Search Publications

2.5D retrieval of atmospheric properties from exoplanet phase curves: application to WASP-43b observations
DOI: 10.1093/mnras/staa238 Bibcode: 2020MNRAS.493..106I

Irwin, Patrick G. J.; Aigrain, Suzanne; Parmentier, Vivien +4 more

We present a novel retrieval technique that attempts to model phase curve observations of exoplanets more realistically and reliably, which we call the 2.5-dimensional (2.5D) approach. In our 2.5D approach we retrieve the vertical temperature profile and mean gaseous abundance of a planet at all longitudes and latitudes simultaneously, assuming th…

2020 Monthly Notices of the Royal Astronomical Society
eHST 71
A measurement of water vapour amid a largely quiescent environment on Europa
DOI: 10.1038/s41550-019-0933-6 Bibcode: 2020NatAs...4..266P

Villanueva, G. L.; Roth, L.; Paganini, L. +4 more

Previous investigations proved the existence of local density enhancements in Europa's atmosphere, advancing the idea of a possible origination from water plumes. These measurement strategies, however, were sensitive either to total absorption or atomic emissions, which limited the ability to assess the water content. Here we present direct search…

2020 Nature Astronomy
eHST 71
Stellar clustering shapes the architecture of planetary systems
DOI: 10.1038/s41586-020-2800-0 Bibcode: 2020Natur.586..528W

Kruijssen, J. M. Diederik; Longmore, Steven N.; Chevance, Mélanie +1 more

Planet formation is generally described in terms of a system containing the host star and a protoplanetary disk1-3, of which the internal properties (for example, mass and metallicity) determine the properties of the resulting planetary system4. However, (proto)planetary systems are predicted5,6 and observed7,…

2020 Nature
Gaia 71
The R-Process Alliance: First Magellan/MIKE Release from the Southern Search for R-process-enhanced Stars
DOI: 10.3847/1538-4357/ab9d1a Bibcode: 2020ApJ...898..150E

Beers, Timothy C.; Placco, Vinicius M.; Hansen, Terese T. +9 more

Extensive progress has recently been made in our understanding of heavy-element production via the r-process in the universe, specifically with the first observed neutron star binary merger (NSBM) event associated with the gravitational-wave signal detected by LIGO, GW170817. The chemical abundance patterns of metal-poor r-process-enhanced stars p…

2020 The Astrophysical Journal
Gaia 71
ALMA reveals a large structured disk and nested rotating outflows in DG Tauri B
DOI: 10.1051/0004-6361/201936950 Bibcode: 2020A&A...634L..12D

Dougados, C.; Louvet, F.; Cabrit, S. +3 more

We present Atacama Large Millimeter Array (ALMA) Band 6 observations at 14-20 au spatial resolution of the disk and CO(2-1) outflow around the Class I protostar DG Tau B in Taurus. The disk is very large, both in dust continuum (Reff, 95% = 174 au) and CO (RCO = 700 au). It shows Keplerian rotation around a 1.1 ± 0.2 M⊙<…

2020 Astronomy and Astrophysics
Gaia 70
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. III. Substructures in Protostellar Disks
DOI: 10.3847/1538-4357/abbad5 Bibcode: 2020ApJ...902..141S

Sheehan, Patrick D.; Megeath, S. Thomas; Looney, Leslie W. +2 more

The prevalence of substructures in ∼1-10 Myr old protoplanetary disks, which are often linked to planet formation, has raised the question of how early such features form and, as a corollary, how early planet formation begins. Here we present observations of seven protostellar disks (aged ∼ 0.1-1 Myr) from the Very Large Array/Atacama Large Millim…

2020 The Astrophysical Journal
Gaia Herschel eHST 70
Anticorrelation between the Bulk Speed and the Electron Temperature in the Pristine Solar Wind: First Results from the Parker Solar Probe and Comparison with Helios
DOI: 10.3847/1538-4365/ab61fc Bibcode: 2020ApJS..246...62M

Maksimovic, M.; Bale, S. D.; Štverák, Š. +25 more

We discuss the solar wind electron temperatures Te as measured in the nascent solar wind by Parker Solar Probe during its first perihelion pass. The measurements have been obtained by fitting the high-frequency part of quasi-thermal noise spectra recorded by the Radio Frequency Spectrometer. In addition we compare these measurements wit…

2020 The Astrophysical Journal Supplement Series
Ulysses 70
Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey
DOI: 10.3847/1538-4365/ab5f13 Bibcode: 2020ApJS..247...12S

Mahler, Guillaume; Rigby, Jane R.; Whitaker, Katherine E. +13 more

We present strong gravitational lensing models for 37 galaxy clusters from the Sloan Digital Sky Survey Giant Arcs Survey. We combine data from multi-band Hubble Space Telescope Wide Field Camera 3 (WFC3) imaging, with ground-based imaging and spectroscopy from Magellan, Gemini, Apache Point Observatory, and the Multiple Mirror Telescope, in order…

2020 The Astrophysical Journal Supplement Series
eHST 70
Explanation for the Increase in High-Altitude Water on Mars Observed by NOMAD During the 2018 Global Dust Storm
DOI: 10.1029/2019GL084354 Bibcode: 2020GeoRL..4784354N

Aoki, S.; Vandaele, A. C.; Daerden, F. +21 more

The Nadir and Occultation for MArs Discovery (NOMAD) instrument on board ExoMars Trace Gas Orbiter measured a large increase in water vapor at altitudes in the range of 40-100 km during the 2018 global dust storm on Mars. Using a three-dimensional general circulation model, we examine the mechanism responsible for the enhancement of water vapor in…

2020 Geophysical Research Letters
ExoMars-16 70
The ESO supernovae type Ia progenitor survey (SPY). The radial velocities of 643 DA white dwarfs
DOI: 10.1051/0004-6361/201629648 Bibcode: 2020A&A...638A.131N

Leibundgut, B.; Reimers, D.; Heber, U. +13 more

Close double degenerate binaries are one of the favoured progenitor channels for type Ia supernovae, but it is unclear how many suitable systems there are in the Galaxy. We report results of a large radial velocity survey for double degenerate (DD) binaries using the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY). Exposures t…

2020 Astronomy and Astrophysics
Gaia 70