cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-040db5bd
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-215)

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 215 of the 2048³ resolution collection.
DOI: 10.7295/w9cil50351
title: CIL:50351, Mus musculus, Spinal cord neuron
DOI: 10.25606/surf.578c6039-b9703c44
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-621)

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 621 of the 2048³ resolution collection.
DOI: 10.7295/w9cil50352
title: CIL:50352, Mus musculus, Spinal cord neuron
DOI: 10.25606/surf.578c6039-f25e5c5e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-182)

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 182 of the 2048³ resolution collection.
DOI: 10.7295/w9cil50353
title: CIL:50353, phantom
DOI: 10.25606/surf.578c6039-caa2fcae
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-177)

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 177 of the 2048³ resolution collection.
DOI: 10.17632/9zrcpp8pym.1
title: Data for: Degradation of ibuprofen with a Fenton-like process triggered by zero-valent iron (ZVI-Fenton)
DOI: 10.25606/surf.578c6039-e98922ee
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-568)

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 568 of the 2048³ resolution collection.
DOI: 10.17632/99dp658c2z.1
title: Data for: Effects of location on Airbnb apartment pricing in Málaga

description: Effects of location on Airbnb apartment pricing in Málaga
DOI: 10.25952/5d8c60ec934c2
title: Supervisory Teaching and Its Impact on Student Agency in Primary Classrooms

description: This exploratory case study utilised three primary classrooms at one Hong Kong international school. Teachers in each classroom utilised a Supervisory Teaching framework for some lessons. Student learning was observed in these lessons over a period of five months, with the aim of noting any instances of student agency. The teachers were interviewed as part of the data collection process. This data set includes transcribed interviews, observation notes, category analysis data, acts of teaching analysis data, and an analysis summary.
DOI: 10.25606/surf.578c6039-80eda233
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-206)

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 206 of the 2048³ resolution collection.
DOI: 10.17632/vyfgdffjxj.1
title: Raw data-Impulsivity trait and proactive cognitive control: An fMRI study

description: Research data
DOI: 10.17632/m7tt68vwyr.2
title: Raw data-Validation of an electronic version of the Self-Awareness Questionnaire in English and Italian healthy samples

description: Research data
DOI: 10.25592/dgs.corpus-2.0-type-17234
title: Tokenliste für das Type $GEST-NM-KOPFNICKEN1^
title: Token list for the type $GEST-NM-NOD-HEAD1^

description: Token list for the type $GEST-NM-NOD-HEAD1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-KOPFNICKEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-17305
title: Tokenliste für das Type $GEST-NM-KOPFSCHÜTTELN1^
title: Token list for the type $GEST-NM-SHAKE-HEAD1^

description: Token list for the type $GEST-NM-SHAKE-HEAD1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-KOPFSCHÜTTELN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-42583
title: Tokenliste für das Type $GEST-NM^
title: Token list for the type $GEST-NM^

description: Token list for the type $GEST-NM^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-54660
title: Tokenliste für das Type $GEST-KÜMMERN1^
title: Token list for the type $GEST-TO-CARE1^

description: Token list for the type $GEST-TO-CARE1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-KÜMMERN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-57117
title: Tokenliste für das Type $GEST-NM-KOPF-ZUSTIMMUNG1^
title: Token list for the type $GEST-NM-HEAD-AGREEMENT1^

description: Token list for the type $GEST-NM-HEAD-AGREEMENT1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-KOPF-ZUSTIMMUNG1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-66805
title: Tokenliste für das Type $GEST-KOMM-HER2^
title: Token list for the type $GEST-COME-HERE2^

description: Token list for the type $GEST-COME-HERE2^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-KOMM-HER2^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-67614
title: Tokenliste für das Type $GEST-NM-KOPFWIPPEN1^
title: Token list for the type $GEST-NM-TO-WIGGLE-ONES-HEAD1^

description: Token list for the type $GEST-NM-TO-WIGGLE-ONES-HEAD1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-KOPFWIPPEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.17632/xv9f5n6fyx.1
title: Raw data-Left inferior frontal cortex can compensate the inhibitory functions of right inferior frontal cortex and pre-supplementary motor area

description: Research data
DOI: 10.25592/dgs.corpus-2.0-type-16636
title: Tokenliste für das Type $GEST-OFF^
title: Token list for the type $GEST-OFF^

description: Token list for the type $GEST-OFF^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-OFF^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-17397
title: Tokenliste für das Type $GEST-NM-SCHULTERZUCKEN1^
title: Token list for the type $GEST-NM-TO-SHRUG1^

description: Token list for the type $GEST-NM-TO-SHRUG1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-SCHULTERZUCKEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-41916
title: Tokenliste für das Type $GEST-OHREN-ZU1^
title: Token list for the type $GEST-TO-COVER-ONES-EARS1^

description: Token list for the type $GEST-TO-COVER-ONES-EARS1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-OHREN-ZU1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-52421
title: Tokenliste für das Type $GEST-NM-KÜSSEN1^
title: Token list for the type $GEST-NM-TO-KISS1^

description: Token list for the type $GEST-NM-TO-KISS1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-KÜSSEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-61282
title: Tokenliste für das Type $GEST-OH-MEIN-GOTT1^
title: Token list for the type $GEST-OH-MY-GOD1^

description: Token list for the type $GEST-OH-MY-GOD1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-OH-MEIN-GOTT1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-67586
title: Tokenliste für das Type $GEST-NM-SPRECHEN1^
title: Token list for the type $GEST-NM-SPEAKING1^

description: Token list for the type $GEST-NM-SPEAKING1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-SPRECHEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-73015
title: Tokenliste für das Type $GEST-NM-ZUNGE-RAUSSTRECKEN1^
title: Token list for the type $GEST-NM-TO-OUTSTRECH-TONGUE1^

description: Token list for the type $GEST-NM-TO-OUTSTRECH-TONGUE1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-ZUNGE-RAUSSTRECKEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-88790
title: Tokenliste für das Type $GEST-NM-ZUSTIMMUNG1^
title: Token list for the type $GEST-NM-AGREEMENT1^

description: Token list for the type $GEST-NM-AGREEMENT1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-NM-ZUSTIMMUNG1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.5281/zenodo.3460555
title: Shipborne measurements of ClNO2 in the Mediterranean Sea and around the Arabian Peninsula during summer

description: Time series of trace gas mixing ratios and other parameters used in this study
DOI: 10.5281/zenodo.3460556
title: Shipborne measurements of ClNO2 in the Mediterranean Sea and around the Arabian Peninsula during summer

description: Time series of trace gas mixing ratios and other parameters used in this study
DOI: 10.17632/dxrp4b656h.1
title: MircoEnv

description: These data were used to quantify the impacts of air pollution policies on population health and health inequalities within a microsimulation model, MicroEnv [1]. They provide a basis for comparing results from similar models and allow researchers to integrate additional model components. [1] P. Symonds, E. Hutchinson, A. Ibbetson, J. Taylor, J. Milner, Z. Chalabi, M. Davies, P. Wilkinson, MicroEnv: A microsimulation model for quantifying the impacts of environmental policies on population health and health inequalities, Science of The Total Environment, Volume 697, (2019) 134105, ISSN 0048-9697, https://doi.org/10.1016/j.scitotenv.2019.134105.
DOI: 10.25592/dgs.corpus-2.0-type-16102
title: Tokenliste für das Type $GEST-SPITZHAND1^
title: Token list for the type $GEST-ALL-FINGERTIPS-CONTACT1^

description: Token list for the type $GEST-ALL-FINGERTIPS-CONTACT1^ (ABROAD1 / FINALLY4 / TURKEY3) from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-SPITZHAND1^ (AUSLAND1 / ENDLICH4 / TÜRKEI3) aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-17561
title: Tokenliste für das Type $GEST-SKEPTISCH1^
title: Token list for the type $GEST-SCEPTICAL1^

description: Token list for the type $GEST-SCEPTICAL1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-SKEPTISCH1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-18635
title: Tokenliste für das Type $GEST-SILBE1^
title: Token list for the type $GEST-SYLLABLE1^

description: Token list for the type $GEST-SYLLABLE1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-SILBE1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-50411
title: Tokenliste für das Type $GEST-SICH-AN-DIE-STIRN-TIPPEN1^
title: Token list for the type $GEST-TO-TAP-ONES-FOREHEAD1^

description: Token list for the type $GEST-TO-TAP-ONES-FOREHEAD1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-SICH-AN-DIE-STIRN-TIPPEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-59986
title: Tokenliste für das Type $GEST-UNGLAUBLICH1^
title: Token list for the type $GEST-INCREDIBLE1^

description: Token list for the type $GEST-INCREDIBLE1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-UNGLAUBLICH1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-60806
title: Tokenliste für das Type $GEST-TAKT1^
title: Token list for the type $GEST-BEATS1^

description: Token list for the type $GEST-BEATS1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-TAKT1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-91328
title: Tokenliste für das Type $GEST-PERSON-SCHICKEN1^
title: Token list for the type $GEST-TO-SEND-PERSON1^

description: Token list for the type $GEST-TO-SEND-PERSON1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-PERSON-SCHICKEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25606/surf.578c6039-9f75c1e6
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-430)

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 430 of the 2048³ resolution collection.
DOI: 10.17632/4dkgsyz5c8.1
title: Data for: Information Communication Technology development and energy demand in African countries

description: The data are used in the paper entitled “Information Communication Technology development and energy demand in African countries” (https://doi.org/10.1016/j.energy.2019.116192). The data concern 28 African countries for the period 1971-2014. The data on Gross Domestic Product (GDP) per capita (constant 2010 US$), electric power consumption (kWh per capita), energy use (kg of oil equivalent per capita), the number of individuals using the Internet (% of population) and the mobile cellular subscriptions per 100 people are extracted from the World Bank’s World Development Indicators. The consumer price index is sourced from the International Monetary Fund’s World Economic Outlook databases.
DOI: 10.25592/dgs.corpus-2.0-type-15883
title: Tokenliste für das Type $GEST-ÜBERLEGEN2^
title: Token list for the type $GEST-TO-PONDER2^

description: Token list for the type $GEST-TO-PONDER2^ (TO-CONTEMPLATE2) from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-ÜBERLEGEN2^ (NACHDENKEN2) aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-44593
title: Tokenliste für das Type $GEST-ÜBERLEGEN1^
title: Token list for the type $GEST-TO-PONDER1^

description: Token list for the type $GEST-TO-PONDER1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-ÜBERLEGEN1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-49916
title: Tokenliste für das Type $GEST-ZUSTIMMUNG1^
title: Token list for the type $GEST-AGREEMENT1^

description: Token list for the type $GEST-AGREEMENT1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-ZUSTIMMUNG1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-58138
title: Tokenliste für das Type $GEST-WÜTEND1^
title: Token list for the type $GEST-MAD1^

description: Token list for the type $GEST-MAD1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-WÜTEND1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-65289
title: Tokenliste für das Type $GEST-VORSICHTIG1^
title: Token list for the type $GEST-CAUTIOUS1^

description: Token list for the type $GEST-CAUTIOUS1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-VORSICHTIG1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.25592/dgs.corpus-2.0-type-74558
title: Tokenliste für das Type $GEST-VERSCHRÄNKTE-ARME1^
title: Token list for the type $GEST-CROSSED-ARMS1^

description: Token list for the type $GEST-CROSSED-ARMS1^ from the DGS Corpus release 2.0.
description: Tokenliste für das Type $GEST-VERSCHRÄNKTE-ARME1^ aus dem DGS-Korpus Release 2.0.
DOI: 10.17632/xhf3dbdrtn.1
title: Data for: Effects of different tube types on patient classification using current diabetes decision limits

description: stability testing of glucose and lactate in tubes with different glycolysis inhibitors from Greiner and Sarstedt. Study performed in volunteers. Storage of samples for up to 48 hrs, centrifugation either immediately after blood drawing or delayed for 48 hrs.
DOI: 10.25592/dgs.corpus-2.0-type-16518
title: Tokenliste für das Type $INDEX-MONITOR1^
title: Token list for the type $INDEX-TO-SCREEN1^

description: Token list for the type $INDEX-TO-SCREEN1^ ($INDEX-TO-SCREEN1) from the DGS Corpus release 2.0.
description: Tokenliste für das Type $INDEX-MONITOR1^ ($INDEX-MONITOR1) aus dem DGS-Korpus Release 2.0.