Search Publications

PHANGS-JWST First Results: Spurring on Star Formation: JWST Reveals Localized Star Formation in a Spiral Arm Spur of NGC 628
DOI: 10.3847/2041-8213/aca674 Bibcode: 2022ApJ...941L..27W

Sandstrom, Karin M.; Henshaw, Jonathan D.; Kruijssen, J. M. Diederik +34 more

We combine JWST observations with Atacama Large Millimeter/submillimeter Array CO and Very Large Telescope MUSE Hα data to examine off-spiral arm star formation in the face-on, grand-design spiral galaxy NGC 628. We focus on the northern spiral arm, around a galactocentric radius of 3-4 kpc, and study two spurs. These form an interesting contrast,…

2022 The Astrophysical Journal
JWST 13
The detection of transiting exoplanets by Gaia
DOI: 10.1051/0004-6361/202243497 Bibcode: 2022A&A...663A.101P

Gomel, Roy; Mazeh, Tsevi; Audard, Marc +14 more

Context. The space telescope Gaia is mainly dedicated to performing high-precision astrometry but is also used to perform spectroscopy and epoch photometry, which can be used to study various types of photometric variability. One such variability type is exoplanetary transits. The photometric data accumulated so far have finally matured enough to …

2022 Astronomy and Astrophysics
Gaia 13
A Solar-cycle Study of Coronal Rotation: Large Variations, Rapid Changes, and Implications for Solar-wind Models
DOI: 10.3847/1538-4357/ac54ba Bibcode: 2022ApJ...928...42E

Morgan, Huw; Williams, Thomas; Kuridze, David +1 more

Information on the rotation rate of the corona, and its variation over latitude and solar cycle, is valuable for making global connections between the corona and the Sun, for global estimates of reconnection rates and as a basic parameter for solar-wind modeling. Here, we use a time series of tomographical maps gained from coronagraph observations…

2022 The Astrophysical Journal
SOHO 13
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