cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5061/dryad.sr7m5/1
title: Intraspecific variation data

description: Data on CTmin, CTmax, Topt and desiccation rate for rainforest sunskinks from numerous populations, as well as environmental variables for each population/collection group
DOI: 10.5281/zenodo.439257
title: Tuning Ch3Nh3Pb(I1-Xbrx)3 Perovskite Oxygen Stability In Thin Films And Solar Cells

description: The rapid development of organic-inorganic lead halide perovskites has resulted in high efficiency photovoltaic devices. However the susceptibility of these devices to degradation under environmental stress has so far hindered commercial development, requiring for example expensive device encapsulation. Herein, we have investigated the stability of CH3NH3Pb(I1-xBrx)3 [x = 0..1] thin film and solar cells under controlled humidity, light, and oxygen conditions. We show that higher bromide ratios increases tolerance to moisture, with x = 1 thin films being stable to 120 hr of moisture stress. Under light and dry air, partial bromide (x &lt; 1) subsitution does not enhance film stability significantly, with the corresponding solar cells degrading within two hours. In contrast CH3NH3PbBr3 films show excellent stability, with device stability being limited by the organic interlayer. For these x = 1 films we show charge carriers are quenched in the presence of oxygen and form superoxide; however in contrast to perovskites containing iodide, this superoxide does not degrade the crystal. Our observations show that iodide limits the oxygen and light stability of CH3NH3Pb(I1-xBrx)3 perovskites, but that CH3NH3PbBr3 provides an opportunity to develop inherently stable high voltage photovoltaic devices and 4-terminal tandem solar cells.
DOI: 10.5281/zenodo.439592
title: Chabada

description: How do we know a program does what it claims to do? After clustering Android apps by their <br>
description topics, we identify outliers in each cluster with respect to their API usage. A <br>
"weather" app that sends messages thus becomes an anomaly; likewise, a "messaging" app would <br>
typically not be expected to access the current location. Applied on a set of 22,500+ Android <br>
applications, our CHABADA prototype identified several anomalies; additionally, it flagged 56% <br>
of novel malware as such, without requiring any known malware patterns.
DOI: 10.14457/mju.the.2006.64
title: การสร้างภาพลักษณ์และภาพลักษณ์ของกองศูนย์ฝึกอบรมแม่เมาะ ตามทรรศนะของกลุ่มเป้าหมาย /
DOI: 10.4225/08/58dd11508e6a1
title: Parkes observations for project P858 semester 2015APRS_BPSR_27

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: 10.4225/08/58dd15499e979
title: Parkes observations for project P858 semester 2015APRS_BPSR_21

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: 10.4225/08/58dd155e73772
title: Parkes observations for project P858 semester 2015APRS_BPSR_25

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: 10.4225/08/58dd157fc7444
title: Parkes observations for project P858 semester 2015APRS_BPSR_46

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.439589
title: Xmlmate

description: <strong>Teaser video</strong>

http://youtu.be/-yKom5mbft0

<strong>Abstract</strong>

Generating system inputs satisfying complex constraints is still a challenge for modern test generators. We present XMLMATE, a search-based test generator specially aimed at XML-based systems. XMLMATE leverages program structure, existing XML schemas, and XML inputs to generate, mutate, recombine, and evolve valid XML inputs.

XMLMATE is a search-based test generator. As sketched in Figure 2, it either takes a population of sample XML inputs or randomly generates one, and then systematically evolves this population over several generations to reach the desired coverage goal. To evolve inputs it applies mutation and crossover operators to individuals and favors the procreation and survival of the fittest according to a fitness function geared towards obtaining coverage and triggering exceptions. Measuring the fitness of an input requires executing the program under test; therefore, the runtime of the approach scales linearly with the runtime of the program.

XMLMATE is a search-based test generator. As sketched in Figure 2, it either takes a population of sample XML inputs or randomly generates one, and then systematically evolves this population over several generations to reach the desired coverage goal. To evolve inputs it applies mutation and crossover operators to individuals and favors the procreation and survival of the fittest according to a fitness function geared towards obtaining coverage and triggering exceptions. Measuring the fitness of an input requires executing the program under test; therefore, the runtime of the approach scales linearly with the runtime of the program.

Over a set of seven XML-based systems, XMLMATE detected 31 new unique failures in production code, all triggered by system inputs and thus true alarms.<br>
DOI: 10.14457/kmutt.res.2002.49
title: ผลของคาร์บอนไดออกไซด์และอุณหภูมิต่อการเจริญของเชื้อจุลินทรีย์บางชนิดและคุณภาพของผักพร้อมบริโภค /
DOI: 10.14457/mju.res.2000.1
title: การพัฒนาธุรกิจการท่องเที่ยวเชิงนิเวศในชุมชนบ้านโปง ตำบลป่าไผ่ อำเภอสันทราย จังหวัดเชียงใหม่ /
DOI: 10.14457/mju.res.2006.100
title: ความพึงพอใจของเกษตรกรผู้เข้าร่วมโครงการส่งเสริมการเลี้ยงปลาทับทิม ในบ่อดินของจังหวัดนครศรีธรรมราช /
DOI: 10.14457/mju.res.2006.95
title: ทัศคติของสมาชิกสหกรณ์ในโครงการส่งเสริมการเลี้ยงโคแม่พันธุ์ตามยุทธศาสตร์จังหวัดพัทลุง /
DOI: 10.14457/mju.the.2006.62
title: การผลิตเมล็ดพันธุ์โหระพา /
DOI: 10.15785/sbgrid/290
title: Micro-Electron Diffraction data from Thermolysin, source of 5k7t structure

description: Micro-electron diffraction data from thermolysin
description: Convert corrected images to SMV:
  $ img2px -d 2640 -s 9.0 -o thermolysin_041015_01/thermo_###.img movie1-5m4s-2+_sq10_05_00?.tvips
  $ img2px -d 3240 -s 9.0 -o thermolysin_041615_09/thermo_###.img movie1-75m4s-2+_sq01_02_00?.tvips
  $ img2px -d 3240 -s 9.0 -o thermolysin_041615_19/thermo_###.img movie1-75m4s-2+_sq12_02_00?.tvips
  $ img2px -d 2640 -s 5.1 -o 20160314_sq_01_01/thermo_###.img 1-5m_4s_sq01_01_000.tvips

MOSFLM processing parameters:
  DATASET                  ADC offset  GAIN  Direction of spindle rotation
  movie1-5m4s-2+_sq10_05   40          4     Forward
  movie1-75m4s-2+_sq01_02  10          5     Forward
  movie1-75m4s-2+_sq12_02  40          5     Forward
  1-5m_4s_sq01_01          14          5     Forward
DOI: 10.4225/08/58dd1173ec102
title: Parkes observations for project P892 semester 2015APRS_BPSR_11

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: 10.4225/08/58dd1599800a3
title: Parkes observations for project P858 semester 2015APRS_BPSR_48

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.439590
title: Taskdict

description: For the empirical analysis, the authors created two datasets: dataset1 includes all change tasks<br>
that have at least one change set associated with them; dataset 2 is a subset of dataset 1 and<br>
includes all change tasks that have at least one change set and one task context associated. For<br>
the AspectJ project the authors only created dataset 1, since only two tasks had a task context<br>
associated. For each project the authors split each dataset into a training set to create the<br>
dictionary and a test set. For reasonable training and test sets and to be able to compare them<br>
across projects, they chose the test set size to be ten. Also, to be able to compare the results<br>
of the dictionaries using dierent in-formation sources (change sets and/or task contexts) as well<br>
as preserving the chronological order, they chose the last ten change tasks in dataset 2 as the<br>
test set for Mylyn.Tasks,Mylyn. Context and Remus and the last ten change tasks in dataset 1 for<br>
AspectJ. All change tasks that were resolved before the ones in the test set were used as the<br>
training set.
DOI: 10.14457/kmutt.res.2002.50
title: ผลของความเร็วไหลขึ้นต่อการสร้างตะกอนเม็ดของระบบบำบัดแบบยูเอเอสบีบำบัดน้ำเสียคาร์โบไฮเดรต /
DOI: 10.14457/kmutt.res.2005.80
title: ผลของคาร์บอนไดออกไซด์ต่อการควบคุมเชื้อรา Aspergillus flavus และการสร้างอะฟลาทอกซิน B1 ในข้าวกล้องพันธุ์ขาวดอกมะลิ 105 ในระหว่างการเก็บรักษา /
DOI: 10.14457/mju.res.2006.101
title: การจัดการทรัพยากรป่าไม้โดยภูมิปัญญาท้องถิ่นของชนเผ่าปกาเกอะญอ ในพื้นที่ศูนย์พัฒนาโครงการหลวงแม่สะป๊อก จังหวัดเชียงใหม่ /
DOI: 10.14457/mju.the.2006.54
title: การพัฒนาวิธีและการศึกษาความเหมาะสมในการใช้ Chromogenic Substrate เพื่อตรวจวิเคราะห์ Escherichia coli ในอุตสาหกรรมอาหาร /
DOI: 10.14457/mju.the.2006.63
title: ผลของการใช้เปลือกกุ้งในอาหารต่อคุณภาพซากและระดับคอเลสเตอรอลในเนื้อสุกรขุน /
DOI: 10.15785/sbgrid/288
title: Micro-Electron Diffraction data from Trypsin, source of 5k7r structure

description: Micro-electron diffraction data from trypsin
description: Convert corrected images to SMV:
  $ img2px -d 2640 -s 6.0 -o 20160310_sq_10_02/tryp_###.img 1-5m_4s_sq10_02_000.tvips
  $ img2px -d 3080 -s 5.0 -o 20160310_sq_05_01/tryp_###.img 1-75m_4s_sq05_01_000.tvips
  $ img2px -d 3080 -s 5.0 -o 20160310_sq_09_02/tryp_###.img 1-75m_4s_sq09_02_000.tvips
  $ img2px -d 2640 -s 4.8 -o 20160318_sq_01_01/tryp_###.img 1-5m_4s_sq01_01_000.tvips
  $ img2px -d 2640 -s 5.0 -o 20160318_sq_04_01/tryp_###.img 1-5m_4s_sq04_01_000.tvips
  $ img2px -d 2640 -s 5.0 -o 20160318_sq_04_02/tryp_###.img 1-5m_4s_sq04_02_000.tvips
  $ img2px -d 2640 -s 4.6 -o 20160318_sq_11_01/tryp_###.img 1-5m_4s_sq11_01_000.tvips
  $ img2px -d 2640 -s 4.4 -o 20160318_sq_11_02/tryp_###.img 1-5m_4s_sq11_02_000.tvips
  $ img2px -d 2640 -s 5.2 -o 20160318_sq_15_01/tryp_###.img 1-5m_4s_sq15_01_000.tvips
  $ img2px -d 2640 -s 5.8 -o 20160316_sq_07_01/tryp_###.img 1-5m_4s_sq07_01_000.tvips

MOSFLM processing parameters:
  DATASET           ADC offset  GAIN  Direction of spindle rotation
  1-5m_4s_sq10_02   13          5     Forward
  1-75m_4s_sq05_01  13          5     Forward
  1-75m_4s_sq09_02  13          5     Forward
  1-5m_4s_sq01_01   15          5     Forward
  1-5m_4s_sq04_01   15          5     Forward
  1-5m_4s_sq04_02   15          5     Forward
  1-5m_4s_sq11_01   15          5     Forward
  1-5m_4s_sq11_02   15          5     Forward
  1-5m_4s_sq15_01   14          5     Forward
  1-5m_4s_sq07_01   13          5     Forward
DOI: 10.4225/08/58dd115c73020
title: Parkes observations for project P858 semester 2015APRS_BPSR_28

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: 10.4225/08/58dd1569a146d
title: Parkes observations for project P858 semester 2015APRS_BPSR_44

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: 10.4225/08/58dd1574d8c67
title: Parkes observations for project P858 semester 2015APRS_BPSR_45

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/kmutt.res.2008.102
title: ผลของความเค็มต่อจุลินทรีย์ กลุ่มออโตโทรปดีไนตริฟายด์ในการกำจัดแอมโมเนีย /
DOI: 10.14457/mju.res.2006.97
title: การวิเคราะห์ต้นทุนและจุดคุ้มทุนของโครงการผลิตลูกสุกร ของสหกรณ์ผู้เลี้ยงสุกรสระบุรี จำกัด /
DOI: 10.14457/mju.the.2006.55
title: การพัฒนาผลิตภัณฑ์เนื้อหมูสันนอกหมักรมควัน โดยวิธีการนวดสุญญากาศ /
DOI: 10.14457/mju.the.2006.60
title: การพัฒนาและการสุกแก่ของเมล็ดพันธุ์ข้าวโพดข้าวเหนียว /
DOI: 10.15785/sbgrid/285
title: Micro-Electron Diffraction data from Lysozyme, source of 5k7o structure

description: Micro-electron diffraction data from lysozyme
description: Convert corrected images to SMV:
  $ img2px -d 2640 -s 5.0  -o 20160310_sq_01_01/lyso_###.img 1-5m_4s_sq01_01_000.tvips
  $ img2px -d 2640 -s 5.0  -o 20160310_sq_02_02/lyso_###.img 1-5m_4s_sq02_02_000.tvips
  $ img2px -d 2640 -s 10.0 -o 20160310_sq_03_02/lyso_###.img 1-5m_4s_sq03_02_000.tvips
  $ img2px -d 2640 -s 4.9  -o 20160311_sq_03_01/lyso_###.img 1-5m_4s_sq03_01_000.tvips
  $ img2px -d 2640 -s 6.0  -o 20160311_sq_06_02/lyso_###.img 1-5m_4s_sq06_02_000.tvips
  $ img2px -d 2640 -s 11.0 -o 20160311_sq_08_01/lyso_###.img 1-5m_4s_sq08_01_000.tvips
  $ img2px -d 2640 -s 6.0  -o 20160311_sq_08_02/lyso_###.img 1-5m_4s_sq08_02_000.tvips

MOSFLM processing parameters:
  DATASET          ADC offset  GAIN  Direction of spindle rotation
  1-5m_4s_sq01_01  14          5     Forward
  1-5m_4s_sq02_02  14          5     Forward
  1-5m_4s_sq03_02  11          5     Forward
  1-5m_4s_sq03_01  14          5     Forward
  1-5m_4s_sq06_02  13          5     Forward
  1-5m_4s_sq08_01  10          5     Forward
  1-5m_4s_sq08_02  13          5     Forward
DOI: 10.14457/mju.the.2006.58
title: ความเป็นไปได้ในการใช้วัตถุดิบทางการเกษตรที่เหลือจากอุตสาหกรรมอาหาร เพื่อทดแทนอาหารเลี้ยงเชื้อสังเคราะห์ ในการเลี้ยงแบคทีเรียกรดแลคติก /
DOI: 10.15785/sbgrid/289
title: Micro-Electron Diffraction data from Proteinase K, source of 5k7s structure

description: Micro-electron diffraction data from proteinase K
description: Convert corrected images to SMV:
  $ img2px -d 2200 -s 4.9  -o movie_01_01/prot_###.img p01_cl1200mm5sp01mv01_000.tvips
  $ img2px -d 2200 -s 5.8  -o movie_05_01/prot_###.img p05_cl1200mm5sp05mv01_000.tvips
  $ img2px -d 2200 -s 10.0 -o movie_06_01/prot_###.img p06_cl1200mm5sp05mv01_000.tvips
  $ img2px -d 2200 -s 11.0 -o movie_08_01/prot_###.img p08_cl1200mm5sp05mv01_000.tvips
  $ img2px -d 2200 -s 12.0 -o movie_09_01/prot_###.img p09_cl1200mm5sp05mv01_000.tvips
  $ img2px -d 2200 -s 6.0  -o movie_10_01/prot_###.img p10_cl1200mm5sp05mv01_000.tvips

MOSFLM processing parameters:
  DATASET                ADC offset  GAIN  Direction of spindle rotation
  p01_cl1200mm5sp01mv01  14          5     Forward
  p05_cl1200mm5sp05mv01  13          5     Forward
  p06_cl1200mm5sp05mv01  11          5     Forward
  p08_cl1200mm5sp05mv01   7          5     Forward
  p09_cl1200mm5sp05mv01   7          5     Forward
  p10_cl1200mm5sp05mv01  12          5     Forward
DOI: 10.18430/m35tey
title: X-ray diffraction data for the human METTL3-METTL14 complex (5TEY)