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Geologic Context of the Bright MARSIS Reflectors in Ultimi Scopuli, South Polar Layered Deposits, Mars
DOI: 10.1029/2022GL098724 Bibcode: 2022GeoRL..4998724L

Landis, M. E.; Whitten, J. L.

Radar-bright basal reflectors have been detected below the South Polar Layered Deposits (SPLD), using Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) data and have an exciting but controversial interpretation: liquid water from subglacial lakes. We mapped the surface of the SPLD immediately above and surrounding the putative la…

2022 Geophysical Research Letters
MEx 3
Asymmetric Interaction of a Solar Wind Reconnecting Current Sheet and Its Magnetic Hole With Earth's Bow Shock and Magnetopause
DOI: 10.1029/2021JA030079 Bibcode: 2022JGRA..12730079M

Liemohn, Michael W.; Karlsson, Tomas; Liu, Terry Z. +3 more

We report results of our multi-spacecraft analysis of a solar wind reconnecting current sheet (RCS) and its solar wind magnetic hole (SWMH) observed on November 20, 2018. In the solar wind, the normal vector to the current sheet plane makes an angle of 32° with the Sun-Earth line. A combination of tilted current sheet plane and foreshock effects c…

2022 Journal of Geophysical Research (Space Physics)
Cluster 3
Shapes of galaxies hosting radio-loud AGNs with z ≤ 1
DOI: 10.1051/0004-6361/202141257 Bibcode: 2022A&A...665A.114Z

van der Wel, A.; Zheng, X. C.; Röttgering, H. J. A. +1 more

Links between the properties of radio-loud active galactic nuclei (RLAGNs) and the morphology of their hosts may provide important clues for our understanding of how RLAGNs are triggered. In this work, focusing on passive galaxies, we study the shape of the hosts of RLAGNs selected from the Karl G. Jansky Very Large Array Cosmic Evolution Survey (…

2022 Astronomy and Astrophysics
eHST 3
SQUAB—I: The First Release of Strange QUasar Candidates With ABnormal Astrometric Characteristics From Gaia EDR3 and SDSS
DOI: 10.3389/fspas.2022.822768 Bibcode: 2022FrASS...922768W

Zheng, Zhen-Ya; Ji, Xiang; An, Tao +5 more

Given their extremely large distances and small apparent sizes, quasars are generally considered as objects with near-zero parallax and proper motion. However, some special quasars may have abnormal astrometric characteristics, such as quasar pairs, lensed quasars, AGNs with bright parsec-scale optical jets, which are scientifically interesting ob…

2022 Frontiers in Astronomy and Space Sciences
Gaia 3
Detecting the Oscillation and Propagation of the Nascent Dynamic Solar Wind Structure at 2.6 Solar Radii Using Very Long Baseline Interferometry Radio Telescopes
DOI: 10.3847/2041-8213/ac96e7 Bibcode: 2022ApJ...940L..32M

He, Jiansen; Venturi, Tiziana; Zhang, Peijin +30 more

Probing the solar corona is crucial to study the coronal heating and solar wind acceleration. However, the transient and inhomogeneous solar wind flows carry large-amplitude inherent Alfvén waves and turbulence, which make detection more difficult. We report the oscillation and propagation of the solar wind at 2.6 solar radii (Rs) by observation o…

2022 The Astrophysical Journal
MEx SOHO 3
Does the Lockstep Growth between Black Holes and Bulges Create Their Mass Relation?
DOI: 10.3847/1538-4357/ac9c68 Bibcode: 2022ApJ...940..146Y

Papovich, Casey; Yang, Guang; Brandt, W. N. +7 more

Recent studies have revealed a strong relation between the sample-averaged black hole (BH) accretion rate (BHAR) and star formation rate (SFR) among bulge-dominated galaxies-i.e., "lockstep" BH-bulge growth-in the distant universe. This relation might be closely connected to the BH-bulge mass correlation observed in the local universe. To further …

2022 The Astrophysical Journal
Herschel 3
The First High-contrast Images of X-Ray Binaries: Detection of Candidate Companions in the γ Cas Analog RX J1744.7-2713
DOI: 10.3847/1538-3881/ac6d57 Bibcode: 2022AJ....164....7P

Fabian, A. C.; Gandhi, P.; Mawet, D. +17 more

X-ray binaries provide exceptional laboratories for understanding the physics of matter under the most extreme conditions. Until recently, there were few, if any, observational constraints on the circumbinary environments of X-ray binaries at ~100-5000 au scales. It remains unclear how the accretion onto the compact objects or the explosions givin…

2022 The Astronomical Journal
Gaia 3
The impact of the presence of water ice on the analysis of debris disk observations
DOI: 10.1051/0004-6361/202141413 Bibcode: 2022A&A...658A.121S

Wolf, S.; Stuber, T. A.

Context. The analysis of debris disk observations is often based on the assumption of a dust phase composed of compact spherical grains consisting of astronomical silicate. Instead, observations indicate the existence of water ice in debris disks.
Aims: We quantify the impact of water ice as a potential grain constituent in debris disks on th…

2022 Astronomy and Astrophysics
Gaia 3
Selection of the Main Control Parameters for the Dst Index Prediction Model Based on a Layer-wise Relevance Propagation Method
DOI: 10.3847/1538-4365/ac616c Bibcode: 2022ApJS..260....6L

Zhang, J.; Wang, Z.; Li, Y. Y. +8 more

The prediction of the Dst index is an important subject in space weather. It has significant progress with the prevalent applications of neural networks. The selection of input parameters is critical for the prediction model of the Dst index or other space-weather models. In this study, we perform a layer-wise relevance propagation (LRP) method to…

2022 The Astrophysical Journal Supplement Series
Gaia 3
Planet Patrol: Vetting Transiting Exoplanet Candidates with Citizen Science
DOI: 10.1088/1538-3873/ac5de0 Bibcode: 2022PASP..134d4401K

Kostov, Veselin B.; Kuchner, Marc J.; Brande, Jonathan +15 more

NASA's TESS mission yields light curves for tens of millions of stars spread across the entire sky, a data set that will be a challenge to fully exploit without help from citizen scientists. To address this, we launched a new citizen science project, called "Planet Patrol", designed to analyze TESS data on exoplanet and eclipsing binary candidates…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3