Search Publications

Exploring the Circular Polarisation of Low-Frequency Solar Radio Bursts with LOFAR
DOI: 10.1007/s11207-022-01976-9 Bibcode: 2022SoPh..297...47M

Kumari, Anshu; Zucca, Pietro; Vocks, Christian +9 more

The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio wavelengths. Low frequency radio bursts have recently been brought back to light with the advancement of novel radio interferometers. However, their polarisation properties have not yet been explored in detail, especially with the Low Frequency Arra…

2022 Solar Physics
PROBA-2 13
Ensemble-based unsupervised machine learning method for membership determination of open clusters using Mahalanobis distance
DOI: 10.1093/mnras/stac2116 Bibcode: 2022MNRAS.515.4685D

Deb, Sukanta; Baruah, Amiya; Kumar, Subhash

We present an improved method for the determination of membership of an open cluster using ensemble-based unsupervised machine learning techniques. The working principle of this method relies on two stages: (i) choosing a suitable range of three astrometric parameters (π, µαcos δ, µδ) using k-nearest neighbour (kN…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
The importance of Fe fragmentation for LiBeB analyses. Is a Li primary source needed to explain AMS-02 data?
DOI: 10.1051/0004-6361/202243446 Bibcode: 2022A&A...668A...7M

Maurin, D.; Ferronato Bueno, E.; Génolini, Y. +2 more

Context. High-precision data from AMS-02 on Li, Be, and B provide the best constraints on Galactic cosmic-ray transport parameters.
Aims: We re-evaluate the impact of Fe fragmentation on the Li, Be, and B modelling. We discuss the consequences on the transport parameter determination and reassess whether a primary source of Li is needed to ma…

2022 Astronomy and Astrophysics
Ulysses 13
TYC 2990-127-1: An Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer
DOI: 10.1093/mnras/stac1177 Bibcode: 2022MNRAS.513.4295K

Han, Zhanwen; Kovalev, Mikhail; Chen, Xuefei +3 more

We present a study of the spectroscopic binary TYC 2990-127-1 from the LAMOST survey. We use full-spectrum fitting to derive radial velocities and spectral parameters. The high mass ratio indicates that the system underwent mass transfer in the past. We compute the orbital solution and find that it is a very close sub-giant/red giant pair on circu…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Measuring weak lensing masses on individual clusters
DOI: 10.1093/mnras/stac689 Bibcode: 2022MNRAS.512.4785M

Melin, Jean-Baptiste; Bartlett, James G.; Murray, Calum +1 more

We present weak lensing mass estimates for a sample of 458 galaxy clusters from the redMaPPer Sloan Digital Sky Survey DR8 catalogue using Hyper Suprime-Cam weak lensing data. We develop a method to quickly estimate cluster masses from weak lensing shear and use this method to estimate weak lensing masses for each of the galaxy clusters in our sam…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
GJ 229B: Solving the Puzzle of the First Known T Dwarf with the APOLLO Retrieval Code
DOI: 10.3847/1538-4357/ac5590 Bibcode: 2022ApJ...935..107H

Mandell, Avi M.; McElwain, Michael W.; Howe, Alex R.

GJ 229B was the first T dwarf to be discovered in 1995, and its spectrum has been more thoroughly observed than that of most other brown dwarfs. Yet a full spectroscopic analysis of its atmosphere has not been done with modern techniques. This spectrum has several peculiar features, and recent dynamical estimates of GJ 229B's mass and orbit have d…

2022 The Astrophysical Journal
eHST 13
MICROSCOPE mission scenario, ground segment and data processing
DOI: 10.1088/1361-6382/ac4b9a Bibcode: 2022CQGra..39t4004R

Bergé, Joel; Chhun, Ratana; Métris, Gilles +9 more

Testing the weak equivalence principle to a precision of 10-15 requires a quantity of data that give enough confidence on the final result: ideally, the longer the measurement the better the rejection of the statistical noise. The science sessions had a duration of 120 orbits maximum and were regularly repeated and spaced out to accommo…

2022 Classical and Quantum Gravity
MICROSCOPE 13
A Deep View into the Nucleus of the Sagittarius Dwarf Spheroidal Galaxy with MUSE. III. Discrete Multicomponent Population-dynamical Models Based on the Jeans Equations
DOI: 10.3847/1538-4357/ac9280 Bibcode: 2022ApJ...939..118K

Lützgendorf, Nora; Böker, Torsten; Kamann, Sebastian +12 more

We present comprehensive multicomponent dynamical models of M54 (NGC 6715), the nuclear star cluster of the Sagittarius (Sgr) dwarf galaxy, which is undergoing a tidal disruption in the Milky Way halo. Previous papers in this series used a large MUSE mosaic data set to identify multiple stellar populations in the system and study their kinematic d…

2022 The Astrophysical Journal
eHST 13
OCCASO. IV. Radial velocities and open cluster kinematics
DOI: 10.1051/0004-6361/202141832 Bibcode: 2022A&A...658A..14C

Jordi, C.; Casamiquela, L.; Cantat-Gaudin, T. +8 more

Context. Open clusters (OCs) are widely used as test particles to investigate a variety of astrophysical phenomena, from stellar evolution to Galactic evolution. Gaia and the complementary massive spectroscopic surveys are providing an unprecedented wealth of information about these systems.
Aims: The Open Cluster Chemical Abundances from Spa…

2022 Astronomy and Astrophysics
Gaia 13
Assessing the role of clay and salts on the origin of MARSIS basal bright reflections
DOI: 10.1016/j.epsl.2022.117370 Bibcode: 2022E&PSL.57917370M

Orosei, Roberto; Caprarelli, Graziella; Pettinelli, Elena +7 more

Anomalously bright basal reflections detected by MARSIS at Ultimi Scopuli have been interpreted to indicate the presence of water-saturated materials or ponded liquid water at the base of the South Polar Layered Deposits (SPLD). Because conventional models assume basal temperatures (≤200 K) much lower than the melting point of water, this interpre…

2022 Earth and Planetary Science Letters
MEx 13