifle, Ryan W.; Weaver, Kimberly A. +2 more

The recently discovered non-magnetic cataclysmic variable TUVO-21acq was serendipitously observed in a quiescent state during an XMM-Newton observing campaign for the starburst galaxy NGC 4945. Data from this campaign was combined with archival serendipitous XMM observations to examine its X-ray and UV/optical characteristics. TUVO-21acq was found…

2024 Publications of the Astronomical Society of the Pacific
XMM-Newton 0
A Diamond Ring in X-Ray: Investigating the Diffuse Emission of Supernova Remnant G28.8+1.5
DOI: 10.1088/1538-3873/ad6105 Bibcode: 2024PASP..136g4301Z

Zhang, Kaiyue

Supernova remnants are products of supernova explosions, which are usually observed in the X-ray band. However, the diffuse emission from the galactic supernova remnant G28.8+1.5 has been overlooked following initial searches for pulsars and pulsar wind nebulae. This paper presents background-subtracted imaging and spatial-resolved spectral analys…

2024 Publications of the Astronomical Society of the Pacific
XMM-Newton 0
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
An Optical and X-Ray Study of the Contact Binary, BH Cassiopeia
DOI: 10.1088/1538-3873/ab247a Bibcode: 2019PASP..131h4202L

Zheng, Jie; Zhang, Yu; Esamdin, Ali +10 more

We present the revised and high-quality CCD time series observations in 2017 and 2018 of the W UMa-type contact binary BH Cas. The combination of our new determinations of minimum times and those collected from the literatures reveal a long-term period increase with a rate of dP/dt = +3.27 × 10-7 day yr-1, which can be accoun…

2019 Publications of the Astronomical Society of the Pacific
XMM-Newton 14
catsHTM: A Tool for Fast Accessing and Cross-matching Large Astronomical Catalogs
DOI: 10.1088/1538-3873/aac410 Bibcode: 2018PASP..130g5002S

Soumagnac, Maayane T.; Ofek, Eran O.

Fast access to large catalogs is required for some astronomical applications. Here we introduce the catsHTM tool, consisting of several large catalogs reformatted into HDF5-based file format, which can be downloaded and used locally. To allow fast access, the catalogs are partitioned into hierarchical triangular meshes and stored in HDF5 files. Se…

2018 Publications of the Astronomical Society of the Pacific
Gaia XMM-Newton 49
Visualization of Multi-mission Astronomical Data with ESASky
DOI: 10.1088/1538-3873/129/972/028001 Bibcode: 2017PASP..129b8001B

de Marchi, Guido; Merín, Bruno; O'Mullane, William +17 more

ESASky is a science-driven discovery portal to explore the multi-wavelength sky and visualize and access multiple astronomical archive holdings. The tool is a web application that requires no prior knowledge of any of the missions involved and gives users world-wide simplified access to the highest-level science data products from multiple astrono…

2017 Publications of the Astronomical Society of the Pacific
INTEGRAL XMM-Newton 20