Search Publications

TESS Asteroseismic Analysis of the Known Exoplanet Host Star HD 222076
DOI: 10.3847/1538-4357/ab8f29 Bibcode: 2020ApJ...896...65J

Chaplin, William J.; Kane, Stephen R.; Stassun, Keivan G. +22 more

The Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission aiming to search for exoplanets that transit bright stars. The high-quality photometric data of TESS are excellent for the asteroseismic study of solar-like stars. In this work, we present an asteroseismic analysis of the red-giant star HD 222076 hosting a long-period (2…

2020 The Astrophysical Journal
Gaia 19
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies
DOI: 10.3847/1538-4357/ab94ac Bibcode: 2020ApJ...896...95O

Rakshit, Suvendu; Dewangan, Gulab Chand; Ojha, Vineet +1 more

We present a detailed comparative systematic study using a sample of 221 narrow-line Seyfert 1 (NLSy1) galaxies in comparison to a redshift-matched sample of 154 broad-line Seyfert 1 (BLSy1) galaxies based on their observations using ROSAT and/or XMM-Newton in soft X-ray band (0.1-2.0 keV). A homogeneous analysis is carried out to estimate their s…

2020 The Astrophysical Journal
XMM-Newton 19
Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M super-Earth and two warm 14.7 and 10.2-M sub-Neptunes
DOI: 10.1051/0004-6361/201937080 Bibcode: 2020A&A...636A..89H

Kuzuhara, M.; Alonso, R.; Erikson, A. +57 more

We report the discovery of a new planetary system with three transiting planets, one super-Earth and two sub-Neptunes, that orbit EPIC 249893012, a G8 IV-V evolved star (M = 1.05 ± 0.05 M, R = 1.71 ± 0.04 R, Teff = 5430 ± 85 K). The star is just leaving the main sequence. We combined K2 ph…

2020 Astronomy and Astrophysics
Gaia 19
First Solar Energetic Particles Measured on the Lunar Far-side
DOI: 10.3847/2041-8213/abbccc Bibcode: 2020ApJ...902L..30X

Wang, Yuming; Xu, Zigong; Guo, Jingnan +7 more

On 2019 May 6 the Lunar Lander Neutron & Dosimetry (LND) Experiment on board the Chang'E-4 lander on the far-side of the Moon detected its first solar energetic particle (SEP) event with proton energies up to 21 MeV. Combined proton energy spectra are studied based on the LND, SOHO/EPHIN, and ACE/EPAM measurements, which show that LND could pr…

2020 The Astrophysical Journal
SOHO 19
Far-infrared Photometric Redshifts: A New Approach to a Highly Uncertain Enterprise
DOI: 10.3847/1538-4357/aba528 Bibcode: 2020ApJ...900...68C

Casey, Caitlin M.

This paper presents a new approach to deriving far-infrared (FIR) photometric redshifts for galaxies based on their reprocessed emission from dust at rest-frame FIR through millimeter wavelengths. FIR photometric redshifts ("FIR-z") have been used over the past decade to derive redshift constraints for highly obscured galaxies that lack photometry…

2020 The Astrophysical Journal
Herschel 19
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background
DOI: 10.3847/1538-4357/ab5aef Bibcode: 2020ApJ...889...17A

Kirkpatrick, Allison; Marchesi, Stefano; Urry, C. Megan +5 more

We constrain X-ray spectral shapes for the ensemble of active galactic nuclei (AGNs) based on the shape of the cosmic X-ray background (CXB). Specifically, we rule out regions of X-ray spectral parameter space that do not reproduce the CXB in the energy range 1-100 keV. The key X-ray spectral parameters are the photon index, Γ; the cutoff energy, …

2020 The Astrophysical Journal
INTEGRAL 19
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