Search Publications

A long-term study of AGN X-ray variability . Structure function analysis on a ROSAT-XMM quasar sample
DOI: 10.1051/0004-6361/201629940 Bibcode: 2017A&A...599A..82M

Bianchi, S.; Paolillo, M.; Middei, R. +3 more

Context. Variability in the X-rays is a key ingredient in understanding and unveiling active galactic nuclei (AGN) properties. In this band, flux variations occur on short timescales (hours) as well as on larger timescales. While short timescale variability is often investigated in single source studies, only a few works are able to explore flux v…

2017 Astronomy and Astrophysics
XMM-Newton 47
Ionized Gas Outflows in Infrared-bright Dust-obscured Galaxies Selected with WISE and SDSS
DOI: 10.3847/1538-4357/aa918a Bibcode: 2017ApJ...850..140T

Toba, Yoshiki; Nagao, Tohru; Wang, Wei-Hao +5 more

We present the ionized gas properties of infrared (IR)-bright dust-obscured galaxies (DOGs) that show an extreme optical/IR color, {(i-[22])}{AB}> 7.0, selected with the Sloan Digital Sky Survey (SDSS) and Wide-field Infrared Survey Explorer (WISE). For 36 IR-bright DOGs that show [O III]λ5007 emission in the SDSS spectra, we perform…

2017 The Astrophysical Journal
AKARI 47
A detection of wobbling brightest cluster galaxies within massive galaxy clusters
DOI: 10.1093/mnras/stx2084 Bibcode: 2017MNRAS.472.1972H

Kneib, J. P.; Harvey, David; Courbin, F. +1 more

A striking signal of dark matter beyond the standard model is the existence of cores in the centre of galaxy clusters. Recent simulations predict that a brightest cluster galaxy (BCG) inside a cored galaxy cluster will exhibit residual wobbling due to previous major mergers, long after the relaxation of the overall cluster. This phenomenon is abse…

2017 Monthly Notices of the Royal Astronomical Society
eHST 47
Testing giant planet formation in the transitional disk of SAO 206462 using deep VLT/SPHERE imaging
DOI: 10.1051/0004-6361/201629896 Bibcode: 2017A&A...601A.134M

Quanz, S. P.; Henning, T.; Ginski, C. +42 more

Context. The SAO 206462 (HD 135344B) disk is one of the few known transitional disks showing asymmetric features in scattered light and thermal emission. Near-infrared scattered-light images revealed two bright outer spiral arms and an inner cavity depleted in dust. Giant protoplanets have been proposed to account for the disk morphology.
Aim…

2017 Astronomy and Astrophysics
Gaia eHST 47
First Results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics of Lensed Galaxies at Cosmic Noon
DOI: 10.3847/1538-4357/aa60c4 Bibcode: 2017ApJ...838...14M

Fontana, Adriano; Schmidt, Kasper B.; Treu, Tommaso +12 more

We present the first results of the K-band Multi-Object Spectrometer (KMOS) Lens-Amplified Spectroscopic Survey, a new ESO Very Large Telescope large program, doing multi-object integral field spectroscopy of galaxies gravitationally lensed behind seven galaxy clusters selected from the Hubble Space Telescope (HST) Grism Lens-Amplified Survey from…

2017 The Astrophysical Journal
eHST 47
A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling
DOI: 10.1016/j.physletb.2017.10.052 Bibcode: 2017PhLB..775..239G

Mena, Olga; Gerbino, Martina; Lattanzi, Massimiliano +1 more

We present a novel approach to derive constraints on neutrino masses, as well as on other cosmological parameters, from cosmological data, while taking into account our ignorance of the neutrino mass ordering. We derive constraints from a combination of current as well as future cosmological datasets on the total neutrino mass Mν and on…

2017 Physics Letters B
Planck 47
MASCARA-1 b. A hot Jupiter transiting a bright mV = 8.3 A-star in a misaligned orbit
DOI: 10.1051/0004-6361/201731282 Bibcode: 2017A&A...606A..73T

Snellen, I. A. G.; Grundahl, F.; Albrecht, S. +11 more

We report the discovery of MASCARA-1 b, which is the first exoplanet discovered with the Multi-site All-Sky CAmeRA (MASCARA). This exoplanet is a hot Jupiter orbiting a bright mV = 8.3, rapidly rotating (vsini > 100 km s-1) A8 star with a period of 2.148780 ± 8 × 10-6 days. The planet has a mass and …

2017 Astronomy and Astrophysics
Gaia 47
The Clouds are breaking: tracing the Magellanic system with Gaia DR1 Mira variables
DOI: 10.1093/mnras/stx263 Bibcode: 2017MNRAS.467.2636D

Erkal, Denis; Belokurov, Vasily; Mackey, Dougal +2 more

We exploit the first data release from the Gaia mission to identify candidate Mira variables in the outskirts of the Magellanic Clouds. The repeated observations of sources during the initial phase of the Gaia mission is used to identify stars that show signs of variability. This variability information, combined with infrared photometry from Two …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 47
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications
DOI: 10.1093/mnras/stx633 Bibcode: 2017MNRAS.468.2938S

Brownstein, Joel R.; Thomas, Daniel; Prada, Francisco +17 more

We investigate the cosmological implications of studying galaxy clustering using a tomographic approach applied to the final Baryon Oscillation Spectroscopic Survey (BOSS) DR12 galaxy sample, including both auto- and cross-correlation functions between redshift shells. We model the signal of the full shape of the angular correlation function, ω(θ)…

2017 Monthly Notices of the Royal Astronomical Society
Planck 47
Complete reionization constraints from Planck 2015 polarization
DOI: 10.1103/PhysRevD.95.023513 Bibcode: 2017PhRvD..95b3513H

Heinrich, Chen He; Miranda, Vinicius; Hu, Wayne

We conduct an analysis of the Planck 2015 data that is complete in reionization observables from the large angle polarization E -mode spectrum in the redshift range 6 <z <30 . Based on 5 principal components, all of which are constrained by the data, this single analysis can be used to infer constraints on any model for reionization in the s…

2017 Physical Review D
Planck 47