cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.17909/7gnq-a471
title: Dataset for A Multi-Wavelength Study of the Symbiotic Mira HM Sge with SOFIA & HST

description: We have targeted the dusty symbiotic mira system HM Sge with four instruments from the IR to the UV. We have used these observations along with archival observations to study how the system has been evolving after its 1975 nova-like outburst. We have detected ro-vibrational water emission in a symbiotic system for the first time using new EXES high spectral resolution infrared spectroscopy. The features, detected in emission, have velocities consistent with the systemic velocity but do not show any clear evidence of high velocity outflows. Mid-infrared photometry and grism spectroscopy show that the oxygen-rich Asymptotic Giant Branch (AGB) dust and dust output has shown little to no change over the past 39 years. In the optical/UV, we detect three main NII nebular features that were detected 22 years ago, and they show little to no movement; several of the previously detected NII features are no longer visible. New UV spectroscopy has shown that the nebular environment continues to steadily relax after the system's 1975 outburst. The data suggest however, that the hot component has increased in temperature from 200,000 K in 1989 to now greater than 250,000 K. Our new and archival observations suggest that the evolution of the system after its outburst is swift with little to no major changes after a period of a couple years.
DOI: 10.17909/9074-ez94
title: HST/COS Europa torus scan

description: COS FUV observations with pointing in the equatorial plane different radial distances, between 8.0 and 12.5 Jupiter radii west to Jupiter.
DOI: 10.17909/9bdf-jn24
title: PHANGS-JWST First Results

description: These are the MAST Level 3 data that represent the observations used in the PHANGS-JWST first results.  The actual data used have had additional processing and can be accessed as described in the Lee et al. PHANGS-JWST survey paper.
DOI: 10.17909/ajqw-7w52
title: Data from "Detection of the Low-Mass Host Galaxy of a z~6.25 Quasar with JWST"

description: We characterize the stellar mass of J2239+0207, a z ∼ 6.25 sub-Eddington quasar (M1450 = −24.6),
using dedicated JWST/NIRCam medium-band observations of a nearby PSF star to remove the central
point source and reveal the underlying galaxy emission. We detect the host galaxy in two bands
longward of the Balmer break, and via calibration to existing Spitzer/IRAC data obtain a stellar
mass of ∼ 1010 M⊙, more than an order of magnitude less than this quasar’s existing measured [C II]
dynamical mass. We additionally calculate the mass of J2239+0207’s central supermassive black hole
using JWST/NIRSpec IFU observations, and determine that the black hole is ∼ 15 times more massive
than predicted by the local MBH-M∗ relation, similar to many high-redshift quasars with dynamical
masses determined via millimeter-wave line widths. We carefully consider potential selection effects
at play, and find that even when the z ∼ 6 quasars are compared to a local sample with similarly
determined dynamical masses, the high-redshift quasars appear to possess overmassive black holes. We
conclude z ∼ 6 quasars are likely to have a larger spread about the MBH-M∗ relation than observed
in the local Universe.
DOI: 10.17909/g5gk-wd13
title: SWP data 21 Peg
DOI: 10.17909/hm6d-qh67
title: Data from paper "Panchromatic HST/WFC3 Imaging Studies of Young, Rapidly Evolving Planetary Nebulae. II. NGC 7027"

description: HST/WFC3 images of NGC 7027 proposed by Dr. Joel H. Kastner (Proposal ID 15953).
DOI: 10.17909/nftp-e621
title: Abell2744 UNCOVER Photometric Catalog DR1

description: All deep HST and JWST in Abell 2744
DOI: 10.17909/w5qb-da07
title: TESS data of HD 182308 for RN
DOI: 10.25392/leicester.data.22203376.v1
title: Solar wind observations from BepiColombo MPO-MAG during Dec 2021

description: This dataset contains unreleased data from the BepiColombo mission for the periods 2021-12-06 to 2021-12-07 and 2021-12-24 to 2021-12-26 during the cruise phase to Mercury. In particular, it contains magnetic field observations from the MPO-MAG instrument (Heyner et al. 2021). <br> ****************IMPORTANT NOTE**************** <br> These data have not been released yet to the Planetary Science Archive (PSA). As consequence, they may still suffer some changes due to future calibrations before they are released to the PSA. <br> Therefore, <strong>we strongly encourage all the users to contact the following people before using this dataset.</strong> <br> - Dr Beatriz Sánchez-Cano, University of Leicester, BepiColombo Guest Investigator, bscmdr1@leicester.ac.uk <br> - Dr Daniel Heyner, TU Braunschweig, Principal Investigator of MPO-MAG, d.heyner@tu-bs.de <br> ********************************************************* File description: <br> It contains derived data from the outbound sensor. These files have 5 columns with the following information: <br> 1 -Data time 2 - Total magnetic field 3 - B_r component of the Magnetic Field 4 - B_t component of the Magnetic Field 5 - B_n component of the Magnetic Field <br> Reference: <br> D. Heyner et al.,(2021), The BepiColombo Planetary Magnetometer MPO-MAG: What can we Learn From the Hermean Magnetic Field? Space Sci Rev, 217, 52. https://doi.org/10.1007/s11214-021-00822-x <br> <br>
DOI: 10.4121/6ee9946f-9ff5-4019-9d91-03e1c5283210
title: Amsterdam floating litter dataset August 2022

description: This dataset contains counts of floating litter within the city center borough of Amsterdam. Floating items were visually identified and counted from quaywalls on August 23rd, and subsequently categorized using the River-OSPAR categorization. The dataset can be used to get a snapshot of plastic hotspot locations within the city center of Amsterdam.
DOI: 10.5281/zenodo.10602427
title: Dataset for Agiadi et al._Coupled otolith and foraminifera oxygen and carbon stable isotopes evidence paleoceanographic changes and fish metabolic responses
DOI: 10.5281/zenodo.11111158
title: Dataset: Reach characteristics and best-fit effective resistance

description: This dataset includes reach characteristics and model output for best-fit effective resistance for 37 river reaches in the Colorado Rockies.
DOI: 10.5281/zenodo.11136274
title: Extracted synthesis conditions for Nb:TiO2 films from scientific papers

description: The csv file contains the dataset for synthesis conditions for Nb doped TiO2 films extracted from scientific papers using a knowledge graph.
DOI: 10.5281/zenodo.12696571
title: Weak, Vertically Stronger Main Himalayan Thrust in the India-Asia Collision

description: This repository includes the used GNSS and InSAR data for the paper:

Li, S., Schulte-Pelkum, V., Barnhart, W. D., Karplus, M., Chen, L., Oncken, O., 2024. "Weak, Vertically Stronger Main Himalayan Thrust in the India-Asia Collision" submitted to Geophysical Research Letters.
DOI: 10.5281/zenodo.12724136
title: Three-dimensional atomic interface between metal and oxide in Zr-ZrO2 nanoparticles

description: Metal-oxide interfaces with poor coherency have unique properties comparing to the bulk materials and offer broad applications in the fields of heterogeneous catalysis, battery, and electronics. However, current understanding of the three-dimensional (3D) atomic metal-oxide interfaces remains limited because of their inherent structural complexity and limitations of conventional two-dimensional imaging techniques. Here, we determine the 3D atomic structure of metal-oxide interfaces in zirconium-zirconia nanoparticles using atomic-resolution electron tomography. We quantitatively analyze the atomic concentration and the degree of oxidation, and find the coherency and translational symmetry of the interfaces are broken. Atoms at the interface have low structural ordering, low coordination and elongated bond length. Moreover, we observe porous structures such as Zr vacancies and nano-pores and investigate their distribution. Our findings provide a clear 3D atomic picture of metal-oxide interface with direct experimental evidence. We anticipate this work could encourage future studies on fundamental problems of oxides such as interfacial structures in semiconductor and atomic motion during oxidation process.
DOI: 10.5281/zenodo.12789272
title: Code and data for "Comparing cost-effectiveness of radio and drone telemetry with playback surveys for assessing translocation outcomes"

description: Overview

Code and data used for the analyses of Stone et al., 2024 "Comparing cost-effectiveness of radio and drone telemetry with playback surveys for assessing translocation outcomes". Forthcoming in Journal of Applied Ecology

Abstract

1. Post-release monitoring is critical for assessing translocation outcomes. Yet the quality of information gained from monitoring can vary greatly, and perceived monitoring costs often results in reduced monitoring effort.  Selecting cost-effective monitoring strategies that provide high quality data is therefore important for assessing translocation outcomes and making informed management decisions. 2. To compare how monitoring strategy affects information gained, we monitored a toutouwai/North Island robin (Petroica longipes) reintroduction in Aotearoa New Zealand, based on monitoring objectives of determining survival, site fidelity and whether the extent of management was large enough to protect dispersing individuals. We compared how these objectives were met through four monitoring strategies: 1) comprehensive surveys with ground radio telemetry and playback; 2) aerial drone telemetry; 3) dedicated playback by trained surveyors and 4) opportunistic playback by predator control contractors. We undertook a viewshed analysis to determine search coverage of each strategy and compared detection rates, efficiency, and cost. 3. Comprehensive ground telemetry and playback, while costly, covered the largest area and provided the most accurate data on dispersal, survival and the translocation outcome.  In comparison, opportunistic playback monitoring detected substantially fewer individuals, giving a false impression of low site fidelity and survival and a failed translocation. Although drone telemetry had considerable site-specific limitations, which limited its effectiveness during our study, it was the most cost-effective with a high detection rate and low search effort. 4. Synthesis and applications: Our study shows the value of intensive monitoring in facilitating management decisions for wildlife translocations. Comprehensive telemetry and playback, while costly, were invaluable for gaining high quality information on the translocation outcome. Without suitable monitoring, reintroduction outcomes can be difficult to assess and potentially result in unnecessary, ineffective, or overly expensive management actions. We recommend that monitoring intensity and methodology should reflect the site, species and level of uncertainty regarding the translocation outcome. Prioritising monitoring can help reduce long-term costs, increase quality of information gained and allow for more informed management decisions that can improve subsequent translocation outcomes.
DOI: 10.5281/zenodo.2654726
title: Sensorscope Data

description: Environmental data from past Sensorscope deployments. Both the meteorological and the monitoring data are available for download. Each text file located in one of the archives bellow contains columns of delimited data from each SensorScope station that was deployed. Each archive also contains a text file which defines those columns. The entry NaN designates unavailable data.
DOI: 10.5281/zenodo.5848048
title: Dataset: A New Infrared Criterion for Selecting Active Galactic Nuclei to Lower Luminosities

description: The dataset accompanying the paper "A New Infrared Criterion for Selecting Active Galactic Nuclei to Lower Luminosities" (Hviding et al. in prep)
DOI: 10.5281/zenodo.7063813
title: Experimental Validation of Cryobot Thermal Models for the Exploration of Ocean Worlds

description: The tables in this repository represent the data used in the figures and analyses of the paper "Experimental Validation of Cryobot Thermal Models for the Exploration of Ocean Worlds", published in the Planetary Science Journal. The provided data was collected between 2020 and 2022. AllResults.xlsx: compilation of tables 4, 5, 6, and 7 on the paper. WarmA1.xlsx: data presented in figures 9, 10, and 11, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Total Power [W], H6 Power [W], H5 Power [W], H4 Power [W], H3 Power [W], H2 Power [W], H1 Power [W]". WarmA2.xlsx: data presented in figures 9, 10, and 11, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Total Power [W], H6 Power [W], H5 Power [W], H4 Power [W], H3 Power [W], H2 Power [W], H1 Power [W]". CryoA1.xlsx: data presented in tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth Estimation [m], Power [W]". CryoB1.xlsx: data presented in figures 9 and 10, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Power [W]". CryoB2.xlsx: data presented in figures 9, 10, 11, and 12, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Power [W]". CryoB3.xlsx: data presented in figures 6, 9, 10, 11, and 12, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Power [W]". CryoC1.xlsx: data presented in figures 9, 10, and 11, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Power [W]". CryoC2.xlsx: data presented in figures 9, 10, 11, and 12, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Depth [m], Power [W]". CryoC3.xlsx: data presented in figures 9, 10, and 11, and tables 4, 5, 6, and 7 on the paper. The spreadsheet columns are "Time [hrs], Truncated Coarse Depth [m], Power [W]".
description: Work at the Jet Propulsion Laboratory, California Institute of Technology, was carried out under a contract (80NM0018D0004) with the National Aeronautics and Space Administration (NASA) and with funding from a NASA Scientific Exploration Subsurface Access Mechanism for Europa (SESAME) grant (80NM0018F0560). Work at the University of Washington was carried out under the same SESAME grant (80NM0018F0560). Work at Stone Aerospace and MIT was carried out under a separate NASA SESAME grant (80NSSC19K0612), as well as under the MIT TVML Fellowship.
DOI: 10.5281/zenodo.7080391
title: Stellar luminosity tracks from Baraffe 1998

description: Stellar luminosity tracks from Baraffe 1998 as compiled by Tim Lichtenberg. Zenodo dataset created for 'showyourwork' integration and automated online paper build
DOI: 10.5281/zenodo.7529681
title: CR2MET: A high-resolution precipitation and temperature dataset for the period 1960-2021 in continental Chile.

description: The Center for Climate and Resilience Research Meteorological dataset (CR2MET) includes two spatially-distributed products of daily precipitation and maximum/minimum near surface temperatures. The dataset covers the domain of continental Chile over a regular 0.05 degree latitude-longitude grid, and spans the period 1960-2021. Both a products are built on statistical models of the corresponding variables, calibrated against quality-controlled observational records. The CR2MET models are nurtured with a combination of data that includes different variables from ECMWF reanalysis ERA5, topographic parameters and land-surface temperature estimates from the Moderate Resolution Imaging Spectroradiometer (MODIS) satellite sensor.
DOI: 10.5281/zenodo.7579831
title: Simulation Data for the article 'The Influence of Cloud Condensation Nucleus (CCN) Coagulation on the Venus Cloud Structure'

description: This dataset contains the NetCDF output files from simulations using PlanetCARMA in support of the work published in the manuscript, "The Influence of Cloud Condensation Nucleus (CCN) Coagulation on the Venus Cloud Structure." A summary of the included NetCDF data is found in the README file that is part of the data object. The submission version of this dataset contains only those simulations that provided data that were discussed in the accepted final manuscript. However, additional simulations were carried out in the course of the work, and are described in the manuscript. Upon request, the authors will revise this data repository by adding such data products from among that list as may be requested by others.
description: This work was supported through the NASA Akatsuki Participating Scientist Program Grant Numbers NNX11AD79G and NNH19ZDA001N. Portions of the Planet CARMA code were developed using SwRI Internal Resources.
DOI: 10.5281/zenodo.7946446
title: Bioverse: The Habitable Zone Inner Edge Discontinuity as an Imprint of Runaway Greenhouse Climates on Exoplanet Demographics

description: This repository contains data required to run the pipeline producing the results and figures in Schlecker+2023, in particular results objects created with expensive model grid runs of Bioverse.
DOI: 10.5281/zenodo.8377186
title: Protostellar cores in Sagittarius B2 N and M: continuum data

description: This is a set of self-calibrated continuum FITS files for the ALMA Cycle 4 project 2016.1.00550.S. The paper "Protostellar cores in Sagittarius B2 N and M" was accepted to ApJ on September 15, 2023. Paper abstract: We present 500 AU and 700 AU resolution 1 mm and 3 mm ALMA observations, respectively, of protostellar cores in protoclusters Sagittarius B2 (Sgr B2) North (N) and Main (M), parts of the most actively star-forming cloud in our Galaxy. Previous lower resolution (5000 AU) 3 mm observations of this region detected \(\sim\)150 sources inferred to be young stellar objects (YSOs) with \(M&gt;8\mathrm{\,M}_\odot\). With a tenfold increase in resolution, we detect 371 sources at 3 mm and 218 sources in the smaller field of view at 1 mm. The sources seen at low resolution are observed to fragment into an average of two objects. About a third of the observed sources fragment.Most of the sources we report are marginally resolved and are at least partially optically thick. We determine that the observed sources are most consistent with Stage 0/I YSOs, i.e., rotationally supported disks with an active protostar and an envelope, that are warmer than those observed in the solar neighborhood.We report source-counting-based inferred stellar mass and the star formation rate of the cloud: \(2800\mathrm{\,M}_\odot\), \(0.0038\mathrm{\,M}_\odot \mathrm{yr}^{-1}\) for Sgr B2 N and \(6900\mathrm{\,M}_\odot, 0.0093\mathrm{\,M}_\odot \mathrm{yr}^{-1}\) for Sgr B2 M respectively.
DOI: 10.5285/7d8e401b-2c75-4ee4-a753-c24b7e91e6e9
title: Atmospheric snow particle flux in the Central Arctic during MOSAiC 2019-20

description: Particle number flux of airborne snow particles was measured near-continuously at 1-min resolution above the sea ice surface from October 2019 to July 2020 during the year-round MOSAiC expedition. Sensors where mounted at 0.1 m and 10 m on the mast in MetCity on the MOSAiC ice floe drifting during the measurement period within an area of 79.2 N to 88.6 N and 2.7 W to 133.6 E. The SPC measurements were part of the BAS measurement suite during MOSAiC to quantify sea salt aerosol production from blowing snow above sea ice and potential impacts on clouds and climate. Instrument and data quality checks during the year-round campaign were carried out by BAS scientists and the MOSAiC ATMOS team. Funding was provided by UKRI Natural Environment Research Council (NERC) project "Sea Salt Aerosol above Arctic Sea Ice - sources, processes and climate impacts" (SSAASI-CLIM) grant NE/S00257X/1. The project was part of the international Multi-disciplinary drifting Observatory for the Study of Arctic Climate (MOSAiC) with the tag MOSAiC20192020.
description: To measure airborne snow particles Snow Particle Counters (SPC) (SPC-95, Niigata Electric Co., Ltd) were employed manufactured and calibrated in Japan. The open-path SPC has a wind vane to steer into the prevailing wind direction and is equipped with a super-luminescent diode sensor, which acts as a constant light source during the measurement. Once a snow particle enters the beam first the light energy detected by the upwind sensor decreases then that seen by the down-wind sensor. These signals are converted to two successive voltage pulses, which are proportional to particle size. Each signal is classified into one of 64 size classes (30 to 500 μm particle diameter). The SPC measures number flux of snow particles within each size class. Number flux can be converted into number concentration or drift density by dividing by horizontal wind speed from the nearest wind speed sensor on the mast (Level 2.4 NOAA doi:10.18739/A2K649V1F). The project was part of the international Multi-disciplinary drifting Observatory for the Study of Arctic Climate (MOSAiC) with the tag MOSAiC20192020.
description: Instrumentation used: Snow Particle Counters SPC-95 (Niigata Electric Co., Ltd)
description: The two SPC units (Unit 1104 at 0.1 m; Unit 1206 at 10 m) did run near-continuously from Oct 2019 until the end of Jul 2020, except during power cuts during March to May, and when the ice floe was abandoned for 5 weeks from mid-May 2020. SPC Unit 1104 started recording only from 2 Dec 2019. Calibrations were done for Unit 1104 on 19.06.2019 and for Unit 1206 26.09.2012. Unit 1206 showed occasionally malfunctioning: i) spurious small particle increases in the absence of drifting snow or precipitation, and ii) size spectra were clipped at the smaller sizes. In this data version no data were removed.
DOI: 10.5285/a07deacaffb8453e93d57ee214676304
title: ESA Lakes Climate Change Initiative (Lakes_cci): Lake products, Version 2.0.2

description: This dataset contains the Lakes Essential Climate Variable, which is comprised of processed satellite observations at the global scale, over the period 1992-2020, for over 2000 inland water bodies. This dataset was produced by the European Space Agency (ESA) Lakes Climate Change Initiative (Lakes_cci) project. For more information about the Lakes_cci please visit the project website. This is version 2.0.2 of the dataset. The five thematic climate variables included in this dataset are: • Lake Water Level (LWL), derived from satellite altimetry, is fundamental to understand the balance between water inputs and water loss and their connection with regional and global climate change. • Lake Water Extent (LWE), modelled from the relation between LWL and high-resolution spatial extent observed at set time-points, describes the areal extent of the water body. This allows the observation of drought in arid environments, expansion in high Asia, or impact of large-scale atmospheric oscillations on lakes in tropical regions for example. . • Lake Surface Water temperature (LSWT), derived from optical and thermal satellite observations, is correlated with regional air temperatures and is informative about vertical mixing regimes, driving biogeochemical cycling and seasonality. • Lake Ice Cover (LIC), determined from optical observations, describes the freeze-up in autumn and break-up of ice in spring, which are proxies for gradually changing climate patterns and seasonality. • Lake Water-Leaving Reflectance (LWLR), derived from optical satellite observations, is a direct indicator of biogeochemical processes and habitats in the visible part of the water column (e.g. seasonal phytoplankton biomass fluctuations), and an indicator of the frequency of extreme events (peak terrestrial run-off, changing mixing conditions). Data generated in the Lakes_cci are derived from multiple satellite sensors including: TOPEX/Poseidon, Jason, ENVISAT, SARAL, Sentinel 2-3, Landsat OLI, ERS, MODIS Terra/Aqua and Metop. Detailed information about the generation and validation of this dataset is available from the Lakes_cci documentation available on the project website.