Search Publications

Probing the physics in the core boundary layers of the double-lined B-type binary KIC 4930889 from its gravito-inertial modes
DOI: 10.1051/0004-6361/202244192 Bibcode: 2023A&A...679A...6M

Aerts, C.; Tkachenko, A.; Van Reeth, T. +1 more

Context. Stellar evolution models of B-type stars are still uncertain in terms of internal mixing properties, notably in the area between the convective core and the radiative envelope. This impacts age determination of such stars in addition to the computation of chemical yields produced at the end of their life.
Aims: We investigated the th…

2023 Astronomy and Astrophysics
Gaia 9
KURVS: the outer rotation curve shapes and dark matter fractions of z 1.5 star-forming galaxies
DOI: 10.1093/mnras/stad1966 Bibcode: 2023MNRAS.524.2814P

Glazebrook, Karl; Obreschkow, Danail; Gillman, Steven +14 more

We present first results from the KMOS Ultra-deep Rotation Velocity Survey (KURVS), aimed at studying the outer rotation curves shape and dark matter content of 22 star-forming galaxies at z ~ 1.5. These galaxies represent 'typical' star-forming discs at z ~ 1.5, being located within the star-forming main sequence and stellar mass-size relation wi…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
The Dark Energy Survey Year 3 high-redshift sample: selection, characterization, and analysis of galaxy clustering
DOI: 10.1093/mnras/stad2402 Bibcode: 2023MNRAS.525.3896S

Bechtol, K.; Smith, M.; Abbott, T. M. C. +98 more

The fiducial cosmological analyses of imaging surveys like DES typically probe the Universe at redshifts z < 1. We present the selection and characterization of high-redshift galaxy samples using DES Year 3 data, and the analysis of their galaxy clustering measurements. In particular, we use galaxies that are fainter than those used in the prev…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Serendipitous Nebular-phase JWST Imaging of SN Ia SN 2021aefx: Testing the Confinement of 56Co Decay Energy
DOI: 10.3847/2041-8213/acb6d8 Bibcode: 2023ApJ...944L..28C

Galbany, L.; Morrell, Nidia; Leroy, Adam K. +29 more

We present new 0.3-21 µm photometry of SN 2021aefx in the spiral galaxy NGC 1566 at +357 days after B-band maximum, including the first detection of any Type Ia supernova (SN Ia) at >15 µm. These observations follow earlier JWST observations of SN 2021aefx at +255 days after the time of maximum brightness, allowing us to probe the t…

2023 The Astrophysical Journal
JWST 9
Deprojecting and constraining the vertical thickness of exoKuiper belts
DOI: 10.1093/mnras/stad1847 Bibcode: 2023MNRAS.524.1229T

Wyatt, Mark C.; Jennings, Jeff; Booth, Richard A. +3 more

Constraining the vertical and radial structure of debris discs is crucial to understanding their formation, evolution, and dynamics. To measure both the radial and vertical structure, a disc must be sufficiently inclined. However, if a disc is too close to edge-on, deprojecting its emission becomes non-trivial. In this paper we show how FRANKENSTE…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
The β Pictoris system: Setting constraints on the planet and the disk structures at mid-IR wavelengths with NEAR
DOI: 10.1051/0004-6361/202245143 Bibcode: 2023A&A...675A..35S

Boccaletti, Anthony; Pantin, Eric; Baruteau, Clément +26 more

Context. β Pictoris is a young nearby system hosting a well-resolved edge-on debris disk, along with at least two exoplanets. It offers key opportunities for carrying out detailed studies of the evolution of young planetary systems and their shaping soon after the end of the planetary formation phase.
Aims: We analyzed high-contrast coronagra…

2023 Astronomy and Astrophysics
Gaia 9
Octofitter: Fast, Flexible, and Accurate Orbit Modeling to Detect Exoplanets
DOI: 10.3847/1538-3881/acf5cc Bibcode: 2023AJ....166..164T

Crotts, Katie A.; Rice, Malena; Do Ó, Clarissa R. +11 more

As next-generation imaging instruments and interferometers search for planets closer to their stars, they must contend with increasing orbital motion and longer integration times. These compounding effects make it difficult to detect faint planets but also present an opportunity. Increased orbital motion makes it possible to move the search for pl…

2023 The Astronomical Journal
Gaia 9
The path from the Chinese and Japanese observations of supernova 1181 AD, to a Type Iax supernova, to the merger of CO and ONe white dwarfs
DOI: 10.1093/mnras/stad717 Bibcode: 2023MNRAS.523.3885S

Schaefer, Bradley E.

In 1181 AD, Chinese and Japanese observers reported an unmoving bright 'Guest Star' in the constellation Chuanshe, visible for 185 d. In 2013, D. Patchick discovered what turned out to be a unique nebula surrounding a unique star, with the structure named 'Pa 30', while subsequent workers made connections to mergers of white dwarfs, to the superno…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Stellar Characterization and Radius Inflation of Hyades M-dwarf Stars from the APOGEE Survey
DOI: 10.3847/1538-4357/acd4bd Bibcode: 2023ApJ...951...90W

Pascucci, Ilaria; Bizyaev, Dmitry; Pan, Kaike +23 more

We present a spectroscopic analysis of a sample of 48 M-dwarf stars (0.2 M < M < 0.6 M ) from the Hyades open cluster using high-resolution H-band spectra from the Sloan Digital Sky Survey/Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey. Our methodology adopts spectrum synthesis with LTE MARCS …

2023 The Astrophysical Journal
Gaia 9
Atomic Transition Probabilities for Transitions of Si I and Si II and the Silicon Abundances of Several Very Metal-poor Stars
DOI: 10.3847/1538-4365/acb642 Bibcode: 2023ApJS..265...42D

Sneden, C.; Roederer, I. U.; Lawler, J. E. +2 more

We report new measurements of branching fractions for 20 UV and blue lines in the spectrum of neutral silicon (Si I) originating in the 3s 23p4s 3Po 1,2,1Po 1, and 3s3p 3 1Do 1,2 upper levels. Transitions studied include both st…

2023 The Astrophysical Journal Supplement Series
eHST 9