cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dissecting an intermediate-mass (IM) protostar: Chemical differentiation in IC1396N
Creators: name: Fuente, A.
name: Castro-Carrizo, A.
name: Alonso-Albi, T.
name: Beltran, M. T.
name: Neri, R.
name: Ceccarelli, C.
name: Lefloch, B.
name: Codella, C.
name: Caselli, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have carried out high-angular resolution (1.4") observations in the continuum at 3.1mm and in the N2H+ 1-0, CH3CN 5_k-4_k and 13CS 2-1 lines using the Plateau de Bure Interferometer (PdBI) towards the intermediate mass (IM) protostar IRAS21391+5802 (IC1396N). In addition, we have merged the PdBI images with previous BIMA (continuum data at 1.2mm and 3.1mm) and single-dish (N2H+ 1-0) data to have a comprehensive description of the region. The combination of our data with BIMA and 30m data show that the bipolar outflow associated has completely eroded the initial molecular globule. The 1.2mm and 3.1mm continuum emissions are extended along the outflow axis tracing the warm walls of the biconical cavity. Most of the molecular gas, however, is located in an elongated feature in the direction perpendicular to the outflow. A strong chemical differentiation is detected across the molecular toroid, with the N2H+ 1-0 emission absent in the inner region.This chemical differentiation can be understood in terms of the different gas kinetic temperature. The [CH3CN]/[N2H+] ratio increases by 5 orders of magnitude with gas temperature, for temperatures between 20K and 100K. The CH3CN abundance towards IRAM 2A, the most massive protostellar core, is similar to that found in hot corinos and lower than that expected towards IM and high mass hot cores. This could indicate that IRAM 2A is a low mass or at most Herbig Ae star (IRAM 2A) instead of the precursor of a massive Be star. Alternatively, the low CH3CN abundance could also be the consequence of IRAM 2A being a Class 0/I transition object which has already formed a small photodissociation region (PDR).
description: accepted A&A
Tensors, non-Gaussianities, and the future of potential reconstruction
Creators: name: Powell, Brian A.
name: Tzirakis, Konstantinos
name: Kinney, William H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present projections for reconstruction of the inflationary potential expected from ESA's upcoming Planck Surveyor CMB mission. We focus on the effects that tensor perturbations and the presence of non-Gaussianities have on reconstruction efforts in the context of non-canonical inflation models. We consider potential constraints for different combinations of detection/null-detection of tensors and non-Gaussianities. We perform Markov Chain Monte Carlo and flow analyses on a simulated Planck-precision data set to obtain constraints. We find that a failure to detect non-Gaussianities precludes a successful inversion of the primordial power spectrum, greatly affecting uncertainties, even in the presence of a tensor detection. In the absence of a tensor detection, while unable to determine the energy scale of inflation, an observable level of non-Gaussianities provides correlations between the errors of the potential parameters, suggesting that constraints might be improved for suitable combinations of parameters. Constraints are optimized for a positive detection of both tensors and non-Gaussianities.
description: 12 pages, 5 figures, LaTeX; V2: version submitted to JCAP
title: ÐÐ·Ð³Ð½Ð°Ð½Ð¸Ðµ Ð¼Ð¾ÑÐ¸ÑÐºÐ¾Ð² Ð¸Ð· ÐÑÐ¿Ð°Ð½Ð¸Ð¸ Ð² XVII Ð².
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¾Ð³Ð¶Ð°Ð½Ð¸Ð½Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÑÐ¿Ð°Ð½Ð¸Ñ
Ð¼Ð¾ÑÐ¸ÑÐºÐ¸
ÑÐµÐºÐ¾Ð½ÐºÐ¸ÑÑÐ°
Ð¸Ð½ÐºÐ²Ð¸Ð·Ð¸ÑÐ¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð·Ð³Ð½Ð°Ð½Ð¸Ñ Ð¼Ð¾ÑÐ¸ÑÐºÐ¾Ð² Ð¸Ð· ÐÑÐ¿Ð°Ð½Ð¸Ð¸ Ð² XVII Ð²ÐµÐºÐµ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ¸ÑÐºÐ¾Ð² â Ð¸ÑÐ¿Ð°Ð½ÑÐºÐ¸Ñ Ð¼Ð°Ð²ÑÐ¾Ð², Ð½Ð°ÑÐ¸Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾ Ð¾Ð±ÑÐ°ÑÐµÐ½Ð½ÑÑ Ð² ÑÑÐ¸ÑÑÐ¸Ð°Ð½ÑÑÐ²Ð¾ Ð² XVI Ð²ÐµÐºÐµ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð¸ Ð¿ÑÐµÐ´Ð¿Ð¾ÑÑÐ»ÐºÐ¸ Ð¸Ð·Ð³Ð½Ð°Ð½Ð¸Ñ Ð¼Ð¾ÑÐ¸ÑÐºÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¸Ð· ÑÐ°Ð¼ÑÑ ÑÑÐºÐ¸Ñ Ð¿ÑÐ¸Ð¼ÐµÑÐ¾Ð² Ð¿ÑÐ¸Ð½ÑÐ´Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð°ÑÐ¾Ð´Ð° Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¸ÑÑÐ¾ÑÐ¸Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ ÐÐ·Ð³Ð½Ð°Ð½Ð¸Ñ Ð´Ð»Ñ ÐÑÐ¿Ð°Ð½Ð¸Ð¸.
Additional file 3 of The predicting role of circulating tumor DNA landscape in gastric cancer patients treated with immune checkpoint inhibitors
Creators: name: Jin, Ying
name: Chen, Dong-Liang
name: Wang, Feng
name: Yang, Chao-pin
name: Chen, Xu-Xian
name: You, Jin-qi
name: Huang, Jin-Sheng
name: Shao, Yang
name: Zhu, Dong-Qin
name: Ouyang, Yu-Ming
name: Luo, Hui-Yan
name: Wang, Zhi-Qiang
name: Wang, Feng-Hua
name: Li, Yu-Hong
name: Xu, Rui-Hua
name: Zhang, Dong-Sheng
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 3: Figure S1. CONSORT diagram. CONSORT diagram of 46 patients enrolled and samples analyzed.
True ternary fission of superheavy nuclei
Creators: name: Zagrebaev, V. I.
name: Karpov, A. V.
name: Greiner, Walter
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We found that a true ternary fission with formation of a heavy third fragment (a new type of radioactivity) is quite possible for superheavy nuclei due to the strong shell effects leading to a three-body clusterization with the two doubly magic tin-like cores. The simplest way to discover this phenomenon in the decay of excited superheavy nuclei is a detection of two tin-like clusters with appropriate kinematics in low-energy collisions of medium mass nuclei with actinide targets. The three-body quasi-fission process could be even more pronounced for giant nuclear systems formed in collisions of heavy actinide nuclei. In this case a three-body clusterization might be proved experimentally by detection of two coincident lead-like fragments in low-energy U+U collisions.
description: 4 pages, 7 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÑÐµÐ¹ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐÐ­Ð¤Ð Ð¸Ð¼ÐµÐ½Ð¸ Ð.Ð. ÐÑÑÐµÐ¼Ð¾Ð²Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð¼Ð°ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð°
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸
economic efficiency
quality improvement
product quality

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ ÐÐÐÐ­Ð¤Ð Ð¸Ð¼ÐµÐ½Ð¸ Ð.Ð. ÐÑÑÐµÐ¼Ð¾Ð²Ð°. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÑÐµÐ¹ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ ÐÐÐÐ­Ð¤Ð Ð¸Ð¼ÐµÐ½Ð¸ Ð.Ð. ÐÑÑÐµÐ¼Ð¾Ð²Ð°. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¾ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐ Â«ÐÐÐÐ­Ð¤Ð Ð¸Ð¼ÐµÐ½Ð¸ Ð.Ð. ÐÑÑÐµÐ¼Ð¾Ð²Ð°Â». Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÑ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð½Ð° ÑÐ»ÑÑÑÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¸Ð·Ð³Ð¾ÑÐ°Ð²Ð»Ð¸Ð²Ð°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸.
description: The object of research is D.V. Efremov Institute of Electro physical Equipment. The purpose of work is development of product quality improvement by example of NIIEFA. During writing the graduation work there was research of current quality system in NIIEFA. As a result of research there were suggested the ways which are directed to improve quality of manufacturing products and increase in profits in NIIEFA.
Cribraria tenella Schrad.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Cribrariales
Cribrariaceae
Cribraria
Cribraria tenella

description: ● Cribraria cf. tenella Schrad.,
maigā lākturīte
- leg. M.Šlapakova-Pjankova, 22 Aug 2023, Čornaja p., on a decaying stump of Picea abies in a mixed forest, det. J. Kluša, 2023; (JK), one locality; differs from typical C. tenella by larger dictydine granules (basically 2-2.5 µm).
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
Additional file 6 of The predicting role of circulating tumor DNA landscape in gastric cancer patients treated with immune checkpoint inhibitors
Creators: name: Jin, Ying
name: Chen, Dong-Liang
name: Wang, Feng
name: Yang, Chao-pin
name: Chen, Xu-Xian
name: You, Jin-qi
name: Huang, Jin-Sheng
name: Shao, Yang
name: Zhu, Dong-Qin
name: Ouyang, Yu-Ming
name: Luo, Hui-Yan
name: Wang, Zhi-Qiang
name: Wang, Feng-Hua
name: Li, Yu-Hong
name: Xu, Rui-Hua
name: Zhang, Dong-Sheng
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 6: Figure S4. The characteristics of 38 patients with available baseline plasma samples.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð¿ÑÐ¾Ð²ÐµÑÐ¾Ðº Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð²ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ ÐÐÐ¤Ð (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ¤ÐÐ¡ Ð Ð¾ÑÑÐ¸Ð¸ â 22 Ð¿Ð¾ Ð¡ÐÐ±)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð½Ð°Ð»Ð¾Ð³ Ð½Ð° Ð´Ð¾Ñ Ð¾Ð´Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸Ñ
Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÐµ Ð²ÑÑÐµÑÑ
Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÐ¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
ÐºÐ°Ð¼ÐµÑÐ°Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ°
Ð²ÑÐµÐ·Ð´Ð½Ð°Ñ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐµÐ¶ÑÐ°Ð¹Ð¾Ð½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¿ÐµÐºÑÐ¸Ð¸ Ð¤ÐÐ¡ Ð Ð¾ÑÑÐ¸Ð¸ â 22 Ð¿Ð¾ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ñ, ÐµÐµ ÑÑÑÑÐºÑÑÑÐ° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ½ÐºÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ ÑÐ±Ð¾ÑÑ Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð²ÑÑÐµÑÐ¾Ð² Ð² ÐÐ Ð¤ÐÐ¡ Ð Ð¾ÑÑÐ¸Ð¸ â22 Ð¿Ð¾ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ñ. Ð¢Ð°ÐºÐ¶Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð°Ñ Ð±Ð°Ð·Ð° Ð¿Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð²ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ ÐÐÐ¤Ð. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð´Ð°Ð½Ð½ÑÐµ Ð¿Ð¾ ÑÐ¾ÑÑÑ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð²ÑÑÐµÑÐ¾Ð² Ð² ÐÑÐ°ÑÐ½Ð¾ÑÐµÐ»ÑÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ ÑÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÐ°Ð¼ÐµÑÐ°Ð»ÑÐ½ÑÑ Ð¸ Ð²ÑÐµÐ·Ð´Ð½ÑÑ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð¿ÑÐ¾Ð²ÐµÑÐ¾Ðº Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ Ð¿ÑÐ¾Ð²ÐµÑÐ¾Ðº.
Additional file 4 of The predicting role of circulating tumor DNA landscape in gastric cancer patients treated with immune checkpoint inhibitors
Creators: name: Jin, Ying
name: Chen, Dong-Liang
name: Wang, Feng
name: Yang, Chao-pin
name: Chen, Xu-Xian
name: You, Jin-qi
name: Huang, Jin-Sheng
name: Shao, Yang
name: Zhu, Dong-Qin
name: Ouyang, Yu-Ming
name: Luo, Hui-Yan
name: Wang, Zhi-Qiang
name: Wang, Feng-Hua
name: Li, Yu-Hong
name: Xu, Rui-Hua
name: Zhang, Dong-Sheng
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 4: Figure S2. 425-gene NGS panel that used for plasma circulating tumor DNA sequencing and tissue tumor DNA sequencing.
title: ÐÐ¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ² Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ°Ð¼Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡Ð¾Ð»Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÐÐ¾Ð»Ð¸Ð¼ÐµÑÑ
ÐÐ¾Ð»Ð¸Ð¼ÐµÑÑ Ð²Ð¾Ð´Ð¾ÑÐ°ÑÑÐ²Ð¾ÑÐ¸Ð¼ÑÐµ

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐ¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ² Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ°Ð¼Ð¸Â» Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 140400 Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â» Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Â«Ð¤Ð¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð¾Ð²ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ðµ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸Â», Â«ÐÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ°Ñ Ð¸ Ð±Ð¸Ð¾Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», Â«Ð¤Ð¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ», Â«Ð¤Ð¸Ð·Ð¸ÐºÐ° Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹Â». ÐÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐ¸Ð½ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÐ¼ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ°Ð¼, Ð¼ÐµÑÐ¾Ð´Ð°Ð¼ Ð¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ, ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼, ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ²ÑÐ·Ð¸ Ð¼ÐµÐ¶Ð´Ñ ÑÑÑÑÐºÑÑÑÐ¾Ð¹ Ð¸ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑÑ, Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¸Ñ Ð² Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ðµ Ð¸ Ð² Ð½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¼ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ðµ. ÐÐ¿Ð¸ÑÐ°Ð½Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¸ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð²Ð¾Ð´Ð¾ÑÐ°ÑÑÐ²Ð¾ÑÐ¸Ð¼ÑÑ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ¾Ð² â Ð½Ð¾ÑÐ¸ÑÐµÐ»ÐµÐ¹ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÑÐµÑÑÐ² (ÑÐµÐ°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½ÑÐµ ÑÐ¾Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ N-Ð²Ð¸Ð½Ð¸Ð»Ð¿Ð¸ÑÑÐ¾Ð»Ð¸Ð´Ð¾Ð½Ð°, N-(2-Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð¿ÑÐ¾Ð¿Ð¸Ð»)Ð¼ÐµÑÐ°ÐºÑÐ¸Ð»Ð°Ð¼Ð¸Ð´Ð° Ð¸ Ð´Ñ.). Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð´Ð¾ÑÐ°ÑÑÐ²Ð¾ÑÐ¸Ð¼ÑÐµ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÐµ Ð²ÐµÑÐµÑÑÐ²Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ»Ð°ÑÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ ÐºÐ¾ÑÐ¿ÑÑÐºÑÐ»ÑÑÐ½ÑÐµ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½ÑÐµ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÑ (Ð¼Ð¸ÐºÑÐ¾ÑÐ°ÑÑÐ¸ÑÑ), ÑÐ°ÑÑÐ²Ð¾ÑÑÑÑÐ¸ÐµÑÑ Ð¸Ð»Ð¸ ÑÐ¸ÑÐºÑÐ»Ð¸ÑÑÑÑÐ¸Ðµ Ð² Ð¶Ð¸Ð²Ð¾Ð¼ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ðµ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð² ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ Ð±Ð¸Ð¾Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¸Ð¸.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
The Runaway White Dwarf LP400-22 Has a Companion
Creators: name: Kilic, Mukremin
name: Brown, Warren R.
name: Prieto, Carlos Allende
name: Swift, B.
name: Kenyon, S. J.
name: Liebert, J.
name: Agueros, M. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the detection of a radial velocity companion to the extremely low mass white dwarf LP400-22. The radial velocity of the white dwarf shows variations with a semi-amplitude of 119 km/s and a 0.98776 day period, which implies a companion mass of M > 0.37 Msun. The optical photometry rules out a main sequence companion. Thus the invisible companion is another white dwarf or a neutron star. Using proper motion measurements and the radial velocity of the binary system, we find that it has an unusual Galactic orbit. LP400-22 is moving away from the Galactic center with a velocity of 396 km/s, which is very difficult to explain by supernova runaway ejection mechanisms. Dynamical interactions with a massive black hole like that in the Galactic center can in principle explain its peculiar velocity, if the progenitor was a triple star system comprised of a close binary and a distant tertiary companion. Until better proper motions become available, we consider LP400-22 to be most likely a halo star with a very unusual orbit.
description: ApJ Letters, in press
title: Ð£ÑÐµÑ Ð¸ Ð°ÑÐ´Ð¸Ñ Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð¸Ð»Ð¸Ð¼Ð¾Ð½Ð¾Ð²Ð°, ÐÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÐµÑ Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
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description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÑÐµÑÐ° Ð¸ Ð°ÑÐ´Ð¸ÑÐ° Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐÐÐ Â«ÐÐ°Ð½ ÐÐµÑ ÐÐ»Ð¸ÑÑ Ð¢ÑÐ°Ð½ÑÐ¿Ð¾ÑÑ Ð¸ Ð¡ÐµÑÐ²Ð¸ÑÐ¸Ð· Ð Ð¾ÑÂ» Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÐµÐ³Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ
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Additional file 5 of The predicting role of circulating tumor DNA landscape in gastric cancer patients treated with immune checkpoint inhibitors
Creators: name: Jin, Ying
name: Chen, Dong-Liang
name: Wang, Feng
name: Yang, Chao-pin
name: Chen, Xu-Xian
name: You, Jin-qi
name: Huang, Jin-Sheng
name: Shao, Yang
name: Zhu, Dong-Qin
name: Ouyang, Yu-Ming
name: Luo, Hui-Yan
name: Wang, Zhi-Qiang
name: Wang, Feng-Hua
name: Li, Yu-Hong
name: Xu, Rui-Hua
name: Zhang, Dong-Sheng
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 5: Figure S3. The landscape of high-frequency genomic alterations detected in 38 tissue samples and 38 baseline plasma samples. High-frequency means genomic alterations detected in tissue or baseline plasma > 5%.
h-> mu^+ mu^- via tth Production at the LHC
Creators: name: Su, Shufang
name: Thomas, Brooks
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work, we examine the process at the LHC in which a Higgs boson is produced in association with a t t-bar pair and subsequently decays to a pair of muons. We show that the statistical significance for the discovery of a light, Standard-Model Higgs boson with a mass around 120 GeV in this channel is comparable to those for other processes (gluon fusion, weak-boson fusion) in which the Higgs decays to a muon pair. Combining all three of these channels, we show that evidence for a Higgs boson with a mass in the range 115 GeV < m_h < 130 GeV could be obtained at the 3 sigma significance level with an integrated luminosity of 300 fb^{-1}. We also calculate the enhancement factor to the cross-section that would be needed to discover a non-standard Higgs boson in this channel.
description: 11 pages, ReVTeX, 1 figure, 5 tables
Bolometric Light Curves for 33 Type II-Plateau Supernovae
Creators: name: Bersten, Melina C.
name: Hamuy, Mario
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Using data of three well-observed type-II plateau supernovae (SNe II-P), SNe 1987A, 1999em and 2003hn; and two atmosphere models by Eastman et al. (1996) and Dessart & Hillier (2005b) we derive calibrations for bolometric corrections and effective temperature from BVI photometry. The typical scatter of the bolometric correction is 0.11 mag. With these results we obtain bolometric light curves and effective temperature evolution for a sample of 33 SNe II-P. The SN sample shows a range of 1 dex in plateau luminosity and plateau durations from 75 to 120 days. Comparing the shape of the transition between the plateau and the radioactive tail, we find that the size of the drop is in the range of 0.8 to 1.12 dex.
description: Accepted for publication in the Astrophysical Journal
Energy-efficient acceleration for autonomous robotics
Creators: name: Shah, Deval
Publisher: name: University of British Columbia
Year: 2024

description: Autonomous robots have great potential to improve our day-to-day lives. Hence, their demand for real-time and safety-critical tasks is increasing, including medical care, home assistance, and autonomous driving. An autonomous robot system consists of several latency-sensitive computation tasks. Further, a crucial aspect of computing for autonomous robots is energy efficiency, as computation can contribute to a significant fraction of the total power consumption. With the recent advancements in machine learning, algorithms for autonomous robots’ operation are explored extensively at the software level. However, their architectural implications are not explored in detail. This thesis explores algorithm and hardware design for energy-efficient computation acceleration of perception and planning tasks in autonomous robotics. It first proposes a motion planning hardware accelerator, MPAccel. MPAccel consists of a Spatially-Aware Scheduler and Collision Prediction Units. The proposed scheduler and predictor exploit the physical-spatial locality of a robot's positions in the environment to reduce redundant computation. Further, MPAccel proposes a hierarchical collision detection approach and corresponding hardware accelerator. MPAccel enables real-time sampling-based motion planning for a 7-DOF robotic arm with less than 1ms latency and 3.5W power consumption. The second part of the thesis focuses on regression networks, as they are used in autonomous robot perception and planning. It explores the design space of regression by binary classification and proposes Binary-Encoded Labels (BEL). This thesis further analyzes the properties of suitable label encodings and proposes manually designed label encodings. It also proposes an end-to-end training approach to learn label encodings and network parameters together for a given task. BEL reduces regression error by 10.9% compared to direct regression, enabling the use of smaller and/or sparser networks for compute- and energy-efficient execution. Further, BEL-based regression networks are explored for smaller and sparser neural motion planners, reducing neural planning computation by a factor of 11.4x. The third part of the thesis explores the impact of soft errors on collision detection hardware accelerators in motion planning. It proposes an application-specific reliability metric, Collision Exposure Factor, and demonstrates its use for faster fault characterization and low-overhead selective error mitigation.
Oxygen isotopic ratios in cool R Coronae Borealis stars
Creators: name: Garcia-Hernandez, D. Anibal
name: Lambert, David L.
name: Rao, N. Kameswara
name: Hinkle, Ken H.
name: Eriksson, Kjell
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate the relationship between R Coronae Borealis (RCB) stars and hydrogen-deficient carbon (HdC) stars by measuring precise 16O/18O ratios for five cool RCB stars. The 16O/18O ratios are derived by spectrum synthesis from high-resolution (R=50,000) K-band spectra. Lower limits to the 16O/17O and 14N/15}N ratios as well as Na and S abundances (when possible) are also given. RCB stars in our sample generally display less 18O than HdC stars - the derived 16O/18O ratios range from 3 to 20. The only exception is the RCB star WX CrA, which seems to be a HdC-like star with 16O/18O=0.3. Our result of a higher 16O/18O ratio for the RCB stars must be accounted for by a theory of the formation and evolution of HdC and RCB stars. We speculate that a late dredge-up of products of He-burning, principally 12C and 16O, may convert a 18O-rich HdC star into a 18O-poor RCB star as the H-deficient star begins its final evolution from a cool supergiant to the top of the white dwarf cooling track.
description: Accepted for publication in the Astrophysical Journal; 21 pages, 3 Tables, 11 Figures
Correlation functions in the non-relativistic AdS/CFT correspondence
Creators: name: Fuertes, Carlos A.
name: Moroz, Sergej
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We study the correlation functions of scalar operators in the theory defined as the holographic dual of the Schroedinger background with dynamical exponent z=2 at zero temperature and zero chemical potential. We offer a closed expression of the correlation functions at tree level in terms of Fourier transforms of the corresponding n-point functions computed from pure AdS in the lightcone frame. At the loop level this mapping does not hold and one has to use the full Schroedinger background, after proper regularization. We explicitly compute the 3-point function comparing it with the specific 3-point function of the non-relativistic theory of cold atoms at unitarity. We find agreement of both 3-point functions, including the part not fixed by the symmetry, up to an overall normalization constant.
description: 32 pages, 7 figures; v2: typos corrected, references added and additional discussion about the case of compact number-direction, includes new appendix with the computations of the 2 and 3 point function for the compact number-direction case. The general results remain the same. Version published in Phys.Rev.D
title: Interactions between radiation, clouds and convective self-aggregation in idealised numerical simulations
Creators: name: Pope, Kieran Nicholas
Publisher: name: University of Reading
Year: 2023

description: Tropical weather is dominated by convection which is organised across a wide range of spatial and temporal scales. The degree of convective organisation has important consequences for weather and climate. The uncertainty in the response of convective organisation to a warming climate is one of the largest sources of uncertainty in climate sensitivity estimates. Self-aggregation is the process in which convection spontaneously clusters despite homogeneous initial conditions and forcing. It has been the focus of many recent studies because of its implications for real world weather and climate. Cloud-radiation interactions have been shown to be crucial drivers and maintainers of aggregation. Yet there remains uncertainty in their role in self-aggregation. In this thesis, we develop a framework to study aggregation and quantify the contributions of radiative interactions with different cloud types to aggregation. We study models that form part of the RadiativeConvective Equilibrium Model Intercomparison Project, comparing models with explicit and parameterised convection across a range of sea surface temperatures (SSTs). We find that longwave interactions with high-topped cloud and clear regions, as well as shortwave interactions with water vapour are key drivers and/or maintainers of aggregation. Their influence on aggregation tends to decrease with SST, but the rate of aggregation remains similar. We find the strength of these interactions strongly correlates with the rate of aggregation in parameterised convection simulations, yet the rate of aggregation in explicit simulations is more strongly influenced by circulations. Parameterised convection simulations often have stronger longwave interactions with high-topped cloud than explicit simulations, resulting in faster aggregation. We find that by artificially reducing this longwave feedback in parameterised simulations, the aggregation behaves more similarly to explicit simulations. This highlights that global weather and climate models may be able to model the effects of real-world aggregation more accurately given an accurate representation of cloud-radiation interactions.
Development of Legal Measures to Regulate Online Advertising of High Fat, Sugar or Sodium Foods and Beverages for Protecting Children and Youth
Creators: name: Keovalin Torpanyacharn
Publisher: name: International Journal of Crime, Law and Social Issues
Year: 2021
Subjects: Consumer Protection Law
High Fat
Sugar and Sodium Food and Beverage
Advertising
Children and Youth

description: International Journal of Crime, Law and Social Issues, 8, 2, 21-31
On the Origin of Chaos in Autonomous Boolean Networks
Creators: name: Cavalcante, Hugo L. D. de S.
name: Gauthier, Daniel J.
name: Socolar, Joshua E. S.
name: Zhang, Rui
Publisher: name: arXiv
Year: 2009
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: FOS: Physical sciences

description: We undertake a systematic study of the dynamics of Boolean networks to determine the origin of chaos observed in recent experiments. Networks with nodes consisting of ideal logic gates are known to display either steady states, periodic behavior, or an ultraviolet catastrophe where the number of logic-transition events circulating in the network per unit time grows as a power-law. In an experiment, non-ideal behavior of the logic gates prevents the ultraviolet catastrophe and may lead to deterministic chaos. We identify certain non-ideal features of real logic gates that enable chaos in experimental networks. We find that short-pulse rejection and the asymmetry between the logic states tends to engender periodic behavior, at least for the simplest networks. On the other hand, we find that a memory effect termed "degradation" can generate chaos. Our results strongly suggest that deterministic chaos can be expected in a large class of experimental Boolean-like networks. Such devices may find application in a variety of technologies requiring fast complex waveforms or flat power spectra, and can be used as a test-bed for fundamental studies of real-world Boolean-like networks.
description: 18 pages, 10 figures, submitted to Delayed Complex Systems International Workshop 2009
Individual and combined relationship of body mass index and waist-to-hip ratio with mortality among patients receiving hemodialysis
Creators: name: Yang, Yaya
name: Luo, Pei
name: Qin, Xianhui
name: Li, Yumin
name: Kong, Yaozhong
name: Wan, Qijun
name: Wang, Qi
name: Huang, Sheng
name: Liu, Yan
name: Liu, Aiqun
name: Liu, Fanna
name: Yang, Shenglin
name: Lu, Yongxin
name: Zhao, Yanhong
name: Chen, Junzhi
name: Lei, Zihan
name: He, Yanhuan
name: Huang, Yan
name: Lin, Zizhen
name: Wang, Jieyu
name: Li, Youbao
name: Liang, Min
Publisher: name: figshare
Year: 2021
Subjects: Diseases

description: Supplementary material for article entitled "Individual and combined relationship of body mass index and waist-to-hip ratio with mortality among patients receiving hemodialysis".
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title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¤ÐµÑÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð ÐµÐ³ÑÐ»ÑÑÐ¾ÑÑ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÐºÑÐ°ÑÐºÐ¾Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ³ÑÐ»ÑÑÐ¾ÑÐ¾Ð² Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ. ÐÐ»Ñ Ð±ÑÑÑÑÐ¾Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ, ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐµÐ³ÑÐ»ÑÑÐ¾Ñ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð¸Ñ ÑÐ¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð° Ð°Ð´Ð°Ð¿ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð°, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ ÐµÐµ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ, Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑÐ¸Ðµ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾ÑÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ.
A cool starspot or a second transiting planet in the TrES-1 system?
Creators: name: Rabus, M.
name: Alonso, R.
name: Belmonte, J. A.
name: Deeg, H. J.
name: Gilliland, R. L.
name: Villa, J. M. Almenara
name: Brown, T. M.
name: Charbonneau, D.
name: Mandushev, G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the origin of a flux increase found during a transit of TrES-1, observed with the HST. This feature in the HST light curve cannot be attributed to noise and is supposedly a dark area on the stellar surface of the host star eclipsed by TrES-1 during its transit. We investigate the likeliness of two possible hypothesis for its origin: A starspot or a second transiting planet. We made use of several transit observations of TrES-1 from space with the HST and from ground with the IAC-80 telescope. On the basis of these observations we did a statistical study of flux variations in each of the observed events, to investigate if similar flux increases are present in other parts of the data set. The HST observation presents a single clear flux rise during a transit whereas the ground observations led to the detection of two such events but with low significance. In the case of having observed a starspot in the HST data, assuming a central impact between the spot and TrES-1, we would obtain a lower limit for the spot radius of 42000 km. For this radius the spot temperature would be 4690 K, 560 K lower then the stellar surface of 5250 K. For a putative second transiting planet we can set a lower limit for its radius at 0.37 R$_J$ and for periods of less than 10.5 days, we can set an upper limit at 0.72 R$_J$. Assuming a conventional interpretation, then this HST observation constitutes the detection of a starspot. Alternatively, this flux rise might also be caused by an additional transiting planet. The true nature of the origin can be revealed if a wavelength dependency of the flux rise can be shown or discarded with a higher certainty. Additionally, the presence of a second planet can also be detected by radial velocity measurements.
description: 8 pages, 6 figures, accepted for publication in A&A
title: ÐÐµÑ Ð°Ð½Ð¸ÐºÐ° Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸ Ð¸ Ð³Ð°Ð·Ð°
title: Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÐµÑÐ³Ð°ÑÐµÐ², ÐÐ¾ÑÐ¸Ñ
name: ÐÐ°Ð¹ÑÐµÐ², ÐÐ»ÐµÐ³
name: ÐÐ¾Ð¶ÐµÐ²Ð½Ð¸ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
name: ÐÐ°ÐºÑÐ±ÐµÑÐ³, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¾ÐºÑÐ¸Ð¾Ð½Ð¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
name: ÐÑÐ»Ð¾Ð², ÐÑÑÐµÑÐ»Ð°Ð²
name: Ð§ÐµÑÐ½ÑÑÐµÐ², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 1997
Subjects: ÐÐ¸Ð´ÑÐ¾Ð¼ÐµÑ Ð°Ð½Ð¸ÐºÐ°

description: ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐµÐ¼Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÐºÑÑÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¸ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸ Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð², Ð¿Ð¾ÑÑÐ½ÑÐµÑÑÑ Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾Â» ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð²ÑÐµÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ Ð²ÐµÑÐµÑÐ½ÐµÐ³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ° Â«ÐÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸ Ð¸ Ð³Ð°Ð·Ð°Â».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
RUBOB CHOLG'USI: AN'ANAVIY MUSIQA ASBOBI SIFATIDA O'RNI
Creators: name: Saitov, Jaqsılıq
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolada O‘zbek xalqining an’anaviy torli cholg‘ularidan biri – rubobning kelib chiqishi, tuzilishi, ijrochilik an’analari hamda hozirgi davrdagi ahamiyati yoritiladi. Rubobning shakllanish tarixi, turli mintaqalar kesimidagi farqlari va yosh avlod orasidagi o‘rni ilmiy manbalar, sahna ijrochiligi va amaliy kuzatuvlar asosida tahlil qilinadi. Maqola etnomusikologik yondashuv asosida yozilgan bo‘lib, rubobning milliy musiqa merosidagi o‘rni haqida ilmiy xulosalar beriladi.
Role of surface states in the Casimir force between semiconducting films
Creators: name: Govoni, Marco
name: Calandra, Carlo
name: Benassi, Andrea
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We present results of first principle calculations of the Casimir force between Si films of nanometric size, which show that it depends significantly upon the configuration of the surface atoms, and give evidence of the importance of surface states.
description: to be published on J.Phys.A
An analysis of the transit times of CoRoT-1b
Creators: name: Bean, Jacob L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: I report the results from a study of the transit times for CoRoT-1b, which was one of the first planets discovered by CoRoT. Analysis of the pipeline reduced CoRoT light curve yields a new determination of the physical and orbital parameters of planet and star, along with 35 individual transit times at a typical precision of 36 s. I estimate a planet-to-star radii ratio of 0.1433 +/- 0.0010, a ratio of the planet's orbital semimajor axis to the host star radius of 4.751 +/- 0.045, and an orbital inclination for the planet of 83.88 +/- 0.29 deg. The observed transit times are consistent with CoRoT-1b having a constant period and there is no evidence of an additional planet in the system. I use the observed constancy of the transit times to set limits on the mass of a hypothetical additional planet in a nearby, stable orbit. I ascertain that the most stringent limits (4 M_earth at 3 sigma confidence) can be placed on planets residing in a 1:2 mean motion resonance with the transiting planet. In contrast, the data yield less stringent limits on planets near a 1:3 mean motion resonance (5 M_jup at 3 sigma confidence) than in the surrounding parameter space. In addition, I use a simulation to investigate what sensitivity to additional planets could be obtained from the analysis of data measured for a similar system during a CoRoT long run (100 sequential transit times). I find that for such a scenario, planets with masses greater than twice that of Mars (0.2 M_earth) in the 1:2 mean motion resonance would cause high-significance transit time deviations. Therefore, such planets could be detected or ruled out using CoRoT long run data. I conclude that CoRoT data will indeed be very useful for searching for planets with the transit timing method.
description: accepted for publication in A&A; v2 replaces with accepted version
title: Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. Ð§. 3
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº ÑÑÑÐ´Ð¾Ð² Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸
titleType: Subtitle
Creators: name: "Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2019; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð½Ð°ÑÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐ±Ð»Ð¸ÐºÑÑÑÑÑ ÑÑÐ°ÑÑÐ¸ Ð¿Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ð¼ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð², Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°ÑÐµÐ´Ð°Ð½Ð¸ÑÑ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ,
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸Â». Ð¡ÑÐ°ÑÑÐ¸ Ð¾ÑÑÐ°Ð¶Ð°ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸, Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸, ÑÐµÑÑÑÑÐºÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½Ð° Ð¼Ð¸ÐºÑÐ¾- Ð¸ Ð¼Ð°ÐºÑÐ¾ÑÑÐ¾Ð²Ð½ÑÑ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ¾Ð¼.
A Method for Evaluating Supply Response to Price Underwriting
Creators: name: Fraser, R. W.
name: Fraser, R. W.
Publisher: name: Unknown
Year: 1988
Subjects: Demand and Price Analysis

description: This paper presents a method for evaluating the supply response of individual producers to a price underwriting scheme. The method includes precise formulae to take account of the impact of price underwriting on the producer's uncertain conditions. The Australian Wheat Board's Guaranteed Minimum Price Scheme is taken as a specific example of price underwriting in practice. Results show the scheme to lead to only relatively small supply responses. The paper also demonstrates the impact on producer behaviour of an increase in price uncertainty in the presence of an underwriting scheme.
Repurposing Itraconazole as an Adjuvant for the Treatment of Glioblastoma Multiforme
Creators: name: Saylan, Demet
Publisher: name: University of Leicester
Year: 2022
Subjects: Uncategorized

description: Glioblastoma multiforme (GBM) is one of the most aggressive human cancers, with a poor prognosis. Despite recent advances in the understanding of GBM's molecular biology, patient outcome continues to be poor due to the disease's incurable, aggressive, and recurrent nature. As a result, novel therapeutic strategies for the management of GBM patients are urgently needed. Itraconazole (ITC), a systemic antifungal, is a key regulator of hedgehog (HH) signalling, which is frequently deregulated in GBM. Because of its inhibitory effects on cell proliferation and tumour angiogenesis, ITC has been identified as a novel potential anticancer agent and is herein investigated in the context of GBM.In the present study, cell viability and reproductive integrity of GBM cells were assessed by AlamarBlue cell viability and clonogenic assays. Spheroid growth and relative colony cell growth were assessed by spheroid and associated absorbance reading assays. DNA damage levels and cell cycle distribution of the GBM cells were assessed by single cell gel electrophoresis (COMET) and flow cytometry, respectively, and O6-methylguanine DNA methyltransferase (MGMT) and HH protein levels were assessed by western blot analysis. Using these techniques we show that ITC, both alone and in combination treatments, inhibits GBM cell and spheroid growth in vitro, increased IR-induced DNA damage and caused G1 cell cycle arrest. Furthermore, ITC treatment decreased the levels of HH signalling pathway proteins sonic hedgehog (SHH) and smoothened (SMO). Together, these findings indicate that ITC inhibition of HH signalling pathway may increase TMZ, radiation and radiochemotherapy (RCT) responses and so serve as a potential adjunct to RCT in the management of GBM.
Local and global statistical distances are equivalent on pure states
Creators: name: Cohen, Scott M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The statistical distance between pure quantum states is obtained by finding a measurement that is optimal in a sense defined by Wootters. As such, one may expect that the statistical distance will turn out to be different if the set of possible measurements is restricted in some way. It nonetheless turns out that if the restriction is to local operations and classical communication (LOCC) on any multipartite system, then the statistical distance is the same as it is without restriction, being equal to the angle between the states in Hilbert space.
description: 5 pages, comments welcome
MPEC 2023-K34 : 2023 JP4
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 JP4

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
title: Reflections on the Social History of Al Muwaij'ei Oasis in the Mid-20th Century/ Shamsa Mohamed Al-Dhahiri.
Creators: name: Al Dhahiri, Shamsa Hamad
Publisher: name: National Library and Archives
Year: 2015
Subjects: Khalifa bin Zayed Al Nahyan, - HH The First, 1855-1945
Al-Muwayjiʻī,Oasis-Al Ain (Abu Dhabi) - History - 20th century
Al Ain (Abu Dhabi) - Social conditions - 20th century

Muwaij'es is a patch of productive land in the extreme west of the Al-Ain Oases in thus part of Al-Ain city. It was virtually a farming estate owned by the Al-Nahyan ruling family and had later developed into their main sphere of influence in the eastern region of the Abu Dhabi Emirate. It was inhabited due to its plentiful water, its beautiful atmosphere, and its central location within the agricultural estates of Sheikh Khalifa Bin Zayed I (1855-1945), eldest son of the rule of Emirate of Abu Dhabi, Sheikh Zayed Bin Khalifa Al-Nahyan (1855-1909), which extended from Al-Mo'tarid oasis to Al-Mas'oudi on the northern edge of Al-Ain. Sheikh Khalifa Bin Zayed made Muwaij'ei a summer resort for himself and his followers.