Search Publications

A New, Large-scale Map of Interstellar Reddening Derived from H I Emission
DOI: 10.3847/1538-4357/aa84af Bibcode: 2017ApJ...846...38L

Hensley, Brandon S.; Doré, Olivier; Lenz, Daniel

We present a new map of interstellar reddening, covering the 39% of the sky with low H I column densities (NHI< 4× 1020 cm-2 or E(B-V)≈ 45 mmag) at 16.1\prime resolution, based on all-sky observations of Galactic H I emission by the HI4PI Survey. In this low-column-density regime, we derive a characteristic valu…

2017 The Astrophysical Journal
Planck 117
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VIII. A Comparison to Cosmological Short-duration Gamma-Ray Bursts
DOI: 10.3847/2041-8213/aa9018 Bibcode: 2017ApJ...848L..23F

Berger, E.; Rest, A.; Annis, J. +19 more

We present a comprehensive comparison of the properties of the radio through X-ray counterpart of GW170817 and the properties of short-duration gamma-ray bursts (GRBs). For this effort, we utilize a sample of 36 short GRBs spanning a redshift range of z≈ 0.12{--}2.6 discovered over 2004-2017. We find that the counterpart to GW170817 has an isotrop…

2017 The Astrophysical Journal
eHST 117
The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec 6 in CANDELS
DOI: 10.1051/0004-6361/201527963 Bibcode: 2017A&A...600A.110T

Maccagni, D.; Cimatti, A.; Ilbert, O. +45 more

This paper describes the first data release (DR1) of the VIMOS Ultra Deep Survey (VUDS). The VUDS-DR1 is the release of all low-resolution spectroscopic data obtained in 276.9 arcmin2 of the CANDELS-COSMOS and CANDELS-ECDFS survey areas, including accurate spectroscopic redshifts zspec and individual spectra obtained with VIM…

2017 Astronomy and Astrophysics
eHST 116
Non-LTE aluminium abundances in late-type stars
DOI: 10.1051/0004-6361/201730427 Bibcode: 2017A&A...607A..75N

Lind, K.; Nordlander, T.


Aims: Aluminium plays a key role in studies of the chemical enrichment of the Galaxy and of globular clusters. However, strong deviations from LTE (non-LTE) are known to significantly affect the inferred abundances in giant and metal-poor stars.
Methods: We present non-local thermodynamic equilibrium (NLTE) modeling of aluminium using re…

2017 Astronomy and Astrophysics
eHST 116
Origin and Structures of Solar Eruptions I: Magnetic Flux Rope
DOI: 10.1007/s11430-017-9074-6 Bibcode: 2017ScChD..60.1383C

Cheng, Xin; Guo, Yang; Ding, MingDe

Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic eruptive phenomena in our solar system and able to release a large quantity of plasma and magnetic flux from the solar atmosphere into the solar wind. When these high-speed magnetized plasmas along with the energetic particles arrive at the Earth, they may intera…

2017 Science China Earth Sciences
IRIS SOHO 116
Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 < z < 2.5
DOI: 10.3847/1538-4357/aa6258 Bibcode: 2017ApJ...838...19W

Giavalisco, Mauro; van Dokkum, Pieter G.; Franx, Marijn +9 more

In this paper, we investigate the relationship between star formation and structure, using a mass-complete sample of 27,893 galaxies at 0.5 < z < 2.5 selected from 3D-HST. We confirm that star-forming galaxies are larger than quiescent galaxies at fixed stellar mass ({M}\star ). However, in contrast with some simulations, there is…

2017 The Astrophysical Journal
eHST 116
Multitemperature mapping of dust structures throughout the Galactic Plane using the PPMAP tool with Herschel Hi-GAL data
DOI: 10.1093/mnras/stx1723 Bibcode: 2017MNRAS.471.2730M

Palmeirim, P.; Schneider, N.; Becciani, U. +13 more

We describe new Hi-GAL based maps of the entire Galactic Plane, obtained using continuum data in the wavelength range 70-500 µm. These maps are derived with the PPMAP procedure, and therefore represent a significant improvement over those obtained with standard analysis techniques. Specifically they have greatly improved resolution (12 arcse…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 116
HELP: XID+, the probabilistic de-blender for Herschel SPIRE maps
DOI: 10.1093/mnras/stw2375 Bibcode: 2017MNRAS.464..885H

Le Floc'h, E.; Valtchanov, I.; Wang, L. +13 more

We have developed a new prior-based source extraction tool, XID+, to carry out photometry in the Herschel SPIRE (Spectral and Photometric Imaging Receiver) maps at the positions of known sources. XID+ is developed using a probabilistic Bayesian framework that provides a natural framework in which to include prior information, and uses the Bayesian…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 115
Planck constraint on relic primordial black holes
DOI: 10.1103/PhysRevD.95.083006 Bibcode: 2017PhRvD..95h3006C

Gao, Yu; Dutta, Bhaskar; Strigari, Louis E. +2 more

We investigate constraints on the abundance of primordial black holes (PBHs) in the mass range 1015- 1017 g using data from the cosmic microwave background (CMB) and MeV extragalactic gamma-ray background (EGB). Hawking radiation from PBHs with lifetime greater than the age of the Universe leaves an imprint on the CMB through…

2017 Physical Review D
Planck 115
Diverse stellar haloes in nearby Milky Way mass disc galaxies
DOI: 10.1093/mnras/stw2992 Bibcode: 2017MNRAS.466.1491H

Bell, Eric F.; Holwerda, Benne W.; Monachesi, Antonela +4 more

We have examined the resolved stellar populations at large galactocentric distances along the minor axis (from 10 kpc up to between 40 and 75 kpc), with limited major axis coverage, of six nearby highly inclined Milky Way (MW) mass disc galaxies using Hubble Space Telescope data from the Galaxy haloes, Outer discs, Substructure, Thick discs, and S…

2017 Monthly Notices of the Royal Astronomical Society
eHST 114