Search Publications

Discovery of Periodic Dips in the Brightest Hard X-Ray Source of M31 with EXTraS
DOI: 10.3847/2041-8213/aa9b2e Bibcode: 2017ApJ...851L..27M

Tiengo, Andrea; Haberl, Frank; Belfiore, Andrea +9 more

We performed a search for eclipsing and dipping sources in the archive of the EXTraS project—a systematic characterization of the temporal behavior of XMM-Newton point sources. We discovered dips in the X-ray light curve of 3XMM J004232.1+411314, which has been recently associated with the hard X-ray source dominating the emission of M31. A system…

2017 The Astrophysical Journal
XMM-Newton 10
Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave
DOI: 10.1051/0004-6361/201630211 Bibcode: 2017A&A...607A..52A

Mas-Hesse, J. M.; Coe, M. J.; Reig, P. +7 more

Context. Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity.
Aims: We investigate the correlation between the optical emission and X-ray activity to predict the occurrence of new X-ray outbursts from …

2017 Astronomy and Astrophysics
INTEGRAL 10
The Evolution of Juventae Chasma, Valles Marineris, Mars: Progressive Collapse and Sedimentation
DOI: 10.1002/2017JE005334 Bibcode: 2017JGRE..122.2223F

Hauber, E.; Rossi, A. P.; Flahaut, J. +3 more

Juventae Chasma is an isolated chasm located north of the interconnected chasms within Valles Marineris. It contains four separate interior layered deposit (ILD) mounds. We have combined layer measurements, as well as mineralogical data of the mounds with topographic data of the remaining chasm and the surrounding plateau. Our observations indicat…

2017 Journal of Geophysical Research (Planets)
MEx 10
Interstellar extinction in Orion: variation of the strength of the ultraviolet bump across the complex
DOI: 10.1093/mnras/stx881 Bibcode: 2017MNRAS.469.2531B

Beitia-Antero, Leire; Gómez de Castro, Ana I.

There is growing observational evidence of dust coagulation in the dense filaments within molecular clouds. Infrared observations show that the dust grain size distribution becomes shallower and the relative fraction of small to large dust grains decreases as the local density increases. Ultraviolet (UV) observations show that the strength of the …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 10
Cosmology with XMM galaxy clusters: the X-CLASS/GROND catalogue and photometric redshifts
DOI: 10.1093/mnras/stx394 Bibcode: 2017MNRAS.468..662R

Greiner, J.; Salvato, M.; Nandra, K. +11 more

The XMM Cluster Archive Super Survey (X-CLASS) is a serendipitously detected X-ray-selected sample of 845 galaxy clusters based on 2774 XMM archival observations and covering an approximately 90 deg2 spread across the high-Galactic latitude (|b| > 20°) sky. The primary goal of this survey is to produce a well-selected sample of galax…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 10
Rapid optical variations correlated with X-rays in the 2015 second outburst of V404 Cygni (GS 2023+338)
DOI: 10.1093/mnras/stx1555 Bibcode: 2017MNRAS.471..373K

Nogami, Daisaku; Shidatsu, Megumi; Kato, Taichi +24 more

We present optical multicolour photometry of V404 Cyg during the outburst from 2015 December to 2016 January together with the simultaneous X-ray data. This outburst occurred less than six months after the previous outburst in 2015 June-July. These two outbursts in 2015 were of a slow-rise and rapid-decay type and showed large-amplitude (∼2 mag) a…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 10
The Wolf-Rayet star population in the dwarf galaxy NGC 625
DOI: 10.1051/0004-6361/201730663 Bibcode: 2017A&A...603A.130M

Walsh, J. R.; Monreal-Ibero, A.; Relaño, M. +4 more

Context. Quantifying the number, type, and distribution of Wolf-Rayet (W-R) stars is a key component in the context of galaxy evolution, since they put constraints on the age of the star formation bursts. Nearby galaxies (distances ≲5 Mpc) are particularly relevant in this context since they fill the gap between studies in the Local Group, where i…

2017 Astronomy and Astrophysics
eHST 10
AKARI/IRC source catalogues and source counts for the IRAC Dark Field, ELAIS North and the AKARI Deep Field South
DOI: 10.1093/mnras/stx1935 Bibcode: 2017MNRAS.472.4259D

Serjeant, S.; Pearson, C.; Matsuhara, H. +4 more

We present the first detailed analysis of three extragalactic fields (IRAC Dark Field, ELAIS-N1, ADF-S) observed by the infrared satellite, AKARI, using an optimized data analysis toolkit specifically for the processing of extragalactic point sources. The InfaRed Camera (IRC) on AKARI complements the Spitzer Space Telescope via its comprehensive c…

2017 Monthly Notices of the Royal Astronomical Society
AKARI 10
On the estimation of the current density in space plasmas: Multi- versus single-point techniques
DOI: 10.1016/j.pss.2017.03.008 Bibcode: 2017P&SS..140....6P

Sorriso-Valvo, Luca; Perri, Silvia; Malara, Francesco +2 more

Thanks to multi-spacecraft mission, it has recently been possible to directly estimate the current density in space plasmas, by using magnetic field time series from four satellites flying in a quasi perfect tetrahedron configuration. The technique developed, commonly called ;curlometer; permits a good estimation of the current density when the ma…

2017 Planetary and Space Science
Cluster 10
Testing the Interacting Dark Energy Model with Cosmic Microwave Background Anisotropy and Observational Hubble Data
DOI: 10.3390/e19070327 Bibcode: 2017Entrp..19..327Y

Yang, Weiqiang; Xu, Lixin; Wu, Yabo +2 more

The coupling between dark energy and dark matter provides a possible approach to mitigate the coincidence problem of the cosmological standard model. In this paper, we assumed the interacting term was related to the Hubble parameter, energy density of dark energy, and equation of state of dark energy. The interaction rate between dark energy and d…

2017 Entropy
Planck 10