Proceedings of the 2nd workshop on Emotion Representations and Modelling for Companion Systems

2016 ◽  
Keyword(s):  
Companion Systems

A Multimodal Dialogue Framework for Cloud-Based Companion Systems

2019 ◽  
pp. 405-410 ◽  
Author(s):  
Matthias Kraus ◽  
Marvin Schiller ◽  
Gregor Behnke ◽  
Pascal Bercher ◽  
Susanne Biundo ◽  
...  
Keyword(s):  
Companion Systems ◽  
Multimodal Dialogue

Environment Adaption for Companion-Systems

2017 ◽  
pp. 301-320
Author(s):  
Stephan Reuter ◽  
Alexander Scheel ◽  
Thomas Geier ◽  
Klaus Dietmayer
Keyword(s):  
Companion Systems

A paradigm for coupling procedural and conceptual knowledge in companion systems

2017 ◽  
Author(s):  
Marvin Schiller ◽  
Gregor Behnke ◽  
Mario Schmautz ◽  
Pascal Bercher ◽  
Matthias Kraus ◽  
...  
Keyword(s):  
Conceptual Knowledge ◽  
Companion Systems

Possible applications of companion systems in psychotherapy - perspectives on a new technology

2017 ◽  
Author(s):  
Steffen Walter ◽  
Matthias Haase ◽  
Andreas Oschlies-Strobel ◽  
Lucia Jerg-Bretzke ◽  
Harald Traue ◽  
...  
Keyword(s):  
New Technology ◽  
Companion Systems

Emotion Identification and Modelling on the Basis of Paired Physiological Data Features for Companion Systems

2012 ◽  
Vol 45 (2) ◽  
pp. 315-319 ◽  
Author(s):  
David Hrabal ◽  
Stefanie Rukavina ◽  
Kerstin Limbrecht ◽  
Sascha Gruss ◽  
Steffen Walter ◽  
...  
Keyword(s):  
Physiological Data ◽  
Emotion Identification ◽  
Companion Systems

scholarly journals Structure of the violet bands of silicon nitride

1929 ◽  
Vol 122 (789) ◽  
pp. 103-121 ◽  
Keyword(s):  
Silicon Nitride ◽  
Isotope Effect ◽  
Visible Spectrum ◽  
Silicon Tetrachloride ◽  
Resolving Power ◽  
Active Nitrogen ◽  
Quantum Numbers ◽  
Long Wave ◽  
Mass Spectrograph ◽  
Companion Systems

The spectrum of the luminescence produced when silicon tetrachloride vapour reacts with glowing active nitrogen was first studied by Jevons. He measured the heads of a group of bands occurring in the more refrangible part of the visible spectrum. These bands have single heads and are degraded towards the long wave-lengths. From the fact that a nitrogen-containing substance is deposited on the walls of the after-glow tube during the reaction, Jevons favoured the view that the bands are due to a nitride of silicon (SiN). This has been verified in a recent study of its spectrum by Mulliken. In this work, which was primarily concerned with the isotope effect, Jevons’ measurements were revised and extended to include two faint companion systems of bands, due to isotopic molecules containing silicon of atomic weights 29 and 30. Further, Mulliken was able to establish spectroscopically the existence of the latter isotope, when the mass-spectrograph evidence was still inconclusive, and he included a description of a weaker system of bands distinct from the above, in that the heads are double and no frequency intervals occurred which agreed with those of the stronger system. Vibrational quantum numbers were assigned for the two systems, and the constants of the rotational structure of the stronger bands were determined by a procedure which was necessarily approximate, since spectrographs of moderate resolving power were used.

Management of Multimodal User Interaction in Companion-Systems

2017 ◽  
pp. 187-207
Author(s):  
Felix Schüssel ◽  
Frank Honold ◽  
Nikola Bubalo ◽  
Michael Weber ◽  
Anke Huckauf
Keyword(s):  
User Interaction ◽  
Companion Systems

scholarly journals Companions to High Redshift Quasars

1992 ◽  
Vol 9 ◽  
pp. 693-694
Author(s):  
Esther M. Hu
Keyword(s):  
Energy Distribution ◽  
High Redshift ◽  
Spectral Energy Distribution ◽  
Spectral Energy ◽  
Radio Sources ◽  
Color Imaging ◽  
Radio Studies ◽  
Companion Systems

AbstractLyman a companions to high-redshift quasars appear associated with radio activity in the quasar. Of the five known companion systems seen at typical Lα fluxes of a few x 10-16 ergs cm-2 sec-1, all are associated with quasars which are radio sources, and lie within a few arcseconds of the quasar. We summarize results of searches for the companions, and report on subsequent investigations into the spectral energy distribution and radio studies of these objects. Multi-color imaging from 3400 Å to 2.2/μ shows the companion to PKS 1614+051 possesses a blue SED similar to an irregular at that redshift. VLA observations show double-lobed structure around Q1033+137 with depolarization of the counterjet lobe.

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