cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of Landscape and climatic features drive genetic differentiation processes in a South American coastal plant
Creators: name: Silva-Arias, Gustavo A.
name: Caballero-Villalobos, Lina
name: Giudicelli, Giovanna C.
name: Freitas, Loreta B.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Ecology

description: Additional file 1: Figure S1. Observed vs. expected heterozygosity for each locus. Figure S2. (A) Plots of the best K estimates for Structure results. (B) Plots of the mean and standard deviation of the deviance information criterion (DIC) obtained for each maxK assessed with TESS. Figure S3. Bar plots of the individual membership for each genetic cluster obtained with Structure. White dashed lines separate populations, and names are indicated on the figure top side. Figure S4. The plot of Bayesian information criterion (BIC) values obtained for each K number assessed using the multivariate method Discriminant Analyses of Principal Components. Figure S5. Graphical representation of the four coalescent migration models tested in Migrate-N for Calibrachoa heterophylla. (A) Source-sink from inland; (B) Source-sink from the west; (C) Step-stone from inland; (D) Step-stone from coast. Figure S6. Graphical representation of the raster layers used to calculate the connectivity values in topographic tests (A) Continuous model; (B) Water bodies model. Table S1. Migration estimates obtained with three independent runs of BAYESASS. The values indicate the estimated posterior mean effective migration rate per generation [the fraction of individuals in population i (rows) that are migrants derived from population j (columns)], and the numbers in parentheses show the standard deviation. Bold values indicate the diagonal (intra-population estimates), and red values indicate the highest migration estimates (those with above zero 95% confidence intervals).
Detection of 15NH2D in dense cores: A new tool for measuring the 14N/15N ratio in the cold ISM
Creators: name: Gerin, Maryvonne
name: Marcelino, Nuria
name: Biver, Nicolas
name: Roueff, Evelyne
name: Coudert, Laurent H.
name: Elkeurti, Mohamed
name: Lis, Dariucz C.
name: Bockelée-Morvan, Dominique
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Ammonia is one of the best tracers of cold dense cores. It is also a minor constituent of interstellar ices and, as such, one of the important nitrogen reservoirs in the protosolar nebula, together with the gas phase nitrogen, in the form of N2 and N. An important diagnostic of the various nitrogen sources and reservoirs of nitrogen in the Solar System is the 14N/15N isotopic ratio. While good data exist for the Solar System, corresponding measurements in the interstellar medium are scarce and of low quality. Following the successful detection of the singly, doubly, and triply deuterated isotopologues of ammonia, we have searched for 15NH2D in dense cores, as a new tool for investigating the 14N/15N ratio in dense molecular gas. With the IRAM-30m telescope, we have obtained deep integrations of the ortho 15NH2D (1(1,1)-1(0,1)) line at 86.4 GHz, simultaneously with the corresponding ortho NH2D line at 85.9 GHz. o-15NH2D is detected in Barnard-1b, NGC1333-DCO+, and L1689N, while we obtained upper limits towards LDN1544 and NGC1333-IRAS4A, and a tentative detection towards L134N(S). The 14N/15N abundance ratio in NH2D ranges between 350 and 850, similar to the protosolar value of ~ 424, and likely higher than the terrestrial ratio of 270.
title: ÐÐµÑÐµÐ³Ð¾Ð·Ð°ÑÐ¸ÑÐ½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¿ÐµÑÐµÑ Ð¾Ð´Ð¾Ð² ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð² Ð² ÐÐµÑÐ¾ÑÑÐºÐ¾Ð¼ Ð¼Ð¾ÑÐµ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
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Year: 2017
Subjects: ÐÐµÑÐµÐ³Ð¾ÑÐºÑÐµÐ¿Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ
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description: Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð·Ð°ÑÐ¸ÑÑ ÑÑÐ°ÑÑÐºÐ° Ð±ÐµÑÐµÐ³Ð¾Ð²Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ Ð² Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð¾Ñ ÑÐ°Ð·Ð¼ÑÐ²Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐÐ Mike21. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð¹ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÑÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑÑ, Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð·Ð° Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÑ Ð±ÐµÑÐµÐ³Ð¾Ð² (Ð±ÐµÑÐµÐ³Ð¾Ð²ÑÑ ÑÑÐ¾Ð·Ð¸Ñ). ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð±ÐµÑÐµÐ³Ð¾Ð·Ð°ÑÐ¸ÑÐ½Ð¾Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð² ÑÐ°Ð¹Ð¾Ð½Ðµ Ð¿Ð¾Ð»ÑÐ¾ÑÑÑÐ¾Ð²Ð° ÐÐµÐ´ÑÐ½ÑÐºÐ¸Ð¹ Ð·Ð°Ð²Ð¾ÑÐ¾Ñ, ÐÐ°ÑÐ°Ð½Ð´ÐµÐ¹, ÐÐµÑÐ¾ÑÑÐºÐ¾Ðµ Ð¼Ð¾ÑÐµ, Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½Ð¾Ðµ Ð´Ð»Ñ Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¿ÐµÑÐµÑÐ¾Ð´Ð¾Ð² ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¸ÑÐ¾Ð´Ð½ÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð², Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»Ð¸Ð²Ð°ÑÑÐ¸Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÑ Ð±ÐµÑÐµÐ³Ð¾Ð²Ð¾Ð¹ Ð·Ð¾Ð½Ñ Ð² ÐÑÐºÑÐ¸ÐºÐµ, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð±ÑÐ»Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹, ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð»ÑÐ»Ð°ÑÑ Ð² Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð±ÐµÑÐµÐ³Ð¾Ð²Ð¾Ð¹ Ð·Ð¾Ð½Ñ ÐÐ°ÑÐ°Ð½Ð´ÐµÐ¹ÑÐºÐ¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ°. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð±ÐµÑÐµÐ³Ð¾Ð·Ð°ÑÐ¸ÑÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð² ÑÐ°Ð¹Ð¾Ð½Ð°Ñ ÐÑÐºÑÐ¸ÐºÐ¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ ÑÐ°Ð·Ð¼ÐµÑÑ Ð±ÐµÑÐµÐ³Ð¾Ð·Ð°ÑÐ¸ÑÐ½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹, Ð¸Ñ Ð´Ð»Ð¸Ð½Ñ, ÑÐ°ÑÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¾Ñ Ð±ÐµÑÐµÐ³Ð°, Ð¸ Ð´Ñ. Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ.
Additional file 1 of Utility of droplet digital polymerase chain reaction for TERT and BRAF mutational profiling of thyroid nodules
Creators: name: Rosvall, Brandon R.
name: Kostiuk, Morris
name: Williams, Jordana
name: Matkin, Ashlee
name: Harris, Jeffrey
name: Seikaly, Hadi
name: O’Connell, Daniel A.
name: Biron, Vincent L.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer

description: Additional file 1: Supplementary Table 1. Histopathology and TERT ddPCR expression in benign thyroid nodules.
title: ÐÐ¾ÐºÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐµ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð² Ð´Ð²ÑÐ¼ÐµÑÐ½ÑÑ ÑÐµÑÑÑÐºÐ°Ñ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ¾ÐºÐ¸Ð½Ð°, ÐÐ»ÐµÐ½Ð°
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°ÑÐºÑÐµÑÐ¸ÑÐ½ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°
Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐ°ÐµÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð½Ð°Ð»Ð¸ÑÐ¸Ñ ÑÐ²ÑÐ·Ð¸ Ð¼ÐµÐ¶Ð´Ñ Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐ¼ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸ÐµÐ¼ (Ñ.Ðµ. ÑÑÑÑÐ¾Ð¼ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð¹ ÑÐ°ÑÑÐ¸ÑÑ Ñ ÑÐ¾ÑÐµÐ´ÑÐ¼Ð¸ Ð±Ð¾Ð»ÐµÐµ Ð´Ð°Ð»ÑÐ½ÐµÐ³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ°) Ð¸ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð°ÑÐºÑÐµÑÐ¸ÑÐ½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² (Ð¾ÑÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ° ÐÑÐ°ÑÑÐ¾Ð½Ð°) Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð¾Ð±Ð»Ð°Ð´Ð°ÑÑÐ¸Ñ ÐºÐ²Ð°Ð´ÑÐ°ÑÐ½Ð¾Ð¹ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÑÑÑÐºÐ¾Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð²Ð¾Ð´Ð¸ÑÑÑ Ð½Ð¾Ð²ÑÐ¹ ÑÐ¾ÑÐ¼Ð°Ð»Ð¸Ð·Ð¼, Ð¿ÑÐ¸Ð·Ð²Ð°Ð½Ð½ÑÐ¹ ÑÐ¿ÑÐ¾ÑÑÐ¸ÑÑ Ð²ÑÐ²Ð¾Ð´ Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹. ÐÐ»Ñ ÑÑÐ¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð½Ð° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÐ¾Ð² ÑÐ´Ð²Ð¸Ð³Ð° Ð¸ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð¸ Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð»ÑÐ±Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ° ÐºÐ°Ðº ÑÑÐ½ÐºÑÐ¸Ð¹ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð¹. Ð¦ÐµÐ»ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð´Ð¾Ð±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð¶ÐµÐ»Ð°Ð½Ð¸Ðµ Ð²ÑÑÑÐ½Ð¸ÑÑ, ÐºÐ°ÐºÐ¸Ðµ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÑÐµÐºÑÑ Ð¿ÑÐ¸Ð²Ð½Ð¾ÑÐ¸Ñ Ð² Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÑÑÑ Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½ÑÑ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð½ÑÑÑ, ÐºÐ°Ðº Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð²Ð»Ð¸ÑÐµÑ Ð½Ð° ÑÐ¿ÑÑÐ³Ð¸Ðµ ÐºÐ¾Ð½ÑÑÐ°Ð½ÑÑ, Ñ. e., ÐºÐ°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼ Ð¾Ð½Ð¸ Ð¼ÐµÐ½ÑÑÑÑÑ Ð¿ÑÐ¸ Ð¿ÐµÑÐµÑÐ¾Ð´Ðµ Ð¾Ñ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ðº Ð½ÐµÐ»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð¼Ñ. Ð¢Ð°ÐºÐ¶Ðµ, Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð´Ð¸ÑÐ¿ÐµÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ, Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½Ð½ÑÑ Ð²ÐºÐ»ÑÑÐµÐ½Ð¸ÐµÐ¼ Ð² ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð±Ð¾Ð»ÐµÐµ Ð´Ð°Ð»ÑÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð»Ð¸Ð½Ð½Ð¾Ð²Ð¾Ð»Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð»Ð¾ÑÐºÐ¾Ð¹ Ð²Ð¾Ð»Ð½Ñ. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, ÐºÐ¾Ð½ÑÐ¸Ð½ÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿ÑÐµÐ´ÐµÐ» Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÑÐ²Ð¸Ð´ÐµÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð´Ð°Ð»ÑÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ Ð½Ð° Ð°ÑÐºÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸. ÐÑÑÐµÐ¿ÐµÑÐµÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ðº ÐºÐ²Ð°Ð´ÑÐ°ÑÐ½Ð¾Ð¹ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÑÑÑÐºÐµ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ°Ðº ÑÐ¾Ð²Ð¾ÐºÑÐ¿Ð½Ð¾ÑÑÑ ÑÐ°ÑÑÐ¸Ñ Ñ Ð¾Ð´Ð¸Ð½Ð°ÐºÐ¾Ð²ÑÐ¼Ð¸ Ð¼Ð°ÑÑÐ°Ð¼Ð¸, ÑÐ¾ÐµÐ´Ð¸Ð½ÑÐ½Ð½ÑÑ Ð¿ÑÑÐ¶Ð¸Ð½Ð°Ð¼Ð¸.
title: Symbiose der Fallbearbeitung: Psychopathologie und Pädagogik in der Heimerziehung
Creators: name: Garz, Jona
name: Deplazes, Daniel
Publisher: name: Publikationsserver der Pädagogischen Hochschule Thurgau
Year: 2024

description: Erziehen, erfassen, erforschen: Kontinuität und Wandel der stationären Erziehung im 20. Jahrhundert am Beispiel des Landerziehungsheims Albisbrunn, p. 115
title: Разработка web-ориентированных информационных систем
Creators: name: ELS IPR BOOKS
Publisher: name: Донской государственный технический университет
Year: 2023

description: Рассмотрены основные понятия и положения, связанные с процессом разработки информационных систем, описаны базовые этапы жизненного цикла информационных систем, методологии и нотации проектирования, изложены архитектурные подходы к разработке. Раскрываются теоретические положения в области проектирования и разработки web-ориентированных информационных систем: специфика их архитектуры; принципы их функционирования и технологии построения; особенности разработки по системе front-end и back-end. Для закрепления и более глубокого изучения теоретического материала предусмотрены задания с примером разработки web-ориентированной информационной системы. Предполагается, что читатель владеет основами: языка разметки HTML, каскадных таблиц стилей CSS, серверного языка программирования PHP, проектирования СУБД MySQL и языка запросов SQL. Соответствует учебной программе дисциплины и Федеральному государственному образовательному стандарту. Может быть использовано при выполнении лабораторных, курсовых и дипломных работ. Предназначено для обучающихся по направлению подготовки УГСН 09.00.00 «Информатика и вычислительная техника».
Higher Genus Abelian Functions Associated with Cyclic Trigonal Curves
Creators: name: England, Matthew
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mathematical Physics (math-ph)
subject: Algebraic Geometry (math.AG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We develop the theory of Abelian functions associated with cyclic trigonal curves by considering two new cases. We investigate curves of genus six and seven and consider whether it is the trigonal nature or the genus which dictates certain areas of the theory. We present solutions to the Jacobi inversion problem, sets of relations between the Abelian function, links to the Boussinesq equation and a new addition formula.
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð½Ð¾Ð¹ ÑÑÑÐ¿ÐµÐ½Ð¸ Ð² Ð¦Ð¡Ð ÑÑÑÐ±Ð¸Ð½Ñ ÑÐ¸Ð¿Ð° Ð-800-240
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ·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: 2018
Subjects: ÐÐ°ÑÐ¾Ð²ÑÐµ ÑÑÑÐ±Ð¸Ð½Ñ
Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð½Ð°Ñ ÑÑÑÐ¿ÐµÐ½Ñ
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ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ( Ð² ÑÐµÐ¶Ð¸Ð¼Ðµ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð° Ñ Ð­ÐÐ ) Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÑÑÑÑÐ° Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ° ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð° Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð½Ð°Ñ Ð¿ÐµÑÐ²Ð°Ñ ÑÑÑÐ¿ÐµÐ½Ñ. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ñ ÑÑÐµÑÐ³Ð¾Ð»ÑÐ½Ð¸ÐºÐ¸ ÑÐºÐ¾ÑÐ¾ÑÑÐµÐ¹ Ð¸ Ð¿ÑÐ¾ÑÐ¸Ð»Ð¸ ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð»Ð¾Ð¿Ð°ÑÐºÐ¸ Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÑÑÐ¿ÐµÐ½Ð¸. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ½ÑÑ ÑÐ°ÑÑÑÑÐ¾Ð² ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð»Ð¾Ð¿Ð°ÑÐºÐ¸ Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÑÑÐ¿ÐµÐ½Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÑÐ½Ð½ÑÑ ÑÐ°ÑÑÑÑÐ¾Ð² Ð±ÑÐ»Ð° ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ°Ð±Ð¾ÑÐ°Ñ Ð»Ð¾Ð¿Ð°ÑÐºÐ° Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÑÑÐ¿ÐµÐ½Ð¸ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ° ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ.
One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
Creators: name: Angulo, Raul E.
name: White, Simon D. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We demonstrate that the output of a cosmological N-body simulation can, to remarkable accuracy, be scaled to represent the growth of large-scale structure in a cosmology with parameters similar to but different from those originally assumed. Our algorithm involves three steps: a reassignment of length, mass and velocity units, a relabelling of the time axis, and a rescaling of the amplitudes of individual large-scale fluctuation modes. We test it using two matched pairs of simulations. Within each pair, one simulation assumes parameters consistent with analyses of the first-year WMAP data. The other has lower matter and baryon densities and a 15% lower fluctuation amplitude, consistent with analyses of the three-year WMAP data. The pairs differ by a factor of a thousand in mass resolution, enabling performance tests on both linear and nonlinear scales. Our scaling reproduces the mass power spectra of the target cosmology to better than 0.5% on large scales (k < 0.1 h/Mpc) both in real and in redshift space. In particular, the BAO features of the original cosmology are removed and are correctly replaced by those of the target cosmology. Errors are still below 3% for k < 1 h/Mpc. Power spectra of the dark halo distribution are even more precisely reproduced, with errors below 1% on all scales tested. A halo-by-halo comparison shows that centre-of-mass positions and velocities are reproduced to better than 90 kpc/h and 5%, respectively. Halo masses, concentrations and spins are also reproduced at about the 10% level, although with small biases. Halo assembly histories are accurately reproduced, leading to central galaxy magnitudes with errors of about 0.25 magnitudes and a bias of about 0.13 magnitudes for a representative semi-analytic model.
description: 14 pages, 12 figures. Submitted to MNRAS
Resolving cell cycling and non-cycling dynamics in scRNA-seq
Creators: name: MacDonald, Haley
Publisher: name: University of British Columbia
Year: 2025

description: Controlled progression through and exit from the cell cycle is essential for normal development and healthy tissue function, while cell cycle dysregulation and sustained proliferation is a key hallmark of cancer. With the advent of large-scale single cell transcriptomics, a variety of methods were developed to detect cells in distinct phases of the cell cycle, including G1, S and G2/M, but characterization of non-cycling cellular states and their role in tumour evolution remains limited. Current tools for inferring cell cycle phase from single cell RNA sequencing (scRNA-seq) datasets have not been comprehensively benchmarked, and most are not compatible with heterogeneous samples containing multiple cell types. Here we present Ouroboros, a comprehensive package to accurately identify cell cycle phase and non-cycling cellular states in scRNA-seq datasets. Ouroboros facilitates integrated cell cycle visualization through the generation of representative cell cycle UMAPs and provides a random forest model that outperforms existing cell cycle tools while classifying two additional non-cycling states. Applied to heterogeneous developmental and tumour datasets, Ouroboros reveals complex cell state dynamics over pseudotime and between patient treatment time points. By enabling comprehensive visualization and classification of cycling and non-cycling cells, we anticipate that Ouroboros will offer a means to explore the complex interplay between cellular proliferation and quiescence in health and disease.
Three-dimensional dust density structure of the Orion, Cygnus X,Taurus, and Perseus star-forming regions
Creators: name: Dharmawardena, T. E.
name: Bailer-Jones, C. A. L.
name: Fouesneau, M.
name: Foreman-Mackey, D.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Interstellar dust affects astronomical observations through absorption and reddening, yet this extinction is also a powerful tool for studying interstellar matter in galaxies. 3D reconstructions of dust extinction and density in the Milky Way have suffered from artefacts such as the fingers-of-god effect and negative densities, and have been limited by large computational costs. Here we aim to overcome these issues with a novel algorithm that derives the 3D extinction density of dust in the Milky Way using a latent variable Gaussian Process and variational inference. Our model maintains non-negative density and hence monotonically non-decreasing extinction along all lines-of-sight, and performs inference within a reasonable computational time. Using extinctions for hundreds of thousands of stars computed from optical and near-IR photometry, together with distances based on Gaia parallaxes, we use our algorithm to infer the structure of the Orion, Taurus, Perseus, and Cygnus X star-forming regions. A number of features superimposed in 2D extinction maps are clearly deblended in 3D dust extinction density maps. We find a large filament on the edge of Orion, identify filament that in the Taurus and Perseus regions, and show that Cygnus X is located at 1300-1500pc. We compute dust masses of the regions and find these to be slightly higher than previous estimates, likely a consequence of our input data recovering the highest column densities more effectively. Comparing our predicted extinctions to Planck data, we find that known relationships between density and dust processing, where high extinction lines of sight have the most processed grains, hold up in resolved observations when density is included, and that they exist at smaller scales than previously suggested. This can be used to study the changes in size or composition of dust as they are processed in molecular clouds. (Abridged)
description: Accepted by A&A; Our code is available at https://github.com/Thavisha/Dustribution and the latest results are available from www.mwdust.com; 12 Pages, 15 figures; Appendix: 21 Pages, 9 figures
Additional file 1 of Herbal medicines use and associated factors among pregnant women in Debre Tabor town, north West Ethiopia: a mixed method approach
Creators: name: Addis, Getu Tesfaw
name: Workneh, Birhanu Demeke
name: Kahissay, Mesfin Haile
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1.
The Spitzer c2d Survey of Nearby Dense Cores VII: Chemistry and Dynamics in L43
Creators: name: Chen, Jo-Hsin
name: Evans, Neal J.
name: Lee, Jeong-Eun
name: Bourke, Tyler L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present results from the Spitzer Space Telescope and molecular line observations of 9 species toward the dark cloud L43. The Spitzer images and molecular line maps suggest it has a starless core and a Class I protostar evolving in the same environment. CO depletion is seen in both sources, and DCO+ lines are stronger toward the starless core. With a goal of testing the chemical characteristics from pre- to protostellar stages, we adopt an evolutionary chemical model to calculate the molecular abundances and compare with our observations. Among the different model parameters we tested, the best-fit model suggests a longer total timescale at the pre-protostellar stage, but with faster evolution at the later steps with higher densities.
Recrystallization and Interdiffusion Processes in Laser-Annealed Strain-Relaxed Metastable Ge$_{0.89}$Sn0$_{.11}$
Creators: name: Abdi, Salim
name: Assali, Simone
name: Atalla, Mahmoud R. M.
name: Koelling, Sebastian
name: Warrender, Jeffrey M.
name: Moutanabbir, Oussama
Publisher: name: arXiv
Year: 2021
Subjects: subject: Applied Physics (physics.app-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The prospect of GeSn semiconductors for silicon-integrated infrared optoelectronics brings new challenges related to the metastability of this class of materials. As a matter of fact, maintaining a reduced thermal budget throughout all processing steps of GeSn devices is essential to avoid possible material degradation. This constraint is exacerbated by the need for higher Sn contents along with an enhanced strain relaxation to achieve efficient mid-infrared devices. Herein, as a low thermal budget solution for post-epitaxy processing, we elucidate the effects of laser thermal annealing (LTA) on strain-relaxed Ge$_{0.89}$Sn0$_{.11}$ layers and Ni-Ge$_{0.89}$Sn0$_{.11}$ contacts. Key diffusion and recrystallization processes are proposed and discussed in the light of systematic microstructural studies. LTA treatment at a fluence of 0.40 J/cm2 results in a 200-300 nm-thick layer where Sn atoms segregate toward the surface and in the formation of Sn-rich columnar structures in the LTA-affected region. These structures are reminiscent to those observed in the dislocation-assisted pipe-diffusion mechanism, while the buried GeSn layers remain intact. Moreover, by tailoring the LTA fluence, the contact resistance can be reduced without triggering phase separation across the whole GeSn multi-layer stacking. Indeed, a one order of magnitude decrease in the Ni-based specific contact resistance was obtained at the highest LTA fluence, thus confirming the potential of this method for the functionalization of direct bandgap GeSn materials.
Additional file 2 of Establishment of an indicator framework for the transmission risk of the mountain-type zoonotic visceral leishmaniasis based on the Delphi-entropy weight method
Creators: name: Luo, Zhuowei
name: Zhou, Zhengbin
name: Hao, Yuwan
name: Feng, Jiaxin
name: Gong, Yanfeng
name: Li, Yuanyuan
name: Huang, Yun
name: Zhang, Yi
name: Li, Shizhu
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 2: Table S2. First round of primary indicators of the risk assessment of MT-ZVL.
Observation of Interplanetary Scintillation with Single-Station Mode at Urumqi
Creators: name: Liu, Lijia
name: Zhang, Xizhen
name: Li, Jianbin
name: Manoharan, P. K.
name: Liu, Zhiyong
name: Peng, Bo
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The Sun affects the Earth's physical phenomena in multiple ways, in particular the material in interplanetary space comes from coronal expansion in the form of inhomogeneous plasma flow (solar wind), which is the primary source of the interplanetary medium. Ground-based Interplanetary Scintillation (IPS) observations are an important and effective method for measuring solar wind speed and the structures of small diameter radio sources. We discuss one mode of ground-based single-station observations: Single-Station Single-Frequency (SSSF) mode. To realize the SSSF mode, a new system has been established at Urumqi Astronomical Observatory (UAO), China, and a series of experimental observations were carried out successfully from May to December, 2008.
Additional file 1 of Establishment of an indicator framework for the transmission risk of the mountain-type zoonotic visceral leishmaniasis based on the Delphi-entropy weight method
Creators: name: Luo, Zhuowei
name: Zhou, Zhengbin
name: Hao, Yuwan
name: Feng, Jiaxin
name: Gong, Yanfeng
name: Li, Yuanyuan
name: Huang, Yun
name: Zhang, Yi
name: Li, Shizhu
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1: Table S1. The indicators for the two rounds of the Delphi consultation.
Additional file 3 of Texture feature extraction from microscope images enables a robust estimation of ER body phenotype in Arabidopsis
Creators: name: Basak, Arpan Kumar
name: Mirzaei, Mohamadreza
name: Strzałka, Kazimierz
name: Yamada, Kenji
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Plant Biology

description: Additional file 3. Detailed schematic for the cell segmentation describing projection, mask using the global parameter file, the segmented cells and image.
Two-Dimensional Matter: Order, Curvature and Defects
Creators: name: Bowick, Mark J.
name: Giomi, Luca
Publisher: name: arXiv
Year: 2008
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Many systems in nature and the synthetic world involve ordered arrangements of units on two-dimensional surfaces. We review here the fundamental role payed by both the topology of the underlying surface and its detailed curvature. Topology dictates certain broad features of the defect structure of the ground state but curvature-driven energetics controls the detailed structured of ordered phases. Among the surprises are the appearance in the ground state of structures that would normally be thermal excitations and thus prohibited at zero temperature. Examples include excess dislocations in the form of grain boundary scars for spherical crystals above a minimal system size, dislocation unbinding for toroidal hexatics, interstitial fractionalization in spherical crystals and the appearance of well-separated disclinations for toroidal crystals. Much of the analysis leads to universal predictions that do not depend on the details of the microscopic interactions that lead to order in the first place. These predictions are subject to test by the many experimental soft and hard matter systems that lead to curved ordered structures such as colloidal particles self-assembling on droplets of one liquid in a second liquid. The defects themselves may be functionalized to create ligands with directional bonding. Thus nano to meso scale superatoms may be designed with specific valency for use in building supermolecules and novel bulk materials. Parameters such as particle number, geometrical aspect ratios and anisotropy of elastic moduli permit the tuning of the precise architecture of the superatoms and associated supermolecules. Thus the field has tremendous potential from both a fundamental and materials science/supramolecular chemistry viewpoint.
description: Review article, 102 pages, 59 figures, submitted to Advances in Physics
Additional file 1 of Retrospective analysis of recurrence patterns and clinical outcome of grade II meningiomas following postoperative radiotherapy
Creators: name: Hoffmann, Elgin
name: Clasen, Kerstin
name: Frey, Bettina
name: Ehlers, Jakob
name: Behling, Felix
name: Skardelly, Marco
name: Bender, Benjamin
name: Schittenhelm, Jens
name: Reimold, Matthias
name: Tabatabai, Ghazaleh
name: Zips, Daniel
name: Eckert, Franziska
name: Paulsen, Frank
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. Table 1. Dose constraints for Organs at Risk (OARs). Table 2. Volume of interest (VOI) definition. Table 3. Statistical information for the comparison of dosimetrical data.
Decoupling of unphysical states in the minimal pure spinor formalism II
Creators: name: Berkovits, Nathan
name: Hoogeveen, Joost
name: Skenderis, Kostas
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This is the second of a series of two papers where decoupling of unphysical states in the minimal pure spinor formalism is investigated. The multi-loop amplitude prescription for the minimal pure spinor superstring formulated in hep-th/0406055 involves the insertion of picture changing operators in the path integral. In the first paper it was shown that these operators are not BRST closed inside correlators. Therefore a new proof of decoupling of BRST exact states is needed. In this paper we present such a proof, which applies to arbitrary genus. It relies in part on a (previously unnoticed) invariance of the path integral measure.
description: 16 pages, corrected typo's
Additional file 2 of Texture feature extraction from microscope images enables a robust estimation of ER body phenotype in Arabidopsis
Creators: name: Basak, Arpan Kumar
name: Mirzaei, Mohamadreza
name: Strzałka, Kazimierz
name: Yamada, Kenji
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Plant Biology

description: Additional file 2. Detailed schematics of image acquisition, image processing, segmentation and data analysis for the quantification of ER body morphology and dynamics.
Supplementary Material-Rev1.pdf from Green quantitative spectrofluorometric analysis of rupatadine and montelukast at nanogram scale using direct and synchronous techniques
Creators: name: Ghonim, Rana
name: El-Awady, Mohamed I.
name: Tolba, Manar M.
name: Ibrahim, Fawzia
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 30199 Analytical Chemistry not elsewhere classified
subject: FOS: Chemical sciences

description: Two green-sensitive spectrofluorometric methods were investigated for assay of rupatadine (RUP) [method I] and its binary mixture with montelukast (MKT) [method II]. Method I depends on measuring native fluorescence of RUP in the presence of 0.10 M H2SO4 and 0.10%w/v sodium dodecyl sulfate at 455 nm after excitation at 277 nm. The range of the first method was 0.20–2.00 µgml−1 with detection and quantitation limits of 59.00 and 179.00 ngml−1, respectively. Method II depends on the first derivative synchronous spectrofluorometry. The derivative intensities were measured for the two drugs in an aqueous solution containing Mcllvaine's buffer pH 2.60 at fixed Δλ of 140 nm. Each drug was estimated at zero-contribution of the other. The intensity was measured at 261 and 371 nm for RUP and MKT, respectively. The method was linear over 0.10–4.00 and 0.20–1.60 µgml−1 with limits of detection 31.00 and 66.00 ngml−1 and limits of quantitation 94.00 and 200.00 ngml−1 for RUP and MKT, respectively. The method was extended to determine this mixture in laboratory-prepared mixtures and combined tablets. Method validation was performed according to ICH guidelines. Statistical interpretation of data revealed good agreement with the comparison method. Method greenness was confirmed by applying three different assessment tools.
Vacuum squeezing via polarization self-rotation and excess noise in hot Rb vapors
Creators: name: Mikhailov, Eugeniy E.
name: Lezama, Arturo
name: Noel, Thomas W.
name: Novikova, Irina
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present experimental and theoretical analysis of quantum fluctuation in a vacuum field in the presence of orthogonal linearly polarized pump field propagating through a Rb vapor cell. Previously reported theoretical and experimental studies provided somewhat contradictory conclusions regarding the possibility to observe the "squeezed vacuum" -- the reduction of vacuum fluctuations below standard quantum limit -- in this system. Here, using the D1 transitions of Rb in a cell without buffer as as an example, we demonstrate that vacuum squeezing is corrupted by incoherent processes (such as spontaneous emission, elastic scattering, etc.), and its observation is only possible in a specific small region of the experimental parameter space. Numerical simulations, in good agreement with the experiment, demonstrate that the two excited state hyperfine levels play a crucial role in the squeezing and excess noise production. The significant influence of far-detuned atoms on the field fluctuations at low noise frequencies imposes the explicit consideration of the full velocity distribution of the atomic vapor.
description: 6 pages, 6 figures
David Ost / Klęska "Solidarności". Gniew i polityka w postkomunistycznej Europie. Warszawa 2007
Creators: name: Laska, Artur
Publisher: name: Świat Idei i Polityki
Year: 2007

description: Świat Idei i Polityki, Tom 7 (2007): Świat Idei i Polityki
Francis Fukuyama / Ameryka na rozdrożu: demokracja, władza i dziedzictwo neokonserwatyzmu. Poznań 2006
Creators: name: Kosman, Michał
Publisher: name: Świat Idei i Polityki
Year: 2007

description: Świat Idei i Polityki, Tom 7 (2007): Świat Idei i Polityki
Variational local moment approach: from Kondo effect to Mott transition in correlated electron systems
Creators: name: Kauch, Anna
name: Byczuk, Krzysztof
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The variational local moment approach (VLMA) solution of the single impurity Anderson model is presented. It generalizes the local moment approach of Logan et al. by invoking the variational principle to determine the lengths of local moments and orbital occupancies. We show that VLMA is a comprehensive, conserving and thermodynamically consistent approximation and treats both Fermi and non-Fermi liquid regimes as well as local moment phases on equal footing. We tested VLMA on selected problems. We solved the single- and multi-orbital impurity Anderson model in various regions of parameters, where different types of Kondo effects occur. The application of VLMA as an impurity solver of the dynamical mean-field theory, used to solve the multi-orbital Hubbard model, is also addressed.
description: 11 pages, 12 figures
title: Ð¦Ð¸ÑÑÐ¾Ð²Ð°Ñ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ. Ð­ÑÑÐµÐºÑÐ¸Ð²Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð² Power Point
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
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: 2021
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
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description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ»ÑÑÐ°ÑÐµÐ»ÑÐ¼ Ð¿Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¼Ñ Ð²ÑÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ½Ð¸ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸. Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¸ÐµÐ¼Ñ ÑÐ°Ð±Ð¾ÑÑ Ð² Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸ Power Point, Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÐµ Ð¿ÑÐ¸Ð¼ÐµÑÑ.
CO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
Creators: name: Domínguez-Gómez, J.
name: Lisenfeld, U.
name: Pérez, I.
name: López-Sánchez, Á. R.
name: Puertas, S. Duarte
name: Falcón-Barroso, J.
name: Kreckel, K.
name: Peletier, R. F.
name: Ruiz-Lara, T.
name: van de Weygaert, R.
name: van der Hulst, J. M.
name: Verley, S.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the first molecular gas mass survey of void galaxies. We compare these new data together with data for the atomic gas mass and star formation rate ($\rm SFR$) from the literature to those of galaxies in filaments and walls in order to better understand how molecular gas and star formation are related to the large-scale environment. We observed at the IRAM 30 m telescope the CO(1-0) and CO(2-1) emission of 20 void galaxies selected from the Void Galaxy Survey (VGS), with a stellar mass range from $\rm 10^{8.5}$ to $\rm 10^{10.3}M_{\odot}$. We detected 15 objects in at least one CO line. We compared the molecular gas mass ($M_{\rm H_2}$), the star formation efficiency ($\rm SFE =SFR/M_{\rm H_2}$), the atomic gas mass, the molecular-to-atomic gas mass ratio, and the specific star formation rate (sSFR) of the void galaxies with two control samples of galaxies in filaments and walls, selected from xCOLD GASS and EDGE-CALIFA, for different stellar mass bins and taking the star formation activity into account. The results for the molecular gas mass for a sample of 20 voids galaxies allowed us to make a statistical comparison to galaxies in filaments and walls for the first time.
description: 24 pages, 15 figures, accepted in A&A, language corrected version
Predicting Phenotype from Multi-Scale Genomic and Environment Data using Neural Networks and Knowledge Graphs: An Introduction to the NSF GenoPhenoEnvo Project
Creators: name: Thessen, Anne E
name: Behrisch, Michael
name: Cain, Emily J
name: Chang, Remco
name: Heidorn, P Bryan
name: Jaiswal, Pankaj
name: LeBauer, David
name: Mosca, Ab
name: Munoz-Torres, Monica C
name: Ross, Arun
name: Swetnam, Tyson
Publisher: name: Zenodo
Year: 2020
Subjects: genomics
phenomics
machine learning
ontology

description: To mitigate the effects of climate change on public health and conservation, we need to better understand the dynamic interplay between biological processes and environmental effects. Machine learning (ML) methods in general, and Deep Learning (DL) methods in particular, are a potential way forward because they are able to cope with the nonlinearity of natural systems. However, there are several barriers that exist, including the opaque nature of the algorithm output and the absence of ML-ready data. We propose to develop a machine learning framework capable of predicting phenotypes based on multi-scale data about genes and environments. A critical part of this framework is a visualization system to contextualize the results of an ML model, that is, to examine model decisions, connect decisions to input samples, and test alternative decisions. Further, we will develop data transformation methods that map the heterogeneous input data, ranging from simple vectors to complex images, into formats that are consumable by the ML techniques. The central hypothesis of this research is that deep learning algorithms and biological knowledge graphs will predict phenotypes more accurately across more taxa and more ecosystems than do current numerical and traditional statistical modeling methods. Our long term goal is to develop predictive analytics for organismal response to environmental perturbations using innovative data science approaches. This pilot project on predicting emergent properties of complex systems and multidimensional interactions is funded by the NSF (Award # 1940330). 
Additional file 1 of An iceberg I can’t handle: a qualitative inquiry on perceptions towards paediatric rheumatology among healthcare workers in Kenya
Creators: name: Migowa, Angela
name: Bernatsky, Sasha
name: Ngugi, Anthony
name: Foster, Helen E.
name: Muriuki, Peter
name: Lusambili, Adelaide
name: Luchters, Stanley
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy

description: Additional file 1: Appendix 1. Consolidated criteria for reporting qualitative studies (coreq): 32-item checklist.
Additional file 1 of Texture feature extraction from microscope images enables a robust estimation of ER body phenotype in Arabidopsis
Creators: name: Basak, Arpan Kumar
name: Mirzaei, Mohamadreza
name: Strzałka, Kazimierz
name: Yamada, Kenji
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Plant Biology

description: Additional file 1. The parameters used as the default for segmentation of cells.
Quantum anti-Zeno effect in artificial quantum systems
Creators: name: Ai, Qing
name: Liao, Jie-Qiao
name: Sun, C. P.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this paper, we study a quantum anti-Zeno effect (QAZE) purely induced by repetitive measurements for an artificial atom interacting with a structured bath. This bath can be artificially realized with coupled resonators in one dimension and possesses photonic band structure like Bloch electron in a periodic potential. In the presence of repetitive measurements, the pure QAZE is discovered as the observable decay is not negligible even for the atomic energy level spacing outside of the energy band of the artificial bath. If there were no measurements, the decay would not happen outside of the band. In this sense, the enhanced decay is completely induced by measurements through the relaxation channels provided by the bath. Besides, we also discuss the controversial golden rule decay rates originated from the van Hove's singularities and the effects of the counter-rotating terms.
description: 12 pages, 8 figures
High cadence pulsar timing with CHIME/Pulsar
Creators: name: Cassity, Alyssa
Publisher: name: University of British Columbia
Year: 2025

description: Pulsars are rapidly rotating, highly magnetized neutron stars—the collapsed remnants of massive stars following a supernova explosion. They produce beams of radiation that reach our observatories on Earth at regular intervals. The precise timing of these radio pulses has many applications, including exploring fundamental physics, testing the predictions of general relativity, probing the interstellar medium, and even detecting gravitational waves. This work investigates variability in pulsar emission using the unprecedented observing cadence of the CHIME telescope. The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a radio telescope near Penticton, British Columbia, Canada. Although initially conceived as a cosmology experiment, it has proven to be an excellent instrument for discovering and studying radio transients. This thesis utilizes the CHIME/Pulsar science backend. First, for PSR B0540+23 we conduct an analysis to explore emission modulation during periods of low solar elongation, which occur once a year. Each year, the pulsar is occulted by the solar wind due to its position in the sky. We observe dispersion measure variations caused by excess solar wind electrons along the line of sight and infer a solar electron density based on these observations. Next, we study nulling and mode-changing behavior in PSRs B0809+74 and B0329+54. We employ a matched filtering pipeline to identify this behavior. We investigate links between these phenomena and an excess of outlier TOAs identified by the NANOGrav Collaboration’s outlier analysis. We find that the outlier analysis is sensitive to mode-changing in PSR B0329+54. These findings highlight the utility of CHIME/Pulsar’s daily observing cadence for studying pulsar emission. With the capabilities of CHIME/Pulsar, we are able to identify yearly occultations of PSR B0540+23 by the solar wind. We also provide a foundation for applying the NANOGrav outlier analysis to identify mode-changing in pulsars. The results of this work highlight the value of CHIME/Pulsar in studying a wide range of pulsar emission phenomena.
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title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¤ÑÐ´Ð¾ÑÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
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 Ð°Ð´Ð¸Ð¾Ð»Ð¾ÐºÐ°ÑÐ¸Ñ
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