output
20022026
most citedA practical tutorial on autoencoders for nonlinear feature fusion: Taxonomy, models, software and guidelines

269 citations

Showing 2008 · astro-phShow all

7 papers · 2 filters

astro-ph2008

Exploring the powering source of the TeV X-ray binary LS 5039

J. Moldon, M. Ribo, Josep M. Paredes +2

LS 5039 is one of the four TeV emitting X-ray binaries detected up to now. The powering source of its multi-wavelength emission can be accretion in a microquasar scenario or wind i…

astro-ph2008

A radio and near-infrared mini-survey of the MGRO J2019+37 complex

J. M. Paredes, J. Marti, C. H. Ishwara-Chandra +9

MGRO J2019+37 is an unidentified source of very high energy gamma-rays originally reported by the MILAGRO collaboration as the brightest TeV source in the Cygnus region. Despite th…

astro-ph2008★ 12 cited

HCN(1-0) enhancement in the bar of NGC 2903

S. Leon, S. Jeyakumar, D. Perez-Ramirez +3

We have mapped the \hcn emission from two spiral galaxies, NGC2903 and NGC3504 to study the gas properties in the bars. The HCN(1-0) emission is detected in the center and along th…

astro-ph2008★ 9 cited

Discovery of thermal X-ray emission in the Supernova Remnant G337.8-0.1 (Kes 41)

J. A. Combi, J. F. Albacete-Colombo, J. Marti

We report here on the first detection at X-ray wavelengths of the Supernova Remnant (SNR) G337.8-0.1, carried out with the XMM-Newton Observatory. Using the X-ray observations, we…

astro-ph2008★ 6 cited

Radio detections towards unidentified variable EGRET sources

J. M. Paredes, J. Marti, C. H. Ishwara-Chandra +6

Context. A considerable fraction of the gamma-ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been…

astro-ph2008★ 54 cited

The changing milliarcsecond radio morphology of the gamma-ray binary LS 5039

M. Ribo, J. M. Paredes, J. Moldon +2

Context. LS 5039 is one of the few TeV emitting X-ray binaries detected so far. The powering source of its multiwavelength emission can be accretion in a microquasar scenario or wi…