Search Publications

Solar-stellar astrophysics and dark matter
DOI: 10.1088/1674-4527/12/8/011 Bibcode: 2012RAA....12.1107T

Turck-Chièze, Sylvaine; Lopes, Ilídio

In this review, we recall how stars contribute to the search for dark matter and the specific role of the Sun. We describe a more complete picture of the solar interior that emerges from neutrino detections, gravity and acoustic mode measurements of the Solar and Heliospheric Observatory (SOHO) satellite, becoming a reference for the most common s…

2012 Research in Astronomy and Astrophysics
SOHO 58
Star-Galaxy Classification in Multi-band Optical Imaging
DOI: 10.1088/0004-637X/760/1/15 Bibcode: 2012ApJ...760...15F

Hogg, David W.; Fadely, Ross; Willman, Beth

Ground-based optical surveys such as PanSTARRS, DES, and LSST will produce large catalogs to limiting magnitudes of r >~ 24. Star-galaxy separation poses a major challenge to such surveys because galaxies—even very compact galaxies—outnumber halo stars at these depths. We investigate photometric classification techniques on stars and galaxies w…

2012 The Astrophysical Journal
eHST 58
The X-ray lightcurve of Sagittarius A* over the past 150 years inferred from Fe-Kα line reverberation in Galactic centre molecular clouds
DOI: 10.1051/0004-6361/201219544 Bibcode: 2012A&A...545A..35C

Capelli, R.; Warwick, R. S.; Porquet, D. +2 more

Context. The spatial distribution and variability of Fe-Kα emission from molecular clouds in the Galactic centre region may provide an important key to the understanding of the recent history of Sgr A*. A very plausible interpretation is that this variability represents an echo in the reflected radiation from the clouds of a past episode of high a…

2012 Astronomy and Astrophysics
XMM-Newton 58
Quantifying the faint structure of galaxies: the late-type spiral NGC 2403
DOI: 10.1111/j.1365-2966.2011.19814.x Bibcode: 2012MNRAS.419.1489B

Jablonka, P.; Ferguson, Annette M. N.; Irwin, M. J. +2 more

Ground-based surveys have mapped the stellar outskirts of Local Group disc galaxies in unprecedented detail, but extending this work to other galaxies is necessary in order to overcome stochastic variations in evolutionary history and provide more stringent constraints on cosmological galaxy formation models. As part of our continuing programme of…

2012 Monthly Notices of the Royal Astronomical Society
eHST 58
Profiling filaments: comparing near-infrared extinction and submillimetre data in TMC-1
DOI: 10.1051/0004-6361/201219573 Bibcode: 2012A&A...544A..50M

Juvela, M.; André, Ph.; Palmeirim, P. +3 more

Context. Interstellar filaments are an important part of the star formation process. In order to understand the structure and formation of filaments, the filament cross-section profiles are often fitted with the so-called Plummer profile function. Currently this profiling is often approached with submillimetre studies, especially with Herschel. If…

2012 Astronomy and Astrophysics
Herschel ISO 58
The Advanced Camera for Surveys General Catalog: Structural Parameters for Approximately Half a Million Galaxies
DOI: 10.1088/0067-0049/200/1/9 Bibcode: 2012ApJS..200....9G

Koekemoer, Anton M.; Conselice, Christopher J.; Weiner, Benjamin +18 more

We present the Advanced Camera for Surveys General Catalog (ACS-GC), a photometric and morphological database using publicly available data obtained with the Advanced Camera for Surveys (ACS) instrument on the Hubble Space Telescope. The goal of the ACS-GC database is to provide a large statistical sample of galaxies with reliable structural and d…

2012 The Astrophysical Journal Supplement Series
eHST 58
Super fast plasma streams as drivers of transient and anomalous magnetospheric dynamics
DOI: 10.5194/angeo-30-1-2012 Bibcode: 2012AnGeo..30....1S

Daly, P. W.; Kozak, L.; Amata, E. +12 more

We present multi spacecraft measurements in the magnetosheath (MSH) and in the solar wind (SW) by Interball, Cluster and Polar, demonstrating that coherent structures with magnetosonic Mach number up to 3 - Supermagnetosonic Plasma Streams (SPS) - generate transient and anomalous boundary dynamics, which may cause substantial displacements of the …

2012 Annales Geophysicae
Cluster 58
Planck intermediate results. I. Further validation of new Planck clusters with XMM-Newton
DOI: 10.1051/0004-6361/201118731 Bibcode: 2012A&A...543A.102P

Böhringer, H.; Kneissl, R.; Dahle, H. +182 more

We present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-noise ratio of 4.5 < S/N < 5.3 in the same 10-month survey maps used in the construction of the Early SZ sample. The sample was selected in order to test internal …

2012 Astronomy and Astrophysics
Planck XMM-Newton 57
A Population of z > 2 Far-infrared Herschel-SPIRE-selected Starbursts
DOI: 10.1088/0004-637X/761/2/139 Bibcode: 2012ApJ...761..139C

Berta, S.; Magnelli, B.; Lutz, D. +29 more

We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 µm selected galaxies (HSGs) at 2 < z < 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg2 in six extragalactic legacy fields. Ob…

2012 The Astrophysical Journal
Herschel 57
The similarity of broad iron lines in X-ray binaries and active galactic nuclei
DOI: 10.1111/j.1365-2966.2012.20809.x Bibcode: 2012MNRAS.422.2510W

Fabian, A. C.; Miller, J. M.; Reis, R. C. +2 more

We have compared the 2001 XMM-Newton spectra of the stellar mass black hole binary XTE J1650-500 and the active galaxy MCG-6-30-15, focusing on the broad, excess emission features at ∼4-7 keV displayed by both sources. Such features are frequently observed in both low-mass X-ray binaries and active galactic nuclei (AGN). For the former case it is …

2012 Monthly Notices of the Royal Astronomical Society
XMM-Newton 57