Search Publications

TESS asteroseismology of the Kepler red giants
DOI: 10.1093/mnras/stac414 Bibcode: 2022MNRAS.512.1677S

Huber, Daniel; García, Rafael A.; Saunders, Nicholas +11 more

Red giant asteroseismology can provide valuable information for studying the Galaxy as demonstrated by space missions like CoRoT and Kepler. However, previous observations have been limited to small data sets and fields of view. The TESS mission provides far larger samples and, for the first time, the opportunity to perform asteroseimic inference …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 42
The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
DOI: 10.1093/mnras/stac1067 Bibcode: 2022MNRAS.513.3510B

Schaerer, D.; Cullen, F.; McLure, R. J. +20 more

We present a study designed to measure the average Lyman-continuum escape fraction (⟨fesc⟩) of star-forming galaxies at z ≃ 3.5. We assemble a sample of 148 galaxies from the VANDELS spectroscopic survey at 3.35 ≤ zspec ≤ 3.95, selected to minimize line-of-sight contamination of their photometry. For this sample, we use ultra…

2022 Monthly Notices of the Royal Astronomical Society
eHST 42
Abundant ammonium hydrosulphide embedded in cometary dust grains
DOI: 10.1093/mnras/stac2440 Bibcode: 2022MNRAS.516.3900A

Altwegg, K.; Fuselier, S. A.; Rubin, M. +7 more

Ammonium hydrosulphide has long since been postulated to exist at least in certain layers of the giant planets. Its radiation products may be the reason for the red colour seen on Jupiter. Several ammonium salts, the products of NH3, and an acid have previously been detected at comet 67P/Churyumov-Gerasimenko. The acid H2S is…

2022 Monthly Notices of the Royal Astronomical Society
Rosetta 42
Planet populations inferred from debris discs. Insights from 178 debris systems in the ISPY, LEECH, and LIStEN planet-hunting surveys
DOI: 10.1051/0004-6361/202142720 Bibcode: 2022A&A...659A.135P

Gennaro, Mario; Launhardt, Ralf; Kennedy, Grant M. +11 more

We know little about the outermost exoplanets in planetary systems because our detection methods are insensitive to moderate-mass planets on wide orbits. However, debris discs can probe the outer-planet population because dynamical modelling of observed discs can reveal properties of perturbing planets. We use four sculpting and stirring arguments…

2022 Astronomy and Astrophysics
AKARI Gaia 42
The Mass of the Milky Way from the H3 Survey
DOI: 10.3847/1538-4357/ac3a7a Bibcode: 2022ApJ...925....1S

Conroy, Charlie; Ting, Yuan-Sen; Cargile, Phillip A. +8 more

The mass of the Milky Way is a critical quantity that, despite decades of research, remains uncertain within a factor of two. Until recently, most studies have used dynamical tracers in the inner regions of the halo, relying on extrapolations to estimate the mass of the Milky Way. In this paper, we extend the hierarchical Bayesian model applied in…

2022 The Astrophysical Journal
Gaia 42
Keck/NIRSPEC Studies of He I in the Atmospheres of Two Inflated Hot Gas Giants Orbiting K Dwarfs: WASP-52b and WASP-177b
DOI: 10.3847/1538-3881/ac722f Bibcode: 2022AJ....164...24K

Kirk, James; López-Morales, Mercedes; Alam, Munazza K. +5 more

We present the detection of neutral helium at 10833 Å in the atmosphere of WASP-52b and tentative evidence of helium in the atmosphere of the grazing WASP-177b, using high-resolution observations acquired with the NIRSPEC instrument on the Keck II telescope. We detect excess absorption by helium in WASP-52b's atmosphere of 3.44% ± 0.31% (11σ), or …

2022 The Astronomical Journal
Gaia 42
Polarization constraints on the X-ray corona in Seyfert Galaxies: MCG-05-23-16
DOI: 10.1093/mnras/stac2634 Bibcode: 2022MNRAS.516.5907M

Antonelli, L. A.; Costa, E.; Bianchi, S. +97 more

We report on the first observation of a radio-quiet active galactic nucleus (AGN) in polarized X-rays: the Seyfert 1.9 galaxy MCG-05-23-16. This source was pointed at with the Imaging X-ray Polarimetry Explorer (IXPE) starting on 2022 May 14 for a net observing time of 486 ks, simultaneously with XMM-Newton (58 ks) and NuSTAR (83 ks). A polarizati…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 42
The Tidal Disruption Event AT2021ehb: Evidence of Relativistic Disk Reflection, and Rapid Evolution of the Disk-Corona System
DOI: 10.3847/1538-4357/ac898a Bibcode: 2022ApJ...937....8Y

Kulkarni, S. R.; Sunyaev, R.; Cenko, S. Bradley +29 more

We present X-ray, UV, optical, and radio observations of the nearby (≈78 Mpc) tidal disruption event AT2021ehb/ZTF21aanxhjv during its first 430 days of evolution. AT2021ehb occurs in the nucleus of a galaxy hosting a≈107 M black hole (M BH inferred from host galaxy scaling relations). High-cadence Swift and Neut…

2022 The Astrophysical Journal
XMM-Newton 42
A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67
DOI: 10.3847/1538-4357/ac90be Bibcode: 2022ApJ...938..118D

Magnier, Eugene A.; van Saders, Jennifer; García, Rafael A. +5 more

We present stellar rotation periods for late K- and early M-dwarf members of the 4 Gyr old open cluster M67 as calibrators for gyrochronology and tests of stellar spin-down models. Using Gaia EDR3 astrometry for cluster membership and Pan-STARRS (PS1) photometry for binary identification, we build this set of rotation periods from a campaign of mo…

2022 The Astrophysical Journal
Gaia 42
Merger-induced galaxy transformations in the ARTEMIS simulations
DOI: 10.1093/mnras/stac1038 Bibcode: 2022MNRAS.513.1867D

Belokurov, Vasily; Dillamore, Adam M.; McCarthy, Ian G. +1 more

Using the ARTEMIS set of 45 high-resolution cosmological simulations, we investigate a range of merger-induced dynamical transformations of Milky Way-like galaxies. We first identify populations of accreted stars on highly radial orbits, similar to the 'Gaia Sausage' in the Milky Way. We show that ≈1/3 of the ARTEMIS galaxies contain a similar fea…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 42