440 research outputs found
A NARRADORA NA CONSTRUĂĂO DO FANTĂSTICO EM DOIS CONTOS DE AUGUSTA FARO
Resumo: Este artigo pretende discutir a construção do fantĂĄstico contemporĂąneo ou neofantĂĄstico na perspectiva da narradora nos contos âA friagemâ e âCheck-upâ, de Augusta Faro, integrantes da obra A friagem (1999). Para tanto, realiza-se uma breve abordagem de teĂłricos do fantĂĄstico como Todorov (2004), Roas (2014) e do neofantĂĄstico como Alazraki (1991). Objetiva-se, tambĂ©m, examinar a questĂŁo do sujeito da enunciação de acordo com Furtado (1980) e do narrador a partir de Fernandes (1996). Os contos de Faro focalizam o sujeito feminino em situaçÔes limite. Em âA friagemâ a personagem central estĂĄ prestes a congelar-se, baldados todos os esforços para debelar o problema. A solução surge com a aparição de Raimundo que reverte a situação. Em âCheck-upâ a narradora protagonista estĂĄ viva, entretanto seu coração estĂĄ clinicamente seco. ApĂłs configurar-se a presença de narradoras, verifica-se, tambĂ©m, que os contos possibilitam uma leitura alegĂłrica, o que confirma a presença do neofantĂĄstico.Palavras-chave: FantĂĄstico; NeofantĂĄstico; Narradora; âA friagemâ; âCheck-upâAbstract: This article aims at discussing the construct of contemporary fantastic or neofantastic from the narratorâs perspective in âA friagemâ and âCheck-upâ by Augusta Faro, which integrate the book âA friagemâ (1999). A brief approach to fantastic and neofantastic theoreticals such as Tododov (2004), Roas (2014) and Alazraki (1991) is made. Another objective is to examine the subject of enunciation according to Furtado (1980), and the narrator under Fernandesâs viewpoint (1996). Faroâs short stories focus on the female subject on the edge. In âA friagemâ, the main character is about to freeze herself, even after all efforts to avoid the situation. The solution appears with Raimundo, who reverts the events. In âCheck-upâ, the narrator and main character is alive, however, her heart is clinically dry. After configuring the female narrators, it is pointed that the short stories allow for the allegorical reading, which confirms the presence of the neofantastic.Keywords: Fantastic; Neofantastic; Narrator; âA friagemâ; âCheck-upâ
Climate outlooks serving agriculture
The Oklahoma Cooperative Extension Service periodically issues revisions to its publications. The most current edition is made available. For access to an earlier edition, if available for this title, please contact the Oklahoma State University Library Archives by email at [email protected] or by phone at 405-744-6311
Extending the Canada-France brown Dwarfs Survey to the near-infrared: first ultracool brown dwarfs from CFBDSIR
We present the first results of the ongoing Canada-France Brown Dwarfs
Survey-InfraRed, hereafter CFBDSIR, a Near InfraRed extension to the optical
wide-field survey CFBDS. Our final objectives are to constrain ultracool
atmosphere physics by finding a statistically significant sample of objects
cooler than 650K and to explore the ultracool brown dwarf mass function
building on a well defined sample of such objects. Candidates are identified in
CFHT/WIRCam J and CFHT/MegaCam z' images using optimised psf-fitting, and we
follow them up with pointed near infrared imaging with SOFI at NTT. We finally
obtain low resolution spectroscopy of the coolest candidates to characterise
their atmospheric physics. We have so far analysed and followed up all
candidates on the first 66 square degrees of the 335 square degrees survey. We
identified 55 T-dwarfs candidates with z'-J > 3:5 and have confirmed six of
them as T-dwarfs, including 3 that are strong later-than-T8 candidates, based
on their far-red and NIR colours. We also present here the NIR spectra of one
of these ultracool dwarfs, CFBDSIR1458+1013 which confirms it as one of the
coolest brown dwarf known, possibly in the 550-600K temperature range. From the
completed survey we expect to discover 10 to 15 dwarfs later than T8, more than
doubling the known number of such objects. This will enable detailed studies of
their extreme atmospheric properties and provide a stronger statistical base
for studies of their luminosity function.Comment: A&A, Accepte
Studying the complexity of change: toward an analytical framework for understanding deliberate social-ecological transformations
Faced with numerous seemingly intractable social and environmental challenges, many scholars and practitioners are increasingly interested in understanding how to actively engage and transform the existing systems holding such problems in place. Although a variety of analytical models have emerged in recent years, most emphasize either the social or ecological elements of such transformations rather than their coupled nature. To address this, first we have presented a definition of the core elements of a social-ecological system (SES) that could potentially be altered in a transformation. Second, we drew on insights about transformation from three branches of literature focused on radical change, i.e., social movements, socio-technical transitions, and social innovation, and gave consideration to the similarities and differences with the current studies by resilience scholars. Drawing on these findings, we have proposed a framework that outlines the process and phases of transformative change in an SES. Future research will be able to utilize the framework as a tool for analyzing the alteration of social-ecological feedbacks, identifying critical barriers and leverage points and assessing the outcome of social-ecological transformations
The background from single electromagnetic subcascades for a stereo system of air Cherenkov telescopes
The MAGIC experiment, a very large Imaging Air Cherenkov Telescope (IACT)
with sensitivity to low energy (E < 100 GeV) VHE gamma rays, has been operated
since 2004. It has been found that the gamma/hadron separation in IACTs becomes
much more difficult below 100 GeV [Albert et al 2008] A system of two large
telescopes may eventually be triggered by hadronic events containing Cherenkov
light from only one electromagnetic subcascade or two gamma subcascades, which
are products of the single pi^0 decay. This is a possible reason for the
deterioration of the experiment's sensitivity below 100 GeV. In this paper a
system of two MAGIC telescopes working in stereoscopic mode is studied using
Monte Carlo simulations. The detected images have similar shapes to that of
primary gamma-rays and they have small sizes (mainly below 400 photoelectrons
(p.e.)) which correspond to an energy of primary gamma-rays below 100 GeV. The
background from single or two electromagnetic subcascdes is concentrated at
energies below 200 GeV. Finally the number of background events is compared to
the number of VHE gamma-ray excess events from the Crab Nebula. The
investigated background survives simple cuts for sizes below 250 p.e. and thus
the experiment's sensitivity deteriorates at lower energies.Comment: 15 pages, 7 figures, published in Journ.of Phys.
Discovery of two L & T binaries with wide separations and peculiar photometric properties
We present spatially resolved photometric and spectroscopic observations of
two wide brown dwarf binaries uncovered by the SIMP near-infrared proper motion
survey. The first pair (SIMP J1619275+031350AB) has a separation of 0.691"
(15.2 AU) and components T2.5+T4.0, at the cooler end of the ill-understood
J-band brightening. The system is unusual in that the earlier-type primary is
bluer in J-Ks than the later-type secondary, whereas the reverse is expected
for binaries in the late-L to T dwarf range. This remarkable color reversal can
possibly be explained by very different cloud properties between the two
components. The second pair (SIMP J1501530-013506AB) consists of an L4.5+L5.5
(separation 0.96", 30-47 AU) with a surprisingly large flux ratio (Delta J
=1.79 mag) considering the similar spectral types of its components. The large
flux ratio could be explained if the primary is itself an equal-luminosity
binary, which would make it one of the first known triple brown dwarf systems.
Adaptive optics observations could not confirm this hypothesis, but it remains
a likely one, which may be verified by high-resolution near-infrared
spectroscopy. These two systems add to the handful of known brown dwarf
binaries amenable to resolved spectroscopy without the aid of adaptive optics
and constitute prime targets to test brown dwarf atmosphere models.Comment: accepted for publication in Ap
On key technologies for realising digital twins for structural dynamics applications
The term digital twin has gained increasing popularity over the last few years. The concept, loosely based on a virtual model framework that can replicate a particular system for contexts of interest over time, will require the development and integration of several key technologies in order to be fully realised. This paper, focusing on vibration-related problems in mechanical systems, discusses these key technologies as the building blocks of a digital twin. The example of a simulation digital twin that can be used for asset management is then considered. After briefly discussing the building blocks required, the process of data-augmented modelling is selected for detailed investigation. This concept is one of the defining characteristics of the digital twin idea, and using a simple numerical example, it is shown how augmenting a model with data can be used to compensate for the inherent model discrepancy. Finally the implications of this type of data augmentation for future digital twin technology is discussed
The ultracool-field dwarf luminosity-function and space density from the Canada-France Brown Dwarf Survey
Context. Thanks to recent and ongoing large scale surveys, hundreds of brown
dwarfs have been discovered in the last decade. The Canada-France Brown Dwarf
Survey is a wide-field survey for cool brown dwarfs conducted with the MegaCam
camera on the Canada-France-Hawaii Telescope telescope. Aims. Our objectives
are to find ultracool brown dwarfs and to constrain the field brown-dwarf
luminosity function and the mass function from a large and homogeneous sample
of L and T dwarfs. Methods. We identify candidates in CFHT/MegaCam i' and z'
images and follow them up with pointed near infrared (NIR) imaging on several
telescopes. Halfway through our survey we found ~50 T dwarfs and ~170 L or
ultra cool M dwarfs drawn from a larger sample of 1400 candidates with typical
ultracool dwarfs i' - z' colours, found in 780 square degrees. Results. We have
currently completed the NIR follow-up on a large part of the survey for all
candidates from mid-L dwarfs down to the latest T dwarfs known with utracool
dwarfs' colours. This allows us to draw on a complete and well defined sample
of 102 ultracool dwarfs to investigate the luminosity function and space
density of field dwarfs. Conclusions. We found the density of late L5 to T0
dwarfs to be 2.0pm0.8 x 10-3 objects pc-3, the density of T0.5 to T5.5 dwarfs
to be 1.4pm0.3 x 10-3 objects pc-3, and the density of T6 to T8 dwarfs to be
5.3pm3.1 x 10-3 objects pc-3 . We found that these results agree better with a
flat substellar mass function. Three latest dwarfs at the boundary between T
and Y dwarfs give the high density 8.3p9.0m5.1 x 10-3 objects pc-3. Although
the uncertainties are very large this suggests that many brown dwarfs should be
found in this late spectral type range, as expected from the cooling of brown
dwarfs, whatever their mass, down to very low temperature.Comment: Accepted for publication in A&
Weak Lensing with SDSS Commissioning Data: The Galaxy-Mass Correlation Function To 1/h Mpc
(abridged) We present measurements of galaxy-galaxy lensing from early
commissioning imaging data from the Sloan Digital Sky Survey (SDSS). We measure
a mean tangential shear around a stacked sample of foreground galaxies in three
bandpasses out to angular radii of 600'', detecting the shear signal at very
high statistical significance. The shear profile is well described by a
power-law. A variety of rigorous tests demonstrate the reality of the
gravitational lensing signal and confirm the uncertainty estimates. We
interpret our results by modeling the mass distributions of the foreground
galaxies as approximately isothermal spheres characterized by a velocity
dispersion and a truncation radius. The velocity dispersion is constrained to
be 150-190 km/s at 95% confidence (145-195 km/s including systematic
uncertainties), consistent with previous determinations but with smaller error
bars. Our detection of shear at large angular radii sets a 95% confidence lower
limit , corresponding to a physical radius of
kpc, implying that galaxy halos extend to very large radii. However, it is
likely that this is being biased high by diffuse matter in the halos of groups
and clusters. We also present a preliminary determination of the galaxy-mass
correlation function finding a correlation length similar to the galaxy
autocorrelation function and consistency with a low matter density universe
with modest bias. The full SDSS will cover an area 44 times larger and provide
spectroscopic redshifts for the foreground galaxies, making it possible to
greatly improve the precision of these constraints, measure additional
parameters such as halo shape, and measure the properties of dark matter halos
separately for many different classes of galaxies.Comment: 28 pages, 11 figures, submitted to A
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