cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.3468591
title: Festival of Frequency Measurement 1 October 2019 KM4YMI 33.83 -84.28 5MHz

description: Festival of Frequency Measurement 1 October 2019 Name: Beau B. Bruce<br> Callsign: KM4YMI<br> Lat/long: 33.83, -84,28<br> Grid Square: EM73ut<br> Start time: 30 Sep 2019 21:54 UTC<br> End time: 1 Oct 2019 00:05 UTC<br> Antenna: 130ft ladder line fed inv vee<br> Receiver: IC-7100<br> Frequency reference: WWV 5Mhz<br> Frequency measurement completed with fldigi's frequency calibration mode with receiver tuned to 4.999MHz in USB mode and cursor at 1000Hz
DOI: 10.5281/zenodo.3466953
title: Phenological Center - Insects

description: Insects Phenology dataset compiled by Komarov Botanical Institute (Russian Federation) by digitizing paper based records of volunteer network of phenological observers (Fenologicheskii Klub) resulting in 1822 records collected for 75 years between 1923 and 1998.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.5281/zenodo.3466954
title: Phenological Center - Insects

description: Insects Phenology dataset compiled by Komarov Botanical Institute (Russian Federation) by digitizing paper based records of volunteer network of phenological observers (Fenologicheskii Klub) resulting in 1822 records collected for 75 years between 1923 and 1998.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.5281/zenodo.3466955
title: Chronicle of Nature - Phenology of Plants of Voronezhsky Nature Biosphere Reserve

description: Plants Phenology dataset compiled in the context of Chronicle of Nature program in Voronezhsky Nature Biosphere Reserve (Russian Federation) consisting of 1802 records collected during 80 years between 1937 and 2017.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.5281/zenodo.3466956
title: Chronicle of Nature - Phenology of Plants of Voronezhsky Nature Biosphere Reserve

description: Plants Phenology dataset compiled in the context of Chronicle of Nature program in Voronezhsky Nature Biosphere Reserve (Russian Federation) consisting of 1802 records collected during 80 years between 1937 and 2017.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.5281/zenodo.3466957
title: Chronicle of Nature - Phenology of Birds of Pechoro-Ilych State Nature Reserve

description: Birds Phenology dataset compiled in the context of Chronicle of Nature program in Pechoro-Ilych State Nature Reserve (Russian Federation) consisting of 1652 records collected during 80 years between 1936 and 2015.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.5281/zenodo.3466958
title: Chronicle of Nature - Phenology of Birds of Pechoro-Ilych State Nature Reserve

description: Birds Phenology dataset compiled in the context of Chronicle of Nature program in Pechoro-Ilych State Nature Reserve (Russian Federation) consisting of 1652 records collected during 80 years between 1936 and 2015.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.5281/zenodo.3468602
title: Festival of Frequency Measurement 1 October 2019

description: Festival of Frequency Measurement Submission —- event: WWV Centennial UTC date:1 oct 2019 beacon frequency: 5 Mhz station name:n1naz latitude and longitude and/or maidenhead grid square: fn42gu city:Londonderry state or region:NH Difficulties had:late start late finish Anything you know about the stability of your equipment: Flex Radio 6500 TXO
DOI: 10.5281/zenodo.3468603
title: Festival of Frequency Measurement 1 October 2019

description: Festival of Frequency Measurement Submission —- event: WWV Centennial UTC date:1 oct 2019 beacon frequency: 5 Mhz station name:n1naz latitude and longitude and/or maidenhead grid square: fn42gu city:Londonderry state or region:NH Difficulties had:late start late finish Anything you know about the stability of your equipment: Flex Radio 6500 TXO
DOI: 10.5281/zenodo.3466960
title: Chronicle of Nature - Phenology of Birds of State Nature Reserve Malaya Sosva

description: Birds Phenology dataset compiled in the context of Chronicle of Nature program in State Nature Reserve Malaya Sosva (Russian Federation) consisting of 1635 records collected during 33 years between 1983 and 2015.
description: This dataset export was created by EarthCape software platform version 18.3.1.17814
DOI: 10.17632/hjn9d5tfj3.3
title: Data for: Holistic economic analysis of building integrated photovoltaics (BIPV) system: case studies evaluation

description: Solar radiation data for the selected cities as well as LCCA and DPP calculation for BIPV system.
DOI: 10.5281/zenodo.3468231
title: Archaeology Vocabulary DEU-ENG

description: This collection of German-English archaeology vocabulary was created in the course of translating archaeological, art historical, historical academic scholarship from German to English for a variety of German and Austrian archaeological institutes and museums. All words underwent extensive research to make sure the words are correct and in some cases references are also included. Not all words have a direct translations. Subjects covered include field archaeology, architecture, pottery, methods, fortification, and many more. The collections archaeology_terminology and term_list_archaeology were originally created in SDL Multiterm 2015 and 2017 and then combined to create archaeology_terminology_complete which was also cleaned in OpenRefine 3.1 File formats uploaded here include xlsx and MultiTerm Termbase.
DOI: 10.5281/zenodo.3468232
title: Archaeology Vocabulary DEU-ENG

description: This collection of German-English archaeology vocabulary was created in the course of translating archaeological, art historical, historical academic scholarship from German to English for a variety of German and Austrian archaeological institutes and museums. All words underwent extensive research to make sure the words are correct and in some cases references are also included. Not all words have a direct translations. Subjects covered include field archaeology, architecture, pottery, methods, fortification, and many more. The collections archaeology_terminology and term_list_archaeology were originally created in SDL Multiterm 2015 and 2017 and then combined to create archaeology_terminology_complete which was also cleaned in OpenRefine 3.1 File formats uploaded here include xlsx and MultiTerm Termbase.
DOI: 10.5281/zenodo.3468606
title: Festival of Frequency Measurement Submission

description: The location of this measurement was La Canada, California<br> A very stable GPS locked receiver was used. (Icom 7610) Test measurements of GPS locked broadcast stations on 980, 1070 and 1260 kHZ showed a system frequency error of .03 Hz high. This .03 Hz high error existed before and after the 24 hour 5 mHz measurement. Thus for absolute frequencies a .03 Hz must be subtracted. The antenna used was a ground mounted electrostatic shielded loop antenna. Software used was fldigi.
DOI: 10.5281/zenodo.3468607
title: Festival of Frequency Measurement Submission

description: The location of this measurement was La Canada, California<br> A very stable GPS locked receiver was used. (Icom 7610) Test measurements of GPS locked broadcast stations on 980, 1070 and 1260 kHZ showed a system frequency error of .03 Hz high. This .03 Hz high error existed before and after the 24 hour 5 mHz measurement. Thus for absolute frequencies a .03 Hz must be subtracted. The antenna used was a ground mounted electrostatic shielded loop antenna. Software used was fldigi.
DOI: 10.17632/cvphcg2hzg.1
title: Data for: AFFIRMATIVE ACTION IN BRAZILIAN UNIVERSITIES: EFFECTS ON THE ENROLLMENT OF TARGETED GROUPS

description: Data and scripts used in the revised version of AFFIRMATIVE ACTION IN BRAZILIAN UNIVERSITIES: EFFECTS ON THE ENROLLMENT OF TARGETED GROUPS by Renato Vieira and Mary Arends-Kuenning
DOI: 10.25606/surf.578c6039-fba3f2c9
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-724)

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 724 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3468598
title: Festival of Frequency Measurement 1 October 2019

description: Festival of Frequency Measurement Submission - event: WWV Centennial UTC date: 2019-10-01 beacon frequency: 5 MHz station name: AC6SL latitude and longitude and/or maidenhead grid square: 37.13N 122.12W CM87wd city: Boulder Creek state or region: California, USA Difficulties had: poor reception during daylight hours Anything you know about the stability of your equipment: receiver stability ~1 Hz, soundcard stability unknown 40m Delta Loop antenna, Elecraft K3 transceiver, Dell laptop, linux, fldigi 4.0.1 recording started 40 minutes before, & ended 30 minutes after target date
DOI: 10.5281/zenodo.3468599
title: Festival of Frequency Measurement 1 October 2019

description: Festival of Frequency Measurement Submission - event: WWV Centennial UTC date: 2019-10-01 beacon frequency: 5 MHz station name: AC6SL latitude and longitude and/or maidenhead grid square: 37.13N 122.12W CM87wd city: Boulder Creek state or region: California, USA Difficulties had: poor reception during daylight hours Anything you know about the stability of your equipment: receiver stability ~1 Hz, soundcard stability unknown 40m Delta Loop antenna, Elecraft K3 transceiver, Dell laptop, linux, fldigi 4.0.1 recording started 40 minutes before, & ended 30 minutes after target date
DOI: 10.25606/surf.578c6039-195dacea
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-208)

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 208 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-b6f51e2c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-570)

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 570 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-f8551990
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-641)

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 641 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-7834d3e0
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-180)

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 180 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3333367
title: Replication Package: Microservice-tailored Generation of Session-based Workload Models for Representative Load Testing

description: This is the replication package for the publication <em>Microservice-tailored Generation of Session-based Workload Models for Representative Load Testing</em>, MASCOTS 2019. It holds the experiment setup, results, and detailed analyses of the results. The README.md (or README.pdf) contains further descriptions and instructions.
description: This work is being supported by the German Federal Ministry of Education and Research (grant no. 01IS17010, ContinuITy) and the European Union's Horizon 2020 research and innovation programme (grant no.825040, RADON). The authors would like to thank the HPI Future SOC Lab for providing the infrastructure.
DOI: 10.5281/zenodo.3468608
title: WWV 5 MHz

description: Festival of Frequency Measurement 01 October 2019<br> Event : WWV Centennial<br> UTC date : 01 October 2019<br> Beacon Frequency : 5 MHz<br> Submitter : Martin H Potter, VE3OAT<br> Data recorded at : 45.2525N 75.5910W<br> City : Greely<br> Region : Ontario, CANADA WARNING : Data recorded during 1330-2230 UTC considered NOT USEFUL/INVALID due<br> to weak or non-existent signal reception. <br> <br> Data file : VE3OAT 45.25 -75.59 5 MHz.csv<br> Data start time : 2019 Sep 30 23:56 UTC<br> Antenna : 80/40 m band inverted-V dipoles with common feed<br> Antenna orientation : NW-SE<br> Receiver : Yaesu FTdx1200 transceiver<br> Frequency reference : internal, undisciplined<br> Receiver mode : USB<br> IF bandwidth : 1800 Hz<br> AGC : fast<br> Digital Noise Reduction (DNR) : off<br> Frequency measurement method : Reciever in USB mode tuned to 4999.000 kHz,<br> audio output to computer sound card, frequency measured and recorded by<br> Fldigi v4.1.06 software.<br> Computer sound card : calibrated by Fldigi "WWV" function Observation : At 0345 UTC, rapid "flutter" fading of the signal was noted with<br> smearing of the displayed signal frequency.
DOI: 10.5281/zenodo.3468609
title: WWV 5 MHz

description: Festival of Frequency Measurement 01 October 2019<br> Event : WWV Centennial<br> UTC date : 01 October 2019<br> Beacon Frequency : 5 MHz<br> Submitter : Martin H Potter, VE3OAT<br> Data recorded at : 45.2525N 75.5910W<br> City : Greely<br> Region : Ontario, CANADA WARNING : Data recorded during 1330-2230 UTC considered NOT USEFUL/INVALID due<br> to weak or non-existent signal reception. <br> <br> Data file : VE3OAT 45.25 -75.59 5 MHz.csv<br> Data start time : 2019 Sep 30 23:56 UTC<br> Antenna : 80/40 m band inverted-V dipoles with common feed<br> Antenna orientation : NW-SE<br> Receiver : Yaesu FTdx1200 transceiver<br> Frequency reference : internal, undisciplined<br> Receiver mode : USB<br> IF bandwidth : 1800 Hz<br> AGC : fast<br> Digital Noise Reduction (DNR) : off<br> Frequency measurement method : Reciever in USB mode tuned to 4999.000 kHz,<br> audio output to computer sound card, frequency measured and recorded by<br> Fldigi v4.1.06 software.<br> Computer sound card : calibrated by Fldigi "WWV" function Observation : At 0345 UTC, rapid "flutter" fading of the signal was noted with<br> smearing of the displayed signal frequency.
DOI: 10.5281/zenodo.3333366
title: Replication Package: Microservice-tailored Generation of Session-based Workload Models for Representative Load Testing

description: This is the replication package for the publication <em>Microservice-tailored Generation of Session-based Workload Models for Representative Load Testing</em>, MASCOTS 2019. It holds the experiment setup, results, and detailed analyses of the results. The README.md (or README.pdf) contains further descriptions and instructions.
description: This work is being supported by the German Federal Ministry of Education and Research (grant no. 01IS17010, ContinuITy) and the European Union's Horizon 2020 research and innovation programme (grant no.825040, RADON). The authors would like to thank the HPI Future SOC Lab for providing the infrastructure.
DOI: 10.5281/zenodo.3468618
title: WWV measurements by VE3YX

description: 3 Files: Fldigi measurement of WWV, Fldigi measurement of stabilized sig gen, and WORD doc describing set up and issues.
DOI: 10.5281/zenodo.3468619
title: WWV measurements by VE3YX

description: 3 Files: Fldigi measurement of WWV, Fldigi measurement of stabilized sig gen, and WORD doc describing set up and issues.
DOI: 10.5281/zenodo.3468620
title: WWV Centennial Frequency Measurement

description: Radio is a ICOM IC 7610 fldigi version 4.0.18 grid EN16aw Stopped data collection at 23:15. The station was needed as the operator was Net Control for the North Dakota Evening net.
DOI: 10.5281/zenodo.3468621
title: WWV Centennial Frequency Measurement

description: Radio is a ICOM IC 7610 fldigi version 4.0.18 grid EN16aw Stopped data collection at 23:15. The station was needed as the operator was Net Control for the North Dakota Evening net.
DOI: 10.5281/zenodo.3468612
title: aj5p 31.73 -89.14 5 MHz.csv

description: Festival of Frequency Measurement 1 October 2019 Call: AJ5P Name: Lester Tarbutton Coord: 31.73 -89.14 (Laurel, MS) Frequency 5 MHz Start 2345 utc 9-30-19 Station: IC-7300, tuned loop ant (east-west), FLDIGI. Stability less than 0.1 Hz after 12 hr warm up of rig and computer. See Addditionl notes
description: Data Interpretation: Good signals until 9:00 a.m.local (1400Z) then deep fades. By 11:15 local signals poor. At 3 p.m. signals began to rebound and were strong by 4:30 p.m. During this time, lock was achieved only on signal peaks and read 5000000.25 plus or minus 0.04 Daytime data outside this range should be regarded as artifact. This also indicates that all frequencies should be adjusted down by 0.25 Hz as daytime frequency is more accurate and stable. Selective fades noted at 5:30 pm at onset of downward doppler shift.
DOI: 10.5281/zenodo.3468613
title: aj5p 31.73 -89.14 5 MHz.csv

description: Festival of Frequency Measurement 1 October 2019 Call: AJ5P Name: Lester Tarbutton Coord: 31.73 -89.14 (Laurel, MS) Frequency 5 MHz Start 2345 utc 9-30-19 Station: IC-7300, tuned loop ant (east-west), FLDIGI. Stability less than 0.1 Hz after 12 hr warm up of rig and computer. See Addditionl notes
description: Data Interpretation: Good signals until 9:00 a.m.local (1400Z) then deep fades. By 11:15 local signals poor. At 3 p.m. signals began to rebound and were strong by 4:30 p.m. During this time, lock was achieved only on signal peaks and read 5000000.25 plus or minus 0.04 Daytime data outside this range should be regarded as artifact. This also indicates that all frequencies should be adjusted down by 0.25 Hz as daytime frequency is more accurate and stable. Selective fades noted at 5:30 pm at onset of downward doppler shift.