cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.8092528
title: The Cosmos in its Infancy: JADES Galaxy Candidates at z &gt; 8 in GOODS-S and GOODS-N (JADES Deep)

description: The JADES dataset of z &gt; 8 galaxies (from the JADES-Deep public region) and galaxy candidates accompanying the paper "The Cosmos in its Infancy: JADES Galaxy Candidates at z &gt; 8 in GOODS-S and GOODS-N" (Hainline et al.). We also include the EAZY template set used for these fits. Please see the README files for descriptions of the datasets. The full dataset, which will be released on paper acceptance, can be found at this link.
description: (This portion of the dataset is only those sources that overlap with the JADES Deep region, the full dataset will be released upon journal acceptance)
DOI: 10.5281/zenodo.8092529
title: The Cosmos in its Infancy: JADES Galaxy Candidates at z &gt; 8 in GOODS-S and GOODS-N (JADES Deep)

description: The JADES dataset of z &gt; 8 galaxies (from the JADES-Deep public region) and galaxy candidates accompanying the paper "The Cosmos in its Infancy: JADES Galaxy Candidates at z &gt; 8 in GOODS-S and GOODS-N" (Hainline et al.). We also include the EAZY template set used for these fits. Please see the README files for descriptions of the datasets. The full dataset, which will be released on paper acceptance, can be found at this link.
description: (This portion of the dataset is only those sources that overlap with the JADES Deep region, the full dataset will be released upon journal acceptance)
DOI: 10.5281/zenodo.8067511
title: Fermi-GBM Data Release for GBM-230619 candidate

description: Localization for Fermi GBM-230619 combined with LIGO-Virgo subthreshold binary merger candidate localization.
DOI: 10.5281/zenodo.8067512
title: Fermi-GBM Data Release for GBM-230619 candidate

description: Localization for Fermi GBM-230619 combined with LIGO-Virgo subthreshold binary merger candidate localization.
DOI: 10.5281/zenodo.8012215
title: btsettl_cifist_xarray_full_grid

description: The grid of precomputed synthetic spectra of planetary atmosphere BT-SETTL CIFIST (Allard et al. 2013) in the xarray format. This format is used in the forward modeling code ForMoSA (https://github.com/exoAtmospheres/ForMoSA, Petrus et al. 2020, 2021, 2023). This grid explores the parameters:<br> Teff = 1200 - 7000<br> log(g) = 2.5 - 5.5
description: If you use this grid, please cite Allard et al. 2013 and Petrus et al. 2020
DOI: 10.5281/zenodo.8012214
title: btsettl_cifist_xarray_full_grid

description: The grid of precomputed synthetic spectra of planetary atmosphere BT-SETTL CIFIST (Allard et al. 2013) in the xarray format. This format is used in the forward modeling code ForMoSA (https://github.com/exoAtmospheres/ForMoSA, Petrus et al. 2020, 2021, 2023). This grid explores the parameters:<br> Teff = 1200 - 7000<br> log(g) = 2.5 - 5.5
description: If you use this grid, please cite Allard et al. 2013 and Petrus et al. 2020
DOI: 10.5281/zenodo.8015968
title: btsettl_cifist_xarray_full_grid

description: The grid of precomputed synthetic spectra of planetary atmosphere BT-SETTL CIFIST (Allard et al. 2013) in the xarray format. This format is used in the forward modeling code ForMoSA (https://github.com/exoAtmospheres/ForMoSA, Petrus et al. 2020, 2021, 2023). This grid explores the parameters:<br> Teff = 1200 - 5000<br> log(g) = 2.5 - 5.5
description: If you use this grid, please cite Allard et al. 2013 and Petrus et al. 2020
DOI: 10.5281/zenodo.8015969
title: btsettl_cifist_xarray_full_grid

description: The grid of precomputed synthetic spectra of planetary atmosphere BT-SETTL CIFIST (Allard et al. 2013) in the xarray format. This format is used in the forward modeling code ForMoSA (https://github.com/exoAtmospheres/ForMoSA, Petrus et al. 2020, 2021, 2023). This grid explores the parameters:<br> Teff = 1200 - 5000<br> log(g) = 2.5 - 5.5
description: If you use this grid, please cite Allard et al. 2013 and Petrus et al. 2020
DOI: 10.5281/zenodo.7926077
title: Galaxies simulated with GALFORM

description: The galaxies in this dataset were simulated with the semi-analytical galaxy formation code GALFORM for the study of Jahns et al. 2023, titled “How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys”. The galaxies are used as the host galaxies of simulated fast radio bursts to do forecasts of their applications. The data comprises the galaxies star formation rate, stellar mass, and the photometric magnitudes in the observer frame, including extinction, in all passbands of the Sloan Digital Sky Survey, the Euclid satellite, the Vera Rubin Observatory, and the DECam.
DOI: 10.5281/zenodo.7926078
title: Galaxies simulated with GALFORM

description: The galaxies in this dataset were simulated with the semi-analytical galaxy formation code GALFORM for the study of Jahns et al. 2023, titled “How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys”. The galaxies are used as the host galaxies of simulated fast radio bursts to do forecasts of their applications. The data comprises the galaxies star formation rate, stellar mass, and the photometric magnitudes in the observer frame, including extinction, in all passbands of the Sloan Digital Sky Survey, the Euclid satellite, the Vera Rubin Observatory, and the DECam.
DOI: 10.5281/zenodo.7887278
title: SEVN parameter file from the paper "Binary neutron star populations in the Milky Way" by Sgalletta et al., 2023

description: The repository contains the runtime parameters used in the SEVN simulations analysed in the paper "Binary neutron star populations in the Milky Way" by Sgalletta et al., 2023. <strong>Repository content: </strong> - <em>used_params_Sgalletta2023.txt<br> </em>The file contains all the runtime parameters used in the SEVN simulations. The parameters that have been varied in different runs are indicated with **** and the explored values are reported in the comment. See the SEVN userguide (https://gitlab.com/sevncodes/sevn/-/blob/SEVN/resources/SEVN_userguide.pdf) for the description of each parameter
DOI: 10.5281/zenodo.7887279
title: SEVN parameter file from the paper "Binary neutron star populations in the Milky Way" by Sgalletta et al., 2023

description: The repository contains the runtime parameters used in the SEVN simulations analysed in the paper "Binary neutron star populations in the Milky Way" by Sgalletta et al., 2023. <strong>Repository content: </strong> - <em>used_params_Sgalletta2023.txt<br> </em>The file contains all the runtime parameters used in the SEVN simulations. The parameters that have been varied in different runs are indicated with **** and the explored values are reported in the comment. See the SEVN userguide (https://gitlab.com/sevncodes/sevn/-/blob/SEVN/resources/SEVN_userguide.pdf) for the description of each parameter
DOI: 10.5517/ccdc.csd.cc2fdjn1
title: CCDC 2246373: Experimental Crystal Structure Determination

description: Related Article: Rui Wang, Chuan Wang|2023|Chemical Science|14|6449|doi:10.1039/D3SC01945D
description: Related Article: Rui Wang|2023|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.cc2ffkct
title: CCDC 2247356: Experimental Crystal Structure Determination

description: Related Article: I Wayan Dasna|2023|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.cc2ffmm4
title: CCDC 2247426: Experimental Crystal Structure Determination

description: Related Article: Yong Yang|2023|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.cc2ffmn5
title: CCDC 2247427: Experimental Crystal Structure Determination

description: Related Article: Yong Yang|2023|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.cc2ffmp6
title: CCDC 2247428: Experimental Crystal Structure Determination

description: Related Article: Yong Yang|2023|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.cc2ffmq7
title: CCDC 2247429: Experimental Crystal Structure Determination

description: Related Article: Yong Yang|2023|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.cc2ffn2m
title: CCDC 2247440: Experimental Crystal Structure Determination

description: Related Article: Xiaochuan Li|2023|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.cc2ffn9v
title: CCDC 2247447: Experimental Crystal Structure Determination

description: Related Article: Yuka  Iwasaki|2023|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.cc2fllyl
title: CCDC 2252210: Experimental Crystal Structure Determination

description: Related Article: CaiXia Jia|2023|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.cc2fln1r
title: CCDC 2252244: Experimental Crystal Structure Determination

description: Related Article: Felix Steinke, Jonas Gosch and Norbert Stock|2023|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.cc2flwvs
title: CCDC 2252486: Experimental Crystal Structure Determination

description: Related Article: cheng yaohang|2023|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.cc2flz89
title: CCDC 2252561: Experimental Crystal Structure Determination

description: Related Article: Xueshu Li, Hans-Joachim Lehmler, Sean Parkin|2023|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.cc2flz9b
title: CCDC 2252562: Experimental Crystal Structure Determination

description: Related Article: Xueshu Li, Hans-Joachim Lehmler, Sean Parkin|2023|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.cc2flzbc
title: CCDC 2252563: Experimental Crystal Structure Determination

description: Related Article: Xueshu Li, Hans-Joachim Lehmler, Sean Parkin|2023|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.cc2flzcd
title: CCDC 2252564: Experimental Crystal Structure Determination

description: Related Article: Xueshu Li, Hans-Joachim Lehmler, Sean Parkin|2023|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: 10.6073/pasta/b92dea4adbcee1d96b89f914a070bda9
title: Survey of Aspen leaf miner (Phyllocnistis populiella) Oviposition Per Leaf Sampled in Interior Alaska Aspen Stands near Fairbanks from 2004 to 2022

description: The datasets contains annual counts of aspen leaf miner eggs, incipient mines, and egg scars (indicating egg predation) on aspen leaves over time. There are two files representing pilot data from 2004-2005 and data 2006-2022. The 2004-05 dataset does not include egg scars, indicaitive of egg removal, and therefore totals underestimate total oviposition. The 2006-2022 dataset does include egg scars and therefore can be used to estimate total oviposition per leaf.
DOI: 10.5281/zenodo.7651607
title: Lightcurves, spectra and model-lightcurves of Luminous Red Novae and Intermediate Luminosity Red Transients by the Zwicky Transient Facility

description: Data release of the objects presented in the paper "Volumetric Rates of Luminous Red Novae and Intermediate Luminosity Red Transients with the Zwicky Transient Facility". This includes multiband optical-near-IR (NIR) lightcurves, optical and NIR spectra of LRNe, ILRTs and possible LBV outbursts presented in the paper. The release also includes Gaussian-Process lightcurve templates of LRNe and ILRTs, that were used to simulate these transients and determine their volumetric rates.
DOI: 10.5281/zenodo.7651606
title: Lightcurves, spectra and model-lightcurves of Luminous Red Novae and Intermediate Luminosity Red Transients by the Zwicky Transient Facility

description: Data release of the objects presented in the paper "Volumetric Rates of Luminous Red Novae and Intermediate Luminosity Red Transients with the Zwicky Transient Facility". This includes multiband optical-near-IR (NIR) lightcurves, optical and NIR spectra of LRNe, ILRTs and possible LBV outbursts presented in the paper. The release also includes Gaussian-Process lightcurve templates of LRNe and ILRTs, that were used to simulate these transients and determine their volumetric rates.
DOI: 10.5281/zenodo.7752544
title: The underlying radial acceleration relation -- supplementary data

description: Supplementary data and plots associated with "The underlying radial acceleration relation", Desmond (2023). See the README for further information.
description: HD is supported by a Royal Society University Research Fellowship (grant no. 211046).
DOI: 10.6073/pasta/3c4412a8298fdee611c12a3ccb7aea09
title: Survey of aspen herbivory and aspen leaf miner (Phyllocnistis populiella) survival and abundance from 2006 to 2022

description: Leaf-level measurements of herbivory damage on quaking aspen caused by the aspen leaf miner (ALM) and externally-feeding herbivores, and ALM abundance and survival, from four sites near Fairbanks, Alaska over time.
DOI: 10.5281/zenodo.7760360
title: Products and Models for "Volatile-to-sulfur Ratios Can Recover a Gas Giant's Accretion History"

description: The newfound ability to detect SO2 in exoplanet atmospheres and presents an opportunity to measure sulfur abundances and so directly test between competing modes of planet formation. To explore the detectability of SO2 in<br> transmission spectra and its ability to diagnose planet formation, we present a grid of atmospheric photochemical models and corresponding synthetic spectra for WASP-39b (where SO2 has recently been detected). Our grid contains 2,662 model atmospheres: spanning 1-100x the solar abundance ratios of C, O, and S (11^3 combinations of abundances) and for two thermal profiles: corresponding to the morning and evening terminators. We also provide 3,993 synthetic spectra: one for each of the morning and evening terminators, plus a set of spectra that are the<br> mean of the morning and evening spectra (corresponding to the transmission spectrum that would be observed during transit). If you use these files, please cite Crossfield (2023). The transmission spectra are simple two-column CSV files -- wavelength in microns, and transit depth. The model atmospheres are in Python pickle format, and are the standard output of the VULCAN photochemistry code. The several data sets are: wasp39_mean_spectra.tar.gz -- average terminator spectra. <strong>Use this for comparing to full-transit observations.</strong> wasp39_morning_spectra.tar.gz -- spectra corresponding to the morning-terminator models. wasp39_evening_spectra.tar.gz -- spectra corresponding to the evening-terminator models. wasp39_evening_profiles.tar.gz -- model atmospheres and chemical profiles for the evening-terminator thermal profile. wasp39_morning_profiles.tar.gz -- model atmospheres and chemical profiles for the morning-terminator thermal profile. All filenames are of the form wasp39b_tsai23-Kzz_SNCHO_10x_z83_C7.5_N10.0_O100.0_S18.0__morn_transmission.csv wasp39b -- planet name tsai23-Kzz -- using Kzz (eddy diffusion) profile from Tsai et al. (2023) SNCHO -- using the VULCAN code's SNCHO chemistry network 10x -- all elements (aside from SNCHO) are set to 10x Solar abundances z83 -- zenith angle set to 83 degrees C7.5 -- the scaling of the Carbon abundance relative to Solar; in this case, 7.5x N10.0 -- the scaling of the Nitrogren abundance relative to Solar (10x for all models) O100.0 -- the scaling of the Oxygen abundance relative to Solar; in this case, 100x S18.0 -- the scaling of the Sulfur abundance relative to Solar; in this case, 18x morn -- morning terminator thermal profile, from Tsai et al. (2023). Options are 'morn', 'eve', 'morn-eve-mean' transmission.csv -- indicates a transmission spectrum file. Other option is 'vulcan-output.vul'
DOI: 10.5281/zenodo.7760359
title: Products and Models for "Volatile-to-sulfur Ratios Can Recover a Gas Giant's Accretion History"

description: The newfound ability to detect SO2 in exoplanet atmospheres and presents an opportunity to measure sulfur abundances and so directly test between competing modes of planet formation. To explore the detectability of SO2 in<br> transmission spectra and its ability to diagnose planet formation, we present a grid of atmospheric photochemical models and corresponding synthetic spectra for WASP-39b (where SO2 has recently been detected). Our grid contains 2,662 model atmospheres: spanning 1-100x the solar abundance ratios of C, O, and S (11^3 combinations of abundances) and for two thermal profiles: corresponding to the morning and evening terminators. We also provide 3,993 synthetic spectra: one for each of the morning and evening terminators, plus a set of spectra that are the<br> mean of the morning and evening spectra (corresponding to the transmission spectrum that would be observed during transit). If you use these files, please cite Crossfield (2023). The transmission spectra are simple two-column CSV files -- wavelength in microns, and transit depth. The model atmospheres are in Python pickle format, and are the standard output of the VULCAN photochemistry code. The several data sets are: wasp39_mean_spectra.tar.gz -- average terminator spectra. <strong>Use this for comparing to full-transit observations.</strong> wasp39_morning_spectra.tar.gz -- spectra corresponding to the morning-terminator models. wasp39_evening_spectra.tar.gz -- spectra corresponding to the evening-terminator models. wasp39_evening_profiles.tar.gz -- model atmospheres and chemical profiles for the evening-terminator thermal profile. wasp39_morning_profiles.tar.gz -- model atmospheres and chemical profiles for the morning-terminator thermal profile. All filenames are of the form wasp39b_tsai23-Kzz_SNCHO_10x_z83_C7.5_N10.0_O100.0_S18.0__morn_transmission.csv wasp39b -- planet name tsai23-Kzz -- using Kzz (eddy diffusion) profile from Tsai et al. (2023) SNCHO -- using the VULCAN code's SNCHO chemistry network 10x -- all elements (aside from SNCHO) are set to 10x Solar abundances z83 -- zenith angle set to 83 degrees C7.5 -- the scaling of the Carbon abundance relative to Solar; in this case, 7.5x N10.0 -- the scaling of the Nitrogren abundance relative to Solar (10x for all models) O100.0 -- the scaling of the Oxygen abundance relative to Solar; in this case, 100x S18.0 -- the scaling of the Sulfur abundance relative to Solar; in this case, 18x morn -- morning terminator thermal profile, from Tsai et al. (2023). Options are 'morn', 'eve', 'morn-eve-mean' transmission.csv -- indicates a transmission spectrum file. Other option is 'vulcan-output.vul'
DOI: 10.5281/zenodo.7533373
title: Dataset for article "From X-rays to physical parameters: a comprehensive analysis of thermal tidal disruption event X-ray spectra"

description: This repository contains the data used in the modeling of TDE X-ray emission within the article: Mummery et al. 2023, " From X-rays to physical parameters: a comprehensive analysis of thermal<br> tidal disruption event X-ray spectra" published as Mummery et al. 2023, MNRAS, 519, 5828