cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.6555145
title: Data Release: "No evidence that the majority of black holes in binaries have zero spin"

description: This dataset contains the results presented in "<em>No evidence that the majority of black holes in binaries have zero spin</em>". In this paper, we systematically explored the effective and component spin distributions of binary black holes among the LIGO/Virgo GWTC-3 catalog. In particular, we tried to answer the following core questions, which have been the subject of active exploration and some debate in the literature: <em>1. Is there an excess of binary black holes with vanishing spin, as predicted by some theories of angular momentum transport in stellar cores?</em> <strong>We find no evidence for an excess of vanishing spin systems.</strong> This finding is confirmed by three complementary analyses: one relying only on the Bayes factors between spinning and non-spinning priors for each BBH observation, one that seeks to model the distribution of effective aligned spins, and one modeling the distribution of component spin magnitudes and misalignment angles. Instead, we find BBH spin magnitudes to be consistent with a single, continuous distribution that remains finite at magnitude zero. <em>2. Do there exist binaries with component spins misaligned by more than 90 degrees relative to their orbits?</em> <strong>We find a strong preference for the existence of such strongly misaligned spins.</strong> Our analysis of the BBH component spin distribution indicates that at least some component spins are misaligned from their orbits by more than 90 degrees. This result is robust under a variety of modeling choices regarding both the distribution of component spin magnitudes and tilts. The code used to generate this data can be found in the repository https://github.com/tcallister/gwtc3-spin-studies/. This repository includes jupyter notebooks that can be used to open, explore, and plot the files contained in this data set. Additional information about reproducing and/or using this dataset can be found in our associated documentation. Further notes: The files <em>sampleDict_FAR_1_in_1_yr.pickle</em> and <em>injectionDict_FAR_1_in_1.pickle</em>, used as inputs to our analyses, are created via code in the repository https://github.com/tcallister/get-lvk-data (see also https://zenodo.org/record/6505409). The file <em>posteriors_gaussian_spin_samples_FAR_1_in_1.json</em>, used for figure generation, was published by the LIGO Scientific Collaboration, Virgo Collaboration, and KAGRA Collaboration in support of the paper "The population of merging compact binaries inferred using gravitational waves through GWTC-3" (see https://zenodo.org/record/5655785).
DOI: 10.5281/zenodo.6505272
title: Data Release: "No evidence that the majority of black holes in binaries have zero spin"

description: This dataset contains the results presented in "<em>No evidence that the majority of black holes in binaries have zero spin</em>". In this paper, we systematically explored the effective and component spin distributions of binary black holes among the LIGO/Virgo GWTC-3 catalog. In particular, we tried to answer the following core questions, which have been the subject of active exploration and some debate in the literature: <em>1. Is there an excess of binary black holes with vanishing spin, as predicted by some theories of angular momentum transport in stellar cores?</em> <strong>We find no evidence for an excess of vanishing spin systems.</strong> This finding is confirmed by three complementary analyses: one relying only on the Bayes factors between spinning and non-spinning priors for each BBH observation, one that seeks to model the distribution of effective aligned spins, and one modeling the distribution of component spin magnitudes and misalignment angles. Instead, we find BBH spin magnitudes to be consistent with a single, continuous distribution that remains finite at magnitude zero. <em>2. Do there exist binaries with component spins misaligned by more than 90 degrees relative to their orbits?</em> <strong>We find a strong preference for the existence of such strongly misaligned spins.</strong> Our analysis of the BBH component spin distribution indicates that at least some component spins are misaligned from their orbits by more than 90 degrees. This result is robust under a variety of modeling choices regarding both the distribution of component spin magnitudes and tilts. The code used to generate this data can be found in the repository https://github.com/tcallister/gwtc3-spin-studies/. This repository includes jupyter notebooks that can be used to open, explore, and plot the files contained in this data set. Additional information about reproducing and/or using this dataset can be found in our associated documentation. Further notes: The files <em>sampleDict_FAR_1_in_1_yr.pickle</em> and <em>injectionDict_FAR_1_in_1.pickle</em>, used as inputs to our analyses, are created via code in the repository https://github.com/tcallister/get-lvk-data (see also https://zenodo.org/record/6505409). The file <em>posteriors_gaussian_spin_samples_FAR_1_in_1.json</em>, used for figure generation, was published by the LIGO Scientific Collaboration, Virgo Collaboration, and KAGRA Collaboration in support of the paper "The population of merging compact binaries inferred using gravitational waves through GWTC-3" (see https://zenodo.org/record/5655785).
DOI: 10.6084/m9.figshare.16649569.v3
title: Network: lter, Domain: hbef

description: MacroSheds timeseries data, shapefiles, and metadata for domain: hbef, within network: lter
DOI: 10.25919/vqrs-x419
title: Parkes observations for project P1054 semester 2022APRS_05

description: With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourteen sources have been discovered in targeted observations of Fermi unidentified point sources, three in the Small Magellanic Cloud, 37 in Globular Clusters and 34 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including at least one double neutron star system and several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries. The UWL has also the unique advantage of allowing detailed studies of the eclipses of the so-called 'spider' pulsars, which make up about 1/3rd of the sources we aim at following-up with this project.
DOI: 10.25919/072w-9x25
title: Parkes observations for project P1032 semester 2022APRS_02

description: This project aims to continue to perform rapid measurements of relativistic parameters of southern binary pulsar systems using data from the Parkes Ultra Wideband Low (UWL) receiver and the MeerKAT telescope thereby enabling measurement of their component masses and in some cases, test theories of gravity. We will use the UWL data to obtain significant orbital coverage and timing baseline on these pulsars and obtain important constraints on orbital and temporal DM variations that will help in identifying the nature of the companion star. We will then use MeerKAT data at crucial orbital phases to improve our chances of measuring the relativistic parameters. Increase in the number of measured NS masses has profound implications for NS internal structure and for stellar and binary evolution physics.
DOI: 10.25919/aav7-h513
title: Parkes observations for project P574 semester 2022APRS_03

description: We request time to observe 260 pulsars on a regular basis in order to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to characterise their high energy (phase-resolved) spectra. In the radio, the observations will also allow us to investigate: neutron stars and pulsar emission via detecting glitches and determining pulse timing parameters; and the ISM via measuring and monitoring dispersion measures, Faraday rotation measures, and scintillation. To date, we are (co-)authors on over 95 papers arising from the collaboration and P574 data, including four which use UWL observations. The data have contributed to the PhD theses of students from Bordeaux, Manchester, Oxford, Stanford, and Swinburne.
DOI: 10.5519/qd.4t7mvhux
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (375 records)
DOI: 10.5281/zenodo.6554852
title: Dataset for "On Closure Phase and Systematic Bias in Multilooked SAR Interferometry"

description: Datasets of the Barstow-Bristol Trough area -- unwrapped interferograms of con-1 through con-10, and con-20 and their associated correlation, connected components. Jupyter notebook of tutorial exercising the python code (https://github.com/insarlab/MintPy/blob/main/mintpy/closure_phase_bias.py) in Mintpy
description: {"references": ["Y. Zheng, H. Fattahi, P. Agram, M. Simons and P. Rosen, \"On Closure Phase and Systematic Bias in Multilooked SAR Interferometry,\" in IEEE Transactions on Geoscience and Remote Sensing, vol. 60, pp. 1-11, 2022, Art no. 5226611, doi: 10.1109/TGRS.2022.3167648."]}
DOI: 10.6084/m9.figshare.16649650.v3
title: Network: lter, Domain: hjandrews

description: MacroSheds timeseries data, shapefiles, and metadata for domain: hjandrews, within network: lter
DOI: 10.6084/m9.figshare.16649671.v3
title: Network: lter, Domain: konza

description: MacroSheds timeseries data, shapefiles, and metadata for domain: konza, within network: lter
DOI: 10.6084/m9.figshare.19775650.v1
title: ChAdOx1 nCoV-19 (AZD1222) or ChAdOx1 nCoV-19-Beta (AZD2816) protect Syrian hamsters against the Beta, Delta, and Omicron variants of concern

description: Raw data accompanying ' <strong>ChAdOx1 nCoV-19 (AZD1222) or ChAdOx1 nCoV-19-Beta (AZD2816) protect Syrian hamsters against the Beta, Delta, and Omicron variants of concern'</strong>
DOI: 10.25919/nn6h-4427
title: Parkes observations for project P960 semester 2022APRS_01

description: We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and 13MM packages. In addition to cross-referencing C007 for flux calibration via pointing, we aim to conduct gain-elevation and system temperature experiments using the Moon, to ensure users of the Parkes Observatory have the most accurate information available for calibration purposes. We also wish to fully characterise the spectro-polarimetry response of the UWL and cryoPAF, by determining the Mueller Matrix for the receivers.
DOI: 10.25919/pcwv-ce32
title: Parkes observations for project P595 semester 2022APRS_02

description: We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the space missions, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.
DOI: 10.6084/m9.figshare.16649677.v3
title: Network: lter, Domain: luquillo

description: MacroSheds timeseries data, shapefiles, and metadata for domain: luquillo, within network: lter
DOI: 10.25919/djhp-wh93
title: Parkes observations for project P885 semester 2022APRS_04

description: We request a continued reduced monitoring cadence for the magnetars 1E 1547.0-5408 and Swift J1818.0-1607 at once every 10 days, to track their rotation, flux density, and polarisation. Swift J1818.0-1607 remains very dynamic, and the unique UWL capabilities promise new opportunities to probe still mysterious radio emission mechanisms in magnetars. Our timing results indicate that 1E 1547.0-5408 is currently a more stable rotator, supporting the diminished cadence. We will observe XTE J1810-197 and PSR J1622-4950 less frequently, to complement monitoring elsewhere. The overall request is 18 hours.
DOI: 10.6084/m9.figshare.19775749
title: Triangle of U Flowering Locus C (FLC) Phylogenetic Tree

description: Alignment file and Newick tree for <em>Flowering Locus C </em>(<em>FLC</em>) orthologs among the Triangle of U species. <br> To investigate orthologs among the Triangle of U species, phylogenetic trees were constructed for three agriculturally important genes: <em>Flowering Locus C</em> (<em>FLC</em>), <em>Fatty Acyl Elongase 1</em> (<em>FAE1</em>) and <em>Fatty Acyl-CoA Reductase 1</em> (<em>FAR1</em>). We aligned the coding sequences and peptide sequences using the MUSCLE alignment software (Edgar, 2004). Next, each alignment was adjusted using PAL2NAL (Suyama et al., 2006) according to the protein sequence alignments. We used a single matrix comprised of the aligned sequences to determine the best-fit nucleotide substitution model under a Bayesian information criterion (BIC) in IQ-TREE (Nguyen et al., 2015). Lastly, the phylogenetic trees were reconstructed using RAxML under the GTR + CAT model with 1,000 bootstrap replicates.
DOI: 10.6084/m9.figshare.19775749.v1
title: Triangle of U Flowering Locus C (FLC) Phylogenetic Tree

description: Alignment file and Newick tree for <em>Flowering Locus C </em>(<em>FLC</em>) orthologs among the Triangle of U species. <br> To investigate orthologs among the Triangle of U species, phylogenetic trees were constructed for three agriculturally important genes: <em>Flowering Locus C</em> (<em>FLC</em>), <em>Fatty Acyl Elongase 1</em> (<em>FAE1</em>) and <em>Fatty Acyl-CoA Reductase 1</em> (<em>FAR1</em>). We aligned the coding sequences and peptide sequences using the MUSCLE alignment software (Edgar, 2004). Next, each alignment was adjusted using PAL2NAL (Suyama et al., 2006) according to the protein sequence alignments. We used a single matrix comprised of the aligned sequences to determine the best-fit nucleotide substitution model under a Bayesian information criterion (BIC) in IQ-TREE (Nguyen et al., 2015). Lastly, the phylogenetic trees were reconstructed using RAxML under the GTR + CAT model with 1,000 bootstrap replicates.
DOI: 10.6084/m9.figshare.19775764.v1
title: Triangle of U Fatty Acid Elongase (FAE1) Phylogenetic Tree

description: Alignment file and Newick tree for <em>Fatty Acid Elongase </em>(<em>FAE1</em>) orthologs among the Triangle of U species. <br> To investigate orthologs among the Triangle of U species, phylogenetic trees were constructed for three agriculturally important genes: <em>Flowering Locus C</em> (<em>FLC</em>), <em>Fatty Acyl Elongase 1</em> (<em>FAE1</em>) and <em>Fatty Acyl-CoA Reductase 1</em> (<em>FAR1</em>). We aligned the coding sequences and peptide sequences using the MUSCLE alignment software (Edgar, 2004). Next, each alignment was adjusted using PAL2NAL (Suyama et al., 2006) according to the protein sequence alignments. We used a single matrix comprised of the aligned sequences to determine the best-fit nucleotide substitution model under a Bayesian information criterion (BIC) in IQ-TREE (Nguyen et al., 2015). Lastly, the phylogenetic trees were reconstructed using RAxML under the GTR + CAT model with 1,000 bootstrap replicates.
DOI: 10.6084/m9.figshare.19775797
title: Triangle of U Fatty Acyl-CoA Reductase 1 (FAR1) Phylogenetic Tree

description: Alignment file and Newick tree for <em>Fatty Acyl-CoA Reductase </em>(<em>FAR1</em>) orthologs among the Triangle of U species. <br> To investigate orthologs among the Triangle of U species, phylogenetic trees were constructed for three agriculturally important genes: <em>Flowering Locus C</em> (<em>FLC</em>), <em>Fatty Acyl Elongase 1</em> (<em>FAE1</em>) and <em>Fatty Acyl-CoA Reductase 1</em> (<em>FAR1</em>). We aligned the coding sequences and peptide sequences using the MUSCLE alignment software (Edgar, 2004). Next, each alignment was adjusted using PAL2NAL (Suyama et al., 2006) according to the protein sequence alignments. We used a single matrix comprised of the aligned sequences to determine the best-fit nucleotide substitution model under a Bayesian information criterion (BIC) in IQ-TREE (Nguyen et al., 2015). Lastly, the phylogenetic trees were reconstructed using RAxML under the GTR + CAT model with 1,000 bootstrap replicates.
DOI: 10.6084/m9.figshare.19775764
title: Triangle of U Fatty Acid Elongase (FAE1) Phylogenetic Tree

description: Alignment file and Newick tree for <em>Fatty Acid Elongase </em>(<em>FAE1</em>) orthologs among the Triangle of U species. <br> To investigate orthologs among the Triangle of U species, phylogenetic trees were constructed for three agriculturally important genes: <em>Flowering Locus C</em> (<em>FLC</em>), <em>Fatty Acyl Elongase 1</em> (<em>FAE1</em>) and <em>Fatty Acyl-CoA Reductase 1</em> (<em>FAR1</em>). We aligned the coding sequences and peptide sequences using the MUSCLE alignment software (Edgar, 2004). Next, each alignment was adjusted using PAL2NAL (Suyama et al., 2006) according to the protein sequence alignments. We used a single matrix comprised of the aligned sequences to determine the best-fit nucleotide substitution model under a Bayesian information criterion (BIC) in IQ-TREE (Nguyen et al., 2015). Lastly, the phylogenetic trees were reconstructed using RAxML under the GTR + CAT model with 1,000 bootstrap replicates.
DOI: 10.6084/m9.figshare.19775797.v1
title: Triangle of U Fatty Acyl-CoA Reductase 1 (FAR1) Phylogenetic Tree

description: Alignment file and Newick tree for <em>Fatty Acyl-CoA Reductase </em>(<em>FAR1</em>) orthologs among the Triangle of U species. <br> To investigate orthologs among the Triangle of U species, phylogenetic trees were constructed for three agriculturally important genes: <em>Flowering Locus C</em> (<em>FLC</em>), <em>Fatty Acyl Elongase 1</em> (<em>FAE1</em>) and <em>Fatty Acyl-CoA Reductase 1</em> (<em>FAR1</em>). We aligned the coding sequences and peptide sequences using the MUSCLE alignment software (Edgar, 2004). Next, each alignment was adjusted using PAL2NAL (Suyama et al., 2006) according to the protein sequence alignments. We used a single matrix comprised of the aligned sequences to determine the best-fit nucleotide substitution model under a Bayesian information criterion (BIC) in IQ-TREE (Nguyen et al., 2015). Lastly, the phylogenetic trees were reconstructed using RAxML under the GTR + CAT model with 1,000 bootstrap replicates.
DOI: 10.5517/ccdc.csd.cc29zn54
title: CCDC 2144616: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc29zn65
title: CCDC 2144617: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc29zn76
title: CCDC 2144618: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc29zn87
title: CCDC 2144619: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc29zn98
title: CCDC 2144620: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc29znb9
title: CCDC 2144621: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc29zncb
title: CCDC 2144622: Experimental Crystal Structure Determination

description: Related Article: Molly M. Haskins, Matteo Lusi, Michael J. Zaworotko|2022|Cryst.Growth Des.|22|3333|doi:10.1021/acs.cgd.2c00150
DOI: 10.5517/ccdc.csd.cc2bnwvr
title: CCDC 2165035: Experimental Crystal Structure Determination

description: Related Article: Alberto Cedillo-Cruz, Diego Martínez-Otero, Joaquín Barroso-Flores and Erick Cuevas-Yañez|2022|J.Mol.Struct.|1264|133225|doi:10.1016/j.molstruc.2022.133225
DOI: 10.5517/ccdc.csd.cc2bnwws
title: CCDC 2165036: Experimental Crystal Structure Determination

description: Related Article: Alberto Cedillo-Cruz, Diego Martínez-Otero, Joaquín Barroso-Flores and Erick Cuevas-Yañez|2022|J.Mol.Struct.|1264|133225|doi:10.1016/j.molstruc.2022.133225
DOI: 10.5517/ccdc.csd.cc2brkd2
title: CCDC 2167594: Experimental Crystal Structure Determination

description: Related Article: P. Chooto, S. Saithong, W. Aemaeg, S. Vataporn, C. Pakawatchai, C. Innuphat, S. Duangthong, W. Puetpaiboon|2022|Acta Crystallogr.,Sect.E:Cryst.Commun.|78|519|doi:10.1107/S2056989022004224
DOI: 10.6084/m9.figshare.16649698.v3
title: Network: lter, Domain: niwot

description: MacroSheds timeseries data, shapefiles, and metadata for domain: niwot, within network: lter
DOI: 10.6084/m9.figshare.16649701.v3
title: Network: lter, Domain: plum

description: MacroSheds timeseries data, shapefiles, and metadata for domain: plum, within network: lter
DOI: 10.6084/m9.figshare.16649704.v3
title: Network: lter, Domain: santa_barbara

description: MacroSheds timeseries data, shapefiles, and metadata for domain: santa_barbara, within network: lter
DOI: 10.6084/m9.figshare.19775818
title: Dive analysis - post-guard 2018

description: Calculated trip statistics derived from GPS deployments during the hoiho post-guard period 2018.
DOI: 10.6084/m9.figshare.16649710.v3
title: Network: usfs, Domain: fernow

description: MacroSheds timeseries data, shapefiles, and metadata for domain: fernow, within network: usfs
DOI: 10.25919/mwgy-0762
title: Parkes observations for project P456 semester 2022APRS_03

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. We are now in an exciting regime where a signal detected in our (and other data sets) has the form expected for a gravitational wave background. We are therefore now attempting to confirm, or deny, this exciting result. With this proposal we aim to maintain our pre-eminent position in the field. Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.6084/m9.figshare.19775824
title: Foraging analysis - pre-moult 2019

description: Calculated trip statistics derived from GPS deployments during the hoiho pre-moult period 2019.
DOI: 10.6084/m9.figshare.19775824.v1
title: Foraging analysis - pre-moult 2019

description: Calculated trip statistics derived from GPS deployments during the hoiho pre-moult period 2019.
DOI: 10.48567/yxkp-nc16
title: AGO-4 Automatic Weather Station, 2015 quality-controlled observational data.