cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5517/ccdc.csd.cc21m4zt
title: CCDC 1895246: Experimental Crystal Structure Determination

description: Related Article: Naoki Ishida, Yoshiki Kamae, Masahiro Murakami|2019|Organometallics|38|1413|doi:10.1021/acs.organomet.9b00057
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21m9ss
title: CCDC 1895395: Experimental Crystal Structure Determination

description: Related Article: Sachin S. Ichake, Bharath Kumar Villuri, Sabbasani Rajasekhara Reddy, Veerababurao Kavala, Ching-Fa Yao|2019|Org.Lett.|21|2256|doi:10.1021/acs.orglett.9b00532
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21m9tt
title: CCDC 1895396: Experimental Crystal Structure Determination

description: Related Article: Sachin S. Ichake, Bharath Kumar Villuri, Sabbasani Rajasekhara Reddy, Veerababurao Kavala, Ching-Fa Yao|2019|Org.Lett.|21|2256|doi:10.1021/acs.orglett.9b00532
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21m9xx
title: CCDC 1895399: Experimental Crystal Structure Determination

description: Related Article: Sachin S. Ichake, Bharath Kumar Villuri, Sabbasani Rajasekhara Reddy, Veerababurao Kavala, Ching-Fa Yao|2019|Org.Lett.|21|2256|doi:10.1021/acs.orglett.9b00532
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.17909/t9-my41-h234
title: Large Magellanic Cloud Cepheid Standards Provide a 1\%   Foundation for the Determination of the Hubble Constant and    Stronger Evidence for Physics Beyond LambdaCDM

description: LMC Cepheid observations
DOI: 10.5517/ccdc.csd.cc1ph4dq
title: CCDC 1563683: Experimental Crystal Structure Determination

description: Related Article: Yu Zhu, Morgan Rose Olsen, May Nyman, Lei Zhang, Jian Zhang|2019|Inorg.Chem.|58|4534|doi:10.1021/acs.inorgchem.9b00093
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21lpp1
title: CCDC 1894803: Experimental Crystal Structure Determination

description: Related Article: Bin Wang, Dhika Aditya Gandamana, Fabien Gagosz, Shunsuke Chiba|2019|Org.Lett.|21|2298|doi:10.1021/acs.orglett.9b00590
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21lpr3
title: CCDC 1894805: Experimental Crystal Structure Determination

description: Related Article: Bin Wang, Dhika Aditya Gandamana, Fabien Gagosz, Shunsuke Chiba|2019|Org.Lett.|21|2298|doi:10.1021/acs.orglett.9b00590
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21lpt5
title: CCDC 1894807: Experimental Crystal Structure Determination

description: Related Article: Bin Wang, Dhika Aditya Gandamana, Fabien Gagosz, Shunsuke Chiba|2019|Org.Lett.|21|2298|doi:10.1021/acs.orglett.9b00590
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21lpv6
title: CCDC 1894808: Experimental Crystal Structure Determination

description: Related Article: Bin Wang, Dhika Aditya Gandamana, Fabien Gagosz, Shunsuke Chiba|2019|Org.Lett.|21|2298|doi:10.1021/acs.orglett.9b00590
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21mc13
title: CCDC 1895434: Experimental Crystal Structure Determination

description: Related Article: Sachin S. Ichake, Bharath Kumar Villuri, Sabbasani Rajasekhara Reddy, Veerababurao Kavala, Ching-Fa Yao|2019|Org.Lett.|21|2256|doi:10.1021/acs.orglett.9b00532
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21mcy0
title: CCDC 1895462: Experimental Crystal Structure Determination

description: Related Article: Sachin S. Ichake, Bharath Kumar Villuri, Sabbasani Rajasekhara Reddy, Veerababurao Kavala, Ching-Fa Yao|2019|Org.Lett.|21|2256|doi:10.1021/acs.orglett.9b00532
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21x9r1
title: CCDC 1904043: Experimental Crystal Structure Determination

description: Related Article: Brian W. Skelton, Murray V. Baker, David H. Brown|2019|CSD Communication|||
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.25606/surf.578c6039-e9b366d1
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-028)

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 028 of the 1024³ resolution collection.
DOI: 10.5517/ccdc.csd.cc20zwpl
title: CCDC 1876730: Experimental Crystal Structure Determination

description: Related Article: Yu Zhu, Morgan Rose Olsen, May Nyman, Lei Zhang, Jian Zhang|2019|Inorg.Chem.|58|4534|doi:10.1021/acs.inorgchem.9b00093
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc2189vh
title: CCDC 1884826: Experimental Crystal Structure Determination

description: Related Article: Samantha Zaiter, Charlotte Kirk, Matthew Taylor, Y. Maximilian Klein, Catherine E. Housecroft, Natasha F. Sciortino, John E. Clements, Richard I. Cooper, Cameron J. Kepert, Suzanne M. Neville|2019|Dalton Trans.|48|7337|doi:10.1039/C8DT05010D
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc2189wj
title: CCDC 1884827: Experimental Crystal Structure Determination

description: Related Article: Samantha Zaiter, Charlotte Kirk, Matthew Taylor, Y. Maximilian Klein, Catherine E. Housecroft, Natasha F. Sciortino, John E. Clements, Richard I. Cooper, Cameron J. Kepert, Suzanne M. Neville|2019|Dalton Trans.|48|7337|doi:10.1039/C8DT05010D
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.25606/surf.578c6039-8deb226b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-029)

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 029 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-b324a89b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-027)

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 027 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-be675dda
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-065)

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 065 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-d989c301
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-002)

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 002 of the 512³ resolution collection.
DOI: 10.6073/pasta/1a05f711ce53c00fcfc17ad550428f56
title: Breeding bird data using 50 m radius counting circles for the Parker River National Wildlife Refuge, Plum Island estuary, Massachusetts

description: This file contains breeding bird censuses using 50 m radius counting circles at locations on Plum Island, Massachusetts in the Parker River National Wildlife Refuge, Massachusetts.
DOI: 10.17632/5nm64pfdfd.1
title: Data for: Joint Contour Net Analysis for Feature Detection in Lattice Quantum Chromodynamics Data

description: The provided files contain the data used in this case study. "config.b190k1680mu0700j02s16t08" contains the raw configuration data as (binary) output from the FORTRAN 'cooling' code. "topological charge density.hvol" captures the scalar field in 4-dimensions by computing the topological charge density at each site on the lattice. "cool0030_sliced.7z" contains each 3D slice of the data across the temporal axis. Read me files are provided for parsing the scalar field in 4D ("data_structure.txt") and 3D ("sliced_data_structure.txt").
DOI: 10.25606/surf.578c6039-557f2daa
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-015)

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 015 of the 512³ resolution collection.
DOI: 10.25606/surf.578c6039-6a7c04ec
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-009)

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 009 of the 512³ resolution collection.
DOI: 10.5281/zenodo.2597687
title: Geographic variation in reproductive assurance of Clarkia pulchella

description: Code and data to accompany the manuscript "Geographic variation in reproductive assurance of <em>Clarkia pulchella"</em>.

On bioRxiv: https://doi.org/10.1101/372375 and in revision at Oecologia.
DOI: 10.5281/zenodo.2597688
title: Geographic variation in reproductive assurance of Clarkia pulchella

description: Code and data to accompany the manuscript "Geographic variation in reproductive assurance of <em>Clarkia pulchella"</em>.

On bioRxiv: https://doi.org/10.1101/372375 and in revision at Oecologia.
DOI: 10.25606/surf.578c6039-8653dbf7
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-005)

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 005 of the 512³ resolution collection.