Search Publications

Selection of the InSight Landing Site
DOI: 10.1007/s11214-016-0321-9 Bibcode: 2017SSRv..211....5G

Golombek, M.; Charalambous, C.; Piqueux, S. +32 more

The selection of the Discovery Program InSight landing site took over four years from initial identification of possible areas that met engineering constraints, to downselection via targeted data from orbiters (especially Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and High-Resolution Imaging Science Experiment (HiRISE) images), to sele…

2017 Space Science Reviews
MEx 124
Stellar inventory of the solar neighbourhood using Gaia DR1
DOI: 10.1093/mnras/stx1277 Bibcode: 2017MNRAS.470.1360B

Bovy, Jo

The absolute number and the density profiles of different types of stars in the solar neighbourhood are a fundamental anchor for studies of the initial mass function, stellar evolution, and Galactic structure. Using data from Gaia DR1, we reconstruct Gaia's selection function and determine Gaia's volume completeness, the local number density, and …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 123
Placing the Spotted T Tauri Star LkCa 4 on an HR Diagram
DOI: 10.3847/1538-4357/836/2/200 Bibcode: 2017ApJ...836..200G

Herczeg, Gregory J.; Jose, Jessy; Liu, Chun-Fan +12 more

Ages and masses of young stars are often estimated by comparing their luminosities and effective temperatures to pre-main-sequence stellar evolution tracks, but magnetic fields and starspots complicate both the observations and evolution. To understand their influence, we study the heavily spotted weak-lined T-Tauri star LkCa 4 by searching for sp…

2017 The Astrophysical Journal
Gaia INTEGRAL 122
Calibrating Star Formation in WISE Using Total Infrared Luminosity
DOI: 10.3847/1538-4357/aa92c7 Bibcode: 2017ApJ...850...68C

Dale, D. A.; Smith, J. -D. T.; Brown, M. J. I. +3 more

We present accurate resolved WISE photometry of galaxies in the combined SINGS and KINGFISH sample. The luminosities in the W3 12 µm and W4 23 µm bands are calibrated to star formation rates (SFRs) derived using the total infrared luminosity, avoiding UV/optical uncertainties due to dust extinction corrections. The W3 relation has a 1σ…

2017 The Astrophysical Journal
Herschel 122
z ∼ 2: An Epoch of Disk Assembly
DOI: 10.3847/1538-4357/aa740c Bibcode: 2017ApJ...843...46S

Trump, Jonathan R.; Weiner, Benjamin J.; Pacifici, Camilla +8 more

We explore the evolution of the internal gas kinematics of star-forming galaxies from the peak of cosmic star formation at z∼ 2 to today. Measurements of galaxy rotation velocity V rot, which quantify ordered motions, and gas velocity dispersion {σ }g, which quantify disordered motions, are adopted from the DEEP2 and SIGMA su…

2017 The Astrophysical Journal
eHST 122
The global meter-level shape model of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201731798 Bibcode: 2017A&A...607L...1P

Jorda, L.; Lara, L. M.; Bertaux, J. -L. +42 more

We performed a stereo-photogrammetric (SPG) analysis of more than 1500 Rosetta/OSIRIS NAC images of comet 67P/Churyumov-Gerasimenko (67P). The images with pixel scales in the range 0.2-3.0 m/pixel were acquired between August 2014 and February 2016. We finally derived a global high-resolution 3D description of 67P's surface, the SPG SHAP7 shape mo…

2017 Astronomy and Astrophysics
Rosetta 121
Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries
DOI: 10.1007/s11214-017-0340-1 Bibcode: 2017SSRv..212...59M

Fürst, Felix; Kretschmar, Peter; Wilms, Jörn +13 more

Massive stars, at least ∼10 times more massive than the Sun, have two key properties that make them the main drivers of evolution of star clusters, galaxies, and the Universe as a whole. On the one hand, the outer layers of massive stars are so hot that they produce most of the ionizing ultraviolet radiation of galaxies; in fact, the first massive…

2017 Space Science Reviews
INTEGRAL XMM-Newton 121
X-Ray Brightening and UV Fading of Tidal Disruption Event ASASSN-15oi
DOI: 10.3847/2041-8213/aaa0c2 Bibcode: 2017ApJ...851L..47G

Cenko, S. B.; Arcavi, I.; Gezari, S.

We present late-time observations by Swift and XMM-Newton of the tidal disruption event (TDE) ASASSN-15oi that reveal that the source brightened in the X-rays by a factor of ∼10 one year after its discovery, while it faded in the UV/optical by a factor of ∼100. The XMM-Newton observations measure a soft X-ray blackbody component with {{kT}}{b…

2017 The Astrophysical Journal
XMM-Newton 121
iPTF Discovery of the Rapid “Turn-on” of a Luminous Quasar
DOI: 10.3847/1538-4357/835/2/144 Bibcode: 2017ApJ...835..144G

Cenko, S. B.; Kulkarni, S. R.; Nugent, P. E. +13 more

We present a radio-quiet quasar at z = 0.237 discovered “turning on” by the intermediate Palomar Transient Factory (iPTF). The transient, iPTF 16bco, was detected by iPTF in the nucleus of a galaxy with an archival Sloan Digital Sky Survey spectrum with weak narrow-line emission characteristic of a low-ionization nuclear emission-line region (LINE…

2017 The Astrophysical Journal
XMM-Newton 121
Evidence for interacting dark energy from BOSS
DOI: 10.1103/PhysRevD.95.043520 Bibcode: 2017PhRvD..95d3520F

Ferreira, Elisa G. M.; Quintin, Jerome; Costa, André A. +2 more

The result presented by the BOSS-SDSS Collaboration measuring the baryon acoustic oscillations of the Lyman-alpha forest from high-redshift quasars indicates a 2.5 σ departure from the standard Λ -cold-dark-matter model. This is the first time that the evolution of dark energy at high redshifts has been measured, and the current results cannot be …

2017 Physical Review D
Planck 121