cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25989/83xg-tn96
title: Materials Experiment and Analysis Database: Electrochemistry analysis in which 0 sub-analyses are performed on plate(s) containing CuV,V,In,W,Ca,Sr,Mo,La annealed at 565.0C to add O on 2018-03-09 from Analysis 20180309.115129

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/83xg-tn96/&lt;/p&gt;</p>20180309.115129.copied-20180310220835719PST.zip 36.5 MB 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25582/data.2019-07.1818167/1927312
title: Data for EMSL Project 49960 from July 2019
DOI: 10.25582/data.2019-09.1841447/1927313
title: Data for EMSL Project 49960 from September 2019
DOI: 10.25989/850d-b095
title: Materials Experiment and Analysis Database: Inkjet chemical deposition analysis in which 0 sub-analyses are performed on plate(s) containing Y,Ce,Cu annealed at 750.0C to add O on 2018-06-04 from Analysis 20180604.151800

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/850d-b095/&lt;/p&gt;</p>20180604.151800.copied-20180927040646355PDT.zip 1.0 kB 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25989/85x9-bh27
title: Materials Experiment and Analysis Database: Inkjet chemical deposition measurements 0 files performed on plate containing CuV,V,In,W,Ca,Sr,Mo,La annealed at 565.0C to add O on 2018-02-01 from Run 20180201.115400

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/85x9-bh27/&lt;/p&gt;</p>20180201.115400.copied-20180927030341191PDT.zip 621.0 B 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25582/data.2019-08.1828078/1927315
title: Data for EMSL Project 49960 from August 2019
DOI: 10.25989/8652-h874
title: Materials Experiment and Analysis Database: X-ray diffraction measurements 3 files performed on plate containing Sr,Co,Bi,Ar annealed at 700.0C to add O on 2018-05-18 from Run 20180518.194954

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/8652-h874/&lt;/p&gt;</p>20180518.194954.copied-20180524174929411PDT.zip 3.8 MB 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25582/data.2019-08.1828742/1927317
title: Data for EMSL Project 49960 from August 2019
DOI: 10.25989/867e-y312
title: Materials Experiment and Analysis Database: X-ray diffraction measurements 7 files performed on plate containing Sr,Co,Bi,Ar annealed at 650.0C to add O on 2018-05-22 from Run 20180522.095237

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/867e-y312/&lt;/p&gt;</p>20180522.095237.copied-20180524174929411PDT.zip 12.3 MB 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25582/data.2019-09.1837619/1927319
title: Data for EMSL Project 49960 from September 2019
DOI: 10.25582/data.2019-07.1819067/1927320
title: Data for EMSL Project 49960 from July 2019
DOI: 10.25989/86aj-dd61
title: Materials Experiment and Analysis Database: Inkjet chemical deposition analysis in which 0 sub-analyses are performed on plate(s) containing Ni,Nb,W,Mo annealed at 800.0C to add reducing on 2018-07-22 from Analysis 20180722.135200

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/86aj-dd61/&lt;/p&gt;</p>20180722.135200.copied-20180927040714176PDT.zip 10.1 kB 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25582/data.2021-02.2147034/1927321
title: Data for EMSL Project 49960 from February 2021
DOI: 10.25582/data.2019-07.1814387/1927322
title: Data for EMSL Project 49960 from July 2019
DOI: 10.25989/873t-8052
title: Materials Experiment and Analysis Database: Electrochemistry analysis in which 0 sub-analyses are performed on plate(s) containing CuV,V,In,W,Ca,Sr,Mo,La annealed at 565.0C to add O on 2018-02-06 from Analysis 20180206.112105

description: This record is a component of the Materials Experiment and
Analysis Database (MEAD). It contains raw data and metadata from millions 
of materials synthesis and characterization experiments, as well as the 
analysis and distillation of that data into property and performance 
metrics. The unprecedented quantity and diversity of experimental data 
are searchable by experiment and analysis attributes generated by both 
researchers and data processing software.

description: Files available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/0_gregoire/873t-8052/&lt;/p&gt;</p>20180206.112105.copied-20180206113240118PST.zip 17.0 MB 
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        &gt; &lt;i class="download icon"&gt;&lt;/i&gt; Download &lt;/a&gt;</p>&lt;/p&gt;</p>
DOI: 10.25582/data.2019-09.1846977/1927323
title: Data for EMSL Project 49960 from September 2019
DOI: 10.7910/dvn/u3stqv/dutk8y
title: EthR1_SIPS_2017.xls

description: :unav
DOI: 10.7910/dvn/u3stqv/kz2asc
title: sectionn.tab

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DOI: 10.7910/dvn/u3stqv/n7wcwu
title: sectionu.tab

description: :unav
DOI: 10.7910/dvn/u3stqv/tefvey
title: sipsR1_child_quantnutrition.tab

description: :unav
DOI: 10.7910/dvn/u3stqv/tti56a
title: sipsR1_dds-intake-anemia_women.tab

description: :unav
DOI: 10.7910/dvn/u3stqv/yqs7nf
title: sectionw.tab

description: :unav
DOI: 10.25606/surf.578c6039-61b80f94
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-143)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 143 of the 2048³ resolution collection.
DOI: 10.7910/dvn/hjgj2a/18tceg
title: 20190809113554913_wifi_33_182_012_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/8lappe
title: 20190809120940687_wifi_33_189_004_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/aau9qs
title: 20190809113539584_wifi_33_181_015_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/dicpln
title: 20190809140942073_wifi_33_180_002_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/ge7mc2
title: 20190809135427086_wifi_33_182_012_chanseok2_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/kg9klr
title: 20190809144708695_wifi_33_189_006_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/n3lp0p
title: 20190809115645531_wifi_33_188_003_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/pobpx0
title: 20190809140450616_wifi_33_186_008_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/wc9gkv
title: 20190809144842564_wifi_33_190_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/8sc6rt
title: sectiond.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/de1zkq
title: sectionb.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/i1ri2l
title: sectionc.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/mi8wyj
title: sectionf.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/qmsuxi
title: sectiona.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/sogqje
title: sectione.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/vlvfrp
title: section0.tab

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DOI: 10.7910/dvn/l3dgck/z4ob7s
title: riskpercp.tab

description: :unav
DOI: 10.17632/c9wtrg69j3.1
title: Data for: Influence of deformation strain rate on the mechanical response in a metastable β titanium alloy with various microstructures
DOI: 10.7910/dvn/hjgj2a/1tzc1o
title: 20190809140927108_wifi_33_180_001_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/3dbry2
title: 20190809120426932_wifi_33_188_001_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/7nxntz
title: 20190809141345563_wifi_33_189_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/gjw7xl
title: 20190809111015900_wifi_33_177_019_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/har7h5
title: 20190809135242157_wifi_33_176_013_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/jnhinq
title: 20190809135524821_wifi_33_177_008_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/mitumn
title: 20190809111743259_wifi_33_179_011_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/uvjop4
title: 20190809105359172_wifi_33_175_010_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/zmum5x
title: 20190809110533012_wifi_33_177_018_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/l3dgck/bttcn3
title: sectionm.tab

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DOI: 10.7910/dvn/l3dgck/gpb8je
title: sectionl.tab

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DOI: 10.7910/dvn/l3dgck/orhugu
title: sectiong.tab

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DOI: 10.7910/dvn/l3dgck/pjqykb
title: sectionh.tab

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DOI: 10.7910/dvn/l3dgck/qdraqc
title: sectionj.tab

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DOI: 10.7910/dvn/l3dgck/r5tyjl
title: sectionkap.tab

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DOI: 10.7910/dvn/l3dgck/rvmg8t
title: sectionn.tab

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DOI: 10.7910/dvn/l3dgck/uxkbal
title: sectionk.tab

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DOI: 10.7910/dvn/hjgj2a/0ee0rt
title: 20190809135000236_wifi_33_176_005_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/dfb048
title: 20190809114434118_wifi_33_185_013_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/dqwvhh
title: 20190809134337179_wifi_33_180_011_chanseok2_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/l8ryuw
title: 20190809115450738_wifi_33_187_013_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/pcowy2
title: 20190809135816739_wifi_33_177_020_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/rwki8e
title: 20190809143417210_wifi_33_186_001_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/u3v4cv
title: 20190809110748108_wifi_33_178_005_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/ujjtxd
title: 20190809112426629_wifi_33_180_015_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/z9cgat
title: 20190809133446241_wifi_33_178_012_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/5ikabn
title: sectionr1.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/8ul1tx
title: sectionr2_s_child.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/9elchj
title: sectionp.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/gq9hdd
title: sectiono.tab

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DOI: 10.7910/dvn/l3dgck/i3m7it
title: sectionv.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/igyeng
title: sectionu1.tab

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DOI: 10.7910/dvn/l3dgck/yr5x1k
title: sectionu.tab

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DOI: 10.7910/dvn/l3dgck/zesrhq
title: sectiont.tab

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DOI: 10.25606/surf.578c6039-b0bdbd1c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-146)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 146 of the 2048³ resolution collection.
DOI: 10.7910/dvn/hjgj2a/1ny1n3
title: 20190809105732234_wifi_33_176_002_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/36y0ec
title: 20190809142859940_wifi_33_185_001_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/7brxmg
title: 20190809105839347_wifi_33_175_015_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/foxvge
title: 20190809114240813_wifi_33_182_014_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/hzdlgh
title: 20190809115327431_wifi_33_185_018_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/jlyelb
title: 20190809110719775_wifi_33_177_009_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/rbx8vw
title: 20190809115830373_wifi_33_188_010_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/rcinhx
title: 20190809105945313_wifi_33_175_018_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/u4bzvk
title: 20190809140404766_wifi_33_183_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/amlske
title: sectionw_mdd.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/g4huxh
title: sectionw_care.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/hbsfka
title: sectionw_diarrhea.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/jwkw3o
title: sectionw_liquids.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/kcb0hp
title: sipsR3_intake-anemia_child.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/llgorl
title: sipsR3_dds-intake-anemia_women.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/o6pep0
title: sectionw_food.tab

description: :unav
DOI: 10.7910/dvn/l3dgck/otd8c5
title: sectiony4.tab

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DOI: 10.7910/dvn/l3dgck/r4jbmv
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DOI: 10.17632/79h4z5yzs2.1
title: Data for: A Greedy Region Growing Algorithm for Adaptive Triangulation of Geometry Images

description: This data is provided to the reviewers to assist the review process. Oriiginal irregular meshes of all models mentioned in the manuscript as well as their geometry images (output of OpenGI library) and triangulations with the algorithms compared (including two variants of the proposed greedy region growing algorithm based on cost functions C_1 and C_2) are presented. The author does not claim any rights on the publicly available original mesh data.
DOI: 10.25606/surf.578c6039-2f65c2dc
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-619)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 619 of the 2048³ resolution collection.
DOI: 10.7910/dvn/eqg0xt/sumyeg
title: sectiona.tab

description: :unav
DOI: 10.7910/dvn/eqg0xt/z8bipl
title: section0.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/1jrxll
title: 20190809141215405_wifi_33_188_009_chanseok2_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/ankdnp
title: 20190809105352190_wifi_33_175_005_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/bpquks
title: 20190809141619167_wifi_33_181_004_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/dv2jqo
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DOI: 10.7910/dvn/l3dgck/6y5rsj
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DOI: 10.7910/dvn/l3dgck/ewdknz
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