cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.4225/08/58dd102bbca10
title: Parkes observations for project P858 semester 2015APRS12

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: 10.4225/08/58dd1055a8b77
title: Parkes observations for project P858 semester 2015APRS15

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: 10.4225/08/58dd1088dfc44
title: Parkes observations for project P858 semester 2015APRS18

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: 10.4225/08/58dd1097b9c3f
title: Parkes observations for project P858 semester 2015APRS19

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: 10.4225/08/58dd112c62bf9
title: Parkes observations for project P858 semester 2015APRS_BPSR_26

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: 10.4225/08/58dd15110a4e2
title: Parkes observations for project P574 semester 2015APRS_BPSR_05

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: 10.5281/zenodo.439578
title: Datatrieve

description: Number of records: 130

Number of attributes: 9<br>
   * 8 condition attributes<br>
   * 1 decision attribute

Attribute Information:

   1 LOC6_0: number of lines of code of module m in version 6.0.<br>
   1 LOC6_1: number of lines of code of module m in version 6.1.<br>
   1 AddedLOC: number of lines of code that were added to module m in version 6.1, i.e., they were not present in module m in version 6.0.<br>
   1 DeletedLOC: number of lines of code that were deleted from module m in version 6.0, i.e.,   they were no longer present in module m in version 6.1.<br>
   1 Different Blocks: number of different blocks module m in between versions 6.0 and 6.1.<br>
   1 Modification Rate: rate of modification of module m, i.e.,   (AddedLOC + DeletedLOC) / (LOC6.0 + AddedLOC).<br>
   1 Module Knowledge: subjective variable that expresses the project team's knowledge on   module m (low or high)<br>
   1 ReusedLOC: number of lines of code of module m in version 6.0 reused in module m in    version 6.1.<br>
   1 Faulty6_1: its value is 0 for all those modules in which no faults were found;   its value is 1 for all other modules.

Missing attributes: none

Class Distribution:<br>
   * 0:   119 = 91.54%<br>
   * 1:   11  =  8.46%<br>
DOI: 10.5281/zenodo.439582
title: Pitse

description: This is a text mining data set generated from project and issue tracking system (PITS) reports.
DOI: 10.14457/kmutnb.the.1996.2
title: การออกแบบและสร้างเครื่องกลแบบเพนดูลัมด้วยมอเตอร์เหนี่ยวนำ /
DOI: 10.14457/kmutnb.the.1997.1
title: การวิเคราะห์และประเมินศักยภาพของระบบกักเก็บความเย็นในรูปน้ำแข็งที่ประยุกต์ใช้กับการปรับอากาศ ขนาด 5 ตัน กรณีศึกษา : อาคาร ท.110 ของการไฟฟ้าฝ่ายผลิตแห่งประเทศไทย /
DOI: 10.4225/08/58dd10c370469
title: Parkes observations for project P858 semester 2015APRS_BPSR_40

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: 10.4225/08/58dd10d253308
title: Parkes observations for project P858 semester 2015APRS_BPSR_41

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: 10.4225/08/58dd151bdd943
title: Parkes observations for project P858 semester 2015APRS03

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.439580
title: Pitsb

description: This is a text mining data set generated from project and issue tracking system (PITS) reports.
DOI: 10.5281/zenodo.439588
title: Conmodels

description: Thomas Fritz, Christoph Bräunlich, and David Shepherd conducted a study of twelve developers performing one of three change tasks using the Eclipse IDE for Java Developers. Here we publish the data collected during this study.  Our data consists of twelve transcripts of developer actions transcribed by hand from the approximately two hours of video collected from each participant. It also includes the patches they submitted as solutions and a drawing/description of the program elements and relationships necessary to complete their task. Further details on the study setup can be found in our paper.
DOI: 10.5281/zenodo.439591
title: Dmtech

description: Direct Monitoring Dataset is a collection of data obtained during an experimental analysis of different direct monitoring techniques.

The analysis based on a fault-injection campaign on a real-world air traffic control (ATC) middleware system conducted by SAFE tool. The transport layer of the considered middleware implements three direct monitoring techniques, i.e., event logs, assertions, and rule-based loging approach supported by LogBus. We injected 12,733 software faults, which types extend the Orthogonal Defect Classification (ODC) for practical injection purposes, into the middleware transport layer source code. For each injected faults, we collected the data generated by considered techniques at middleware level, but we also collected the event logs produced by the operating system (Red Hat 5 El) and the legacy ATC applications running on the top of the target middleware. In summary, collected data include:

* data generated by middleware:<br>
* logs (MwLog)<br>
* assertions (MwAss);<br>
* rule-based logs (MwR-BLog);<br>
* operating system logs (OsLog);<br>
* application logs (AppLog).

The dataset contains a folder for each technique mentioned above. Each folder contains 12,733 files, a file for each experiments (i.e., faults injected in the middleware). Each file cotains the data generated by technique when we inject that fault in the middleware transport layer source code. The name of file indicates the source code file where the fault is injected and the type of fault.<br>
DOI: 10.14457/kmutnb.the.1992.1
title: การสร้างชุดการสอนวิชาอิเล็กทรอนิกส์กำลัง เรื่อง การแปลงแรงดันไฟฟ้ากระแสสลับเป็นแรงดันไฟฟ้ากระแสตรงปรับค่าได้ ตามหลักสูตรประกาศนียบัตรวิชาชีพชั้นสูง สถาบันเทคโนโลยีราชมงคล พุทธศักราช 2527 /
DOI: 10.14457/kmutnb.the.1994.3
title: การสร้างและหาประสิทธิภาพชุดประลองไมโครโปรเซสเซอร์ 1 เรื่อง การอินเตอร์เฟสระดับปริญญาครุศาสตร์อุตสาหกรรมสถาบันเทคโนโลยีราชมงคล /
DOI: 10.14457/kmutnb.the.1996.3
title: การพัฒนาวิธีปรับตั้งค่าตัวควบคุมโดยอัตโนมัติสำหรับระบบควบคุมความเร็วที่ขับด้วยดีซีชอปเปอร์ /
DOI: 10.14457/kmutnb.the.1996.4
title: การสร้างหลักสูตรฝึกอบรมเกี่ยวกับการบริหารงานในอุตสาหกรรมการผลิต /
DOI: 10.14457/kmutnb.the.1997.2
title: การนำน้ำลงใต้ดินเพื่อแก้ไขปัญหาน้ำท่วมกรุงเทพมหานคร /
DOI: 10.4225/08/58dd10f4c8a00
title: Parkes observations for project P858 semester 2015APRS_BPSR_52

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: 10.4225/08/58dd1111cf2f7
title: Parkes observations for project P887 semester 2015APRS_BPSR_01

description: Searches for radio pulsations from Fermi sources have been astonishingly fruitful, both in discovering new pulsars and in probing the physics of high-energy emission.  We propose observations of members of two promising Fermi source classes: (1) candidate enshrouded millisecond pulsars (2) new "blind search" gamma-ray pulsars.  The former are fascinating systems in which the wind of an energetic recycled millisecond pulsar is disintegrating its companion; detecting pulsations turns them into laboratories for this process.  The latter are pulsars recently discovered in computational tour de force trawls of the Fermi data.  Radio pulsations greatly add to the information we can obtain; conversely, deep upper limits constrain emission models.
DOI: 10.4225/08/58dd1137cf7f0
title: Parkes observations for project P858 semester 2015APRS

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.1996.1
title: การสร้างและหาประสิทธิภาพชุดประลองการติดต่อสื่อสารด้วยเส้นใยแก้วนำแสง /
DOI: 10.14457/mu.the.2000.272
title: การสื่อสารในกระบวนการเจรจาต่อรองช่วยเหลือผู้พยายามฆ่าตัวตาย /
DOI: 10.4225/08/58dd152825ebd
title: Parkes observations for project P858 semester 2015APRS04

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.439579
title: Mb2

description: For more information on this data, see T. Menzies and M. Benson and K. Costello and M. Northey and J. Richardson, Learning Better IV&V Practices CSEE WVU and NASA IV&V, May 2007, http://menzies.us/pdf/07ivv.pdf .

WBS.awk:<br>
A list of tasks and their ids, and how they are selected based on<br>
consequence (co) and error potential (ep). task 1. are management<br>
tasks that occur across the lifecycle. tasks 2,3,4,5,6,7 are tasks at<br>
"concept", "requirements", "design", "coding","testing", and "other"<br>
phases (respectively)

CM10.csv:

The relative costs of performing IV&V tasks (sanitized, normalized, sums to 100).

Silap433.csv:

SILAP scores given to 433 NASA software components (parts of a project that received individual attention by IV&V)

TM1:

Frequency of IV&;V tasks (generated by running distributions of<br>
Silap433 through SILAP).

KC10robot.csv:

The pattern of issue severity seen in robotic systems;

KC10human.csv:

The pattern of issue severity seen in human-rated systems.

Silap211.csv:

A mapping of SILAP scores on 211 components to their final issue<br>
severities.
DOI: 10.5281/zenodo.439583
title: Bugreport

description: The data files have been extracted from the eclipse, gnome, and mozilla bug repositories (many thanks goes to all the contributors of these projects). The data is until the year 2009.

Each row denotes the values extracted from one bug report. For each of the bug report attributes (listed below), we obtained the values at different points in time: current entry, the first entry (when the bug was reported), and the entries/measures after 1,3,7,14, and 30 days after the bug has been reported.
DOI: 10.5281/zenodo.439584
title: Mtdjedit

description: More info can be found at http://openscience.us/repo/issues/mtdjedit.html.
DOI: 10.5517/ccdc.csd.cc1nr6l6
title: CCDC 1541648: 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/mju.the.2006.53
title: การปรับเปลี่ยนวัฒนธรรมกับแนวคิดเศรษฐกิจชุมชนทางเลือก "เพื่อความยั่งยืน" : กรณีศึกษาโรงสีชุมชน /
DOI: 10.14457/mju.the.2006.59
title: สมบัติทางกายภาพและสมบัติการต้านออกซิเดชันของผลมะเกี๋ยง ในระหว่างกระบวนการผลิตเครื่องดื่มผงและการเก็บรักษา /
DOI: 10.15129/f56324dd-5f25-4775-86e1-087d09b3e75d
title: Interaction angle dependence of stochastic photon emission in the collision of electrons with intense focussed laser pulses

description: This dataset provides example trajectories for electrons colliding with a high-intensity focussed laser pulse using a stochastic single-photon emission model for radiation reaction. Along with these, the final properties for an enemble of 1000 initially-identical electrons is provided for interaction angles varying from 0 to 150 degrees. The data files themselves are described in the attached README.txt file.