cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The unusual spectral energy distribution of LBQS 0102-2713
Creators: name: Boller, Th.
name: Linguri, K.
name: Heftrich, T.
name: Weigand, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have studied the SED of the quasar LBQS 0102-2713. The available multiwavelength data are one optical spectrum between 3200 and 7400 A, 7 HST FOS spectra between 1700 and 2300 A, one GALEX NUV flux density and a K_S magnitude obtained from NED, and 3 public ROSAT PSPC pointed observations in the 0.1$-$2.4 keV energy band. The alpha_ox values obtained are -2.3 and -2.2, respectively, comparable to BAL quasars. The ROSAT photon index is 6.0+-1.3. The 2500 A luminosity density is about a factor of 10 higher compared to the mean of the most luminous SDSS quasars. We argue that the object might be indicative for a new class of quasars with an unusual combination in their UV-, X-ray, and N_H properties.
description: 16 pages, 8 figures, accepted by ApJ
การถ่ายทอดเทคโนโลยีและการใช้งานแอปพลิเคชันธุรกิจตรวจสภาพรถ
Creators: name: เบญจรัตน์ ศิริชู
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: การถ่ายทอดเทคโนโลยี
การใช้งาน
แอปพลิเคชัน
ธุรกิจตรวจสภาพรถ

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 1-13
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÑÐµÑÑÐ¾ÑÐ°Ð½Ð½Ð¾Ð¼ Ð±Ð¸Ð·Ð½ÐµÑÐµ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð¢Ð¾Ðº Ð Ð°Ð¹ÑÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÐºÐ¾Ð²Ð°, 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¿ÐµÑÑÐ¾Ð½Ð°Ð»
Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
Ð¿ÑÐ¸ÑÐ¸Ð½Ñ ÑÐ²Ð¾Ð»ÑÐ½ÐµÐ½Ð¸Ñ
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð¢Ð¾Ðº Ð Ð°Ð¹ÑÂ». ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ° ÑÐµÑÑÐ¾ÑÐ°Ð½Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¸ÑÐ¸Ð½ ÑÐ²Ð¾Ð»ÑÐ½ÐµÐ½Ð¸Ð¹, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÑÐ¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐºÑÑÐ¸Ðµ Ð·Ð°ÑÑÐ°ÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð·Ð°Ð¿ÑÑÐºÐ°Ð¼Ð¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. ÐÐ°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ Ð¾Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÑÑÐ´Ð°, Ð²ÑÑÐ°Ð¶Ð°ÑÑÐ¸ÑÑÑ Ð² Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ð¸ ÑÐ¿ÑÐ¾ÑÐ° Ð½Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ, ÑÐ²Ð»ÑÐµÑÑÑ Ð¼Ð¾ÑÐ½ÑÐ¼ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð¼ Ð´Ð»Ñ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð¸ÑÐ¸Ð°ÑÐ¸Ð²Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°.
Paranal-La Palma: ecco i siti per CTA
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Il Cherenkov Telescope Array sarà una batteria di telescopi destinati a studiare le sorgenti di radiazione gamma provenienti dall’Universo che, una volta realizzato, sarà il più potente e sensibile osservatorio per i raggi gamma mai costruito
The Build-Up of the Hubble Sequence in the COSMOS Field
Creators: name: Oesch, P. A.
name: Carollo, C. M.
name: Feldmann, R.
name: Hahn, O.
name: Lilly, S. J.
name: Sargent, M. T.
name: Scarlata, C.
name: Aller, M. C.
name: Aussel, H.
name: Bolzonella, M.
name: Bschorr, T.
name: Bundy, K.
name: Capak, P.
name: Ilbert, O.
name: Kneib, J. -P.
name: Koekemoer, A. M.
name: Kovac, K.
name: Leauthaud, A.
name: Floc'h, E. Le
name: Massey, R.
name: McCracken, H. J.
name: Pozzetti, L.
name: Renzini, A.
name: Rhodes, J.
name: Salvato, M.
name: Sanders, D. B.
name: Scoville, N.
name: Sheth, K.
name: Taniguchi, Y.
name: Thompson, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use ~8,600 >5e10 Msol COSMOS galaxies to study how the morphological mix of massive ellipticals, bulge-dominated disks, intermediate-bulge disks, bulge-less disks and irregular galaxies evolves from z=0.2 to z=1. The morphological evolution depends strongly on mass. At M>3e11 Msol, no evolution is detected in the morphological mix: ellipticals dominate since z=1, and the Hubble sequence has quantitatively settled down by this epoch. At the 1e11 Msol mass scale, little evolution is detected, which can be entirely explained with major mergers. Most of the morphological evolution from z=1 to z=0.2 takes place at masses 5e10 - 1e11 Msol, where: (i) The fraction of spirals substantially drops and the contribution of early-types increases. This increase is mostly produced by the growth of bulge-dominated disks, which vary their contribution from ~10% at z=1 to >30% at z=0.2 (cf. the elliptical fraction grows from ~15% to ~20%). Thus, at these masses, transformations from late- to early-types result in disk-less elliptical morphologies with a statistical frequency of only 30% - 40%. Otherwise, the processes which are responsible for the transformations either retain or produce a non-negligible disk component. (ii) The bulge-less disk galaxies, which contribute ~15% to the intermediate-mass galaxy population at z=1, virtually disappear by z=0.2. The merger rate since z=1 is too low to account for the disappearance of these massive bulge-less disks, which most likely grow a bulge via secular evolution.
description: 5 pages, 3 figures, submitted to ApJL
การพัฒนาเครื่องตัดย่อยผักตบชวา สู่การใช้ประโยชน์ทางการเกษตร
Creators: name: อธิรัช ลี้ตระกูล
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: เครื่องตัดย่อย
ผักตบชวา

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 14-27
Markets and capital : a history of the lumber industry of British Columbia (1778-1952)
Creators: name: Lawrence, Joseph Collins
Publisher: name: University of British Columbia
Year: 2012

description: The history of the lumber trade of British Columbia has been one of considerable fluctuation and recurring crises occasioned by historical changes over which the industry has had no control. With no large permanent home market to depend upon for stability, it has had to attain a flexibility which would allow it to accommodate itself to the ever-changing complexity of world markets, In its pioneer phase (1851-1886) the trade could depend on only small local markets in Victoria, New Westminster and, to some extent, San Francisco. With a scarcity of operating capital , no rail transportation whatever, and inadequate water transportation controlled by San Francisco brokers, the infant industry located on Vancouver Island, on Burrard Inlet and at New Westminster struggled for survival. Despite these handicaps, certain fairly reliable markets were gradually established In the awakening Pacific community in Australia, Chile, the Sandwich Islands, and China. The completion of the Canadian Pacific Railroad (1886) marked the real beginning of the lumber trade in British Columbia, it made possible the exploitation of the interior forests, presented the trade with the Prairie market, which was to sustain it until 1913 and it attracted plentiful capital to the industry for the first time. The completion of the Panama Canal in 1914 marked the third phase of the history of the trade, for it opened to the industry the communities of the Atlantic, especially the seaboard of the United States and the important United Kingdom market, This new cargo trade rescued the ailing industry from the collapse of the Prairie demand. The pattern of the lumber trade changed again after 1940. War-time shipping difficulties, followed by a seemingly permanent dollar shortage in the sterling area largely diminished the importance of the United Kingdom market a sustained period of prosperity in the United States, however, facilitated a shift of trade lines from the Old World to the New. The change was accelerated and consolidated by the rise of giant American cellulose corporations which invested heavily In British Columbia forest lands and production plants and integrated them into vast international complexes of industries whose main market is the pulp, lumber, and cellulose-hungry industries of the United States. This thesis attempts to trace these economic changes in the light of changing historical conditions and to discover the pattern which emerges from them.
C’è ‘aria’ di nuovi mondi
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Come si formano ed evolvono i sistemi planetari? A queste domande potrà dare risposta ARIEL, se verrà selezionata, tra una rosa di tre candidati, quale missione spaziale che l’ESA manderà in orbita tra circa dieci anni. Nel team internazionale del progetto, numerosi ricercatori italiani e dell'INAF
Plutone e le sue lune: che spettacolo!
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Rilasciate dalla NASA le prime spettacolari immagini ad alta definizione e i primi dati scientifici del pianeta nano e dei suoi satelliti naturali inviati dalla sonda NASA. Fabrizio Capaccioni (INAF): «Le immagini indicano una superficie giovane, probabilmente modellata da fenomeni di criovulcanismo»
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð²Ð²Ð¾Ð·Ð° Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÑÑÑ Ð¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ²ÑÐ¾Ð¿Ð°Ðº Ð¢ÑÐµÐ¹Ð´Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¾Ð»ÐµÐ²Ð°, Ð¯Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð²Ð²Ð¾Ð·Ð° Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÑÑÑ
Ð°Ð½Ð°Ð»Ð¸Ð· Ð²ÑÐ±Ð¾ÑÐ° Ð¼Ð°ÑÑÑÑÑÐ¾Ð²
ÑÐ°ÑÑÐµÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð²Ð²Ð¾Ð·Ð° ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÑÑÐ¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ²ÑÐ¾Ð¿Ð°Ðº Ð¢ÑÐµÐ¹Ð´Â». Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð²Ð²Ð¾Ð·Ð° Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÑÑÑ Ð¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ. ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð´Ð¾ÑÑÐ°Ð²ÐºÐ¸ ÑÑÑÑÑ. ÐÑÐ¾ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð´Ð¾ÑÑÐ°Ð²ÐºÐ¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÑÑÐ¸Ñ Ð¸Ð· ÐÐ¸ÑÐ°Ñ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ ÑÐµÑÐµÐ· Ð¿Ð¾ÑÑ ÐÐ»Ð°Ð´Ð¸Ð²Ð¾ÑÑÐ¾Ðº.
Three-Dimensional Propagation of Magnetohydrodynamic Waves in Solar Coronal Arcades
Creators: name: Rial, S.
name: Arregui, I.
name: Terradas, J.
name: Oliver, R.
name: Ballester, J. L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We numerically investigate the excitation and temporal evolution of oscillations in a two-dimensional coronal arcade by including the three-dimensional propagation of perturbations. The time evolution of impulsively generated perturbations is studied by solving the linear, ideal magnetohydrodynamic (MHD) equations in the zero-beta approximation. As we neglect gas pressure the slow mode is absent and therefore only coupled MHD fast and Alfven modes remain. Two types of numerical experiments are performed. First, the resonant wave energy transfer between a fast normal mode of the system and local Alfven waves is analyzed. It is seen how, because of resonant coupling, the fast wave with global character transfers its energy to Alfvenic oscillations localized around a particular magnetic surface within the arcade, thus producing the damping of the initial fast MHD mode. Second, the time evolution of a localized impulsive excitation, trying to mimic a nearby coronal disturbance, is considered. In this case, the generated fast wavefront leaves its energy on several magnetic surfaces within the arcade. The system is therefore able to trap energy in the form of Alfvenic oscillations, even in the absence of a density enhancement such as that of a coronal loop. These local oscillations are subsequently phase-mixed to smaller spatial scales. The amount of wave energy trapped by the system via wave energy conversion strongly depends on the wavelength of perturbations in the perpendicular direction, but is almost independent from the ratio of the magnetic to density scale heights.
description: 27 pages, 11 figures
การพัฒนาชุดการเคลื่อนไหวด้วยโมชันแคปเจอร์สำหรับการสอนนาฏศิลป์ ในรูปแบบออนไลน์ของนักศึกษาระดับปริญญาตรี
Creators: name: นวัฒกร โพธิสาร
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: ชุดการเคลื่อนไหว
โมชันแคปเจอร์
นาฏศิลป์
การสอนออนไลน์
ฉุยฉาย

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 28-41
Evidence for Ground- and Excited-State Efimov Trimers in a Three-State Fermi Gas
Creators: name: Williams, J. R.
name: Hazlett, E. L.
name: Huckans, J. H.
name: Stites, R. W.
name: Zhang, Y.
name: O'Hara, K. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We observe enhanced three-body recombination in an ultracold three-component $^6$Li Fermi gas with large but unequal scattering lengths attributable to an excited Efimov trimer state near the three-atom scattering threshold. We find excellent agreement between the measured three-body recombination rate and the recombination rate calculated in the zero-range approximation where the only free parameters are the Efimov parameters $κ_*$ and $η_*$. The value of $κ_*$ determined by the location of the Efimov resonance we observe at 895 G also predicts the locations of loss features previously observed near 130 and 500 G \cite{Jochim08,OHara09} suggesting that all three features are associated with universal Efimov trimer states. We also report on the first realization of a quantum degenerate three-state Fermi gas with approximate SU(3) symmetry.
description: 4 pages, 2 figures
การพัฒนาตู้อบพลังงานแสงอาทิตย์เพื่อการแปรรูปอาหารควบคุมด้วยระบบ Internet of Things (IoT)
Creators: name: อภิญญา สายศรีแก้ว
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: ตู้อบพลังงานแสงอาทิตย์
การแปรรูปอาหาร
ระบบ IoT

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 42-52
In goal con il “pallone” interstellare
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Confermata su Nature la presenza di Buckminsterfullerene, il “pallone da calcio” dei fullereni, nel mezzo interstellare. Un tassello cruciale per risolvere l’annoso enigma sui composti chimici all’origine delle cosiddette “bande diffuse interstellari”
Il gemello di Giove e il gemello del Sole
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

La scoperta con il telescopio da 3,6 metri dell'ESO: è stato identificato un pianeta simile a Giove in orbita a una distanza simile a quella di Giove attorno a una stella simile al Sole, HIP 11915
GSC2.3 N152008120 - a new SU UMa-type dwarf nova in Draco
Creators: name: Boyd, David
name: Graham, Keith
name: Kato, Taichi
name: Koff, Robert
name: Miller, Ian
name: Oksanen, Arto
name: Pickard, Roger
name: Poyner, Gary
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report observations during 2008 October of the first recorded superoutburst of a previously unknown SU UMa-type dwarf nova in Draco located at 19h 14m 43.52s +60d 52m 14.1s (J2000). Simbad lists a 21st magnitude star at this position with identifiers GSC2.3 N152008120 and USNO-B1.0 1508-0249096. The outburst reached magnitude 14.9, its amplitude was approximately 6 magnitudes and its duration at least 11 days. About 11 days after the end of the main outburst there was a short-lived rebrightening by more than 2 magnitudes. Superhumps were observed with a mean period of 0.07117(1) d and amplitude 0.12 mag. There was a distinct shortening in the superhump period around cycle 80 with Psh = 0.07137(2) d before and Psh = 0.07091(2) d after. We saw weak evidence of an increasing Psh before cycle 80 with dPsh/dt = 3.4(2.0) * 10-5.
description: Accepted for publication in Journal of the British Astronomical Association, 9 pages, 6 figures
Curiosity: ecco la crosta continentale di Marte
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Lo strumento ChemCam montato sul rover NASA Curiosity, in missione sul Pianeta Rosso, ha individuato tracce di formazioni rocciose primitive appartenenti a una potenziale “crosta continentale” marziana, che presenta punti in comune con formazioni trovate sulla Terra
การพัฒนาประสิทธิภาพอุปกรณ์ต่อพ่วงรถไถแบบนั่งขับให้สามารถใช้ในการเกษตรแบบครบวงจรในชุดเดียวเพื่อเพิ่มความสามารถในการแข่งขันเป็นผู้ประกอบการข้าวหอมมะลิและพืชไร่ จังหวัดสุรินทร์
Creators: name: วัลลภ โคตรพันธ์
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: อุปกรณ์ต่อพ่วง
การเกษตรครบวงจร
ผู้ประกอบการข้าวหอมมะลิและพืชไร่

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 53-65
title: ÐÑÐ»ÑÑÐ¸ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑ Ð½Ð¸ÐºÐ¸
title: Ð´Ð¸Ñ. â¦ ÐºÐ°Ð½Ð´. ÑÐµÑ Ð½. Ð½Ð°ÑÐº: 05.09.05
titleType: Subtitle
Creators: name: ÐÑÐ±Ð¸ÑÐºÐ¸Ð¹, Ð¡ÐµÐ¼ÐµÐ½
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: 2019
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾ÑÐµÑ Ð½Ð¸ÐºÐ°
ÐÐ°Ð±ÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑ Ð½Ð¸ÐºÐ°
Ð¡Ð²Ð°ÑÐ¾ÑÐ½ÑÐµ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ
ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð§Ð¸ÑÐ»ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼ÑÐ»ÑÑÐ¸ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð¿Ð¾Ð»ÐµÐ²ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ², Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ð±ÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð¸ ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ°. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐµÐ´ÐµÐ»Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° ÐÐ­Ð 60287 Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð½Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½ÑÑ ÐºÐ°Ð±ÐµÐ»ÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸Ð¹, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÑ Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ ÐºÐ°Ð±ÐµÐ»ÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸Ð¹ Ð² Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð¸ Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½ÑÐ¼ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð¼ ÐºÐ°Ð±ÐµÐ»ÐµÐ¹, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ² Ð²ÑÑÐ°Ð²Ð½Ð¸Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð² ÐºÐ°Ð±ÐµÐ»ÑÐ½ÑÑ Ð¼ÑÑÑÐ°Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð° Ð¾ÑÑÑÐµÑÑÐ²Ð¸Ð¼Ð¾ÑÑÑ ÑÐºÐ²Ð¾Ð·Ð½Ð¾Ð³Ð¾ ÑÐ°ÑÑÐµÑÐ° ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ° Ð¿ÑÑÐµÐ¼ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ, ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ñ ÑÑÐµÑÐ¾Ð¼ Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð·ÑÑÐµÐ½Ð° ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÑ Ð³ÑÐ¾Ð·Ð¾Ð·Ð°ÑÐ¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾ÑÐ° Ð²Ð¾Ð·Ð´ÑÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ ÑÐ¾ Ð²ÑÑÑÐ¾ÐµÐ½Ð½ÑÐ¼ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð²Ð¾Ð»Ð¾ÐºÐ½Ð¾Ð¼.
Localized closed timelike curves can perfectly distinguish quantum states
Creators: name: Brun, Todd A.
name: Harrington, Jim
name: Wilde, Mark M.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that qubits traveling along closed timelike curves are a resource that a party can exploit to distinguish perfectly any set of quantum states. As a result, an adversary with access to closed timelike curves can break any prepare-and-measure quantum key distribution protocol. Our result also implies that a party with access to closed timelike curves can violate the Holevo bound.
description: 4.1 pages, 2 figures; v2: revised title, abstract, introduction and conclusion, plus added references
การพัฒนาแพลตฟอร์มออนไลน์เพื่อเสริมศักยภาพวิสาหกิจชุมชนบ้านท่าก่อ จังหวัดอุบลราชธานี โดยใช้แนวคิดแบบอไจล์
Creators: name: รัตน์ชฎาพร ศรีสุระ
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: แพลตฟอร์มออนไลน์
การส่งเสริมศักยภาพวิสาหกิจชุมชน
อไจล์
สกรัม

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 66-79
Strisce zebrate nello spazio terrestre
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Svelato dalla missione Cluster dell’ESA un enigma che ha tenuto col fiato sospeso gli scienziati per quasi mezzo secolo. I dati raccolti da due satelliti hanno permesso di rivelare per la prima volta il meccanismo fisico che sta alla base del “rumore” dovuto alla produzione di onde di plasma in prossimità dello spazio terrestre. I risultati su Nature
Bidirectional Associations Between Affect and Sleep Polysomnography
Creators: name: ten Brink, Maia
name: Kreibig, Sylvia
name: Gross, James
name: Zhang, Jinxiao
name: Goldstein-Piekarski, Andrea
name: Yan, Yan
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Clinical Psychology
subject: Health Psychology
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: Change to 8/25/20 pre-registration: "● Confirmatory Hypotheses ○ Based on Component 1 (https://osf.io/anfqm) findings: 2.1.3 ○ Based on robust literature: 2.1.1, 2.1.2, 2.1.4" Hypothesis 2.1.1. moved from line 1 to line 2.
title: Action Research at Educare: Shifting Focus to the Learner for the 21st Century
Creators: name: Vandarakis, Anthony
name: Farmer, Frederick
name: Wood, Elizabeth
Publisher: name: The International Academic Forum
Year: 2020

description: The European Conference on Education 2020: Official Conference Proceeding, London, United Kingdom, Friday, July 17 - Sunday, July 19, 2020.
description: A new small-school, Educare or Edu2 (pronounced edu-car-ai; from the Latin word meaning "to draw out") opened its doors in Montreal, Canada, in September 2019. Edu2 has launched an innovative educational environment to address the challenges of preparing students to live meaningful and fulfilling lives in the 21st century. In order to achieve that, Edu2 has engaged in the challenging work of rethinking how schools should organize and what constitutes worthwhile knowledge. Edu2 sees the need for school to foster a supportive community, promote a healthy and happy learning environment, advance digital and traditional literacies, and view learner-generated knowledge as essential. The Action Research at Educare: Shifting Focus to the Learner for the 21st Century research team is led by professor Elizabeth Wood. We are investigating, in partnership with the founder-educators of Edu2, the extent to which the school’s vision has materialized. An ongoing focus of the partnership research is community building, educational technology, and student-centered pedagogy: Edu2 is committed to these core tenets while meeting the global academic standards of the Quebec Education Program (QEP). Our research team is committed to chronicling Edu2’s first year of operation through the (voices) experiences of all community members - teachers, students, parents, and researchers. This presentation will explore the experiences of both students and teachers as they engage with the various opportunities, challenges and feelings of belonging to this unique community during the initial year.
Un ponte di materia oscura a due passi da noi
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Uno studio recente ha analizzato il moto delle galassie nei nostri dintorni scoprendo la presenza di un ponte di materia oscura, legato ai due estremi da bolle prive di galassie. Questo ponte e questi vuoti potrebbero aiutarci a chiarire il dilemma delle orbite delle galassie nane, che non rispettano le previsioni del modello standard della cosmologia
Total Current Fluctuations in ASEP
Creators: name: Tracy, Craig A.
name: Widom, Harold
Publisher: name: arXiv
Year: 2009
Subjects: subject: Probability (math.PR)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 60K35 (Primary); 60J25, 82C23 (Secondary)

description: A limit theorem for the total current in the asymmetric simple exclusion process (ASEP) with step initial condition is proved. This extends the result of Johansson on TASEP to ASEP.
การพัฒนาระบบปั๊มน้ำด้วยเซลล์แสงอาทิตย์อัตโนมัติ
Creators: name: สุชาติ ดุมนิล
Publisher: name: คณะเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์
Year: 2022
Subjects: ปั๊มน้ำ
เซลล์แสงอาทิตย์
อัตโนมัติ

description: วารสารวิชาการเทคโนโลยีอุตสาหกรรม มหาวิทยาลัยราชภัฏสุรินทร์, 7, 2, 80-92
Caesar's strategy in the Civil War
Creators: name: Cadman, Frederick William
Publisher: name: University of British Columbia
Year: 2012

description: The purpose of this study is to determine Caesar's strategy in the Civil War of Rome, 49 B, C. to 45 B. C. The Civil War with all its political intrigues has received less attention than the Gallic War but it is in many mays more interesting. Roman is pitted against Roman with an empire as the prize for the victor. Caesar is struggling for his life against forces in Italy and other parts of Europe who do not wish to see Rome ruled by a Dictator. The Civil War rings the death knell of the Republic and heralds the birth of the Empire. The basic works for this study are the three books of the Civil War (De Bello Civili) written by Caesar himself, the Alexandrine War (De Bello Alexandrino), the African War (De Bello Africo) and the Spanish War (De Bello Hispanienal), all of doubtful origin but nevertheless important and of great value to the student of military strategy. I have referred often to the Letters of Cicero, which reveal much information about the military scene at the time of Caesar's march through Italy. Cicero's work is the only contemporary account of Caesar's activities available to the scholar, but I have supplemented this by a study of later historians of Rome. Such writers as Cassius Dio and Appian provide the military historian with data on many of Caesar's movements and clarify his strategy. I have augmented the ancient accounts of Caesar's campaigns in the Civil War by modern studies, as is evident from the Bibliography. The analysis of all the campaigns of the Civil War produces a definite strategic pattern. The elements of surprise, manoeuvre, anticipation, and a general understanding of an enemy's mind, which are displayed by all skilful military leaders, were also part of Caesar's strategic equipment. Most often through skill but sometimes by luck he applied the above techniques where they were needed and, in all the major conflicts, these elements of strategy provided him with victory. Though tactics and strategy are closely linked on the battle field, no attempt has been made in this study to give much detail to tactics except where such information is necessary in explaining the strategic movement concerned. The field of tactics is beyond the scope of my study. Throughout the history of man, certain principles of war have been followed by great military leaders. Caesar was no exception. When Caesar is compared with generals today and his conditions of warfare with those that exist now he displays certain common principles: the selection and maintenance of the aim, the maintenance of morale, concentration of force, flexibility and offensive action. Caesar, in combining the principles of war with sound strategic methods, created for himself a name respected and feared in the annals of history.
Discovery of the Coldest Imaged Companion of a Sun-Like Star
Creators: name: Thalmann, Christian
name: Carson, Joseph
name: Janson, Markus
name: Goto, Miwa
name: McElwain, Michael
name: Egner, Sebastian
name: Feldt, Markus
name: Hashimoto, Jun
name: Hayano, Yutaka
name: Henning, Thomas
name: Hodapp, Klaus W.
name: Kandori, Ryo
name: Klahr, Hubert
name: Kudo, Tomoyuki
name: Kusakabe, Nobuhiko
name: Mordasini, Christoph
name: Morino, Jun-Ichi
name: Suto, Hiroshi
name: Suzuki, Ryuji
name: Tamura, Motohide
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present the discovery of a brown dwarf or possible planet at a projected separation of 1.9" = 29 AU around the star GJ 758, placing it between the separations at which substellar companions are expected to form by core accretion (~5 AU) or direct gravitational collapse (typically >100 AU). The object was detected by direct imaging of its thermal glow with Subaru/HiCIAO. At 10-40 times the mass of Jupiter and a temperature of 550-640 K, GJ 758 B constitutes one of the few known T-type companions, and the coldest ever to be imaged in thermal light around a Sun-like star. Its orbit is likely eccentric and of a size comparable to Pluto's orbit, possibly as a result of gravitational scattering or outward migration. A candidate second companion is detected at 1.2" at one epoch.
description: 5 pages, 3 figures, 2 tables. Accepted for publication in ApJ Letters
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐ´Ð¾Ð²Ð¾Ð¹ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑÑ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¼ ÑÑÐ½ÐºÐµ ÑÑÑÐ´Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð¹Ð½ÐµÐºÐ¾ , 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: 2016
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
ÑÑÑÐ´Ð¾Ð²Ð°Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑ
Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¹ ÑÑÐ½Ð¾Ðº ÑÑÑÐ´Ð°
ÑÐµÐ»Ð¾ÐºÐ°ÑÐ¸Ñ
ÐºÐ°Ð´ÑÐ¾Ð²ÑÐ¹ ÑÐµÐ·ÐµÑÐ²
personnel management
labor mobility
internal labor market
relocation
personnel reserve

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÑÑÐ´Ð¾Ð²Ð°Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¼ ÑÑÐ½ÐºÐµ ÑÑÑÐ´Ð°. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Accor Group, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐµÐµ ÑÑÑÐ´Ð¾Ð²ÑÐ¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ðµ Ð¸ Ð²Ð½ÐµÑÐ½Ð¸Ðµ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² Ð¾ÑÐµÐ»Ðµ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐ´Ð¾Ð²Ð¾Ð¹ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑÑ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÑÐ½ÐºÐ° ÑÑÑÐ´Ð°.
description: Labor mobility of personnel in the domestic labour-market is considered in this work. The economic activity of the Accor Group is analysed, also the analysis of supportability of the company with labour resourses is carried out. Internal and external transfers of personnel in hotel are considered. The labor mobility management system of personnel within the domestic labour-market is formed on the basis of these data.
title: ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð² ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÐµ Ð¸ ÑÐ¿Ð¾ÑÑÐµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ½Ð¸Ñ, Ð¡ÑÐ°Ð½Ð¸ÑÐ»Ð°Ð²
name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð°, ÐÐ°Ð»ÐµÑÐ¸Ñ
name: ÐÐ¾ÑÐ¾Ð²ÐµÐ½ÐºÐ¾, ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ°
ÑÐ¿Ð¾ÑÑ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ð¹ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐµÐ¼ Ð¸ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð² ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÐµ Ð¸ ÑÐ¿Ð¾ÑÑÐµÂ», ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð° ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð²Ð¾Ð¼, Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¹, Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´ÑÑÐ³Ð¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÐ¼Ð¸ ÑÑÐ¿ÐµÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ Ð¸Ð½ÑÐµÑÐµÑ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ°Â», Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ° Ð¸ ÑÐ¿Ð¾ÑÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¸ ÑÑÐµÐ½ÐµÑÐ¾Ð², ÑÑÐ°ÑÑÐ²ÑÑÑÐ¸Ñ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ Ð¸ ÑÐ¿Ð¾ÑÑÐ°.
Optical and near infra-red colours as a discriminant of the age and metallicity of stellar populations
Creators: name: Carter, David
name: Smith, Daniel J. B.
name: Percival, Susan M.
name: Baldry, Ivan K.
name: Collins, Christopher A.
name: James, Philip A.
name: Salaris, Maurizio
name: Simpson, Chris
name: Stott, John P.
name: Mobasher, Bahram
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a comprehensive analysis of the ability of current stellar population models to reproduce the optical (ugriz) and near infra-red (JHK) colours of a small sample of well-studied nearby elliptical and S0 galaxies. We find broad agreement between the ages and metallicities derived using different population models, although different models show different systematic deviations from the measured broad-band fluxes. Although it is possible to constrain Simple Stellar Population models to a well defined area in age-metallicity space, there is a clear degeneracy between these parameters even with such a full range of precise colours. The precision to which age and metallicity can be determined independently, using only broad band photometry with realistic errors, is Delta{[Fe/H]} ~ 0.18 and Delta{log(Age)} ~ 0.25. To constrain the populations and therefore the star formation history further it will be necessary to combine broad-band optical-IR photometry with either spectral line indices, or else photometry at wavelengths outside of this range.
description: 15 pages, 5 figures, accepted for publication in Monthly Notices of the Royal Astronomomical Society
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° DC/DC Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ð½Ð° Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÂ­ÑÐ¾Ð»Ð»ÐµÑÐµ STM32
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐºÐ°Ñ, Ð¡ÐµÑÐ³ÐµÐ¹
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¿Ð¾Ð²ÑÑÐ°ÑÑÐ¸Ð¹ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ
Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÂ­ÑÐ¾Ð»Ð»ÐµÑ
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STM32

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾Ð²ÑÑÐ°ÑÑÐµÐ³Ð¾ DC/DC Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ°ÑÑÐµÑÐ°, ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¿ÐµÑÐ°ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ° ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°.
Tutti pazzi per Plutone
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

I primi a  raccogliere i segnali provenienti dalla sonda New Horizons non saranno i tecnici della NASA, bensì gli esperti che lavorano al Canberra Deep Space Communication Complex (CDSCC) del CSIRO, che poi manderanno le immagini direttamente al Jet Propulsion Laboratory (JPL). E sui social è partita l'iniziativa Pluto Time
title: ÐÐ¾ÑÑÐ¾Ð³ÐµÐ½ÐµÐ· ÐºÐ¾Ð¶Ð¸ Ð² Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´Ð¸ÑÑÐµÑÐµÐ½ÑÐ¸ÑÐ¾Ð²ÐºÐ¸ ÑÐ¼Ð±ÑÐ¸Ð¾Ð¸Ð´Ð½ÑÑ ÑÐµÐ»ÐµÑ Ð¸Ð· ÐÐÐ¡Ð ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð² ÐºÐ¾Ð¶Ð½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¾Ð¸Ð´Ñ
title: Skin morphogenesis in the model of embryoid HIPSCS-derived bodies into skin organoids
Creators: name: Ð ÑÐ±Ð¸Ð½Ð¸Ð½, Ð.
name: ÐÐ°Ð»Ð°Ð±ÑÑÐµÐ²Ð°, Ð.
name: ÐÐ¾ÑÐ¾ÑÐµÐ»ÑÐº, Ð.
name: "ÐÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð¸ ÐºÑÐ»ÑÑÑÑ ÐºÐ»ÐµÑÐ¾Ðº ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ : ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð²ÑÐ·Ð¾Ð²Ñ Ð¸ ÑÐµÑÐµÐ²ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ ÑÐºÐ¾Ð»Ð°-ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÐÐ»ÐµÑÐºÐ° (Ð±Ð¸Ð¾Ð».)
ÑÐµÐ³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð²Ð½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°
ÐºÐ»ÐµÑÐ¾ÑÐ½Ð°Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð½Ð°ÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¾ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¶Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¾Ð¸Ð´Ð¾Ð², ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð² ÑÐ²Ð¾ÐµÐ¹ ÑÑÑÑÐºÑÑÑÐµ Ð²Ð¾Ð»Ð¾ÑÑÐ½ÑÐµ ÑÐ¾Ð»Ð»Ð¸ÐºÑÐ»Ñ (ÐÐ¤), in vitro Ð±ÐµÐ· Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ²Ð¾ÑÐ¾ÑÐºÐ¸, Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ Ð°Ð½ÑÐ¸Ð±Ð¸Ð¾ÑÐ¸ÐºÐ¾Ð² â Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð´Ð¸ÑÑÐµÑÐµÐ½ÑÐ¸ÑÐ¾Ð²ÐºÐ¸ ÑÐ¼Ð±ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ ÑÐµÐ»ÐµÑ Ð¸Ð· ÐÐÐ¡Ð â Ð¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð±ÐµÐ»ÐºÐ° YAP Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑÐ°Ñ ÐºÐ¾Ð¶Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¾Ð¸Ð´Ð¾Ð² Ð² ÑÐ¾Ð´Ðµ Ð¸Ñ Ð¼Ð¾ÑÑÐ¾Ð³ÐµÐ½ÐµÐ·Ð°.
Benvenuti nel mondo dei pentaquark
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Il team di scienziati della collaborazione LHCb, uno dei quattro grandi esperimenti del superacceleratore del CERN a Ginevra, ha riportato la scoperta di una classe di particelle esotiche note come pentaquark.  Il risultato dell’esperimento LHCb è forte di un’analisi dei dati estremamente accurata a rigorosa, basata su un’elevatissima statistica, mai raggiunta prima, e su un’altissima precisione del rivelatore
MOESM1 of Poor outcomes of immunoglobulin D multiple myeloma patients in the era of novel agents: a single-center experience
Creators: name: Zhao, Qian
name: Li, Feng
name: Song, Ping
name: Zhou, Xiaogang
name: An, Zhiming
name: Mei, Jiangang
name: Shao, Jingjing
name: Li, Hanqing
name: Wang, Xuli
name: Guo, Xing
name: Zhai, Yongping
Publisher: name: figshare
Year: 2019
Subjects: Space Science
Medicine
Biological Sciences not elsewhere classified
Cancer
Science Policy
Hematology

description: Additional file 1: Table S1. Univariate analysis for PFS and OS of 216 patients with multiple myeloma.
title: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¥Ð°ÑÐ¸Ð½Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ°
Ð²ÑÐ±Ð¾ÑÐºÐ°
Ð³Ð¸Ð¿Ð¾ÑÐµÐ·Ð°
Ð¼ÐµÑÐ¾Ð´ ÑÑÐ¼Ð¼
Ð¼ÐµÑÐ¾Ð´ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾ ÑÑÐ´Ñ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² ÐºÑÑÑÐ° Â«ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¸Ì, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ñ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½ÑÐ¼Ð¸ ÑÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸ Ð¾ÑÐ²ÐµÑÐ°Ð¼Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ (Ð¾ÑÐ½Ð¾Ð¸Ì, Ð²ÐµÑÐµÑÐ½ÐµÐ¸Ì Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¸Ì) Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐµÑ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð².
Scintillation Pulse Shape Discrimination in a Two-Phase Xenon Time Projection Chamber
Creators: name: Kwong, J.
name: Brusov, P.
name: Shutt, T.
name: Dahl, C. E.
name: Bolozdynya, A. I.
name: Bradley, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The energy and electric field dependence of pulse shape discrimination in liquid xenon have been measured in a 10 gm two-phase xenon time projection chamber. We have demonstrated the use of the pulse shape and charge-to-light ratio simultaneously to obtain a leakage below that achievable by either discriminant alone. A Monte Carlo is used to show that the dominant fluctuation in the pulse shape quantity is statistical in nature, and project the performance of these techniques in larger detectors. Although the performance is generally weak at low energies relevant to elastic WIMP recoil searches, the pulse shape can be used in probing for higher energy inelastic WIMP recoils.
description: 7 pages, 11 figures
2030, torna l’era glaciale? Improbabile
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

I risultati di un modello di fisica solare presentati la scorsa settimana al National Astronomy Meeting di Llandudno hanno evocato scenari apocalittici. Ma come stanno davvero le cose? Lo abbiamo chiesto a Mauro Messerotti dell’INAF di Trieste
Systematic Review of Interventions to Improve Post-Surgery Outcomes in Elderly with Hip Fractures
Creators: name: Ying, Lim
name: Leng, A/Prof
name: Heng, Kwan
name: Kie, Phang
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Public Health
subject: Medicine and Health Sciences
subject: Medical Specialties
subject: Rehabilitation and Therapy

description: The aim of this systematic review is to summarize the literature on interventions provided post-surgery to improve outcomes for elderly patients with hip fractures. This would consolidate the latest evidence-based information, enabling healthcare providers to compare the effects of various interventions, thus providing clarity on effective ways to intervene.
Venature d’idrogeno sulle ali della Farfalla
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Grazie al telescopio Gemini sud, in Cile, ripresi dettagli mai visti di nodi e filamenti di idrogeno molecolare nelle “ali” della nebulosa planetaria bipolare NGC 2346, conosciuta da tempo come Nebulosa Farfalla. Si tratta di una stella in una fase breve ma altamente spettacolare del suo ciclo di vita
Strong Anomalous Optical Dispersion of Graphene: Complex Refractive Index Measured by Picometrology
Creators: name: Wang, Xuefeng
name: Chen, Yong P.
name: Nolte, David D.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We apply spinning-disc picometrology to measure the complex refractive index of graphene on thermal oxide on silicon. The refractive index varies from n = 2.4-1.0i at 532 nm to n = 3.0-1.4i at 633 nm at room temperature. The dispersion is five times stronger than bulk graphite (2.67-1.34i to 2.73-1.42i from 532 nm to 633 nm).
Le scoperte che hanno cambiato la scienza
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

L'atomo, il Big Bang, il DNA, la selezione naturale e molto altro. Attraverso undici nuove prospettive, Michael Brooks ci porta - capitolo dopo capitolo - verso le frontiere estreme di ciò che noi chiamiamo mondo, di ciò che noi chiamiamo universo
The Case of AB Aurigae's Disk in Polarized Light: Is There Truly a Gap?
Creators: name: Perrin, Marshall D.
name: Schneider, Glenn
name: Duchene, Gaspard
name: Pinte, Christophe
name: Grady, Carol A.
name: Wisniewski, John P.
name: Hines, Dean C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Using the NICMOS coronagraph, we have obtained high-contrast 2.0 micron imaging polarimetry and 1.1 micron imaging of the circumstellar disk around AB Aurigae on angular scales of 0.3-3 arcsec (40-550 AU). Unlike previous observations, these data resolve the disk in both total and polarized intensity, allowing accurate measurement of the spatial variation of polarization fraction across the disk. Using these observations we investigate the apparent "gap" in the disk reported by Oppenheimer et al. 2008. In polarized intensity, the NICMOS data closely reproduces the morphology seen by Oppenheimer et al., yet in total intensity we find no evidence for a gap in either our 1.1 or 2.0 micron images. We find instead that region has lower polarization fraction, without a significant decrease in total scattered light, consistent with expectations for back-scattered light on the far side of an inclined disk. Radiative transfer models demonstrate this explanation fits the observations. Geometrical scattering effects are entirely sufficient to explain the observed morphology without any need to invoke a gap or protoplanet at that location.
description: Accepted to ApJ Letters
The relativistic massless harmonic oscillator
Creators: name: Kowalski, K.
name: Rembielinski, J.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A detailed study of the relativistic classical and quantum mechanics of the massless harmonic oscillator is presented.
description: 15 pages, 4 figures
Giganti cosmici contro galassie nane
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Uno studio recente riporta i risultati di una campagna osservativa condotta su oltre 20.000 galassie e mostra che del tasso di formazione stellare a seguito di una collisione dipende dalle dimensioni della galassia rispetto a quella con cui sta collidendo. L’articolo sul Monthly Notices of the Royal Astronomical Society
Spiral grain in second growth Douglas fir and western hemlock
Creators: name: Elliott, Geoffrey Kenyon
Publisher: name: University of British Columbia
Year: 2012

description: Spiral grain in timber may cause severe twisting of lumber and plywood. In the primary forest products industries the presence of spiral grain in the tree results in cross-grained products. Cross grain affects the strength properties of lumber to a marked degree. Thus a grain deviation of 1 In 25 (2°18') results in decreased tensile strength whereas a slope of 1 in 10 (5°43') will reduce compression strength. Spiral grain is a condition well known to the wood technologist and the silviculturalist. Until recently it was considered the exception rather than the rule. From recently published papers, however, and from unpublished data available to the author, strong evidence has been produced to show that spiral grain is the normal growth pattern in trees. This thesis is designed to investigate the spiral pattern of second-growth Douglas fir and western hemlock. Accordingly three sites were chosen: a good, a medium and a low site in a typical British Columbia coastal forest of second growth. Two crown classes for each species were sampled from each site and three trees in each crown class for each species were felled and their spiral patterns investigated. A general trend of spirality was established, the twist being initially left (at first), decreasing to the left and becoming right with increasing age. This pattern holds good for both species. The effect of site on spiral development was established as highly significant with both species. On high quality sites the chief factor influencing spiral development was found to be distance from the pith. On sites of lower quality, age from the pith was found to have the most significant influence on spiral development.