Search Publications

Radial distribution of dust, stars, gas, and star-formation rate in DustPedia face-on galaxies
DOI: 10.1051/0004-6361/201731020 Bibcode: 2017A&A...605A..18C

Bianchi, S.; Fritz, J.; Madden, S. C. +18 more


Aims: The purpose of this work is the characterization of the radial distribution of dust, stars, gas, and star-formation rate (SFR) in a sub-sample of 18 face-on spiral galaxies extracted from the DustPedia sample.
Methods: This study is performed by exploiting the multi-wavelength DustPedia database, from ultraviolet (UV) to sub-millim…

2017 Astronomy and Astrophysics
Herschel 111
Interacting neutrinos in cosmology: exact description and constraints
DOI: 10.1088/1475-7516/2017/11/027 Bibcode: 2017JCAP...11..027O

Tram, Thomas; Wong, Yvonne Y. Y.; Oldengott, Isabel M. +1 more

We consider the impact of neutrino self-interactions described by an effective four-fermion coupling on cosmological observations. Implementing the exact Boltzmann hierarchy for interacting neutrinos first derived in [1] into the Boltzmann solver CLASS, we perform a detailed numerical analysis of the effects of the interaction on the cosmic microw…

2017 Journal of Cosmology and Astroparticle Physics
Planck 111
The VMC survey - XXV. The 3D structure of the Small Magellanic Cloud from Classical Cepheids
DOI: 10.1093/mnras/stx2096 Bibcode: 2017MNRAS.472..808R

Piatti, Andrés E.; de Grijs, Richard; Marconi, Marcella +13 more

The VISTA near-infrared YJKs survey of the Magellanic System (VMC) is collecting deep Ks-band time-series photometry of pulsating stars hosted by the two Magellanic Clouds and their connecting bridge. Here, we present Y, J, Ks light curves for a sample of 717 Small Magellanic Cloud (SMC) Classical Cepheids (CCs). T…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 111
An ALMA Survey of CO Isotopologue Emission from Protoplanetary Disks in Chamaeleon I
DOI: 10.3847/1538-4357/aa78fc Bibcode: 2017ApJ...844...99L

Pascucci, Ilaria; Herczeg, Gregory J.; Henning, Thomas +8 more

The mass of a protoplanetary disk limits the formation and future growth of any planet. Masses of protoplanetary disks are usually calculated from measurements of the dust continuum emission by assuming an interstellar gas-to-dust ratio. To investigate the utility of CO as an alternate probe of disk mass, we use ALMA to survey 13CO and …

2017 The Astrophysical Journal
Gaia eHST 110
Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
DOI: 10.1088/1475-7516/2017/01/028 Bibcode: 2017JCAP...01..028C

Costa, André A.; Abdalla, E.; Wang, Bin +1 more

We investigate phenomenological interactions between dark matter and dark energy and constrain these models by employing the most recent cosmological data including the cosmic microwave background radiation anisotropies from Planck 2015, Type Ia supernovae, baryon acoustic oscillations, the Hubble constant and redshift-space distortions. We find t…

2017 Journal of Cosmology and Astroparticle Physics
Planck 110
The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data
DOI: 10.1093/mnras/stx898 Bibcode: 2017MNRAS.469.1445A

Kochanek, C. S.; Stanek, K. Z.; Adams, S. M. +1 more

We report updated results for the first 7 yr of our programme to monitor 27 galaxies within 10 Mpc using the Large Binocular Telescope to search for failed supernovae (SNe) - core collapses of massive stars that form black holes without luminous SNe. In the new data, we identify no new compelling candidates and confirm the existing candidate. Give…

2017 Monthly Notices of the Royal Astronomical Society
eHST 110
Athena: ESA's X-ray observatory for the late 2020s
DOI: 10.1002/asna.201713323 Bibcode: 2017AN....338..153B

Piro, L.; Nandra, K.; Barcons, X. +8 more

Observations of the X-ray sky after the next decade will most likely be dominated by Athena (Advanced Telescope for High ENergy Astrophysics), the second large mission of ESA's Cosmic Vision 2015-2035 programme. Athena has been conceived to address the "Hot and Energetic Universe" science theme, which focuses on the assembly and evolution of hot b…

2017 Astronomische Nachrichten
XMM-Newton 110
Radial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticals
DOI: 10.1051/0004-6361/201630075 Bibcode: 2017A&A...603A..80M

Zhang, Y. -Y.; Simionescu, A.; Kaastra, J. S. +10 more

The hot intra-cluster medium (ICM) permeating galaxy clusters and groups is not pristine, as it has been continuously enriched by metals synthesised in Type Ia (SNIa) and core-collapse (SNcc) supernovae since the major epoch of star formation (z ≃ 2-3). The cluster/group enrichment history and mechanisms responsible for releasing and mixing the me…

2017 Astronomy and Astrophysics
XMM-Newton 109
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
DOI: 10.1093/mnras/stw3384 Bibcode: 2017MNRAS.467.2085G

Streblyanska, Alina; Brownstein, Joel R.; Eisenstein, Daniel J. +25 more

We extract cosmological information from the anisotropic power-spectrum measurements from the recently completed Baryon Oscillation Spectroscopic Survey (BOSS), extending the concept of clustering wedges to Fourier space. Making use of new fast-Fourier-transform-based estimators, we measure the power-spectrum clustering wedges of the BOSS sample b…

2017 Monthly Notices of the Royal Astronomical Society
Planck 108
A powerful flare from Sgr A* confirms the synchrotron nature of the X-ray emission
DOI: 10.1093/mnras/stx596 Bibcode: 2017MNRAS.468.2447P

Genzel, R.; Hailey, C.; Harrison, F. +21 more

We present the first fully simultaneous fits to the near-infrared (NIR) and X-ray spectral slope (and its evolution) during a very bright flare from Sgr A*, the supermassive black hole at the Milky Way's centre. Our study arises from ambitious multiwavelength monitoring campaigns with XMM-Newton, NuSTAR and SINFONI. The average multiwavelength spe…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 108