Search Publications

The period-luminosity relation for δ Scuti stars using Gaia DR2 parallaxes
DOI: 10.1093/mnras/stz1110 Bibcode: 2019MNRAS.486.4348Z

Bedding, Timothy R.; Murphy, Simon J.; Hey, Daniel R. +2 more

We have examined the period-luminosity (P-L) relation for δ Scuti stars using Gaia DR2 parallaxes. We included 228 stars from the catalogue of Rodríguez et al., as well as 1124 stars observed in the 4-yr Kepler mission. For each star, we considered the dominant pulsation period, and used DR2 parallaxes and extinction corrections to determine absol…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 65
Cluster Difference Imaging Photometric Survey. I. Light Curves of Stars in Open Clusters from TESS Sectors 6 and 7
DOI: 10.3847/1538-4365/ab4a7e Bibcode: 2019ApJS..245...13B

Winn, J. N.; Bouma, L. G.; Bhatti, W. +2 more

The Transiting Exoplanet Survey Satellite (TESS) is providing precise time-series photometry for most star clusters in the solar neighborhood. Using the TESS images, we have begun a Cluster Difference Imaging Photometric Survey, in which we are focusing both on stars that are candidate cluster members and on stars that show indications of youth. O…

2019 The Astrophysical Journal Supplement Series
Gaia 65
Highly Magnified Stars in Lensing Clusters: New Evidence in a Galaxy Lensed by MACS J0416.1-2403
DOI: 10.3847/1538-4357/ab2888 Bibcode: 2019ApJ...880...58K

Miralda-Escudé, Jordi; Frye, Brenda; Dai, Liang +2 more

We examine a caustic-straddling arc at z = 0.9397 in the field of the galaxy cluster MACS J0416.1-2403 (z = 0.397) using archival multiband Hubble Space Telescope images and show that its surface brightness exhibits anomalies that can be explained by a single highly magnified star undergoing microlensing. First, we show that the surface brightness…

2019 The Astrophysical Journal
eHST 65
NGTS-4b: A sub-Neptune transiting in the desert
DOI: 10.1093/mnras/stz1084 Bibcode: 2019MNRAS.486.5094W

Jackman, James A. G.; Wheatley, Peter J.; Bayliss, Daniel +48 more

We report the discovery of NGTS-4b, a sub-Neptune-sized planet transiting a 13th magnitude K-dwarf in a 1.34 d orbit. NGTS-4b has a mass M = 20.6 ± 3.0 M and radius R = 3.18 ± 0.26 R, which places it well within the so-called `Neptunian Desert'. The mean density of the planet (3.45 ± 0.95 g cm-3) is consistent wi…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 65
A New Technique for Finding Galaxies Leaking Lyman-continuum Radiation: [S II]-deficiency
DOI: 10.3847/1538-4357/ab418f Bibcode: 2019ApJ...885...57W

Heckman, Timothy M.; Leitherer, Claus; Wang, Bingjie +3 more

The source responsible for the reionization of the universe is believed to be the population of star-forming galaxies at z ∼ 6 to 12. The biggest uncertainty concerns the fraction of Lyman-continuum photons that actually escape from the galaxies. In recent years, several relatively small samples of “leaky” galaxies have been discovered, and clues …

2019 The Astrophysical Journal
eHST 65
Coronal bright points
DOI: 10.1007/s41116-019-0018-8 Bibcode: 2019LRSP...16....2M

Madjarska, Maria S.

Coronal bright points (CBPs) are a fundamental class of solar activity. They represent a set of low-corona small-scale loops with enhanced emission in the extreme-ultraviolet and X-ray spectrum that connect magnetic flux concentrations of opposite polarities. CBPs are one of the main building blocks of the solar atmosphere outside active regions u…

2019 Living Reviews in Solar Physics
Hinode IRIS SOHO 65
ExoEarth yield landscape for future direct imaging space telescopes
DOI: 10.1117/1.JATIS.5.2.024009 Bibcode: 2019JATIS...5b4009S

Stark, Christopher C.; Mazoyer, Johan; Pueyo, Laurent +19 more

The expected yield of potentially Earth-like planets is a useful metric for designing future exoplanet-imaging missions. Recent yield studies of direct-imaging missions have focused primarily on yield methods and trade studies using "toy" models of missions. Here, we increase the fidelity of these calculations substantially, adopting more realisti…

2019 Journal of Astronomical Telescopes, Instruments, and Systems
Gaia 64
The mean Hα EW and Lyman-continuum photon production efficiency for faint z ≈ 4-5 galaxies
DOI: 10.1051/0004-6361/201935227 Bibcode: 2019A&A...627A.164L

Bacon, Roland; Boogaard, Leindert A.; Mahler, Guillaume +9 more

We present the first measurements of the Lyman-continuum photon production efficiency ξion, 0 at z ∼ 4-5 for galaxies fainter than 0.2 L* (-19 mag). ξion, 0 quantifies the production rate of ionizing photons with respect to the UV luminosity density assuming a fiducial escape fraction of zero. Extending previous me…

2019 Astronomy and Astrophysics
eHST 64
AKARI/IRC near-infrared asteroid spectroscopic survey: AcuA-spec
DOI: 10.1093/pasj/psy125 Bibcode: 2019PASJ...71....1U

Hasegawa, Sunao; Onaka, Takashi; Usui, Fumihiko +1 more

Knowledge of water in the solar system is important for the understanding of a wide range of evolutionary processes and the thermal history of the solar system. To explore the existence of water in the solar system, it is indispensable to investigate hydrated minerals and/or water ice on asteroids. These water-related materials show absorption fea…

2019 Publications of the Astronomical Society of Japan
AKARI 64
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
DOI: 10.3847/1538-4357/ab2f90 Bibcode: 2019ApJ...882...69G

Bradač, M.; Venturi, T.; Jee, M. J. +13 more

Golovich et al. present an optical imaging and spectroscopic survey of 29 radio relic merging galaxy clusters. In this paper, we study this survey to identify substructure and quantify the dynamics of the mergers. Using a combined photometric and spectroscopic approach, we identify the minimum number of substructures in each system to describe the…

2019 The Astrophysical Journal
XMM-Newton eHST 64