Search Publications

Perfecting Our Set of Spectrophotometric Standard DA White Dwarfs
DOI: 10.3847/1538-4357/ac96f4 Bibcode: 2022ApJ...940...19C

Rest, Armin; Matheson, Thomas; Raddi, Roberto +17 more

We verified for photometric stability a set of DA white dwarfs with Hubble Space Telescope magnitudes from the near-ultraviolet to the near-infrared and ground-based spectroscopy by using time-spaced observations from the Las Cumbres Observatory network of telescopes. The initial list of 38 stars was whittled to 32 final ones, which comprise a hig…

2022 The Astrophysical Journal
Gaia eHST 5
Unbound Close Stellar Encounters in the Solar Neighborhood
DOI: 10.3847/1538-3881/ac3a8b Bibcode: 2022AJ....163...44H

Hansen, Bradley M. S.

We present a catalog of unbound stellar pairs, within 100 pc of the Sun, that are undergoing close, hyperbolic, encounters. The data are drawn from the GAIA EDR3 catalog, and the limiting factors are errors in the radial distance and unknown velocities along the line of sight. Such stellar pairs have been suggested to be possible events associated…

2022 The Astronomical Journal
Gaia 5
Exploring the Fundamental Mechanism in Driving Highest-Velocity Ionized Outflows in Radio AGNs
DOI: 10.3390/universe8110559 Bibcode: 2022Univ....8..559A

Xue, Yongquan; Woo, Jong-Hak; He, Zhicheng +4 more

We investigate the ionized gas kinematics relationship with X-ray, radio and accreting properties using a sample of 348 nearby (z<0.4) SDSS-FIRST-X-ray detected AGNs. X-ray properties of our sample are obtained from XMM-Newton, Swift and Chandra observations. We unveil the ionized gas outflows in our sample manifested by the non-gravitational b…

2022 Universe
XMM-Newton 5
X-Ray and Radio Observations of Central Black Holes in Nearby Low-mass Early-type Galaxies: Preliminary Evidence for Low Eddington Fractions
DOI: 10.3847/1538-4357/ac96e6 Bibcode: 2022ApJ...940..111U

Neumayer, Nadine; Strader, Jay; Seth, Anil C. +5 more

We present new radio and X-ray observations of two nearby (<4 Mpc) low-mass early-type galaxies with dynamically confirmed central black holes: NGC 5102 and NGC 205. NGC 5102 shows a weak nuclear X-ray source and has no core radio emission. However, for the first time we demonstrate that it shows luminous extended radio continuum emission in lo…

2022 The Astrophysical Journal
Gaia eHST 5
Relationship between gamma-ray loudness and X-ray spectra of radio galaxies
DOI: 10.1093/pasj/psac036 Bibcode: 2022PASJ...74..791K

Fukazawa, Yasushi; Kayanoki, Taishu

The Fermi satellite has detected ~ 60 radio galaxies (RGs). In this study, we investigate the difference in the properties of X-ray spectra between GeV-loud RGs and GeV-quiet RGs. Our sample comprises 68 objects: 36 RGs detected with Fermi and 32 RGs not detected with gamma-rays. We analyzed the X-ray spectra of these 68 objects using data from th…

2022 Publications of the Astronomical Society of Japan
XMM-Newton 5
Application of Random Forest Regressions on Stellar Parameters of A-type Stars and Feature Extraction
DOI: 10.1088/1674-4527/ac41c5 Bibcode: 2022RAA....22b5017C

He, Ying; Chen, Shu-Xin; Sun, Wei-Min

Measuring the stellar parameters of A-type stars is more difficult than FGK stars because of the sparse features in their spectra and the degeneracy between effective temperature (T eff) and gravity (log g). Modeling the relationship between fundamental stellar parameters and features through machine learning is possible because we can …

2022 Research in Astronomy and Astrophysics
Gaia 5
VVVX Near-IR Photometry for 99 Low-mass Stars in the Gaia EDR3 Catalog of Nearby Stars
DOI: 10.1051/0004-6361/202141759 Bibcode: 2022A&A...660A.131M

Minniti, D.; Solano, E.; Saito, R. K. +3 more

Context. Red dwarf stars, which represent 75% of stars in the Milky Way, can be studied in great detail in the solar neighborhood, where the sample is more complete.
Aims: We intend to better characterize red-dwarf candidates selected from the Gαìα Catalog of Nearby Stars using optical and near-infrared multi-filter photometry from the Vista …

2022 Astronomy and Astrophysics
Gaia 5
Temperature Discrepancy with Photoionization Models of the Narrow-Line Region
DOI: 10.22201/ia.01851101p.2022.58.01.11 Bibcode: 2022RMxAA..58..133B

Binette, L.; Villar Martín, M.; Magris C., G. +4 more

Using published work on the narrow-line region of Active Galactic Nuclei, a comparison is carried out among the [OIII] λ4363Å/5007Å ratios (ROIII) observed in quasars, Seyfert 2's and the spatially resolved ENLR plasma. Using the weak [ArIV] λ4711Å/λ4740Å doublet observed by Koski (1978) among Seyfert 2's, we find …

2022 Revista Mexicana de Astronomia y Astrofisica
eHST 5
The XXL Survey - XLVIII. X-ray follow-up of distant XXL clusters: masses, scaling relations, and AGN contamination
DOI: 10.1093/mnras/stac617 Bibcode: 2022MNRAS.512.2525D

Valtchanov, I.; Pierre, M.; Gastaldello, F. +11 more

We use deep follow-up XMM-Newton observations of six clusters discovered in the XXL Survey at z > 1 to gain robust measurements of their X-ray properties and to investigate the extent to which scaling relations at low redshift are valid at z > 1. This sample is unique as it has been investigated for active galactic nucleus (AGN) contaminatio…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
The relation between X-ray and ultraviolet variability of quasars
DOI: 10.1093/mnras/stac738 Bibcode: 2022MNRAS.512.5511S

Xie, Zhang-Liang; Cai, Zhen-Yi; Wang, Jun-Xian +2 more

The relation between X-ray and UV/optical variability in AGNs has been explored in many individual sources, however a large sample study is yet absent. Through matching the XMM-Newton serendipitous X-ray and UV source catalogs with SDSS quasars, we build a sample of 802 epoch-pairs of 525 quasars showing clear variability in logFX - log…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5