cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ ÑÑÑÐ°Ñ Ð¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÐµÐµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ»ÑÑÐ°Ð¡ÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸ÐµÂ»)
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°Ð¹Ð´Ð°ÑÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸
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Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÑ ÑÑÑÐ°Ñ Ð¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ»ÑÑÐ°Ð¡ÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ» Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑ Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ¾Ð² Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ðµ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ¸ÑÐºÐ¾Ð² Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ ÑÐµÐºÑÑÐµÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ»ÑÑÐ°Ð¡ÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ» Ð½Ð° ÑÑÐ½ÐºÐµ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÑÑÐ°ÑÐ¾Ð²ÑÐ¸ÐºÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ¾Ð², Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ»ÑÑÐ°Ð¡ÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ» Ð½ÐµÐ»ÑÐ·Ñ Ð½Ð°Ð·Ð²Ð°ÑÑ Ð°Ð±ÑÐ¾Ð»ÑÑÐ½Ð¾ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²ÑÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÑ Ð´Ð»Ñ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ¾Ð² ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿Ð¾Ð²Ð»ÐµÑÐµÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ðµ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°ÑÐ¾Ð²ÑÐ¸ÐºÐ°. ÐÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¸ÑÐºÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐµÐ´ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾ÑÐ¸Ð½Ð³Ð° Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÑÑÐ°ÑÐ¾Ð²Ð°ÑÐµÐ»ÐµÐ¹. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐºÐ¾ÑÐ¸Ð½Ð³Ð° Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
Near Infrared Spectroscopic Monitoring of EXor variables: First Results
Creators: name: Lorenzetti, D.
name: Larionov, V. M.
name: Giannini, T.
name: Arkharov, A. A.
name: Antoniucci, S.
name: Nisini, B.
name: Di Paola, A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present low resolution (R approximately 250) spectroscopy in the near-IR (0.8 to 2.5um) of the EXor variables. These are the initial results (obtained during the period 2007-2008) from a long term photometric and spectroscopic program aimed to study the variability in the accretion processes of pre-Main Sequence (PMS) stars, by correlating the continuum fluctuations with the spectroscopical properties. Eight sources have been observed in different epochs, for a total of 25 acquired spectra. EXor spectra show a wide variety of emission features dominated by HI recombination (Paschen and Brackett series). We have investigated whether line and continuum variability could be due to a variable extinction, but such hypothesis is applicable only to the peculiar source PV Cep. By comparing the observed spectra with a wind model, mass loss rates in the range (2-10)x10^(-8) M_sun} yr^(-1) are derived, along with other wind parameters. Consistent results are also obtained by assuming that HI lines are due to accretion. CO overtone is also detected in the majority of the sources both in absorption and in emission. It appears to come from regions more compact than winds, likely the stellar photosphere (when in absorption) and the circumstellar disk (when in emission). NaI and CaI IR lines behave as the CO does, thus they are thought to arise in the same locations. For some targets multiple spectra correspond to different activity stages of the source. Those exhibiting the largest continuum variation at 2um (DeltaK > 1 mag) present a significant line flux fading during the continuum declining phases. In particular, CO absorption (emission) appears associated to inactive (active) stages, respectively.
description: To be published in ApJ
title: ÐÑÐ°ÑÐºÐ¸Ð¹ ÑÐ»Ð¾Ð²Ð°ÑÑ ÑÐµÑÐ¼Ð¸Ð½Ð¾Ð² Ð¿Ð¾ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Creators: name: ÐÐ¾Ð»ÑÐºÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÐ¸Ð»Ð¾Ð²Ð°, ÐÐ°Ð»ÐµÐ½ÑÐ¸Ð½Ð°
name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð²Ð° , ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: ÐÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ñ

description: Ð ÑÐ»Ð¾Ð²Ð°ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÑÐ¼Ð¸Ð½Ñ Ð¸ Ð¿Ð¾Ð½ÑÑÐ¸Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸: Ð¾ÑÐ½Ð¾Ð² Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾Ð¹ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð½ÐµÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ Ð¸ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÑÐ¾ÑÐ¼ Ð¶Ð¸Ð·Ð½Ð¸ (Ð²Ð¸ÑÑÑÑ, ÑÐ°Ð³Ð¸, Ð¿ÑÐ¾ÐºÐ°ÑÐ¸Ð¾ÑÑ, ÑÑÐºÐ°ÑÐ¸Ð¾ÑÑ), ÑÐ¼Ð±ÑÐ¸Ð¾Ð³ÐµÐ½ÐµÐ·Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð³ÐµÐ½ÐµÑÐ¸ÐºÐ¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð¹ Ð³ÐµÐ½ÐµÑÐ¸ÐºÐ¸, Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð¾Ð±ÑÐµÐ¹ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸: ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸, ÑÐ¸Ð»Ð¾Ð³ÐµÐ½ÐµÐ·Ð°, ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¼Ð¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸, Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð³ÐµÐ½ÐµÐ·Ñ, ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ð¸ Ð±Ð¸Ð¾ÑÑÐµÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÑÑ ÑÐ¸Ð·Ð¸ÐºÑ Ð¸ Ð±Ð¸Ð¾Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¸Ñ, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ²ÑÐ·Ð°Ð½Ð° Ñ Ð¾Ð±ÑÐµÐ±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹, Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð¹ Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¾Ð¹, Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ Ð²ÑÐ·Ð¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·ÐµÐ½ ÐºÐ°Ðº Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð°Ð¼, ÑÐ°Ðº Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼, Ð¸Ð·Ð±ÑÐ°Ð²ÑÐ¸Ð¼ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÑ ÑÐ²Ð¾ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ, ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ ÐºÐ°Ðº ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½Ð¾Ðµ Ð¸Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 223200.02, Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð´Ð¾ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ°Ðº ÑÐ°ÐºÑÐ¾Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð Ð¾ÑÑ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Ð¾Ð½Ð´Ð°Ðº, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
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ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°
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ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ðµ Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð´Ð¾ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ°Ðº ÑÐ°ÐºÑÐ¾ÑÐ° Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ Ð¸ ÑÑÑÐ½Ð¾ÑÑÐ¸ Ð·Ð´Ð¾ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸; Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ Ð·Ð´Ð¾ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸; Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð·Ð´Ð¾ÑÐ¾Ð²ÑÑ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¸. ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ°ÐºÑÐ¾ÑÐ¾Ð², ÑÐ³ÑÐ¾Ð¶Ð°ÑÑÐ¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð·Ð´Ð¾ÑÐ¾Ð²ÑÑ; Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð¼ÐµÑÑ Ð¿Ð¾ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð·Ð´Ð¾ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸; ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÑÑÑÑ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¿ÑÐ¾ÑÐ¸Ð»Ð°ÐºÑÐ¸ÐºÐ¸ Ð½ÐµÐ¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð°ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð·Ð´Ð¾ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¾Ð¶Ð¸Ð´Ð°ÐµÐ¼ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÑÐ¸ÑÑÐ²Ð°ÐµÑÑÑ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð½Ð°Ñ Ð¿ÑÐ¾Ð´Ð¾Ð»Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð° 2016-2020 Ð³Ð³. Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¿ÑÐ¾ÑÐ¸Ð»Ð°ÐºÑÐ¸ÐºÐ¸ Ð½ÐµÐ¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð° Ð¶Ð¸Ð·Ð½Ð¸.
Axinos as Dark Matter Particles
Creators: name: Covi, Laura
name: Kim, Jihn E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The identification of dark matter in our particle physics model is still a very open question. Here we will argue that axinos can be successful dark matter candidates in models with supersymmetry and the axion solution of the strong CP problem. Axinos can be the lightest supersymmetric particle (LSP), or can be heavier than the LSP. Axinos can be produced in the right abundance by thermal scatterings and if they are the LSP also by out of equilibrium decays of the lightest superpartner of SM fields (LSPSMs). On the other hand heavier (not LSP) axinos can generate a part of the neutralino LSP dark matter. Depending on the nature of the supersymmetric spectrum, and if R-parity is strictly conserved or slightly broken, very different signals of the LSP axino scenario can arise at colliders and in astrophysics.
description: 15 pages, 2 figures, invited contribution to NJP Focus Issue on 'Dark Matter and Particle Physics'
L’Etiopia alla scoperta dell’universo
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Il secondo stato più popoloso dell'Africa sta per inaugurare una struttura da 3 milioni di dollari americani che potrà competere con gli osservatori più all'avanguardia. Il programma spaziale non si ferma qui: l'Etiopia sta progettando anche un satellite e un razzo spaziale
Certain studies on the digestive enzyme systems (sucrase, maltase and lactase) of the small intestine of the Wistar rat
Creators: name: Bose, Robert John
Publisher: name: University of British Columbia
Year: 2012

description: The primary objective of this study was to establish the nature and extent of the changes with age in sucrase, maltase and lactase activity in the small intestine of the laboratory Wistar rat, raised on a basal diet. The author was, in addition, interested in the possibility of these changes being brought about by the presence or absence of certain specific dietary factors. Analysis have shown marked changes in the activities of these three enzymes with advancing age in Wistar rats weaned at 21 days on to a basal diet. Lactase activity was found to remain at a high level from 18 to 20 days during which time a sharp and uniform drop in activity was indicated. The extent of this drop was found to be great, approximately 80 per cent of the pre-weaned level. In contrast sucrase activity of the small intestine in the pre-weaned rat was negligible and underwent a sharp increase in activity at the weaning age of 21 days. Maltase activity in the pre-weaned Wistar rat was appreciable and was found to increase significantly at weaning. Early weaning at 15 days brought about an earlier decline in lactase activity and a corresponding early rise in sucrase and maltase activities. When early weaning was immediately followed by the feeding of condensed milk no apparent maintenance of lactase activity was noted. Similarily when older rats, 28 days of age, were fed condensed milk no increase in lactase activity was apparent. Neither the condensed milk nor basal diets induced apparent differences on the effect of early weaning on sucrase and maltase activity. Apparent maintenance of lactase activity above those levels demonstrated in rats weaned at 21 days on to a basal diet was accomplished by fostering 16 day old rats on dams which had littered from four to five days prior to this transfer and which were assumed to be lactating at a somewhat greater rate than had the original mothers. It was noted however that this fostering process had no apparent influence on the extent of the changes in sucrase and maltase activities. The feeding of purified sugar diets containing two different levels of each of the three sugars, sucrose, maltose and lactose, had little effect on any of the three carbohydrases studied. Growth rates of the rats on these purified diets showed marked differences. The author suggests that the maintenance of lactase activity might be associated with the presence of an inductive component present in the milk of the freshly lactating dam, a component not necessarily present in the milk of the later period of lactation, and not necessarily a component of processed cow's milk. The absence of an adaptive lactase response to the feeding of lactose in this study and those of other workers suggest that lactose itself is unlikely this inducer. No adaptive response to substrates could be demonstrated for either sucrase or maltase.
title: ÐÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð´ÑÐ°ÑÑÐµÐ², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2011
Subjects: ÐÐµÑÐ°Ð»Ð»Ñ

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¿ÑÑÐ³Ð¸Ðµ Ð¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·ÑÑÑÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð¸ ÑÐ¿Ð»Ð°Ð²Ð¾Ð². ÐÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ ÑÐ¿Ð¾Ñ ÑÐ´ÐµÐ»Ð°Ð½ Ð½Ð° Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ñ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÐ¼, ÑÑÑÑÐºÑÑÑÐ¾Ð¹ Ð¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¾ÑÑÐ°Ð²Ð¾Ð¼ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð². ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð² Ð»Ð¸ÑÐ¾Ð¼, Ð´ÐµÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¼ Ð¸ ÑÐµÑÐ¼Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¼ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸ÑÑ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÐ¼ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð¸ ÑÐ¿Ð»Ð°Ð²Ð¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²ÐµÐ´ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ âÐÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²â Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² âÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ñâ. ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð² ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ñ.
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°.
Ceratotingis zeteki Drake 1950
Creators: name: Costa, Sara Itzel Montemayor and Luiz Antônio Alves
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Tingidae
Ceratotingis
Ceratotingis zeteki

description: Ceratotingis zeteki (Drake, 1950) (Figs 2H, 3H, 4H, 5Hand 6D) Macrotingis zeteki Drake, 1950: 299; Drake & Ruhoff, 1965: 294; Froeschner, 2003: 29. Ceratotingis zeteki: Montemayor, 2008: 448. Diagnosis. General colour yellowish brown. Cuticle anterodorsal to eyes with same characteristics as the rest of the head. Occipital spines gradually diverging. Segment Iapproximately five times longer than the head. Hood well developed. Median pronotal carina same height along its entire length. Paranota with two rows of areolae. Mesosternal lamina subparallel. Costal area with two rows of areolae. Total body length (male holotype): 4.79. Type material examined. Holotype: ♂, Panama, Barro Colorado IS., Canal Zone, vii.1946 (NMNH). Distribution (Fig. 7). Panama. Discussion. Ceratotingis zeteki can be distinguished from other members of the genus as it has a biseriate costal area.
description: Published as part of Costa, Sara Itzel Montemayor and Luiz Antônio Alves, 2009, Systematic revision of Macrotingis and phylogenetic analysis of the genera Macrotingis and Ceratotingis (Heteroptera: Tingidae), pp. 631-642 in European Journal of Entomology 106 (4) on page 639, DOI: 10.14411/eje.2009.079, http://zenodo.org/record/3564588
description: {"references": ["DRAKE C. J. 1950: Anew tingid from the Canal Zone (Hemiptera). Proc. Entomol. Soc. Wash. 52: 299 - 300.", "DRAKE C. J. & RUHOFF F. A. 1965: Lacebugs of the world: A Catalog (Hemiptera: Tingidae). Bull. U. S. Nat. Mus. 243: 1 - 634.", "FROESCHNER R. C. 2003: Review of the Middle American Lace Bug genus Macrotingis (Heteroptera: Tingidae) with a key and anew species from Mexico. Entomol. News 114: 29 - 32.", "MONTEMAYOR S. I. 2008: Anew genus and two new species of Tingidae (Heteroptera) from Central America. Zool. Sci. 25: 444 - 450."]}
title: Ð¤Ð¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
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¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ
ÑÑÐ°Ð²ÐºÐ° Ð´Ð¸ÑÐºÐ¾Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð±ÑÐµÑÑÐ²Ð¾ Ñ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÑ Â«ÐÐ  Ð¤ÐµÑÐ½Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð»Ð°Ð½Ð° Ð¿Ð¾ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð¸ ÑÐ°ÑÑÐµÑ ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð», ÑÑÐ¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ ÑÐ°ÑÑÐ¸ÑÑÑÑÑÑ (Ð¾ÑÐºÑÑÐ²Ð°ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¾ÑÐ³Ð¾Ð²ÑÐµ ÑÐ¾ÑÐºÐ¸). Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð»Ð°Ð½ Ð¿Ð¾ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð¸ ÑÐ´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ Ð½Ð° Ð³Ð¾Ð´ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°.
Simple proof of the completeness theorem for second order classical and intuitionictic logic by reduction to first-order mono-sorted logic
Creators: name: Nour, Karim
name: Raffalli, Christophe
Publisher: name: arXiv
Year: 2009
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics

description: We present a simpler way than usual to deduce the completeness theorem for the second-oder classical logic from the first-order one. We also extend our method to the case of second-order intuitionistic logic.
Mercurio strattonato da Giove?
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Grazie alle misure altimetriche della sonda spaziale MESSENGER, si è potuto determinare che la velocità di rotazione su sé stesso di Mercurio è, in media, un po’ più veloce di quanto misurato da Terra. Una delle spiegazioni possibili è l'influsso del campo gravitazionale gioviano
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹
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»Ð¸ÑÐ¸Ð½Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
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: Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð¦ÐµÐ»ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÑÑÐ¿Ð¿Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ Ð¡Ð°ÑÑÑÐ½Â». ÐÐ»Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°, Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°, ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ° Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ² Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð·Ð° Ð¿Ð¾ÑÐ»ÐµÐ´Ð½Ð¸Ðµ 10 Ð»ÐµÑ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐÐÐ Â«ÐÑÑÐ¿Ð¿Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ Ð¡Ð°ÑÑÑÐ½Â» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐ»Ð¸ Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ. ÐÑÐ¾Ð³Ð½Ð¾Ð·Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» ÑÐ´ÐµÐ»Ð°ÑÑ Ð²ÑÐ²Ð¾Ð´ Ð¾ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ.
Field-based Determination of Critical Power and Critical Speed Among Recreational Runners
Creators: name: Ledger, Adam
Publisher: name: UH Research Archive
Year: 2022
Subjects: Wearable Technology
Field Tests
Critical Speed
Recreational Runners
Relationship

description: Background Critical power (CP) is a highly regarded threshold, delineating the boundary between heavy and severe intensities of exercise. Determination of CP has long been hindered by testing protocols that are time consuming and require maximal effort. The aim was to investigate the relationship and reliability of field-based methods of determining CP/critical speed (CS) among recreational runners. Method 23 participants (women n = 4, male n = 19; age = 45 ± 7 years, height =178 ± 7 cm, mass = 83.3 ± 22.6 kg) completed six weeks of habitual training (HAB), consisting of the participant continuing their preexisting program. This was then followed by three individual time trial (TT) efforts across a one week period, the durations of which being 3, 7 and 12 minutes for all participants. Then three, two 3-minute all out tests (3MT) were completed across another one-week period, these consisted of running for 3 minutes at a maximal sprint from start to finish. A leading foot pod was worn during all activities, allowing for data to be recorded remotely and trials to be self-administered by participants due to COVID-19 restrictions. CS, CP, W′ and D′ was calculated from each of these sets of data and compared. Results No significant difference was observed between CSHAB (3.44 ± 0.47 m·s-1) and CSTT (3.50 ± 0.53 m·s-1), CPHAB (282 ± 42 W) and CPTT (288 ± 44 W), D′HAB (113 ± 75 m) and either D′TT (141 ± 35 m) or D′3MT (81 ± 42 m), and W′HAB (7.73 ± 4.63 kJ) and either W′TT (9.32 ± 3.46 kJ) or W′3MT (5.03 ± 2.77 kJ) (p > 0.05). Of these, a good level of agreement was observed between CSHAB and CSTT (r = 0.858, p < 0.001, CoV = 5.6 %) in addition to between CPHAB and CPTT (r = 0.869, p < 0.001, CoV =6.0 %). A lower level of agreement was observed between D′HAB and D′3MT (r = 0.478, p = 0.021, CoV = 50.6 %) with all other pairs showing no significant correlation (p > 0.05). No significant difference was observed across 3MT1 and 3MT2 for CS (3MT1: 3.75 ± 0.57 m·s-1, 3MT2: 3.78 ± 0.57 m·s-1),CP (3MT1: 305 ± 53 W, 3MT2: 307 ± 51 W), D′ (3MT1:87 ± 45 m, 3MT2: 75 ± 45 m) or W′ (3MT1: 5.21 ± 2.86 kJ, 3MT2: 4.86 ± 3.17 kJ) (p > 0.05). Agreement was high across 3MT1 and 3MT2 for CS and CP (CoV = 4.3 % and 3.7 % respectively), but lower for D′ and W′ (54.7 % and 113.3 %). Conclusion Estimating CS and CP from HAB training data appears to be a valid method of determination that requires no intentional bouts or expensive equipment. Determination of D′ and W′ using this method, however requires great caution. The 3MT was found to be reliable for CP and CS but not D′ and W′, however the 3MT should not be administered without proper supervision.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¼Ð½Ð¾Ð³Ð¾Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÐ°Ð½ÐºÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð²ÑÐ·Ð¾Ð²
titleType: Subtitle
Creators: name: ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
name: ÐÑÐ±Ð°ÑÐµÐ², Ð®ÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐÐÐ°Ñ
Year: 1997
Subjects: ÐÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ðµ ÑÑÐ°Ð½ÐºÐ¸ Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð½Ð¾Ð³Ð¾Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÐ°Ð½ÐºÐ¾Ð² ÑÐ²ÐµÑÐ»Ð¸Ð»ÑÐ½Ð¾-ÑÑÐµÐ·ÐµÑÐ½Ð¾-ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð¹ Ð³ÑÑÐ¿Ð¿Ñ. ÐÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ»ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ð¹, ÑÐµÐ¶ÑÑÐ¸Ñ Ð¸ Ð²ÑÐ¿Ð¾Ð¼Ð¾Ð³Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð². ÐÑÑÐ°Ð¶ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ¸Ð¿Ð¾Ð²ÑÐµ ÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°ÑÐ½ÑÑ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐµÐ¹. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÑÑÐ°Ð½ÐºÐ¾Ð² Ñ Ð§ÐÐ£.
On $D$-spaces and Discrete Families of Sets
Creators: name: Dzamonja, Mirna
Publisher: name: arXiv
Year: 2008
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 03E35, 54E20, 03E55

description: We prove several reflection theorems on $D$-spaces, which are Hausdorff topological spaces $X$ in which for every open neighbourhood assignment $U$ there is a closed discrete subspace $D$ such that \[ \bigcup\{U(x): x\in D\}=X. \] The upwards reflection theorems are obtained in the presence of a forcing axiom, while most of the downwards reflection results use large cardinal assumptions. The combinatorial content of arguments showing that a given space is a $D$-space, can be formulated using the concept of discrete families. We note the connection between non-reflection arguments involving discrete families and the well known question of the existence of families allowing partial transversals without having a transversal themselves, and use it to give non-trivial instances of the incompactness phenomenon in the context of discretisations.
description: and old paper, the previous version on arxiv only contained the latex macros
Additional file 1 of Influence of SARS-CoV-2 surveillance outputs produced by the UK health security agency (UKHSA) outbreak surveillance team on decision-making by local stakeholders
Creators: name: Willgert, Katriina
name: Hardstaff, Jo
name: Shadwell, Stephanie
name: Bhattacharya, Alex
name: Blomquist, Paula
name: Vivancos, Roberto
name: Simms, Ian
Publisher: name: figshare
Year: 2023
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences

description: Supplementary Material 1
CRESST va a caccia di ‘pesi piuma’
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Diversi modelli suggeriscono che la massa delle particelle di materia oscura si trovi al di sotto del valore previsto per le WIMP, le particelle maggiormente candidate. Oggi, grazie alla sensibilità dell’esperimento CRESST, situato nel più grande laboratorio sotterraneo del mondo, gli scienziati hanno fatto un passo importante verso la ricerca di particelle più leggere. I risultati sono riportati sull’European Physical Journal C
Coannihilation Scenarios and Particle Spectroscopy in SU(4)_c x SU(2)_L x SU(2)_R
Creators: name: Gogoladze, Ilia
name: Khalid, Rizwan
name: Shafi, Qaisar
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We identify a variety of coannihilation scenarios in a supersymmetric SU(4)_c x SU(2)_L x SU(2)_R model with discrete left-right symmetry. Non-universal gaugino masses, compatible with the gauge symmetry, play an essential role in realizing gluino and bino-wino coannihilation regions that are consistent with the WMAP dark matter constraints. We also explore regions of the parameter space in which the little hierarchy problem is partially resolved. We present several phenomenologically interesting benchmark points and the associated sparticle and Higgs mass spectra.
description: 16 pages, 5 figures and 1 table
Understanding enablers and barriers to using technology with people with aphasia
Creators: name: Dubas, Emily
name: Godlove, Jason
name: Swathi Kiran
name: Gerst, Kyle
Publisher: name: F1000 Research Limited
Year: 2019

description: Introduction:
Research has shown that people with aphasia (PWA) can show improvement for years after onset.  Despite this, barriers such as insurance, geography, and limited services impact access to more therapy.  With technology becoming more prevalent, research has investigated technology-based aphasia rehabilitation.  When considering the LPAA framework, technology could fall into several categories including participating in life situations (e.g. emailing), communication environment (e.g. FaceTime), and targeting impairments (e.g. therapy  applications). While technology-based research shows promise, the feasibility of PWA using technology outside of the laboratory or clinic is not well understood.

Methods:
Constant Therapy (CT) is a technology used by PWA. We examined user demographics (e.g. age, gender, time post-onset, education, geography) to understand what characteristics result in more successful use of CT. Sample includes 3367 users endorsing language deficits. Activity metrics examined were number of sessions in the first 20 weeks and the average number of active days/week.
Results:
Individuals >70-years-old completed fewer sessions and had fewer active days/week compared to individuals 51-70. Those in the chronic stage completed more sessions than the acute stage. There was no significant association between time post-onset and average active days/week. Gender and education were not significantly different to any activity metric. Analyses associated with geographic location will be discussed.
Discussion:
Results suggest gender, time post-onset, and education do not pose a significant barrier to engagement. Although older PWA (>70) were observed to be less active compared to 51-70 group, they still showed a considerable activity, suggesting that adults at any age can benefit from accessing digital therapies.  In this poster, we discuss CT data and whether the results appear consistent with current practice, as well as what are the enablers and barriers to access and use technology.
title: ÐÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð¸ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÑ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ PR Ð¸ ÑÐµÐºÐ»Ð°Ð¼Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼Ð¾Ð´ÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð»Ñ Â«Rise UpÂ»)
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ÐµÐ³Ð¾ÑÑÐ°ÐµÐ²Ð°, ÐÐ½Ð°ÑÑ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: 2018
Subjects: Ð¼Ð¾Ð´ÐµÐ»ÑÐ½ÑÐµ Ð°Ð³ÐµÐ½ÑÑÐ²Ð°
Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐµÐºÐ»Ð°Ð¼Ð°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ PR Ð¸ ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÑ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð¸ PR Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð° Â«Rise UpÂ» Ð¿Ð¾ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° ÑÑÐ½ÐºÐµ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ PR Ð¸ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð° Â«Rise UpÂ».
Additional file 2 of Influence of SARS-CoV-2 surveillance outputs produced by the UK health security agency (UKHSA) outbreak surveillance team on decision-making by local stakeholders
Creators: name: Willgert, Katriina
name: Hardstaff, Jo
name: Shadwell, Stephanie
name: Bhattacharya, Alex
name: Blomquist, Paula
name: Vivancos, Roberto
name: Simms, Ian
Publisher: name: figshare
Year: 2023
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences

description: Supplementary Material 2
Anisotropic evolution of a D-brane
Creators: name: Gusin, Pawel
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The evolution of a probe D-brane in the p-brane background has been considered. The anisotropic evolution of the world-volume of the D-brane with a given topology of a world-volume in a form of a direct product of a n-dimensional flat space and (3-n)-dimensional sphere has been obtained. In this case the anisotropy is described with the aid of two parameters (Hubble parameters). The special case of this evolution, namely the isotropic evolution corresponds to equality of these two parameters. In the latter case the masses and charges of the background p-branes have been derived.
Alfven Wave Reflection and Turbulent Heating in the Solar Wind from 1 Solar Radius to 1 AU: an Analytical Treatment
Creators: name: Chandran, Benjamin D. G.
name: Hollweg, Joseph V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We study the propagation, reflection, and turbulent dissipation of Alfven waves in coronal holes and the solar wind. We start with the Heinemann-Olbert equations, which describe non-compressive magnetohydrodynamic fluctuations in an inhomogeneous medium with a background flow parallel to the background magnetic field. Following the approach of Dmitruk et al, we model the nonlinear terms in these equations using a simple phenomenology for the cascade and dissipation of wave energy, and assume that there is much more energy in waves propagating away from the Sun than waves propagating towards the Sun. We then solve the equations analytically for waves with periods of hours and longer to obtain expressions for the wave amplitudes and turbulent heating rate as a function of heliocentric distance. We also develop a second approximate model that includes waves with periods of roughly one minute to one hour, which undergo less reflection than the longer-period waves, and compare our models to observations. Our models generalize the phenomenological model of Dmitruk et al by accounting for the solar wind velocity, so that the turbulent heating rate can be evaluated from the coronal base out past the Alfven critical point - that is, throughout the region in which most of the heating and acceleration occurs. The simple analytical expressions that we obtain can be used to incorporate Alfven-wave reflection and turbulent heating into fluid models of the solar wind.
description: 9 pages, 9 figures, accepted for publication in ApJ
title: PÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²Ð¸Ð½ÑÐ¸Ð¸ ÐÑÐ¾Ð½Ð¸Ð½ ÐÐÐ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÑÐ½Ñ Ð®Ð½Ð±Ð¸Ð½Ñ
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: Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ
ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐµÐ³Ð¸Ð¾Ð½Ð¾Ð²

description: ÐÐ½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ³Ð¸Ð¾Ð½Ð° Ð¸Ð³ÑÐ°ÐµÑ Ð²Ð°Ð¶Ð½ÑÑ ÑÐ¾Ð»Ñ Ð² ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ. ÐÐ±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÐºÐ°Ðº ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹, ÑÐ°Ðº Ð¸ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¸Ð¼Ð¿Ð¾ÑÑÐ¾Ð·Ð°Ð¼ÐµÑÐµÐ½Ð¸Ñ. ÐÐ¼Ð¿Ð¾ÑÑÐ¾Ð·Ð°Ð¼ÐµÑÐµÐ½Ð¸Ðµ - ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ðµ Ð¸Ð»Ð¸ Ð¿ÑÐµÐºÑÐ°ÑÐµÐ½Ð¸Ðµ Ð¸Ð¼Ð¿Ð¾ÑÑÐ° Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð²Ð°ÑÐ° Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð² ÑÑÑÐ°Ð½Ðµ ÑÐ¾Ð³Ð¾ Ð¶Ðµ Ð¸Ð»Ð¸ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ÑÐ½ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð². ÐÐ¾Ð´Ð¾Ð±Ð½ÑÐµ ÑÐ¾Ð²Ð°ÑÑ Ð½Ð°Ð·ÑÐ²Ð°ÑÑ Ð¸Ð¼Ð¿Ð¾ÑÑÐ¾Ð·Ð°Ð¼ÐµÑÐ°ÑÑÐ¸Ð¼Ð¸. ÐÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð¸Ð¼Ð¿Ð¾ÑÑÐ¾Ð·Ð°Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð´Ð»Ñ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐÐ°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸. ÐÐ°Ð¶Ð½Ð¾ Ð¾ÑÐ¼ÐµÑÐ¸ÑÑ, ÑÑÐ¾ Ð´Ð»Ñ Ð°Ð´ÐµÐºÐ²Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¿Ð¾ÑÑÐ¾Ð·Ð°Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ ÑÑÐ¸ÑÑÐ²Ð°ÑÑ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÑ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸: ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð´Ð¾ÑÑÑÐ¿Ð½ÑÐ¹ Ð¾Ð±ÑÐµÐ¼ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² Ð½Ð¾Ð²ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ, Ð¾ÑÑÐ°ÑÐ»ÐµÐ²ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÐ°Ð½Ñ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð°. ÐÑÐ¾Ð¼Ðµ ÑÑÐ¾Ð³Ð¾, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸Ð¼Ð¿Ð¾ÑÑÐ¾Ð·Ð°Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð½Ð° ÑÑÐ¾Ð²Ð½Ðµ Ð¿ÑÐ¾Ð²Ð¸Ð½ÑÐ¸Ð¹ ÐÐÐ .
La galassia irregolare iperattiva
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Grazie ai dati raccolti da ALMA, un team internazionale di astronomi ha scoperto la presenza di formazione stellare all’interno di una galassia nana irregolare, dove in teoria la formazione di nuove stelle dovrebbe essere molto poco probabile. La scoperta rimette in discussione i modelli di evoluzione delle galassie
Come ti scovo le prime galassie
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Un nuovo metodo statistico di analisi delle riprese infrarosse realizzate da Hubble e proposto da un gruppo di astronomi guidato da ricercatori dell’Università della California, a Irvine, indica che, quasi 13 miliardi di anni fa, c'erano molte più galassie di quanto si pensasse finora. Il commento di Adriano Fontana (INAF)
Additional file 1 of Investigating the effect of nanolime treatment on the drying kinetics of Clipsham limestone
Creators: name: Browne, Dáire E.
name: Peverall, Robert
name: Ritchie, Grant A. D.
name: Viles, Heather A.
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Scanning electron microscopy images of a control sample, E5 sample and E25 sample after 28 day curing period at T = 20 °C, % RH = 75. Table S1. Sample variation, pre- and post-treatment with E5. Table S2. Sample variation, pre- and post-treatment with E25. Table S3. Temperature dependence, pre- and post-treatment with E5. Table S4. Temperature dependence, pre- and post-treatment with E25.
title: Ð§ÐµÐ»Ð¾Ð²ÐµÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾Ð¹ Ð»ÐµÐ±ÐµÐ´ÐºÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð¿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: 2016
Subjects: ÐÐ½ÑÐµÑÑÐµÐ¹ÑÑ
ÐÐµÐ±ÑÐ´ÐºÐ¸
"Ð§ÐµÐ»Ð¾Ð²ÐµÐº Ð¸ Ð¼Ð°ÑÐ¸Ð½Ð°", ÑÐ¸ÑÑÐµÐ¼Ð°
Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÑÐºÐ°Ñ Ð¿Ð°Ð½ÐµÐ»Ñ
ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
human-machine interfaces
winchs
operator panel
control systems

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÐºÐ¾ÑÐ°Ð±ÐµÐ»ÑÐ½Ð°Ñ Ð»ÐµÐ±ÐµÐ´ÐºÐ° Ð¼Ð¸Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð»ÑÑÐ¸ÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° 12700 âÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ¸Ñâ. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ HMI ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÐ·ÑÑÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÑÐµÐ´ÑÑÐ² Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð²ÑÐ±Ð¾Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾-Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð´Ð»Ñ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ° ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð»ÐµÐ±ÐµÐ´ÐºÐ¸ Ð¼Ð¸Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð»ÑÑÐ¸ÐºÐ°. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»Ñ.
description: Object of research: ship winch of a minesweeper of the project 12700 âAlexandriteâ. Purpose of research: design of HMI of a control system. The technology of design of the user interface is studied. Comparison of an automation equipment and control is carried out. A choice of software and hardware tools for the human machine interface of control system of the ship winch of a minesweeper is made. Design of the human-machine interface is executed. The instruction of the user is developed.
The ground state energy of the weakly interacting Bose gas at high density
Creators: name: Giuliani, Alessandro
name: Seiringer, Robert
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mathematical Physics (math-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We prove the Lee-Huang-Yang formula for the ground state energy of the 3D Bose gas with repulsive interactions described by the exponential function, in a simultaneous limit of weak coupling and high density. In particular, we show that the Bogoliubov approximation is exact in an appropriate parameter regime, as far as the ground state energy is concerned.
description: RevTeX4, 16 pages
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸ ÑÑÐµÐ´ÑÑÐ² Ð·Ð°ÑÐ¸ÑÑ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¸Ñ Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¾Ñ Ð¸ÑÐºÑÐ¾Ð²ÑÑ Ð¸ Ð´ÑÐ³Ð¾Ð²ÑÑ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð² Ð½Ð¸Ð·ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐµÑÑ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Ð¸Ñ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: 2016
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ
Ð£ÐÐÑ
ÐÐ­Ð
Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÐµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°Ð·ÑÑÐ´Ñ
Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
UZIs
AER
neural networks

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð±ÑÐ»Ð° Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð´ÐµÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð·ÑÑÐ´Ð¾Ð². Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð±ÑÐ» Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ñ ÐÐÐ Ð¡ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹. Ð ÑÐµÑÐ²ÐµÑÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð£ÐÐÑ. Ð Ð¿ÑÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð±ÑÐ»Ð¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ðµ Ð£ÐÐÑ Ð½Ð¾ÑÐ¼Ð°Ð¼ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð°.
description: In the first chapter of the work it has been defined to date. The second chapter discussed the main methods of detection of emergency electrical discharges. The third chapter has been proposed a method of analyzing emergency processes NVRS using neural networks. The fourth chapter describes the economic efficiency UZIs. In the fifth chapter was reviewed UZIs compliance norms of the Russian legislation.
XMASS: i primi risultati sulla materia oscura
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

I risultati preliminari dell'esperimento giapponese XMASS contraddicono i dati di un altro precedente test sulla modulazione annua di un segnale che potrebbe essere correlato alla presenza di materia oscura. E' quanto emerge dalla conferenza Topics in Astroparticle and Underground Physics che si sta svolgendo in questi giorni a Torino
Nao, il robot dalla memoria di ferro
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Questo piccolo robottino è stato dotato di un memoria autobiografica, che permetterà di rendere più agevoli i cambi tra i diversi equipaggi a bordo della ISS. Nao aiuterà gli astronauti a svolgere compiti complicati e missioni di bordo tramite la conoscenza acquisita con i precedenti membri dell'equipaggio
Target mass corrections and beyond
Creators: name: Accardi, Alberto
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I examine the uncertainty of perturbative QCD factorization for (un)polarized hadron structure functions in deep inelastic scattering at a large value of the Bjorken variable xB. The focus will be on Target Mass Corrections and Jet Mass Corrections in the collinear factorization framework.
description: 4 pages, 1 figure. Talk given at "SPIN2008", University of Virginia, October 6-11 2008
Van Gogh e le Nubi di Magellano
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

La Piccola e la Grande Nube di Magellano in un nuovo affascinante scatto del satellite europeo Planck. Il mix di emissioni provenienti da stelle, galassie e radiazione cosmica di fondo regalano all’insieme una curiosa atmosfera da quadro espressionista