cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.4225/08/58dd10a566b78
title: Parkes observations for project P858 semester 2015APRS_BPSR_20

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd10b5e2a62
title: Parkes observations for project P858 semester 2015APRS_BPSR_30

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd14e574e69
title: Parkes observations for project P574 semester 2015APRS_BPSR_01

description: We request time to observe 230 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 find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we
are (co-)authors on 48 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from the Bordeaux group and Stanford and are in remain in active use (detailed within).
DOI: 10.4225/08/58dd15064d706
title: Parkes observations for project P574 semester 2015APRS_BPSR_04

description: We request time to observe 230 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 find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we
are (co-)authors on 48 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from the Bordeaux group and Stanford and are in remain in active use (detailed within).
DOI: 10.14457/mu.the.2000.42
title: ความสัมพันธ์ของการให้วัคซีนป้องกันโรคบาดทะยักในหญิงวัยเจริญพันธุ์ กับการเกิดโรคบาดทะยักในเด็กแรกเกิดในพื้นที่เสี่ยงต่อการเกิดโรค /
DOI: 10.4225/08/58dd14f15d2ac
title: Parkes observations for project P574 semester 2015APRS_BPSR_02

description: We request time to observe 230 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 find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we
are (co-)authors on 48 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from the Bordeaux group and Stanford and are in remain in active use (detailed within).
DOI: 10.4225/08/58dd1532bf4c5
title: Parkes observations for project P858 semester 2015APRS05

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.14457/kmutnb.the.1994.1
title: สมรรถนะของช่างเทคนิคเครื่องกลอุตสาหกรรมตามความต้องการของผู้ประกอบการอุตสาหกรรม /
DOI: 10.14457/kmutnb.the.1994.2
title: รูปแบบความร่วมมือระหว่างสถานศึกษากับสถานประกอบการในการจัดส่งนักศึกษาระดับประกาศนียบัตรวิชาชีพ (ปวช.) สาขาเทคนิคแว่นตาและเลนส์ ออกฝึกงาน /
DOI: 10.4225/08/58dd0fc641958
title: Parkes observations for project P858 semester 2015APRS_BPSR_22

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd0fd47d86b
title: Parkes observations for project P858 semester 2015APRS06

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd10e2553a2
title: Parkes observations for project P858 semester 2015APRS_BPSR_51

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd14fbd43b0
title: Parkes observations for project P574 semester 2015APRS_BPSR_03

description: We request time to observe 230 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 find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we
are (co-)authors on 48 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from the Bordeaux group and Stanford and are in remain in active use (detailed within).
DOI: 10.4231/d33t9d758
title: NNCI Modeling/Simulation Tools List

description: NNCI Modeling/Simulation Tools List provides a collective inventory of modeling and simulation resources and capabilities across NNCI sites and includes helpful information such as a point of contact for each tool, any access restrictions, and academic citations.
DOI: 10.5061/dryad.g9k46/3
title: Supplementary Tables S1-S12

description: Pearson correlation coefficient between original, discretized and reconstructed richness and rates time series : Supplementary Tables S1-S12
DOI: 10.4225/08/58dd0ff28c456
title: Parkes observations for project P858 semester 2015APRS08

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd10003701c
title: Parkes observations for project P858 semester 2015APRS09

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd11439f056
title: Parkes observations for project P858 semester 2015APRS_BPSR_23

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.4225/08/58dd153ebe386
title: Parkes observations for project P456 semester 2015APRS_BPSR_01

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 gravitational waves until they are finally detected. Continued Parkes observations will remain valuable until the first stage of the SKA is able to offer the same sensitivity as Parkes and the same observing time. 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: 10.4225/08/58dd1554200f8
title: Parkes observations for project P858 semester 2015APRS_BPSR_24

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.5281/zenodo.439581
title: Pitsc

description: This is a text mining data set generated from project and issue tracking system (PITS) reports.
DOI: 10.5281/zenodo.439585
title: Identifier Splitters

description: The oracle, found in the file loyola-udelaware-identifier-splitting-oracle (ludiso) consists of 2663 identifiers. These identifiers were split by volunteers using a web interface. In all 8522 splitting judgements were collected for 2731 identifiers. The data set was curated based on the sum of confidence associated with a particular split. In order to provide a single correct split in the oracle, the split receiving the highest confidence sum was used as the correct split. Of the 2731 identifers, 68 do not appear in the oracle because of ties. (These identifiers can be found in the raw data.) Details on the construction of the oracle can be found in "An empirical study of identifier splitting technique".

<strong>Attribute Information</strong>

Each line of the oracle represents one of the 2663 remaining oracle identifiers and includes the following.

the identifier's unique identification number,<br>
the original identifier as extracted from the source,<br>
the dominant language of the program that the id was extracted from,<br>
the program from which it was extracted,<br>
the identifier as shown to subjects where a '-' denotes a hard split,<br>
the number of splittings (always 1 in the oracle, but not in the raw data),<br>
the identifier as split by users,<br>
the number of confidences (1 - 5) and then each confidence.<br>
DOI: 10.14457/kmutnb.the.1993.1
title: การศึกษาเปรียบเทียบสภาพการปฏิบัติงานของพนักงานระหว่างกะปกติและกะพิเศษในโรงงานอุตสาหกรรมโลหะการ ตามทัศนะของหัวหน้างานและช่างเทคนิค /
DOI: 10.4225/08/58dd101e375cd
title: Parkes observations for project P858 semester 2015APRS11

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.5281/zenodo.439483
title: Dataset For A Mouse And Rat Liver Trancriptomic Analysis

description: Data used for the anlaysis. R scripts used can be found on github: https://github.com/gdevailly/liver_mouse_rat


	matrixLiverMouse.txt and rat_full_data_matrix.txt contain GEO expression matrix for mouse and rat rexperiments.
	GSEmouse.txt and GSErat.txt contain experiment IDs from GEO and experiment titles.
	GEORat.txt and GEOMouse.txt contain experiment IDs and series IDs from GEO.
	quantNormData_mouse.tsv and quantNormData_rat.tsv contain normalised expression matrices.
	fileForSCHypeThreshold0.5.txt is the input for SCHype. schype_output_0.5th.nodes.txt and schype_output_0.5th.edges.txt are the outputs.
	mouse_rat_ampping.txt is the probe mapping used to compare mouse and rat data.
	geneLists.zip contains gene lists used for ontology analysis (ENSEMBL gene id)
description: Do contact me if you encounter any issues with the files.
DOI: 10.5517/ccdc.csd.cc1nr82r
title: CCDC 1541694: Experimental Crystal Structure Determination

description: Related Article: Brian W. Skelton|2017|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: 10.14457/kmutnb.the.1995.1
title: การตรวจหาปฏิบัติการชั้นเลิศและการสร้างคู่มือประเมินเพื่อพัฒนาตนเองทางการบริหารอาชีวะและเทคนิคศึกษา /
DOI: 10.14457/mju.the.2006.52
title: ศักยภาพของบ้านปากหลาที่สามารถพัฒนาเป็นแหล่งท่องเที่ยวนิเวศ เมืองหล้า แขวงอุดมไชย สาธารณรัฐประชาธิปไตยประชาชนลาว (ส.ป.ป.ลาว) /