Search Publications

3D stellar reddening map from 2MASS photometry: An improved version
DOI: 10.1134/S1063773717070039 Bibcode: 2017AstL...43..472G

Gontcharov, G. A.

An improved version of the 3D stellar reddening map in a space with a radius of 1200 pc around the Sun and within 600 pc of the Galactic midplane is presented. As in the previous 2010 and 2012 versions of the map, photometry with an accuracy better than 0.05 m in the J and Ks bands for more than 70 million stars from the 2MASS catalogu…

2017 Astronomy Letters
Gaia 48
Cosmological constraints on the neutrino mass including systematic uncertainties
DOI: 10.1051/0004-6361/201730927 Bibcode: 2017A&A...606A.104C

Couchot, F.; Henrot-Versillé, S.; Perdereau, O. +4 more

When combining cosmological and oscillations results to constrain the neutrino sector, the question of the propagation of systematic uncertainties is often raised. We address this issue in the context of the derivation of an upper bound on the sum of the neutrino masses (Σmν) with recent cosmological data. This work is performed within …

2017 Astronomy and Astrophysics
Planck 48
Powerful H2 Line Cooling in Stephan’s Quintet. II. Group-wide Gas and Shock Modeling of the Warm H2 and a Comparison with [C II] 157.7 µm Emission and Kinematics
DOI: 10.3847/1538-4357/836/1/76 Bibcode: 2017ApJ...836...76A

Boulanger, F.; Appleton, P. N.; Xu, C. K. +7 more

We map for the first time the two-dimensional H2 excitation of warm intergalactic gas in Stephan's Quintet on group-wide (50 × 35 kpc2) scales to quantify the temperature, mass, and warm H2 mass fraction as a function of position using Spitzer. Molecular gas temperatures are seen to rise (to T > 700 K) and the s…

2017 The Astrophysical Journal
Herschel eHST 48
A Probabilistic Approach to Fitting Period-luminosity Relations and Validating Gaia Parallaxes
DOI: 10.3847/1538-4357/aa643b Bibcode: 2017ApJ...838..107S

Rix, Hans-Walter; Fouesneau, Morgan; Price-Whelan, Adrian M. +3 more

Pulsating stars, such as Cepheids, Miras, and RR Lyrae stars, are important distance indicators and calibrators of the “cosmic distance ladder,” and yet their period-luminosity-metallicity (PLZ) relations are still constrained using simple statistical methods that cannot take full advantage of available data. To enable optimal usage of data provid…

2017 The Astrophysical Journal
Gaia 48
No hydrogen exosphere detected around the super-Earth HD 97658 b
DOI: 10.1051/0004-6361/201629253 Bibcode: 2017A&A...597A..26B

Ehrenreich, D.; Lecavelier des Etangs, A.; Udry, S. +5 more

The exoplanet HD 97658 b provides a rare opportunity to probe the atmospheric composition and evolution of moderately irradiated super-Earths. It transits a bright K star at a moderate orbital distance of 0.08 au. Its low density is compatible with a massive steam envelope that could photodissociate at high altitudes and become observable as escap…

2017 Astronomy and Astrophysics
XMM-Newton eHST 48
Super-Eddington QSO RX J0439.6-5311 - I. Origin of the soft X-ray excess and structure of the inner accretion flow
DOI: 10.1093/mnras/stx718 Bibcode: 2017MNRAS.468.3663J

Done, Chris; Ward, Martin; Jin, Chichuan

We report the results from a recent 133 ks XMM-Newton observation of a highly super-Eddington narrow-line Type-1 quasi-stellar object RX J0439.6-5311. This source has one of the steepest active galactic nuclei hard X-ray slopes, in addition to a prominent and smooth soft X-ray excess. Strong variations are found throughout the 0.3-10 keV energy ra…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 48
Challenging Some Contemporary Views of Coronal Mass Ejections. II. The Case for Absent Filaments
DOI: 10.3847/1538-4357/834/1/86 Bibcode: 2017ApJ...834...86H

DeForest, C. E.; Howard, T. A.; Schneck, U. G. +1 more

When a coronal mass ejection (CME) appears in a coronagraph it often exhibits three parts. This “classic” three-part configuration consists of a bright leading edge, a dark circular- or teardrop-shaped cavity, and a bright core within the cavity. It is generally accepted that these are manifestations of coronal plasma pileup, the driving magnetic …

2017 The Astrophysical Journal
SOHO 48
Calibrating the Planck cluster mass scale with CLASH
DOI: 10.1051/0004-6361/201629971 Bibcode: 2017A&A...604A..89P

Bartlett, J. G.; Evrard, A. E.; Rykoff, E. +5 more

We determine the mass scale of Planck galaxy clusters using gravitational lensing mass measurements from the Cluster Lensing And Supernova survey with Hubble (CLASH). We have compared the lensing masses to the Planck Sunyaev-Zeldovich (SZ) mass proxy for 21 clusters in common, employing a Bayesian analysis to simultaneously fit an idealized CLASH …

2017 Astronomy and Astrophysics
Planck eHST 47
The Grism Lens-amplified Survey from Space (Glass). IX. The Dual Origin of Low-mass Cluster Galaxies as Revealed by New Structural Analyses
DOI: 10.3847/1538-4357/835/2/254 Bibcode: 2017ApJ...835..254M

Schmidt, Kasper B.; Treu, Tommaso; Bradač, Maruša +10 more

Using deep Hubble Frontier Fields imaging and slitless spectroscopy from the Grism Survey from Space, we study 2200 cluster and 1748 field galaxies at 0.2≤slant z≤slant 0.7 to determine the impact of environment on galaxy size and structure at stellar masses {log}{M}* /{M}> 7.8, an unprecedented limit at these redshifts.…

2017 The Astrophysical Journal
eHST 47
Instrumental response model and detrending for the Dark Energy Camera
DOI: 10.1088/1538-3873/aa858e Bibcode: 2017PASP..129k4502B

Abbott, T. M. C.; Desai, S.; Gruen, D. +12 more

We describe the model for mapping from sky brightness to the digital output of the Dark Energy Camera (DECam) and the algorithms adopted by the Dark Energy Survey (DES) for inverting this model to obtain photometric measures of celestial objects from the raw camera output. This calibration aims for fluxes that are uniform across the camera field o…

2017 Publications of the Astronomical Society of the Pacific
Gaia 47