research data records

This file contains raw data for cameras and wearables of the ConfLab dataset.

./cameras

contains the overhead video recordings for 9 cameras (cam2-10) in MP4 files.

These cameras cover the whole interaction floor, with camera 2 capturing the

bottom of the scene layout, and camera 10 capturing top of the scene layout.

Note that cam5 ran out of battery before the other cameras and thus the recordings

are cut short. However, cam4 and 6 contain significant overlap with cam 5, to

reconstruct any information needed.

Note that the annotations are made and provided in 2 minute segments.

The annotated portions of the video include the last 3min38sec of x2xxx.MP4

video files, and the first 12 min of x3xxx.MP4 files for cameras (2,4,6,8,10),

with "x" being the placeholder character in the mp4 file names. If one wishes

to separate the video into 2 min segments as we did, the "video-splitting.sh"

script is provided.

./camera-calibration contains the camera instrinsic files obtained from

https://github.com/idiap/multicamera-calibration. Camera extrinsic parameters can

be calculated using the existing intrinsic parameters and the instructions in the

multicamera-calibration repo. The coordinates in the image are provided by the

crosses marked on the floor, which are visible in the video recordings.

The crosses are 1m apart (=100cm).

./wearables

subdirectory includes the IMU, proximity and audio data from each

participant at the Conflab event (48 in total). In the directory numbered

by participant ID, the following data are included:

1. raw audio file

2. proximity (bluetooth) pings (RSSI) file (raw and csv) and a visualization

3. Tri-axial accelerometer data (raw and csv) and a visualization

4. Tri-axial gyroscope data (raw and csv) and a visualization

5. Tri-axial magnetometer data (raw and csv) and a visualization

6. Game rotation vector (raw and csv), recorded in quaternions.

All files are timestamped.

The sampling frequencies are:

- audio: 1250 Hz

- rest: around 50Hz. However, the sample rate is not fixed

and instead the timestamps should be used.

For rotation, the game rotation vector's output frequency is limited by the

actual sampling frequency of the magnetometer. For more information, please refer to

https://invensense.tdk.com/wp-content/uploads/2016/06/DS-000189-ICM-20948-v1.3.pdf

Audio files in this folder are in raw binary form. The following can be used to convert

them to WAV files (1250Hz):

ffmpeg -f s16le -ar 1250 -ac 1 -i /path/to/audio/file

Synchronization of cameras and werables data

Raw videos contain timecode information which matches the timestamps of the data in

the "wearables" folder. The starting timecode of a video can be read as:

ffprobe -hide_banner -show_streams -i /path/to/video

./audio

./sync: contains wav files per each subject

./sync_files: auxiliary csv files used to sync the audio. Can be used to improve the synchronization.

The code used for syncing the audio can be found here:

https://github.com/TUDelft-SPC-Lab/conflab/tree/master/preprocessing/audio

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DAWN GRaND Mars Bundle: Raw Data Collection

This dataset presents the quantitative raw data that was collected under the H2020 RRI2SCALE project for the D1.4 - “Large scale regional citizen surveys report”. The dataset includes the answers that were provided by almost 8,000 participants from 4 pilot European regions (Kriti, Vestland, Galicia, and Overijssel) regarding the general public's views, concerns, and moral issues about the current and future trajectories of their RTD&I ecosystem. The original survey questionnaire was created by White Research SRL and disseminated to the regions through supporting pilot partners. Data collection took place from June 2020 to September 2020 through 4 different waves – one for each region. Based on the conclusion of a consortium vote during the kick-off meeting, it was decided that instead of resource-intensive methods that would render data collection unduly expensive, to fill in the quotas responses were collected through online panels by survey companies that were used for each region. For the statistical analysis of the data and the conclusions drawn from the analysis, you can access the "Large scale regional citizen surveys report" (D1.4).

This collection consists of raw image products acquired by the TTCam instrument during the Lucy Mission Dinkinesh Encounter. The purpose of the Dinkinesh encounter was primarily as an in-flight test of an autonomous range-finding and tracking system that is a critical component of Lucy's operations.

NEAR Raw TRO Data Collection This collection was migrated from PDS3 to PDS4 in 2024 by the Radio Science Sub-Node. This bundle contains all the raw data from the PDS3 data sets NEAR_A_RSS_1_5_EROS_FLYBY_V1_0, NEAR_A_RSS_1_5_EROS_ORBIT_V1_0, and NEAR_A_RSS_1_5_MATHILDE_V1_0.

The East Australian Current mooring raw data collection 2021-2022 contains all the raw instrument data files and instrument setup information, build documentation, deployment and recovery log sheets and scanned paper documentation for the deployment covering the period May, 2021 to July, 2022. Quality controlled data and gridded data products from this mooring deployment can be accessed via the links in the Related Links section of this collection record. Lineage: The raw data instrument data files and associated documentation were collected from the East Australian Current (EAC) moorings (6 moorings) during the 2021-2022 deployment. The deployment voyage was undertaken on the Marine National Facility voyage IN2021_V03 and recovery on IN2022_V06. Data included in the collection is in the instrument formats created from each instrument type. The data was uploaded from each instrument at the end of the deployment and these uploaded files are what are included in this collection.
Documentation in the collection includes scanned paper notes, log sheets in excel format, pdf diagrams of the moorings, instrument setup files and other documentation considered essential records associated with the deployment. No quality control or data analysis has been completed on the data in this collection, quality controlled data and data products are available through the links section.

The raw data and coding table of the manuscript: The relationship between insecure attachment and Machiavellianism

This collection contains raw panchromatic (350 - 850 nm) images acquired by the L'LORRI instrument during the Lucy Mission Dinkinesh Encounter.

The East Australian Current mooring raw data collection 2018-2019 contains all the raw instrument data files and instrument setup information, build documentation, deployment and recovery log sheets and scanned paper documentation for the deployment covering the period April, 2018 to September, 2019. Quality controlled data and gridded data products from this mooring deployment can be accessed via the links in the Related Links section of this collection record. Lineage: The raw data instrument data files and associated documentation were collected from the East Australian Current (EAC) moorings (6 moorings) during the 2018-2019 deployment. The deployment voyage was undertaken on the Marine National Facility voyage IN2018_V03 and the recovery on IN2019_V05. Data included in the collection is in the instrument formats created from each instrument type. The data was uploaded from each instrument at the end of the deployment and these uploaded files are what are included in this collection. Documentation in the collection includes scanned paper notes, log sheets in excel format, pdf diagrams of the moorings, instrument setup files and other documentation considered essential records associated with the deployment. No quality control or data analysis has been completed on the data in this collection, quality controlled data and data products are available through the links section.

CaSSIS

CaSSIS (Colour and Stereo Surface Imaging System), is a high-resolution, 4.5 m per pixel (15 ft/pixel), colour stereo camera, designed for building accurate digital elevation models of the Martian surface. CaSSIS is designed to acquire targeted images of Mars at a rate of 10–20 images per day from a roughly circular orbit 400 km above the surface. Each image can be acquired in up to four colours and stereo capability is provided by the use of a novel rotation mechanism. A typical product from one image acquisition will be a 9.5 km × ∼45 km swath, in full colour and in stereo, and from one over-flight of the target thereby reducing atmospheric influences inherent in stereo and colour products from previous high resolution imagers. The Principal Investigator is Nick Thomas, from the University of Bern, Switzerland.

The Raw_Data Collection

The raw data collection contains the raw science and housekeeping data from the instrument and the data is released publicly on a daily basis with a six month lag from the data being obtained. Physically the collection is organised by science phase, then orbit range in groups of 100 orbits, then orbit. Housekeeping is then organised into a Housekeeping directory. Science data is organised into a Science directory, then by CaSSIS unique ID (to distinguish a single observation), then CaSSIS filter. The reason for this separation is that a single observation can have up to a few hundred raw frame lets per filter, so each science directory will contain from tens to hundreds of files. (Note a download from the PSA will also include accompanying browse images but these are actually housed in the Browse Collection.)
A description of the raw data products can be found in the CaSSIS Experiment to Archive ICD (EAICD). This can be found under documents in the user interface or via the Document Collection in the PSA ftp distribution. A quick start guide can also be found at:

This collection consists of raw image products acquired by the MVIC instrument during the Lucy Mission Dinkinesh Encounter.

The Mars Global Surveyor (MGS) Radio Science (RS) Raw Data Archive (RDA) is a time-ordered collection of raw and partially processed data collected during the MGS Mission to Mars. For more information on the investigations proposed see [TYLERETAL1992].

This collection contains all the raw data collected from the XRS instrument during the NEAR mission.

The East Australian Current mooring raw data collection 2016-2018 contains all the raw instrument data files and instrument setup information, build documentation, deployment and recovery log sheets and scanned paper documentation for the deployment covering the period November, 2016 to May, 2018. Quality controlled data and gridded data products from this mooring deployment can be accessed via the links in the Related Links section of this collection record. Lineage: The raw data instrument data files and associated documentation were collected from the East Australian Current (EAC) moorings (6 moorings) during the 2016-2018 deployment. The deployment voyage was undertaken on the Marine National Facility voyage IN2016_V06 and the recovery on IN2018_V03. Data included in the collection is in the instrument formats created from each instrument type. The data was uploaded from each instrument at the end of the deployment and these uploaded files are what are included in this collection.
Documentation in the collection includes scanned paper notes, log sheets in excel format, pdf diagrams of the moorings, instrument setup files and other documentation considered essential records associated with the deployment. No quality control or data analysis has been completed on the data in this collection, quality controlled data and data products are available through the links section.

The raw data in a compressed archive of .CINE format video files created and analyzed in the research project focused on moth drinking rates and proboscis submergence for adult Manduca sexta.This is the raw data for the submission to PLOS ONE titled "Feeding rate in adult Manduca sexta is unaffected by proboscis submergence depth."The file data_package.tar.gz is a gzip-compressed tar archive containing the video files used for the analysis described in the mentioned paper, which is implemented by the code in the GitHub repository at https://github.com/Tomas-Pierce-at-UNC/MothDrinks.Each video in the archive is in the .cine format defined by Phantom Vision and depicts a feeding bout for a moth and date identified in the file name. Video data is 8-bit and single-channel (grayscale). The code expects the data files to be within a folder named data2/ within the same folder the code is stored, so that the relative file paths for data files are data2/*.cine.

NEAR RSS Raw Ionosphere Data Collection

This collection consists of raw science products acquired by the L'TES instrument during the Lucy Mission Dinkinesh Encounter.

Raw water quality data collected from a fixed pier at 1 meter below mean lower low water. Instrument collecting data is a YSI 6600 V4 sonde with a conductivity/temperature probe, strain gauge pressure sensor, optical dissolved oxygen probe, optical fluorescence chlorophyll probe, optical fluorescence turbidity probe and potentiometric glass bulb pH probe. Data are raw and not flagged or curated in any manner other than curtailed for deployment periods where the YSI sonde is deployed in the water. Download at your own risk. These data may be used and redistributed for free but they are not intended for legal use, since they may contain inaccuracies. For use for publications please reference the Central and Northern California Ocean Observing system (CeNCOOS) and NOAA. Neither the data provider, CeNCOOS, NOAA, nor the United States Government, nor any of their employees or contractors, makes any warranty, express or implied, including warranties of merchantability and fitness for a particular purpose, or assumes any legal liability for the accuracy, completeness, or usefulness, or this information. Please see http://erddap.cencoos.org/erddap/tabledap/tiburon-water-tibc1.html for QA/QC data with flagging.