Search Publications

Constraint on the abundance of primordial black holes in dark matter from Planck data
DOI: 10.1088/1475-7516/2016/12/044 Bibcode: 2016JCAP...12..044C

Huang, Qing-Guo; Wang, Ke; Chen, Lu

We use Planck data released in 2015 to constrain the abundance of primordial black holes (PBHs) in dark matter in two different reionization models (one is the instantaneous reionization and the other is the asymmetric reionization), and significantly improve the existing upper limits on the abundance of PBHs by around two orders of magnitude. The…

2016 Journal of Cosmology and Astroparticle Physics
Planck 77
New CMB constraints for Abelian Higgs cosmic strings
DOI: 10.1088/1475-7516/2016/10/042 Bibcode: 2016JCAP...10..042L

Kunz, Martin; Lizarraga, Joanes; Urrestilla, Jon +2 more

We present cosmic microwave background (CMB) power spectra from recent numerical simulations of cosmic strings in the Abelian Higgs model and compare them to CMB power spectra measured by Planck. We obtain revised constraints on the cosmic string tension parameter Gµ. For example, in the ΛCDM model with the addition of strings and no primord…

2016 Journal of Cosmology and Astroparticle Physics
Planck 76
Dust properties of Lyman-break galaxies at z ~ 3
DOI: 10.1051/0004-6361/201527190 Bibcode: 2016A&A...587A.122A

Pérez-Fournon, I.; Rodighiero, G.; Ilbert, O. +18 more

Context. Since the mid-1990s, the sample of Lyman-break galaxies (LBGs) has been growing thanks to the increasing sensitivities in the optical and in near-infrared telescopes for objects at z> 2.5. However, the dust properties of the LBGs are poorly known because the samples are small and/or biased against far-infrared (far-IR) or submillimeter…

2016 Astronomy and Astrophysics
Herschel 76
Probing primordial features with future galaxy surveys
DOI: 10.1088/1475-7516/2016/10/041 Bibcode: 2016JCAP...10..041B

Finelli, F.; Moscardini, L.; Ballardini, M. +1 more

We study the capability of future measurements of the galaxy clustering power spectrum to probe departures from a power-law spectrum for primordial fluctuations. On considering the information from the galaxy clustering power spectrum up to quasi-linear scales, i.e. k < 0.1 h Mpc-1, we present forecasts for DESI, Euclid and SPHEREx i…

2016 Journal of Cosmology and Astroparticle Physics
Planck 76
The Rotation of the Hot Gas around the Milky Way
DOI: 10.3847/0004-637X/822/1/21 Bibcode: 2016ApJ...822...21H

Bregman, Joel N.; Miller, Matthew J.; Hodges-Kluck, Edmund J.

The hot gaseous halos of galaxies likely contain a large amount of mass and are an integral part of galaxy formation and evolution. The Milky Way has a 2× {10}6 K halo that is detected in emission and by absorption in the O vii resonance line against bright background active galactic nuclei (AGNs), and for which the best current model i…

2016 The Astrophysical Journal
XMM-Newton 76
Systematic comparison of photoionised plasma codes with application to spectroscopic studies of AGN in X-rays
DOI: 10.1051/0004-6361/201628721 Bibcode: 2016A&A...596A..65M

Kaastra, J. S.; Mehdipour, M.; Kallman, T.

Atomic data and plasma models play a crucial role in the diagnosis and interpretation of astrophysical spectra, thus influencing our understanding of the Universe. In this investigation we present a systematic comparison of the leading photoionisation codes to determine how much their intrinsic differences impact X-ray spectroscopic studies of hot…

2016 Astronomy and Astrophysics
XMM-Newton 76
Candidate Gravitationally Lensed Dusty Star-forming Galaxies in the Herschel Wide Area Surveys
DOI: 10.3847/0004-637X/823/1/17 Bibcode: 2016ApJ...823...17N

Ivison, R. J.; Frayer, D. T.; Omont, A. +21 more

We present a list of candidate gravitationally lensed dusty star-forming galaxies (DSFGs) from the HerMES Large Mode Survey and the Herschel Stripe 82 Survey. Together, these partially overlapping surveys cover 372 deg2 on the sky. After removing local spiral galaxies and known radio-loud blazars, our candidate list of lensed DSFGs is c…

2016 The Astrophysical Journal
Herschel 76
Deep XMM observations of Draco rule out at the 99 per cent confidence level a dark matter decay origin for the 3.5 keV line
DOI: 10.1093/mnras/stw578 Bibcode: 2016MNRAS.458.3592J

Profumo, Stefano; Jeltema, Tesla

We searched for an X-ray line at energies around 3.5 keV in deep, ∼1.6 Ms XMM-Newton observations of the dwarf spheroidal galaxy Draco. No line was found in either the Metal Oxide Semi-conductor (MOS) or the p-type/n-type semiconductor (PN) detectors. The data in this energy range are completely consistent with a single, unfolded power-law modelli…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 75
The High Resolution Stereo Camera (HRSC) of Mars Express and its approach to science analysis and mapping for Mars and its satellites
DOI: 10.1016/j.pss.2016.02.014 Bibcode: 2016P&SS..126...93G

Jaumann, R.; Oberst, J.; Preusker, F. +32 more

The High Resolution Stereo Camera (HRSC) of ESA's Mars Express is designed to map and investigate the topography of Mars. The camera, in particular its Super Resolution Channel (SRC), also obtains images of Phobos and Deimos on a regular basis. As HRSC is a push broom scanning instrument with nine CCD line detectors mounted in parallel, its unique…

2016 Planetary and Space Science
MEx 75
Deep Chandra observations of Pictor A
DOI: 10.1093/mnras/stv2553 Bibcode: 2016MNRAS.455.3526H

Stawarz, Ł.; Hardcastle, M. J.; Croston, J. H. +7 more

We report on deep Chandra observations of the nearby broad-line radio galaxy Pictor A, which we combine with new Australia Telescope Compact Array (ATCA) observations. The new X-ray data have a factor of 4 more exposure than observations previously presented and span a 15 yr time baseline, allowing a detailed study of the spatial, temporal and spe…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 75