Search Publications

TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet
DOI: 10.1051/0004-6361/202244617 Bibcode: 2023A&A...675A.115K

Mustill, A. J.; Dai, F.; Gandolfi, D. +59 more

The TOI-1130 is a known planetary system around a K-dwarf consisting of a gas giant planet, TOI-1130 c on an 8.4-day orbit that is accompanied by an inner Neptune-sized planet, TOI-1130 b, with an orbital period of 4.1 days. We collected precise radial velocity (RV) measurements of TOI-1130 with the HARPS and PFS spectrographs as part of our ongoi…

2023 Astronomy and Astrophysics
Gaia 17
Extreme Solar Events: Setting up a Paradigm
DOI: 10.1007/s11214-023-01018-1 Bibcode: 2023SSRv..219...73U

Notsu, Yuta; Maehara, Hiroyuki; Dalla, Silvia +17 more

The Sun is magnetically active and often produces eruptive events on different energetic and temporal scales. Until recently, the upper limit of such events was unknown and believed to be roughly represented by direct instrumental observations. However, two types of extreme events were discovered recently: extreme solar energetic particle events o…

2023 Space Science Reviews
Gaia SOHO Ulysses 17
CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles
DOI: 10.1051/0004-6361/202346189 Bibcode: 2023A&A...674A.179B

Arnaud, M.; Pointecouteau, E.; Pratt, G. W. +25 more

We investigate the statistical properties and the origin of the scatter within the spatially resolved surface brightness profiles of the CHEX-MATE sample, formed by 118 galaxy clusters selected via the SZ effect. These objects have been drawn from the Planck SZ catalogue and cover a wide range of masses, M500 = [2 − 15]×1014

2023 Astronomy and Astrophysics
XMM-Newton 17
DELVE 6: An Ancient, Ultra-faint Star Cluster on the Outskirts of the Magellanic Clouds
DOI: 10.3847/2041-8213/aced84 Bibcode: 2023ApJ...953L..21C

Geha, M.; James, D. J.; Kuropatkin, N. +24 more

We present the discovery of DELVE 6, an ultra-faint stellar system identified in the second data release of the DECam Local Volume Exploration (DELVE) survey. Based on a maximum-likelihood fit to its structure and stellar population, we find that DELVE 6 is an old (τ > 9.8 Gyr at 95% confidence) and metal-poor ([Fe/H] < -1.17 dex at 95% conf…

2023 The Astrophysical Journal
Gaia 17
The STIX Imaging Concept
DOI: 10.1007/s11207-023-02205-7 Bibcode: 2023SoPh..298..114M

Volpara, Anna; Massa, Paolo; Krucker, Säm +18 more

We provide a mathematical description of the imaging concept of the Spectrometer/Telescope for Imaging X-rays (STIX) onboard Solar Orbiter. Specifically, we describe the STIX indirect-imaging technique, which is based on spatial modulation of the X-ray photon flux by means of tungsten grids, and we show that each of 30 STIX imaging sub-collimators…

2023 Solar Physics
SolarOrbiter 17
The Distribution of Metallicities in the Local Galactic Interstellar Medium
DOI: 10.3847/1538-4357/acda25 Bibcode: 2023ApJ...952...57R

Jenkins, Edward B.; Savage, Blair D.; Shull, J. Michael +3 more

In this investigation, we present an analysis of the metallicity distribution that pertains to neutral gas in the local Galactic interstellar medium (ISM). We derive relative ISM metallicities for a sample of 84 sight lines probing diffuse atomic and molecular gas within 4 kpc of the Sun. Our analysis is based in large part on column density measu…

2023 The Astrophysical Journal
Gaia eHST 17
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA). I. The final word on the origin of NGC 6388 and NGC 6441
DOI: 10.1051/0004-6361/202347289 Bibcode: 2023A&A...680A..20M

Salaris, Maurizio; Ruiz-Lara, Tomás; Stokholm, Amalie +11 more

We present CARMA, the Cluster Ages to Reconstruct the Milky Way Assembly project, the aim of which is to determine precise and accurate age measurements for the entire system of known Galactic globular clusters (GCs) and to use them to trace the most significant merger events experienced by the Milky Way. The strength of CARMA relies on the use of…

2023 Astronomy and Astrophysics
Gaia eHST 17
DAHe white dwarfs from the DESI Survey
DOI: 10.1093/mnras/stad727 Bibcode: 2023MNRAS.521.4976M

Brooks, D.; Honscheid, K.; Miquel, R. +16 more

A new class of white dwarfs, dubbed DAHe, that present Zeeman-split Balmer lines in emission has recently emerged. However, the physical origin of these emission lines remains unclear. We present here a sample of 21 newly identified DAHe systems and determine magnetic field strengths and (for a subset) periods that span the ranges of ≃6.5-147 MG a…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 17
Hubble Constant Measurement from Three Large-separation Quasars Strongly Lensed by Galaxy Clusters
DOI: 10.3847/1538-4357/ad045a Bibcode: 2023ApJ...959..134N

Mahler, Guillaume; Rigby, Jane R.; Bayliss, Matthew +5 more

Tension between cosmic microwave background-based and distance ladder-based determinations of the Hubble constant H 0 motivates the pursuit of independent methods that are not subject to the same systematic effects. A promising alternative, proposed by Refsdal in 1964, relies on the inverse scaling of H 0 with the delay betwe…

2023 The Astrophysical Journal
eHST 17
Dissecting the RELICS cluster SPT-CLJ0615-5746 through intracluster light: Confirmation of the multiple merging state of the cluster formation
DOI: 10.1051/0004-6361/202346580 Bibcode: 2023A&A...676A..39J

Vílchez, J. M.; Lopes, P. A. A.; Dupke, R. A. +1 more

The intracluster light (ICL) fraction, measured at certain specific wavelengths, has been shown to provide a good marker for determining the dynamical stage of galaxy clusters, that is, merging versus relaxed, for low to intermediate redshifts. We apply it for the first time to a high-redshift system, SPT-CLJ0615-5746 at z = 0.97, using its Reioni…

2023 Astronomy and Astrophysics
eHST 17