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15 results for “Shooter”
Real and Synthetic Dataset for Active Shooter Situations
<p>This dataset includes annotations for shooters (both person and visible portion of the gun) and guns in a primarily indoor setting. The synthetic data was generated using Unreal Engine 4 and Unreal Engine 5 and contains both the default semi-realistic textures of the environments and segmentation masks as a form of domain randomization. The textured synthetic data was further augmented with camera sensor effects as another domain adaptation technique. The folders use the following notation: T denotes textured synthetic, M denotes masked synthetic, R denotes real, and the prefix A denotes augmented. We also include some annotated videos for evaluating tracking performance.</p>
Can a Wi-Fi WLAN Support a First Person Shooter?
<p>Jose Saldana, Juan Luis de la Cruz, Luis Sequeira, Julian Fernandez-Navajas, Jose Ruiz-Mas, "Can a Wi-Fi WLAN Support a First Person Shooter?," NetGames 2015, The 14th International Workshop on Network and Systems Support for Games Zagreb, Croatia, December 3-4, 2015.<br /> ISBN: 978-1-5090-0067-8</p> <p>This work has been partially ?nanced by the EU H2020 Wi-5 project (Grant Agreement no: 644262), and European Social Fund in collaboration with the Government of Aragon.</p> <p><br /> - The file "netgames_2015_in_proc.pdf" contains the paper published in the proceedings of the conference.</p> <p><br /> - Support files and results:</p> <p><br /> "captures" directory contains the ".pcap" captures made for both tests using Wireshark.</p> <p><br /> "files" directory contains the filtered data from the captures or from the D-ITG raw output. The ".log" files are binary. They have been obtained with D-ITG (Distributed Internet Traffic Generator, http://traffic.comics.unina.it/software/ITG/)</p> <p>A. Botta, A. Dainotti, A. Pescapè, "A tool for the generation of realistic network workload for emerging networking scenarios", Computer Networks (Elsevier), 2012, Volume 56, Issue 15, pp 3531-3547. </p> <p> </p> <p>"src" directory contains the ".m" matlab script and functions used for processing the raw data obtained. MATLAB R2013 compatible. It also includes the ".fig" files, to be opened with the same version of MATLAB.</p> <p>NOTE: It is MANDATORY adding the directories to the MATLAB path.</p> <p>Juan Luis de la Cruz, September 2015</p> <p> </p> <p><em>Abstract</em>—In corporate and commercial environments, the deployment of a set of coordinated Wi-Fi APs is becoming a common solution to provide Internet coverage to moving users. In these scenarios, real-time services as online games can also be present. This paper presents a set of experiments developed in a test scenario where an end device moves between different APs while generating game traffic. A WLAN solution based on virtual APs is used, in order to make the handoffs transparent for Layer 3. The results show that it is possible to maintain an acceptable level of subjective quality during the handoff. At the same time, it is set clear that the fact of having a gamer in an AP could be taken into account by radio resource management algorithms, in order to provide a better quality.</p>
PENELLOPE - X-Shooter spectra of targets in the Chamaeleon I, eta Cha, and eps Cha regions
<p>Spectra of the targets in the Chamaeleon I, eps-Cha and eta-Cha regions observed with the VLT/X-Shooter spectrograph. These spectra are part of the PENELLOPE Large Program and are obtained close in time to the HST/ULLYSES spectra of the same targets. </p><p>Here one can find the 1D absolute flux-calibrated and telluric corrected spectra. Each object is observed simultaneously in three arms, UVB, VIS, and NIR, and the spectrum of each arm is saved in one file. The units of the spectra are: Flux [erg/s/cm2/nm]; Wavelength [nm]. In some cases, multiple observations for one target have been taken.</p><p>Data are public, we ask to ask to the authors of this release, who contributed to the observation preparation and data reduction, whether they want to be included in any publication using these data. The data reduction procedure is presented in Manara et al. (2021). Please quote this paper in any related publication. Please contact Carlo Manara for estimates of the stellar and accretion properties of these targets based on this data. </p><p>For questions or comments please contact Carlo Manara, cmanara@eso.org</p>
PENELLOPE - X-Shooter spectra of targets in the Taurus and CrA regions (survey targets)
<p>Spectra of the targets in the Taurus and CrA regions observed with the VLT/X-Shooter spectrograph. These spectra are part of the PENELLOPE Large Program and are obtained close in time to the HST/ULLYSES spectra of the same targets. </p><p>Here one can find the 1D absolute flux-calibrated and telluric corrected spectra. Each object is observed simultaneously in three arms, UVB, VIS, and NIR, and the spectrum of each arm is saved in one file. The units of the spectra are: Flux [erg/s/cm2/nm]; Wavelength [nm]. In some cases, multiple observations for one target have been taken.</p><p>Data are public, we ask to ask to the authors of this release, who contributed to the observation preparation and data reduction, whether they want to be included in any publication using these data. The data reduction procedure is presented in Manara et al. (2021). Please quote this paper in any related publication. Please contact Carlo Manara for estimates of the stellar and accretion properties of these targets based on this data. </p><p>For questions or comments please contact Carlo Manara, cmanara@eso.org</p>
PENELLOPE - X-Shooter spectra of targets in Lupus (all survey targets)
<p>Spectra of the targets in the Lupus star-forming region observed with the VLT/X-Shooter spectrograph. These spectra are part of the PENELLOPE Large Program and are obtained close in time to the HST/ULLYSES spectra of the same targets. </p><p>Here one can find the 1D absolute flux-calibrated and telluric corrected spectra. Each object is observed simultaneously in three arms, UVB, VIS, and NIR, and the spectrum of each arm is saved in one file. The units of the spectra are: Flux [erg/s/cm2/nm]; Wavelength [nm]. In some cases, multiple observations for one target have been taken.</p><p>Data are public, we ask to ask to the authors of this release, who contributed to the observation preparation and data reduction, whether they want to be included in any publication using these data. The data reduction procedure is presented in Manara et al. (2021). Please quote this paper in any related publication. Please contact Carlo Manara for estimates of the stellar and accretion properties of these targets based on this data. </p><p>For questions or comments please contact Carlo Manara, cmanara@eso.org</p><p> </p>
Investigating the asymmetry of young stellar outflows: A combined MUSE-X-Shooter study of the Th 28 jet
<h3>This record contains supplementary tables and figures for the article <em>'Investigating the asymmetry of young stellar outflows: A combined MUSE-X-Shooter study of the Th 28 jet' </em>by A. Murphy, E. T. Whelan, F. Bacciotti, D. Coffey, F. Comeron, J. Eisloffel, B. Nisini, S. Antoniucci, J. M. Alcala and T. P. Ray, accepted for publication by Astronomy & Astrophysics.</h3> <p> </p> <p><strong>Abstract: </strong></p> <p>Characterising stellar jet asymmetries is key to providing robust constraints for jet launching models, and hence to understanding the underlying mechanisms of jet launching. This study aims to characterise the asymmetric properties of the bipolar jet from the Classical T Tauri Star Th 28. We combine data from integral field spectroscopy with VLT/MUSE and high-resolution spectra from VLT/X-Shooter to map optical emission line ratios in both jet lobes. We carry out a diagnostic analysis of these ratios to compare the density, electron temperature, and ionisation fraction within both lobes. The mass accretion rate is derived from the emission lines at the source, and compared with the mass outflow rate derived in both lobes using the estimated densities and measured [O I]λ6300 and [S II]λ6731 luminosities. The blue-shifted jet shows a significantly higher electron temperature and moderately higher ionisation fraction than the red-shifted jet. In contrast to previous studies we also estimate higher densities n H in the blue-shifted jet by a factor ∼2. These asymmetries are traced to within 1′′ (160 au) of the source in the line ratio maps. We find Ṁacc = 2.4 × 10^−7 M⊙ yr ^−1 , with an estimated obscuration factor of ∼54 due to grey scattering around the star. Estimated values of Ṁout range between 0.66 – 13.7 × 10^−9 M⊙ yr^−1 in the blue-shifted jet and 5-9 × 10^−9 M⊙ yr^−1 in the red-shifted jet.<em> </em>The emission line maps and diagnostic results suggest that the jet asymmetries originate close to the source and are likely intrinsic to the jet. Furthermore, the combined dataset allows access to a broad array of accretion tracers. This in turn enables a more accurate estimation of the mass accretion rate, revealing Ṁacc higher by a factor > 350 than would otherwise be determined.</p> <p> </p> <p><strong>Summary of supplemental material:</strong></p> <p>Table 1: Emission lines detected in X-shooter observations of the jet. Fluxes are measured from the red-shifted jet lobe.</p> <p>Tables 2 and 3: Mass accretion rates measured from MUSE and X-Shooter observations of Th 28, respectively, assuming an on-source extinction of 2.5 mags.</p> <p>Tables 4 and 5: As in Tables 2 and 3, for an on-source extinction of 1.26 mags.</p> <p>Figures 1-4: Position-velocity maps of detected emission lines from the UV and VIS arms of the X-shooter observations.</p> <p>Figure 5: Accretion luminosities measured from MUSE and X-Shooter data, before and after correction for on-source obscuration. Left and right panels show the corresponding values if the fluxes are corrected for a wavelength-dependent extinction of 2.5 and 1.26 mags, respectively.</p> <div> </div> <div> </div>
Data for the paper "Effective Emission Heights of Various OH Lines From X-shooter and SABER Observations of a Passing Quasi-2-Day Wave"
<p>The provided ASCII tables are related to the paper "Effective Emission Heights of Various OH Lines From X-shooter and SABER Observations of a Passing Quasi-2-Day Wave", which has been published in Journal of Geophysical Research: Atmospheres, Vol. 127, 2022 (DOI: 10.1029/2022JD036610).</p>
Data for the paper "Climatologies of Various OH Lines From About 90,000 X-shooter spectra"
<p>The provided ASCII tables are related to the paper "Climatologies of Various OH Lines From About 90,000 X-shooter spectra", which has been published in Journal of Geophysical Research: Atmospheres, Vol. 128, 2023 (DOI: 10.1029/2022JD038275).</p> <p>v1.0.0: initial submission</p> <p>v1.1.0: ohclp_linepar.dat with additional column for line wavelengths</p>
PENELLOPE - X-Shooter spectra of targets in the Orion OB1 and sigma-Orionis regions
<p>Spectra of the targets in the Orion OB1 and sigma Orionis regions observed with the VLT/X-Shooter spectrograph in November-December 2020. These spectra are part of the PENELLOPE Large Program and are obtained close in time to the HST/ULLYSES spectra of the same targets. </p> <p>Here one can find the 1D absolute flux-calibrated and telluric corrected spectra. Each object is observed simultaneously in three arms, UVB, VIS, and NIR, and the spectrum of each arm is saved in one file. The units of the spectra are: Flux [erg/s/cm2/nm]; Wavelength [nm].</p> <p>Data are public, we ask to ask to the authors of this release, who contributed to the observation preparation and data reduction, whether they want to be included in any publication using these data. The data are presented in Manara et al. (2021), currently in prep.</p> <p>For questions or comments please contact Carlo Manara, cmanara@eso.org</p>
Shooters Hill Milestone
A milestone on Shooters Hill (north side) just east of Red Lion Place, London. A sign on one side reads: "7 MILES TO DARTFORD". 141 photos taken in June 2022 with a Sony a7R III and processed in Reality Capture. Source: Objaverse 1.0 / Sketchfab
PENELLOPE - X-Shooter spectra of targets in the Lupus and Chamaeleon regions observed in 2021
<p>Spectra of the targets in the Lupus, Chamaeleon I and eta-Cha regions observed with the VLT/X-Shooter spectrograph in May-August 2021. These spectra are part of the PENELLOPE Large Program and are obtained close in time to the HST/ULLYSES spectra of the same targets. </p> <p>Here one can find the 1D absolute flux-calibrated and telluric corrected spectra. Each object is observed simultaneously in three arms, UVB, VIS, and NIR, and the spectrum of each arm is saved in one file. The units of the spectra are: Flux [erg/s/cm2/nm]; Wavelength [nm]. In some cases, multiple observations for one target have been taken.</p> <p>Data are public, we ask to ask to the authors of this release, who contributed to the observation preparation and data reduction, whether they want to be included in any publication using these data. The data reduction procedure is presented in Manara et al. (2021). Please quote this paper in any related publication. Please contact Carlo Manara for estimates of the stellar and accretion properties of these targets based on this data. </p> <p>For questions or comments please contact Carlo Manara, cmanara@eso.org</p>
Shooters Hill Mounting Block
A portland stone horse mounting block located slightly east of and opposite the junction of Kenilworth Gardens and Shooters Hill, London. Date: (probably) 18th Century. https://historicengland.org.uk/listing/the-list/list-entry/1289811 125 photos taken in June 2022 with a Sony a7R III and processed in Reality Capture. Source: Objaverse 1.0 / Sketchfab
Shooters Hill Spigot Mortar
A spigot mortar emplacement at the north west corner of Eltham Common (in the trees at the corner of the buildings), Shooters Hill, London. This spigot mortar featured in Series 15, Episode 6 of Time Team where the surrounding trench and cast iron revetment were excavated. https://archaeologydataservice.ac.uk/archives/view/dob/ai_full_r.cfm?refno=6759 166 photos taken in June 2022 with a Sony a7R III and processed in Reality Capture. Source: Objaverse 1.0 / Sketchfab
X-Shooter spectrum of VHS 1256-1257 b
<p>A detailed description of these data is provided in Petrus et al. 2022</p>
Effect of Violent First-Person Shooter (FPS) Video Games on Shooting Accuracy
ClinicalTrials.gov study NCT03445156. IPD Sharing: YES. Countries: 0. Publications: 0.
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