cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5517/ccdc.csd.cc20y2jl
title: CCDC 1874989: Experimental Crystal Structure Determination

description: Related Article: Yassine Beldjoudi,  Ana Arauzo,  Javier Campo,  Emma L. Gavey,  Melanie Pilkington,  Mitchell A. Nascimento,  Jeremy M. Rawson|2019|J.Am.Chem.Soc.|141|6875|doi:10.1021/jacs.8b11528
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.cc20y2km
title: CCDC 1874990: Experimental Crystal Structure Determination

description: Related Article: Yassine Beldjoudi,  Ana Arauzo,  Javier Campo,  Emma L. Gavey,  Melanie Pilkington,  Mitchell A. Nascimento,  Jeremy M. Rawson|2019|J.Am.Chem.Soc.|141|6875|doi:10.1021/jacs.8b11528
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.578c6039-392c9e09
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-039)

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 039 of the 512³ resolution collection.
DOI: 10.25606/surf.578c6039-5760cdd0
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-036)

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 036 of the 512³ resolution collection.
DOI: 10.25606/surf.578c6039-87b60c3c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-084)

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 084 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-a03822f6
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-083)

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 083 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-a0b52515
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-085)

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 085 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-ac4246d0
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-038)

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 038 of the 512³ resolution collection.
DOI: 10.25606/surf.578c6039-d875bb95
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-086)

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 086 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.2652268
title: 0.3 ms of asymmetric GM1:POPC/POPC (2:98/100) bilayer

description: Cone-like GM1. Fifth 25 microseconds of total 300 microseconds.
DOI: 10.5517/ccdc.csd.cc20y2ln
title: CCDC 1874991: Experimental Crystal Structure Determination

description: Related Article: Yassine Beldjoudi,  Ana Arauzo,  Javier Campo,  Emma L. Gavey,  Melanie Pilkington,  Mitchell A. Nascimento,  Jeremy M. Rawson|2019|J.Am.Chem.Soc.|141|6875|doi:10.1021/jacs.8b11528
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.cc20y2mp
title: CCDC 1874992: Experimental Crystal Structure Determination

description: Related Article: Yassine Beldjoudi,  Ana Arauzo,  Javier Campo,  Emma L. Gavey,  Melanie Pilkington,  Mitchell A. Nascimento,  Jeremy M. Rawson|2019|J.Am.Chem.Soc.|141|6875|doi:10.1021/jacs.8b11528
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.cc21ck00
title: CCDC 1887931: Experimental Crystal Structure Determination

description: Related Article: Zhenxing Liu, Chaofan Xu, Juan del Pozo, Sebastian Torker, Amir H. Hoveyda|2019|J.Am.Chem.Soc.|141|7137|doi:10.1021/jacs.9b02318
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.cc21ck11
title: CCDC 1887932: Experimental Crystal Structure Determination

description: Related Article: Zhenxing Liu, Chaofan Xu, Juan del Pozo, Sebastian Torker, Amir H. Hoveyda|2019|J.Am.Chem.Soc.|141|7137|doi:10.1021/jacs.9b02318
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.cc21hjvy
title: CCDC 1891770: Experimental Crystal Structure Determination

description: Related Article: Zhen Zhang,  Sujun Xie,  Bin Cheng,  Hongbin Zhai,  Yun Li|2019|J.Am.Chem.Soc.|141|7147|doi:10.1021/jacs.9b02362
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.cc21hk26
title: CCDC 1891777: Experimental Crystal Structure Determination

description: Related Article: Zhen Zhang,  Sujun Xie,  Bin Cheng,  Hongbin Zhai,  Yun Li|2019|J.Am.Chem.Soc.|141|7147|doi:10.1021/jacs.9b02362
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.cc21hk6b
title: CCDC 1891781: Experimental Crystal Structure Determination

description: Related Article: Zhen Zhang,  Sujun Xie,  Bin Cheng,  Hongbin Zhai,  Yun Li|2019|J.Am.Chem.Soc.|141|7147|doi:10.1021/jacs.9b02362
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.cc21hk9f
title: CCDC 1891784: Experimental Crystal Structure Determination

description: Related Article: Zhen Zhang,  Sujun Xie,  Bin Cheng,  Hongbin Zhai,  Yun Li|2019|J.Am.Chem.Soc.|141|7147|doi:10.1021/jacs.9b02362
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.cc21p474
title: CCDC 1897145: Experimental Crystal Structure Determination

description: Related Article: Zhen Zhang,  Sujun Xie,  Bin Cheng,  Hongbin Zhai,  Yun Li|2019|J.Am.Chem.Soc.|141|7147|doi:10.1021/jacs.9b02362
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.cc225xjq
title: CCDC 1912313: Experimental Crystal Structure Determination

description: Related Article: Alex L. Nguyen, Frank R. Fronczek, M. Graca H. Vicente|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: 10.5517/ccdc.csd.cc2260bn
title: CCDC 1912400: Experimental Crystal Structure Determination

description: Related Article: Kabali Senthilkumar,  Mateusz Kondratowicz,  Tadeusz Lis,  Piotr J. Chmielewski,  Joanna Cybińska,  José L. Zafra,  Juan Casado,  Thomas Vives,  Jeanne Crassous,  Ludovic Favereau,  Marcin Stępień|2019|J.Am.Chem.Soc.|141|7421|doi:10.1021/jacs.9b01797
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: 10.18716/nmrshiftdb2/60000003/chemie_koeln_cd2cl2
title: chemie koeln NMR dataset for Cytisin in Methylenchloride-D2 (CD2Cl2)
DOI: 10.5517/ccdc.csd.cc1pqd4y
title: CCDC 1570650: Experimental Crystal Structure Determination

description: Related Article: Arzu Binici, Aytuğ Okumuş, Gamze Elmas, Zeynel Kılıç, Nagehan Ramazanoğlu, Leyla Açık, Hülya Şimşek, Beste Çağdaş Tunalı, Mustafa Türk, Remziye Güzel, Tuncer Hökelek|2019|New J.Chem.|43|6856|doi:10.1039/C9NJ00577C
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.cc1zhqfm
title: CCDC 1832361: Experimental Crystal Structure Determination

description: Related Article: D. Anu, P. Naveen, B. VijayaPandiyan, Christopher S. Frampton, M.V. Kaveri|2019|Polyhedron|167|137|doi:10.1016/j.poly.2019.04.021
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.cc1zn9jg
title: CCDC 1836766: Experimental Crystal Structure Determination

description: Related Article: Tapashi Das, Kajal Krishna Rajak|2019|Dalton Trans.|48|6879|doi:10.1039/C9DT00901A
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.cc1zn9kh
title: CCDC 1836767: Experimental Crystal Structure Determination

description: Related Article: Tapashi Das, Kajal Krishna Rajak|2019|Dalton Trans.|48|6879|doi:10.1039/C9DT00901A
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.cc1zn9lj
title: CCDC 1836768: Experimental Crystal Structure Determination

description: Related Article: Tapashi Das, Kajal Krishna Rajak|2019|Dalton Trans.|48|6879|doi:10.1039/C9DT00901A
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.cc1znrjx
title: CCDC 1837200: Experimental Crystal Structure Determination

description: Related Article: Jala Ranjith, Palakodety Radha Krishna|2019|Tetrahedron Lett.|60|1437|doi:10.1016/j.tetlet.2019.04.041
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.cc1zrpv8
title: CCDC 1840031: Experimental Crystal Structure Determination

description: Related Article: Wei Zhou, Hao Liu, Yongyi Guo, Yiting Gu, Jing Han, Jie Chen, Hongmei Deng, Min Shao, Hui Zhang, Weiguo Cao|2019|J.Fluorine Chem.|222-223|51|doi:10.1016/j.jfluchem.2019.04.015
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.cc2007gr
title: CCDC 1847273: Experimental Crystal Structure Determination

description: Related Article: Jie Li|2019|J.Mol.Struct.|1190|160|doi:10.1016/j.molstruc.2019.04.057
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.