Search Publications

ACCESS: Confirmation of No Potassium in the Atmosphere of WASP-31b
DOI: 10.3847/1538-3881/abb806 Bibcode: 2020AJ....160..230M

Fortney, Jonathan J.; Kirk, James; López-Morales, Mercedes +12 more

We present a new optical (400-950 nm) transmission spectrum of the hot Jupiter WASP-31b (M = 0.48 MJ; R = 1.54 RJ; P = 3.41 days), obtained by combining four transit observations. These transits were observed with IMACS on the Magellan Baade Telescope at Las Campanas Observatory as part of the ACCESS project. We investigate t…

2020 The Astronomical Journal
eHST 18
Is Superorbital Modulation in SMC X-1 Caused by Absorption in a Warped Precessing Accretion Disk?
DOI: 10.3847/1538-4357/ab8224 Bibcode: 2020ApJ...895...10P

Maitra, Chandreyee; Paul, Biswajit; Pradhan, Pragati

We present a broadband spectral-timing analysis of SMC X-1 at different intensity states of its superorbital variation using 10 Suzaku and 6 Nuclear Spectroscopic Telescope Array (NuSTAR) observations. The spectrum in all the states can be described by an absorbed power law with a high-energy cutoff and a blackbody component along with an iron emi…

2020 The Astrophysical Journal
Suzaku 18
The VANDELS survey: Discovery of massive overdensities of galaxies at z > 2. Location of Lyα-emitting galaxies with respect to environment
DOI: 10.1051/0004-6361/201935855 Bibcode: 2020A&A...640A.107G

Bauer, F. E.; Thomas, R.; Bolzonella, M. +19 more

Context. The advent of deep, multi-wavelength surveys, together with the availability of extensive numerical simulations, now allow us for the systematic search and study of (proto)clusters and their surrounding environment as a function of redshift.
Aims: We aim to define the environment and to identify overdensities in the VANDELS Chandra D…

2020 Astronomy and Astrophysics
eHST 18
A Real-time Automatic Validation System for Optical Transients Detected by GWAC
DOI: 10.1088/1538-3873/ab7a73 Bibcode: 2020PASP..132e4502X

Xu, Y.; Wang, J.; Xin, L. P. +4 more

The ground-based wide-angle camera array generates millions of single frame alerts per night. After the complicated and elaborate filters by multiple methods, a couple of dozens of candidates are still needed to be confirmed by follow-up observations in real-time. In order to free scientists from the complex and high-intensity follow-up tasks, we …

2020 Publications of the Astronomical Society of the Pacific
Gaia 18
High-resolution, 3D radiative transfer modelling. V. A detailed model of the M 51 interacting pair
DOI: 10.1051/0004-6361/202038939 Bibcode: 2020A&A...643A..90N

Clark, Christopher J. R.; Mosenkov, Aleksandr V.; De Looze, Ilse +13 more

Context. Investigating the dust heating mechanisms in galaxies provides a deeper understanding of how the internal energy balance drives their evolution. Over the last decade radiative transfer simulations based on the Monte Carlo method have emphasised the role of the various stellar populations heating the diffuse dust. Beyond the expected heati…

2020 Astronomy and Astrophysics
Herschel 18
The Flare-dominated Accretion Mode of a Radio-bright Candidate Transitional Millisecond Pulsar
DOI: 10.3847/1538-4357/ab8f28 Bibcode: 2020ApJ...895...89L

Strader, Jay; Chomiuk, Laura; Heinke, Craig O. +2 more

We report new simultaneous X-ray and radio continuum observations of 3FGL J0427.9-6704, a candidate member of the enigmatic class of transitional millisecond pulsars. These XMM-Newton and Australia Telescope Compact Array observations of this nearly edge-on, eclipsing low-mass X-ray binary were taken in the sub-luminous disk state at an X-ray lumi…

2020 The Astrophysical Journal
Gaia XMM-Newton 18
Clusterix 2.0: a virtual observatory tool to estimate cluster membership probability
DOI: 10.1093/mnras/stz3610 Bibcode: 2020MNRAS.492.5811B

Jordi, C.; Balaguer-Núñez, L.; Masana, E. +6 more

Clusterix 2.0 is a web-based, Virtual Observatory compliant, interactive tool for the determination of membership probabilities in stellar clusters based on proper-motion data using a fully non-parametric method. In an area occupied by a cluster, the frequency function is made up of two contributions: cluster and field stars. The tool performs an …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 18
New insight into the origin of the GeV flare in the binary system PSR B1259-63/LS 2883 from the 2017 periastron passage
DOI: 10.1093/mnras/staa1876 Bibcode: 2020MNRAS.497..648C

van Soelen, B.; Murphy, D.; Chernyakova, M. +4 more

PSR B1259-63 is a gamma-ray binary system hosting a radio pulsar orbiting around an O9.5Ve star, LS 2883, with a period of ∼3.4 yr. The interaction of the pulsar wind with the LS 2883 outflow leads to unpulsed broad-band emission in the radio, X-rays, GeV, and TeV domains. While the radio, X-ray, and TeV light curves show rather similar behaviour,…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 18
In the Trenches of the Solar-Stellar Connection. I. Ultraviolet and X-Ray Flux-Flux Correlations across the Activity Cycles of the Sun and Alpha Centauri AB
DOI: 10.3847/1538-4365/aba3c6 Bibcode: 2020ApJS..250...16A

Ayres, Thomas R.

This study focuses on high-energy proxies of stellar magnetic activity over long-term starspot cycles of three low-activity Sun-like stars: α Centauri A (HD 128620: G2 V), α Cen B (HD 128621: K1 V), and the Sun itself. Data sets include: daily solar ultraviolet irradiance spectra and X-ray fluxes from the Solar Radiation and Climate Experiment, du…

2020 The Astrophysical Journal Supplement Series
IRIS eHST 18
Evolution of High-Speed Jets and Plasmoids Downstream of the Quasi-Perpendicular Bow Shock
DOI: 10.1029/2019JA027667 Bibcode: 2020JGRA..12527667G

Gunell, H.; Hamrin, M.; Goncharov, O. +1 more

Plasma structures with enhanced dynamic pressure, density, or speed are often observed in Earth's magnetosheath. We present a statistical study of these structures, known as jets and fast plasmoids, in the magnetosheath, downstream of both the quasi-perpendicular and quasi-parallel bow shocks. Using measurements from the four Magnetospheric Multis…

2020 Journal of Geophysical Research (Space Physics)
Cluster 18