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HerMES: point source catalogues from deep Herschel-SPIRE observations
DOI: 10.1111/j.1365-2966.2011.19709.x Bibcode: 2012MNRAS.419..377S

Pérez-Fournon, I.; Rodighiero, G.; Valtchanov, I. +38 more

We describe the generation of single-band point source catalogues from submillimetre Herschel-SPIRE observations taken as part of the Science Demonstration Phase of the Herschel Multi-tiered Extragalactic Survey (HerMES). Flux densities are found by means of peak finding and the fitting of a Gaussian point-response function. With highly confused i…

2012 Monthly Notices of the Royal Astronomical Society
Herschel 67
Wide-field imaging of NGC 4365's globular cluster system: the third subpopulation revisited
DOI: 10.1111/j.1365-2966.2011.19963.x Bibcode: 2012MNRAS.420...37B

Spitler, Lee R.; Forbes, Duncan A.; Blom, Christina

Analysis of the globular cluster (GC) system of the giant elliptical (E3) galaxy NGC 4365, from eight Hubble Space Telescope/Advanced Camera for Surveys pointings and a wide-field Subaru/Suprime-Cam image, is presented. Using magnitude, colour and size criteria, we obtain a catalogue of GC candidates. We also measure the photometric properties of …

2012 Monthly Notices of the Royal Astronomical Society
eHST 66
Spectroscopic Signature of Alfvén Waves Damping in a Polar Coronal Hole up to 0.4 Solar Radii
DOI: 10.1088/0004-637X/751/2/110 Bibcode: 2012ApJ...751..110B

Bemporad, A.; Abbo, L.

Between 2009 February 24 and 25, the EUV Imaging Spectrometer (EIS) spectrometer on board the Hinode spacecraft performed special "sit and stare" observations above the south polar coronal hole continuously over more than 22 hr. Spectra were acquired with the 1'' slit placed off-limb covering altitudes up to 0.48 R (3.34 × 102

2012 The Astrophysical Journal
Hinode 66
Nanostructuration of carbonaceous dust as seen through the positions of the 6.2 and 7.7 µm AIBs
DOI: 10.1051/0004-6361/201118700 Bibcode: 2012A&A...548A..40C

Dartois, E.; d'Hendecourt, L.; Brunetto, R. +7 more

Context. Carbonaceous cosmic dust is observed through infrared spectroscopy either in absorption or in emission. The details of the spectral features are believed to shed some light on its structure and finally enable the study of its life cycle.
Aims: The goal is to combine several analytical tools in order to decipher the intimate nanostruc…

2012 Astronomy and Astrophysics
ISO 66
Nuclear star clusters and the stellar spheroids of their host galaxies
DOI: 10.1111/j.1365-2966.2012.21365.x Bibcode: 2012MNRAS.424.2130L

Böker, Torsten; Knigge, Christian; Leigh, Nathan

We combine published photometry for the nuclear star clusters (NSCs) and stellar spheroids of 51 low-mass, early-type galaxies in the Virgo cluster with empirical mass-to-light ratios, in order to complement previous studies that explore the dependence of NSC masses on various properties of their host galaxies. We confirm a roughly linear relation…

2012 Monthly Notices of the Royal Astronomical Society
eHST 66
The Rest-frame UV-to-optical Colors and Spectral Energy Distributions of z ~ 4-7 Galaxies
DOI: 10.1088/0004-637X/755/2/148 Bibcode: 2012ApJ...755..148G

Franx, Marijn; Labbé, Ivo; Bouwens, Rychard J. +4 more

We use the ultra-deep HUDF09 and the deep Early Release Science data from the HST WFC3/IR camera, along with the wide-area Spitzer/IRAC data from GOODS-S to derive spectral energy distributions (SEDs) of star-forming galaxies from the rest-frame UV to the optical over a wide luminosity range (M 1500 ~ -21 to M 1500 ~ -18) fro…

2012 The Astrophysical Journal
eHST 66
The Early Early Type: Discovery of a Passive Galaxy at z spec ~ 3
DOI: 10.1088/2041-8205/759/2/L44 Bibcode: 2012ApJ...759L..44G

Cimatti, A.; Daddi, E.; Béthermin, M. +6 more

We present the discovery of a massive, quiescent galaxy at z = 2.99. We have obtained an Hubble Space Telescope WFC3 spectrum of this object and measured its redshift from the detection of a deep 4000 Å break consistent with an old population and a high metallicity. By stellar population modeling of both its grism spectrum and broadband photometry…

2012 The Astrophysical Journal
eHST 66
Nitrogen hydrides in interstellar gas. II. Analysis of Herschel/HIFI observations towards W49N and G10.6 - 0.4 (W31C)
DOI: 10.1051/0004-6361/201118686 Bibcode: 2012A&A...543A.145P

Menten, K. M.; Godard, B.; Persson, C. M. +14 more

As a part of the Herschel key programme PRISMAS, we have used the Herschel/HIFI instrument to observe interstellar nitrogen hydrides along the sight-lines towards eight high-mass star-forming regions in order to elucidate the production pathways leading to nitrogen-bearing species in diffuse gas. Here, we report observations towards W49N of the NH…

2012 Astronomy and Astrophysics
Herschel 66
Hinode/EIS Spectroscopic Validation of Very Hot Plasma Imaged with the Solar Dynamics Observatory in Non-flaring Active Region Cores
DOI: 10.1088/2041-8205/750/1/L10 Bibcode: 2012ApJ...750L..10T

Testa, Paola; Reale, Fabio

We use coronal imaging observations with the Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA), and Hinode/Extreme-ultraviolet Imaging Spectrometer (EIS) spectral data to explore the potential of narrowband EUV imaging data for diagnosing the presence of hot (T >~ 5 MK) coronal plasma in active regions. We analyze observations of tw…

2012 The Astrophysical Journal
Hinode 66
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive
DOI: 10.1111/j.1365-2966.2012.21153.x Bibcode: 2012MNRAS.423.3561C

Altieri, B.; Valtchanov, I.; Pierre, M. +5 more

We have processed 2774 high galactic observations from the XMM archive (as of 2010 May) and extracted a serendipitous catalogue of some 850 clusters of galaxies based on purely X-ray criteria, following the methodology developed for the XMM-Large-Scale Survey. Restricting the sample to the highest signal-to-noise ratio objects (347 clusters), we p…

2012 Monthly Notices of the Royal Astronomical Society
XMM-Newton 66