cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.7910/dvn/hjgj2a/dnuwma
title: 20190809143601184_wifi_33_186_008_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/o30ry6
title: 20190809135920236_wifi_33_178_002_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/rvayzs
title: 20190809134359059_wifi_33_175_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/yfwqzq
title: 20190809140204610_wifi_33_185_017_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/zktuyg
title: 20190809135818642_wifi_33_185_001_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/zpttz6
title: 20190809141015319_wifi_33_180_004_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/zxkmn4
title: 20190809132938289_wifi_33_177_011_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.25606/surf.578c6039-bed82fc6
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-685)

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 685 of the 2048³ resolution collection.
DOI: 10.7910/dvn/hjgj2a/6hkvmd
title: 20190809111526096_wifi_33_178_014_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/foo8wx
title: 20190809112903252_wifi_33_180_017_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ifcqo0
title: 20190809111322096_wifi_33_178_007_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/kjizrr
title: 20190809141547753_wifi_33_190_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/lhbytu
title: 20190809142537046_wifi_33_182_015_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/mauov2
title: 20190809114225036_wifi_33_185_005_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/phjgds
title: 20190809115844556_wifi_33_188_011_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/qneb14
title: 20190809144653516_wifi_33_189_005_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/vkviyx
title: 20190809114000267_wifi_33_182_005_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/1qvpzv
title: 20190809115251458_wifi_33_187_006_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/2yd82h
title: 20190809133349705_wifi_33_178_008_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/9kt1ia
title: 20190809114009352_wifi_33_184_003_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/bthuid
title: 20190809141045665_wifi_33_188_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/cutrzf
title: 20190809135220605_wifi_33_182_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/j3rvlt
title: 20190809110953580_wifi_33_177_018_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/jl575h
title: 20190809111916953_wifi_33_179_001_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/jv3gj9
title: 20190809113519080_wifi_33_181_014_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/nozgd7
title: 20190809135422842_wifi_33_177_004_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/uozp29
title: 20190809105843653_wifi_33_176_006_chanseok_SM-G950N.tab

description: :unav
DOI: 10.25606/surf.578c6039-577736ff
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-593)

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 593 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-d02ee451
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-147)

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 147 of the 2048³ resolution collection.
DOI: 10.7910/dvn/hjgj2a/3qhd03
title: 20190809113505725_wifi_33_181_013_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/9ltw4l
title: 20190809112018682_wifi_33_180_001_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/bxo6ha
title: 20190809105101260_wifi_33_175_004_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ngi2n5
title: 20190809112620853_wifi_33_180_008_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/rcjtkt
title: 20190809110412474_wifi_33_176_012_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/rrwqmh
title: 20190809134532245_wifi_33_180_019_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/t5wemv
title: 20190809121319346_wifi_33_190_005_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/w0bvig
title: 20190809134402727_wifi_33_180_013_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ym923p
title: 20190809134824864_wifi_33_175_019_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/6uyyfb
title: 20190809145035156_wifi_33_191_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/bzb0hd
title: 20190809132433725_wifi_33_176_003_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/hwcue2
title: 20190809110435000_wifi_33_177_014_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/lionr4
title: 20190809112128784_wifi_33_180_005_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ol6ecz
title: 20190809132152863_wifi_33_175_011_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/qmvxbf
title: 20190809140159739_wifi_33_178_012_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/swrvci
title: 20190809111148630_wifi_33_178_002_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/xwmwgl
title: 20190809113923987_wifi_33_182_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.21227/t49n-5d45
title: Coronavirus (COVID-19) Tweets Dataset

description: This dataset includes CSV files that contain IDs and sentiment scores of the tweets related to the COVID-19 pandemic. The tweets have been collected by an on-going project deployed at https://live.rlamsal.com.np. The model monitors the real-time Twitter feed for coronavirus-related tweets using 54 different keywords that are commonly used while referencing the pandemic. This dataset has been wholly re-designed on March 20, 2020, to comply with the content redistribution policy set by Twitter. Below is the quick overview of this dataset.— Number of tweets : 359,786,493 tweets
DOI: 10.7910/dvn/hjgj2a/1cjeli
title: 20190809140330066_wifi_33_186_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/b3hsv3
title: 20190809121016083_wifi_33_189_006_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/cgfsna
title: 20190809135104069_wifi_33_176_008_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/dbqfin
title: 20190809115944826_wifi_33_187_002_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/dofcru
title: 20190809134349835_wifi_33_180_012_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/gf2uci
title: 20190809141842900_wifi_33_191_003_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/i6tzjd
title: 20190809132231830_wifi_33_175_014_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/onkvjk
title: 20190809134323729_wifi_33_180_010_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/pzjnzi
title: 20190809140715777_wifi_33_179_009_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/2deplo
title: 20190809143546529_wifi_33_186_007_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/g67ye0
title: 20190809110805587_wifi_33_177_012_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/geh3qt
title: 20190809120616329_wifi_33_191_002_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/j1gf6d
title: 20190809114955190_wifi_33_186_010_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/pcy6iq
title: 20190809113709880_wifi_33_181_020_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/uxq3fn
title: 20190809115712184_wifi_33_186_009_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/yys25v
title: 20190809141829448_wifi_33_191_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/zriuqz
title: 20190809113555382_wifi_33_181_016_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/5tqxva
title: 20190809113744232_wifi_33_182_019_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/9hrngr
title: 20190809135750681_wifi_33_184_004_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/bfss9n
title: 20190809110719349_wifi_33_178_003_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/nalrzn
title: 20190809133041130_wifi_33_177_016_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/nrken1
title: 20190809112738516_wifi_33_181_004_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ppbxk3
title: 20190809135950742_wifi_33_178_004_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/swzfve
title: 20190809110203410_wifi_33_176_005_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/vi0ddo
title: 20190809120846116_wifi_33_189_001_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/wvpsy8
title: 20190809132924550_wifi_33_177_010_chanseok2_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/yr7g15
title: 20190809144617750_wifi_33_189_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/9rflwv
title: 20190809142246924_wifi_33_182_004_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/digoyw
title: 20190809144752211_wifi_33_189_009_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/eixqhb
title: 20190809110153095_wifi_33_177_003_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/fjoif2
title: 20190809114334194_wifi_33_185_009_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/npmxv1
title: 20190809134839874_wifi_33_175_020_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/o3dmst
title: 20190809132501441_wifi_33_176_005_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/peu3xm
title: 20190809114702081_wifi_33_184_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/qz2plp
title: 20190809134918387_wifi_33_181_012_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.5519/qd.keb7uta7
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (21961 records)
DOI: 10.7910/dvn/hjgj2a/bxkhkf
title: 20190809110354879_wifi_33_176_011_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/djbk2p
title: 20190809120659912_wifi_33_188_009_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/epy2mm
title: 20190809120645909_wifi_33_191_004_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/olvm9f
title: 20190809140535249_wifi_33_186_011_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/qk3iy2
title: 20190809133333208_wifi_33_178_007_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/skj6do
title: 20190809113153702_wifi_33_181_020_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/twteok
title: 20190809111502383_wifi_33_179_001_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/zrao92
title: 20190809120001752_wifi_33_189_001_chanseok_SM-G950N.tab

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DOI: 10.21227/fq14-q173
title: Ruling Power Tautology: Error in Big Bang Theory

description: -If Ruling Power were able and willing to create Sun/Mars, he would do so. If Ruling Power were unable to create Sun/Mars, he would be incapable; if he were unwilling to create Sun/Mars, he would be malevolent. Ruling Power creates Sun/Mars. If Ruling Power exists, he is neither incapable nor malevolent. Therefore, Ruling Power exists. The World of PC can’t be created itself just from one factor light. I (programmer) die & consequently light (big bang) become useless.
DOI: 10.7910/dvn/hjgj2a/4qigyw
title: 20190809144332007_wifi_33_188_007_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/ciw7ss
title: 20190809140804378_wifi_33_187_007_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/cxyoli
title: 20190809133821375_wifi_33_179_004_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/lfugmm
title: 20190809134629385_wifi_33_175_012_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/q5q8dk
title: 20190809134808258_wifi_33_181_007_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/qpheyk
title: 20190809120430823_wifi_33_190_003_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/vy2jqk
title: 20190809111046839_wifi_33_178_014_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/xc0yty
title: 20190809113822806_wifi_33_182_001_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/xgivcr
title: 20190809133650626_wifi_33_183_004_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/88u4cb
title: 20190809120016578_wifi_33_189_002_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/9vrd2q
title: 20190809140229742_wifi_33_178_014_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ax7qod
title: 20190809132740477_wifi_33_177_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/fv5zc3
title: 20190809143500240_wifi_33_186_004_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/gpnyar
title: 20190809135607988_wifi_33_177_011_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/jw1ks0
title: 20190809105801688_wifi_33_175_013_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/r8wsxl
title: 20190809135733535_wifi_33_177_017_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/rqmhnx
title: 20190809140420171_wifi_33_183_004_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/xrhest
title: 20190809112410815_wifi_33_180_014_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/zd7xho
title: 20190809114222401_wifi_33_182_013_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/ozlxpb/6svg79
title: Figure 1C.tab

description: cytotoxicity induced by inducers and inhibitors of necrosis and apotosis
DOI: 10.7910/dvn/ozlxpb/bgc92z
title: Figure 6C-3.tab

description: LIX production in BALF
DOI: 10.7910/dvn/ozlxpb/if1z57
title: Figure 3C.tab

description: cell viabilities in wide-type and TfR-KD cells
DOI: 10.7910/dvn/ozlxpb/loxwcz
title: Figure 6C-1.tab

description: IL-1β production in BALF
DOI: 10.7910/dvn/ozlxpb/or1498
title: Figure 6C-2.tab

description: TNF-α production in BALF
DOI: 10.7910/dvn/ozlxpb/web3gt
title: Figure 2B.tab

description: cytotoxicity induced by TMDs with CD
DOI: 10.7910/dvn/hjgj2a/jwt7uz
title: 20190809135505811_wifi_33_182_015_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/jxmv7u
title: 20190809140215521_wifi_33_178_013_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/rtvdvt
title: 20190809110238607_wifi_33_177_006_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/uxe1z3
title: 20190809113313974_wifi_33_182_001_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/vtxeym
title: 20190809115814996_wifi_33_188_009_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/yha7wn
title: 20190809135725342_wifi_33_184_002_chanseok2_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/ykikjq
title: 20190809141747903_wifi_33_181_010_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/ozlxpb/flcaoi
title: Figure 1B-1.tab

description: ATP assay of 2D nanomaterials cytotoxicity
DOI: 10.7910/dvn/ozlxpb/q5mbee
title: Figure 1B - 2.tab

description: MTS assay of 2D nanomaterials cytotoxicity
DOI: 10.7910/dvn/ozlxpb/xydcml
title: Figure 3B.xlsx

description: cytotoxicity induced by TMDs with Fe2+ chelators
DOI: 10.7910/dvn/hjgj2a/0kz9ey
title: 20190809120253165_wifi_33_187_013_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/afbneg
title: 20190809140126965_wifi_33_178_010_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/d1sd88
title: 20190809132139777_wifi_33_175_010_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/fgqwh8
title: 20190809134836810_wifi_33_181_009_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/kagknj
title: 20190809112858360_wifi_33_181_009_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/pjnjjm
title: 20190809110545945_wifi_33_177_019_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/qizzq4
title: 20190809105414557_wifi_33_175_006_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/rz00c0
title: 20190809140647628_wifi_33_179_007_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/x5tmog
title: 20190809141046177_wifi_33_180_006_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/fzo0za
title: 20190809143824654_wifi_33_187_003_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/halbfz
title: 20190809133914597_wifi_33_179_008_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/hfc9tu
title: 20190809132417581_wifi_33_176_002_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/indyan
title: 20190809134725462_wifi_33_181_004_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/kgz4px
title: 20190809135452957_wifi_33_182_014_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/oqwwlj
title: 20190809110827223_wifi_33_177_013_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/ubmmhg
title: 20190809112456700_wifi_33_180_017_chanseok_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/wo70wy
title: 20190809121301682_wifi_33_190_004_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/z3olhe/aa6kaq
title: 7 Viable embedded Tunga penetrans.AVI

description: :unav
DOI: 10.7910/dvn/z3olhe/azletx
title: 6 LC-Qt of-MS Chromatogram of neem oil 05072017.doc

description: :unav
DOI: 10.7910/dvn/z3olhe/m9eg50
title: 4 Contaminant Certification for neem oil 05072017.pdf

description: :unav
DOI: 10.7910/dvn/z3olhe/uwd5r6
title: 5 Composition of neem oil 05072017.pdf

description: :unav
DOI: 10.25606/surf.578c6039-fbbda750
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-067)

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 067 of the 2048³ resolution collection.
DOI: 10.7910/dvn/hjgj2a/2nyfa2
title: 20190809120034847_wifi_33_187_005_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/3griej
title: 20190809132557716_wifi_33_176_009_chanseok2_SM-G950N.tab

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DOI: 10.7910/dvn/hjgj2a/5fpvyr
title: 20190809112415379_wifi_33_180_001_g6_LGM-G600L.tab

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DOI: 10.7910/dvn/hjgj2a/cfagur
title: 20190809115125056_wifi_33_185_012_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/een8nh
title: 20190809144603846_wifi_33_189_002_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/iwntuf
title: 20190809140518247_wifi_33_179_001_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/kusyir
title: 20190809120902660_wifi_33_189_002_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/vzhnd7
title: 20190809135053727_wifi_33_181_019_chanseok2_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/a2jnft
title: 20190809105526420_wifi_33_175_008_g6_LGM-G600L.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/g3thw2
title: 20190809112324575_wifi_33_180_011_chanseok_SM-G950N.tab

description: :unav
DOI: 10.7910/dvn/hjgj2a/gm1ndj
title: 20190809114757888_wifi_33_186_004_chanseok_SM-G950N.tab

description: :unav