cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5ccd1cc556a1e
title: Parkes observations for project P456 semester 2019APRS_06

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5ccd1d6c95ce4
title: Parkes observations for project P456 semester 2019APRS_07

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5ccd1d91ba8e4
title: Parkes observations for project P456 semester 2019APRS_08

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5ccd1e77425ce
title: Parkes observations for project P456 semester 2019APRS_09

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5ccd1ea5ca4b4
title: Parkes observations for project P456 semester 2019APRS_10

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.14469/hpc/5605
title: DFT Coordinates File

description: DFT coordinates for mechanistic analysis of hydrodefluorination
DOI: 10.25919/5ccf62dbf39e7
title: Parkes observations for project P970 semester 2018APRS_13

description: During the past 6 years, we at Parkes and collaborators at other radio telescopes have been remarkably successful at discovering millisecond pulsars (MSPs) associated with unidentified Fermi-LAT gamma-ray sources. Based on lessons learned, we here propose to carry out targeted searches with the new Ultra-wideband Low (UWL) receiver that will be installed next semester. The ultra-wide frequency coverage will enable us to detect MSPs with steep spectrum and avoid difficulties caused by interstellar scintillation and dispersive and scattering smearing. We propose to revisit highly ranked pulsar candidates that remain unidentified. Such a pilot survey will help us designing future searches of the coming 4FGL gamma-ray source catalog using the UWL. The overall time request is 23 hours on source, or 26 hours including overheads.
DOI: 10.14469/hpc/5606
title: NMR spectra

description: NMR spectra for the hydroborated compounds 3, 4 and 5 (PPh3 adducts), plus splitting analysis and simulation for compounds 4 and 5.
DOI: 10.25919/5ccd219933b34
title: Parkes observations for project P456 semester 2019APRS_12

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5ccd225ac4e7f
title: Parkes observations for project P985 semester 2019APRS_02

description: We propose to use the ultra-wide-bandwidth, low frequency receiver installed at the Parkes telescope in order to quantify the broad-band intermittency time scale, polarization, quasi-periodicities, and mode changing of a newly discovered pulsar, PSR J1926-0653. The pulsar is unique in its emission properties. It has multiple pulse components, that change with time (both mode- changing and sub-pulse drifting phenomena are evident). The pulsar exhibits nulls in which a few individual pulses seem to be missing. It also exhibits longer-scale (hour-scale) intermittency behaviour in which the emission switches off for long periods of time. The pulse flux densities often, but not always, seem to exhibit quasi-periodic variations. Clearly this pulsar may hold the key to many different emission phenomena and we request time on Parkes, FAST and ATCA to parameterise the pulsar and its emission properties in detail.
DOI: 10.25919/5ccd225def4dd
title: Parkes pulsar observations with undefined project IDs for 2019_BPSR_01

description: Parkes pulsar observations with undefined project IDs for 2019. This collection contains observations from P955.
DOI: 10.7910/dvn/mcgz1s
title: The Oxidized Cholesterol Strategy

description: The Oxidized Cholesterol Strategy isn’t just a system that tackles your cholesterol plaque; it’s a lifestyle regime that teaches you how to completely clean out plaque buildup in your arteries. High cholesterol is a condition many people suffer from and the effects are detrimental and sometimes even fatal. So, it’s imperative to find a way to reduce your cholesterol to healthy levels – and without some weird pills and dangerous medications that come with side effects.The Oxidized Cholesterol Strategy is a unique system that’s based around dropping nothing more than one simple ingredient from your diet. The shocking thing is that, it’s not talking about cutting out butter or other salty foods commonly associated with high cholesterol. Instead, it’s all about a dangerous ingredient that you consume every single day, without even knowing it. This ingredient isn’t even listed in the ingredient list, which is terrifying. Once you read more about it in this system, you’ll be even more terrified that it’s been in your body all this time.The Oxidized Cholesterol Strategy was created by Scott Davis, a member of Blue Heron Health News, a highly renowned health website. He’s written various articles, many of which that specialize in heart health. He also has personal experience dealing with heart health, as he once had a heart attack due to clogged arteries that were a result of high cholesterol.
DOI: 10.7910/dvn/nwynzh
title: The Neuropathy Solution Program

description: Neuropathy Solution is a product that is designed for anyone who suffers from nerve pain, whether it is caused by diabetes, disease, chemotherapy, alcohol problems, hypertension or the aging process. Neuropathy can be a very uncomfortable and painful problem and its symptoms include tingling, numbness, stabbing pains, burning sensations and much more. It is an issue that affects your peripheral nervous system, which is the important part of your nervous system that sends information from your brain and spinal cord to the rest of your body. The Neuropathy Solution program offers you a natural way to fight against neuropathy without the use of prescription drugs. This is advantageous because you are not at risk of side effects. You will be able to cure your nerve pain without ever having to leave the comfort of your own home by following natural procedures. The steps to doing this are all outlined in an easy to follow way within the ebook The Neuropathy Solution, which is available to download online.The author of this program is a man called Randall Labrum, who suffered from peripheral neuropathy for many years. He worked hard to research the issue and he came up with this solution after studying for more than 35 years. The program that he has developed is a very efficient and effective solution to neuropathy pain and it promises long term relief. He knows what it feels like to suffer from neuropathy pain, which is why he worked so hard to put together this program and make sure that everyone could benefit from these very effective solutions.The Neuropathy Solution is a step by step treatment program that will provide you relief from your neuropathy pain. It is divided into several different sections that examine certain aspects of neuropathy. It will go into a discussion about diabetes and its relationship to peripheral neuropathy, as well as how the aging process leads to degeneration of your sensory nerves which will cause you nerve pain. It will explain to you what you can do to counteract this. The book also focuses on ways that you can revitalise the tissues of the body that have been irritated and damaged and how you can reverse the damage done to your nerve endings. You’ll also learn a lot of ways that you can improve your circulatory well being and overturn the effects of neuropathy. You’ll discover a lot about how your nerves work and why they start to malfunction and send these pain and tingling messages to your brain.
DOI: 10.7910/dvn/zovvp4
title: Yeast Infection No More

description: Yeast Infection No More is the only clinically proven 5-step Candida Yeast Infection healing system out there. With so many online programs out there, it can seem impossible to narrow in on the ones that actually work. After all, anyone can put together some content, post it online and call it an effective system. So, knowing that this program is the only Candida Yeast Infection healing system that’s been clinically proven should give you some peace of mind – and confidence that it will actually provide results.Yeast Infection No More is an online system that introduces natural, holistic remedies into your life. It’s a 5-step system that’s been clinically proven to provide amazing results. In fact, you can gain complete relief in as little as 12 hours. Long term, you can treat Candida Yeast Infections completely within 2 months. There’s no need to take (or worse – insert) weird pills or tablets, nor is there a need to take harmful prescription medications. You just have to follow the 5 steps provided. The entire program can be accessed online as soon as you purchase. You simply download the content onto your desktop, laptop, tablet or smartphone, depending on your preference. This allows you to start healing right away, even if you’re constantly on the go, as you can read through the program and follow the steps at your leisure, whenever and wherever you are. Huge bonus!As mentioned, the guide is backed by more than 35,000 hours of nutritional expertise, conducted by Linda Allen. She’s a certified Nutrition Specialist, Health Consultant, Medical Researcher and author. Her unique approach to treating Candida overgrowth has led her to being highly renowned within the holistic health industry. So, if there’s anyone you want to take advice from, it’s Linda.
DOI: 10.5517/ccdc.csd.cc2170s3
title: CCDC 1883584: Experimental Crystal Structure Determination

description: Related Article: Quentin Gaydon, Harrison Cassidy, Ohhyeon Kwon, Pierre-Louis Lagueux-Tremblay, D. Scott Bohle|2019|J.Mol.Struct.|1192|252|doi:10.1016/j.molstruc.2019.04.132
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: 10.5517/ccdc.csd.cc22454k
title: CCDC 1910627: Experimental Crystal Structure Determination

description: Related Article: A.P. Purdy, R.J. Butcher|2019|Acta Crystallogr.,Sect.E:Cryst.Commun.|75|714|doi:10.1107/S2056989019005310
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: 10.5517/ccdc.csd.cc224hzq
title: CCDC 1910963: Experimental Crystal Structure Determination

description: Related Article: E. Sylvester, M. McGovern, A. Young Lee, P. Nguyen, J. Park, J.B. Benedict|2019|Acta Crystallogr.,Sect.E:Cryst.Commun.|75|728|doi:10.1107/S2056989019005334
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: 10.5517/ccdc.csd.cc225nzx
title: CCDC 1912079: Experimental Crystal Structure Determination

description: Related Article: H. Wang, Z. Yin|2019|Acta Crystallogr.,Sect.E:Cryst.Commun.|75|711|doi:10.1107/S205698901900567X
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: 10.5517/ccdc.csd.cc22651j
title: CCDC 1912546: Experimental Crystal Structure Determination

description: Related Article: O.B.O. Moreira, M.C.R. Freitas, K.C. Souza, A.K. Jordão, J.A.L.C. Resende|2019|Acta Crystallogr.,Sect.E:Cryst.Commun.|75|738|doi:10.1107/S2056989019005711
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: 10.5517/ccdc.csd.cc226gj9
title: CCDC 1912840: Experimental Crystal Structure Determination

description: Related Article: G. Gokila, A.A. Thiruvalluvar, C. Ramachandra Raja|2019|IUCrData|4|x190593|doi:10.1107/S2414314619005935
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: 10.5517/ccdc.csd.cc226pbb
title: CCDC 1913051: Experimental Crystal Structure Determination

description: Related Article: N.K. Sebbar, B. Hni, T. Hökelek, A. Jaouhar, M. Labd Taha, J.T. Mague, E.M. Essassi|2019|Acta Crystallogr.,Sect.E:Cryst.Commun.|75|721|doi:10.1107/S2056989019005966
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: 10.25919/5ccd276b725c5
title: Parkes observations for project P970 semester 2018APRS_10

description: During the past 6 years, we at Parkes and collaborators at other radio telescopes have been remarkably successful at discovering millisecond pulsars (MSPs) associated with unidentified Fermi-LAT gamma-ray sources. Based on lessons learned, we here propose to carry out targeted searches with the new Ultra-wideband Low (UWL) receiver that will be installed next semester. The ultra-wide frequency coverage will enable us to detect MSPs with steep spectrum and avoid difficulties caused by interstellar scintillation and dispersive and scattering smearing. We propose to revisit highly ranked pulsar candidates that remain unidentified. Such a pilot survey will help us designing future searches of the coming 4FGL gamma-ray source catalog using the UWL. The overall time request is 23 hours on source, or 26 hours including overheads.
DOI: 10.21227/d4z8-p407
title: Audio Steganalysis Dataset

description: This is a dataset for audio steganalysis.
DOI: 10.5281/zenodo.2642214
title: Phylogeny of Cimicidae

description: Alignment file

Chronogramme under different phylogenetic assumptions

GBlock alignment tests, Bayesian analysis of individual gene trees, consenus tree, Maximum Likelihood tree
DOI: 10.5281/zenodo.2642215
title: Phylogeny of Cimicidae

description: Alignment file

Chronogramme under different phylogenetic assumptions

GBlock alignment tests, Bayesian analysis of individual gene trees, consenus tree, Maximum Likelihood tree