Search Publications

Semi-supervised standardized detection of extrasolar planets
DOI: 10.1051/0004-6361/202142486 Bibcode: 2022A&A...667A.104S

Deleuil, M.; Sulis, S.; Mary, D. +1 more

Context. The detection of small exoplanets with the radial velocity (RV) technique is limited by various poorly known noise sources of instrumental and stellar origin. As a consequence, current detection techniques often fail to provide reliable estimates of the significance levels of detection tests in terms of false-alarm rates or p-values.

2022 Astronomy and Astrophysics
SOHO 3
Evaluation of the Capability of ExoMars-TGO NOMAD Infrared Nadir Channel for Water Ice Clouds Detection on Mars
DOI: 10.3390/rs14174143 Bibcode: 2022RemS...14.4143R

Daerden, Frank; Ristic, Bojan; Bellucci, Giancarlo +13 more

As part of the payload of the 2016 ExoMars Trace Gas Orbiter (TGO) mission, the Nadir and Occultation for MArs Discovery (NOMAD) suite instrument has been observing the Martian atmosphere since March 2018. NOMAD is mainly dedicated to the study of trace atmospheric species taking advantage of a high-spectral resolution. We demonstrate that when NO…

2022 Remote Sensing
ExoMars-16 3
Seasonal southern circum-polar spots and araneiforms observed with the colour and stereo surface imaging system (CaSSIS)
DOI: 10.1016/j.pss.2022.105593 Bibcode: 2022P&SS..22405593C

Tornabene, Livio L.; Cremonese, Gabriele; Thomas, Nicolas +5 more

The southern polar area of Mars is home to various seasonal activity commonly explained by the Kieffer model. During southern spring, the ice covering the polar area sublimates and leaves distinct features (spiders, spots, fans) observable from orbit. The Colour and Stereo Surface Imaging System (CaSSIS) onboard the ExoMars Trace Gas Orbiter (TGO)…

2022 Planetary and Space Science
ExoMars-16 3
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