Search Publications

Evolution of the Dust Size Distribution of Comet 67P/Churyumov-Gerasimenko from 2.2 au to Perihelion
DOI: 10.3847/0004-637X/821/1/19 Bibcode: 2016ApJ...821...19F

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +74 more

The Rosetta probe, orbiting Jupiter-family comet 67P/Churyumov-Gerasimenko, has been detecting individual dust particles of mass larger than 10-10 kg by means of the GIADA dust collector and the OSIRIS Wide Angle Camera and Narrow Angle Camera since 2014 August and will continue until 2016 September. Detections of single dust particles …

2016 The Astrophysical Journal
Rosetta 174
The Swift GRB Host Galaxy Legacy Survey. II. Rest-frame Near-IR Luminosity Distribution and Evidence for a Near-solar Metallicity Threshold
DOI: 10.3847/0004-637X/817/1/8 Bibcode: 2016ApJ...817....8P

Berger, E.; Chary, R.; Fynbo, J. P. U. +9 more

We present rest-frame near-IR (NIR) luminosities and stellar masses for a large and uniformly selected population of gamma-ray burst (GRB) host galaxies using deep Spitzer Space Telescope imaging of 119 targets from the Swift GRB Host Galaxy Legacy Survey spanning 0.03 < z < 6.3, and we determine the effects of galaxy evolution and chemical …

2016 The Astrophysical Journal
eHST 168
Carbon and Oxygen Abundances in Low Metallicity Dwarf Galaxies
DOI: 10.3847/0004-637X/827/2/126 Bibcode: 2016ApJ...827..126B

Skillman, Evan D.; Erb, Dawn K.; Berg, Danielle A. +2 more

The study of carbon and oxygen abundances yields information on the time evolution and nucleosynthetic origins of these elements, yet they remain relatively unexplored. At low metallicities, (12+log(O/H) < 8.0), nebular carbon measurements are limited to rest-frame UV collisionally excited emission lines. Therefore, we present the UV spectropho…

2016 The Astrophysical Journal
eHST 167
The Shape of the Inner Milky Way Halo from Observations of the Pal 5 and GD--1 Stellar Streams
DOI: 10.3847/1538-4357/833/1/31 Bibcode: 2016ApJ...833...31B

Bovy, Jo; Kallivayalil, Nitya; Fritz, Tobias K. +1 more

We constrain the shape of the Milky Way’s halo by dynamical modeling of the observed phase-space tracks of the Pal 5 and GD-1 tidal streams. We find that the only information about the potential gleaned from the tracks of these streams are precise measurements of the shape of the gravitational potential—the ratio of vertical to radial acceleration…

2016 The Astrophysical Journal
Gaia 164
Mass Measurements in Protoplanetary Disks from Hydrogen Deuteride
DOI: 10.3847/0004-637X/831/2/167 Bibcode: 2016ApJ...831..167M

Henning, Th.; van Dishoeck, E. F.; Pontoppidan, K. M. +8 more

The total gas mass of a protoplanetary disk is a fundamental, but poorly determined, quantity. A new technique has been demonstrated to assess directly the bulk molecular gas reservoir of molecular hydrogen using the HD J = 1-0 line at 112 µm. In this work we present a Herschel Space Observatory 10 survey of six additional T Tauri…

2016 The Astrophysical Journal
AKARI Herschel 162
Q1549-C25: A Clean Source of Lyman-Continuum Emission at z = 3.15
DOI: 10.3847/2041-8205/826/2/L24 Bibcode: 2016ApJ...826L..24S

Siana, Brian; Shapley, Alice E.; Steidel, Charles C. +5 more

We present observations of Q1549-C25, an ∼ {L}* star-forming galaxy at z = 3.15 for which Lyman-continuum (LyC) radiation is significantly detected in deep Keck/LRIS spectroscopy. We find no evidence of contamination from a lower-redshift interloper close to the line of sight in the high signal-to-noise spectrum of Q1549-C25. Furthermo…

2016 The Astrophysical Journal
eHST 157
The Coupled Physical Structure of Gas and Dust in the IM Lup Protoplanetary Disk
DOI: 10.3847/0004-637X/832/2/110 Bibcode: 2016ApJ...832..110C

Wilner, David J.; Cleeves, L. Ilsedore; Andrews, Sean M. +4 more

The spatial distribution of gas and solids in protoplanetary disks determines the composition and formation efficiency of planetary systems. A number of disks show starkly different distributions for the gas and small grains compared to millimeter-centimeter-sized dust. We present new Atacama Large Millimeter/Submillimeter Array observations of th…

2016 The Astrophysical Journal
Gaia 156
Beyond 31 mag arcsec-2: The Frontier of Low Surface Brightness Imaging with the Largest Optical Telescopes
DOI: 10.3847/0004-637X/823/2/123 Bibcode: 2016ApJ...823..123T

Trujillo, Ignacio; Fliri, Jüergen

The detection of structures in the sky with optical surface brightnesses fainter than 30 mag arcsec-2 (3σ in 10 × 10 arcsec boxes; r-band) has remained elusive in current photometric deep surveys. Here we show how present-day telescopes of 10 m class can provide broadband imaging 1.5-2 mag deeper than most previous results within a reas…

2016 The Astrophysical Journal
Planck 154
The Atmospheric Circulation of a Nine-hot-Jupiter Sample: Probing Circulation and Chemistry over a Wide Phase Space
DOI: 10.3847/0004-637X/821/1/9 Bibcode: 2016ApJ...821....9K

Fortney, Jonathan J.; Sing, David K.; Kataria, Tiffany +4 more

We present results from an atmospheric circulation study of nine hot Jupiters that compose a large transmission spectral survey using the Hubble and Spitzer Space Telescopes. These observations exhibit a range of spectral behavior over optical and infrared wavelengths, suggesting diverse cloud and haze properties in their atmospheres. By utilizing…

2016 The Astrophysical Journal
eHST 153
The Bright End of the z ∼ 9 and z ∼ 10 UV Luminosity Functions Using All Five CANDELS Fields*
DOI: 10.3847/0004-637X/830/2/67 Bibcode: 2016ApJ...830...67B

Trenti, M.; Oesch, P. A.; Fazio, G. G. +14 more

The deep, wide-area (∼800-900 arcmin2) near-infrared/WFC3/IR + Spitzer/IRAC observations over the CANDELS fields have been a remarkable resource for constraining the bright end of high-redshift UV luminosity functions. However, the lack of Hubble Space Telescope (HST) 1.05 µm observations over the CANDELS fields has made it diffic…

2016 The Astrophysical Journal
eHST 152