Search Publications

Elemental Abundances in the Diffuse Interstellar Medium from Joint Far-ultraviolet and X-Ray Spectroscopy: Iron, Oxygen, Carbon, and Sulfur
DOI: 10.3847/1538-3881/ad306b Bibcode: 2024AJ....167..217P

Costantini, E.; Mehdipour, M.; García, J. A. +10 more

In this study, we investigate interstellar absorption lines along the line of sight toward the galactic low-mass X-ray binary Cygnus X-2. We combine absorption line data obtained from high-resolution X-ray spectra collected with the Chandra and XMM-Newton satellites, along with far-UV absorption lines observed by the Hubble Space Telescope's (HST)…

2024 The Astronomical Journal
XMM-Newton eHST 4
Firmamento: A Multimessenger Astronomy Tool for Citizen and Professional Scientists
DOI: 10.3847/1538-3881/ad216a Bibcode: 2024AJ....167..116T

Giommi, Paolo; Doro, Michele; Pollock, A. M. T. +12 more

Firmamento (https://firmamento.hosting.nyu.edu) is a new-concept, web-based, and mobile-friendly data analysis tool dedicated to multifrequency/multimessenger emitters, as exemplified by blazars. Although initially intended to support a citizen researcher project at New York University–Abu Dhabi, Firmamento has evolved to be a valuable tool for pr…

2024 The Astronomical Journal
XMM-Newton 4
Fast and Robust Noise Background Modeling and Quasiperiodic Oscillation Detection for Astronomical Time Series
DOI: 10.3847/1538-3881/ad7d81 Bibcode: 2024AJ....168..213X

Xu, Chang

Spectrum with confidence levels is a commonly used method for quasiperiodic oscillation (QPO) detection, but it is prone to yield false positives for two reasons: poor choice and/or biased modeling of the null hypothesis (or noise background). Motivated by this, we propose a new time-domain maximum-likelihood estimation method, which can quickly a…

2024 The Astronomical Journal
XMM-Newton 2
Extinction of Taurus, Orion, Perseus and California Molecular Clouds Based on the LAMOST, 2MASS, and Gaia Surveys. II. The Extinction Law
DOI: 10.3847/1538-3881/ad813e Bibcode: 2024AJ....168..256C

Wang, Shu; Jiang, Biwei; Li, Jun +1 more

The extinction law from ultraviolet (UV) to infrared (IR; 0.2–24 µm) is determined by relying on the blue-edge method and color-excess ratios for some nearby molecular clouds, from the low-mass star-forming region to the massive star-forming region. The observational data are collected from nine photometric surveys, along with stellar parame…

2024 The Astronomical Journal
Gaia XMM-Newton 1
Demography of Stellar Radio Population within 500 pc: A VLASS-Gaia DR3 Study
DOI: 10.3847/1538-3881/ad84e7 Bibcode: 2024AJ....168..288A

Narang, Mayank; Tyagi, H.; Shridharan, B. +5 more

In this work, we have carried out a systematic analysis of the Very Large Array Sky Survey (VLASS) quick look catalogs together with Gaia DR3 to identify the optical counterparts of 3 GHz radio emitters within 500 pc to obtain a homogeneous statistical sample of stellar radio sources. We have identified distinct populations of 3 GHz emitters acros…

2024 The Astronomical Journal
Gaia XMM-Newton 1
Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes
DOI: 10.3847/1538-3881/ad6d60 Bibcode: 2024AJ....168..177C

Cilley, Raven; King, George W.; Corrales, Lía

Detecting exoplanet transits at X-ray wavelengths would provide a window into the effects of high-energy irradiation on the upper atmospheres of planets. However, stars are relatively dim in the X-ray, making exoplanet transit detections difficult with current X-ray telescopes. To date, only one exoplanet (HD 189733 b) has an X-ray transit detecti…

2024 The Astronomical Journal
Gaia XMM-Newton 1
A Phenomenon Resembling Early Superhumps in a New SU UMa-type Dwarf Nova with a 2 hr Orbital Period
DOI: 10.3847/1538-3881/acf718 Bibcode: 2024AJ....167...71B

Garnavich, Peter; Littlefield, Colin; Szkody, Paula +4 more

We investigate K2BS5, an optical transient that we identified in Campaign 13 of the Kepler/K2 archives by the K2 Background Survey, and classify it as a new SU UMa-type dwarf nova. Using the light curve generated from Keplers long-cadence observation mode, we analyze the dwarf nova during quiescence and superoutburst. Following 20 days of quiescen…

2024 The Astronomical Journal
Gaia XMM-Newton 1
Joint Deconvolution of Astronomical Images in the Presence of Poisson Noise
DOI: 10.3847/1538-3881/ad6b98 Bibcode: 2024AJ....168..182D

van Dyk, David A.; Kashyap, Vinay L.; Siemiginowska, Aneta +2 more

We present a new framework for joint likelihood deconvolution (Jolideco) of a set of astronomical observations of the same sky region in the presence of Poisson noise. The observations may be obtained from different instruments with different resolution, and different point-spread functions (PSFs). Jolideco reconstructs a single flux image by opti…

2024 The Astronomical Journal
XMM-Newton 0
Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE
DOI: 10.3847/1538-3881/ad781c Bibcode: 2024AJ....168..210M

Zhang, Jingyi; Zhang, Yanxia; Kang, Zihan +3 more

Classifying and summarizing large data sets from different sky survey projects is essential for various subsequent scientific research. By combining data from 4XMM-DR13, Sloan Digital Sky Survey (SDSS) DR18, and CatWISE, we formed an XMM-WISE-SDSS sample that included information in the X-ray, optical, and infrared bands. By cross matching this sa…

2024 The Astronomical Journal
XMM-Newton 0