Search Publications

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
Three Hypervelocity White Dwarfs in Gaia DR2: Evidence for Dynamically Driven Double-degenerate Double-detonation Type Ia Supernovae
DOI: 10.3847/1538-4357/aad55b Bibcode: 2018ApJ...865...15S

Foley, Ryan J.; Boubert, Douglas; Smith, Nathan +23 more

Double detonations in double white dwarf (WD) binaries undergoing unstable mass transfer have emerged in recent years as one of the most promising Type Ia supernova (SN Ia) progenitor scenarios. One potential outcome of this “dynamically driven double-degenerate double-detonation” (D6) scenario is that the companion WD survives the expl…

2018 The Astrophysical Journal
Gaia 200
The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies
DOI: 10.3847/1538-4357/aaa3e7 Bibcode: 2018ApJ...853...56R

van Dokkum, Pieter G.; Illingworth, Garth D.; Labbé, Ivo +13 more

We use a newly assembled sample of 3545 star-forming galaxies with secure spectroscopic, grism, and photometric redshifts at z = 1.5-2.5 to constrain the relationship between UV slope (β) and dust attenuation (L IR/L UV ≡ IRX). Our sample significantly extends the range of L UV and β probed in previous UV-selected …

2018 The Astrophysical Journal
Herschel eHST 200
Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6
DOI: 10.3847/1538-4357/aaee7a Bibcode: 2018ApJ...869..150M

Ono, Yoshiaki; Ouchi, Masami; Goto, Tomotsugu +44 more

We present new measurements of the quasar luminosity function (LF) at z ∼ 6 over an unprecedentedly wide range of the rest-frame ultraviolet luminosity M 1450 from -30 to -22 mag. This is the fifth in a series of publications from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, which exploits the deep multiban…

2018 The Astrophysical Journal
eHST 199
The Sausage Globular Clusters
DOI: 10.3847/2041-8213/aad7f7 Bibcode: 2018ApJ...863L..28M

Myeong, G. C.; Evans, N. W.; Belokurov, V. +2 more

The Gaia Sausage is an elongated structure in velocity space discovered by Belokurov et al. using the kinematics of metal-rich halo stars. They showed that it could be created by a massive dwarf galaxy (∼5 × 1010 {M}) on a strongly radial orbit that merged with the Milky Way at a redshift z ≲ 3. This merger would also have …

2018 The Astrophysical Journal
Gaia eHST 197
A Decline in the X-Ray through Radio Emission from GW170817 Continues to Support an Off-axis Structured Jet
DOI: 10.3847/2041-8213/aad637 Bibcode: 2018ApJ...863L..18A

Berger, E.; Chornock, R.; Fong, W. +17 more

We present new observations of the binary neutron star merger GW170817 at Δt ≈ 220-290 days post-merger, at radio (Karl G. Jansky Very Large Array; VLA), X-ray (Chandra X-ray Observatory), and optical (Hubble Space Telescope; HST) wavelengths. These observations provide the first evidence for a turnover in the X-ray light curve, mirroring a declin…

2018 The Astrophysical Journal
eHST 194