cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¶Ð¸Ð»Ð¾Ð¹ Ð´Ð¾Ð¼
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ»Ð¸Ðº, ÐÐ²Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
ÐºÐ¾ÑÑÐµÐ´Ð¶
ÑÐ°ÑÑÐµÑÑ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¼ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½Ñ ÑÑÐ°Ð¿Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¾Ð±ÑÐµÐºÑÐ° Ð¼Ð°Ð»Ð¾ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð´Ð²ÑÑÑÐµÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°, ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð²Ð¾ ÐÑÐµÐ²Ð¾Ð»Ð¾Ð¶ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸, ÐÑÐ±Ð¾ÑÐ³ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐµ, ÐÐ°Ð²Ð¾Ð´ÑÐºÐ°Ñ ÑÐ». ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ¼Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ ÑÐ¾ÑÑÐ¾Ð¼ ÑÐ¿ÑÐ¾ÑÐ° Ð½Ð° Ð¶Ð¸Ð»ÑÐµ Ð² Ð½Ð¾Ð²Ð¾ÑÑÑÐ¾Ð¹ÐºÐ°Ñ ÑÐ¾ ÑÑÐ¾ÑÐ¾Ð½Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ð¼ Ð¿ÑÐ¸ÑÐ¸Ð½Ð°Ð¼: ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÑÐ°Ð²Ð¾Ðº Ð¿Ð¾ Ð¸Ð¿Ð¾ÑÐµÑÐ½ÑÐ¼ ÐºÑÐµÐ´Ð¸ÑÐ°Ð¼; Ð²ÑÐµ ÑÐ°ÑÐµ Ð²ÑÐ±Ð¾Ñ Ð¿Ð¾ÐºÑÐ¿Ð°ÑÐµÐ»ÐµÐ¹ Ð¿ÑÐ¸ Ð¿Ð¾ÐºÑÐ¿ÐºÐµ Ð¶Ð¸Ð»ÑÑ Ð¾Ð±ÑÐ°ÑÐ°ÐµÑÑÑ Ð² ÑÑÐ¾ÑÐ¾Ð½Ñ Ð±Ð»Ð¸Ð¶Ð°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÐ¸Ð³Ð¾ÑÐ¾Ð´Ð°; Ð´Ð¾ÑÑÑÐ¿Ð½Ð°Ñ ÑÐµÐ½Ð°, Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ ÑÐµÐ½Ð¾Ð¹ Ð² Ð¿ÑÐµÐ´ÐµÐ»Ð°Ñ ÐÐÐ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð¾Ð²ÑÑ Ð¼Ð¸ÐºÑÐ¾ÑÐ°Ð¹Ð¾Ð½Ð°Ñ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð½Ð° Ð³ÑÐ°Ð½Ð¸ÑÐµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°; ÑÑÐ°ÑÐµÐ½Ð¸Ðµ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð°. Ð¡ ÐºÐ°Ð¶Ð´ÑÐ¼ Ð³Ð¾Ð´Ð¾Ð¼ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ Ð²ÑÐµ ÑÐ»Ð¾Ð¶Ð½ÐµÐµ Ð½Ð°Ð¹ÑÐ¸ ÐºÐ²Ð°ÑÑÐ¸ÑÑ Ð½Ð° Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾Ð¼ ÑÑÐ½ÐºÐµ, Ð¾ÑÐ²ÐµÑÐ°ÑÑÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð¿Ð¾ÐºÑÐ¿Ð°ÑÐµÐ»ÐµÐ¹. ÐÑÐ¾ÑÐµÑÑ ÑÑÐ°ÑÐµÐ½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð½ÐµÐ¾Ð±ÑÐ°ÑÐ¸Ð¼, Ð° Ð² ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ Ð¾Ð½ ÑÑÑÐ³ÑÐ±Ð»ÑÐµÑÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ½ÑÐ¼ Ð²ÐµÑÑÐ¸Ð¼ ÑÐ¾Ð½Ð´Ð¾Ð¼. Ð ÑÑÐ¾Ñ Ð¿ÑÐ¾ÑÐµÑÑ Ð½ÐµÐ»ÑÐ·Ñ ÐºÐ¾Ð¼Ð¿ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°ÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¼Ð¾Ð½ÑÐ°.
MPEC 2023-K113 : 2023 KA2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 KA2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Yves Klein, un artista e il suo blu
Creators: Francesca Brunetti
Publisher: name: Media Inaf
Year: 2018

Martedì 3 luglio, all’Inaf di Arcetri (FI), laboratorio di pittura per bambini con Fausto Gilberti, illustratore e artista. Il protagonista sarà il colore blu: il blu del cielo e il blu saturo e luminoso brevettato da Yves Klein come International Klein Blue
The effects of atmospheric ionization on insects measured with a stationary flight apparatus
Creators: name: Hildebrandt, Jacob
Publisher: name: University of British Columbia
Year: 2012

description: In recent years a number of publications have shown a renewed interest in the possible effects of atmospheric electricity on biological systems. The work here presented is an attempt to measure the changes in the behaviour, or the power output, of certain insects during stationary flight in a unipolar atmosphere. Since several published references indicate the existence of a "weather sense" in insects, which has been attributed to sensitivity to atmospheric space charge fluctuations, various species of flies were chosen for this study. Various studies have been carried out on insect flight endurance with flight mills. For this work a new type of closed insect flight, apparatus has been developed, in which environmental conditions can be altered, and the pull and wing beat frequency of the fly under test recorded simultaneously. Insects were attached to a mechano-electrical transducer either directly or indirectly. The transducer output was resolved into an AC component, whose frequency corresponds to the wing beat frequency, and a DC component whose magnitude corresponds to the force exerted by the insect in flight. Both components were traced on graphical recorders. In a modified apparatus two transducers were used for measuring the pull and wing beat frequency independently. Even under identical physical conditions insects were found to behave in an erratic manner, so that possible small effects due to variations of the ion concentration were difficult to establish. The spiracles of some flies were dilated by increasing the ambient CO₂ concentration up to 15% causing various changes in the flight patterns without rendering them more regular. From a statistical analysis of the energies produced, some evidence can be obtained that individuals of Muscina stabulans and Lucilia sericata under a negative ionization excess display greater activity than those under normal conditions or under positive ion excess. More tests will be necessary to substantiate the results. The use of the apparatus as an entomological olfactometer or for the test of other insect responses is suggested; several insect repellents were tested on the same apparatus.
Angelo Secchi, un francobollo per il bicentenario
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2018

L’illustre scienziato gesuita – nato duecento anni fa, il 28 giugno 1818 – divenne famoso a livello internazionale per i suoi studi in diverse branche, ma lasciò il segno nella comunità astronomica per il suo ruolo fondamentale nello studio degli spettri delle stelle e della loro classificazione che è a fondamento dell’indagine astronomica moderna
A forma di sigaro, ma pur sempre una cometa
Creators: Sara Venturi
Publisher: name: Media Inaf
Year: 2018

Postulando che si tratti di una cometa in miniatura, dalla peculiare forma oblunga, uno studio su Nature guidato da Marco Micheli, ricercatore dell'Esa, ha scoperto che la spinta dei gas emessi da ‘Oumuamua può essere una spiegazione fisica coerente della componente non gravitazionale del moto di questo pellegrino interstellare
Nuovi limiti dimensionali per le stelle di neutroni
Creators: Matteo Boni
Publisher: name: Media Inaf
Year: 2018

Il rilevamento dell’onda gravitazionale Gw 170817 aiuta a rispondere ad un vecchio quesito riguardante i corpi più densi dell’universo: un nuovo calcolo statistico stima che il raggio di una stella di neutroni media sia compreso tra i 12 e i 13.5 chilometri
Twins: The Two Shortest Period Non-Interacting Double Degenerate White Dwarf Stars
Creators: name: Mullally, F.
name: Badenes, Carles
name: Thompson, Susan E.
name: Lupton, Robert
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report on the detection of the two shortest period non-interacting white dwarf binary systems. These systems, SDSS J143633.29+501026.8 and SDSS J105353.89+520031.0, were identified by searching for radial velocity variations in the individual exposures that make up the published spectra from the Sloan Digital Sky Survey. We followed up these systems with time series spectroscopy to measure the period and mass ratios of these systems. Although we only place a lower bound on the companion masses, we argue that they must also be white dwarf stars. With periods of approximately 1 hour, we estimate that the systems will merge in less than 100 Myr, but the merger product will likely not be massive enough to result in a Type 1a supernova.
description: 9 pages, accepted by ApJ Letters
Implementation of knowledge models
Creators: name: Van Bekkum, Michael
name: Rongen, Sjoerd
name: Nikolova, Nikoletta
Publisher: name: Zenodo
Year: 2022
Subjects: AAS, Ontology, Semantics, Knowledge model

description: Formal knowledge models are one of the underpinnings of the MAS4AI project. MAS4AI implements a Multi Agent System (MAS), with many assets in the manufacturing processes represented by agents. Knowledge models provide a common reference for knowledge among the agents and function as a basis for a common language in the use cases and in the project.
 There are two different sources of knowledge for the agent in MAS4AI: (1) knowledge about a manufacturing application domain, which is defined in the ontology and (2) characteristics and properties of individual agents, which are defined in the Asset Administration Shell (AAS). Within MAS4AI the latter serves to communicate more specific semantics and defines the messages sent between agents.
On the minimal norm of a non-regular generalized character of an arbitrary finite group
Creators: name: Robinson, Geoffrey R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Representation Theory (math.RT)
subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 20C20

description: We prove that for any finite group G, the sum across non-identity elements of the squared absolute value of any generalized character of G which does not vanish on all non-identity elements of G is at least |G|/d -1, where d is the maximal degree of a complex irreducible character of G, and we identify all cases where this minimum possible value is attained.
description: 7 pages
title: ÐÐµÑÐµÐ¶Ð»Ð¸Ð²Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ ÐºÐ°Ðº ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼
Creators: name: ÐÑÑÐ°Ð¿ÐµÐ½ÐºÐ¾, Ð®Ð»Ð¸Ñ
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ  ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð²ÑÐ·Ð¾Ð²ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2019; 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: 2019

description: Ð ÑÐ¾Ð´Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°ÑÐ¸ÐºÐ¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð±ÐµÑÐµÐ¶Ð»Ð¸Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð¾Ð±Ð¾Ð·Ð½Ð°ÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð±ÐµÑÐµÐ¶Ð»Ð¸Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÐºÐ°Ðº ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐ¹ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð ÑÑÐ°ÑÑÐµ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Â«Ð±ÐµÑÐµÐ¶Ð»Ð¸Ð²Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾Â» ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ, ÑÐµÐ»ÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿ÑÑÐµÐ¼ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð°, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð·Ð° ÑÑÐµÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð½Ðµ Ð¿ÑÐ¸Ð½Ð¾ÑÑÑÐ¸Ðµ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸, ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¸ ÑÑÐ»ÑÐ³.
Il Governatore Generale d’Australia visita l’Inaf
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2018

Una splendida giornata ha fatto da cornice alla visita di Sir Peter Cosgrove, accompagnato dalla moglie, l'Ambasciatore australiano in Italia, Greg French. La delegazione ufficiale ha ha incontrato il Presidente dell'Inaf, il Nichi D'Amico, e il suo staff.  Il Governatore Generale ha detto: «L'Australia e l'Italia sono partner nella ricerca di una maggiore conoscenza del nostro universo. È stato meraviglioso ascoltare come il lavoro dell’Inaf, in collaborazione con scienziati e ricercatori australiani, contribuirà a ottenere importanti scoperte scientifiche»
La ricetta degli ammassi stellari
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2018

Trovato un modello convincente per la formazione degli ammassi stellari, che si applica a tutte le scale di massa, dai piccoli ai grandi ammassi. Il processo sembra essere universale, nello spazio e nel tempo. In altre parole, dovrebbe funzionare in qualsiasi momento della storia dell'universo, in ogni galassia
Additional file 1 of Factors associated with intraoperative extracorporeal membrane oxygenation support during lung transplantation
Creators: name: Zhang, Rong
name: Xu, Yonghao
name: Sang, Ling
name: Chen, Sibei
name: Huang, Yongbo
name: Nong, Lingbo
name: Yang, Chun
name: Liu, Xuesong
name: Liu, Dongdong
name: Xi, Yin
name: He, Weiqun
name: Wei, Bing
name: He, Jianxing
name: Li, Yimin
name: Liu, Xiaoqing
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Science Policy

description: Additional file 1 Figure 4. Process reports intraoperative ECMO support in LTX patients. PA (pulmonary artery); LTX (lung transplantation).
Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud
Creators: name: Bonanos, A. Z.
name: Massa, D. L.
name: Sewilo, M.
name: Lennon, D. J.
name: Panagia, N.
name: Smith, L. J.
name: Meixner, M.
name: Babler, B. L.
name: Bracker, S.
name: Meade, M. R.
name: Gordon, K. D.
name: Hora, J. L.
name: Indebetouw, R.
name: Whitney, B. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a catalog of 1750 massive stars in the Large Magellanic Cloud, with accurate spectral types compiled from the literature, and a photometric catalog for a subset of 1268 of these stars, with the goal of exploring their infrared properties. The photometric catalog consists of stars with infrared counterparts in the Spitzer SAGE survey database, for which we present uniform photometry from 0.3-24 microns in the UBVIJHKs+IRAC+MIPS24 bands. The resulting infrared color-magnitude diagrams illustrate that the supergiant B[e], red supergiant and luminous blue variable (LBV) stars are among the brightest infrared point sources in the Large Magellanic Cloud, due to their intrinsic brightness, and at longer wavelengths, due to dust. We detect infrared excesses due to free-free emission among ~900 OB stars, which correlate with luminosity class. We confirm the presence of dust around 10 supergiant B[e] stars, finding the shape of their spectral energy distributions (SEDs) to be very similar, in contrast to the variety of SED shapes among the spectrally variable LBVs. The similar luminosities of B[e] supergiants (log L/Lo>=4) and the rare, dusty progenitors of the new class of optical transients (e.g. SN 2008S and NGC 300 OT), plus the fact that dust is present in both types of objects, suggests a common origin for them. We find the infrared colors for Wolf-Rayet stars to be independent of spectral type and their SEDs to be flatter than what models predict. The results of this study provide the first comprehensive roadmap for interpreting luminous, massive, resolved stellar populations in nearby galaxies at infrared wavelengths.
description: 57 pages, 19 figures, 5 tables, accepted for publication in the Astronomical Journal (v3 corrects typos)
title: ÐÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð¾Ñ ÑÐ°Ð½Ð° ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹
Creators: name: Ð¡ÑÐµÐ¿Ð°Ð½Ð¾Ð², ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 2001
Subjects: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÐµÐ³Ð¾ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð¾ÑÑÐ°Ð½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÐºÐ°Ðº ÑÐ¾Ð²Ð¾ÐºÑÐ¿Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹, ÑÑÐ°ÑÑÐ²ÑÑÑÐ¸Ñ Ð² Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð¼ Ð¾Ð±Ð¾ÑÐ¾ÑÐµ. ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ðº Ð²Ð¸Ð´Ð° Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¸Ñ Ð¿ÑÐ°Ð². ÐÐ³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ðµ Ð¾Ð±Ð¾ÑÐ¾ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð°Ð²ÑÐ¾Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑ ÐºÐ°Ðº Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ°Ð²Ð¾Ð¼Ð¾ÑÐ¸Ð¹ ÑÑÐ±ÑÐµÐºÑÐ¾Ð² Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÐ¼ÑÑ Ð½Ð¾ÑÐ¼Ð°Ð¼Ð¸ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð°ÐºÑÐ¾Ð², ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð½ÑÑ Ð·Ð° ÑÑÐµÑ ÑÑÐµÐ´ÑÑÐ² ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÐ´Ð¶ÐµÑÐ°.
The status of breeding Hen Harriers Circus cyaneus in the UK and Isle of Man in 2023
Creators: name: Kelly, Leah A.
name: Tománková, Irena
name: Downing, Stephen
name: Lindley, Patrick
name: Mattingley, Wendy
name: Morris, Neil G.
name: Murphy, Stephen
name: Orr-Ewing, Duncan
name: Owens, Ronan
name: Rooney, Eimear
name: Ruddock, Marc
name: Stevenson, Andrew
name: Thomas, Mark
name: Wotton, Simon R.
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Infectious Diseases
subject: FOS: Health sciences

description: The sixth national survey of breeding Hen Harriers in 2023 revealed a near-significant 20% increase in the UK and Isle of Man population since 2016, with variation between and within constituent countries. To estimate the size of the breeding Hen Harrier population in the UK and Isle of Man, constituent countries, Scottish regions and the UK Special Protection Area (SPA) network for breeding Hen Harriers in 2023, and calculate population changes since 2016. Surveys were conducted in all 10-km squares likely to be occupied by breeding birds in England, Northern Ireland, Wales and the Isle of Man, using standard methods. In Scotland, a stratified random selection of 10-km squares within the known breeding range was surveyed alongside squares selected by volunteers. Surveys were conducted in the UK in 2023 and Isle of Man in 2022. The UK and Isle of Man population was estimated at 691 territorial pairs (95% confidence limits, 593–802), a near-significant 20% increase since 2016. Populations increased by differing degrees in all countries and the Isle of Man, except in Northern Ireland where they declined. Scotland held 77% of the population with 529 (95% confidence limits, 431–640) pairs, with only tens of pairs in the other surveyed areas. Overall abundance within SPAs scarcely changed since 2016, but Scottish and Northern Irish SPAs held fewer pairs (−28% and −18%). As in 2016, most Hen Harriers were found on heather-dominated moorland. In Scotland, abundance declines on grouse-shooting moors continued between 2016 and 2023 (−23%), following a significant 67% decline between 2010 and 2016. The 2023 survey showed a near-significant 20% increase in the UK and Isle of Man breeding Hen Harrier population since 2016. There was a substantial increase in England and moderate increases in Scotland, Wales and the Isle of Man, but a continuing decline in Northern Ireland. Breeding numbers within much of the SPA network in Scotland and Northern Ireland were below citation levels, with a more encouraging picture in England and particularly in Wales.
CMB anisotropies induced by tensor modes in Massive Gravity
Creators: name: Bessada, Dennis
name: Miranda, Oswaldo D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study Gravitational Waves (GWs) in the context of Massive Gravity, an extension to General Relativity (GR) where the fluctuations of the metric have a nonzero mass, and specifically investigate the effect of the tensor modes on the Cosmic Microwave Background (CMB) anisotropies. We first study the time evolution of the tensor modes in Massive Gravity and show that there is a graviton mass limit $m_l=10^{-66}g\sim 10^{-29}cm^{-1}$, so that for masses $m\leq m_l$ the tensor perturbations in Massive Gravity are indistinguishable from the corresponding ones in GR. Also, we show that short wavelength massive modes behave almost indistinguishably from their massless counterparts. Later on, we show that massive gravitons with masses within the range $m= 10^{-27}cm^{-1}$ - $m=10^{-26}cm^{-1}$ would leave a clear signature on the lower multipoles ($\ell< 30$) in the CMB anisotropy power spectrum. Hence, our results show that CMB anisotropies measurements might be decisive to show whether the tensor modes are massive or not.
description: Minor typos corrected and title changed to match the version published by JCAP
Agent knowledge access framework
Creators: name: Ronger, Sjoerd
name: Nikolova, Nikoletta
name: Van Bekkum, Michael
Publisher: name: Zenodo
Year: 2022
Subjects: Ontology, AAS, API, Agent knowledge model

description: Whereas deliverable D3.1 showed the design of the knowledge models, this deliverable provides an overview and documentation of the actual models that have been developed as software artefacts. Both the ontology and the AAS models for the agents have been formalized and have been made available as tangible software components. The ontology is created as an RDF model serialized in a Turtle format (.ttl), the AAS models have been created as package files (.aasx).
 The development of the knowledge models follows the design principles of deliverable D3.1 on reusability and extensibility. This means that the ontology practically integrates and extends existing ontologies (MASON, RAMI) and the AAS agent models are developed as a collection of AAS submodels that can be reused across multiple agents.
 In order to be useful, the knowledge models need to be accessible to the use cases, i.e., both need to be hosted in a platform that allows programmatic access via APIs. This document describes how the ontology is hosted in an RDF store in the MAS4AI architecture, whereas the AAS models are hosted in a AAS hosting platform, typically BaSyx.
 The main purpose of this document is:
 - To describe the schema of the ontology, its concepts and the mechanism to access the ontology via queries in a practical use case.
 - Describe the mapping of the models to the standardized AAS metamodel and describe the submodels that have been created for the various agents based on the design in deliverable D3.1.
 The document concludes with a reflection on the practical application of the ontology in use cases, several considerations on the continued development of the AAS models in alignment with the use cases as well as a useful solution to lack of findability of AAS (sub)models.
title: ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº Ð¸Ð· ÑÑÐ°Ð»Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÐ½Ð¸ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ°ÑÐ²ÐµÐµÐ², ÐÐ³Ð¾ÑÑ
name: ÐÐµÑÐ½Ð¸ÑÐºÐ°Ñ, ÐÑÐ´Ð¼Ð¸Ð»Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÐÑÐ»Ð¸Ð²ÐºÐ¸ ÑÑÐ°Ð»ÑÐ½ÑÐµ

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÐºÑÐ°ÑÐºÐ¾ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð·Ð½Ð°Ð½Ð¸Ñ Ð¾ ÑÑÑÑÐºÑÑÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾-ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾Ð³Ð¾ Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð¾ÑÐ½Ð°ÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ²ÐµÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° 22.03.02 Â«ÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÂ», Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº Ð¸Ð· ÑÑÐ°Ð»Ð¸Â» Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÑÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ 22.04.02 â Â«ÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÂ», Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑ Â«Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð»Ð¸ÑÑÑÂ».
Structure, Kinematics, and Chemical Enrichment Patterns after Major Gas-Rich Disc-Disc Mergers
Creators: name: Richard, Simon
name: Brook, Chris B.
name: Martel, Hugo
name: Kawata, Daisuke
name: Gibson, Brad K.
name: Sanchez-Blazquez, Patricia
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 used an N-body smoothed particle hydrodynamics algorithm, with a detailed treatment of star formation, supernovae feedback, and chemical enrichment, to perform eight simulations of mergers between gas-rich disc galaxies. We vary the mass ratio of the progenitors, their rotation axes, and their orbital parameters and analyze the kinematic, structural, and chemical properties of the remnants. Six of these simulations result in the formation of a merger remnant with a disc morphology as a result of the large gas-fraction of the remnants. We show that stars formed during the merger (a sudden starburst occur in our simulation and last for 0.2-0.3 Gyr) and those formed after the merger have different kinematical and chemical properties. The first ones are located in thick disc or the halo. They are partially supported by velocity dispersion and have high [alpha/Fe] ratios even at metallicities as high as [Fe/H]=-0.5. The former ones -- the young component -- are located in a thin disc rotationally supported and have lower [alpha/Fe] ratios. The difference in the rotational support of both components results in the rotation of the thick disc lagging that of the thin disc by as much as a factor of two, as recently observed.We find that, while the kinematic and structural properties of the merger remnant depends strongly upon the orbital parameters of the mergers, there is a remarkable uniformity in the chemical properties of the mergers. This suggests that general conclusions about the chemical signature of gas-rich mergers can be drawn.
description: 17 pages, 20 figures, to be published in MNRAS
Metti alla prova le stelle della galassia nana
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2018

Con i dati della missione Gaia, «prima o poi dovrebbe essere possibile determinare se le stelle delle galassie nane raffigurano un universo in cui è presente materia oscura, oppure no», dice il ricercatore modenese Enrico Garaldi, dottorando all’Università di Bonn e primo autore di uno studio teorico sul comportamento delle stelle nelle piccole galassie satelliti della Via Lattea
New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars
Creators: name: Hubrig, S.
name: Briquet, M.
name: De Cat, P.
name: Schoeller, M.
name: Morel, T.
name: Ilyin, I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B-type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three beta Cephei stars and two stars suspected to be beta Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3sigma has been diagnosed in two normal B-type stars, the nitrogen-rich early B-type star HD52089 and in the B5 IV star HD153716. Roughly one third of beta Cephei stars have detected magnetic fields: Out of 13 beta Cephei stars studied to date with FORS1, four stars possess weak magnetic fields, and out of the sample of six suspected beta Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: roughly half of the 34 SPB stars have been found to be magnetic and among the 16 candidate SPBs eight stars possess magnetic fields. In an attempt to understand why only a fraction of pulsating stars exhibit magnetic fields, we studied the position of magnetic and non-magnetic pulsating stars in the H-R diagram. We find that their domains in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. It is possible that stronger fields tend to be found in stars with lower pulsating frequencies and smaller pulsating amplitudes. A somewhat similar trend is found if we consider a correlation between the field strength and the v sin i-values, i.e. stronger magnetic fields tend to be found in more slowly rotating stars.
description: 13 pages, 10 figures, 4 tables, accepted for publication in Astronomische Nachrichten
รูปแบบการบูรณาการหลักสูตรโดยน้อมนำตามศาสตร์พระราชาร่วมกับ การใช้อัตลักษณ์เชิงพื้นที่เพื่อเสริมสร้างการรู้เรื่องสิ่งแวดล้อมสำหรับ ผู้เรียนระดับการศึกษาขั้นพื้นฐาน
Creators: name: สมเกียรติ อินทสิงห์
Publisher: name: มหาวิทยาลัยราชภัฏเชียงใหม่
Year: 2021
Subjects: การบูรณาการหลักสูตร
ศาสตร์พระราชา
อัตลักษณ์เชิงพื้นที่
การรู้เรื่องสิ่งแวดล้อม

description: วารสารวิจัยราชภัฏเชียงใหม่, 22, 3, 74-93
Additional file 5 of Establishment of a prognostic signature for lung adenocarcinoma using cuproptosis-related lncRNAs
Creators: name: Yalimaimaiti, Saiyidan
name: Liang, Xiaoqiao
name: Zhao, Haili
name: Dou, Hong
name: Liu, Wei
name: Yang, Ying
name: Ning, Li
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Additional file 5. The detail data of nomogram and calibration.
An analysis of short period (10-30 seconds) geomagnetic micropulsations
Creators: name: Hassett, John Henry
Publisher: name: University of British Columbia
Year: 2012

description: Geomagnetic micropulsations are described and possible origins discussed. Previous work in Canada is reviewed with particular attention to the normal daytime Pc oscillations with periods from 10 - 30 seconds. A description is given of the work done correlating the amplitude and direction of the exciting vector at two stations. Field work at Ralston, Alberta during July -August 1959 is described in detail. A digital computer is used to obtain the auto-correlation coefficient and the covariance of the horizontal components of the vector. From these two paramenters the dominant frequency, amplitude, and polorization of the vector are obtained. The conclusion is reached that normal daytime Pc's seem to occur in a small band centred around a dominant frequency. Two such dominant frequencies may occur simultaneously and the vectors can have different polarization. The amplitude and direction of a given Pc seems to follow a closed diurnal pattern reaching a maximum slightly before local noon.
Nasa: come riconoscere la vita?
Creators: Paolo Soletta
Publisher: name: Media Inaf
Year: 2018

Questa domanda, apparentemente banale, è alla base della formazione del Nexus for Exoplanet System Science (NExSS), piattaforma di studio multidisciplinare in cui gli astronomi, biologi e geologi possono confrontarsi sui criteri da applicare alle biosignature su altri mondi
What works in schools? Revising expert and novice teachers' beliefs about school effectiveness: An international comparison
Creators: name: Stricker, Luisa
Publisher: name: PsychArchives
Year: 2025
Subjects: subject: Hattie
subject: Visible learning
subject: Teacher beliefs
subject: School effectiveness
subject: Teacher training
subject: International comparison (Norway and Germany)
subject: 150

description: Fleckenstein et al. (2015) found that teachers' beliefs about school effectiveness were misaligned with findings of John Hattie's (2008) first comprehensive meta-analysis concerning the determinants of student achievement. The beliefs of expert teachers were more congruent with Hattie’s findings than those of novice teachers who were more likely to underestimate achievement-related variables and overestimate variables related to school surface and infrastructure conditions and student-internal factors. This study re-examines these findings with current samples in Germany and Norway and compares teachers' beliefs with Hattie's updated meta-analysis from 2023. It also examines whether pre-service teachers’ beliefs are influenced by the type of higher education institution (Pädagogische Hochschule vs. University) and the cultural background (German vs. Norwegian). This research aims to understand how professional experience, higher education and cultural context influence teachers' beliefs, and to provide insights for enhancing professional development and educational policy.
Ingegneria al femminile: Maria Grazia Labate
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2018

Le quote rosa nella scienza e nell'ingegneria ci sono e vanno celebrate. Ecco, allora, come una delle italiane che lavorano per il progetto Square Kilometre Array sta cambiando il futuro dell'ingegneria per le radiofrequenze
องค์ประกอบความเป็นครูนักนวัตกรในการศึกษายุคดิจิทัลเพื่อการพัฒนาท้องถิ่นอย่างยั่งยืน
Creators: name: นวพร ชลารักษ์
Publisher: name: มหาวิทยาลัยราชภัฏเชียงใหม่
Year: 2021
Subjects: ครูนักนวัตกร
ความเป็นครูนักนวัตกร
การพัฒนาท้องถิ่นอย่างยั่งยืน

description: วารสารวิจัยราชภัฏเชียงใหม่, 22, 3, 94-108
Stelle appena nate ma già piene di polvere
Creators: Matteo Boni
Publisher: name: Media Inaf
Year: 2018

Grazie al radiotelescopio Alma, un team europeo di astronomi ha scoperto che le particelle di polvere attorno a una stella in formazione si addensano in grani più grandi prima di quanto atteso. La crescita delle particelle di polvere è il primo passo nella formazione dei pianeti
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ°ÑÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨ÑÑÐµÐºÐµÑ, ÐÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÐµÑÐµÐ´Ð²Ð¸Ð¶Ð½Ð°Ñ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ð°
ÐºÐ°ÑÑÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð²ÑÐ¾Ð¼Ð°Ñ
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Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÑ ÐµÐ¼Ñ
ÑÐ°ÑÑÐµÑÑ
ÑÐµÑÑÐµÐ¶Ð¸
ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÐºÐ°ÑÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐµÐ¼Ð° Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ±Ð¾ÑÐºÐ¸ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÑÑÑÐºÑÑÑÐ½Ð¾-ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¸ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÑÐµÐ¼Ñ ÐºÐ°ÑÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ¸ÐºÐ»Ð¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ ÐºÐ°ÑÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ½Ð¾-ÑÐ¸ÐºÑÐ¸ÑÑÑÑÐµÐ³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð³Ð°Ð±Ð°ÑÐ¸ÑÐ½ÑÐ¹ ÑÐµÑÑÐµÐ¶ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°, ÑÐ±Ð¾ÑÐ¾ÑÐ½ÑÐ¹ ÑÐµÑÑÐµÐ¶ Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ½Ð¾-ÑÐ¸ÐºÑÐ¸ÑÑÑÑÐµÐ³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð°, ÑÐ°Ð±Ð¾ÑÐ¸Ðµ ÑÐµÑÑÐµÐ¶Ð¸ Ð´Ð²ÑÑ Ð´ÐµÑÐ°Ð»ÐµÐ¹ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð´ÑÐ¼Ð°Ð½ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð²ÑÐ±Ð¾Ñ Ð¸ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹, ÐºÐ¸Ð½ÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÑÐ·Ð¸ Ð²ÑÐ¾Ð´ÑÑÐ¸Ñ Ð² Ð½Ð¸Ñ ÐµÐ´Ð¸Ð½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ° Ð¸ ÑÐ°ÑÑÐµÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°.
SU(N) membrane $B\wedge F$ theory with dual-pairs
Creators: name: Singh, Harvendra
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct a SU(N) membrane $B\wedge F$ theory with dual pairs of scalar and tensor fields. The moduli space of the theory is precisely that of $N$ M2-branes on the noncompact flat space. The theory possesses explicit SO(8) invariance and is an extension of the maximal SU(N) super-Yang-Mills theory.
description: 8 pages; Corrected typos and references added; v3: Error deleted and new discussion on quantisation added
title: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
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»ÐµÐ¿Ð¾Ð², ÐÐ¸ÐºÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¿ÑÑÐµÐ¼ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ½Ð°ÑÑÐºÐ¸ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð°ÑÑÐ¸Ð²Ð° ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸. Ð Ð°Ð±Ð¾ÑÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð´Ð»Ñ ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ ÐÐÐ Â«Ð¡Ð¸Ð»Ð¾Ð²ÑÐµ Ð¼Ð°ÑÐ¸Ð½ÑÂ». Ð ÐµÑÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð´Ð¾ÑÑÐ¸Ð³Ð°ÐµÑÑÑ Ð¿ÑÑÐµÐ¼ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐµÐ³Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð³ÑÐ°ÑÐ¸ÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½Ð¾ÑÐ¼ Ð²ÑÐµÐ¼ÐµÐ½Ð¸, ÑÐºÐ°Ð·Ð°Ð½Ð½ÑÑ Ð² ÑÑÐ°Ð½Ð´Ð°ÑÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾ÑÑÐ»ÐµÐ¶Ð¸Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸, ÐµÐµ ÑÐ¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, ÑÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ´Ð°ÑÐ° Ð² Ð°ÑÑÐ¸Ð². ÐÐ¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ¼Ð¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÑÐ¸ÐºÐ¸ Ð¸ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾Ð¹ Ð³ÑÑÐ¿Ð¿Ñ. Ð ÑÐ¾ÑÑÐ°Ð² Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð²ÑÐ¾Ð´Ð¸Ñ Ð±Ð°Ð·Ð° Ð´Ð°Ð½Ð½ÑÑ, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ°Ñ Ð½Ð¾ÑÐ¼Ð°Ð»Ñ Ð¾Ð±Ð¾Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ ÑÐ·Ð»Ð¾Ð² Ð¸ Ð´ÐµÑÐ°Ð»ÐµÐ¹, Ð½Ð¾ÑÐ¼Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ ÑÐµÑÑÐµÐ¶ÐµÐ¹, Ð´Ð°Ð½Ð½ÑÐµ Ð´Ð»Ñ Ð°Ð²ÑÐ¾ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹, ÑÐ°Ð±Ð»Ð¸ÑÑ Ñ Ð·Ð°Ð¿Ð¸ÑÑÐ¼Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð² ÑÐµÑÑÐµÐ¶ÐµÐ¹ Ð¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸Ñ Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¹ Ð°ÑÑÐ¸Ð². ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ñ ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ðµ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¸ Ð¿Ð¾Ð²ÑÑÐ¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹.
title: ÐÐ¸ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¸ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½ÑÑ ÑÑÑÐºÐ¾Ð»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÑÑÐ½ÐµÐ½ÐºÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»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: Ð½Ð°ÑÑÐ¸ÐµÐ²Ð¾-ÐºÐ°Ð»ÑÑÐ¸ÐµÐ²ÑÐµ ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½ÑÐµ ÑÑÐµÐºÐ»Ð°
ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸Ð½Ð³
Ð´Ð¸ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°

description: ÐÐ°ÑÑÐ¸ÐµÐ²Ð¾-ÐºÐ°Ð»ÑÑÐ¸ÐµÐ²ÑÐµ ÑÐ¸Ð»Ð¸ÐºÐ°ÑÐ½ÑÐµ ÑÑÐµÐºÐ»Ð° Ð¿ÑÐ¾ÑÐ²Ð»ÑÑÑ ÑÐ½Ð¸ÐºÐ°Ð»ÑÐ½ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¿Ð¾ÑÐ»Ðµ ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ¸Ð»ÑÐ½Ð¾Ð¼ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¿Ð¾Ð»Ðµ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð²Ð¿ÐµÑÐ²ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð´Ð¸ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ÑÑÐ¾Ð´Ð½ÑÑ Ð¸ Ð·Ð°Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÑÑÐºÐ¾Ð» Ð² ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¼ Ð¸ ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð¼ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ð°Ñ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ ÑÐ°Ð·Ð»Ð¸ÑÐ¸Ðµ Ð¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð¸ÑÐ¿ÐµÑÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐµÐ¹ Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹.
K2 scopre 78 esopianeti in tempi record
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2018

Nei dati di due campagne osservative del satellite Kepler i ricercatori hanno trovato velocemente 30 candidati pianeta di alta qualità, 48 eventi più ambigui che possono essere pianeti o falsi positivi, 164 binari eclissanti e 231 altre fonti variabili. Lo studio pubblicato su The Astrophysical Journal
On The Origin of Lyman-alpha Absorption in Nearby Starbursts and Implications for Other Galaxies
Creators: name: Atek, Hakim
name: Schaerer, Daniel
name: Kunth, Daniel
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: (Abridged) Despite the privileged position that Lyman-alpha (Lya) emission line holds in the exploration of the distant universe and modern observational cosmology, the origin of the observed diversity of lya profiles remains to be thoroughly explained. Observations of nearby star forming galaxies bring their batch of apparent contradictions between Lya emission and their physical parameters, and call for a detailed understanding of the physical processes at work. IZw 18, one of the most metal-poor galaxies known is of particular interest in this context. We use a 3D Lya radiation transfer code to model Hubble Space Telescope (HST) observations of IZw 18 and to fit its Lya spectrum. Different geometrical configurations of the source and the neutral gas are explored. The integrated Lya profile of NW region of IZw 18 is reproduced using the observed small amount of dust (E(B-V) ~ 0.05) and a spherical HI shell with N(HI) = 6.5 x 10^(21) cm^(-2). Such a high column density makes it possible to transform a strong Lya emission (EW(Lya) = 60 A) into a damped absorption even with a small extinction. When a slab geometry is applied and a given line of sight is chosen, the Lya profile can be successfully reproduced with no dust at all and N(HI) = 3 x 10^(21) cm^(-2). The spatial variations of the profile shape are naturally explained by radiation transfer effects. In the case of outflowing Inter Stellar Medium (ISM), as commonly observed in Lyman Break Galaxies (LBGs), a high N(H) and dust content are required to observe Lya in absorption. For nearly static neutral gas as observed in IZw 18 and other low luminosity galaxies only a small amount of dust is required provided a sufficiently high N(H) covers the galaxy.
description: 11 pages, 10 figures. Accepted for publication in Astronomy and Astrophysics
Additional file 2 of Establishment of a prognostic signature for lung adenocarcinoma using cuproptosis-related lncRNAs
Creators: name: Yalimaimaiti, Saiyidan
name: Liang, Xiaoqiao
name: Zhao, Haili
name: Dou, Hong
name: Liu, Wei
name: Yang, Ying
name: Ning, Li
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Additional file 2. The result of univariate Cox regression analysis.
Advances in Glaucoma Treatment and Management: Gene Therapy
Creators: name: Borras, Terete
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2012

description: Glaucoma is characterized by the death of retinal ganglion cells (RGCs) and loss of vision. It is the second most frequent cause of irreversible blindness in the world and affects primarily the older population. Projections of prevalence show that by 2020 there will be an estimated 79.6 million people worldwide with glaucoma, with a higher proportion of women than men. Glaucoma can be treated but is not yet curable. Treatments currently available, such as the daily administration of eye drops, lead to high levels of noncompliance, especially in the aged population. In several laboratories, including ours, intense research is ongoing to search for alternative treatments of the disease. Using genes, we seek to develop gene drug therapies that can be many times more efficient than conventional drugs and allow less frequent administration—perhaps just once every 1 or 2 years. In cases of inherited glaucoma caused by either recessive or dominant genes, we seek gene replacement and gene knockdown strategies that could reverse the undesired outcome of the mutation. Technology for this new state-of-the-art treatment is currently available and has been successfully applied in other diseases, including conditions in the eye.
การพัฒนาแอปพลิเคชันคัดกรองกลุ่มเสี่ยงโรคเบาหวานและความดันโลหิตสูง
Creators: name: จุฬาวลี มณีเลิศ
Publisher: name: มหาวิทยาลัยราชภัฏเชียงใหม่
Year: 2021
Subjects: แอปพลิเคชันบนมือถือ
กลุ่มเสี่ยง
เบาหวาน
ความดันโลหิตสูง

description: วารสารวิจัยราชภัฏเชียงใหม่, 22, 3, 109-125
Additional file 4 of Establishment of a prognostic signature for lung adenocarcinoma using cuproptosis-related lncRNAs
Creators: name: Yalimaimaiti, Saiyidan
name: Liang, Xiaoqiao
name: Zhao, Haili
name: Dou, Hong
name: Liu, Wei
name: Yang, Ying
name: Ning, Li
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Additional file 4. The detail result of KEGG enrichment analysis.
การเสริมสร้างพลังอำนาจสตรีวัยทองในการเตรียมความพร้อมสู่สังคมผู้สูงอายุคุณภาพ
Creators: name: มุจลินท์ แปงศิริ
Publisher: name: มหาวิทยาลัยราชภัฏเชียงใหม่
Year: 2021
Subjects: สตรีวัยทอง
การตรียมตัว
สังคมสูงอายุ
การเสริมสร้างพลังอำนาจ

description: วารสารวิจัยราชภัฏเชียงใหม่, 22, 3, 126-140
Enhancement of quark number susceptibility with an alternative pattern of chiral symmetry breaking in dense matter
Creators: name: Harada, M.
name: Sasaki, C.
name: Takemoto, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We explore a possible phase where chiral $SU(2)_L \times SU(2)_R$ symmetry is spontaneously broken while its center $Z_2$ symmetry remains unbroken and its consequence on thermal quantities. In this phase, chiral symmetry breaking is driven by a quartic quark condensate although a bilinear quark condensate vanishes. A Ginzburg-Landau free energy leads to a new tricritical point (TCP) between the $Z_2$ broken and unbroken phases. Furthermore, a critical point can appear even in the chiral limit where explicit breaking is turned off, instead of a TCP at which restoration of chiral and its center symmetries takes place simultaneously. The net quark number density exhibits an abrupt change near the restoration of the center symmetry rather than that of the chiral symmetry. Hadron masses in possible phases are also studied in a linear sigma model. We show that, in the $Z_2$ symmetric phase, the $\bar{q}q$-type scalar meson with zero isospin I=0 splits from the $\bar{q}q$-type pseudoscalar meson with I=1.
description: 11 pages, 5 figures, 3 tables
La pioggia fredda che ingrassa il buco nero
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2018

Alcune rare e antiche galassie, piccole ma molto massicce, sono rimaste isolate per miliardi di anni. Questo provoca che il buco nero centrale cresca a dismisura a scapito della formazione stellare, come ha rivelato un nuovo studio, a cui ha partecipato l’italiano Massimo Gaspari dell’Università di Princeton