TU Wien Research Data
Not a member yet
512 research outputs found
Sort by
Was wirt es doch des wunders noch (New_1536-7_n55) Audio recording
No full text<h1>Audio recording of a lute piece from the E-LAUTE project</h1><h2>Overview</h2><p>This dataset contains an audio recording of the piece "Was wirt es doch des wunders noch", a 16th century lute music piece originally notated in lute tablature, created as part of the E-LAUTE project (<a href="https://e-laute.info/">https://e-laute.info/</a>). The recording preserves and makes historical lute music from the German-speaking regions during 1450-1550 accessible.</p><p>The recording is based on the work with the title "Was wirt es doch des wunders noch" and the id "New_1536-7_n55" in the e-lautedb. It is found on the page(s) or folio(s) Ddiiijr-Eev in the source "Der ander theil des Lautenbúchs" with the source-id "New_1536-7".</p><p>The original source and multiple transcriptions of the work can be found on the E-LAUTE platform: <a href="https://edition.onb.ac.at/fedora/objects/o:lau.New_1536-7/methods/sdef:TEI/get?mode=n55" target="_blank">https://edition.onb.ac.at/fedora/objects/o:lau.New_1536-7/methods/sdef:TEI/get?mode=n55</a>.</p><p>Links to the source: <a href="https://nbn-resolving.org/urn:nbn:de:gbv:3:1-336930-p0001-4" target="_blank">https://nbn-resolving.org/urn:nbn:de:gbv:3:1-336930-p0001-4</a>, <a href="https://opac.rism.info/rism/Record/rism993104151" target="_blank">https://opac.rism.info/rism/Record/rism993104151</a>, <a href="https://gateway-bayern.de/VD16+ZV+11665" target="_blank">https://gateway-bayern.de/VD16+ZV+11665</a>, .</p><h2>Dataset Contents</h2><p>This dataset includes:</p><ul><li><strong>Audio file</strong>: An audio recording of the lute piece in .wav format</li> <li><strong>Metadata file</strong>: A metadata file with detailed information about the recording in .json format</li></ul><h2>About the E-LAUTE Project</h2><p><strong>E-LAUTE: Electronic Linked Annotated Unified Tablature Edition - The Lute in the German-Speaking Area 1450-1550</strong></p><p>The E-LAUTE project creates innovative digital editions of lute tablatures from the German-speaking area between 1450 and 1550. This interdisciplinary "open knowledge platform" combines musicology, music practice, music informatics, and literary studies to transform traditional editions into collaborative research spaces.</p><p>For more information, visit the project website: <a href="https://e-laute.info/">https://e-laute.info/</a></p>
Data - Koppenwallner et al. - Short pulse epiretinal stimulation allows focal activation of retinal ganglion cells
No full text<h2>Patch clamp data associated with <em>Koppenwallner et al. - Short pulse epiretinal stimulation allows focal activation of retinal ganglion cells</em></h2>
<p>Data, as well as simplified load and plot functions. The data is the basis for figures 2-4 in Koppenwallner et al. (<a href="https://doi.org/10.1109/TNSRE.2025.3529940">10.1109/TNSRE.2025.3529940</a>). Functionality includes loading results from a specified retinal ganglion cell (RGC) and plotting spiking output (e.g., membrane voltage over time) but does not perform threshold searching or other, more complex, analysis.</p>
<h3>Context and methodology</h3>
<ul>
<li>Data was created by patch clamp electrophysiology of mouse retinal ganglion cells</li>
<li>Electrical stimulation was applied to test the effect of 10-μs-long biphasic pulses on RGC activation threshold</li>
</ul>
<h3>Technical details</h3>
<ul>
<li>Data can directly be loaded and plotted in Matlab running <em>plotData.m</em> (tested in Matlab R2024b)</li>
<li>Parameters to be specified:
<ul>
<li><em>cellID</em> - identifier of each recorded cell, see list on top of <em>plotData.m</em>. Don't forget to add the folder prefix specifiying healthy (<em>wt</em>) and diseased (<em>rd</em>) animals</li>
<li><em>loc</em> - location of the stimulating electrode during the experiemtn (<em>soma</em> or <em>axon</em>)</li>
<li><em>dur</em> - pulse duration (10, 25, 50, 250 or 500, in us)</li>
</ul>
</li>
<li>The <em>Data</em> folder is structured into wild-type (<em>wt</em>, healthy animal) and retinal degneration (<em>rd</em>, blind animal) data</li>
<li>If help is needed feel free to reach out to Paul Werginz</li>
</ul><p>Epiretinal implants suffer from a lack of spatial resolution, which is greatly influenced by the undesired co-activation of distal cells with their axons passing close to targeted somas. Short current pulses in the range of 50μs have been shown to preferentially activate somas, but the low specificity may limit practical applications. In this paper, we explored decreasing pulse durations down to 10μs for achieving focal activation, i.e., a large differentiation between axonal and somatic activation in epiretinal configuration. We determined thresholds for pulses ranging between 10 and 500μs in retinal ganglion cells of both wild-type and photoreceptor-degenerated mouse retina. Ex-vivo stimulation using biphasic rectangular pulses was performed using a custom-built modified Howland-type current-controlled stimulator and a microelectrode. We demonstrate reliable direct activation of retinal ganglion cells using 10μs pulses for both somatic and axonal electrode positions. Cells from wild-type and photoreceptor-degenerated retinas exhibited similar thresholds. Axonal thresholds were significantly higher for all pulse durations, with the ratio between axonal and somatic thresholds strongly increasing with decreasing pulse duration (1.32 and 4.39 for pulse durations of 500 and 10μs, respectively). Computational modeling points to somatic polarization as the underlying mechanism for lower somatic thresholds. Our results demonstrate focal activation with pulses in the range of 10μs as a potential strategy to avoid the long-standing problem of axonal co-activation in epiretinal implants.</p>
Characterization of giant porous cages; porous-meltable and janus-type metal organic polyhedra
No full text<h2>Raw Data for three Publications entitled: </h2>
<h3>1. "Porous and Meltable Metal–Organic Polyhedra for the Generation and Shaping of Porous Mixed-Matrix Composites"</h3>
<p>This paper was published on 2024-03-11 in Journal of the American Chemical Society</p>
<p>J. Am. Chem. Soc. 2024, 146, 11, 7159–7164</p>
<p>DOI: 10.1021/jacs.4c00407</p>
<p>Authors: Cornelia von Baeckmann, Jordi Martínez-Esaín, José A. Suárez del Pino, Lingxin Meng, Joan Garcia-Masferrer, Jordi Faraudo, Jordi Sort, Arnau Carné-Sánchez<em><strong>, </strong>Daniel Maspoch</em></p>
<p><strong>Funded by: </strong>Austrian Sciene Fund (FWF, project number J4637) ; Spanish MINECO (project RTI2018-095622-B-I00), the Catalan AGAUR (projects 2021 SGR 00458 and 2021 SGR 00651), the CERCA Program/Generalitat de Catalunya, the MCIN/AEI/10.13039/501100011033, and by the European Union “NextGenerationEU”/PRTR (EUR2020-112294); ICN2 is supported by the Severo Ochoa program from the Spanish MINECO (grant SEV-2017-0706). The project that gave rise to these results received the support of a fellowship (LCF/BQ/PR20/11770011) from “la Caixa” Foundation (ID 100010434). A.C.S. is indebted to the Ramón y Cajal Program (RYC2020-029749-I Fellowship) and the Europa Excelencia grant (EUR2021-121997). J.F. acknowledges the financial support from MCIN/AEI/10.13039/501100011033 agency through Grant PID2021-124297NB-C33 and the “Severo Ochoa” Programme for Centres of Excellence in R&D (CEX2019-000917-S) awarded to ICMAB. We also thank the Government of Catalonia (AGAUR) for Grant 2021SGR01519. L.M. acknowledges the China Scholarship Council for scholarship support.</p>
<h3>2. " Stepwise assembly of heterometallic, heteroleptic “triblock Janus-type” metal–organic polyhedra" </h3>
<p>This paper was published on 2023-02-13 in Chem. Commun.</p>
<p>Chem. Commun., 2023, 59, 3423-3426</p>
<p>DOI: 10.1039/D2CC06815J </p>
<p>Authors: Cornelia von Baeckmann, Sara Ruiz-Relaño, Inhar Imaz, Marcel Handke, Judith Juanhuix , Felipe Gándara , Arnau Carné-Sanchez and Daniel Maspoch</p>
<p><strong>Funded by: </strong>Austrian Sciene Fund (FWF, project number J4637); Spanish MINECO (project RTI2018-095622-B-I00), the Catalan AGAUR (project 2021 SGR 00458), the CERCA Program/Generalitat de Catalunya, and the MCIN/AEI/10.13039/501100011033. ICN2 is supported by the Severo Ochoa program from the Spanish MINECO (grant SEV-2017-0706). The project that gave rise to these results received the support of a fellowship (LCF/BQ/PR20/11770011) from “la Caixa” Foundation (ID 100010434). </p>
<h3>3. "Giant oligomeric porous cage-based molecules" </h3>
<p>This paper was published on 2024-04-30 in Chemical Science</p>
<p>Chem. Sci., 2024, 15, 7992-7998</p>
<p>DOI: 10.1039/D4SC01974A</p>
<p>Authors: Alba Cortés-Martínez, Cornelia von Baeckmann, Laura Hernández-López, Arnau Carné-Sánchez and Daniel Maspoch</p>
<p><strong>Funded by: </strong>Austrian Sciene Fund (FWF, project number J4637); Europa Excelencia grant (EUR2021-121997) and the Catalan AGAUR (project 2017 SGR 238). It was also funded by the CERCA Programme/Generalitat de Catalunya. ICN2 is supported by the Severo Ochoa Centres of Excellence programme, Grant CEX2021-001214-S, funded by MCIN/AEI/10.13039.501100011033. A. C. S. is indebted to the Ramón y Cajal Program (RYC2020-029749-I Fellowship)</p>
<h2>Context and methodology</h2>
<p>In these three Publications the synthesis of giant porous cages; porous-meltable and Janus-type metal organic polyhedra are described. The publications and the corresponding supporting informations can be found as open-access files on the publisher´s websites (see DOI above). </p>
<p>Raw data files covering 1H and 13C NMR spectra, gas-adsorption measurments and SEM images for compounds described in these publications are uploaded. </p>
<h2>Technical details</h2>
<p>The Zip Files contains raw data obtained from nuclear magnetic resonance measurements; scanning electron microscopy images and gas adsorption measurments.</p>
<p>Specific software required for NMR data = Bruker TopSpin or MestreNova and for gas adsorption = Micromeritics</p>
<p>In case of questions; do not hesitate to contact the PI of this Project; Dr. Cornelia von Baeckmann ([email protected])</p>
<p> </p>
[Coree Rosina] (A-Wn_Mus.Hs._18688_n02) Audio recording
No full text<h1>Audio recording of a lute piece from the E-LAUTE project</h1><h2>Overview</h2><p>This dataset contains an audio recording of the piece "[Coree Rosina]", a 16th century lute music piece originally notated in lute tablature, created as part of the E-LAUTE project (<a href="https://e-laute.info/">https://e-laute.info/</a>). The recording preserves and makes historical lute music from the German-speaking regions during 1450-1550 accessible.</p><p>The recording is based on the work with the title "[Coree Rosina]" and the id "A-Wn_Mus.Hs._18688_n02" in the e-lautedb. It is found on the page(s) or folio(s) 5v in the source "[Lautentabulatur des Stephan Craus]" with the source-id "A-Wn_Mus.Hs._18688".</p><p>The original source and multiple transcriptions of the work can be found on the E-LAUTE platform: <a href="https://edition.onb.ac.at/fedora/objects/o:lau.A-Wn_Mus.Hs._18688/methods/sdef:TEI/get?mode=n02" target="_blank">https://edition.onb.ac.at/fedora/objects/o:lau.A-Wn_Mus.Hs._18688/methods/sdef:TEI/get?mode=n02</a>.</p><p>Links to the source: <a href="http://data.onb.ac.at/rec/AC14316391" target="_blank">http://data.onb.ac.at/rec/AC14316391</a>, <a href="https://rism.online/sources/600141880" target="_blank">https://rism.online/sources/600141880</a>, .</p><h2>Dataset Contents</h2><p>This dataset includes:</p><ul><li><strong>Audio file</strong>: An audio recording of the lute piece in .wav format</li> <li><strong>Metadata file</strong>: A metadata file with detailed information about the recording in .json format</li></ul><h2>About the E-LAUTE Project</h2><p><strong>E-LAUTE: Electronic Linked Annotated Unified Tablature Edition - The Lute in the German-Speaking Area 1450-1550</strong></p><p>The E-LAUTE project creates innovative digital editions of lute tablatures from the German-speaking area between 1450 and 1550. This interdisciplinary "open knowledge platform" combines musicology, music practice, music informatics, and literary studies to transform traditional editions into collaborative research spaces.</p><p>For more information, visit the project website: <a href="https://e-laute.info/">https://e-laute.info/</a></p>
Time series of VLBI radio source positions at X-band
No full text<h3>Content</h3>
<p>Time series of radio source positions at X-band from Very Long Baseline Interferometry.</p>
<p>Number of radio sources with session-wise estimated coordinates:</p>
<ul>
<li>5676 in vie_sx_250816a</li>
<li>5675 in vie_sx_250816b</li>
</ul>
<p>Positions of defining ICRF3sx radio sources which are not included in the respective _sts.txt file (~150) were fixed in the adjustment. About one half of the ICRF3sx defining sources was fixed in vie_sx_250816a solution, the other half in vie_sx_250816b.</p>
<h3>Dataset</h3>
<p>Time span: vgosDB from 1990.0 until 2025.5<br>Origin of input data: databases from IVS data center, usno observing program if not from IVS<br>Software used for analysis: VieVS v4.0</p>
<p>Source coordinates<br> - Apriori source coordinates: ICRF3sx<br> - Amplitude of Galactocentric acceleration vector: 5.8 uas/yr<br> - Epoch of coordinates: 2015.0</p>
<p>More details about the solution are provided in readme_vie_sx_250816_sts.txt file.</p>
<p>General information about the VLBI analysis done at the VIE IVS Analysis Center are given in <a title="VLBI Celestial and Terrestrial Reference Frames" href="https://doi.org/10.1051/0004-6361/202245434" target="_blank" rel="noopener">Krasna et al. (2023)</a></p>
<p> </p>
<h3>Acknowledgement</h3>
<p>The International VLBI Service for Geodesy and Astrometry (IVS) and all its components are acknowledged for providing VLBI data. </p>
Dataset for the Paper "Comparing Eye-Tracking and SSVEP-BCI Interfaces for Target Selection with a Projected Augmented Reality System"
No full text<h2>Description</h2>
<p>This is the dataset of the paper titled "Comparing Eye-Tracking and SSVEP-BCI Interfaces for Target Selection with a Projected Augmented Reality System".</p>
<p>The main goal is to assess two different eye-tracking systems and one SSVEP-BCI durin some static and moving tasks in Projected Augemented Reality environments.</p>
<h2>Abstract</h2>
<p><strong>Problem</strong>. Projected Augmented Reality (PAR) systems overlay virtual assets onto real-world horizontal surfaces in an asymmetric manner, making interaction performance highly dependent on user–surface distance. This limitation disproportionately affects people with severe motor disabilities, who cannot close this distance through voluntary movement.<br><strong>Aim</strong>. We investigate and compare three hands‑free input modalities, two eye‑tracking dwell‑based systems (300 ms and 2.5 s dwell times) and a steady‑state visually evoked potential Brain–Computer Interface (SSVEP‑BCI), for selecting both static and moving targets in an asymmetric PAR environment.<br><strong>Methods</strong>. We first derived appropriate metrics by adapting the Shannon Formulation for Fitts’ equation and the Hoffman variation to asymmetric target selection tasks. Then, in a within‑subjects study, 24 participants performed target‑selection tasks under static and moving target conditions using each input modality. Performance metrics included selection accuracy, task completion time, information throughput, and subjective user preference.<br><strong>Results</strong>. The slow eye‑tracking interface (2.5 s) yielded the best balance between error rate and throughput for static target selection, whereas the fast dwell‑based interface (300 ms) excelled at moving‑target selection. The SSVEP‑BCI achieved an average throughput of approximately 1 bit/s, comparable to desktop‑based SSVEP systems, and outperformed the slow dwell interface when selecting moving targets.<br><strong>Conclusion</strong>. Slow and fast dwell‑based eye‑tracking interfaces offer versatile solutions for static and dynamic target selection, respectively, while the SSVEP‑BCI represents a compelling alternative to slow dwell control for moving‑target interactions</p>
<h2>Dataset</h2>
<p>The dataset is composed of three different <code>.xlsx</code> files:</p>
<ol>
<li><strong>user_data.xlsx</strong>
<ol>
<li>data related to the users' knowledge of PAR systems and their expertise with the NextMind and the HoloLens 2 devices. </li>
<li>data related to the users' eyesight</li>
</ol>
</li>
<li><strong>static_data.xlsx</strong>: data collecetd during the<strong> static task</strong>
<ol>
<li>time out error</li>
<li>wrong selection error</li>
<li>throughput</li>
<li>ease of use</li>
<li>adoption</li>
<li>fatigue</li>
</ol>
</li>
<li><strong>moving_data.xlsx</strong>: data collecetd during the <strong>moving task</strong>
<ol>
<li>time out error</li>
<li>wrong selection error</li>
<li>throughput</li>
<li>ease of use</li>
<li>adoption</li>
<li>fatigue</li>
</ol>
</li>
</ol>
VLBI schedules for Galileo Frame Tie Study
No full text<h2>Description</h2>
<p>The dataset contains Very Long Baseline Interferometry (VLBI) schedules in form of NGS files that include observations of both quasars and Galileo satellites are were created with the scheduling software VieSched++ (version v1.3.1; <a href="https://iopscience.iop.org/article/10.1088/1538-3873/ab1820" target="_blank" rel="noopener">Schartner and Böhm 2019</a>, available on <a href="https://github.com/TUW-VieVS">GitHub</a>). These schedules are used to find the optimal distribution of VLBI transmitters (VT) in the Galileo space segement for frame ties. Therefore different numbers and distributions of Galileo satellites being equipped with a VT are investigated. The scenarios having either one, two or three satellites of the Galileo space segment equipped with a VT are investigated. </p>
<h3>Context and methodology</h3>
<p>In total, six different satellite configurations ("scenarios") are considered, varying in the number and orbital plane distribution of Galileo satellites equipped with a VT:</p>
<ul>
<li>1A – 1 satellite with VT in plane A</li>
<li>1A1B – 1 satellite with VT in plane A and 1 in plane B</li>
<li>2A – 2 satellites with VT in plane A</li>
<li>1A2B – 1 satellite with VT in plane A and 2 in plane B</li>
<li>3A – 3 satellites with VT in plane A</li>
<li>1A1B1C – 1 satellite with VT in each of the planes A, B, and C</li>
</ul>
<p>For each scenario, different proportions of satellite observations relative to the total number of observations are tested. These satellite-to-quasar observation ratios range from 10% to 60%, except for scenarios 1A and 1A1B, for which only 10% to 40% are tested due to limited visibility of the satellite(s).</p>
<p>Each schedule file is named according to the scenario and the satellite observation ratio. For example:</p>
<ul>
<li><strong>2A_10p</strong> refers to the scenario with <strong>two satellites in plane A</strong> and <strong>10%</strong> <strong>satellite observations</strong>.</li>
<li><strong>1A1B_30p</strong> refers to the scenario with <strong>one satellite in plane A and one in plane B</strong> and <strong>30%</strong> <strong>satellite observations</strong>.</li>
</ul>
Dataset of an experimental campaign of a Digital Twin for a biomass-to-SNG pilot plant
No full text<p>This dataset contains the results of the Digital Twin for a biomass-to-SNG pilot plant created within the <a href="https://projekte.ffg.at/projekt/3862075" target="_blank" rel="noopener">ADORe-SNG project</a>. </p>
<h2><strong>Changes</strong></h2>
<p>In version 1.1.0, a small error in the IPSEpro simulation data was corrected.</p>
<h2><strong>Context and methodology</strong></h2>
<ul>
<li>A Digital Twin was created for a biomass-to-SNG pilot plant at TU Wien.</li>
<li>The plant was automated and optimised using model predictive control (MPC), online process simulation and a soft sensor.</li>
<li>The data presented here is the output of these software tools that controlled the plant and were presented to the operators in real time.</li>
<li>The plant data stems from an excerpt of 9.5 hours from an experimental campaign in November 2023</li>
</ul>
<p>The dataset accompanies a publication wherein further details regarding methods can be found.</p>
<h2><strong>Technical details</strong></h2>
<ul>
<li>The data consist of four files:</li>
<ul>
<li>Two CSV files with the outputs of the MPC</li>
<ul>
<li>Data_MPC_DFB.csv with a sampling rate of 5 seconds</li>
<li>Data_MPC_Syngas.csv with a sampling rate of 1 second</li>
</ul>
<li>One CSV file with the results of the soft sensor</li>
<ul>
<li>Data_SoftSensor.csv with a sampling rate of 1 second retimed to 1 minute</li>
</ul>
<li>One JSON file with the inputs and outputs of the online process simulation in the software IPSEpro</li>
<ul>
<li>Data_IPSE.json with a sampling rate of 1 minute</li>
</ul>
</ul>
<li>The variable names in the files are explained in the attached README.txt</li>
</ul>
<h2><strong>Further details</strong></h2>
<p>For further details see the publication “Design and Implementation of a Digital Twin for a Biomass-to-Gas plant” by Stefan Jankovic, Lukas Stanger, Alexander Bartik, Martin Hammerschmid, Florian Benedikt, Michael Mittermayr, Matthias Binder, Martin Kozek and Stefan Müller submitted to “Applied Energy”</p>
Radio telescope dimensions for geodetic and astrometric VLBI thermal expansion modeling
No full text<h2>Description</h2>
<p>The dataset contains the dimensions of structural parts of radio telescopes used for geodetic and astrometric VLBI for the purpose of thermal expansion modeling in geodetic and astrometric VLBI Level-2 data analysis. New version as of 2025-10-26.</p>
<h3>Changes</h3>
<ul>
<li>Only format corrections and deletion of duplicate entry (WIDE85_3)</li>
</ul>
<h3>Context and methodology</h3>
<ul>
<li>The dataset belongs to publication: A<em>xel Nothnagel (2009) Conventions on thermal expansion modelling of radio telescopes for geodetic and astrometric VLBI; Journal of Geodesy, Vol. 83(3), 787-792, DOI: <a href="https://doi.org/10.1007/s00190-008-0284-z">10.1007/s00190-008-0284-z</a></em>, where the general concept of thermal expansion modeling is described.</li>
<li>The data was collected from on-site personnel who measured the dimensions of the structural parts or extracted them from construction drawings.</li>
</ul>
<h3>Technical details</h3>
<ul>
<li>The data is stored in fixed format ASCII, with the data of each telescope in a single line. The format is described in the header of the file. </li>
<li>No special software is needed to read and use the data.</li>
</ul>
K21-1883
No full text<h2>Related work</h2>
<p>This dataset is part of the digital documentation of the Tomb of Meret Neith, Umm el Qaab, Abydos, Egypt about 3000BC, its artefacts, and the reconstruction of the tomb. For an overview of the related work, please visit <a href="https://researchdata.tuwien.at/communities/meretneith/">https://researchdata.tuwien.at/communities/meretneith/</a>.</p>
<h2>Archaeological information</h2>
<h3>Object name</h3>
<p>Inscribed sealing fragment</p>
<h3>Object number(s)</h3>
<p>LN2153; K21-1883</p>
<h3>Description</h3>
<p>inscribed mud sealing fragment</p>
<h3>Location of object at time of photographs</h3>
<p>MoTA storage</p>
<h3>Find location</h3>
<p>Tomb Y; Y-3 (Petrie), Y-KK3 (DAI); context L36 S2</p>
<h3>Bibliography</h3>
<p>N/A</p>
<h2>Technical Information</h2>
<p>For imaging, Canon RAW and Apple RAW images were captured.</p>
<h3>Physical properties</h3>
<table>
<tbody>
<tr>
<td>Length (cm)</td>
<td>N/A</td>
</tr>
<tr>
<td>Width (cm)</td>
<td>N/A</td>
</tr>
<tr>
<td>Height (cm)</td>
<td>N/A</td>
</tr>
<tr>
<td>Weight (g)</td>
<td>N/A</td>
</tr>
<tr>
<td>Volume (cm3)</td>
<td>N/A</td>
</tr>
<tr>
<td>Density (g/cm3)</td>
<td>N/A</td>
</tr>
</tbody>
</table>
<h3>Comments</h3>
<p>not sufficient images for reconstruction</p>
<h3>Files overview</h3>
<ul>
<li><strong>images_videos.zip</strong> contains photographs of the real object in RAW format.</li>
<li>[optional] <strong>exports_{H,M,L}Q.zip</strong> archives contain the scanned object as 3D model in OBJ format including MTL and texture files. HQ, MQ, and LQ refer to high, medium and low quality versions of the model.</li>
<li>[optional] <strong>{objectName}_report.pdf</strong> contains further technical information of the reconstruction process.</li>
</ul>