Search Publications

WFIRST Exoplanet Mass-measurement Method Finds a Planetary Mass of 39 ± 8 M for OGLE-2012-BLG-0950Lb
DOI: 10.3847/1538-3881/aaed46 Bibcode: 2018AJ....156..289B

Bennett, D. P.; Udalski, A.; Anderson, J. +13 more

We present the analysis of the simultaneous high-resolution images from the Hubble Space Telescope and Keck adaptive optics system of the planetary event OGLE-2012-BLG-0950 that determine that the system consists of a 0.58 ± 0.04 {M} host star orbited by a 39 ± 8 {M}\oplus planet at a projected separation of 2.54 ± 0.23 au…

2018 The Astronomical Journal
eHST 78
X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field
DOI: 10.3847/1538-4365/aab9b4 Bibcode: 2018ApJS..236...48K

Papovich, Casey; Kocevski, Dale D.; Koekemoer, Anton M. +25 more

We present the X-UDS survey, a set of wide and deep Chandra observations of the Subaru-XMM Deep/UKIDSS Ultra Deep Survey (SXDS/UDS) field. The survey consists of 25 observations that cover a total area of 0.33 deg2. The observations are combined to provide a nominal depth of ∼600 ks in the central 100 arcmin2 region of the fi…

2018 The Astrophysical Journal Supplement Series
eHST 77
Fornax3D project: Overall goals, galaxy sample, MUSE data analysis, and initial results
DOI: 10.1051/0004-6361/201833137 Bibcode: 2018A&A...616A.121S

de Zeeuw, P. T.; McDermid, R. M.; Falcón-Barroso, J. +10 more

The Fornax cluster provides a uniquely compact laboratory in which to study the detailed history of early-type galaxies and the role played by the environment in driving their evolution and their transformation from late-type galaxies. Using the superb capabilities of the Multi Unit Spectroscopic Explorer on the Very Large Telescope, high-quality …

2018 Astronomy and Astrophysics
eHST 77
The origin of interstellar asteroidal objects like 1I/2017 U1 `Oumuamua
DOI: 10.1093/mnrasl/sly088 Bibcode: 2018MNRAS.479L..17P

Torres, Santiago; Portegies Zwart, Simon; Bédorf, Jeroen +2 more

We study the origin of the interstellar object 1I/2017 U1 `Oumuamua by juxtaposing estimates based on the observations with simulations. We speculate that objects like `Oumuamua are formed in the debris disc as left over from the star and planet formation process, and subsequently liberated. The liberation process is mediated either by interaction…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 77
Compressible Magnetohydrodynamic Turbulence in the Earth's Magnetosheath: Estimation of the Energy Cascade Rate Using in situ Spacecraft Data
DOI: 10.1103/PhysRevLett.120.055102 Bibcode: 2018PhRvL.120e5102H

Sahraoui, F.; Huang, S. Y.; Hadid, L. Z. +1 more

The first estimation of the energy cascade rate |ɛC| of magnetosheath turbulence is obtained using the Cluster and THEMIS spacecraft data and an exact law of compressible isothermal magnetohydrodynamics turbulence. The mean value of |ɛC| is found to be close to 10-13 J m-3 s-1 , at least 2 ord…

2018 Physical Review Letters
Cluster 77
Time-resolved WISE/NEOWISE Coadds
DOI: 10.3847/1538-3881/aacbcd Bibcode: 2018AJ....156...69M

Lang, D.; Meisner, A. M.; Schlegel, D. J.

We have used the first ∼3 years of 3.4 µm (W1) and 4.6 µm (W2) observations from the WISE and NEOWISE missions to create a full-sky set of time-resolved coadds. As a result of the WISE survey strategy, a typical sky location is visited every six months and is observed during ≳12 exposures per visit, with these exposures spanning a ∼1 d…

2018 The Astronomical Journal
Gaia 77
Structure of photodissociation fronts in star-forming regions revealed by Herschel observations of high-J CO emission lines
DOI: 10.1051/0004-6361/201832611 Bibcode: 2018A&A...615A.129J

Le Bourlot, J.; Le Petit, F.; Pinto, C. +17 more

Context. In bright photodissociation regions (PDR) associated with massive star formation, the presence of dense "clumps" that are immersed in a less dense interclump medium is often proposed to explain the difficulty of models to account for the observed gas emission in high-excitation lines.
Aims: We aim to present a comprehensive view of t…

2018 Astronomy and Astrophysics
Herschel 77
Retrieval of exoplanet emission spectra with HyDRA
DOI: 10.1093/mnras/stx2748 Bibcode: 2018MNRAS.474..271G

Madhusudhan, Nikku; Gandhi, Siddharth

Thermal emission spectra of exoplanets provide constraints on the chemical compositions, pressure-temperature (P-T) profiles, and energy transport in exoplanetary atmospheres. Accurate inferences of these properties rely on the robustness of the atmospheric retrieval methods employed. While extant retrieval codes have provided significant constrai…

2018 Monthly Notices of the Royal Astronomical Society
eHST 77
MIKiS: The Multi-instrument Kinematic Survey of Galactic Globular Clusters. I. Velocity Dispersion Profiles and Rotation Signals of 11 Globular Clusters
DOI: 10.3847/1538-4357/aabe2f Bibcode: 2018ApJ...860...50F

Dalessandro, E.; Valenti, E.; Bellazzini, M. +10 more

We present the first results of the Multi-Instrument Kinematic Survey of Galactic Globular Clusters (GGCs), a project aimed at exploring the internal kinematics of a representative sample of GGCs from the radial velocity of individual stars, covering the entire radial extension of each system. This is achieved by exploiting the formidable combinat…

2018 The Astrophysical Journal
eHST 76
Fourteen candidate RR Lyrae star streams in the inner Galaxy
DOI: 10.1093/mnras/stx2937 Bibcode: 2018MNRAS.474.4112M

Kawata, Daisuke; Mateu, Cecilia; Read, Justin I.

We apply the GC3 stream-finding method to RR Lyrae stars (RRLSs) in the Catalina survey. We find 2 RRLS stream candidates at >4σ confidence and another 12 at >3.5σ confidence over the Galactocentric distance range 4 < D/kpc < 26. Of these, only two are associated with known globular clusters (NGC 1261 and Arp2). The remainder are candi…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 76