Search Publications

Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ∼ 6-10 and a Consistent Picture of Cosmic Reionization
DOI: 10.3847/1538-4357/aaa544 Bibcode: 2018ApJ...854...73I

Ono, Yoshiaki; Ouchi, Masami; Shimasaku, Kazuhiro +3 more

We present UV luminosity functions of dropout galaxies at z∼ 6{--}10 with the complete Hubble Frontier Fields data. We obtain a catalog of ∼450 dropout-galaxy candidates (350, 66, and 40 at z∼ 6{--}7, 8, and 9, respectively), with UV absolute magnitudes that reach ∼ -14 mag, ∼2 mag deeper than the Hubble Ultra Deep Field detection limits. We caref…

2018 The Astrophysical Journal
eHST 288
Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2
DOI: 10.3847/1538-4357/aada83 Bibcode: 2018ApJ...866...99B

van Saders, Jennifer L.; Huber, Daniel; Berger, Travis A. +1 more

One bottleneck for the exploitation of data from the Kepler mission for stellar astrophysics and exoplanet research has been the lack of precise radii and evolutionary states for most of the observed stars. We report revised radii of 177,911 Kepler stars derived by combining parallaxes from the Gaia Data Release 2 with the DR25 Kepler Stellar Prop…

2018 The Astrophysical Journal
Gaia 277
Evidence for a Systematic Offset of -80 µas in the Gaia DR2 Parallaxes
DOI: 10.3847/1538-4357/aacafc Bibcode: 2018ApJ...862...61S

Torres, Guillermo; Stassun, Keivan G.

We reprise the analysis of Stassun & Torres, comparing the parallaxes of the eclipsing binaries reported in that paper to the parallaxes newly reported in the Gaia second data release (DR2). We find evidence for a systematic offset of -82 ± 33 µas, in the sense of the Gaia parallaxes being too small, for brightnesses (G ≲ 12) and for dis…

2018 The Astrophysical Journal
Gaia 273
Kinematic Evidence for an Embedded Protoplanet in a Circumstellar Disk
DOI: 10.3847/2041-8213/aac6dc Bibcode: 2018ApJ...860L..13P

Pinte, C.; Ménard, F.; Duchêne, G. +6 more

Disks of gas and dust surrounding young stars are the birthplace of planets. However, the direct detection of protoplanets forming within disks has proved elusive to date. We present the detection of a large, localized deviation from Keplerian velocity in the protoplanetary disk surrounding the young star HD 163296. The observed velocity pattern i…

2018 The Astrophysical Journal
Gaia 272
A Kinematical Detection of Two Embedded Jupiter-mass Planets in HD 163296
DOI: 10.3847/2041-8213/aac6d7 Bibcode: 2018ApJ...860L..12T

Foreman-Mackey, Daniel; Bae, Jaehan; Bergin, Edwin A. +2 more

We present the first kinematical detection of embedded protoplanets within a protoplanetary disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we demonstrate a new technique to measure the rotation curves of CO isotopologue emission to sub-percent precision relative to the Keplerian rotation. These rotation curve…

2018 The Astrophysical Journal
Gaia 272
Elucidating ΛCDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
DOI: 10.3847/1538-4357/aaa1ed Bibcode: 2018ApJ...853..119A

Halpern, M.; Weiland, J. L.; Hinshaw, G. +3 more

We examine the impact of baryon acoustic oscillation (BAO) scale measurements on the discrepancy between the value of the Hubble constant (H 0) inferred from the local distance ladder and that from Planck cosmic microwave background (CMB) data. While the BAO data alone cannot constrain H 0, we show that combining the latest B…

2018 The Astrophysical Journal
Planck 240
H- Opacity and Water Dissociation in the Dayside Atmosphere of the Very Hot Gas Giant WASP-18b
DOI: 10.3847/2041-8213/aab272 Bibcode: 2018ApJ...855L..30A

Fortney, Jonathan J.; Stevenson, Kevin B.; Désert, Jean-Michel +7 more

We present one of the most precise emission spectra of an exoplanet observed so far. We combine five secondary eclipses of the hot Jupiter WASP-18b (T day ∼ 2900 K) that we secured between 1.1 and 1.7 µm with the Wide Field Camera 3 instrument on board the Hubble Space Telescope. Our extracted spectrum (S/N = 50, R ∼ 40) does not …

2018 The Astrophysical Journal
eHST 236
Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate
DOI: 10.3847/1538-4357/aaa5a9 Bibcode: 2018ApJ...853..126R

Dickinson, Mark; Ferguson, Henry C.; Grogin, Norman A. +31 more

We present an analysis of 15 Type Ia supernovae (SNe Ia) at redshift z> 1 (9 at 1.5< z< 2.3) recently discovered in the CANDELS and CLASH Multi-Cycle Treasury programs using WFC3 on the Hubble Space Telescope. We combine these SNe Ia with a new compilation of ∼1050 SNe Ia, jointly calibrated and corrected for simulated survey biases to pr…

2018 The Astrophysical Journal
eHST 225
Extremely Irradiated Hot Jupiters: Non-oxide Inversions, H- Opacity, and Thermal Dissociation of Molecules
DOI: 10.3847/1538-4357/aadd9e Bibcode: 2018ApJ...866...27L

Lothringer, Joshua D.; Barman, Travis; Koskinen, Tommi

Extremely irradiated hot Jupiters, exoplanets reaching dayside temperatures >2000 K, stretch our understanding of planetary atmospheres and the models we use to interpret observations. While these objects are planets in every other sense, their atmospheres reach temperatures at low pressures comparable only to stellar atmospheres. In order to u…

2018 The Astrophysical Journal
eHST 222
The ATLAS All-Sky Stellar Reference Catalog
DOI: 10.3847/1538-4357/aae386 Bibcode: 2018ApJ...867..105T

Wolf, C.; Smartt, S. J.; Stalder, B. +6 more

The Asteroid Terrestrial-impact Last Alert System (ATLAS) observes most of the sky every night in search of dangerous asteroids. Its data are also used to search for photometric variability, where sensitivity to variability is limited by photometric accuracy. Since each exposure spans 7.°6 corner to corner, variations in atmospheric transparency i…

2018 The Astrophysical Journal
Gaia Hipparcos 220