Search Publications

Abundance measurements of H2O and carbon-bearing species in the atmosphere of WASP-127b confirm its supersolar metallicity
DOI: 10.1093/mnras/staa3116 Bibcode: 2021MNRAS.500.4042S

Deming, Drake; Nikolov, Nikolay; Carter, Aarynn L. +14 more

The chemical abundances of exoplanet atmospheres may provide valuable information about the bulk compositions, formation pathways, and evolutionary histories of planets. Exoplanets with large, relatively cloud-free atmospheres, and which orbit bright stars provide the best opportunities for accurate abundance measurements. For this reason, we meas…

2021 Monthly Notices of the Royal Astronomical Society
eHST 54
A comprehensive reanalysis of Spitzer's 4.5 µm phase curves, and the phase variations of the ultra-hot Jupiters MASCARA-1b and KELT-16b
DOI: 10.1093/mnras/stab1027 Bibcode: 2021MNRAS.504.3316B

Fortney, Jonathan J.; Stevenson, Kevin B.; Désert, Jean-Michel +12 more

We have developed an open-source pipeline for the analysis of Spitzer/IRAC channel 1 and 2 time-series photometry, incorporating some of the most popular decorrelation methods. We applied this pipeline to new phase curve observations of ultra-hot Jupiters MASCARA-1b and KELT-16b, and we performed the first comprehensive reanalysis of 15 phase curv…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 54
Constraining stellar evolution theory with asteroseismology of γ Doradus stars using deep learning. Stellar masses, ages, and core-boundary mixing
DOI: 10.1051/0004-6361/202039543 Bibcode: 2021A&A...650A..58M

Aerts, C.; Van Reeth, T.; Mombarg, J. S. G.

Context. The efficiency of the transport of angular momentum and chemical elements inside intermediate-mass stars lacks proper calibration, thereby introducing uncertainties on a star's evolutionary pathway. Improvements require better estimation of stellar masses, evolutionary stages, and internal mixing properties.
Aims: Our aim was to deve…

2021 Astronomy and Astrophysics
Gaia 54
The BepiColombo Planetary Magnetometer MPO-MAG: What Can We Learn from the Hermean Magnetic Field?
DOI: 10.1007/s11214-021-00822-x Bibcode: 2021SSRv..217...52H

Balogh, A.; Glassmeier, K. -H.; Nakamura, R. +29 more

The magnetometer instrument MPO-MAG on-board the Mercury Planetary Orbiter (MPO) of the BepiColombo mission en-route to Mercury is introduced, with its instrument design, its calibration and scientific targets. The instrument is comprised of two tri-axial fluxgate magnetometers mounted on a 2.9 m boom and are 0.8 m apart. They monitor the magnetic…

2021 Space Science Reviews
BepiColombo 54
Measuring fundamental jet properties with multiwavelength fast timing of the black hole X-ray binary MAXI J1820+070
DOI: 10.1093/mnras/stab820 Bibcode: 2021MNRAS.504.3862T

Maccarone, T. J.; Dhillon, V. S.; Gandhi, P. +9 more

We present multiwavelength fast timing observations of the black hole X-ray binary MAXI J1820+070 (ASASSN-18ey), taken with the Karl G. Jansky Very Large Array (VLA), Atacama Large Millimeter/Sub-Millimeter Array (ALMA), Very Large Telescope (VLT), New Technology Telescope (NTT), Neutron Star Interior Composition Explorer (NICER), and XMM-Newton. …

2021 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 53
Einstein@Home discovery of the gamma-ray millisecond pulsar PSR J2039-5617 confirms its predicted redback nature
DOI: 10.1093/mnras/staa3484 Bibcode: 2021MNRAS.502..915C

Dhillon, V. S.; Guillemot, L.; Harding, A. K. +19 more

The Fermi Large Area Telescope gamma-ray source 3FGL J2039.6-5618 contains a periodic optical and X-ray source that was predicted to be a 'redback' millisecond pulsar (MSP) binary system. However, the conclusive identification required the detection of pulsations from the putative MSP. To better constrain the orbital parameters for a directed sear…

2021 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 53
Distances to Galactic X-ray binaries with Gaia DR2
DOI: 10.1093/mnras/stab345 Bibcode: 2021MNRAS.502.5455A

Barmby, P.; Bahramian, A.; Arnason, R. M. +2 more

Precise and accurate measurements of distances to Galactic X-ray binaries (XRBs) reduce uncertainties in the determination of XRB physical parameters. We have cross-matched the XRB catalogues of Liu, van Paradijs & van den Heuvel to the results of Gaia Data Release 2. We identify 86 XRBs with a Gaia candidate counterpart, of which 32 are low-m…

2021 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 53
1D atmospheric study of the temperate sub-Neptune K2-18b
DOI: 10.1051/0004-6361/202039072 Bibcode: 2021A&A...646A..15B

Bézard, B.; Charnay, B.; Blain, D.

Context. The atmospheric composition of exoplanets with masses between 2 and 10 M is poorly understood. In that regard, the sub-Neptune K2-18b, which is subject to Earth-like stellar irradiation, offers a valuable opportunity for the characterisation of such atmospheres. Previous analyses of its transmission spectrum from the Kepler, H…

2021 Astronomy and Astrophysics
eHST 53
How to Identify Exoplanet Surfaces Using Atmospheric Trace Species in Hydrogen-dominated Atmospheres
DOI: 10.3847/1538-4357/abfdc7 Bibcode: 2021ApJ...914...38Y

Fortney, Jonathan J.; Moses, Julianne I.; Zhang, Xi +1 more

Sub-Neptunes (Rp ~ 1.25-4 REarth) remain the most commonly detected exoplanets to date. However, it remains difficult for observations to tell whether these intermediate-sized exoplanets have surfaces and where their surfaces are located. Here we propose that the abundances of trace species in the visible atmospheres of these…

2021 The Astrophysical Journal
IUE 53
The all-sky PLATO input catalogue
DOI: 10.1051/0004-6361/202140717 Bibcode: 2021A&A...653A..98M

Heras, A. M.; Deleuil, M.; Rauer, H. +29 more

Context. The ESA PLAnetary Transits and Oscillations of stars (PLATO) mission will search for terrestrial planets in the habitable zone of solar-type stars. Because of telemetry limitations, PLATO targets need to be pre-selected.
Aims: In this paper, we present an all sky catalogue that will be fundamental to selecting the best PLATO fields a…

2021 Astronomy and Astrophysics
Gaia 53