Search Publications

The GAPS Programme at TNG: LXV. Precise density measurement of TOI-1430 b, a young planet with an evaporating atmosphere
DOI: 10.1051/0004-6361/202452236 Bibcode: 2025A&A...693A..32N

Baratella, M.; Mallonn, M.; Scandariato, G. +34 more

Context. Small-sized (<4 R) exoplanets in tight orbits around young stars (10–1000 Myr) give us the opportunity to investigate the mechanisms that led to their formation, the evolution of their physical and orbital properties, and, in particular, their atmospheres. Thanks to the all-sky survey carried out by the TESS spacecraft, man…

2025 Astronomy and Astrophysics
Gaia 0
Luminosity Distance and Extinction by Submicrometer-sized Grains
DOI: 10.3847/2041-8213/ada894 Bibcode: 2025ApJ...979L..45S

Siebenmorgen, R.; Chini, R.; Heymann, Frank

The distance to the stars is a fundamental parameter, which is determined via two primary methods—parallax and luminosity. While the parallax is a direct trigonometric method, the luminosity distance is usually influenced by interstellar extinction. As long as the optical properties of dust grains are wavelength-dependent this contamination can be…

2025 The Astrophysical Journal
Gaia 0
Spectral features and variable circular polarisation in the radio emission from the pre-cataclysmic variable QS Vir
DOI: 10.1051/0004-6361/202452711 Bibcode: 2025A&A...695A..96R

Heinke, C. O.; Sivakoff, G. R.; Hughes, A. K. +2 more

Context. QS Vir is a low-accretion rate cataclysmic variable (CV), or pre-CV, as the M dwarf companion is just filling its Roche lobe. We recently identified radio emission from QS Vir in the Very Large Array Sky Survey (VLASS), at a flux of ∼1 mJy. The origin of radio emission from CVs is not fully understood, with evidence for synchrotron emissi…

2025 Astronomy and Astrophysics
Gaia 0
BiSpeD: Binary Spectral Disentangling applied to binary low-mass star searches
DOI: 10.1051/0004-6361/202451496 Bibcode: 2025A&A...694A..32M

González, J. F.; Martínez, C. I.

Context. In a companion paper, we present a novel method for the spectroscopic detection of low-luminosity secondary companions of binary stars. An interesting application field is the identification of very low-mass stars as companions of late-type main-sequence stars. Aims. To provide a simple tool based on our method, we developed Binary Spectr…

2025 Astronomy and Astrophysics
Gaia 0
Examining the evolution of the supersoft X-ray source RX J0513.9 ‑ 6951
DOI: 10.1051/0004-6361/202453039 Bibcode: 2025A&A...694A..73T

Werner, K.; Santangelo, A.; Suleimanov, V. F. +1 more

Context. Supersoft X-ray sources (SSSs) are thought to be accreting white dwarfs (WDs) in close binary systems, with thermonuclear burning on their surfaces. The SSS RX J0513.9 ‑ 6951 in the Large Magellanic Cloud (LMC) exhibits cyclic variations between optical low and high states, which are anti-correlated with its X-ray flux. This behaviour is …

2025 Astronomy and Astrophysics
XMM-Newton 0
Global comparative basin hypsometric analysis of Earth and Mars: Implications for early Mars climate
DOI: 10.1016/j.epsl.2025.119226 Bibcode: 2025E&PSL.65319226F

Fang, J.; Luo, W.; Howard, A. D. +3 more

While there is a consensus that water played at least some role in the formation of various Martian landforms, including valley networks (VNs), the specific mechanisms and climate conditions are still debated. Basin hypsometric curves, reflecting elevation distributions, offer insights into past processes and climates. Our study presents a global-…

2025 Earth and Planetary Science Letters
MEx 0
Advanced charge control dynamics simulation for the LISA gravitational reference sensor
DOI: 10.1088/1361-6382/adaf00 Bibcode: 2025CQGra..42e5013K

Kenyon, Samantha Parry; Apple, Stephen; Siu, John +2 more

A gravitational wave detector in space, the Laser Interferometer Space Antenna (LISA) will be able to detect gravitational waves in the frequency range of 0.1 mHz–1 Hz, adding to humanity's knowledge of the dark cosmos. The LISA gravitational reference sensor contains a test mass (TM) and is used to determine the local inertial reference frame and…

2025 Classical and Quantum Gravity
LISAPathfinder 0
Martian Atmospheric Disturbances From Orbital Images and Surface Pressure at Jezero Crater, Mars, During Martian Year 36
DOI: 10.1029/2024JE008565 Bibcode: 2025JGRE..13008565S

Hueso, R.; Sánchez-Lavega, A.; Toledo, D. +13 more

We present a study of atmospheric disturbances at Jezero Crater, Mars, using ground-based measurements of surface pressure by the Perseverance rover in combination with orbital images from the Mars Express and Mars Reconnaissance Orbiter missions. The study starts at Ls ∼ 13.3° in MY36 (6 March 2021) and extends up to Ls ∼ 30…

2025 Journal of Geophysical Research (Planets)
MEx 0
Revisiting Variable Stars Near Globular Clusters South of ‑29° Declination
DOI: 10.1002/asna.20240135 Bibcode: 2025AN....34640135L

Layden, Andrew C.; Evangelista, Julia; Gupta, Sakshi +5 more

We review an often-cited but seldom-accessed catalogue by Fourcade and Laborde (1966) of 785 variable stars near 47 southern Galactic globular clusters, and recover the locations of 85 stars that were not incorporated into subsequent variable star catalogues and hence have become "lost" to the literature. We match the positions of these stars with…

2025 Astronomische Nachrichten
Gaia 0
Cleaning WASP-33 b transits from the host star photometric variability: analysis of TESS data from two sectors
DOI: 10.1093/mnras/staf011 Bibcode: 2025MNRAS.537..171B

Baluev, Roman V.; Sokov, Eugene N.

Based on TESS observations of a $\delta$ Scuti variable WASP-33 obtained in 2019 and 2022, we thoroughly investigate the power spectrum of this target photometric flux and construct a statistically exhaustive model for its variability. This model contains 30 robustl…

2025 Monthly Notices of the Royal Astronomical Society
Gaia 0