23,014 research outputs found
Predicting the Quality of Short Narratives from Social Media
An important and difficult challenge in building computational models for
narratives is the automatic evaluation of narrative quality. Quality evaluation
connects narrative understanding and generation as generation systems need to
evaluate their own products. To circumvent difficulties in acquiring
annotations, we employ upvotes in social media as an approximate measure for
story quality. We collected 54,484 answers from a crowd-powered
question-and-answer website, Quora, and then used active learning to build a
classifier that labeled 28,320 answers as stories. To predict the number of
upvotes without the use of social network features, we create neural networks
that model textual regions and the interdependence among regions, which serve
as strong benchmarks for future research. To our best knowledge, this is the
first large-scale study for automatic evaluation of narrative quality.Comment: 7 pages, 2 figures. Accepted at the 2017 IJCAI conferenc
Revisiting the distance, environment and supernova properties of SNR G57.2+0.8 that hosts SGR 1935+2154
We have performed a multi-wavelength study of supernova remnant (SNR)
G57.2+0.8 and its environment. The SNR hosts the magnetar SGR 1935+2154, which
emitted an extremely bright ms-duration radio burst on 2020 Apr 28 (The
Chime/Frb Collaboration et al. 2020; Bochenek et al. 2020). We used the 12CO
and 13CO J=1-0 data from the Milky Way Image Scroll Painting (MWISP) CO line
survey to search for molecular gas associated with G57.2+0.8, in order to
constrain the physical parameters (e.g., the distance) of the SNR and its
magnetar. We report that SNR G57.2+0.8 is likely impacting the molecular clouds
(MCs) at the local standard of rest (LSR) velocity V_{LSR} ~ 30 km/s and
excites a weak 1720 MHz OH maser with a peak flux density of 47 mJy/beam. The
chance coincidence of a random OH spot falling in the SNR is <12%, and the
OH-CO correspondence chance is 7% at the maser spot. This combines to give < 1%
false probability of the OH maser, suggesting a real maser detection. The LSR
velocity of the MCs places the SNR and magnetar at a kinematic distance of
d=6.6 +/- 0.7 kpc. The nondetection of thermal X-ray emission from the SNR and
the relatively dense environment suggests G57.2+0.8 be an evolved SNR with an
age (d/6.6 kpc) yr. The explosion energy of G57.2+0.8 is
lower than erg,
which is not very energetic even assuming a high ambient density = 10
cm. This reinforces the opinion that magnetars do not necessarily result
from very energetic supernova explosions.Comment: 9 pages, 5 figures, accepted for publication in the Astrophysical
Journa
Effect of Qianliexin capsule on quality of life, NIH-CPSI score and IIEF-5 score in patients with prostatitis complicated with erectile dysfunction
Purpose: To study the influence of Qianliexin capsule on quality of life, NIH-CPS Index, and 5-item version of the 15-item International Index of Erectile Function (IIEF-5) scores in patients with prostatitis complicated with erectile dysfunction (ED).Methods: Patients with prostatitis complicated with ED (128) who were treated from November 2015 to December 2017 participated in this study. The patients were assigned to two groups (64 per group) according to the treatment given: study group which was given routine treatment plus Qianliexin capsule, and control group which received routine treatment only. Clinical effectiveness, adverse reactions, Quality of Life-Bref (QOL-BREF) scores, etc, of the two groups were determined.Results: The QOL-BREF score of the study group was significantly higher than that of the control group (p < 0.05). While NIH-CPSI scores were significantly decreased in both groups, the decrease in the study group was lower (p < 0.05). In contrast, IIEF-5 score significantly increased in both groups, but the increase in the study group was higher than in control (p < 0.05).Conclusion: Qianliexin capsule is an effective and reasonably safely drug for enhancing the quality of life, NIH-CPSI and IIEF-5 scores, as well as the lecithin bodies in prostatitis patients with ED.Keywords: Qianliexin capsule, Prostatitis, Erectile dysfunction NIH-CPSI score, IIEF-5 scor
Multi-wavelength Stellar Polarimetry of the Filamentary Cloud IC5146: I. Dust Properties
We present optical and near-infrared stellar polarization observations toward
the dark filamentary clouds associated with IC5146. The data allow us to
investigate the dust properties (this paper) and the magnetic field structure
(Paper II). A total of 2022 background stars were detected in -, -,
-, and/or -bands to mag. The ratio of the polarization
percentage at different wavelengths provides an estimate of ,
the wavelength of peak polarization, which is an indicator of the small-size
cutoff of the grain size distribution. The grain size distribution seems to
significantly change at 3 mag, where both the average and dispersion
of decrease. In addition, we found
0.6-0.9 m for mag, which is larger than the 0.55 m
in the general ISM, suggesting that grain growth has already started in low
regions. Our data also reveal that polarization efficiency (PE ) decreases with as a power-law in -, -, and
-bands with indices of -0.710.10, -1.230.10 and -0.530.09.
However, -band data show a power index change; the PE varies with
steeply (index of -0.950.30) when mag but softly
(index of -0.250.06) for greater values. The soft decay of PE in
high regions is consistent with the Radiative Aligned Torque model,
suggesting that our data trace the magnetic field to mag.
Furthermore, the breakpoint found in -band is similar to the where we
found the dispersion significantly decreased. Therefore, the
flat PE- in high regions implies that the power index changes result
from additional grain growth.Comment: 31 pages, 17 figures, and 3 tables; accepted for publication in Ap
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