cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5c2af4f3c6129
title: Parkes observations for project P456 semester 2018APRS_16

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.25919/5c2b040a103a2
title: Parkes observations for project P737 semester 2018APRS_20

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.  We will also use P737 to commission new receivers such as the UWB.
DOI: 10.25919/5c2b0ae44bd5c
title: Parkes observations for project P737 semester 2018APRS_21

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.  We will also use P737 to commission new receivers such as the UWB.
DOI: 10.25919/5c2b0ca39007d
title: Parkes observations for project P456 semester 2018APRS_17

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.5281/zenodo.2529598
title: MoMA Collection - Automatic Monthly Update

description: Temporary Description
DOI: 10.5281/zenodo.2529599
title: MoMA Collection - Automatic Monthly Update

description: Temporary Description
DOI: 10.5517/ccdc.csd.cc21cs3b
title: CCDC 1888151: Experimental Crystal Structure Determination

description: Related Article: Brian W. Skelton, Michael I. Bruce, Benjamin G. Ellis|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: 10.7910/dvn/hn7ncb/5iijte
title: africancabinets_africa.log
DOI: 10.7910/dvn/koo6mp/mc6rra
title: 2015_wave1.tab

description: Dataset used in the analysis
DOI: 10.5281/zenodo.2449795
title: Underwater Images

description: Underwater image database
DOI: 10.5281/zenodo.2449796
title: Underwater Images

description: Underwater image database
DOI: 10.5281/zenodo.2529726
title: 'Retrodiction' experiment Western Kho-Bwa languages: data

description: These files contain all the data belonging to the retro-diction/pre-diction experiment in a historical-comparative linguistic study on the Western Kho-Bwa languages. This data set has all the raw as well as cut sound files of all the concepts elicited in the field work sessions in Arunachal Pradesh.

The research was registered online as:

Bodt, Timotheus A., Nathan W. Hill and Johann-Mattis List. 2018. <em>Prediction experiment for missing words in Kho-Bwa language data.</em> Open Science Framework Preregistrations October 5.  https://osf.io/evcbp/
description: Swiss National Science Foundation Postdoc Mobility grant number P2BEP1_181779
DOI: 10.5281/zenodo.2529727
title: 'Retrodiction' experiment Western Kho-Bwa languages: data

description: These files contain all the data belonging to the retro-diction/pre-diction experiment in a historical-comparative linguistic study on the Western Kho-Bwa languages. This data set has all the raw as well as cut sound files of all the concepts elicited in the field work sessions in Arunachal Pradesh.

The research was registered online as:

Bodt, Timotheus A., Nathan W. Hill and Johann-Mattis List. 2018. <em>Prediction experiment for missing words in Kho-Bwa language data.</em> Open Science Framework Preregistrations October 5.  https://osf.io/evcbp/
description: Swiss National Science Foundation Postdoc Mobility grant number P2BEP1_181779
DOI: 10.7910/dvn/075w8o/yrpxdk
title: 2017JSJ_TiltedScales_ReplicationData-1.tab
DOI: 10.7910/dvn/gm5syq/mjpzz1
title: output4.zip
DOI: 10.7910/dvn/hn7ncb/dlm1ic
title: figure5.log
DOI: 10.7910/dvn/koo6mp/djez7p
title: 2015_wave2.tab

description: Dataset used in the analysis
DOI: 10.26300/w07g-xm58
title: Aryballos 1 (Spherical) JI1718
DOI: 10.5281/zenodo.2529865
title: Dataset (Table 1)

description: Experimental and theoretical data that has been used throughout the paper.
DOI: 10.5281/zenodo.2529866
title: Dataset (Table 1)

description: Experimental and theoretical data that has been used throughout the paper.
DOI: 10.5281/zenodo.2529926
title: Heatmap2 (training data)

description: Files for a Galaxy heatmap2 tutorial.
DOI: 10.5517/ccdc.csd.cc1zs755
title: CCDC 1840537: Experimental Crystal Structure Determination

description: Related Article: Alireza Akbari, Hoda Ghateazadeh, Reza Takjoo, Batool Sadeghi-Nejad, Mehrab Mehrvar, Joel T. Mague|2019|J.Mol.Struct.|1181|287|doi:10.1016/j.molstruc.2018.12.109
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.cc1zs788
title: CCDC 1840540: Experimental Crystal Structure Determination

description: Related Article: Alireza Akbari, Hoda Ghateazadeh, Reza Takjoo, Batool Sadeghi-Nejad, Mehrab Mehrvar, Joel T. Mague|2019|J.Mol.Struct.|1181|287|doi:10.1016/j.molstruc.2018.12.109
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.cc1zs799
title: CCDC 1840541: Experimental Crystal Structure Determination

description: Related Article: Alireza Akbari, Hoda Ghateazadeh, Reza Takjoo, Batool Sadeghi-Nejad, Mehrab Mehrvar, Joel T. Mague|2019|J.Mol.Struct.|1181|287|doi:10.1016/j.molstruc.2018.12.109
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.cc1zs7bb
title: CCDC 1840542: Experimental Crystal Structure Determination

description: Related Article: Alireza Akbari, Hoda Ghateazadeh, Reza Takjoo, Batool Sadeghi-Nejad, Mehrab Mehrvar, Joel T. Mague|2019|J.Mol.Struct.|1181|287|doi:10.1016/j.molstruc.2018.12.109
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.cc206pvs
title: CCDC 1853485: Experimental Crystal Structure Determination

description: Related Article: Armağan Günsel, Ahmet T. Bilgiçli, Burak Tüzün, Hasan Pişkin, Göknur Yaşa Atmaca, Ali Erdoğmuş, M. Nilüfer Yarasir|2019|J.Photochem.Photobiol.A:Chem.|373|77|doi:10.1016/j.jphotochem.2018.12.038
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.cc213z7d
title: CCDC 1880653: Experimental Crystal Structure Determination

description: Related Article: Mani Ramanathan, Ming-Tsung Hsu, Shiuh-Tzung Liu|2019|Tetrahedron|75|791|doi:10.1016/j.tet.2018.12.065
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.cc21cv4f
title: CCDC 1888214: Experimental Crystal Structure Determination

description: Related Article: Manik Lal Saha, Jan W. Bats, Michael Schmittel|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: 10.25919/5c2c093ad1449
title: Parkes observations for project P456 semester 2018APRS_18

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.25919/5c2c093ad4ed2
title: Parkes observations for project P456 semester 2018APRS_19

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.25919/5c2c095745d8e
title: Parkes observations for project P737 semester 2018APRS_22

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.  We will also use P737 to commission new receivers such as the UWB.
DOI: 10.25919/5c2c095a5b2f2
title: Parkes observations for project P737 semester 2018APRS_23

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.  We will also use P737 to commission new receivers such as the UWB.
DOI: 10.25919/5c2c09680e128
title: Parkes observations for project P737 semester 2018APRS_24

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.  We will also use P737 to commission new receivers such as the UWB.
DOI: 10.25919/5c2c096e390dd
title: Parkes observations for project P456 semester 2018APRS_20

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.25919/5c2c097b5d32a
title: Parkes observations for project P456 semester 2018APRS_21

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.25919/5c2c098951157
title: Parkes observations for project P456 semester 2018APRS_22

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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: 10.25919/5c2c098dd71e7
title: Parkes observations for project P456 semester 2018APRS_23

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. 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!