cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.14457/mju.res.2003.3
title: การศึกษาพ่อ-แม่พันธุ์ปลาบึก จากการเลี้ยงเพื่อการอนุรักษ์และพัฒนาการเพาะเลี้ยงสัตว์น้ำเชิงพาณิชย์ /
DOI: 10.14457/mju.res.2005.10
title: โครงสร้าง องค์ประกอบและการใช้ประโยชน์จากป่าในพื้นที่ลุ่มน้ำขุนสมุน กรณีศึกษา : บ้านกาใสและบ้านละเบ้ายา จังหวัดน่าน /
DOI: 10.14457/mju.res.2005.13
title: ปัญหาและแนวทางแก้ไขธุรกิจเงินฝากของธนาคารเพื่อการเกษตรและสหกรณ์การเกษตร ในจังหวัดเพชรบุรี /
DOI: 10.4225/08/58dd15fe60497
title: Parkes observations for project P892 semester 2015APRS_BPSR_16

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: 10.14457/mju.res.2005.11
title: การศึกษาภาพลักษณ์ร้านสหกรณ์ธนาคารเพื่อการเกษตรและสหกรณ์การเกษตร จำกัด /
DOI: 10.14457/mju.res.2005.12
title: ความคิดเห็นในการปรับปรุงโครงสร้างและการพัฒนาระบบสารสนเทศ ในสหกรณ์ออมทรัพย์ กรมทรัพยากรธรณี จำกัด /
DOI: 10.14457/mju.res.2005.15
title: ความคิดเห็นและความคาดหวังต่อภาวะผู้นำของเจ้าหน้าที่ส่งเสริมการเกษตร ของสมาชิกศูนย์ส่งเสริมและผลิตเมล็ดพันธุ์ข้าวชุมชน อำเภอสันทราย จังหวัดเชียงใหม่ /
DOI: 10.14457/mju.res.2005.16
title: ความคิดเห็นของพนักงานธนาคารเพื่อการเกษตรและสหกรณ์การเกษตร ที่มีต่อการจำหน่ายสินค้าของร้านสหกรณ์ธนาคารเพื่อการเกษตรและสหกรณ์การเกษตร จำกัด /
DOI: 10.4225/08/58dd11c0960e2
title: Parkes observations for project P885 semester 2015APRS

description: We propose to monitor for one year 1E 1547.0-5408 and PSR J1622-4950,
two of the three magnetars known to currently emit radio waves.
Both were discovered at Parkes and their radio pulsations can only
be studied there. As magnetars (of which only 23 are confirmed in
the Galaxy), the aim is to develop a more reliable understanding
of the dynamical behaviour of their magnetospheres and ultra-strong
magnetic fields, which are responsible for X-ray and gamma-ray
outbursts, magnetospheric currents and particle acceleration, and
heating of the neutron star surface. We do this by tracking their
unsteady rotation in detail (the variable rotation period derivative
provides a measure of the changing torque) and also by comparing
to the X-ray flux when available (currently via the Swift satellite
for 1E 1547.0-5408). As radio magnetars (only four have been
identified, and the first one no longer emits radio waves), our aim
is to understand the conditions under which radio emission takes
place (both for each particular object, and in the larger context
of the known population of magnetars, most of which aren't known 
to emit in the radio), and to characterize the variable radio
emission in order to place constraints on the emission mechanisms,
which at least in part differ from those of ordinary pulsars. We
do this by measuring their varying radio flux density and (full-Stokes)
pulse profiles, and by comparing the radio characteristics to their
torque and X-ray behaviour.
DOI: 10.4225/08/58dd15d0c105e
title: Parkes observations for project P860 semester 2015APRS_BPSR_04

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: 10.5281/zenodo.266823
title: Whole-Cell Escherichia Coli Lactate Biosensor For Monitoring Mammalian Cell Cultures During Biopharmaceutical Production-- Dataset

description: Raw data for Goers et al, (2017), Biotech Bioeng. doi:10.1002/bit.26254.

Each graph including the supplementary figures is a separate tab.
DOI: 10.5517/ccdc.csd.cc1nqqx0
title: CCDC 1541193: Experimental Crystal Structure Determination

description: Related Article: Cai Minghan|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: 10.4225/08/58dd11d265304
title: Parkes observations for project P886 semester 2015APRS

description: The Parkes radio telescope has discovered more than half of the known radio pulsars.  Much of the raw data from historical surveys has now been collated and stored in the CSIRO data archive. This allows us to reprocess these surveys with modern search algorithms.  We expect to discover pulsars that were not discovered in the original processing (such as pulsars in fast binary systems, intermittent pulsars, burst events, etc.). This proposal is to request observing time to confirm our expected candidates.
DOI: 10.14457/mju.res.2000.2
title: การปรับปรุงพันธุ์เบญจมาศ โดยวิธีการชักนำให้เกิดการกลายพันธุ์ /
DOI: 10.4225/08/58dd15e90af51
title: Parkes observations for project P892 semester 2015APRS_BPSR_01

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: 10.4225/08/58dd15f3831fa
title: Parkes observations for project P892 semester 2015APRS_BPSR_02

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: 10.4225/08/58dd162a1b408
title: Parkes observations for project P892 semester 2015APRS_BPSR_03

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: 10.5255/ukda-sn-6689-8
title: Annual Survey of Hours and Earnings, 1997-2016: Secure Access
DOI: 10.5517/ccdc.csd.cc1nr4vd
title: CCDC 1541594: 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: 10.4225/08/58dd11e4aced5
title: Parkes observations for project P892 semester 2015APRS_BPSR_19

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: 10.4225/08/58dd16147ec19
title: Parkes observations for project P892 semester 2015APRS_BPSR_18

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: 10.4225/08/58dd164153a16
title: Parkes observations for project P892 semester 2015APRS_BPSR_05

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: 10.14457/mju.res.2005.17
title: การศึกษาการดำเนินงานของสหกรณ์การเกษตร เพื่อการตลาดลูกค้าธนาคารเพื่อการเกษตรและสหกรณ์การเกษตรในภาคตะวันออก ปีบัญชี 2538-2547 /
DOI: 10.14457/mju.res.2005.9
title: ความเป็นไปได้ในการประกันภัยพืช : กรณีศึกษา การปลูกอ้อยของเกษตรกรสมาชิกสหกรณ์การเกษตรเพื่อการตลาด ลูกค้า ธ.ก.ส.กาญจนบุรี จำกัด (สกต.) /
DOI: 10.14457/kmutnb.the.1995.4
title: การศึกษาปัจจัยที่มีผลต่อความร่วมมือทางวิชาการของสถาบันการศึกษากับสถานประกอบการด้านอุตสาหกรรม /
DOI: 10.14457/kmutnb.the.1997.3
title: การศึกษาเปรียบเทียบความชอบอักษรและพื้นที่มีระดับความเข้มในการพิมพ์สีขาว-ดำ แตกต่างกันของนักเรียน นักศึกษา /
DOI: 10.14457/kmutnb.the.1997.4
title: การประยุกต์ใช้การบำรุงรักษาเครื่องจักรแบบทวีผลที่ทุกคนมีส่วนร่วมกับสายการผลิตวงจรรวมอิเล็กทรอนิกส์ /
DOI: 10.14457/mju.res.2004.5
title: การศึกษาอิทธิพลของช่วงระยะเวลาปลูก วิธีการให้น้ำและการควบคุมการเจริญเติบโต ต่อการเกิดดอกของแคลล่าลิลลี /
DOI: 10.4225/08/58dd1609087f2
title: Parkes observations for project P892 semester 2015APRS_BPSR_17

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: 10.14457/kmutnb.the.1993.17
title: การเผาไหม้ขี้เลื่อยในห้องเผาไหม้แบบไซโคลน ชนิดอากาศเข้าหลายช่องทาง /
DOI: 10.14457/kmutnb.the.1996.10
title: สมรรถนะในการปฏิบัติงานของเลขานุการ ที่ปฏิบัติงานในสถานประกอบการเพื่อการส่งออกในสภาพที่เป็นจริง และควรจะเป็นตามความคิดเห็นของผู้บังคับบัญชา /
DOI: 10.14457/kmutnb.the.1997.6
title: ความสัมพันธ์ระหว่าง Unconfined Compressive Strength กับ Soaked CBR ของหินกรวดเหลี่ยมผสมซีเมนต์ และหินกรวดเหลี่ยมผสมแอสฟัลต์ /
DOI: 10.14457/mju.res.2005.14
title: แนวทางการพัฒนาศักยภาพการบริหารงานของคณะกรรมการสหกรณ์การเกษตร โดยกระบวนการฝึกอบรม /
DOI: 10.4225/08/58dd161f359fd
title: Parkes observations for project P860 semester 2015APRS

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: 10.4225/08/58dd1635dcabf
title: Parkes observations for project P892 semester 2015APRS_BPSR_04

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: 10.14457/kmutnb.the.1993.13
title: ปัญหาและอุปสรรคด้านปัจจัยพื้นฐานในการประกอบกิจการอุตสาหกรรมกุ้งแช่แข็งขนาดย่อมและขนาดกลาง /
DOI: 10.4225/08/58dd120149db1
title: Parkes observations for project P737 semester 2015APRS

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.
DOI: 10.14457/kmutnb.the.1993.37
title: การศึกษาพฤติกรรมการไหลของยิบซั่มในไซโล /
DOI: 10.14457/kmutnb.the.1996.7
title: การวิเคราะห์มุมคมตัดในกระบวนการตัดเจาะ /
DOI: 10.14457/kmutnb.the.1996.8
title: การสร้างและหาประสิทธิภาพชุดการสอนวิชาการออกแบบแม่พิมพ์โลหะ เรื่องชนิดและลักษณะการทำงานของแม่พิมพ์โลหะ หลักสูตรครุศาสตร์อุตสาหกรรมบัณฑิต ภาควิชาครุศาสตร์อุตสาหการ คณะครุศาสตรอุตสาหกรรม สถาบันเทคโนโลยีราชมงคล /
DOI: 10.4225/08/58dd1212c7a6b
title: Parkes observations for project P858 semester 2015APRS01

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.1993.10
title: การสร้างและหาประสิทธิภาพชุดการสอน เรื่องการทำความเย็นหลักสูตรครุศาสตร์อุตสาหกรรมบัณฑิต สาขาวิชาวิศวกรรมเครื่องกล สถาบันเทคโนโลยีพระจอมเกล้าพระนครเหนือ /
DOI: 10.14457/kmutnb.the.1993.11
title: ปัญหาและอุปสรรคด้านปัจจัยพื้นฐานของอุตสาหกรรมเครื่องจักรกลการเกษตรขนาดย่อมและขนาดกลาง /
DOI: 10.14457/kmutnb.the.1997.5
title: โปรแกรมคอมพิวเตอร์สำหรับเลือกตำแหน่งและความสูงที่เหมาะสมที่สุดของเสาไฟฟ้าแรงสูง /
DOI: 10.4225/08/58dd121f0b650
title: Parkes observations for project P858 semester 2015APRS02

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.