cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Gut microbiome structure and evolution in Parnassius species on the Qinghai-Tibet Plateau
Creators: name: Su, Chengyong
name: Xie, Tingting
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 310405
subject: Evolutionary ecology
classificationCode: 310409
subject: Microbial taxonomy

description: Based on the aggregated genome-based phylogeny and microbial data of Parnassius species at the population level which were generated with the same collection methods, we utilized a robust analytical framework to resolve the relative importance of host genetics, geography, altitude, and larval host-plant on gut microbial community structure and evolution. Our findings indicate that both host genetics and larval host-plant modulated gut microbial diversity and community structure. Moreover, we decoupled the effects of host genetics and larval diet on gut microbiome and showed that host genetics mainly governed gut microbial beta diversity and community structure, while larval host-plant functionally influenced gut microbiome evolution. Our findings help to resolve the major modulators of gut microbiome diversity and evolution in butterfly species, which have not been well studied in wild insects with varying degrees of ecological niche divergence and evolutionary relatedness, especially those inhabit on the QTP.
Mira, stella variabile e con la coda
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Una stella simile al Sole ma molto più evoluta, vede oscillare la sua luminosità di ben 8 magnitudini nell'arco di undici mesi circa. E' Omicron Ceti, uno dei più peculiari oggetti che popolano il cielo serale di questo mese. Cielo che sarà anche caratterizzato da alcune splendide congiunzioni
On a Logarithmic Deformation of the Supersymmetric bc-system on Curved Manifolds
Creators: name: Vogeler, Kirsten
name: Flohr, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: E. Frenkel, A. Losev and N. Nekrasov claim that a certain class of theories on compact Kahler manifolds and in particular the "gauged" supersymmetric bc-system on CP^1 are logarithmic conformal field theories. We discuss that proposition on a classical level for the bc-system on CP^1. The outcome of our investigation conforms to their conjecture. The property of being a logarithmic CFT thus can be interpreted as an effect of gravity.
Caronte e il suo cratere più giovane
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Organa è molto simile a Skywalker, l'altro famoso cratere sulla luna più grande di Plutone. I due però sono diversi in composizione: l'uno ricco di ammoniaca, l'altro ricco di acqua sotto forma di ghiaccio
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±ÑÑÑÑÐ¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Ð´Ð»Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ»ÑÐ·Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° ÑÑÐ´Ð¾Ñ Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÐºÐ°Ð½Ð°Ð»Ð°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ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: 2017
Subjects: Ð¡ÑÐ´Ð¾Ñ Ð¾Ð´Ð½ÑÐµ ÐºÐ°Ð½Ð°Ð»Ñ
Ð¨Ð»ÑÐ·Ñ ÑÑÐ´Ð¾Ñ Ð¾Ð´Ð½ÑÐµ
ÑÐµÐ¾ÑÐ¸Ñ ÑÐ°ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ð¹
Ð¼ÐµÑÐ¾Ð´Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸
Ð´Ð¸ÑÐºÑÐµÑÐ½Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð° Ð¸ ÑÐ¾ÑÐ¼Ð°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð° Ð·Ð°Ð´Ð°ÑÐ° Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð´Ð»Ñ ÑÐµÑÐ¸Ð¸ ÑÐ»ÑÐ·Ð¾Ð². ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð½Ð°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð·Ð°Ð´Ð°ÑÐµÐ¹ ÑÐ¼ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ»Ð¾ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ»Ñ ÑÐ°ÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ Ð½Ðµ ÑÑÑÐµÑÑÐ²ÑÐµÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² Ð¾Ð±ÑÐµÐ¼ Ð²Ð¸Ð´Ðµ. Ð Ð¾ÑÐ½Ð¾Ð²Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð»ÐµÐ³ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼, ÑÑÐ¸ÑÑÐ²Ð°ÑÑÐ¸Ð¹ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÑ Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸. ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÑ Ð¾Ð±ÑÑÑ Ð¸Ð´ÐµÑ Ð²ÐµÑÐ²ÐµÐ¹ Ð¸ Ð³ÑÐ°Ð½Ð¸Ñ. ÐÐ»Ð°Ð³Ð¾Ð´Ð°ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¼Ñ Ð¿ÑÐ°Ð²Ð¸Ð»Ñ ÑÐ°Ð·Ð±Ð¸ÐµÐ½Ð¸Ñ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð° ÑÐµÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¿Ð¾Ð´Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ¾ÑÐ½Ð¾Ð¹ Ð½Ð¸Ð¶Ð½ÐµÐ¹ Ð³ÑÐ°Ð½Ð¸ÑÑ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¿Ð¾Ð´Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð° ÑÐ´Ð°Ð»Ð¾ÑÑ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ. Ð¢Ð°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð¸ÑÐºÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÐµÑÑÑ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°, Ð¿Ð¾ÑÐ»Ðµ Ð½Ð°ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÑÐµÐºÑÑÐµÐ³Ð¾ Ð½Ð°Ð¸Ð»ÑÑÑÐµÐ³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð¸ÑÐºÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð½Ð° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ¼ÑÑÐ»Ðµ ÑÐµÑÐµÐ½Ð¸Ñ, Ð° Ð½Ðµ Ð½Ð° ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¿Ð¾Ð´ÑÐ¾Ð´Ðµ Ð¿Ð¾Ð¸ÑÐºÐ° Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐºÑÑÑÐµÐ¼ÑÐ¼Ð°. ÐÐ±ÑÑÑÐ½ÑÐµÑÑÑ ÑÑÐ¾ ÑÐµÐ¼, ÑÑÐ¾ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐµ ÐºÑÐ°Ð¹Ð½Ðµ ÑÑÑÐ´Ð¾ÐµÐ¼Ð¾Ðº Ð¿Ð¾Ð¸ÑÐº Ð´Ð¾Ð¿ÑÑÑÐ¸Ð¼Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÑÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°, ÐµÐ³Ð¾ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¿ÐµÑÐµÐ´ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð¼ Ð²ÐµÑÐ²ÐµÐ¹ Ð¸ Ð³ÑÐ°Ð½Ð¸Ñ Ð¾Ð±ÑÐµÐ¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð±Ð¸Ð½Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð¢Ð°Ðº Ð¶Ðµ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ñ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð°Ð²ÑÐ¾ÑÐ¾Ð², Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ ÑÐµÑÐ°Ð»Ð°ÑÑ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ÑÐ½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ°.
title: История жизни Будимира Тукумцева, написанная им самим. На территории ГУЛАГа (картинки с натуры), 1941–1943 годы
Creators: name: Тукумцев, Б. Г.
Publisher: name: Реноме
Year: 2023

description: Данная публикация продолжает издание разделов автобиографической книги российского социолога Будимира Гвидоновича Тукумцева (1927-2021) «История Будимира Тукумцева, написанная им самим» (малотиражное издание книги осуществлено в 2022 г.). Публикуется с разрешения Ирины Будимировны Олимпиевой. В последующих выпусках ПСС публикация разделов из книги Б. Г. Тукумцева будет продолжена.
title: ÐÑÑÐ¾ÐºÐ¾Ð¿ÑÐ¾ÑÐ½ÑÐµ ÑÑÐ°Ð»Ð¸ Ð´Ð»Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÐºÑÐ·Ð¾Ð²Ð¾Ð² Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹ Ð¸ Ð¸Ñ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð°Ñ ÑÐ¾ÑÐµÑÐ½Ð°Ñ ÑÐ²Ð°ÑÐºÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ»ÑÐ±Ð°ÐµÐ²Ð° , Ð®Ð»Ð¸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: 2016
Subjects: ÑÑÐ°Ð»Ð¸ Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸
ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð°Ñ ÑÐ¾ÑÐµÑÐ½Ð°Ñ ÑÐ²Ð°ÑÐºÐ°
ÑÐµÐ¶Ð¸Ð¼ ÑÐ²Ð°ÑÐºÐ¸
steel for the automotive industry
resistance spot welding
welding mode

description: Ð¡Ð¾Ð±ÑÐ°Ð½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÑÐµÑ Ð½Ð¾Ð²ÑÑ Ð²ÑÑÐ¾ÐºÐ¾Ð¿ÑÐ¾ÑÐ½ÑÑ ÑÑÐ°Ð»ÑÑ: Dual Phase (DP), Transformation-Induced Plasticity (TRIP) Ð¸ Twinning-Induced Plasticity (TWIP). ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐµ ÑÐµÐ¶Ð¸Ð¼Ñ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐµÑÐ½Ð¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÑ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ ÑÐ²Ð°ÑÐ½ÑÑ ÑÐ¾ÑÐµÐº (ÑÐ¸Ð»Ð° ÑÑÐµÐ·Ð°, ÑÐ¸Ð»Ð° Ð¾ÑÑÑÐ²Ð° Ð¸ ÑÐ²ÐµÑÐ´Ð¾ÑÑÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð° ÑÐ²Ð° Ð¸ Ð·Ð¾Ð½Ñ ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ).
I crateri lunari visti da GRAIL
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

I dati raccolti dalle due sonde spaziali Gravity Recovery and Interior Laboratory hanno raccolto dati preziosi sulle variazioni gravitazionali del suolo lunare. I risultati, presentati oggi sulla rivista Science Advances, identificano nuovi bacini da impatto e mostrano un quadro più chiaro per quanto riguarda le dimensioni e la distribuzione dei bacini già noti sulla superficie del nostro satellite naturale
Neutrino-induced coherent pion production off nuclei
Creators: name: Leitner, T.
name: Mosel, U.
name: Winkelmann, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: All available theoretical estimates of neutrino-induced coherent pion production rely on the 'local approximation' for the Delta propagator. The validity of this approximation is scrutinized. It is found that the local approximation overestimates the neutrino-induced coherent pion production on nuclei significantly, by up to 100%.
description: To appear in the proceedings of 6th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region (NuInt09), Sitges, Spain, 18 - 22 May 2009
L’antica Roma fa scudo a Cuore
Creators: Antonella Varaschin
Publisher: name: Media Inaf
Year: 2015

CUORE è un esperimento ideato per studiare le proprietà̀ dei neutrini e, in particolare, un fenomeno raro chiamato doppio decadimento beta senza emissione di neutrini. I ricercatori hanno progettato, infatti, di dotarlo di uno “scudo” realizzato grazie alla fusione di lingotti di piombo recuperati da una nave romana affondata oltre 2000 anni fa, al largo delle coste della Sardegna
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸Ñ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ÑÑÐºÐ¾, ÐÐ°ÑÑ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: ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ´Ñ
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÑÐºÑÑÑÐ°
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ ÑÑÐµÐ´Ð°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð´ÐµÑÑÐºÐ¸Ð¹ Ð¸Ð½ÑÐµÑÐ°ÐºÑÐ¸Ð²Ð½Ð¾-ÑÐ°Ð·Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¼ÑÐ·ÐµÐ¹ Â«MUZEUSÂ». Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÑÐ°Ð¿Ð¾Ð² ÐµÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾ â ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Â«MUZEUSÂ», Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ ÑÑÐµÐ´Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Â«MUZEUSÂ» Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ SWOT Ð¸ PEST- Ð°Ð½Ð°Ð»Ð¸Ð·Ð°, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð´Ð°Ð½Ð¾ ÐµÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ.
Encelado vista da vicino
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Le prime immagini "grezze" inviate dalla sonda Cassini all'indomani del flyby della luna di Saturno Encelado. Nelle prossime settimane arriveranno le analisi scientifiche e le aspettative sono tali che la luna Encelado è oggi un obiettivo primario per le future esplorazioni alla ricerca della vita nel nostro sistema solare
Dawn in discesa verso l’orbita finale
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Il motore ionico è stato azionato venerdì scorso, fa sapere la NASA, e per metà dicembre avranno inizio le operazioni scientifiche dalla quarta e ultima orbita, la più ravvicinata, ad appena 380 km dalla superficie del pianeta nano Cerere
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð±Ð¾ÑÑÐ±Ðµ Ñ Ð¿Ð°Ð²Ð¾Ð´ÐºÐ¾Ð²ÑÐ¼Ð¸ ÑÐ²Ð»ÐµÐ½Ð¸ÑÐ¼Ð¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÐÐÐ¡-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐµÐº ÐÐ°Ð»ÑÐ½ÐµÐ³Ð¾ ÐÐ¾ÑÑÐ¾ÐºÐ°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¸ÐºÐ¾Ð½Ð¾ÑÐ¾Ð², 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: 2016
Subjects: ÐÐ°Ð²Ð¾Ð´ÐºÐ¸
ÐÐ°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ñ
ÐÐ¸Ð´ÑÐ¾Ð»Ð¾Ð³Ð¸Ñ
ÐÐ¸Ð´ÑÐ¾Ð»Ð¾Ð³Ð¸Ñ ÑÐµÑÐ½Ð°Ñ
ÐÐÐ¡-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
floods
GIS-technology
hydrological modelling

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð°Ð²Ð¾Ð´ÐºÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÐÐÐ¡-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð±Ð¾ÑÑÐ±Ðµ Ñ Ð½Ð¸Ð¼Ð¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾Ð±ÑÐ¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¸ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð´Ð°Ð½Ð½ÑÐµ. ÐÐ·ÑÑÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÐÐÐ¡-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð³Ð¸Ð´ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿Ð°Ð²Ð¾Ð´ÐºÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð´Ð»Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð°Ð²Ð¾Ð´ÐºÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð² Ð´Ð»Ñ Ð¿Ð¾Ð¸ÑÐºÐ° Ð°Ð´ÐµÐºÐ²Ð°ÑÐ½ÑÑ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹, Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐ°ÑÑÐ¸Ñ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¸ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¼ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÑÑ ÑÑÐµÐ´Ñ.
description: This work is based on analysis of flood events using GIS-environment and managerial solutions to prevent them. General concepts and statistical data are given. Modern GIS-technologies, which are used for flash flood hydrological model creation, are examined. The test models, which allow analyzing possible engineering solution with the aim of minimization of risks and consequences, are developed.
Statistics of subgap states in $s_\pm$ superconductors
Creators: name: Glatz, A.
name: Koshelev, A. E.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: There is strong support in favor of an unusual $s_{\pm}$ superconducting state in the new iron-based superconductors, in which the gap parameter has opposite signs in different bands. In this case scattering between different bands by impurities has a pair-breaking effect and introduces states inside the gap. We studied the statistics of disorder-induced subgap states in $s_{\pm}$ superconductors due to collective effects of impurities. Numerically solving the two-band Bogolyubov equations, we explored the behavior of the density of states and localization length. We located the mobility edge separating the localized and delocalized states for the 3D case and the crossover between the weak and strong localization regimes for the 2D case. We found that the widely used self-consistent T-matrix approximation is not very accurate in describing subgap states.
description: 7 pages, 5 figures, RevTex 4.1
A model for the electromagnetic spectrum of the inner jets of Cen A
Creators: name: Orellana, M.
name: Romero, G. E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Centaurus A, the closest active galaxy, has been detected from radio to high-energy gamma-rays. The synchrotron radiation by extremely high energy protons may be a suitable mechanism to explain the MeV to GeV emission detected by the instruments of the Compton Gamma-Ray Observatory, as coming from the inner jets. This scenario requires a relatively large magnetic field of about 10^4 G that could be present only close to the central black hole. We investigate the spectral energy distribution (SED) resulting from a one-zone compact acceleration region, where both leptonic and hadronic relativistic populations arise. We present here results of such a model, where we have considered synchrotron radiation by primary electrons and protons, inverse Compton interactions, and gamma-ray emission originated by the inelastic hadronic interactions between relativistic protons and cold nuclei within the jets themselves. Photo-meson production by relativistic hadrons were also taken into account, as well as the effects of secondary particles injected by all interactions. The internal and external absorption of gamma rays is shown to be of great relevance to shape the observable SED, which was also recently constrained by the results of HESS.
description: 13 pages (ref. style), submitted to MNRAS on December 04, 2008. Waiting for review
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²Ð¸Ð´Ð¾Ð² ÑÐ¿Ð¾ÑÑÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð Ð¾Ð»Ð»ÐµÑ Ð¢Ð°Ð¹Ð¼Â»)
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ÐµÐ»Ð°Ñ, ÐÑÐµÐ½Ð¸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: ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ñ
ÑÑÐ°Ð¿Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸
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ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° ÑÐµÐ¼Ñ Â«Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²Ð¸Ð´Ð¾Ð² ÑÐ¿Ð¾ÑÑÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¾Ð»Ð»ÐµÑ ÑÐºÐ¾Ð»Ñ ÐÐÐ Â«Ð Ð¾Ð»Ð»ÐµÑ Ð¢Ð°Ð¹Ð¼Â»)Â» Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² ÑÐ¾Ð»Ð»ÐµÑ ÑÐºÐ¾Ð»Ðµ ÐÐÐ Â«Ð Ð¾Ð»Ð»ÐµÑ Ð¢Ð°Ð¹Ð¼Â» Ñ ÑÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÑÐ¾Ð»Ð»ÐµÑÑÐºÐ¾Ð»Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
Punctuation restoration in Swedish through fine-tuned KB-BERT
Creators: name: Nilsson, John Björkman
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computation and Language (cs.CL)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Presented here is a method for automatic punctuation restoration in Swedish using a BERT model. The method is based on KB-BERT, a publicly available, neural network language model pre-trained on a Swedish corpus by National Library of Sweden. This model has then been fine-tuned for this specific task using a corpus of government texts. With a lower-case and unpunctuated Swedish text as input, the model is supposed to return a grammatically correct punctuated copy of the text as output. A successful solution to this problem brings benefits for an array of NLP domains, such as speech-to-text and automated text. Only the punctuation marks period, comma and question marks were considered for the project, due to a lack of data for more rare marks such as semicolon. Additionally, some marks are somewhat interchangeable with the more common, such as exclamation points and periods. Thus, the data set had all exclamation points replaced with periods. The fine-tuned Swedish BERT model, dubbed prestoBERT, achieved an overall F1-score of 78.9. The proposed model scored similarly to international counterparts, with Hungarian and Chinese models obtaining F1-scores of 82.2 and 75.6 respectively. As further comparison, a human evaluation case study was carried out. The human test group achieved an overall F1-score of 81.7, but scored substantially worse than prestoBERT on both period and comma. Inspecting output sentences from the model and humans show satisfactory results, despite the difference in F1-score. The disconnect seems to stem from an unnecessary focus on replicating the exact same punctuation used in the test set, rather than providing any of the number of correct interpretations. If the loss function could be rewritten to reward all grammatically correct outputs, rather than only the one original example, the performance could improve significantly for both prestoBERT and the human group.
LHC ad alta luminosità
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Dopo quattro anni di studio, il progetto High-Luminosity LHC passa alla fase operativa con sviluppo di prototipi industriali. L’obiettivo è aumentare di un fattore 10 la luminosità dello strumento e le potenziali scoperte, a partire dal 2025
Exclusive diffractive final states in electron-proton collisions
Creators: name: Fazio, S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The exclusive diffractive production of vector mesons and real photons in ep collisions has been studied at HERA in a wide kinematic range. The most recent experimental results are presented.
description: Presented at the Lake Louise Winter Institute 2008, Lake Louise (Calgary), Canada, 18-23 Feb. 2008
Mattang lucente
Creators: Mariateresa Crosta
Publisher: name: Media Inaf
Year: 2015

L'installazione è una metafora della navigazione esplorativa aperta e richiama il concetto della mappatura relativistica in corso nella nostra Galassia attraverso la luce stellare che sta raccogliendo nello spazio, ad 1,5 milioni di km dalla Terra, la missione europea Gaia
Stellar Clusters in the NGC 6334 Star Forming Complex
Creators: name: Feigelson, Eric D.
name: Martin, Amanda L.
name: McNeill, Collin J.
name: Broos, Patrick S.
name: Garmire, Gordon P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The full stellar population of NGC 6334, one of the most spectacular regions of massive star formation in the nearby Galaxy, have not been well-sampled in past studies. We analyze here a mosaic of two Chandra X-ray Observatory images of the region using sensitive data analysis methods, giving a list of 1607 faint X-ray sources with arcsecond positions and approximate line-of-sight absorption. About 95 percent of these are expected to be cluster members, most lower mass pre-main sequence stars. Extrapolating to low X-ray levels, the total stellar population is estimated to be 20-30,000 pre-main sequence stars. The X-ray sources show a complicated spatial pattern with about 10 distinct star clusters. The heavily-obscured clusters are mostly associated with previously known far-infrared sources and radio HII regions. The lightly-obscured clusters are mostly newly identified in the X-ray images. Dozens of likely OB stars are found, both in clusters and dispersed throughout the region, suggesting that star formation in the complex has proceeded over millions of years. A number of extraordinarily heavily absorbed X-ray sources are associated with the active regions of star formation.
description: To appear in the Astronomical Journal. A version with high-quality figures appears at http://www.astro.psu.edu/users/edf/NGC6334.pdf
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÐµÐ·ÐµÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐºÐ° Ð´Ð»Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÑÐ½ÑÑ Ð¿ÐµÑÐ°ÑÐ½ÑÑ Ð¿Ð»Ð°Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÑÐ¼Ð±Ð°ÑÐ¾Ð²Ð°, ÐÐ°ÑÐ¸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¿ÐµÑÐ°ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ°
ÑÐ°Ð³Ð¾Ð²ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ
ÑÑÐ°Ð½Ð¾Ðº
ÑÐ°ÑÐ¸ÐºÐ¾Ð²ÑÐµ ÑÐµÐ»ÑÑÐ¾Ð²ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ
ÑÐ°ÑÑÐµÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐ°Ð½ÐºÐ° Ñ Ð§ÐÐ£ Ð´Ð»Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÐ°ÑÐ½ÑÑ Ð¿Ð»Ð°Ñ, Ð²ÑÐ±Ð¾ÑÐ° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ±Ð¾ÑÐ° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð´Ð»Ñ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÐµÐµ Ð½Ð°ÑÑÑÐ¾Ð¹ÐºÐ°.
title: Foster Care for Unaccompanied Immigrant and Refugee Children and Youth
Creators: name: Iii, Robert G. Hasson
name: Evans, Kerri
name: Crea, Thomas M.
Publisher: name: Oxford University Press
Year: 2024

description: Unaccompanied children are immigrants under 18 years old without a parent or guardian at their time of arrival to their host countries. In the United States, the numbers of unaccompanied children arriving at the Southern border have steadily increased since 2012, with a record number arriving in 2023. Many unaccompanied children migrate to the US to escape extreme poverty and community violence, or to reunite with family members. Like other displaced populations, unaccompanied children are vulnerable to further violence and exploitation during their migration journeys and after arrival to the US. Yet, this population is uniquely vulnerable given their developmental needs and often complicated health and mental health challenges.The vast majority of unaccompanied children (98.9%) are placed with community sponsors and are essentially lost to follow up. A small number enter foster care under the auspices of the Office of Refugee Resettlement (ORR), either through the long term foster care program or the unaccompanied refugee minors program. Theis introduction of the paperpaper provides an overview of the foster care process and policies in place to ensure the safety and wellbeing of unaccompanied children who require foster care in the US. There are sections ofs of paper begins with analysis of key policies impacting unaccompanied children, presents information related to ORR’s foster care system in the US, followed by in-depth analysis of the placement process and well-being outcomes from the existing empirical literature. The paper conclusion includesdes with a discussion of future policy developments to ensure the best interests of unaccompanied children are identified and met in the context of rapidly changing circumstances related to global migration.
About the blowup of quasimodes on Riemannian manifolds
Creators: name: Sogge, Christopher D.
name: Toth, John A.
name: Zelditch, Steve
Publisher: name: arXiv
Year: 2009
Subjects: subject: Analysis of PDEs (math.AP)
subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 58J50, 35P20

description: On any compact Riemannian manifold $(M, g)$ of dimension $n$, the $L^2$-normalized eigenfunctions ${ϕ_λ}$ satisfy $||ϕ_λ||_{\infty} \leq C λ^{\frac{n-1}{2}}$ where $-Δϕ_λ = λ^2 ϕ_λ.$ The bound is sharp in the class of all $(M, g)$ since it is obtained by zonal spherical harmonics on the standard $n$-sphere $S^n$. But of course, it is not sharp for many Riemannian manifolds, e.g. flat tori $\R^n/Γ$. We say that $S^n$, but not $\R^n/Γ$, is a Riemannian manifold with maximal eigenfunction growth. The problem which motivates this paper is to determine the $(M, g)$ with maximal eigenfunction growth. In an earlier work, two of us showed that such an $(M, g)$ must have a point $x$ where the set ${\mathcal L}_x$ of geodesic loops at $x$ has positive measure in $S^*_x M$. We strengthen this result here by showing that such a manifold must have a point where the set ${\mathcal R}_x$ of recurrent directions for the geodesic flow through x satisfies $|{\mathcal R}_x|>0$. We also show that if there are no such points, $L^2$-normalized quasimodes have sup-norms that are $o(λ^{n-1)/2})$, and, in the other extreme, we show that if there is a point blow-down $x$ at which the first return map for the flow is the identity, then there is a sequence of quasi-modes with $L^\infty$-norms that are $Ω(λ^{(n-1)/2})$.
description: 20 pages
Monetary and banking system of Turkey
Creators: name: Harmankaya, Nejat Cemil
Publisher: name: University of British Columbia
Year: 2012

description: Although Turkey is a very old country, lying across between the Near East and the West, it has only quite recently acquired a modern system of its money and banking institutions. For the many centuries which preceded the Revolution of 1923 and the institution of the program of Westernization, the prerogative of coinage was exercised by the ruling Sultans as much, it would appear, as a fiscal device for meeting the emergency needs of the royal treasury, as a convenience for the business community. The country's modest banking needs were: supplied by merchants, exchange dealers and casual money lenders. Banking as a separate undertaking did not make its appearance until the middle of the nineteenth century and then legally as a result of the fiscal emergencies in which the Ottoman Rulers bartered banking monopolies and the privilege of issue for the support of the country’s credit abroad. The recipient of the exclusive right of note issue was the British-French owned and operated Osmanli Bankasi which for many years was the country's leading bank. Since 1923 the country has experienced a growth and expansion in the banking structure as the result of the undertaken economic development program which has no parallel in modern history. A major part of this growth has been the consciously planned result of the relative vast reconstruction program through which the government is attempting to modernize the Turkish economy and to exploit its latent natural resources. At the center of this new financial revolution is the Central Bank of the Turkish Republic. Surrounding it are a number of government owned and operated quasi-public institutions charged with the responsibility of carrying out the State's program of industrialization, and the purely private banks. While considerable capital has been obtained from abroad and from domestic saving they have been a substantial part of these investment sources and have not been sufficient to meet the needs of the reconstruction program. During the past few years an increasing reliance has been placed on the issue privilege of the Central Bank, causing a serious decline in the purchasing power of the Turkish Lira. The recovery of the existing inflation in the country would appear to depend upon the by no means certain success of the economic development program. The future of the new banking community would also appear to depend upon the success of this program.
Quanto è vecchia la Via Lattea?
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Grazie a uno studio condotto su svariate migliaia di stelle della nostra galassia, un team internazionale di astronomi è riuscito ad ottenere una mappa cronografica estremamente dettagliata dell’alone galattico. Il risultato sorprendente è che la distribuzione di stelle vecchie sembra estendersi dal centro fino a regioni vicine al Sole
The distance upon contact: Determination from roughness profile
Creators: name: van Zwol, P. J.
name: Svetovoy, V. B.
name: Palasantzas, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: The point at which two random rough surfaces make contact takes place at the contact of the highest asperities. The distance upon contact d_0 in the limit of zero load has crucial importance for determination of dispersive forces. Using gold films as an example we demonstrate that for two parallel plates d_0 is a function of the nominal size of the contact area L and give a simple expression for d_0(L) via the surface roughness characteristics. In the case of a sphere of fixed radius R and a plate the scale dependence manifests itself as an additional uncertainty δd(L) in the separation, where the scale L is related with the separation d via the effective area of interaction L^2\simπRd. This uncertainty depends on the roughness of interacting bodies and disappears in the limit L\to \infty.
description: 5 pages, 4 figures, to be published in PRB
D7.1 – Knowledge Sharing Platforms for Food Systems
Creators: name: Ciolacu, Luminita
Publisher: name: Zenodo
Year: 2024
Subjects: subject: Food
subject: Agricultural waste
subject: Crop waste
subject: valorization
subject: Food waste
subject: Food Loss and Waste

description: WASTELESS will create or become a part of a Knowledge Sharing Platform (KSP) for Food systems as part of its Clustering activities and this document, deliverable D7.1, explains the basis of the decision taken for the WASTELESS project to become a part of the Sustainable Food System Innovation Platform (SFSI Platform). This deliverable provides (i) an overview of KSPs for Food Systems available through a basic desk study search, (ii) a deeper analysis, including technical specifications like: governance, features and exploitation of 5 selected platforms with focus on topics related to WASTELESS: food loss and waste, sustainability and innovation, taking in consideration stakeholders of the value chain, (ii) an analysis of food actors’ knowledge and desires for online platforms through a google form survey and (iv) a critical review of the results presented in accordance with WASTELESS needs and objectives.
title: Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÑ. ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÐºÐ¾Ð² Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸
title: Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð¸Ð½Ð¸Ð½, ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2010
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð°Ñ, Ð½Ð° ÐºÐ¾ÑÐ¾ÑÑÑ Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ ÐºÐ°Ðº Ð²Ð°Ð¶Ð½Ð°Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ°Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÐ°Ð½Ñ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¾ÑÐµÐ½ÐºÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÐºÐ¾Ð² Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸ Ð² Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿ÑÑÐµÐ¼ ÑÐ¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð·Ð°ÑÐ¸ÑÐ½ÑÑ Ð¼ÐµÑ, Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¿Ð¾ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐµÐ½Ð½ÑÑ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ Ð·Ð°Ð´Ð°Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÑ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹ ÐºÐ°ÑÐµÐ´ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ 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°. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 090102.65 Ð¸ 090105.65. ÐÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Ð¿Ð¾Ð»ÐµÐ·ÐµÐ½ Ð´Ð»Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐ¸ÑÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð´ÑÑÐ³Ð¸Ð¼ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑÐ¼.
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°.
Voyager 1 e il confine labile dell’eliosfera
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Ufficialmente ha superato il confine dell’eliosfera nel 2012, ma slitterà “infangata” in un residuo di campo magnetico fino al 2025, quando finalmente raggiungerà una regione di spazio interstellare incontaminata, sperando che nel frattempo la batteria a bordo non si scarichi del tutto
Vento forte….su tutta la galassia
Creators: Francesco D'Alessio
Publisher: name: Media Inaf
Year: 2015

Un team composto da astronomi in larghissima parte italiani ha usato l’interferometro Plateau de Bure sulle alpi francesi, e dati dei satelliti a raggi X Chandra e NuSTAR, per mappare rispettivamente i superventi freddi e caldi nella galassia Mrk 231
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½ÑÑÑÑÐµÐ², ÐÑÑÐµÐ¼
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: ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾Ñ
ÑÐ°ÐºÑÐ¾ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð²Ð°Ð»Ð¾Ð²Ð¾Ð¹ Ð´Ð¾Ñ Ð¾Ð´
Ð¸Ð·Ð´ÐµÑÐ¶ÐºÐ¸ Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ
ÑÐ¾ÑÐ³Ð¾Ð²ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»

description: ÐÐ°Ð½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¡ÐÐÐ¢ÐÂ». ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÐµÑÑÑÑÐ½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÐµÐ³Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾Ð±ÑÑÐ¼Ð° ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½Ð° Ð¾Ð±ÑÑÐ¼ ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¸Ð½Ð´ÐµÐºÑÐ¾Ð² ÑÐµÐ·Ð¾Ð½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´Ð°Ð¶. ÐÐ°Ð»ÐµÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¾ÑÐ¾Ð´Ð¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´Ð°Ð¶, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ ÑÐ°ÐºÑÐ¾ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐºÐ°Ðº ÑÐµÑÐµÐ· Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹, ÑÐ°Ðº Ð¸ Ð¾Ð±Ð¾Ð±ÑÐ°ÑÑÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¸ Ð¿Ð¾Ð´Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÐ¾Ð³Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¡ÐÐÐ¢ÐÂ».
A Study of the Effect of Molecular and Aerosol Conditions in the Atmosphere on Air Fluorescence Measurements at the Pierre Auger Observatory
Creators: name: The Pierre Auger Collaboration
Publisher: name: arXiv
Year: 2010
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The air fluorescence detector of the Pierre Auger Observatory is designed to perform calorimetric measurements of extensive air showers created by cosmic rays of above 10^18 eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group of monitoring instruments to record atmospheric conditions across the detector site, an area exceeding 3,000 km^2. The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierre Auger Observatory since the start of regular operations in 2004, and includes a discussion of the impact of these measurements on air shower reconstructions. Between 10^18 and 10^20 eV, the systematic uncertainties due to all atmospheric effects increase from 4% to 8% in measurements of shower energy, and 4 g/cm^2 to 8 g/cm^2 in measurements of the shower maximum.
description: Accepted for publication in Astroparticle Physics
Ecco come si formano le stelle
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Le stelle massicce si formerebbero allo stesso modo delle stelle di massa inferiore. È quanto emerge da un recente studio secondo cui è stato possibile studiare per la prima volta un oggetto di 25 volte la massa del Sole dove, grazie al potere esplorativo dello strumento ALMA, è stata rivelata una struttura a disco che rispecchia la formazione di stelle di massa più piccola. I risultati su ApJ Letters
Eruption of magnetic flux ropes during flux emergence
Creators: name: Archontis, V.
name: Torok, T.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Aims: We investigate the formation of flux ropes in a flux emergence region and their rise into the outer atmosphere of the Sun. Methods: We perform 3D numerical experiments solving the time-dependent and resistive MHD equations. Results: A sub-photospheric twisted flux tube rises from the solar interior and expands into the corona. A flux rope is formed within the expanding field, due to shearing and reconnection of field lines at low atmospheric heights. If the tube emerges into a non-magnetized atmosphere, the flux rope rises, but remains confined inside the expanding magnetized volume. On the contrary, if the expanding tube is allowed to reconnect with a preexisting coronal field, the flux rope experiences a full eruption with a rise profile which is in qualitative agreement with erupting filaments and Coronal Mass Ejections.
Vision for Research Data & Software management training at TU Delft
Creators: name: Martinez-Lavanchy Paula, M.
name: Dunning, Alastair
name: Teperek, Marta
name: Will, Nicole
name: Verbakel, Ellen
name: Zormpa, Eirini
Publisher: name: Zenodo
Year: 2019
Subjects: Research Data Managament
Training
RDM skills
Research Data training
Software skills
FAIR skills

description: This is TU Delft Library vision for Research Data and Software Management training as part of the education and skills development of students and researchers. The courses (some already available and some in preparation) are organised in four different modules, which build upon each other (Fig. 1). The different levels (from bottom to top) increases the specificity of the content from considering data into a general context (e.g. open science) to skills that apply to a specific data type or a research discipline. The realization of this vision will be a collaborative work of TU Delft Library with different relevant stakeholders within the university (e.g. Data Stewards, researchers, other support services offices, etc.) and with external organizations that have already developed training material and/or courses. This collaborative effort aims at ensuring the sustainability of the training. Status update - October 2021- v2.0 Since the publication of the TU Delft Library ‘Vision for Research Data and Software’ in 2019, the Research Data Services team has focused on the implementation of this vision in collaboration with the Education Support team, the Graduate School, the Faculty Data Stewards, the newly established Digital Competence Centre (DCC) and the TU Delft Data Champions. The publication of version 2.0 of the vision intends to report on the status of the implementation and reflect on what has been achieved. Publishing a new version is also an indication that we see the vision constantly evolving, which should be revised on a regular basis (so new versions are to be expected).
Una boccata d’ossigeno primordiale
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Pubblicato su Nature uno studio, guidato dall'Università di Berna, sulla inaspettata presenza di ossigeno molecolare nella chioma della cometa 67P/Churyumov-Gerasimenko. Ma non si pensi ad aria fresca: sono molecole più vecchie del Sistema Solare stesso
Building Merger Trees from Cosmological N-body Simulations
Creators: name: Tweed, D.
name: Devriendt, J.
name: Blaizot, J.
name: Colombi, S.
name: Slyz, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Although a fair amount of work has been devoted to growing Monte-Carlo merger trees which resemble those built from an N-body simulation, comparatively little effort has been invested in quantifying the caveats one necessarily encounters when one extracts trees directly from such a simulation. To somewhat revert the tide, this paper seeks to provide its reader with a comprehensive study of the problems one faces when following this route. The first step to building merger histories of dark matter haloes and their subhaloes is to identify these structures in each of the time outputs (snapshots) produced by the simulation. Even though we discuss a particular implementation of such an algorithm (called AdaptaHOP) in this paper, we believe that our results do not depend on the exact details of the implementation but extend to most if not all (sub)structure finders. We then highlight different ways to build merger histories from AdaptaHOP haloes and subhaloes, contrasting their various advantages and drawbacks. We find that the best approach to (sub)halo merging histories is through an analysis that goes back and forth between identification and tree building rather than one which conducts a straightforward sequential treatment of these two steps. This is rooted in the complexity of the merging trees which have to depict an inherently dynamical process from the partial temporal information contained in the collection of instantaneous snapshots available from the N-body simulation.
description: 19 pages, 28 figures
Nuovo algoritmo per il mare di Fermi
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Grazie a una nuova simulazione Monte Carlo è ora possibile studiare con maggior dettaglio il comportamento di un mare di Fermi in cui venga introdotta una singola impurità. L’algoritmo mostra che la transizione da quasiparticella a molecola legata è molto semplice e che c’è una fase ambigua, di interazione senza formazione di legame. Interessanti le implicazioni sullo studio dello stato della materia all’interno delle stelle di neutroni
Swift fa mille GRB
Creators: Patrizia Caraveo
Publisher: name: Media Inaf
Year: 2015

Dopo quasi 11 anni dal lancio, ieri, 27 ottobre alle 22:40:40 GMT, la missione Swift* ha rivelato il lampo gamma numero 1000. Si tratta di GRB 151227B, un lampo della durata di circa 50 secondi con una controparte ottica per la quale, poche ore dopo, lo strumento X-Shooter al VLT dell’ESO ha misurato il rispettabile redshift di 4,063 che, tradotto in distanza, ci dice che il lampo è avvenuto a circa 12 miliardi di anni luce da noi, quando l’Universo aveva appena un miliardo e mezzo di anni
Measurements design and phenomena discrimination
Creators: name: Rebollo-Neira, Laura
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The construction of measurements suitable for discriminating signal components produced by phenomena of different types is considered. The required measurements should be capable of cancelling out those signal components which are to be ignored when focusing on a phenomenon of interest. Under the hypothesis that the subspaces hosting the signal components produced by each phenomenon are complementary, their discrimination is accomplished by measurements giving rise to the appropriate oblique projector operator. The subspace onto which the operator should project is selected by nonlinear techniques in line with adaptive pursuit strategies.
Una componente sconosciuta della Via Lattea
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Una componente della Via Lattea prima sconosciuta. E' quanto hanno scoperto alcuni astronomi utilizzando il telescopio VISTA all'Osservatorio dell'ESO al Paranal. Mappando le posizioni di alcune stelle variabili appartenenti alla classe nota come Cefeidi, hanno trovato, nel rigonfiamento centrale, un disco di stelle giovani nascosto dietro a spesse nubi di polvere