cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.4225/08/58dd118d3e42d
title: Parkes observations for project P892 semester 2015APRS_BPSR_13

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Recent results show that there is a strong latitude dependence to FRB detectability so SUPERBx will search above 25 degrees in Galactic latitude. It will use 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 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 other radio telescopes (Molonglo, GMRT, MWA) 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.
DOI: 10.4225/08/58dd15a479671
title: Parkes observations for project P858 semester 2015APRS_BPSR_49

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/mju.res.2006.96
title: สัมฤทธิผลการเรียนรู้เชิงพุทธิพิสัย โดยเทคนิคการสร้างความสนใจที่แตกต่างกันจากรายการวิดีทัศน์ ของนักศึกษาสถาบันเทคโนโลยีราชมงคล /
DOI: 10.4225/08/58dd11682af1b
title: Parkes observations for project P858 semester 2015APRS_BPSR_29

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.439593
title: Mcintosh

description: In order to evaluate the impact that code review coverage and participation have on software quality, the authors extract code review data from the Gerrit review databases of the studied systems, and link the review data to the integrated patches recorded in the corresponding VCSs.

The data extraction approach is broken down into three steps: (1) extract review data from the Gerrit review database, (2) extract Gerrit change IDs from the VCS commits, and (3) calculate version control metrics.<br>
DOI: 10.7910/dvn/bsheml
title: Test image for data-pack
DOI: 10.14457/mju.the.2006.56
title: การพัฒนาวิธีที่รวดเร็วสำหรับตรวจวิเคราะห์ยีนที่เกี่ยวข้องกับการสร้างสารพิษที่สร้างโดย Bacillus cereus /
DOI: 10.14457/mju.the.2006.57
title: การสกัดและการแยกเอนไซม์ย่อยไฟบรินจากถั่วเน่า /
DOI: 10.14457/mju.the.2006.61
title: การเปรียบเทียบผลผลิตและระยะการพักตัวของถั่วลิสง 6 สายพันธุ์ใหม่ /
DOI: 10.14457/mju.the.2006.65
title: การศึกษาวิธีการลดปริมาณซัลเฟอร์ไดออกไซด์ตกค้างในผลลำไยสด /
DOI: 10.14457/mju.the.2006.68
title: การใช้ปุ๋ยหมักจุลินทร์ EM ในนาข้าวของเกษตรกร ภายใต้โครงการเศรษฐกิจแบบพอเพียงของกรมทหารราบที่ 6 จังหวัดอุบลราชบุรี /
DOI: 10.14457/mju.the.2006.69
title: การศึกษาการสกัดน้ำมันและคุณสมบัติของน้ำมันจากแมคคาเดเมียที่ปลูกที่บ้านดอยช้าง /
DOI: 10.14457/mju.the.2006.70
title: การศึกษาการจัดทรงต้น 4 แบบ ต่อการเจริญเติบโตทางกิ่งใบ และการออกดอก และคุณภาพผลผลิตของลำไยพันธุ์อีดอ /
DOI: 10.4225/08/58dd158e59393
title: Parkes observations for project P858 semester 2015APRS_BPSR_47

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.439595
title: Jzinference

description: directory<br>
*this package contains all 1-MRs and 2-MRs our MRI inferred from the four libraries. Notice that all files are the original data our MRI produced, that is, all the MRs listed in this package are presented with a series of parameters.*<br>
* MRs_apache<br>
 1. MRs_apache[1-MRs inferred from Apache. Every function’s MRs are presented in the txt file in this directory named by the function’s name, including series of parameters, number of MRs, and the run time. Same to the other similar packages.]<br>
 2. MRs_apache<br>
* MRs_gsl<br>
 1. MRs_gsl<br>
 2. MRs_gsl<br>
* MRs_jdk<br>
 1. MRs_jdk<br>
 2.MRs_jdk<br>
* MRs_matlab<br>
 1. MRs_matlab<br>
 2. MRs_matlab<br>
* time&MRnumber

*statistics on MR number and run time of all the MRs inferred from four libraries.*<br>
DOI: 10.5523/bris.3mi7qse4pwhwe23mryb8j9rxdk
title: Data for the paper Updating of Aerodynamic Reduced Order Generated using Computational Fluid Dynamics

description: open access data
DOI: 10.14457/mju.res.2006.98
title: การโฆษณาสินค้าประเภทเครื่องดื่มชูกำลังผ่านสื่อโทรทัศน์ ตามทรรศนะของผู้ประกอบอาชีพขับรถสี่ล้อแดง ในจังหวัดเชียงใหม่ /
DOI: 10.14457/mju.res.2006.99
title: การสังเคราะห์สารตัวเร่งปฏิกิริยาวัลคาไนเซชั่น เพื่อใช้ในอุตสาหกรรมยางธรรมชาติ /
DOI: 10.14457/mju.the.2006.67
title: คุณค่าทางอาหารและการย่อยได้ของกากส่าเหล้าในอาหารโคนม /
DOI: 10.15785/sbgrid/284
title: Micro-Electron Diffraction data from Tau VQIVYK peptide, source of 5k7n structure

description: Micro-electron diffraction data from tau VQIVYK peptide
description: Convert images to SMV:
  $ tvips2smv -d 1314 -r 0.188 -o 0p3dps_mov03/vqivyk_###.img in10c5_730m_2s_0p3dps_mov03_000.tvips
  $ tvips2smv -d 1314 -r 0.188 -o 0p3pds_mov04/vqivyk_###.img in10c5_730m_2s_0p3dps_mov04_000.tvips

Processing parameters:
  DATASET                      GAIN  Direction of spindle rotation
  in10c5_730m_2s_0p3dps_mov03  5     Forward
  in10c5_730m_2s_0p3dps_mov04  5     Forward
DOI: 10.15785/sbgrid/287
title: Micro-Electron Diffraction data from Thaumatin, source of 5k7q structure

description: Micro-electron diffraction data from thaumatin
description: Convert corrected images to SMV:
  $ img2px -d 2640 -s 11 -o movie_01/thau_###.img movie1-5m4s+2-_04_00?.tvips
  $ img2px -d 3600 -s 10 -o movie_06/thau_###.img movie2m4s-2+_sq11_01_00?.tvips
  $ img2px -d 3240 -s 12 -o movie_32/thau_###.img movie1-75m4s-2+_sq07_01_000.tvips

MOSFLM processing parameters:
  DATASET                  ADC offset  GAIN  Direction of spindle rotation
  movie1-5m4s+2-_04        44          5     Backward
  movie2m4s-2+_sq11_01     41          5     Forward
  movie1-75m4s-2+_sq07_01  37          5     Forward
DOI: 10.5255/ukda-sn-8128-3
title: United Kingdom Time Use Survey, 2014-2015
DOI: 10.5281/zenodo.439811
title: Train-B Dataset For Icdar2017 Competition On Handwritten Text Recognition On The Read Dataset (Icdar2017 Htr). Batch 1 And Batch 2.

description: Train-B Dataset.   Dataset of pages without any layout or text line information. The corresponding transcripts are provided at page level with line breaks. It has 10k pages, though for convenience it is divided into two 5k page batches. This information is provided in PAGE format. 

This dataset is complementary to this other dataset:

https://zenodo.org/record/439807#.WOIBZ3WLSkA

More information at:

https://scriptnet.iit.demokritos.gr/competitions/~icdar2017htr/
DOI: 10.14457/kmutt.res.2004.62
title: ผลของความเข้มข้นต่อสมบัติของน้ำแตงโมใส /
DOI: 10.15785/sbgrid/286
title: Micro-Electron Diffraction data from Xylanase, source of 5k7p structure

description: Micro-electron diffraction data from xylanase
description: Convert corrected images to SMV:
  $ img2px -d 3240 -s 11 -o sq_06_02/xyl_###.img movie1-75m4s-2+_sq06_02_00?.tvips
  $ img2px -d 3240 -s 11 -o sq_08_02/xyl_###.img movie1-75m4s-2+_sq08_02_00?.tvips
  $ img2px -d 3240 -s 10 -o sq_09_01/xyl_###.img movie1-75m4s-2+_sq09_01_00?.tvips
  $ img2px -d 3240 -s 10 -o sq_10_02/xyl_###.img movie1-75m4s-2+_sq10_02_00?.tvips

MOSFLM processing parameters:
  DATASET                  ADC offset  GAIN  Direction of spindle rotation
  movie1-75m4s-2+_sq06_02  37          5     Forward
  movie1-75m4s-2+_sq08_02  38          5     Forward
  movie1-75m4s-2+_sq09_01  39          5     Backward
  movie1-75m4s-2+_sq10_02  39          5     Backward
DOI: 10.4225/08/58dd118023b4c
title: Parkes observations for project P892 semester 2015APRS_BPSR_12

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Recent results show that there is a strong latitude dependence to FRB detectability so SUPERBx will search above 25 degrees in Galactic latitude. It will use 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 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 other radio telescopes (Molonglo, GMRT, MWA) 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.
DOI: 10.4225/08/58dd11998a173
title: Parkes observations for project P880 semester 2015APRS

description: XSS J1227-4859 is the second "Transitional" pulsar binary system discovered in the galactic field. We plan to set up a campaign of observations at 50cm, 20cm, and 10cm with the aims of: (i) discriminating the various proposed mechanisms responsible for the orbital variations seen in the system; (ii) studying the time evolution and the nature of the radio eclipses; (iii) investigating the nature of the gamma-ray emission from the binary; (iv) determining the critical X-ray luminosity above which the pulsed radio emission disappears;  (v) constraining the geometry of the emission from the system in the radio, X-ray and gamma-ray bands.
DOI: 10.14457/kmutt.res.2005.81
title: ผลของความเร็วและความเข้มข้นของสารอาหาร ต่อการเกิดฟิล์มบนวัสดุตัวกลาง ในช่วงเริ่มต้นระบบของถังปฏิกรณ์ไร้อากาศแบบลูกผสม /
DOI: 10.18430/m35ttf
title: X-ray diffraction data for the crystal structure of catalytic domain of G9a with MS012 (5TTF)
DOI: 10.18430/m35uba
title: X-ray diffraction data for the human RNA Pseudouridylate Synthase Domain Containing 4 (5UBA)
DOI: 10.18430/m35una
title: X-ray diffraction data for the fragment of 7SK snRNA methylphosphate capping enzyme (5UNA)
DOI: 10.18430/m35upd
title: X-ray diffraction data for the methyltransferase domain of human Wolf-Hirschhorn Syndrome Candidate 1-Like protein 1 (WHSC1L1) (5UPD)
DOI: 10.4225/08/58dd11a58f83b
title: Parkes observations for project P860 semester 2015APRS_BPSR_02

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 60 pulsars from 50% of processed data. Extrapolation and population synthesis show that the Galactic plane survey will result in at least a further 60 discoveries. Currently, with data processing on-going employing all available computing resources, we expect about 15 new discoveries per semester.

The discovery of pulsars is just a ?rst step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any individual interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the ?rst time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.4225/08/58dd15dc33e5d
title: Parkes observations for project P860 semester 2015APRS_BPSR_05

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 60 pulsars from 50% of processed data. Extrapolation and population synthesis show that the Galactic plane survey will result in at least a further 60 discoveries. Currently, with data processing on-going employing all available computing resources, we expect about 15 new discoveries per semester.

The discovery of pulsars is just a ?rst step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any individual interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the ?rst time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.14457/kmutt.res.2002.51
title: ผลของความเร็วไหลขึ้นต่อการสร้างตะกอนเม็ดของระบบบำบัดแบบยูเอเอสบีที่บำบัดน้ำเสียที่มีโปรตีนเป็นองค์ประกอบหลัก /
DOI: 10.14457/kmutt.the.2007.485
title: ผลของความเข้มข้นของซัลไฟด์ละลาย ต่อการออกซิไดซ์ซัลไฟด์ /
DOI: 10.17632/y5r8rzf3xg.1
title: Data for: Benefits and Drawbacks of Software Reference Architectures: A Case Study

description: - annexA.pdf --&gt; Instruments and analysis used in the paper "Benefits and Drawbacks of Software Reference Architectures: A Case Study" - annexB.xlsx --&gt; Data collected in the case study of the paper "Benefits and Drawbacks of Software Reference Architectures: A Case Study"
DOI: 10.18430/m35ttg
title: X-ray diffraction data for the crystal structure of catalytic domain of GLP with MS012 (5TTG)
DOI: 10.4225/08/58dd15b039383
title: Parkes observations for project P858 semester 2015APRS_BPSR_50

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: 10.4225/08/58dd15bb0dee9
title: Parkes observations for project P860 semester 2015APRS_BPSR_01

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 60 pulsars from 50% of processed data. Extrapolation and population synthesis show that the Galactic plane survey will result in at least a further 60 discoveries. Currently, with data processing on-going employing all available computing resources, we expect about 15 new discoveries per semester.

The discovery of pulsars is just a ?rst step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any individual interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the ?rst time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.
DOI: 10.14457/kmutt.res.2001.20
title: ผลของความร้อนต่อสมบัติทางกายภาพของพลอยทับทิม /
DOI: 10.18430/m35kkp
title: X-ray diffraction data for the crystal Structure of Human Pseudouridylate Synthase 7 (5KKP)
DOI: 10.18430/m35ubb
title: X-ray diffraction data for the crystal structure of human alpha N-terminal protein methyltransferase 1B (5UBB)
DOI: 10.4225/08/58dd15c638759
title: Parkes observations for project P858 semester 2015APRS_BPSR_54

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/mju.the.2006.66
title: ศึกษาศักยภาพการผลิตถั่วอะซูกิในพื้นที่นาบนที่สูง /
DOI: 10.14457/mju.the.2006.71
title: ภาพลักษณ์มหาวิทยาลัยราชภัฏอุตรดิตถ์ในทรรศนะ ของนักเรียนชั้นมัธยมศึกษาตอนปลาย /
DOI: 10.4225/08/58dd11b294f5c
title: Parkes observations for project P860 semester 2015APRS_BPSR_03

description: This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have already discovered 60 pulsars from 50% of processed data. Extrapolation and population synthesis show that the Galactic plane survey will result in at least a further 60 discoveries. Currently, with data processing on-going employing all available computing resources, we expect about 15 new discoveries per semester.

The discovery of pulsars is just a ?rst step and interesting science can usually only be revealed when a follow-up timing campaign is carried out. One year of initial timing is the minimal timespan required to fully-characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities.

This follow-up timing project is necessary for identifying any individual interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are followed-up for the ?rst time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar phase space. Given the large number of discoveries expected and the long integration length required, this dedicated follow-up timing campaign is vital for achieving our science goals.