Search Publications

What are the spectroscopic binaries with high-mass functions near the Gaia DR3 main sequence?
DOI: 10.1093/mnras/stac1797 Bibcode: 2022MNRAS.515.1266E

Rix, Hans-Walter; El-Badry, Kareem

The third data release of the Gaia mission includes orbital solutions for >105 single-lined spectroscopic binaries, representing more than an order of magnitude increase in sample size over all previous studies. This data set is a treasure trove for searches for quiescent black hole + normal star binaries. We investigate one populati…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 26
Speckle Interferometry at SOAR in 2021
DOI: 10.3847/1538-3881/ac78e7 Bibcode: 2022AJ....164...58T

Tokovinin, Andrei; Mason, Brian D.; Mendez, Rene A. +1 more

The speckle interferometry program at the the 4.1 m Southern Astrophysical Research Telescope (SOAR), which started in 2008, now has accumulated over 30,300 individual observations of 12,700 distinct targets. Its main goal is to monitor orbital motion of close binaries, including members of high-order hierarchies and low-mass dwarfs in the solar n…

2022 The Astronomical Journal
Gaia Hipparcos 26
Classifying Unidentified X-Ray Sources in the Chandra Source Catalog Using a Multiwavelength Machine-learning Approach
DOI: 10.3847/1538-4357/ac952b Bibcode: 2022ApJ...941..104Y

Kargaltsev, Oleg; Chen, Steven; Yang, Hui +3 more

The rapid increase in serendipitous X-ray source detections requires the development of novel approaches to efficiently explore the nature of X-ray sources. If even a fraction of these sources could be reliably classified, it would enable population studies for various astrophysical source types on a much larger scale than currently possible. Clas…

2022 The Astrophysical Journal
Gaia INTEGRAL XMM-Newton 26
Periodic variable A-F spectral type stars in the northern TESS continuous viewing zone. I. Identification and classification
DOI: 10.1051/0004-6361/202244037 Bibcode: 2022A&A...666A.142S

Mašek, M.; Paunzen, E.; Skarka, M. +11 more

Context. In the time of large space surveys that provide tremendous amounts of precise data, it is highly desirable to have a commonly accepted methodology and system for the classification of variable stars. This is especially important for A-F stars, which can show intrinsic brightness variations due to both rotation and pulsations.
Aims: T…

2022 Astronomy and Astrophysics
Gaia 26
Supermassive Black Hole and Broad-line Region in NGC 5548: Results from Five-season Reverberation Mapping
DOI: 10.3847/1538-4365/ac94d3 Bibcode: 2022ApJS..263...10L

Zhang, Zhi-Xiang; Du, Pu; Hu, Chen +9 more

NGC 5548 is one of the active galactic nuclei (AGNs) selected for our long-term spectroscopic monitoring with the Lijiang 2.4 m telescope, aiming at investigating the origin and evolution of broad-line regions (BLRs), accurately measuring the mass of supermassive black holes (SMBHs), and understanding the structure and evolution of the AGN. We hav…

2022 The Astrophysical Journal Supplement Series
Gaia 26
Hazy Blue Worlds: A Holistic Aerosol Model for Uranus and Neptune, Including Dark Spots
DOI: 10.1029/2022JE007189 Bibcode: 2022JGRE..12707189I

Fletcher, L. N.; Pérez-Hoyos, S.; Wong, M. H. +7 more

We present a reanalysis (using the Minnaert limb-darkening approximation) of visible/near-infrared (0.3-2.5 µm) observations of Uranus and Neptune made by several instruments. We find a common model of the vertical aerosol distribution i.e., consistent with the observed reflectivity spectra of both planets, consisting of: (a) a deep aerosol …

2022 Journal of Geophysical Research (Planets)
eHST 26
The stellar content of the ROSAT all-sky survey
DOI: 10.1051/0004-6361/202142573 Bibcode: 2022A&A...664A.105F

Schmitt, J. H. M. M.; Czesla, S.; Robrade, J. +2 more


Aims: We present and apply a method to identify the stellar content of the ROSAT all-sky survey (RASS).
Methods: We performed a crossmatch between the RASS sources and stellar candidates selected from Gaia Early Data Release 3 (EDR3) and estimated stellar probabilities for every RASS source from the geometric properties of the match and …

2022 Astronomy and Astrophysics
Gaia 26
Homologous Accelerated Electron Beams, a Quasiperiodic Fast-propagating Wave, and a Coronal Mass Ejection Observed in One Fan-spine Jet
DOI: 10.3847/2041-8213/ac4df2 Bibcode: 2022ApJ...926L..39D

Shen, Yuandeng; Zhou, Chengrui; Zhou, Xinping +3 more

Using imaging and radio multi-wavelength observations, we studied the origin of two homologous accelerated electron beams and a quasiperiodic fast-propagating (QFP) wave train associated with a solar jet on 2012 July 14. The jet occurred in a small-scale fan-spine magnetic system embedded in a large-scale pseudostreamer associated with a GOES C1.4…

2022 The Astrophysical Journal
SOHO 26
Two-spacecraft detection of short-period decayless kink oscillations of solar coronal loops
DOI: 10.1093/mnras/stac2545 Bibcode: 2022MNRAS.516.5989Z

Berghmans, David; Nakariakov, Valery M.; Verbeeck, Cis +2 more

Decayless kink oscillations of an ensemble of loops are captured simultaneously by the High Resolution Imager (HRI) of the Extreme Ultraviolet Imager (EUI) and the Atmospheric Imaging Assembly (AIA) from 22:58 UT on 2021 November 5 to 00:27 UT on 2021 November 6. Oscillations are analysed by processing image sequences taken by the two instruments …

2022 Monthly Notices of the Royal Astronomical Society
SolarOrbiter 26
Single-spacecraft techniques for shock parameters estimation: A systematic approach
DOI: 10.3389/fspas.2022.1005672 Bibcode: 2022FrASS...905672T

Vainio, R.; Horbury, T.; Dresing, N. +8 more

Spacecraft missions provide the unique opportunity to study the properties of collisionless shocks utilising in situ measurements. In the past years, several diagnostics have been developed to address key shock parameters using time series of magnetic field (and plasma) data collected by a single spacecraft crossing a shock front. A critical aspec…

2022 Frontiers in Astronomy and Space Sciences
SolarOrbiter 26