cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5e057d027e85d
title: Parkes observations for project P1032 semester 2019OCTS_07

description: We propose timing observations of southern double neutron star (DNS) systems to obtain precise estimates of the component masses and thus increase the statistics of neutron star mass distribution. The improved sensitivity of the Ultra Wideband Low (UWL) receiver will provide a 3X increase in the precision of the time of arrivals (ToAs) of the pulses compared to the multibeam data. This has the potential to perform quick measurements of masses for a number of binary systems in the next 1-2 years. We will also use MeerKAT observations at crucial orbital phases to increase our chances of mass measurements. Increase in the number of measured NS masses has significant implications for understanding NS internal structure and for stellar and binary evolution physics.
DOI: 10.14458/hu.res.2016.2
title: พฤติกรรมการสื่อสารในองค์การ: กรณีศึกษาโรงแรมไตรตรัง บีช รีสอร์ท ภูเก็ต
DOI: 10.14458/hu.res.2016.3
title: ศักยภาพการจัดการกลุ่มวิสาหกิจชุมชนสุชาวดี ตำบลปริก อำเภอสะเดา จังหวัดสงขลา
DOI: 10.14458/hu.res.2016.4
title: ปัจจัยที่มีความสัมพันธ์กับคุณภาพบัณฑิต และคุณภาพงานวิจัยในสถาบันอุดมศึกษา
DOI: 10.14458/hu.res.2016.5
title: พฤติกรรมและความพึงพอใจของนักท่องเที่ยวชาวมาเลเซียต่อการท่องเที่ยวเชิงวัฒนธรรมในพื้นที่จังหวัดสงขลา
DOI: 10.14458/hu.res.2016.6
title: ปัจจัยแวดล้อมที่มีความสัมพันธ์กับความผูกพันของบุคลากรต่อองค์กร : สำนักงานก่อสร้างชลประทานที่ 16 กองพัฒนาแหล่งน้ำขนาดกลาง
DOI: 10.7910/dvn/hnvkjq/i2axag
title: Fukumoto_Matsuo_replication.tar.gz

description: :unav
DOI: 10.7910/dvn/nr6dsh/sluznu
title: pack.tar.gz

description: :unav
DOI: 10.7910/dvn/nr6dsh/zcti8x
title: readme.txt

description: :unav
DOI: 10.7910/dvn/pqr36b/khtksd
title: packaging_self-tests-testing_report_q2_final_report_060614.pdf

description: Final study report. Questionnaires in annex.
DOI: 10.7910/dvn/8hapxb/6k4lol
title: G045.5-04.3DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/avre3p
title: G041.3+03.2DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/co0agc
title: G041.5+02.3DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/co5wtl
title: G048.3-01.7DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/ii2atz
title: G043.3+03.1DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/viwjb7
title: G026.9-03.5DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/wl5rfn
title: G046.5-03.3DistanceAG.pdf

description: :unav
DOI: 10.17632/63pc653jgg.1
title: A simulation optimization tool for incorporating occupancy data in scheduling building equipment

description: The following zip file contains the codes and research data for the implementation of the simulation optimization framework proposed in the associated paper. Detailed step-by-step instructions for running the code is provided in the "Instructions.docx" file. You will need both MATLAB and GAMS (with an MIP solver) installed on your computer to be able to use the code and replicate the results presented in the paper.
DOI: 10.7910/dvn/8hapxb/1omkqd
title: G048.9+02.3DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/1trsnk
title: G042.0-00.9DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/awm6jl
title: G030.3+01.2DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/cxzfws
title: G036.6-00.9DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/em0n40
title: G029.6+03.7DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/fo6rzq
title: G046.2+03.1DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/o2wu4y
title: G035.0+00.6DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/rmrfjk
title: G037.5+04.0DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/xrhzjb
title: G046.2-01.6DistanceAG.pdf

description: :unav
DOI: 10.17632/zdj7trnzr5.1
title: Supplementary Data for: Basalt lava flows of the intraplate Newer Volcanic Province in south-east Australia (Melbourne region): 40Ar/39Ar geochronology reveals ~8 Ma of episodic activity.

description: Supplementary 40Ar/39Ar and XRF Data for: Basalt lava flows of the intraplate Newer Volcanic Province in south-east Australia (Melbourne region): 40Ar/39Ar geochronology reveals ~8 Ma of episodic activity.
DOI: 10.7910/dvn/8hapxb/1ekvrs
title: G046.9-02.9DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/a5tm45
title: G037.0-01.4DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/iwczuz
title: G049.0+03.4DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/ksswdc
title: G030.6-03.6DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/okawbn
title: G028.8-01.9DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/qysagj
title: G043.2+02.1DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/vfou8a
title: G044.8+04.0DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/x4qaxd
title: G027.8-02.1DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/xkqscg
title: G040.7-04.1DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/2e5rfz
title: G038.3-00.1DistanceAG.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/2ubev4
title: G039.4-02.7DistanceAV.pdf

description: :unav
DOI: 10.7910/dvn/8hapxb/2ydwyc
title: G044.5+02.6DistanceAG.pdf

description: :unav
DOI: 10.5281/zenodo.3593322
title: The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones For Testing The Effects of Starspots on Structure and Colors

description: <strong>The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones For Testing The Effects of Starspots on Structure and Colors</strong> This repository contains the Stellar Parameters of Tracks with Starspots (SPOTS) grid of theoretical stellar evolutionary tracks and isochrones, presented in Somers, Pinsonneault, and Cao (2020, in prep). Our models were calculated with the Yale Rotating Evolution Code (e.g. van Saders & Pinsonneault, 2013, ApJ 776, 67), including updated which incorporate a treatment of surface starspots (Somers & Pinsonneault, 2015, ApJ 807, 174S). Modelling details can be found in these references. The purpose of this evolutionary suite is to provide the community with state-of-the-art predictions for the influence of starspots and magnetic activity on the structure of stars. The grid includes both isochrones and tracks. They can be downloaded individually from this repository, or in bulk by downloading the .zip files. <strong>Isochrones (.isoc):</strong> Each isochrone file contains a series of isochrones (stellar properties for a range of masses at fixed age) for ages between 1 Myrs and 4 Gyrs. Each file contains these isochrones for a different surface starspot covering fraction, given by the name of the file -- f000.isoc = 0% covering fraction, f017.isoc = 17% covering fraction, etc. Each isochrone contains several columns with different information, including, Fundamental properties: mass, age, luminosity, radius, logg, Teff, convective overturn timescale (TauCZ), lithium abundance relative to initial (Li/Li0). Starspot properties: Covering fraction (Fspot), ratio of spot temperature to ambient temperature (Xspot), the temperatures of hot and cool regions (T_hot, T_cool). Two-temperature colors, including Johnson BV, Cousins RI, 2MASS JHK, WISE W1, and Gaia G, BP, RP. Colors that fell outside of the calibrated range are listed as -99.0. <strong>Tracks (.track):</strong> We also include individual tracks for every combination of Fspot and Mass considered in the paper. Each .track file lists the mass and starspot covering fraction in the filename -- i.e. m055_f034.track is the model of mass 0.55Msun and with a 34% surface covering fraction. In addition to all the properties included in the isochrones, the track files also include: The total moment of interia of the model (total_I) and the moment of interia of the surface convection zone (CZ_I) The central and surface hydrogen abundances (X_cen, X_surf) and the surface metallicity (Z/X_surf) The deuterium abundance relative to initial (H2/H2_0)
DOI: 10.5281/zenodo.3593323
title: The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones For Testing The Effects of Starspots on Structure and Colors

description: <strong>The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones For Testing The Effects of Starspots on Structure and Colors</strong> This repository contains the Stellar Parameters of Tracks with Starspots (SPOTS) grid of theoretical stellar evolutionary tracks and isochrones, presented in Somers, Pinsonneault, and Cao (2020, in prep). Our models were calculated with the Yale Rotating Evolution Code (e.g. van Saders & Pinsonneault, 2013, ApJ 776, 67), including updated which incorporate a treatment of surface starspots (Somers & Pinsonneault, 2015, ApJ 807, 174S). Modelling details can be found in these references. The purpose of this evolutionary suite is to provide the community with state-of-the-art predictions for the influence of starspots and magnetic activity on the structure of stars. The grid includes both isochrones and tracks. <strong>Isochrones (.isoc):</strong> Each isochrone file contains a series of isochrones (stellar properties for a range of masses at fixed age) for ages between 1 Myrs and 4 Gyrs. Each file contains these isochrones for a different surface starspot covering fraction, given by the name of the file -- f000.isoc = 0% covering fraction, f017.isoc = 17% covering fraction, etc. Each isochrone contains several columns with different information, including, Fundamental properties: mass, age, luminosity, radius, logg, Teff, convective overturn timescale (TauCZ), lithium abundance relative to initial (Li/Li0). Starspot properties: Covering fraction (Fspot), ratio of spot temperature to ambient temperature (Xspot), the temperatures of hot and cool regions (T_hot, T_cool). Two-temperature colors, including Johnson BV, Cousins RI, 2MASS JHK, WISE W1, and Gaia G, BP, RP. Colors that fell outside of the calibrated range are listed as -99.0. <strong>Tracks (.track):</strong> We also include individual tracks for every combination of Fspot and Mass considered in the paper. Each .track file lists the mass and starspot covering fraction in the filename -- i.e. m055_f034.track is the model of mass 0.55Msun and with a 34% surface covering fraction. In addition to all the properties included in the isochrones, the track files also include: The total moment of interia of the model (total_I) and the moment of interia of the surface convection zone (CZ_I) The central and surface hydrogen abundances (X_cen, X_surf) and the surface metallicity (Z/X_surf) The deuterium abundance relative to initial (H2/H2_0)
DOI: 10.5281/zenodo.3593339
title: The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones For Testing The Effects of Starspots on Structure and Colors

description: <strong>The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones For Testing The Effects of Starspots on Structure and Colors</strong> This repository contains the Stellar Parameters of Tracks with Starspots (SPOTS) grid of theoretical stellar evolutionary tracks and isochrones, presented in Somers, Pinsonneault, and Cao (2020, in prep). Our models were calculated with the Yale Rotating Evolution Code (e.g. van Saders & Pinsonneault, 2013, ApJ 776, 67), including updated which incorporate a treatment of surface starspots (Somers & Pinsonneault, 2015, ApJ 807, 174S). Modelling details can be found in these references. The purpose of this evolutionary suite is to provide the community with state-of-the-art predictions for the influence of starspots and magnetic activity on the structure of stars. The grid includes both isochrones and tracks. They can be downloaded individually from this repository, or in bulk by downloading the .zip files. <strong>Isochrones (.isoc):</strong> Each isochrone file contains a series of isochrones (stellar properties for a range of masses at fixed age) for ages between 1 Myrs and 4 Gyrs. Each file contains these isochrones for a different surface starspot covering fraction, given by the name of the file -- f000.isoc = 0% covering fraction, f017.isoc = 17% covering fraction, etc. Each isochrone contains several columns with different information, including, Fundamental properties: mass, age, luminosity, radius, logg, Teff, convective overturn timescale (TauCZ), lithium abundance relative to initial (Li/Li0). Starspot properties: Covering fraction (Fspot), ratio of spot temperature to ambient temperature (Xspot), the temperatures of hot and cool regions (T_hot, T_cool). Two-temperature colors, including Johnson BV, Cousins RI, 2MASS JHK, WISE W1, and Gaia G, BP, RP. Colors that fell outside of the calibrated range are listed as -99.0. <strong>Tracks (.track):</strong> We also include individual tracks for every combination of Fspot and Mass considered in the paper. Each .track file lists the mass and starspot covering fraction in the filename -- i.e. m055_f034.track is the model of mass 0.55Msun and with a 34% surface covering fraction. In addition to all the properties included in the isochrones, the track files also include: The total moment of interia of the model (total_I) and the moment of interia of the surface convection zone (CZ_I) The central and surface hydrogen abundances (X_cen, X_surf) and the surface metallicity (Z/X_surf) The deuterium abundance relative to initial (H2/H2_0)
DOI: 10.17632/49py6xkftk.1
title: Cyclostratigraphy of Lower Triassic terrestrial successions in the Junggar Basin, northwestern China
DOI: 10.17632/ffhvzrr3jd.3
title: Data for: Late Ordovician obliquity-forced glacio-eustasy recorded in the Yangtze Block, South China

description: The raw data of magnetic susceptibility (MS) and anhysteretic remnant magnetization (ARM) in depth domain. The detailed result data: 1) interpolation and detrending of the whole log-transformed ARM series in depth domain; 2) cyclostratigraphic analysis on the log-transformed ARM series of Subsets 1, 2, and 3 in depth domain, including interpolation, detrending, 2π MTM spectrum, and filtering; 3) 405-kyr and 33.8-kyr astronomical calibrations of the whole log-ARM series, including the agemodels used for calibrations, as well as interpolation, detrending, 2π MTM spectrum, and filtering in time domain; 4) the long-period amplitude modulation analysis on the 33.83-kyr-calibrated log-ARM series, including the e/T and O/T series and their amplitude spectra, as well as the g4-g3, s4-s3, and s3-s6 filter outputs.
DOI: 10.21227/qdkj-j555
title: Cocoa beans spectral image with three fermentation levels

description: The target scene consists of a black cardwith six cocoa beans of three different fermentation levels (High, correct, and low fermentation),two beans for each class, whosefalse-color composite is shown in the provided Figure (a),ground-truth map is shownin Fig. (b), and Fig. (c) presents its representative spectralsignatures. The spectral imagewas acquired by the AVT Stingray F-080Bcamera by acquiring one band each time from350 - 950 nm. The acquired image hasa spatial resolution of 1096x712 pixels and 300 spectral bands of 2 nm width.
DOI: 10.17632/wjs9727h8v.1
title: Data for: Temporal regularity and stimulus control in multiple fixed interval schedules

description: Data from all 85 sessions of training. Each row is one time bin (1 s). Columns are labels for: (1) rat number, (2) session number, (3) trial number, (4) block_size (i.e., group), (5) FI, (6) time bin, (7) training phase, and (8) responses per minute.
DOI: 10.17632/5fykspdg9y.1
title: Data for: Energy Intensity and Green Energy Innovation: heterogeneous country effects in the OECD

description: we provide macroeconomic data and some code files other info may be required
DOI: 10.25345/c58d7s
title: MassIVE MSV000084736 - Integrated multi-omics analysis of RB-loss identifies widespread cellular programming and synthetic weaknesses
title: Multiplexed proteomics using TMT10 and the SPS-MS3 method on an Orbitrap Fusion mass spectrometer has been used to study the loss of retinoblastoma 1, RB, in human cell lines. Samples were measured in three TMT pools (TMT1, TMT2, TMT3). Each pool was fractionated by basic pH reversed-phase liquid chromatography (bRPLC) and per pool twelve fractions were analyzed by mass spectrometry. A bridge channel from combined digests of all samples was used to enable a combined analysis of the data from the three TMT pools. The RAW files are: Miles_RB_TMT1_fraction01 to 12 Miles_RB_TMT2_fraction01 to 12 Miles_RB_TMT3_fraction01 to 12 The TMT labeling of the samples was as follows: FF-DOX (TMT1, 127n), FF+DOX (TMT1, 127c), RB25-DOX (TMT1, 128n), RB25-DOX (TMT1, 128c), RB25+DOX (TMT1, 130c), RB25+DOX (TMT2, 127n), RB26-DOX (TMT2, 129c), RB26-DOX ((TMT2, 130n), RB26+DOX (TMT3, 128n), RB26+DOX (TMT3, 128c). The bridge channel was at 126 for all three TMT pools.
DOI: 10.5281/zenodo.3593844
title: Dataset from: Common–Envelope Episodes that lead to Double Neutron Star formation

description: The results of all simulations shown in "Common–Envelope Episodes that lead to Double Neutron Star formation" (arXiv:2001.09829) Contents: COMPASOutput.h5<br> MATLABscripts.zip<br> README All simulations made using COMPAS
DOI: 10.21227/8rce-m345
title: Simulation data for a Monte Carlo Wave-Particle Event-Based Interaction Model

description: The data made available are the simulations of a time-resolved Monte Carlo model for use in quantitative as well as qualitative analysis of different types of particle atmospheres.
DOI: 10.21227/hn54-hb10
title: Simulation data for a Monte Carlo Wave-Particle Event-Based Interaction Model

description: The data made available are the simulations of a time-resolved Monte Carlo model for use in quantitative as well as qualitative analysis of different types of particle atmospheres.
DOI: 10.18169/papdeott008252
title: Software-Sollbruchstelle
DOI: 10.17632/jjmdwwzjm9.1
title: Data for: Revisiting The Persistence of Real Exchange Rates

description: data for real exchange rates
DOI: 10.5281/zenodo.3593394
title: Supplementary Data S1 for Rosen et al. Li and Ca enrichment in the Bristol Dry Lake brine, California

description: Supplementary file S1: Chemical groundwater data used for analysis in the Journal article entitled "<strong>Li and Ca enrichment in the Bristol Dry Lake brine compared to brines from Cadiz and Danby Dry Lakes, Barstow-Bristol Trough, California, USA" </strong>by Michael R. Rosen, Lisa L. Stillings, Tyler Kane, Kate Campbell-Hay, and Matthew Vitale, P.G., Ray Spanjers, P.G.in the Journal Minerals Supplementary file S2: Chemical data from extractions from 10 clay samples from Bristol Dry lake by acid digestion. used in "<strong>Li and Ca enrichment in the Bristol Dry Lake brine compared to brines from Cadiz and Danby Dry Lakes, Barstow-Bristol Trough, California, USA" </strong>by Michael R. Rosen, Lisa L. Stillings, Tyler Kane, Kate Campbell-Hay, and Matthew Vitale, P.G., Ray Spanjers, P.G.in the Journal Minerals. Methods for all data are in the journal article. Data is for Bristol, Cadiz and Danby playas (Dry Lakes). Most data has been previously published either online in the California Division of Water Resources website, or in other USGS publications or journal articles. Some data from Cadiz Dry lake has not been previously published and publication of these data has been granted by Tetra Technologies Inc. and Standard Lithium LLC.
DOI: 10.5281/zenodo.3593395
title: Supplementary Data S1 for Rosen et al. Li and Ca enrichment in the Bristol Dry Lake brine, California

description: Supplementary file S1: Chemical groundwater data used for analysis in the Journal article entitled "<strong>Li and Ca enrichment in the Bristol Dry Lake brine compared to brines from Cadiz and Danby Dry Lakes, Barstow-Bristol Trough, California, USA" </strong>by Michael R. Rosen, Lisa L. Stillings, Tyler Kane, Kate Campbell-Hay, and Matthew Vitale, P.G., Ray Spanjers, P.G.in the Journal Minerals Supplementary file S2: Chemical data from extractions from 10 clay samples from Bristol Dry lake by acid digestion. used in "<strong>Li and Ca enrichment in the Bristol Dry Lake brine compared to brines from Cadiz and Danby Dry Lakes, Barstow-Bristol Trough, California, USA" </strong>by Michael R. Rosen, Lisa L. Stillings, Tyler Kane, Kate Campbell-Hay, and Matthew Vitale, P.G., Ray Spanjers, P.G.in the Journal Minerals. Methods for all data are in the journal article. Data is for Bristol, Cadiz and Danby playas (Dry Lakes). Most data has been previously published either online in the California Division of Water Resources website, or in other USGS publications or journal articles. Some data from Cadiz Dry lake has not been previously published and publication of these data has been granted by Tetra Technologies Inc. and Standard Lithium LLC.
DOI: 10.17632/kn3xxtxc6x.1
title: Data for: An analytical solution for buckling and vibration problems of delaminated doubly curved shells

description: Abaqus validation
DOI: 10.5281/zenodo.3593408
title: RONO2 and HNO3 formation rates from BEARPEX 07

description: This repository contains data from the BEARPEX07 Field campaign used in Romer et al., 2020 to calculate the formation rates of RONO2 and HNO3. For additional information about the campaign, see the campaign website: https://www.ocf.berkeley.edu/~bearpex/ <br> Reference information for the BEARPEX07 Field Campaign<br> Dates: Aug 15 - Oct 10 2007<br> Location: Blodgett Forest Research Station, Georgetown CA. 38.91 N, -120.66 W<br> Elevation: 1315 m above sea level<br> Campaign website: https://www.ocf.berkeley.edu/~bearpex/ Measurements listed:<br> utc_date: The date and time of the midpoint of the measurements, in UTC time<br> local_solar_time: The local solar time of the midpoint of the measurements, reported in Pacific Standard Time (UTC-08:00)<br> VOCR_hz: The reactivity to OH of all volatile organic compounds (VOCs), defined as the sum of the concentration of all measured VOCs multiplied by their reaction rate with OH. VOCR is reported in s^-1.<br> NO2_ppt: The concentration of NO2, measured in parts per trillion.<br> Total_RONO2_ppt: The concentration of total organic nitrates (=\(\Sigma\)ANs = \(\Sigma\)RONO2), measured in parts per trillion. Includes organic nitrates in both the gas and particle phase, but does not include HNO3 or inorganic nitrate ions.<br> Total_HNO3_ppt: The concentration of nitric acid, measured in parts per trillion. Includes both gaseous nitric acid and thermally labile particle phase nitrate ion.<br> alpha_eff: The effective organic nitrate branching ratio. Defined as the yield of RONO2 compounds when an RO2 radical reacts with NO, averaged over all RO2 species. <br> YRO2_eff: The effective yield of RO2 radicals. Defined as the yield of RO2 radicals when a VOC is oxidized by OH, averaged over all VOCs.<br> fNO_eff: The average probability that an RO2 radical will react with NO, instead of being lost through some other pathway.<br> pressure_bar: The pressure at the measurement location, measured in bar.<br> temperature_K: The temperature at the measurement location, measured in Kelvin.