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66 results for “ALMA”
ALMA Band 7 observations of G11.92-0.61 MM2
<p>We deposit the final data products underpinning this article:</p> <p>Filamentary mass accretion towards the high-mass protobinary system G11.92-0.61 MM2, Zhang et al. 2024, MNRAS, accepted (available at <a href="https://arxiv.org/abs/2407.19552">arxiv</a>)</p> <p>A detailed description of the data files are provided in README.md.</p>
Supplementary material of ALMA-IMF XV (Louvet et al. 2024)
<p>We show the supplementary material of the ALMA-IMF XV article, accepted by A&A on the 24th of July and accessible on arXiv with the identifier 2407.18719</p>
REsolved ALMA and SMA Observations of Nearby Stars (REASONS): Observation Logs
<p>Observation Details for millimetre-wavelength data gathered and modelled as part of the REsolved ALMA and SMA Observations of Nearby Stars (REASONS) paper (same DOI as this table). For the processed data and modelling results, see https://doi.org/10.5281/zenodo.12583396.</p> <ul> <li>Table A.1 refers to targets observed as part of the REASONS <em>Observational</em> ALMA program</li> <li>Table A.2 refers to targets observed as part of the REASONS <em>Observational</em> SMA program</li> <li>Table A.3 refers to targets previously observed whose raw data was retrieved from the ALMA archive and reanalysed as part of REASONS.</li> </ul>
Regular rotation and low turbulence in a diverse sample of z~4.5 galaxies observed with ALMA
<p>Clean [CII] line-emission datacubes, parameter files and outputs of 3DBarolo.</p>
Spectra and retrieval data from CO and HCN observations of Jupiter with ALMA (project 2016.1.01235.S)
<p>Spectra and retrieval data from:</p> <p>Title: Evidence for auroral influence on Jupiter's nitrogen and oxygen chemistry revealed by ALMA<br> Authors: T. Cavalié, L. Rezac, R. Moreno, E. Lellouch, T. Fouchet, B. Benmahi, T. K. Greathouse,<br> J. A. Sinclair, V. Hue, P. Hartogh, M. Dobrijevic, N. Carrasco, Z. Perrin<br> Journal: Nature Astronomy<br> Year: 2023</p> <p>########################<br> # Description of files #<br> ########################</p> <p>CO_data/<br> latitudes_CO.dat: planetocentric latitudes of the 540 pointings from which the CO spectra have been extracted<br> spectrum_*.dat : CO spectra, one per pointing. Frequency in GHz and continuum-subtracted flux density in Jy/beam<br> profiles_*.dat : vertical profiles, one per pointing. Pressure in mbar, temperature in K (local average, see paper for details), and retrieved CO volume mixing ratio</p> <p>HCN_data/<br> latitudes_HCN.dat: planetocentric latitudes of the 557 pointings from which the HCN spectra have been extracted<br> spectrum_*.dat : HCN spectra, one per pointing. Frequency in GHz and continuum-subtracted flux density in Jy/beam<br> profiles_*.dat : vertical profiles, one per pointing. Pressure in mbar, temperature in K (local average, see paper for details), and retrieved HCN volume mixing ratio</p> <p> </p>
ALMA-IMF + Single Dish data (B3 + MGPS90, B6 + BGPS)
<pre>For internal use of the ALMA-IMF consortium. Data will become public with the publication of Díaz-González, Daniel J. et al. (2023, submitted to AAS Journals). Version 1.0 contains combination of ALMA-IMF 12m bsensnobright images published in Paper II (Ginsburg et al. 2022) with BOLOCAM GPS for Band 6 (Aguirre et al. 2011, Ginsburg et al. 2013) and MGPS90 for Band 3 (Ginsburg et al. 2020). Combination was done using an adaptation of the uvcombine repository: <a href="https://github.com/radio-astro-tools/uvcombine">https://github.com/radio-astro-tools/uvcombine</a> For further inquiries contact: Daniel Jacobo Díaz González, d.diaz@irya.unam.mx Roberto Galván Madrid, r.galvan@irya.unam.mx </pre>
ALMA and VLA observations of the Extended Green Object G19.01-0.03
<p>In this repository, we deposit final data products that underlie the following two articles:</p> <p>- ALMA observations of the Extended Green Object G19.01--0.03 - I. A Keplerian disc in a massive protostellar system, Williams et al. 2022, MNRAS, 509, 748</p> <p>- ALMA observations of the Extended Green Object G19.01--0.03 - II. A massive protostar with typical chemical abundances surrounded by four low-mass prestellar core candidates, Williams et al. 2023, MNRAS, 525, 6146</p> <p>The included README.md file describes the data files in detail.</p>
Mock visibilities produced from ALMA Logo Cube
<p>CASA measurement sets produced from the ALMA Logo FITS Cube (https://doi.org/10.5281/zenodo.4460127) using CASA simobserve. Noiseless and Noisey measurement sets provided as tarred files.</p> <p>Sampled with the Cycle 7 43-7 antenna positions, at the location of HD 163296, for 3600s.</p>
FIGURE 11. Olisthella alma n. gen., n in Resolving the status of Pyriporoides and Daisyella (Bryozoa: Cheilostomata), with the systematics of some additional taxa of Calloporoidea having an ooecial heterozooid
FIGURE 11. Olisthella alma n. gen., n. sp., A C, holotype, NIWA 98229; B, E, F, paratype, NIWA 98230; D, unregistered, on same substratum as paratype: A, zooids, one with an ooecium; B, zooids with well-preserved cryptocystal shelves; C, ooecium of zooid illustrated in A; D, zooid in profile; E, reparative kenozooid functioning as an opesial closure; F, complete autozooid with opesia occluded by reparative kenozooid. Scalebars: A, 500 µm; B, 200 µm; C, D, F, 100 µm; E, 50 µm.
Animation, MESA inlists, and post-processing package for "Is Betelgeuse really rotating? Synthetic ALMA observations of large-scale convection in 3D simulations of Red Supergiants"
<p>Videos, post-processing package for mock ALMA observations, MESA (r23.05.1 with mesasdk-x86_64-linux-23.7.3) inlists and history files, Jupyter notebook and data to reproduce figures of the paper "Is Betelgeuse really rotating? Synthetic ALMA observations of large-scale convection in 3D simulations of Red Supergiants".</p>
PILETA FUENTE DEL ALMA
Pileta de piedra ubicada en Alhama de Granada Source: Objaverse 1.0 / Sketchfab
Friedrich Schlegel: O conceito de "ironia" e a arte como forma suprema do espírito & Schiller: A concepção da "alma bela" e da educação estética
<p>Esse seminário tem como objetivo enfatizar a importância dos pensamentos de <strong>Friedrich Schlegel & <strong>Schiller</strong></strong> para o ensino no curso de graduação em enfermagem.</p>
Vozes da alma (Stimmen der Seele)
<p><strong>Lizenz:</strong><br> Für den ganzen Film, wie für die Ausschnitte vergibt der Urheber Peter von Gunten die Lizenz: «Other: Not open» mit folgenden Präzisierungen:</p> <p>1. In jedem Fall ist der Titel des Films (<em>Vozes da alma</em>) und der Urheber Peter von Gunten anzugeben.</p> <p>2. Erlaubt ist der Gebrauch der ganzen Filme und von Ausschnitten im privaten Rahmen und für jede Anwendung im Bereich von Forschung und Bildung.</p> <p>3. Erlaubt ist die Zugänglichmachung der ganzen Filme oder von Ausschnitten daraus auf Online-Plattformen wie Youtube, Vimeo oder anderen Plattformen falls die Zugänglichmachung unter der gleichen Lizenz erfolgt.</p> <p>4. Eine Erlaubnis muss für alle öffentlichen kommerziellen und nichtkommerziellen Vorführungen (auch ohne Eintritt), Kinovorführungen, TV-Ausstrahlungen sowie für die Herstellung und den Vertrieb von DVD und allen weiteren und zukünftigen AV-Medien beim Urheber bzw. seinen Rechtsnachfolgern eingeholt werden.<br> <br> Peter von Gunten<br> Filmregisseur / Cinov Filmproduktion<br> Gerberngasse 27<br> 3011 Bern</p> <p><strong>Inhaltsangaben:</strong><br> Drei Monate lang folgte das Filmteam der afro-brasilianischen Heilerin Mae Gil (Gilvanete Dornelas Da Silva), die als Priesterin eines synkretistischen Candomblé-Kultes afrikanische Naturreligionspraxen mit christlichen Elementen vermischte. Im Zentrum des Films stehen denn auch Szenen, welche die Praxis des Heilens durch Anrufen der Geister und Tanzrituale zeigen.</p> <p><strong>Personen:</strong><br> Regie: Peter von Gunten<br> Produktion: Cinov AG<br> Buch: Peter von Gunten, Marian Zaugg<br> Kamera, Schnitt: Peter von Gunten<br> Ton: Pavol Jasovsky</p> <p><strong>Technische Angaben:</strong><br> Format: 16 mm, Farbe. Dauer: 180 Min. (Festivalversion). Produzierte Sprachversion: Portugiesisch mit deutschen Untertiteln. Weitere Versionen: 125 Min. (Verleih), 100 Min. (Fernsehen)<br> Aufnahmetechnik: Eclair ACL, Nagra 4-2 Quarz<br> Archivierte Elemente in Cinémathèque suisse (Lausanne), Signaturen: 1987 0735 01; 2005 1397 00</p> <p><em>Vozes da alma</em> ist auf LORY gespeichert, weil der Film eine Quelle für die Dissertation von Felix Rauh ist. Die Dissertation „Bewegte Bilder für eine entwickelte Welt. Die Dokumentarfilme von René Gardi, Ulrich Schweizer und Peter von Gunten in der Schweizer Entwicklungsdebatte, 1959-1986“ erschien 2018 als gedrucktes Buch im Chronos-Verlag und ist als Open Access-Publikation auf LORY zugänglich: DOI <a href="https://zenodo.org/record/1228755">https://zenodo.org/record/1228755</a> </p> <p>Die auf LORY gespeicherten MP4-Dateien von <em>Vozes da alma </em>(Version 125 Min. in HD, ganzer Film und Ausschnitt in:16:9) wurden von Felix Rauh hergestellt. Als Vorlage diente ein HD-Scan, den die Lichtspiel / Kinemathek Bern für diese Publikation neu mit der Kopie 1987 0735 01 aus der Cinémathèque suisse herstellte.</p> <p><strong>Dateien:</strong><br> 01_Vozes_da_alma_ganz<br> 02_Vozes_da_alma_Ausschnitt1_0.06.12-0.07.26</p>
Aquatic insect in Das Almas River
<p>Data set of aquatic insects collected in Das Almas River, Brazil, model and results.</p> <p>The first sheet is the all data, and the next five are the data used in occurrence bayseian analyses. There is a sheet with the model to be used in R environment and there are three sheets with results. The first is the values of sampled CODA, the second the estimation of number of taxa, and the last is the values of posterior distribution.</p>
ALMA cubes and integrated maps of the d203-506 protoplanetary disk
<p>These are the ALMA reduced data of the d203-506 protoplanetary disk. The data was obtained as part of the project 2017.1.01478.S (PI J.~Champion). The data was reduced at the ALMA regional node in Grenoble thanks to the help of Edwige Chapillon. </p>
ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1
<p>Input files and data for the MESA simulations in the paper "ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1". Runs where performed with version r23.05.1 of the MESA code using the MESA SDK version x86_64-linux-22.6.1. Folder named "Decin" contains the simulation with the new mass loss rate described in the paper, while the folder named NdJ contains the input files for the simulation performed with the Nieuwenhuijzen & de Jager rates.</p>
Ultrasound Evaluation and Vestibular Perception Thresholds Changes in Women Affected by Vestibulodynia (VBD) After One Cycle of Pixel CO2-Alma Fractionated Laser
ClinicalTrials.gov study NCT05156489. IPD Sharing: Not stated. Countries: 1. Publications: 8.
Latina Friends Motivating the Soul (ALMA)
ClinicalTrials.gov study NCT03749278. IPD Sharing: Not stated. Countries: 1. Publications: 2.
alma
<p>alma</p> <p> </p>
ALMA Titan image cubes for CH3CN, HC3N and HNC observed August 2016 and May 2017
<p>These 3D FITS files contain spectral line emission flux from Titan (in Janskys per beam) as a function of RA, dec. and frequency, observed using Atacama Large Millimeter/submillimeter Array (ALMA).</p> <p>ALMA observations of Titan were obtained on 2017-05-08 and 2017-05-16 (as part of ALMA program 2016.A.00014.S; PI: Cordiner) and on 2016-08-18 and 2016-08-19 (as part of ALMA program 2015.1.01023.S; PI: Gurwell). The HNC (J=4-3), HC3N (J=40-39) and CH3CN (J=19-18) transitions were observed in 2017, whereas the HNC (J=4-3), HC3N (J=39-38) and CH3CN (J=19-18) were observed in 2016.</p> <p>The raw observations were calibrated using standard scripts supplied by the observatory. The resulting measurement sets were continuum-subtracted using low-order polynomial fits to the line-free spectral regions adjacent to our lines of interest. The data were then imaged and cleaned (deconvolved) using the tclean algorithm in CASA 5.6. This routine implicitly corrects for the time-variability of Titan's position and radial velocity with respect to the observer, so the resulting image cubes are in the rest frame of Titan's center-of-mass. To facilitate meaningful intercomparisons, accounting for Titan's varying Geocentric distance, the 2016 and 2017 datasets were convolved to common circular beam dimensions, as projected in the plane of the sky. The image cubes were then cropped to isolate the emission lines of interest.</p>
ScienceDex guides
Understand access before you commit
These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.