Search Publications

The selection function of the RAVE survey
DOI: 10.1093/mnras/stx606 Bibcode: 2017MNRAS.468.3368W

Grebel, Eva K.; Steinmetz, Matthias; Bland-Hawthorn, Joss +23 more

We characterize the selection function of RAdial Velocity Experiment (RAVE) using 2 Micron All Sky Survey (2MASS) as our underlying population, which we assume represents all stars that could have potentially been observed. We evaluate the completeness fraction as a function of position, magnitude and colour in two ways: first, on a field-by-field…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 37
The age of 47 Tuc from self-consistent isochrone fits to colour-magnitude diagrams and the eclipsing member V69
DOI: 10.1093/mnras/stx378 Bibcode: 2017MNRAS.468..645B

Grundahl, F.; Milone, A. P.; Bedin, L. R. +3 more

Our aim is to derive a self-consistent age, distance and composition for the globular cluster 47 Tucanae (47 Tuc; NGC104). First, we re-evaluate the reddening towards the cluster resulting in a nominal E(B - V) = 0.03 ± 0.01 as the best estimate. The Teff of the components of the eclipsing binary member V69 is found to be 5900 ± 72 K fr…

2017 Monthly Notices of the Royal Astronomical Society
eHST 37
Ultraviolet C II and Si III Transit Spectroscopy and Modeling of the Evaporating Atmosphere of GJ436b
DOI: 10.3847/2041-8213/834/2/L17 Bibcode: 2017ApJ...834L..17L

Loyd, R. O. Parke; Redfield, Seth; France, Kevin +2 more

Hydrogen gas evaporating from the atmosphere of the hot-Neptune GJ436b absorbs over 50% of the stellar Lyα emission during transit. Given the planet’s atmospheric composition and energy-limited escape rate, this hydrogen outflow is expected to entrain heavier atoms such as C and O. We searched for C and Si in the escaping atmosphere of GJ436b usin…

2017 The Astrophysical Journal
eHST 37
The ISLAnds Project. III. Variable Stars in Six Andromeda Dwarf Spheroidal Galaxies
DOI: 10.3847/1538-4357/aa9381 Bibcode: 2017ApJ...850..137M

McQuinn, Kristen B. W.; Dolphin, Andrew E.; Skillman, Evan D. +15 more

We present a census of variable stars in six M31 dwarf spheroidal satellites observed with the Hubble Space Telescope. We detect 870 RR Lyrae (RRL) stars in the fields of And I (296), II (251), III (111), XV (117), XVI (8), and XXVIII (87). We also detect a total of 15 Anomalous Cepheids, three eclipsing binaries, and seven field RRL stars compati…

2017 The Astrophysical Journal
eHST 37
CMB signatures of metal-free star formation and Planck 2015 polarization data
DOI: 10.1093/mnras/stx306 Bibcode: 2017MNRAS.467.4050M

Heinrich, Chen He; Miranda, Vinicius; Hu, Wayne +1 more

Standard analyses of the reionization history of the Universe from Planck cosmic microwave background (CMB) polarization measurements consider only the overall optical depth to electron scattering (τ), and further assume a step-like reionization history. However, the polarization data contain information beyond the overall optical depth, and the a…

2017 Monthly Notices of the Royal Astronomical Society
Planck 37
Inflation model selection meets dark radiation
DOI: 10.1088/1475-7516/2017/01/046 Bibcode: 2017JCAP...01..046T

Tram, Thomas; Vennin, Vincent; Vallance, Robert

We investigate how inflation model selection is affected by the presence of additional free-streaming relativistic degrees of freedom, i.e. dark radiation. We perform a full Bayesian analysis of both inflation parameters and cosmological parameters taking reheating into account self-consistently. We compute the Bayesian evidence for a few represen…

2017 Journal of Cosmology and Astroparticle Physics
Planck 37
MC2: Multiwavelength and Dynamical Analysis of the Merging Galaxy Cluster ZwCl 0008.8+5215: An Older and Less Massive Bullet Cluster
DOI: 10.3847/1538-4357/aa667f Bibcode: 2017ApJ...838..110G

Dawson, William A.; Jee, M. James; van Weeren, Reinout J. +2 more

We present and analyze a rich data set including Subaru/SuprimeCam, HST/Advanced Camera for Surveys and Wide Field Camera 3, Keck/DEIMOS, Chandra/ACIS-I, and JVLA/C and D array for the merging cluster of galaxies ZwCl 0008.8+5215. With a joint Subaru+HST weak gravitational lensing analysis, we identify two dominant subclusters and estimate the mas…

2017 The Astrophysical Journal
eHST 37
Constraining the ΛCDM and Galileon models with recent cosmological data
DOI: 10.1051/0004-6361/201628878 Bibcode: 2017A&A...600A..40N

Möller, A.; Astier, P.; Guy, J. +4 more


Aims: The Galileon theory belongs to the class of modified gravity models that can explain the late-time accelerated expansion of the Universe. In previous works, cosmological constraints on the Galileon model were derived, both in the uncoupled case and with a disformal coupling of the Galileon field to matter. There, we showed that these mo…

2017 Astronomy and Astrophysics
Planck 37
IRIS Burst Spectra Co-spatial to a Quiet-Sun Ellerman-like Brightening
DOI: 10.3847/1538-4357/aa7e7a Bibcode: 2017ApJ...845...16N

Erdélyi, R.; Mathioudakis, M.; Oliver, R. +3 more

Ellerman bombs (EBs) have been widely studied over the past two decades; however, only recently have the counterparts of these events been observed in the quiet-Sun. The aim of this article is to further understand small-scale quiet-Sun Ellerman-like brightenings (QSEBs) through research into their spectral signatures, including investigating whet…

2017 The Astrophysical Journal
IRIS 37
Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance
DOI: 10.1051/0004-6361/201629666 Bibcode: 2017A&A...599A..34R

Adam, R.; Benoît, A.; Catalano, A. +37 more

Magnetic fields, which play a major role in a large number of astrophysical processes can be traced via observations of dust polarization. In particular, Planck low-resolution observations of dust polarization have demonstrated that Galactic filamentary structures, where star formation takes place, are associated to well organized magnetic fields.…

2017 Astronomy and Astrophysics
Planck 37