Search Publications

The IRX-β relation on subgalactic scales in star-forming galaxies of the Herschel Reference Survey
DOI: 10.1051/0004-6361/201118624 Bibcode: 2012A&A...539A.145B

Ciesla, L.; Buat, V.; Boquien, M. +13 more


Aims: It is still not understood why star-forming galaxies deviate from the ultraviolet colour-attenuation relation of starburst galaxies. Previous work and models hint that the role of the shape of the attenuation curve and the age of stellar populations play an important role. In this paper we aim at understanding the fundamental reasons fo…

2012 Astronomy and Astrophysics
Herschel 121
Evolution of the Quasar Luminosity Function over 3 < z < 5 in the COSMOS Survey Field
DOI: 10.1088/0004-637X/755/2/169 Bibcode: 2012ApJ...755..169M

Salvato, M.; Hasinger, G.; Capak, P. +10 more

We investigate the high-redshift quasar luminosity function (QLF) down to an apparent magnitude of I AB = 25 in the Cosmic Evolution Survey (COSMOS). Careful analysis of the extensive COSMOS photometry and imaging data allows us to identify and remove stellar and low-redshift contaminants, enabling a selection that is nearly complete fo…

2012 The Astrophysical Journal
eHST 120
The SLUGGS survey: calcium triplet-based spectroscopic metallicities for over 900 globular clusters
DOI: 10.1111/j.1365-2966.2012.21801.x Bibcode: 2012MNRAS.426.1475U

Spitler, Lee R.; Forbes, Duncan A.; Romanowsky, Aaron J. +6 more

Although the colour distribution of globular clusters in massive galaxies is well known to be bimodal, the spectroscopic metallicity distribution has been measured in only a few galaxies. After redefining the calcium triplet index-metallicity relation, we use our relation to derive the metallicity of 903 globular clusters in 11 early-type galaxies…

2012 Monthly Notices of the Royal Astronomical Society
eHST 120
Analysis of astrometric catalogues with vector spherical harmonics
DOI: 10.1051/0004-6361/201219927 Bibcode: 2012A&A...547A..59M

Mignard, F.; Klioner, S.


Aims: We compare stellar catalogues with position and proper motion components using a decomposition on a set of orthogonal vector spherical harmonics. We aim to show the theoretical and practical advantages of this technique as a result of invariance properties and the independence of the decomposition from a prior model.
Methods: We de…

2012 Astronomy and Astrophysics
Hipparcos 120
Information Content of Exoplanetary Transit Spectra: An Initial Look
DOI: 10.1088/0004-637X/749/1/93 Bibcode: 2012ApJ...749...93L

Line, Michael R.; Zhang, Xi; Yung, Yuk L. +3 more

It has been shown that spectroscopy of transiting extrasolar planets can potentially provide a wealth of information about their atmospheres. Herein, we set up the inverse problem in spectroscopic retrieval. We use nonlinear optimal estimation to retrieve the atmospheric state (pioneered for Earth sounding by Rodgers). The formulation quantifies t…

2012 The Astrophysical Journal
eHST 120
Comparative study of CH+ and SH+ absorption lines observed towards distant star-forming regions⋆⋆⋆
DOI: 10.1051/0004-6361/201117664 Bibcode: 2012A&A...540A..87G

Menten, K. M.; Falgarone, E.; Godard, B. +8 more


Aims: The HIFI instrument onboard Herschel has allowed high spectral resolution and sensitive observations of ground-state transitions of three molecular ions: the methylidyne cation CH+, its isotopologue 13CH+, and sulfanylium SH+. Because of their unique chemical properties, a comparative analysis…

2012 Astronomy and Astrophysics
Herschel 120
A Jet Break in the X-Ray Light Curve of Short GRB 111020A: Implications for Energetics and Rates
DOI: 10.1088/0004-637X/756/2/189 Bibcode: 2012ApJ...756..189F

Troja, E.; Sakamoto, T.; Berger, E. +8 more

We present broadband observations of the afterglow and environment of the short GRB 111020A. An extensive X-ray light curve from Swift/XRT, XMM-Newton, and Chandra, spanning ~100 s to 10 days after the burst, reveals a significant break at δt ≈ 2 days with pre- and post-break decline rates of α X, 1 ≈ -0.78 and α X, 2 <~ -…

2012 The Astrophysical Journal
XMM-Newton 120
A Suzaku survey of Fe K lines in Seyfert 1 active galactic nuclei
DOI: 10.1111/j.1365-2966.2012.21868.x Bibcode: 2012MNRAS.426.2522P

Porquet, D.; Reeves, J. N.; Braito, V. +3 more

We construct full broad-band models in an analysis of Suzaku observations of nearby Seyfert 1 active galactic nuclei (AGN) (z ≤ 0.2) with exposures >50 ks and with greater than 30 000 counts in order to study their iron line profiles. This results in a sample of 46 objects and 84 observations. After a full modelling of the broad-band Suzaku and…

2012 Monthly Notices of the Royal Astronomical Society
Suzaku 120
A chronology of early Mars climatic evolution from impact crater degradation
DOI: 10.1029/2011JE004005 Bibcode: 2012JGRE..117.4003M

Mangold, N.; Ansan, V.; Adeli, S. +2 more

The degradation of impact craters provides a powerful tool to analyze surface processes in the Martian past. Previous studies concluded that large impact craters (20-200 km in diameter) were strongly degraded by fluvial erosion during early Martian history. Our goal is to study the progression of crater degradation through time with a particular e…

2012 Journal of Geophysical Research (Planets)
MEx 119
A remarkably high fraction of strong Lyα emitters amongst luminous redshift 6.0 < z < 6.5 Lyman-break galaxies in the UKIDSS Ultra-Deep Survey
DOI: 10.1111/j.1365-2966.2012.20720.x Bibcode: 2012MNRAS.422.1425C

McLure, R. J.; Dunlop, J. S.; Cirasuolo, M. +8 more

We present spectroscopic confirmation of 10 highly luminous (L≥ 2L) Lyα emitters (LAEs) in the redshift range 6.01 < z < 6.49 (nine galaxies and one active galactic nucleus), initially drawn from a sample of 14 zphot≥ 6 Lyman-break galaxies (LBGs) selected from an area of 0.25 deg2 within the UK Infrared Dee…

2012 Monthly Notices of the Royal Astronomical Society
eHST 119