cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.2544247
title: Encuesta de Ocupación en Alojamientos Turísticos. Establecimientos hoteleros

description: .
DOI: 10.5281/zenodo.2544248
title: Encuesta de Ocupación en Alojamientos Turísticos. Establecimientos hoteleros

description: .
DOI: 10.5281/zenodo.2544249
title: Encuesta de Ocupación en Alojamientos Turísticos. Apartamentos turísticos

description: .
DOI: 10.5281/zenodo.2544250
title: Encuesta de Ocupación en Alojamientos Turísticos. Apartamentos turísticos

description: .
DOI: 10.5281/zenodo.2544251
title: Encuesta de Ocupación en Alojamientos Turísticos. Campings

description: .
DOI: 10.5281/zenodo.2544252
title: Encuesta de Ocupación en Alojamientos Turísticos. Campings

description: .
DOI: 10.14469/hpc/4970
title: Epoxidation, cyanoethene

description: Molden files
DOI: 10.25919/5c435a0db83d6
title: Parkes observations for project PX500 semester 2018OCTS_06

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first, relating to this proposal, will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.5281/zenodo.2544253
title: Encuesta de Ocupación en Alojamientos Turísticos. Alojamientos de turismo rural

description: .
DOI: 10.5281/zenodo.2544254
title: Encuesta de Ocupación en Alojamientos Turísticos. Alojamientos de turismo rural

description: .
DOI: 10.14469/hpc/4971
title: Epoxidation, cis-dicyanoethene

description: Molden files
DOI: 10.14469/hpc/4972
title: Epoxidation, trans dicyanoethene

description: Molden files
DOI: 10.25919/5c435c2dd5053
title: Parkes observations for project PX500 semester 2018OCTS_08

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first, relating to this proposal, will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c435ccab9aeb
title: Parkes observations for project PX500 semester 2018OCTS_09

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first, relating to this proposal, will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c435d0ae74c6
title: Parkes observations for project PX500 semester 2018OCTS_10

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX501) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first, relating to this proposal, will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c435e2a4c695
title: Parkes observations for project P789 semester 2018OCTS_01

description: Recently there has been great success at Parkes discovering millisecond pulsars (MSPs), a class that includes some of the most interesting and scientifically valuable pulsars known. In the last few years, we have discovered more than 40 MSPs though the High Time Resolution Universe Survey (P630) and Fermi searches (P675/P814). Here we propose to carry out precision timing of these sources to fully exploit these discoveries. Additionally, we continue to study the most significant of the discoveries from the Parkes Multibeam Pulsar Survey (P268). 
To maximise scientific impact, we have combined the most important sources from various previous proposals into this project, reducing total observation time required and easing the burden on the scheduler.
DOI: 10.25919/5c435f8b098cb
title: Parkes observations for project P789 semester 2018OCTS_02

description: Recently there has been great success at Parkes discovering millisecond pulsars (MSPs), a class that includes some of the most interesting and scientifically valuable pulsars known. In the last few years, we have discovered more than 40 MSPs though the High Time Resolution Universe Survey (P630) and Fermi searches (P675/P814). Here we propose to carry out precision timing of these sources to fully exploit these discoveries. Additionally, we continue to study the most significant of the discoveries from the Parkes Multibeam Pulsar Survey (P268). 
To maximise scientific impact, we have combined the most important sources from various previous proposals into this project, reducing total observation time required and easing the burden on the scheduler.
DOI: 10.25919/5c435ff31f2b3
title: Parkes observations for project P971 semester 2018OCTS_03

description: We propose timing observations of the relativistic pulsar - white-dwarf binary PSR J1141-6545. This unique system offers access to a wide range of physics, from relativistic phenomena through pulsar emission cone studies, to the structure and distribution of interstellar plasma along our line-of-sight. The recently installed Parkes Ultra Wide Band Low Frequency (UWL) receiver has opened up the possibility of performing first-ever studies of its orbital dynamics at high temporal resolution and study of the effects of the intra-binary medium on the dispersion and polarisation of the pulse profile. Our analysis of data obtained to date suggests that the pulsar would precess away from our line-of-sight in the next 3-5 years. Hence, regular observations are crucial to maximizing its science outcome
DOI: 10.25919/5c43621acc692
title: Parkes observations for project P986 semester 2018OCTS_01

description: Pulsar survey is one of the top priorities of the Square Kilometer Arrays (SKA). The discovery of pulsars in relativistic binaries, pulsars in binary with black holes and pulsars in the Galactic Center (GC) will improve our understanding of gravity theories, physics of black holes and stellar population and environment in the GC region. However, conventional periodic searches for pulsars are only sensitive to strictly periodic signals with low duty cycles. Although various methods have been developed to search for pulsars in these extreme systems, it is still very challenging and computationally expensive. 

One of the solutions is to find pulsar candidates in radio continuum surveys and then carry out targeted searches (e.g. Frail et al 2017). This technique allows a search over the full field of view while avoiding the need for expensive pixel-by-pixel high time resolution searches. We propose to observe 32 compact, steep spectrum candidates selected from NVSS and TGSS surveys using the Ultra-Wideband Low (UWL) receiver. The frequency coverage (as low as 700MHz) and low system temperature (~20K) of UWL will enable us to carry out a sensitive search of steep spectrum sources.
DOI: 10.25919/5c43623a0b6ed
title: Parkes observations for project PX501 semester 2018OCTS_06

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX500) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first (PX500) will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time (relating to this proposal) will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c4362b02255b
title: Parkes observations for project PX501 semester 2018OCTS_07

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX500) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first (PX500) will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time (relating to this proposal) will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c4364ed1e575
title: Parkes observations for project PX501 semester 2018OCTS_08

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX500) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first (PX500) will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time (relating to this proposal) will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c43654fa1fa9
title: Parkes observations for project PX501 semester 2018OCTS_09

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX500) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first (PX500) will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time (relating to this proposal) will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c4365991b6a5
title: Parkes observations for project PX501 semester 2018OCTS_10

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX500) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first (PX500) will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time (relating to this proposal) will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.25919/5c4365ee8e898
title: Parkes observations for project P970 semester 2018APRS_07

description: During the past 6 years, we at Parkes and collaborators at other radio telescopes have been remarkably successful at discovering millisecond pulsars (MSPs) associated with unidentified Fermi-LAT gamma-ray sources. Based on lessons learned, we here propose to carry out targeted searches with the new Ultra-wideband Low (UWL) receiver that will be installed next semester. The ultra-wide frequency coverage will enable us to detect MSPs with steep spectrum and avoid difficulties caused by interstellar scintillation and dispersive and scattering smearing. We propose to revisit highly ranked pulsar candidates that remain unidentified. Such a pilot survey will help us designing future searches of the coming 4FGL gamma-ray source catalog using the UWL. The overall time request is 23 hours on source, or 26 hours including overheads.
DOI: 10.25919/5c436633c6744
title: Parkes observations for project P996 semester 2018OCTS_03

description: We propose to measure the polarisation of ~200 pulsars (~100 this semester) using the Ultra-Wideband Low (UWL) receiver to investigate the structure of the Galactic disk magnetic field in and between distant spiral arms. Previous Parkes pulsar observations have revealed field reversals in nearby arm and interarm regions. We wish to exploit the greater sensitivity of the UWL receiver to extend this to more distant regions, thereby allowing us to distinguish more clearly between different models for the structure of the disk field. This work will have important implications for theories for the generation of Galactic magnetic fields and for other areas, e.g., cosmic-ray physics, which depend on a knowledge of the large-scale Galactic magnetic field for their interpretation.
DOI: 10.25919/5c436674d3919
title: Parkes observations for project P996 semester 2018OCTS_04

description: We propose to measure the polarisation of ~200 pulsars (~100 this semester) using the Ultra-Wideband Low (UWL) receiver to investigate the structure of the Galactic disk magnetic field in and between distant spiral arms. Previous Parkes pulsar observations have revealed field reversals in nearby arm and interarm regions. We wish to exploit the greater sensitivity of the UWL receiver to extend this to more distant regions, thereby allowing us to distinguish more clearly between different models for the structure of the disk field. This work will have important implications for theories for the generation of Galactic magnetic fields and for other areas, e.g., cosmic-ray physics, which depend on a knowledge of the large-scale Galactic magnetic field for their interpretation.
DOI: 10.25919/5c43671fddd16
title: Parkes pulsar observations with undefined project IDs for 2018_14

description: Parkes pulsar observations with undefined project IDs for 2018
DOI: 10.5517/ccdc.csd.cc21hry8
title: CCDC 1891990: Experimental Crystal Structure Determination

description: Related Article: Joel Mague, Mohamed El Hafi|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: 10.5281/zenodo.1424648
title: Données de fouille du site de Kition-Pervolia

description: <strong>Présentation du site de Kition-<em>Pervolia</em></strong>

 

            Localisé au nord-ouest de la ville ancienne de Kition (aujourd’hui Larnaca, Chypre), dans une zone périurbaine, le site de <em>Pervolia</em> est une nécropole de l’âge du Fer, caractérisée par des tombes à chambre creusées dans le substrat rocheux. Les découvertes, renseignées dans les archives du Département des Antiquités depuis 1918, montrent que la nécropole a été utilisée entre le début de l’époque géométrique (X<sup>e</sup> s.) et la fin de l’époque classique (fin du IV<sup>e</sup> s. av. J.-C.), période des royaumes de Chypre.

            De gros travaux de terrassement, en 1958, ont entraîné une destruction partielle du site (et la fouille de sauvetage de plusieurs caveaux). La parcelle a été classée zone archéologique en 1960. La mission française de Kition y a conduit trois campagnes de fouilles programmées (2012-2014).
DOI: 10.5281/zenodo.1424649
title: Données de fouille du site de Kition-Pervolia

description: <strong>Présentation du site de Kition-<em>Pervolia</em></strong>

 

            Localisé au nord-ouest de la ville ancienne de Kition (aujourd’hui Larnaca, Chypre), dans une zone périurbaine, le site de <em>Pervolia</em> est une nécropole de l’âge du Fer, caractérisée par des tombes à chambre creusées dans le substrat rocheux. Les découvertes, renseignées dans les archives du Département des Antiquités depuis 1918, montrent que la nécropole a été utilisée entre le début de l’époque géométrique (X<sup>e</sup> s.) et la fin de l’époque classique (fin du IV<sup>e</sup> s. av. J.-C.), période des royaumes de Chypre.

            De gros travaux de terrassement, en 1958, ont entraîné une destruction partielle du site (et la fouille de sauvetage de plusieurs caveaux). La parcelle a été classée zone archéologique en 1960. La mission française de Kition y a conduit trois campagnes de fouilles programmées (2012-2014).
DOI: 10.25919/5c437bdb97c6d
title: Parkes observations for project P456 semester 2018OCTS_08

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: 10.25919/5c437cb0c40f5
title: Parkes observations for project P456 semester 2018OCTS_07

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.2544520
title: Bibliometric dataset: list of highly cited papers in bibliometric

description: <strong>Motivation</strong>

My motivation in providing this dataset is to invite more interests from Indonesia's librarian to understand their diverse field of study.  

<strong>Method</strong>

This dataset is harvested in 19 January 2019 from Scopus database provided by The University of Sydney. I used the keyword "bibliometric" in title, sort the search results by total citation, then download the first 2000 papers as RIS file. This file can be converted to other formats like bibtex or csv using available reference manager, like Zotero.

<strong>Visualisations</strong>

I did two small visualisations using the following options:


	"create a map based on bibliographic data"
	"create a map based on text data"


Both mappings are done using VosViewer open source app from CWTS Leiden University.
DOI: 10.5281/zenodo.2544521
title: Bibliometric dataset: list of highly cited papers in bibliometric

description: <strong>Motivation</strong>

My motivation in providing this dataset is to invite more interests from Indonesia's librarian to understand their diverse field of study.  

<strong>Method</strong>

This dataset is harvested in 19 January 2019 from Scopus database provided by The University of Sydney. I used the keyword "bibliometric" in title, sort the search results by total citation, then download the first 2000 papers as RIS file. This file can be converted to other formats like bibtex or csv using available reference manager, like Zotero.
DOI: 10.21227/k84s-t916
title: OOK Data

description: This is the python code for our article
DOI: 10.21227/zt6t-ea83
title: OOK Data

description: This is the python code for our article
DOI: 10.26300/hys7-c858
title: Mindfulness Based Blood Pressure Reduction Study Derived Variables and Codebook