Search Publications

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Continuum Number Counts, Resolved 1.2 mm Extragalactic Background, and Properties of the Faintest Dusty Star-forming Galaxies
DOI: 10.3847/1538-4357/833/1/68 Bibcode: 2016ApJ...833...68A

Smail, I.; Magnelli, B.; Daddi, E. +31 more

We present an analysis of a deep (1σ = 13 µJy) cosmological 1.2 mm continuum map based on ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field. In the 1 arcmin2 covered by ASPECS we detect nine sources at \gt 3.5σ significance at 1.2 mm. Our ALMA-selected sample has a median redshift of z=1.6+/- 0.4, with only one …

2016 The Astrophysical Journal
Planck eHST 134
Estimating Distances from Parallaxes. II. Performance of Bayesian Distance Estimators on a Gaia-like Catalogue
DOI: 10.3847/0004-637X/832/2/137 Bibcode: 2016ApJ...832..137A

Bailer-Jones, Coryn A. L.; Astraatmadja, Tri L.

Estimating a distance by inverting a parallax is only valid in the absence of noise. As most stars in the Gaia catalog will have non-negligible fractional parallax errors, we must treat distance estimation as a constrained inference problem. Here we investigate the performance of various priors for estimating distances, using a simulated Gaia cata…

2016 The Astrophysical Journal
Gaia 133
LOFAR/H-ATLAS: a deep low-frequency survey of the Herschel-ATLAS North Galactic Pole field
DOI: 10.1093/mnras/stw1763 Bibcode: 2016MNRAS.462.1910H

Prandoni, I.; Brunetti, G.; White, G. J. +25 more

We present Low-Frequency Array (LOFAR) High-Band Array observations of the Herschel-ATLAS North Galactic Pole survey area. The survey we have carried out, consisting of four pointings covering around 142 deg2 of sky in the frequency range 126-173 MHz, does not provide uniform noise coverage but otherwise is representative of the quality…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 132
A New Distortion Solution for NIRC2 on the Keck II Telescope
DOI: 10.1088/1538-3873/128/967/095004 Bibcode: 2016PASP..128i5004S

Ghez, A. M.; Anderson, J.; Lu, J. R. +3 more

We present a new geometric distortion model for the narrow-field mode of the near-infrared camera (NIRC2) fed by the adaptive optics system on the W. M. Keck II telescope. The adaptive optics system and NIRC2 camera were realigned on 2015 April 13. Observations of the crowded globular cluster, M53, were obtained before and after the realignment to…

2016 Publications of the Astronomical Society of the Pacific
eHST 132
Planetary surface dating from crater size-frequency distribution measurements: Poisson timing analysis
DOI: 10.1016/j.icarus.2016.05.019 Bibcode: 2016Icar..277..279M

Michael, G. G.; Kneissl, T.; Neesemann, A.

The predictions of crater chronology models have customarily been evaluated by dividing a crater population into discrete diameter intervals, plotting the crater density for each, and finding a best-fit model isochron, with the uncertainty in the procedure being assessed using 1/√n estimates, where n is the number of craters in an interval. This a…

2016 Icarus
MEx 131
The discovery, monitoring and environment of SGR J1935+2154
DOI: 10.1093/mnras/stw008 Bibcode: 2016MNRAS.457.3448I

Campana, S.; Tiengo, A.; Götz, D. +13 more

We report on the discovery of a new member of the magnetar class, SGR J1935+2154, and on its timing and spectral properties measured by an extensive observational campaign carried out between 2014 July and 2015 March with Chandra and XMM-Newton (11 pointings). We discovered the spin period of SGR J1935+2154 through the detection of coherent pulsat…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 131
An evaporating planet in the wind: stellar wind interactions with the radiatively braked exosphere of GJ 436 b
DOI: 10.1051/0004-6361/201628362 Bibcode: 2016A&A...591A.121B

Vidotto, A. A.; Ehrenreich, D.; Lecavelier des Etangs, A. +2 more

Observations of the warm Neptune GJ 436 b were performed with HST/STIS at three different epochs (2012, 2013, 2014) in the stellar Lyman-α line. They showed deep, repeated transits that were attributed to a giant exosphere of neutral hydrogen. The low radiation pressure from the M-dwarf host star was shown to play a major role in the dynamics of t…

2016 Astronomy and Astrophysics
eHST 131
Enceladus's internal ocean and ice shell constrained from Cassini gravity, shape, and libration data
DOI: 10.1002/2016GL068634 Bibcode: 2016GeoRL..43.5653C

Bourgeois, Olivier; Massé, Marion; Čadek, Ondřej +8 more

The intense plume activity at the South Pole of Enceladus together with the recent detection of libration hints at an internal water ocean underneath the outer ice shell. However, the interpretation of gravity, shape, and libration data leads to contradicting results regarding the depth of ocean/ice interface and the total volume of the ocean. Her…

2016 Geophysical Research Letters
Cassini 130
Estimating Distances from Parallaxes. III. Distances of Two Million Stars in the Gaia DR1 Catalogue
DOI: 10.3847/1538-4357/833/1/119 Bibcode: 2016ApJ...833..119A

Bailer-Jones, Coryn A. L.; Astraatmadja, Tri L.

We infer distances and their asymmetric uncertainties for two million stars using the parallaxes published in the Gaia DR1 (GDR1) catalogue. We do this with two distance priors: A minimalist, isotropic prior assuming an exponentially decreasing space density with increasing distance, and an anisotropic prior derived from the observability of stars…

2016 The Astrophysical Journal
Gaia 130
Gamma-ray spectroscopy of positron annihilation in the Milky Way
DOI: 10.1051/0004-6361/201527510 Bibcode: 2016A&A...586A..84S

Diehl, Roland; Greiner, Jochen; Siegert, Thomas +5 more

Context. The annihilation of positrons in the Galaxy's interstellar medium produces characteristic gamma-rays with a line at 511 keV. This gamma-ray emission has been observed with the spectrometer SPI on ESA's INTEGRAL observatory, confirming a puzzling morphology with bright emission from an extended bulge-like region, while emission from the di…

2016 Astronomy and Astrophysics
INTEGRAL 130