cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð¸ÐºÑÐ¾Ð­ÐÐ: Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐµ ÑÐµÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐ°ÐºÐ¾Ð²ÑÐºÐ¸Ð¹, ÐÐ¾ÑÐ¸Ñ
name: ÐÑÐ¾Ð±Ð¸Ð½ÑÐµÐ², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: ÐÐ¾ÑÐ»ÑÑÐ¾Ð², ÐÑÐµÐ²Ð¾Ð»Ð¾Ð´
name: ÐÐ¸ÑÑÐºÐ¾, ÐÐ½Ð´ÑÐµÐ¹
name: Ð ÑÐ¶ÐµÐ²Ð½Ð¸Ð½, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐÐ
Year: 1987
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð½Ð° Ð±Ð¾Ð»ÑÑÐ¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½ÑÑ ÑÑ ÐµÐ¼Ð°Ñ

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¸ Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ¹ Ð½Ð° Ð±Ð°Ð·Ðµ Ð¼Ð¸ÐºÑÐ¾Ð­ÐÐ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÑÐµÐ´ÑÑÐ²Ð° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð² Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ ÐÐ¡ ÐÐÐ Ð¸ Ð¤ÐÐÐÐ¡. ÐÐ¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ², Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÐ¸ÐµÑÑ Ð½Ð° ÑÐ±Ð¾ÑÐ¾ÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¼ Ð¿Ð¾Ð´ÑÐ¾Ð´Ðµ Ðº Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹. ÐÐ±ÑÑÐ¶Ð´Ð°ÐµÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð½Ð° Ð±Ð°Ð·Ðµ Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ¹. ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½Ð¾-Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÑÐµÑÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð² ÑÐµÑÐ½Ð¸ÐºÐµ Ð¼Ð°ÐºÑÐ¾ÑÑÐµÐ´ÑÑÐ², Ð¿Ð¾Ð´Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼, Â«ÑÐ¸ÑÐ¾Ð³Ð¾ ÐºÐ¾Ð´Ð°Â» Ð¸ Ð½Ð° ÑÐ·ÑÐºÐ°Ñ Ð°ÑÑÐµÐ¼Ð±Ð»ÐµÑ, ÐÐ°ÑÐºÐ°Ð»Ñ, Ð¤Ð¾ÑÑÑÐ°Ð½, Ð¤Ð¾ÑÑ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Â«ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÂ», Â«Ð¡ÐÐÐ Â», Â«Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Â», Ð° ÑÐ°ÐºÐ¶Ðµ Â«ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹Â».
The HARPS search for southern extra-solar planets. XX. Planets around the active star BD-08:2823
Creators: name: Hebrard, G.
name: Udry, S.
name: Curto, G. Lo
name: Robichon, N.
name: Naef, D.
name: Ehrenreich, D.
name: Benz, W.
name: Bouchy, F.
name: Etangs, A. Lecavelier des
name: Lovis, C.
name: Mayor, M.
name: Moutou, C.
name: Pepe, F.
name: Queloz, D.
name: Santos, N. C.
name: Segransan, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report the detection of a planetary system around BD-08:2823, that includes at least one Uranus-mass planet and one Saturn-mass planet. This discovery serendipitously originates from a search for planetary transits in the Hipparcos photometry database. This program preferentially selected active stars and did not allow the detection of new transiting planets. It allowed however the identification of the K3V star BD-08:2823 as a target harboring a multiplanet system, that we secured and characterized thanks to an intensive monitoring with the HARPS spectrograph at the 3.6-m ESO telescope in La Silla. The stellar activity level of BD-08:2823 complicates the analysis but does not prohibit the detection of two planets around this star. BD-08:2823b has a minimum mass of 14.4+/-2.1 M_Earth and an orbital period of 5.60 days, whereas BD-08:2823c has a minimum mass of 0.33+/-0.03 M_Jup and an orbital period of 237.6 days. This new system strengthens the fact that low-mass planets are preferentially found in multiplanetary systems, but not around high-metallicity stars as this is the case for massive planets. It also supports the belief that active stars should not be neglected in exoplanet searches, even when searching for low-mass planets.
description: 10 pages, 8 figures, 3 tables, accepted for publication in A&A
The Isospectral Fruits of Representation Theory: Quantum Graphs and Drums
Creators: name: Band, Ram
name: Parzanchevski, Ori
name: Ben-Shach, Gilad
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 35P05; 58J32; 58J53

description: We present a method which enables one to construct isospectral objects, such as quantum graphs and drums. One aspect of the method is based on representation theory arguments which are shown and proved. The complementary part concerns techniques of assembly which are both stated generally and demonstrated. For that purpose, quantum graphs are grist to the mill. We develop the intuition that stands behind the construction as well as the practical skills of producing isospectral objects. We discuss the theoretical implications which include Sunada's theorem of isospectrality arising as a particular case of this method. A gallery of new isospectral examples is presented and some known examples are shown to result from our theory.
Microcanonical phase diagrams of short-range ferromagnets
Creators: name: Kastner, Michael
name: Pleimling, Michel
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A phase diagram is a graph in parameter space showing the phase boundaries of a many-particle system. Commonly, the control parameters are chosen to be those of the (generalized) canonical ensemble, such as temperature and magnetic field. However, depending on the physical situation of interest, the (generalized) microcanonical ensemble may be more appropriate, with the corresponding control parameters being energy and magnetization. We show that the phase diagram on this parameter space looks remarkably different from the canonical one. The general features of such a microcanonical phase diagram are investigated by studying two models of ferromagnets with short-range interactions. The physical consequences of the findings are discussed, including possible applications to nuclear fragmentation, adatoms on surfaces, and cold atoms in optical lattices.
description: 5 pages, 3 figures
Thermal conductivity of graphene in Corbino membrane geometry
Creators: name: Faugeras, C.
name: Faugeras, B.
name: Orlita, M.
name: Potemski, M.
name: Nair, R. R.
name: Geim, A. K.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Local laser excitation and temperature readout from the intensity ratio of Stokes to anti-Stokes Raman scattering signals are employed to study the thermal properties of a large graphene membrane. The concluded value of the heat conductivity coefficient κ~ 600 W/m \cdot K is smaller than previously reported but still validates the conclusion that graphene is a very good thermal conductor.
description: 4 pages, 3 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ðº Ð²Ð½ÐµÑÐ½Ð¸Ð¼ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°Ð¼ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸ÑÐ° Ð¿Ð¾Ð´Ð±Ð¾ÑÐ° Ð¿ÑÑÐµÐ²Ð¾Ðº
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¶Ð¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
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Ð²ÐµÐ±-ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°
ÑÑÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð³ÑÐµÐ³Ð°ÑÐ¾Ñ
Ð¿Ð¾Ð´Ð±Ð¾Ñ ÑÑÑÐ¾Ð²
Ð³Ð¾ÑÐ½Ð¾Ð»ÑÐ¶Ð½ÑÐ¹ ÑÑÑÐ¸Ð·Ð¼
Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ðº Ð²Ð½ÐµÑÐ½Ð¸Ð¼ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°Ð¼ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸ÑÐ° Ð¿Ð¾Ð´Ð±Ð¾ÑÐ° ÑÑÑÐ¾Ð². ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸ÑÑ Ð¿Ð¾Ð´Ð±Ð¾ÑÐ° ÑÑÑÐ¾Ð². ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð¿Ð¾Ð´Ð±Ð¾Ñ Ð³Ð¾ÑÐ½Ð¾Ð»ÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð². Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð¸ÑÐºÐ° Ð³Ð¾ÑÐ½Ð¾Ð»ÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð² Ð² Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸ÑÐµ Ð¿Ð¾Ð´Ð±Ð¾ÑÐ° ÑÑÑÐ¾Ð². ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð°Ð½Ð°Ð»Ð¸Ð·, ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ, Ð°Ð±ÑÑÑÐ°Ð³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, ÑÐ¸Ð½ÑÐµÐ·. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð¿Ð¾Ð¸ÑÐºÐ° Ð¸ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð³Ð¾ÑÐ½Ð¾Ð»ÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð² Ð¿Ð¾ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð², ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ñ Ð³Ð¾ÑÐ½Ð¾Ð»ÑÐ¶Ð½ÑÐµ ÐºÑÑÐ¾ÑÑÑ Ð¸ Ð¾ÑÐµÐ»Ð¸.
Measurement of the Spin Relaxation Time of Single Electrons in a Silicon MOS-Based Quantum Dot
Creators: name: Xiao, M.
name: House, M. G.
name: Jiang, H. W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report on measurements of the spin relaxation time T1 of individual electron spins in the few electron regime of a Si/SiO2-based quantum dot (QD). Energy-spectroscopy of the QD has been performed using a charge sensing technique. The spin relaxation times are subsequently measured in the time-domain by a pump-and-probe method. For the QD that contains an unpaired spin, likely only a single electron, we find that T1 depends strongly on the applied magnetic field. Possible mechanisms leading to the observed spin relaxation are discussed.
description: 11 pages, 4 figures
Explosive events associated with a surge
Creators: name: Madjarska, M. S.
name: Doyle, J. G.
name: de Pontieu, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The solar atmosphere contains a wide variety of small-scale transient features. Here, we explore the inter-relation between some of them such as surges, explosive events and blinkers via simultaneous spectral and imaging data taken with the TRACE imager, the SUMER, and CDS spectrometers on board SoHO, and SVST La Palma. The alignment of all data both in time and solar XY shows that SUMER line profiles, which are attributed to explosive events, are due to a surge phenomenon. The surge is triggered, most probably, by one or more Elerman bombs which are best visible in Halpha +-350 A but were also registered by TRACE Fe IX/X 171 A and correspond to a strong radiance increase in the CDS Mg IX 368.07 A line. With the present study we demonstrate that the division of small-scale transient events into a number of different subgroups, for instance explosive events, blinkers, spicules, surges or just brightenings, is ambiguous, implying that the definition of a feature based only on either spectroscopic or imaging characteristics as well as insufficient spectral and spatial resolution can be incomplete.
description: 17 pages, 7 figures, 1 table
title: Pushing the Car of Progress Forward: The Salt Lake Tribune's Quest to Change Utah for Statehood, 1871-1896
Creators: name: Mills, Robert Patrick
Publisher: name: Utah State University
Year: 2007

description: The debate over Utah statehood involved several controversial issues that the United States government and the American public wanted resolved before admission would be granted. One strong advocate for such changes in Utah was the widely published newspaper, the Salt Lake Tribune, which continually published anti-statehood and anti-Mormon ideas in the final decades before Utah was finally admitted in 1896. This thesis studies and analyzes the Tribune’s editorials and news stories to better understand which issues opponents of statehood worried the most over and what they wanted to accomplish with their protest. It finds that Mormon political domination was the paper’s central concern throughout the last decade of the debate, even after developments showed change on the horizon. This thesis also examines the Tribune’s ability to reach Utah readers and a national audience through its connections with the Associated Press. By citing numerous newspapers from throughout the United States and members of Congress who were close to the statehood debate, this thesis shows that the Tribune got its message out and that it played a strong part in the statehood struggle.
title: Ð§Ð¸ÑÐ°ÐµÐ¼ ÑÑÐ¸Ñ Ð¸ Ð¿Ð¾ÑÑÐ¾Ð² Ð Ð¾ÑÑÐ¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð¸Ð½Ð¾ÑÑÑÐ°Ð½ÑÐµÐ²
titleType: Subtitle
Creators: name: ÐÑÐ½Ð¸Ð½Ð°, Ð.
Publisher: name: Ð¡ÐÐ±ÐÐÐ£
Year: 2005
Subjects: ÑÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½ÑÐµÐ²

description: ÐÐ°Ð½Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÐ°Ð±Ð¾ÑÑ Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼Ð¸ ÑÑÐ°ÑÐ¸Ð¼Ð¸ÑÑ Ð½Ð° ÑÑÐ°Ð¿Ðµ Ð¿ÑÐµÐ´Ð²ÑÐ·Ð¾Ð²ÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð´Ð²ÑÑ ÑÐ°ÑÑÐµÐ¹. Ð I ÑÐ°ÑÑÑ Ð²Ð¾ÑÐ»Ð¸ ÑÑÐ¸ÑÐ¸, Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐµ Ð´Ð»Ñ Ð·Ð°ÑÑÐ¸Ð²Ð°Ð½Ð¸Ñ Ð² I ÑÐµÐ¼ÐµÑÑÑÐµ, Ð° Ð²Ð¾ II ÑÐ°ÑÑÑ - ÑÑÐ¸ÑÐ¸ Ð´Ð»Ñ Ð·Ð°ÑÑÐ¸Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾ II ÑÐµÐ¼ÐµÑÑÑÐµ. ÐÐ½ÑÑÑÐ¸ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÑÐ¸ÑÐ¸ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ñ Ð² ÑÑÐ¾Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð¿Ð¾ÑÑÐ´ÐºÐµ. Ð¢ÐµÐºÑÑÐ°Ð¼ ÑÑÐ¸ÑÐ¾Ð² Ð¿ÑÐµÐ´ÑÐµÑÑÐ²ÑÐµÑ Ð±Ð¸Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¿ÑÐ°Ð²ÐºÐ° Ð¿Ð¾ÑÑÐ¾Ð². ÐÑÐ½Ð¾Ð²Ð¾Ð¹ Ð´Ð»Ñ Ð¾ÑÐ±Ð¾ÑÐ° ÑÑÐ¸ÑÐ¾Ð² Ð² Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ÑÐ»ÑÐ¶Ð¸Ð»Ð¸ Ð´Ð²Ð° Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÐ¼ Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¼Ñ. Ð¢Ð°Ðº, ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÑÐ¾ÑÐ¾Ð½Ð° ÑÑÐ¸ÑÐ¾Ð² - ÑÑÐ¾ Ð¿ÑÐµÐ¶Ð´Ðµ Ð²ÑÐµÐ³Ð¾ ÑÐ°Ð·Ð¼ÑÑÐ»ÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¿Ð¾ÑÑÐ¾Ð² Ð¾Ð± Ð¾Ð±ÑÐµÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ñ ÑÐµÐ½Ð½Ð¾ÑÑÑÑ: Ð¾ Ð»ÑÐ±Ð²Ð¸, Ð´ÑÑÐ¶Ð±Ðµ, Ð¼Ð¸ÑÐµ Ð¸ Ð¾ Ð¿ÑÐ¸ÑÐ¾Ð´Ðµ. Ð ÑÐ¾ÑÐ¼Ðµ ÑÑÐ¸ÑÐ¾Ð² Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÐ»Ð¾ÑÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÑÐ¾ÑÑ Ð¸ Ð´Ð¾ÑÑÑÐ¿Ð½Ð¾ÑÑÐ¸ Ð½Ð° Ð»ÐµÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼, ÑÐµÐ¼Ð°Ð½ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¸ ÑÐ¸Ð½ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÑÐ¾Ð²Ð½ÑÑ. ÐÐ±ÑÑÐ¼ Ð¿Ð¾ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ»ÑÑ ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¾Ð¹: Ð´Ð»Ñ I ÑÐµÐ¼ÐµÑÑÑÐ° â 8 ÑÑÑÐ¾Ðº, Ð´Ð»Ñ II ÑÐµÐ¼ÐµÑÑÑÐ° - 12 ÑÑÑÐ¾Ðº. Ð¡ÑÐ¸ÑÐ¾ÑÐ²Ð¾ÑÐµÐ½Ð¸Ñ Ð±Ð¾Ð»ÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÑÐ¼Ð° Ð¸ Ð±Ð¾Ð»ÑÑÐµÐ¹ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐ´Ð½Ð¾ÑÑÐ¸, Ð²ÐºÐ»ÑÑÑÐ½Ð½ÑÐµ Ð² Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÑÑ ÑÐ¾Ð±Ð¾Ð¹ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÑÐµÐ±Ð½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ðº ÐÐ»Ð¸Ð¼Ð¿Ð¸Ð°Ð´Ðµ Ð¿Ð¾ ÑÑÑÑÐºÐ¾Ð¼Ñ ÑÐ·ÑÐºÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð° Ð·Ð°Ð½ÑÑÐ¸ÑÑ ÑÐ¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ ÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð²Ð»Ð°Ð´ÐµÐ½Ð¸Ñ ÑÑÑÑÐºÐ¸Ð¼ ÑÐ·ÑÐºÐ¾Ð¼. ÐÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ "ÐÑÐ°ÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½Ð¾Ð¹ ÑÐ½ÑÐ¸ÐºÐ»Ð¾Ð¿ÐµÐ´Ð¸Ð¸". Ð. 1962, Ð±Ð¸Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ»Ð¾Ð²Ð°ÑÑ "Ð ÑÑÑÐºÐ¸Ðµ Ð¿Ð¸ÑÐ°ÑÐµÐ»Ð¸" Ð¿Ð¾Ð´ ÑÐµÐ´Ð°ÐºÑÐ¸ÐµÐ¹ Ð. Ð¡. ÐÐ¸ÑÐ°ÑÐµÐ²Ð°. Ð. 1971 Ð³. Ð¸ ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐ¸ ÑÑÐ¸ÑÐ¾Ð² Ð¿Ð¾ÑÑÐ¾Ð² Ð Ð¾ÑÑÐ¸Ð¸. Ð ÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð¾ ÐºÐ°ÑÐµÐ´ÑÐ¾Ð¹ ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð¸ Ð½Ð°ÑÑÐ½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¾Ð²ÐµÑÐ¾Ð¼ ÐÐÐÐ Ð¡ÐÐ±ÐÐÐ£.
Constraints on the symmetry energy and on neutron skins from the pygmy resonances in 68Ni and 132Sn
Creators: name: Carbone, Andrea
name: Coló, Gianluca
name: Bracco, Angela
name: Cao, Li-Gang
name: Bortignon, Pier Francesco
name: Camera, Franco
name: Wieland, Oliver
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Correlations between the behavior of the nuclear symmetry energy, the neutron skins, and the percentage of energy-weighted sum rule (EWSR) exhausted by the Pygmy Dipole Resonance (PDR) in 68Ni and 132Sn have been investigated by using different Random Phase Approximation (RPA) models for the dipole response, based on a representative set of Skyrme effective forces plus meson-exchange effective Lagrangians. A comparison with the experimental data has allowed us to constrain the value of the derivative of the symmetry energy at saturation. The neutron skin radius is deduced under this constraint.
description: Accepted for publication in PRC Rapid Comminication
Background-Source Separation in astronomical images with Bayesian probability theory (I): the method
Creators: name: Guglielmetti, F.
name: Fischer, R.
name: Dose, V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: A probabilistic technique for the joint estimation of background and sources with the aim of detecting faint and extended celestial objects is described. Bayesian probability theory is applied to gain insight into the coexistence of background and sources through a probabilistic two-component mixture model, which provides consistent uncertainties of background and sources. A multi-resolution analysis is used for revealing faint and extended objects in the frame of the Bayesian mixture model. All the revealed sources are parameterized automatically providing source position, net counts, morphological parameters and their errors.
description: 28 pages, 23 figures, 5 tables, accepted for publication in MNRAS
Supplemental Table 3 Supplemental Materials - American Journal of Physiology Gastrointestinal and Liver Physiology 2021
Creators: name: Shneider, Benjamin
Publisher: name: figshare
Year: 2021
Subjects: subject: 60802 Animal Cell and Molecular Biology
subject: FOS: Biological sciences

description: Supplemental Table 3
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¾ÑÑÐ¾ÐºÂ»
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Ð¾Ð²Ð¾ÑÐµÐ»Ð¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ
Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð½ÐµÐ¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

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Ð¾ÑÑÐ¾ÐºÂ».
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° ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÐÐÐ Â«ÐÐ¾ÑÑÐ¾ÐºÂ».
ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾- ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÐÐÐ Â«ÐÐ¾ÑÑÐ¾ÐºÂ». Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð°Ð½ÐºÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, Ð² ÑÐ¾Ð´Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð±ÑÐ»Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¸ Ð½Ðµ ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÐµÐ½Ñ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
ÐÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¼Ñ Ð¸ Ð½ÐµÐ¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÐÐÐ Â«ÐÐ¾ÑÑÐ¾ÐºÂ» Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°.
Supplemental Table 2A Supplemental Materials - American Journal of Physiology Gastrointestinal and Liver Physiology 2021
Creators: name: Shneider, Benjamin
Publisher: name: figshare
Year: 2021
Subjects: subject: 60802 Animal Cell and Molecular Biology
subject: FOS: Biological sciences

description: Supplemental Table 2A
Stemonitis marjana Y. Yamam., Marjas
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Stemonitidales
Stemonitidaceae
Stemonitis
Stemonitis marjana

description: B● Stemonitis cf. marjana Y. Yamam., Marjas
vālenīte (šokolādes gļotsēne)
- leg. I.Ojere, 23 Jul 2023, Carnikava p., on a log of Pinus sylvestris in a pine forest, det. E.Johannesen, 2023; leg. A.Baroniņš, 15 Aug 2020, Slampe p., on a log of Pinus sylvestris in a forest, det. E.Johannesen, 2023; (NMKK), very rare. Two localities and both specimens with slight deviations from the species description - in one case grows in large tufts, in the other case sporocarps are too large compared to the description. However, considering that the original description was based only on the type collection, the mentioned deviations might not be considered as very significant.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
Bistability, multistability and nonreciprocal light propagation in Thue-Morse multilayered structures
Creators: name: Grigoriev, Victor
name: Biancalana, Fabio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The nonlinear properties of quasiperiodic photonic crystals based on the Thue-Morse sequence are investigated. The intrinsic spatial asymmetry of these one-dimensional structures for odd generation numbers results in bistability thresholds which are sensitive to the propagation direction. Along with resonances of perfect transmission, this feature allows to achieve strongly non-reciprocal propagation and to create an all-optical diode. The salient qualitative features of such optical diode action is readily explained through a simple coupled resonator model. The efficiency of a passive scheme, which does not necessitate of an additional short pump signal, is compared to an active scheme, where such a signal is required.
description: 18 pages, 8 figures
title: ÐÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ñ Ð² Ð¿Ð¾Ð»Ð¸ÐºÐ¾Ð´Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ: Ð»Ð¸Ð½Ð³Ð²Ð¾-ÐºÑÐ»ÑÑÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð´Ð¸Ð´Ð°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ, ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ
title: Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸
titleType: Subtitle
Creators: name: "ÐÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ñ Ð² Ð¿Ð¾Ð»Ð¸ÐºÐ¾Ð´Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ: Ð»Ð¸Ð½Ð³Ð²Ð¾-ÐºÑÐ»ÑÑÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð´Ð¸Ð´Ð°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ, ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2015; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: Ð¿Ð¾Ð»Ð¸ÐºÐ¾Ð´Ð¾Ð²Ð¾ÑÑÑ
ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ñ
ÑÐ·ÑÐºÐ¾Ð·Ð½Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, ÑÐ¾ÑÑÐ¾ÑÐ²ÑÐµÐ¹ÑÑ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ Ð² Ð¼Ð°Ðµ 2015 Ð³., Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð½Ð°ÑÑÐ½ÑÑ ÑÐºÐ¾Ð» Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÑÐºÐ¸Ñ ÑÐµÐ½ÑÑÐ¾Ð² Ð¿Ð¾ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼ Ð¿Ð¾Ð»Ð¸ÐºÐ¾Ð´Ð¾Ð²Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐµÐ¼Ð¸Ð¾ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð³ÐµÑÐµÑÐ¾Ð³ÐµÐ½Ð½Ð¾ÑÑÑ ÑÐµÐºÑÑÐ° Ð¸ Ð´Ð¸ÑÐºÑÑÑÐ°, ÐºÑÐ»ÑÑÑÑÐ½Ð¾-ÑÐ·ÑÐºÐ¾Ð²Ð°Ñ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾-ÑÐµÑÐµÐ²ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ¾Ð´Ð¾Ð²ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð² Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÐ·ÑÐºÐ¾Ð². ÐÐ´ÑÐµÑÐ¾Ð²Ð°Ð½Ð¾ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ°Ð¼, ÐºÑÐ»ÑÑÑÑÐ¾Ð»Ð¾Ð³Ð°Ð¼, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼ Ð¿Ð¾ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐµ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÐ·ÑÐºÐ¾Ð².
Supplemental Table 1.docx Supplemental Materials - American Journal of Physiology Gastrointestinal and Liver Physiology 2021
Creators: name: Shneider, Benjamin
Publisher: name: figshare
Year: 2021
Subjects: subject: 60802 Animal Cell and Molecular Biology
subject: FOS: Biological sciences

description: Supplemental Table 1
The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements II. The Full Sample of Reverberation-Mapped AGNs
Creators: name: Bentz, Misty C.
name: Peterson, Bradley M.
name: Netzer, Hagai
name: Pogge, Richard W.
name: Vestergaard, Marianne
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high-resolution HST images of all 35 AGNs with optical reverberation-mapping results, which we have modeled to create a nucleus-free image of each AGN host galaxy. From the nucleus-free images, we determine the host-galaxy contribution to ground-based spectroscopic luminosity measurements at 5100A. After correcting the luminosities of the AGNs for the contribution from starlight, we re-examine the Hbeta R-L relationship. Our best fit for the relationship gives a powerlaw slope of 0.52 with a range of 0.45 - 0.59 allowed by the uncertainties. This is consistent with our previous findings, and thus still consistent with the naive assumption that all AGNs are simply luminosity-scaled versions of each other. We discuss various consistency checks relating to the galaxy modeling and starlight contributions, as well as possible systematic errors in the current set of reverberation measurements from which we determine the form of the R-L relationship.
description: 29 pages, 5 figures and 9 tables, submitted to ApJ; PDF with full-resolution figures available at http://www.physics.uci.edu/~mbentz/rl.bentz08.pdf
Full-sky map of the ISW and Rees-Sciama effect from Gpc simulations
Creators: name: Cai, Yan-Chuan
name: Cole, Shaun
name: Jenkins, Adrian
name: Frenk, Carlos S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a new method for constructing maps of the secondary temperature fluctuations imprinted on the cosmic microwave background (CMB) radiation by photons propagating through the evolving cosmic gravitational potential. Large cosmological N-body simulations are used to calculate the complete non-linear evolution of the peculiar gravitational potential. Tracing light rays back through the past lightcone of a chosen observer accurately captures the temperature perturbations generated by linear (the integrated Sachs-Wolfe or ISW effect) and non-linear (the Rees-Sciama or RS effect) evolution. These effects give rise to three kinds of non-linear features in the temperature maps. (a) In overdense regions, converging flows of matter induce cold spots of order 100 Mpc in extent which can dominate over the ISW effect at high redshift, and are surrounded by hot rings. (b) In underdense regions, the RS effect enhances ISW cold spots which can be surrounded by weak hot rings. (c) Transverse motions of large lumps of matter produce characteristic dipole features, consisting of adjacent hot and cold spots separated by a few tens of Megaparsecs. These non-linear features are not easily detectable; they modulate the ISW sky maps at about the 10 percent level. The RS effect causes the angular power spectrum to deviate from linear theory at l~50 and generates non-Gaussianity, skewing the one-point distribution function to negative values. Cold spots of similar angular size, but much smaller amplitude than the CMB cold spot reported by Cruz et al. are produced. Joint analysis of our maps and the corresponding galaxy distribution may enable techniques to be developed to detect these non-linear, non-Gaussian features. Our maps are available at http://astro.dur.ac.uk/~cai/ISW
description: typos corrected, version with high resolution images at http://star-www.dur.ac.uk/~cai/ISWPaper/ISW.pdf
Nuclear energy density functional from chiral pion-nucleon dynamics revisited
Creators: name: Kaiser, N.
name: Weise, W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We use a recently improved density-matrix expansion to calculate the nuclear energy density functional in the framework of in-medium chiral perturbation theory. Our calculation treats systematically the effects from $1π$-exchange, iterated $1π$-exchange, and irreducible $2π$-exchange with intermediate $Δ$-isobar excitations, including Pauli-blocking corrections up to three-loop order. We find that the effective nucleon mass $M^*(ρ)$ entering the energy density functional is identical to the one of Fermi-liquid theory when employing the improved density-matrix expansion. The strength $F_\nabla(ρ)$ of the $(\vec\nabla ρ)^2$ surface-term as provided by the pion-exchange dynamics is in good agreement with that of phenomenological Skyrme forces in the density region $ρ_0/2
description: 18 pages, 7 figures, submitted to Nuclear Physics A
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐ½Ð¾Ð², Ð®ÑÐ¸Ð¹
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: Ð²ÐµÐ±-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ
ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ°
Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð°

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ ÑÐ°ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð¸ ÑÑÐµÑÐ° ÐºÐ½Ð¸Ð³ Ð² ÑÐ¾Ð½Ð´Ðµ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð¡ÐÐ±ÐÐ£. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¾Ð½Ð´Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÑÐºÑÑÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾ ÑÐ¾Ð½Ð´Ðµ Ð¸ ÑÐ¸ÑÐ°ÑÐµÐ»ÑÑ Ð² Ð±Ð°Ð·Ð°Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½Ð¾-Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ (ÐÐÐÐ¡), ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð¸Ð·Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐ¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð²Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ñ ÐÐÐÐ¡, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½ÑÐµÐ³ÑÐ°ÑÐ¸Ð¸ ÐÐÐÐ¡ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÑÐ»Ñ Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸. Ð¦ÐµÐ»ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð° Ð¡ÐÐ±ÐÐ£. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐµ Ð¸Ð·Ð²Ð»ÐµÐºÐ°ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÐºÐ½Ð¸Ð³Ð°Ñ Ð¸Ð· ÐÐÐÐ¡ Ð¿Ð¾ Ð·Ð°ÑÐ°Ð½ÐµÐµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð²ÑÐ±Ð¾ÑÐºÐµ ÐºÐ½Ð¸Ð³, Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¾ÑÑ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÑÐ¸ÑÐ°Ð½Ñ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÑÐºÐµ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð°, Ð¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÑÑÑ ÑÑÐ¸ ÐºÐ½Ð¸Ð³Ð¸ Ð¿Ð¾ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼ Ð³ÑÑÐ¿Ð¿Ð°Ð¼ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾Ð± ÑÑÐ¾Ð¹ ÐºÐ½Ð¸Ð³Ðµ, ÐºÐ¾ÑÐ¾ÑÐ°Ñ ÑÑÐ°Ð½Ð¸ÑÑÑ Ð² Ð±Ð°Ð·Ðµ Ð´Ð°Ð½Ð½ÑÑ. ÐÐ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¾ÑÑÐµÑÑ Ð² Ð²Ð¸Ð´Ðµ ÑÐ°Ð¹Ð»Ð° MS Word (Ð´Ð»Ñ Ð²ÑÐ³ÑÑÐ·ÐºÐ¸) Ð¸ Ð² Ð²Ð¸Ð´Ðµ HTML-ÑÑÑÐ°Ð½Ð¸ÑÑ Ð´Ð»Ñ Ð¿ÑÐ¾ÑÐ¼Ð¾ÑÑÐ°.
The Black Hole Mass-Bulge Luminosity Relationship for Active Galactic Nuclei from Reverberation Mapping and Hubble Space Telescope Imaging
Creators: name: Bentz, Misty C.
name: Peterson, Bradley M.
name: Pogge, Richard W.
name: Vestergaard, Marianne
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the relationship between black hole mass and bulge luminosity for AGNs with reverberation-based black hole mass measurements and bulge luminosities from two-dimensional decompositions of Hubble Space Telescope host galaxy images. We find that the slope of the relationship for AGNs is 0.76-0.85 with an uncertainty of ~0.1, somewhat shallower than the M_BH \propto L^{1.0+/-0.1} relationship that has been fit to nearby quiescent galaxies with dynamical black hole mass measurements. This is somewhat perplexing, as the AGN black hole masses include an overall scaling factor that brings the AGN M_BH-sigma relationship into agreement with that of quiescent galaxies. We discuss biases that may be inherent to the AGN and quiescent galaxy samples and could cause the apparent inconsistency in the forms of their M_BH-L_bulge relationships.
description: 5 pages, 3 figures and 2 tables, submitted to ApJ Letters
title: ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² ÑÐµÐ¾ÑÐ¸Ñ Ð½ÐµÑÐ¿Ð¾ÑÑÐ´Ð¾ÑÐµÐ½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼. ÐÐ¾ÐºÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¾Ð±ÑÐºÐ¸Ð½, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 2000
Subjects: Ð¢Ð²ÐµÑÐ´ÑÐµ ÑÐµÐ»Ð°

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ ââÐ¤Ð¸Ð·Ð¸ÐºÐ° ÑÐ²ÐµÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°â Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 553100 âÐ¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°â Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑÐ¼ 553102 âÐ¤Ð¸Ð·Ð¸ÐºÐ° Ð¸ ÑÐµÑÐ½Ð¸ÐºÐ° Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²â Ð¸ 553104 âÐ¤Ð¸Ð·Ð¸ÐºÐ° Ð½Ð¸Ð·ÐºÐ¾ÑÐ°Ð·Ð¼ÐµÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑâ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð¿ÐµÑÐ²ÑÑ ÑÐ°ÑÑÑ ÐºÑÑÑÐ° Ð»ÐµÐºÑÐ¸Ð¹ "Ð¢ÐµÐ¾ÑÐ¸Ñ Ð½ÐµÑÐ¿Ð¾ÑÑÐ´Ð¾ÑÐµÐ½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼", ÑÐ¸ÑÐ°ÐµÐ¼ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¡ÐÐ±ÐÐ¢Ð£ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾ Ñ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ ÐºÑÑÑÐ¾Ð¼ "Ð¤Ð¸Ð·Ð¸ÐºÐ° ÑÐ²ÐµÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°", Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½ÑÐ¼ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð°Ð¼. ÐÐ±ÑÑÐ¶Ð´Ð°ÑÑÑÑ ÑÑÑÑÐºÑÑÑÐ° Ð½ÐµÑÐ¿Ð¾ÑÑÐ´Ð¾ÑÐµÐ½Ð½ÑÑ ÑÐ²ÐµÑÐ´ÑÑ ÑÐµÐ», ÑÐµÐ¾ÑÐ¸Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹, Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÑÑ Ð¸ Ð´ÐµÑÐµÐºÑÐ°Ñ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð°, Ð¸ Ð¿ÑÑÐ¶ÐºÐ¾Ð²Ð°Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¿Ð¾ Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐ¼ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸ÑÐ¼.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Discrete Hirota dynamics for AdS/CFT
Creators: name: Hegedus, Arpad
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Recently a set of functional equations defining the anomalous dimensions of arbitrary local single trace operators in planar N=4 supersymmetric Yang-Mills theory has been conjectured. These functional equations take the form of a Y-system defined on a special shaped domain. This Y-system can be equivalently reformulated as a T-system defined on a "T-shaped fat hook". The elements of the T-system satisfy discrete Hirota equations. In the present paper the discrete Hirota equations for AdS/CFT are solved by means of a chain of Backlund transformations and as a result TT-, TQ-, and QQ-relations are obtained for AdS/CFT.
description: published version, typos corrected
General Electric Quarterly Survey 78-02, Versions I & II and College Student Version
Creators: name: Electric, General
Publisher: name: Roper Center for Public Opinion Research
Year: 2022

description: Adult sample: Most interesting concerns (3); local community interests (1); solving community issues (2); interest in national issues (1); national issues discussions (15); race relations (1); future race relations (1); companies helping race relations (1); electricity fuels (3); future fuels (2); electricity rates (3); taxes for community services (28); thinking about government policies (14); government controlling labor (1); health measures (1); company effects (1); dollar value changes (5); free time (1); television viewing habits (2); reading habits (2); income change (1); price changes (4); financial situation (1); unemployment (1); saving money (1); inflation (1); spending habits (8); housing expenses (1); automobile expenses (1). College student sample: Most interesting concern (3); national issues discussions (15); race relations (1); future race relations (1); companies helping race relations (1); electricity fuels (2); future fuels (2); government activity changes (12); defense spending (7); company effects (1); dollar value changes (5); free time (1); television viewing habits (2); reading habits (2); college attended (2); class year (1); major (1); degree (1); preferred career (2); academic standing (1); saving money (1).
Additional file 1 of Ethnic differences in COVID-19 mortality in the second and third waves of the pandemic in England during the vaccine rollout: a retrospective, population-based cohort study
Creators: name: Bosworth, Matthew L.
name: Ahmed, Tamanna
name: Larsen, Tim
name: Lorenzi, Luke
name: Morgan, Jasper
name: Ali, Raghib
name: Goldblatt, Peter
name: Islam, Nazrul
name: Khunti, Kamlesh
name: Raleigh, Veena
name: Ayoubkhani, Daniel
name: Bannister, Neil
name: Glickman, Myer
name: Nafilyan, Vahé
Publisher: name: figshare
Year: 2023
Subjects: Medicine
Biotechnology
Science Policy
Computational Biology

description: Additional file 1: Fig. S1. Percentage of people with different postcodes in GP records and 2011 Census by age group. Fig. S2. Directed acyclic graph of the hypothesised relationship between ethnicity and COVID-19 mortality. Table S1. Rates and odds ratios of linkage failure between the 2011 Census and 2011 to 2013 NHS Patient Registers for people living in England at the 2011 Census who were aged 30-100 years in 2020, by sex, age group, ethnicity, region and IMD decile. Table S2. Coding and source of variables included in the analysis. Table S3. Weighted mean follow-up time in days by ethnic groups for wave two and wave three. Table S4. Age-standardised mortality rates (ASMRs) of death involving COVID-19 (8 December 2020 to 1 December 2021) for disaggregated ‘White other’ and ‘Other’ ethnic groups.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ²Ð¸ÑÐ° push-ÑÐ²ÐµÐ´Ð¾Ð¼Ð»ÐµÐ½Ð¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð°ÑÐ±Ð°Ð·Ð¾Ð², ÐÐ»Ð³Ð°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: push
grpc
android
amazon

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¾ÑÐ½Ð¾ÑÐ¸ÑÑÑ Ðº ÑÑÐµÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²ÐµÐ± ÑÐµÑÐ²Ð¸ÑÐ¾Ð². Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐÐ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð¾Ð±ÑÐµÐ½Ð¸Ñ Ñ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼Ð¸. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐµÑÑ Ð¸Ð´ÐµÑ Ð¾ Ð²ÑÐ±Ð¾ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÑÑÑ Ð¸ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°. Ð ÑÐµÑÐ²ÐµÑÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÑÑÐ½Ð¾Ðµ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°.
title: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÐµÐ¼Ðµ: Â«Ð¡Ð¸ÑÑÐµÐ¼Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹Â».
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¼Ð¾ÑÐ¾Ð²Ð°, ÐÐ°ÑÐ°Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: ÐÐ¸Ð½ÐµÐ¹Ð½ÑÐµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ
ÐÐ°ÑÑÐ¸ÑÑ (Ð¼Ð°Ñ.)
ÐÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»Ð¸ (Ð¼Ð°Ñ. )

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²ÐºÐ¸ ÑÐµÐ¾ÑÐµÐ¼, ÐºÐ¾ÑÐ¾ÑÑÐ¼Ð¸ Ð´Ð¾Ð»Ð¶ÐµÐ½ Ð¾Ð²Ð»Ð°Ð´ÐµÑÑ ÑÑÑÐ´ÐµÐ½Ñ, Ð¸Ð·ÑÑÐ¸Ð² ÑÐ°Ð·Ð´ÐµÐ» Â«Ð¡Ð¸ÑÑÐµÐ¼Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹Â». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÐÐÐÐ£ ÐÐ Â«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¸ÐºÐ¾Ð³Ð¾Â» Ð¿Ð¾ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÑÑÑÐ°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°Â» Ð¿Ð¾ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð²ÑÐµÑ Ð¾Ð±ÑÐµÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²ÑÑ Ð´Ð²ÑÑ ÐºÑÑÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð±Ð°Ð·Ð¾Ð²ÑÐ¹ ÐºÑÑÑ Ð²ÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸.
A Synchrotron Self-Compton Scenario for the Very High Energy Gamma-ray Emission of the Intermediate BL Lacertae object W Comae
Creators: name: Zhang, Jin
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: W Comae has significant variability in multi-wavelengthes, from the radio to the gamma-ray bands. A bright outburst in the optical and X-ray bands was observed in 1998, and most recently, a strong TeV flare was detected by VERITAS in 2008. It is the first TeV intermediate-frequency-peaked BL Lacertae (IBL) source. I find that both the broadband spectral energy distributions (SEDs) quasi-simultaneously obtained during the TeV flare and during the optical/X-ray outburst are well fit by using a single-zone synchrotron + synchrotron-self-Compton (SSC) model. The satisfactory fitting requires a large beaming factor, i.e., $δ\sim 25$ and $δ\sim 20$ for the TeV flare and the optical/X-ray outburst, respectively, suggesting that both the optical/X-ray outburst and the TeV flare are from a relativistic jet. The size of the emission region of the TeV flare is three times larger than that of the optical/X-ray outburst, and the strength of the magnetic field for the TeV flare is $\sim 14$ times smaller than that of the X-ray/optical outburst, likely indicating that the region of the TeV flare is more distant from the core than that of the X-ray/optical outburst. The IC component of the TeV flare peaks at around 1.3 GeV, but it is around 20 MeV for the X-ray/optical outburst, lower than that for the TeV flare with 2 orders of magnitude. The model predicts that the optical/X-ray outburst might be accompanied by a strong MeV/GeV emission, but the TeV flare may be not associated with the X-ray/optical outburst. The GeV emission is critical to characterize the SEDs of the optical/X-ray outburst and the TeV flare. The predicted GeV flux is above the sensitivity of \emph{Fermi}/LAT, and it could be verified with the observations by \emph{Fermi}/LAT in near future.
description: 7 pages, including 1 table and 1 figure. To appear in Research in Astronomy and Astrophysics (RAA)
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð»Ð°Ð½Ð´ÑÐ°ÑÑÐ¾Ð²
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
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Year: 2018
Subjects: Ð»Ð°Ð·ÐµÑÐ½Ð¾Ðµ ÑÐºÐ°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐµÐ¹ Ð¿Ð¾ Ð¾Ð±Ð»Ð°ÐºÐ°Ð¼ ÑÐ¾ÑÐµÐº, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¿ÑÑÐµÐ¼ Ð½Ð°Ð·ÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð»Ð°Ð·ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐºÐ°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð´Ð»Ñ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð´Ð°Ð½Ð¸Ð¹. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð²ÑÐ±Ð¾Ñ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ñ Ð² ÑÐµÐ±Ñ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð»Ð°Ð½Ð´ÑÐ°ÑÑÐ° Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÐ°ÑÑÐµÑÐ½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ.
Developing, testing, and fabricating a novel bileaflet mechanical heart valve : the iValve
Creators: name: Goode, Dylan James Ellingham
Publisher: name: University of British Columbia
Year: 2024

description: Valvular heart disease primarily affects the aortic and mitral valves due to higher left-sided heart pressures, often leading to complications like leaflet calcification (stenosis), which impairs valve function and can result in congestive heart failure, necessitating valve replacement. Three forms of valve replacement exist: bioprosthetic valves using bovine or porcine tissue, transcatheter valves combining bioprosthetic components with collapsible stents, and mechanical heart valves (MHVs) made from rigid synthetic materials ensuring unidirectional blood flow. Among MHVs, the bileaflet mechanical heart valve (BMHV) is a modern and durable option that can last a patient’s lifetime, unlike bioprosthetic valves. However, BMHVs require lifelong anticoagulation therapy to prevent thrombosis. Thrombogenicity in BMHVs primarily occurs during the closing phase, where regurgitant flow converts into jets as the orifice narrows, and during hinge washing in the closed phase, which can generate high shear stress and trigger thrombosis. This research addresses the design, testing, and fabrication challenges of developing a novel BMHV that mimics the native valve’s hemodynamics while potentially reducing the need for lifelong anticoagulation therapy. The objectives include: (1) designing a BMHV with improved hemodynamic characteristics; (2) performing structural, kinematic, and kinetic analyses to validate performance; (3) experimentally testing the BMHV under various conditions and comparing it to industry-standard valves; and (4) identifying opportunities for further optimization. The central hypothesis suggests that the novel BMHV will exhibit hemodynamic performance akin to the native valve, potentially reducing or eliminating the need for anticoagulation while ensuring durability. Computational simulations, finite element analysis, and in vitro testing were used to assess the novel BMHV prototypes. Validation results highlighted a stress-dispersing hinge design that minimizes stress concentrations and ensures hinge washing during low-stress forward flow. Kinematic and kinetic findings supported the hypothesis, indicating native-like performance during the valve opening and closing phases, potentially negating the need for anticoagulation therapy. This research offers advancements in cardiovascular care, reducing anticoagulation risks, improving patient outcomes, and enhancing the quality of life for individuals with valvular heart disease.