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Multi-frequency observations of SNR J0453-6829 in the LMC. A composite supernova remnant with a pulsar wind nebula
DOI: 10.1051/0004-6361/201218971 Bibcode: 2012A&A...543A.154H

Pietsch, W.; Haberl, F.; Filipović, M. D. +7 more

Context. The Large Magellanic Cloud (LMC) is rich in supernova remnants (SNRs), which can be investigated in detail with radio, optical, and X-ray observations. SNR J0453-6829 is an X-ray and radio-bright remnant in the LMC, within which previous studies revealed the presence of a pulsar wind nebula (PWN), making it one of the most interesting SNR…

2012 Astronomy and Astrophysics
XMM-Newton 24
Accurate classification of 29 objects detected in the 39 month Palermo Swift/BAT hard X-ray catalogue
DOI: 10.1051/0004-6361/201219192 Bibcode: 2012A&A...545A.101P

Palazzi, E.; Minniti, D.; Masetti, N. +15 more

Through an optical campaign performed at four telescopes located in the northern and the southern hemispheres, plus archival data from two on-line sky surveys, we obtained optical spectroscopy for 29 counterparts of unclassified or poorly studied hard X-ray emitting objects detected with Swift /Burst Alert Telescope (BAT) and listed in the 39 mont…

2012 Astronomy and Astrophysics
XMM-Newton 24
The relative and absolute timing accuracy of the EPIC-pn camera on XMM-Newton, from X-ray pulsations of the Crab and other pulsars
DOI: 10.1051/0004-6361/201116576 Bibcode: 2012A&A...545A.126M

Guainazzi, M.; Freyberg, M. J.; Wellbrock, A. +13 more


Aims: Reliable timing calibration is essential for the accurate comparison of XMM-Newton light curves with those from other observatories, to ultimately use them to derive precise physical quantities. The XMM-Newton timing calibration is based on pulsar analysis. However, because pulsars show both timing noise and glitches, it is essential to…

2012 Astronomy and Astrophysics
INTEGRAL XMM-Newton 23
Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kα line
DOI: 10.1051/0004-6361/201117126 Bibcode: 2012A&A...537A...6C

Nandra, K.; Merloni, A.; Comastri, A. +3 more


Aims: The aim of this work is to characterize the average Fe K emission properties of active galactic nuclei (AGNs) in the source rest-frame.
Methods: We selected a sample of 248 AGNs from the 2XMM catalog, covering a wide redshift range 0 < z < 5 and with the EPIC-PN net 2-10 keV rest-frame counts ≥ 200 and power law photon indice…

2012 Astronomy and Astrophysics
XMM-Newton 23
Planetary transit candidates in the CoRoT-SRc01 field
DOI: 10.1051/0004-6361/201116934 Bibcode: 2012A&A...539A..14E

Mazeh, T.; Aigrain, S.; Alapini, A. +52 more

Context. The space mission CoRoT is devoted to the analysis of stellar variability and the photometric detection of extrasolar planets.
Aims: We present the list of planetary transit candidates detected in the first short run observed by CoRoT that targeted SRc01, towards the Galactic center in the direction of Aquila, which lasted from April…

2012 Astronomy and Astrophysics
CoRoT 23
Chromospheric jets around the edges of sunspots
DOI: 10.1051/0004-6361/201219137 Bibcode: 2012A&A...543A...6M

Morton, R. J.


Aims: Evidence is beginning to be put forward that demonstrates the role of the chromosphere in supplying energy and mass to the corona. We aim to assess the role of chromospheric jets in active region dynamics.
Methods: Using a combination of the Hinode/SOT Ca II H and TRACE 1550 Å and 1600 Å filters we examine chromospheric jets situat…

2012 Astronomy and Astrophysics
Hinode 23
Galaxy counterparts of intervening high-z sub-DLAs/DLAs and Mg ii absorbers towards gamma-ray bursts
DOI: 10.1051/0004-6361/201118647 Bibcode: 2012A&A...546A..20S

Vreeswijk, P. M.; Milvang-Jensen, B.; Fynbo, J. P. U. +19 more

We present the first search for galaxy counterparts of intervening high-z (2 < z < 3.6) sub-damped Lyα absorbers (sub-DLAs) and DLAs towards gamma-ray bursts (GRBs). Our final sample comprises five intervening sub-DLAs and DLAs in four GRB fields. To identify candidate galaxy counterparts of the absorbers we used deep optical- and near-infra…

2012 Astronomy and Astrophysics
eHST 23
Shape reconstruction of irregular bodies with multiple complementary data sources
DOI: 10.1051/0004-6361/201219267 Bibcode: 2012A&A...543A..97K

Kaasalainen, M.; Viikinkoski, M.

We discuss inversion methods for shape reconstruction with complementary data sources. The current main sources are photometry, adaptive optics or other images, occultation timings, and interferometry, and the procedure can readily be extended to include range-Doppler radar and thermal infrared data as well. We introduce the octantoid, a generally…

2012 Astronomy and Astrophysics
eHST 23
Study of the first productive active region in solar cycle 24
DOI: 10.1051/0004-6361/201015796 Bibcode: 2012A&A...539A...7L

Zhang, J.; Li, L. P.; Li, T. +2 more

Context. The Sun is very quiet with less sunspots and activity since the beginning of solar cycle 24. However, the active region (AR) 11 045 emerged on February 5, 2010, is associated with 43 (8 M- and 35 C-class) flares, 53 coronal mass ejections (CMEs), 29 filament eruptions, 19 extreme ultraviolet (EUV) waves and abundant jets, indicating that …

2012 Astronomy and Astrophysics
SOHO 23
A relativistic iron emission line from the neutron star low-mass X-ray binary GX 3+1
DOI: 10.1051/0004-6361/201219283 Bibcode: 2012A&A...542L..27P

Santangelo, A.; Kaaret, P.; Egron, E. +7 more

We present the results of a spectroscopic study of the Fe Kα emission of the persistent neutron-star atoll low-mass X-ray binary and type I X-ray burster GX 3+1 with the EPIC-PN on board XMM-Newton. The source shows a flux modulation over several years and we observed it during its fainter phase, which corresponds to an X-ray luminosity of LX…

2012 Astronomy and Astrophysics
XMM-Newton 23