Search Publications

Stellar Mass-Gas-phase Metallicity Relation at 0.5 ≤ z ≤ 0.7: A Power Law with Increasing Scatter toward the Low-mass Regime
DOI: 10.3847/0004-637X/822/2/103 Bibcode: 2016ApJ...822..103G

Barro, Guillermo; Pérez-González, Pablo G.; Hathi, Nimish P. +21 more

We present the stellar mass ({M}*)-gas-phase metallicity relation (MZR) and its scatter at intermediate redshifts (0.5≤slant z≤slant 0.7) for 1381 field galaxies collected from deep spectroscopic surveys. The star formation rate (SFR) and color at a given {M}* of this magnitude-limited (R≲ 24 AB) sample are representative of …

2016 The Astrophysical Journal
eHST 41
Transition Region and Chromospheric Signatures of Impulsive Heating Events. I. Observations
DOI: 10.3847/0004-637X/829/1/35 Bibcode: 2016ApJ...829...35W

Warren, Harry P.; Crump, Nicholas A.; Reep, Jeffrey W. +1 more

We exploit the high spatial resolution and high cadence of the Interface Region Imaging Spectrograph (IRIS) to investigate the response of the transition region and chromosphere to energy deposition during a small flare. Simultaneous observations from the Reuven Ramaty High Energy Solar Spectroscopic Imager provide constraints on the energetic ele…

2016 The Astrophysical Journal
Hinode IRIS 41
Setting constraints on the nature and origin of the two major hydrous sulfates on Mars: Monohydrated and polyhydrated sulfates
DOI: 10.1002/2015JE004889 Bibcode: 2016JGRE..121..678W

Liu, Yang; Wang, Alian; Jolliff, Bradley L. +1 more

Monohydrated Mg sulfate (MgSO4·H2O) and polyhydrated sulfate are the most common and abundant hydrous sulfates observed thus far on Mars. They are widely distributed and coexist in many locations. On the basis of results from two new sets of experiments, in combination with past experimental studies and the subsurface salt mi…

2016 Journal of Geophysical Research (Planets)
MEx 41
On the red giant branch mass loss in 47 Tucanae: Constraints from the horizontal branch morphology
DOI: 10.1051/0004-6361/201628181 Bibcode: 2016A&A...590A..64S

Salaris, Maurizio; Cassisi, Santi; Pietrinferni, Adriano

We obtain stringent constraints on the actual efficiency of mass loss for red giant branch stars in the Galactic globular cluster 47 Tuc, by comparing synthetic modelling based on stellar evolution tracks with the observed distribution of stars along the horizontal branch in the colour-magnitude-diagram. We confirm that the observed, wedge-shaped …

2016 Astronomy and Astrophysics
eHST 41
High ionisation absorption in low mass X-ray binaries
DOI: 10.1002/asna.201612339 Bibcode: 2016AN....337..512P

Merloni, A.; Bianchi, S.; Ponti, G. +3 more

The advent of the new generation of X-ray telescopes yielded a significant step forward in our understanding of ionised absorption generated in the accretion discs of X-ray binaries. It has become evident that these relatively weak and narrow absorption features, sporadically present in the X-ray spectra of some systems, are actually the signature…

2016 Astronomische Nachrichten
XMM-Newton 41
The Total Solar Irradiance Climate Data Record
DOI: 10.3847/0004-637X/830/1/25 Bibcode: 2016ApJ...830...25D

Dewitte, Steven; Nevens, Stijn

We present the composite measurements of total solar irradiance (TSI) as measured by an ensemble of space instruments. The measurements of the individual instruments are put on a common absolute scale, and their quality is assessed by intercomparison. The composite time series is the average of all available measurements. From 1984 April to the pr…

2016 The Astrophysical Journal
SOHO 41
Four and one more: The formation history and total mass of globular clusters in the Fornax dSph
DOI: 10.1051/0004-6361/201527580 Bibcode: 2016A&A...590A..35D

Fraser, M.; de Boer, T. J. L.

We have determined the detailed star formation history and total mass of the globular clusters in the Fornax dwarf spheroidal using archival HST WFPC2 data. Colour-magnitude diagrams were constructed in the F555W and F814W bands and corrected for the effect of Fornax field star contamination, after which we used the routine Talos to derive the qua…

2016 Astronomy and Astrophysics
eHST 41
Testing chirality of primordial gravitational waves with Planck and future CMB data: no hope from angular power spectra
DOI: 10.1088/1475-7516/2016/07/044 Bibcode: 2016JCAP...07..044G

Melchiorri, Alessandro; Shiraishi, Maresuke; Gerbino, Martina +2 more

We use the 2015 Planck likelihood in combination with the Bicep2/Keck likelihood (BKP and BK14) to constrain the chirality, χ, of primordial gravitational waves in a scale-invariant scenario. In this framework, the parameter χ enters theory always coupled to the tensor-to-scalar ratio, r, e.g. in combination of the form χ ṡ r. Thus, the capability…

2016 Journal of Cosmology and Astroparticle Physics
Planck 41
Physical Properties of Spectroscopically Confirmed Galaxies at z ≥ 6. III. Stellar Populations from SED Modeling with Secure Lyα Emission and Redshifts
DOI: 10.3847/0004-637X/816/1/16 Bibcode: 2016ApJ...816...16J

Ouchi, Masami; Shimasaku, Kazuhiro; Fan, Xiaohui +9 more

We present a study of stellar populations in a sample of spectroscopically confirmed Lyman-break galaxies (LBGs) and Lyα emitters (LAEs) at 5.7< z< 7. These galaxies have deep images from Subaru, the Hubble Space Telescope, and Spitzer/IRAC. We focus on 27 galaxies with IRAC detections, and characterize their stellar populations based on the…

2016 The Astrophysical Journal
eHST 41
Alluvial Fan Morphology, distribution and formation on Titan
DOI: 10.1016/j.icarus.2016.02.013 Bibcode: 2016Icar..270..238B

Hayes, A. G.; Birch, S. P. D.; Radebaugh, J. +2 more

Titan is a hydrologically active world, with dozens of alluvial fans that are evidence of sediment transport from high to low elevations. However, the distribution and requirements for the formation of fans on Titan are not well understood. We performed the first global survey of alluvial fans on Titan using Cassini Synthetic Aperture Radar (SAR) …

2016 Icarus
Cassini 41