Search Publications

Updated constraints and forecasts on primordial tensor modes
DOI: 10.1103/PhysRevD.93.063508 Bibcode: 2016PhRvD..93f3508C

Melchiorri, Alessandro; Cabass, Giovanni; Gerbino, Martina +3 more

We present new, tight, constraints on the cosmological background of gravitational waves (GWs) using the latest measurements of CMB temperature and polarization anisotropies provided by the Planck, BICEP2 and Keck Array experiments. These constraints are further improved when the GW contribution NeffGW to the effective number…

2016 Physical Review D
Planck 70
A free-form prediction for the reappearance of supernova Refsdal in the Hubble Frontier Fields cluster MACSJ1149.5+2223
DOI: 10.1093/mnras/stv2638 Bibcode: 2016MNRAS.456..356D

Broadhurst, Tom; Zheng, Wei; Zitrin, Adi +7 more

The massive cluster MACSJ1149.5+2223(z = 0.544) displays five very large lensed images of a well-resolved spiral galaxy at zspect = 1.491. It is within one of these images that the first example of a multiply lensed supernova (SN) has been detected recently as part of the Grism Lens-Amplified Survey from Space. The depth of this data al…

2016 Monthly Notices of the Royal Astronomical Society
eHST 70
A package for the automated classification of periodic variable stars
DOI: 10.1051/0004-6361/201527188 Bibcode: 2016A&A...587A..18K

Bailer-Jones, Coryn A. L.; Kim, Dae-Won

We present a machine learning package for the classification of periodic variable stars. Our package is intended to be general: it can classify any single band optical light curve comprising at least a few tens of observations covering durations from weeks to years with arbitrary time sampling. We use light curves of periodic variable stars taken …

2016 Astronomy and Astrophysics
Hipparcos 70
The plasma structure of coronal hole solar wind: Origins and evolution
DOI: 10.1002/2016JA022686 Bibcode: 2016JGRA..121.5055B

Borovsky, Joseph E.

Whereas slow solar wind is known to be highly structured, the fast (coronal hole origin) wind is usually considered to be homogeneous. Using measurements from Helios 1 + 2, ACE, Wind, and Ulysses, structure in the coronal hole origin solar wind is examined from 0.3 AU to 2.3 AU. Care is taken to collect and analyze intervals of "unperturbed corona…

2016 Journal of Geophysical Research (Space Physics)
Ulysses 70
Fission and reconfiguration of bilobate comets as revealed by 67P/Churyumov-Gerasimenko
DOI: 10.1038/nature17670 Bibcode: 2016Natur.534..352H

Mottola, Stefano; Steckloff, Jordan; Naidu, Shantanu P. +6 more

The solid, central part of a comet—its nucleus—is subject to destructive processes, which cause nuclei to split at a rate of about 0.01 per year per comet. These destructive events are due to a range of possible thermophysical effects; however, the geophysical expressions of these effects are unknown. Separately, over two-thirds of comet nuclei th…

2016 Nature
Rosetta 70
Tracing outflows in the AGN forbidden region with SINFONI
DOI: 10.1051/0004-6361/201527968 Bibcode: 2016A&A...592A.148K

Piconcelli, E.; Brusa, M.; Mainieri, V. +8 more

Context. Active galactic nucleus (AGN) driven outflows are invoked in numerical simulations to reproduce several observed properties of local galaxies. The z > 1 epoch is of particular interest as it was during this time that the volume averaged star formation and the accretion rate of black holes were at their maximum. Radiatively driven outfl…

2016 Astronomy and Astrophysics
eHST 70
HST Hot-Jupiter Transmission Spectral Survey: Clear Skies for Cool Saturn WASP-39b
DOI: 10.3847/0004-637X/827/1/19 Bibcode: 2016ApJ...827...19F

Deming, Drake; Nikolov, Nikolay; Fortney, Jonathan J. +13 more

We present the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) optical transmission spectroscopy of the cool Saturn-mass exoplanet WASP-39b from 0.29-1.025 µm, along with complementary transit observations from Spitzer IRAC at 3.6 and 4.5 µm. The low density and large atmospheric pressure scale height of WASP-3…

2016 The Astrophysical Journal
eHST 69
The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-to-Earth Analysis
DOI: 10.3847/0004-637X/817/1/14 Bibcode: 2016ApJ...817...14P

Gontikakis, C.; Patsourakos, S.; Tsinganos, K. +33 more

During the interval 2012 March 7-11 the geospace experienced a barrage of intense space weather phenomena including the second largest geomagnetic storm of solar cycle 24 so far. Significant ultra-low-frequency wave enhancements and relativistic-electron dropouts in the radiation belts, as well as strong energetic-electron injection events in the …

2016 The Astrophysical Journal
SOHO 69
The Evolution of the Intracluster Medium Metallicity in Sunyaev Zel’dovich-selected Galaxy Clusters at 0 < z < 1.5
DOI: 10.3847/0004-637X/826/2/124 Bibcode: 2016ApJ...826..124M

Hlavacek-Larrondo, J.; Bleem, L. E.; Stalder, B. +16 more

We present the results of an X-ray spectral analysis of 153 galaxy clusters observed with the Chandra, XMM-Newton, and Suzaku space telescopes. These clusters, which span 0 < z < 1.5, were drawn from a larger, mass-selected sample of galaxy clusters discovered in the 2500 square degree South Pole Telescope Sunyaev Zel’dovich (SPT-SZ) survey.…

2016 The Astrophysical Journal
Suzaku XMM-Newton 69
The Relationship Between Molecular Gas, H I, and Star Formation in the Low-mass, Low-metallicity Magellanic Clouds
DOI: 10.3847/0004-637X/825/1/12 Bibcode: 2016ApJ...825...12J

Bot, Caroline; Bolatto, Alberto D.; Leroy, Adam K. +14 more

The Magellanic Clouds provide the only laboratory to study the effects of metallicity and galaxy mass on molecular gas and star formation at high (∼⃒20 pc) resolution. We use the dust emission from HERITAGE Herschel data to map the molecular gas in the Magellanic Clouds, avoiding the known biases of CO emission as a tracer of {{{H}}}2. U…

2016 The Astrophysical Journal
Herschel 69