176 research outputs found
Kepler Archive Manual
A description of Kepler, its design, performance and operational constraints may be found in the Kepler Instrument Handbook (KIH, Van Cleve Caldwell 2016). A description of Kepler calibration and data processing is described in the Kepler Data Processing Handbook (KDPH, Jenkins et al. 2016; Fanelli et al. 2011). Science users should also consult the special ApJ Letters devoted to early Kepler results and mission design (April 2010, ApJL, Vol. 713 L79-L207). Additional technical details regarding the data processing and data qualities can be found in the Kepler Data Characteristics Handbook (KDCH, Christiansen et al. 2013) and the Data Release Notes (DRN). This archive manual specifically documents the file formats, as they exist for the last data release of Kepler, Data Release 25(KSCI-19065-002). The earlier versions of the archive manual and data release notes act as documentation for the earlier versions of the data files
Gastrointestinal nematodes of goats: host–parasite relationship differences in breeds at summer mountain pasture in northern Italy
Introduction: The Orobic goat is a hardy breed native to the Orobic Alps (Lombardy, northern Italy). The aim of the study was the assessment of gastrointestinal nematode (GIN) egg excretion in Alpine and Saanen (cosmopolite breeds) and Orobic grazing goats, after a strategic treatment with eprinomectin in late June.
Material and methods: Individual faecal samples from a mixed flock of cosmopolite and Orobic goats were collected and analysed by the FLOTAC double technique every three weeks from June to September.
Results: Strongylida was the primary GIN infection observed in goats that grazed on Alpine pastures; a strategic treatment with eprinomectin led to a prolonged reduction of egg excretion during the whole study period. Egg excretion was also influenced by breed. Pluriparous Orobic does were able to control reinfection better than the pluriparous cosmopolite does. Regarding Nematodirus sp. eggs per gram of faeces (EPG), the autochthonous Orobic breed presented higher values than the cosmopolite breeds. However, cosmopolite goats presented higher EPG values of Strongyloides papillosus than their Orobic counterparts in August.
Conclusions: Further studies on genetic features of local autochthonous goats, such as the Orobic breed, are needed, since they could reveal peculiar characteristics of susceptibility, resistance or resilience to GIN infection, providing genetic resources for selection
The frequency of nuclear star-formation in Seyfert 2 galaxies
We investigate the detectability of starburst signatures in the nuclear
spectrum of Seyfert 2 galaxies by constructing spectral models in the
wavelength range 3500-4100A, combining the spectrum of a bulge population (of
age ~10Gyr) with that of younger stellar populations, spanning ages from ~3 Myr
to 1 Gyr. We also construct models combining the bulge template with a
power-law (PL) continuum, which is observed in some Seyfert 2's in polarized
light, contributing with typically 10-40% of the flux at 4020A. We conclude
that such continuum cannot be distinguished from that of a very young stellar
population (age < 10 Myr), contributing with less than ~0.02% of the mass of
the bulge. The models are compared with nuclear spectra - corresponding to a
radius of 200-300 pc at the galaxy - of 20 Seyfert 2 galaxies, in which we
specifically look for the signatures above of young to intermediate age stellar
populations. We find them in ten galaxies, thus 50% of the sample. But only in
six cases (30% of the sample) they can be attributed to young stars (age < 500
Myr): Mrk 1210, ESO 362-G8, NGC 5135, NGC 5643, NGC 7130 and NGC 7582. In the
remaining four cases, the signatures are due to intermediate age stars (~1
Gyr). We find a tendency for the young stars to be found more frequently among
the late type Seyfert's. This tendency is supported by a comparison between the
equivalent widths (W) of absorption lines of the nuclear spectra of the Seyfert
2's with those of normal galaxies of the same Hubble type.Comment: 18 figures, revised version published in ApJ, December 2000, vol.
544, p. 74
Planet Hunters: Assessing the Kepler Inventory of Short Period Planets
We present the results from a search of data from the first 33.5 days of the
Kepler science mission (Quarter 1) for exoplanet transits by the Planet Hunters
citizen science project. Planet Hunters enlists members of the general public
to visually identify transits in the publicly released Kepler light curves via
the World Wide Web. Over 24,000 volunteers reviewed the Kepler Quarter 1 data
set. We examine the abundance of \geq 2 R\oplus planets on short period (< 15
days) orbits based on Planet Hunters detections. We present these results along
with an analysis of the detection efficiency of human classifiers to identify
planetary transits including a comparison to the Kepler inventory of planet
candidates. Although performance drops rapidly for smaller radii, \geq 4
R\oplus Planet Hunters \geq 85% efficient at identifying transit signals for
planets with periods less than 15 days for the Kepler sample of target stars.
Our high efficiency rate for simulated transits along with recovery of the
majority of Kepler \geq 4 R\oplus planets suggest suggests the Kepler inventory
of \geq 4 R\oplus short period planets is nearly complete.Comment: 41 pages,13 figures, 8 tables, accepted to Ap
Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)
\We present the sixth catalog of Kepler candidate planets based on nearly 4
years of high precision photometry. This catalog builds on the legacy of
previous catalogs released by the Kepler project and includes 1493 new Kepler
Objects of Interest (KOIs) of which 554 are planet candidates, and 131 of these
candidates have best fit radii <1.5 R_earth. This brings the total number of
KOIs and planet candidates to 7305 and 4173 respectively. We suspect that many
of these new candidates at the low signal-to-noise limit may be false alarms
created by instrumental noise, and discuss our efforts to identify such
objects. We re-evaluate all previously published KOIs with orbital periods of
>50 days to provide a consistently vetted sample that can be used to improve
planet occurrence rate calculations. We discuss the performance of our planet
detection algorithms, and the consistency of our vetting products. The full
catalog is publicly available at the NASA Exoplanet Archive.Comment: 18 pages, to be published in the Astrophysical Journal Supplement
Serie
Saints and lovers: myths of the avant-garde in Michel Georges-Michel's Les Montparnos
This article examines Michel Georges-Michelâs 1924 novel Les Montparnos as a study of the myths circulating around the Montparnasse avant-garde of the 1920s, and their function in relation to art. Key amongst these myths is the idea of art as a religion, according to which avant-garde artists are conceived as secular saints and martyrs. While this notion of artist as saint is strongly present in early-twentieth-century biographies of Van Gogh, Georges-Michel explicitly relates his fictionalized version of Modiglianiâs life not to such recent models but rather to the Renaissance masters, and especially to Raphael, a link which is explained in terms of the post-war âretour Ă lâordreâ in French artistic culture. The novelâs references to Raphael as archetypal painter-lover are also related to its construction of a myth of the artist as virile and sexually prolific, and to its identification of creative and sexual impulses
OASIS integral-field spectroscopy of the central kpc in 11 Seyfert 2 galaxies
We map narrow-line regions (NLRs) of 11 nearby Seyfert 2 galaxies with the
optical integral-field spectrograph OASIS mounted at CFHT. We model
emission-line profiles of 5 forbidden-line doublets and 2 Balmer lines,
correcting for the underlying stellar absorption by reconstructing stellar
spectra with synthetic evolutionary stellar population models. For each of the
11 targets, we present 2D maps of surface brightness in the observed emission
lines, diagnostic line intensity ratios, gas kinematics (mean line-of-sight
velocity and velocity dispersion), electron density, and interstellar
reddening, and we plot spatially resolved spectral-diagnostic diagrams. The
stellar data are represented by maps of mean line-of-sight (LOS) velocities and
of the relative mass fractions of the young stellar populations. The gas
velocity fields in 80% of the sample exhibit twisted S-shaped isovelocity
contours, which are signatures of non-circular orbits and indicate
non-axisymmetric gravitational potentials, gas motions out of the galactic
plane, or possible outflows and inflows. Based on the kinematic measurements,
we identified a possible nuclear ring or radial gas flow in NGC 262 (Mrk 348),
not reported before. Eight of the eleven observed objects exhibit strongly
asymmetric or multi-component emission-line profiles, in most cases confined to
an elongated region passing through the galactic centre, perpendicular to the
major axis of emission.Comment: 40 pages, 25 figure
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