1,234 research outputs found
CDP: A Connectionist Deterministic Parser A Dissertation Proposal
We propose to address problems related to the problem of Natural Language Processing. Neural networks approach will be used in attaching these problems. In this proposal a number of problems are considered: parsing of ill-formed sentences in addition to well-formed sentences, resolutions of some lexical ambiguities using syntactic context, and parsing of sentences sequentially over an input stream which is unbounded in length. Two network training approaches will be examined. Deductive training, based on grammar rules, and inductive training, based on sentence processing will be fully investigated. Comparisons with each approach to its corresponding symbolic approach will be made
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Competition and Learning in a Connectionist Deterministic Parser
Deterministic parsing promises to (almost) never backtrack. Neural network technology promises competition, and learning capabilities. The marriage of these two ideas is being investigated in an experimental natural language parsing system that combines some of the best features of each. The result is a deterministic parser that learns, generalizes, and supports competition among structures and lexical interpretations. The performance of the parser is being evaluated on predicted as well as unpredicted sentence forms. Several mildly ungrammatical sentences have been successfully processed into structures judged reasonable when compared to their grammatical counterparts. Lexic^ ambiguities can create problems for traditional parsers, or at least require additional backtracking. With the use of neural netwoilcs, ambiguities can be resolved through the wider syntactic context. The results have shown the potential for parsing using this approach
Determinism and Connectionism in a Rule-Based Natural Language System
The processing of Natural Language is, at the same time, natural symbolic and naturally symbolic and naturally sub-symbolic. It is symbolic because ultimately symbols play a critical role. Writing systems, for example, owe their existence to the symbolic nature of language. It is also sub-symbolic because of the nature of speech, the fuzziness of concepts, and the high degree of parallelism that is difficult to explain as a purely symbolic phenomenon. This report details a set of experiments which support the claim that Natural Language can be syntactically processed in a robust manner using a connectionist deterministic parser. The model is trained based on a deterministic grammar and tested with sentences which are grammatically and ones that ill-formed. Tests are also conducted with sentences containing lexically ambiguous items. Some new directions for this work are explored in the final section. The goal of fully connectionistic parsing is discussed and a detail plan for its achievements is present
Two new pulsating low-mass pre-white dwarfs or SX Phenix stars?*
Context. The discovery of pulsations in low-mass stars opens an opportunity
for probing their interiors and to determine their evolution, by employing the
tools of asteroseismology. Aims. We aim to analyze high-speed photometry of
SDSSJ145847.02070754.46 and SDSSJ173001.94070600.25 and discover
brightness variabilities. In order to locate these stars in the diagram we fit optical spectra (SDSS) with synthetic non-magnetic
spectra derived from model atmospheres. Methods. To carry out this study, we
used the photometric data obtained by us for these stars with the 2.15m
telescope at CASLEO, Argentina. We analyzed their light curves and we apply the
Discrete Fourier Transform to determine the pulsation frequencies. Finally, we
compare both stars in the diagram, with known two
pre-white dwarfs, seven pulsating pre-ELM white dwarf stars, Scuti and
SX Phe stars. Results. We report the discovery of pulsations in
SDSSJ145847.02070754.46 and SDSSJ173001.94070600.25. We determine their
effective temperature and surface gravity to be = 7 972 200
K, = 4.25 0.5 and = 7 925 200 K, =
4.25 0.5, respectively. With these parameters these new pulsating
low-mass stars can be identified with either ELM white dwarfs (with ~ 0.17 Mo)
or more massive SX Phe stars. We identified pulsation periods of 3 278.7 and 1
633.9 s for SDSSJ145847.02070754.46 and a pulsation period of 3 367.1 s for
SDSSJ173001.94070600.25. These two new objects together with those of Maxted
et al. (2013, 2014) indicate the possible existence of a new instability domain
towards the late stages of evolution of low-mass white dwarf stars, although
their identification with SX Phe stars cannot be discarded.Comment: 5 pages, 5 figures, 1 table, accepted for publication in A&A
The environment of the fast rotating star Achernar - Thermal infrared interferometry with VLTI/MIDI and SIMECA modeling
Context: As is the case of several other Be stars, Achernar is surrounded by
an envelope, recently detected by near-IR interferometry.
Aims: We search for the signature of circumstellar emission at distances of a
few stellar radii from Achernar, in the thermal IR domain.
Methods: We obtained interferometric observations on three VLTI baselines in
the N band (8-13 mic), using the MIDI instrument.
Results: From the measured visibilities, we derive the angular extension and
flux contribution of the N band circumstellar emission in the polar direction
of Achernar. The interferometrically resolved polar envelope contributes 13.4
+/- 2.5 % of the photospheric flux in the N band, with a full width at half
maximum of 9.9 +/- 2.3 mas (~ 6 Rstar). This flux contribution is in good
agreement with the photometric IR excess of 10-20% measured by fitting the
spectral energy distribution. Due to our limited azimuth coverage, we can only
establish an upper limit of 5-10% for the equatorial envelope. We compare the
observed properties of the envelope with an existing model of this star
computed with the SIMECA code.
Conclusions: The observed extended emission in the thermal IR along the polar
direction of Achernar is well reproduced by the existing SIMECA model. Already
detected at 2.2mic, this polar envelope is most probably an observational
signature of the fast wind ejected by the hot polar caps of the star.Comment: A&A Letter, in pres
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