Search Publications

The Herschel Multi-tiered Extragalactic Survey: HerMES
DOI: 10.1111/j.1365-2966.2012.20912.x Bibcode: 2012MNRAS.424.1614O

Altieri, B.; Aussel, H.; Elbaz, D. +101 more

The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling ∼380 deg2. Fields range in size from 0.01 to ∼20 deg2, using the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) (at 250, 350 and 500 µm) and the Herschel-Photodetector Array Camera a…

2012 Monthly Notices of the Royal Astronomical Society
Herschel ISO 729
Herschel-ATLAS: multi-wavelength SEDs and physical properties of 250 µm selected galaxies at z < 0.5
DOI: 10.1111/j.1365-2966.2012.21930.x Bibcode: 2012MNRAS.427..703S

Ivison, R. J.; Clements, D. L.; Scott, D. +38 more

We present a pan-chromatic analysis of an unprecedented sample of 1402 250 µm selected galaxies at z < 0.5 (z¯=0.24) from the Herschel-ATLAS survey. We complement our Herschel 100-500 µm data with UV-K-band photometry from the Galaxy And Mass Assembly (GAMA) survey and apply the MAGPHYS energy-balance technique to produce pan-chroma…

2012 Monthly Notices of the Royal Astronomical Society
Herschel ISO 143
On the metallicity dependence of crystalline silicates in oxygen-rich asymptotic giant branch stars and red supergiants
DOI: 10.1111/j.1365-2966.2012.21978.x Bibcode: 2012MNRAS.427.3209J

Zijlstra, A. A.; Boyer, M. L.; Gielen, C. +10 more

We investigate the occurrence of crystalline silicates in oxygen-rich evolved stars across a range of metallicities and mass-loss rates. It has been suggested that the crystalline silicate feature strength increases with increasing mass-loss rate, implying a correlation between lattice structure and wind density. To test this, we analyse Spitzer I…

2012 Monthly Notices of the Royal Astronomical Society
ISO 52
Formation of unsaturated hydrocarbons in interstellar ice analogues by cosmic rays
DOI: 10.1111/j.1365-2966.2012.21031.x Bibcode: 2012MNRAS.423.2209P

Pilling, S.; da Silveira, E. F.; Rothard, H. +3 more

The formation of C=C and C≡C bonds from the processing of pure c-C6H12 (cyclohexane) and mixed H2O:NH3:c-C6H12 (1:0.3:0.7) ices by highly charged and energetic ions (219-MeV 16O7 + and 632-MeV 58Ni24 +) is studied. The experiments simulate…

2012 Monthly Notices of the Royal Astronomical Society
ISO 28
Solid-phase C60 in the peculiar binary XX Oph?
DOI: 10.1111/j.1745-3933.2012.01213.x Bibcode: 2012MNRAS.421L..92E

van Loon, J. Th.; Gehrz, R. D.; Eyres, S. P. S. +8 more

We present infrared spectra of the binary XX Oph obtained with the Infrared Spectrograph on the Spitzer Space Telescope. The data show some evidence for the presence of solid C60- the first detection of C60 in the solid phase - together with the well-known 'unidentified infrared' emission features. We suggest that, in the cas…

2012 Monthly Notices of the Royal Astronomical Society
AKARI ISO 19
Evolution of the luminosity function and obscuration of active galactic nuclei: comparison between X-ray and infrared
DOI: 10.1111/j.1365-2966.2012.20890.x Bibcode: 2012MNRAS.423..464H

Han, Zhanwen; Zhang, Fenghui; Wang, Bo +2 more

We present a detailed comparison between the 2-10 keV hard X-ray and infrared (IR) luminosity functions (LFs) of active galactic nuclei (AGNs). The composite X-ray to IR spectral energy distributions (SEDs) of AGNs, which are used to compare the hard X-ray LF (HXLF) and the IRLF, are modelled with a simple, but well-tested torus model, based on th…

2012 Monthly Notices of the Royal Astronomical Society
ISO 11
Automated measurement of redshifts from mid-infrared low-resolution spectroscopy
DOI: 10.1111/j.1365-2966.2012.22047.x Bibcode: 2012MNRAS.427..816H

Hernán Caballero, Antonio

Obtaining accurate redshifts from mid-infrared (MIR) low-resolution (R ∼ 100) spectroscopy is challenging because the wavelength resolution is too low to detect narrow lines in most cases. Yet, the number of degrees of freedom and diversity of spectral features are too high for regular spectral energy distribution (SED) fitting techniques to be co…

2012 Monthly Notices of the Royal Astronomical Society
AKARI ISO 11
Optical and infrared imaging and spectroscopy of the multiple-shell planetary nebula NGC 6369
DOI: 10.1111/j.1365-2966.2011.20075.x Bibcode: 2012MNRAS.420.1977R

Guerrero, M. A.; Ramos-Larios, G.; Phillips, J. P. +1 more

NGC 6369 is a double-shell planetary nebula consisting of a bright annular inner shell with faint bipolar extensions and a filamentary envelope. We have used ground- and space-based narrow-band optical and near-infrared (near-IR) images, broad-band mid-IR images, optical long-slit echelle spectra and mid-IR spectra to investigate its physical stru…

2012 Monthly Notices of the Royal Astronomical Society
ISO eHST 11