cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐ°ÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸
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description: ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ¼Ñ Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½Ð° ÑÑÑÐµÐ¼Ð»ÐµÐ½Ð¸ÐµÐ¼ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ðº ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¸ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÑÐ½ÐºÐµ, Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð» Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐµÐ¼ ÑÐµÑÑÑÑÐ¾Ð¼, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÐµÑ ÑÑÐ¾. ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÐÐÐ Â«ÐÐ¡ÐÐÂ». Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð´Ð»Ñ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ°Ð±Ð¾ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² ÑÐµÐºÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° ÐÐÐ Â«ÐÐ¡ÐÐÂ». Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ°ÑÐ¾Ð¹ Ð¸ Ð½Ð¾Ð²Ð¾Ð¹ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð´Ð»Ñ ÐÐÐ Â«ÐÐ¡ÐÐÂ». ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
An experimental investigation of some factors influencing the rate of leaching of the Britiannia ore.
Creators: name: Hansuld, John Alexander
Publisher: name: University of British Columbia
Year: 2012

description: Experimental investigations are carried out to establish a satisfactory technique and to study some factors -- variations in the chemical character of the attacking solutions, rate of flow, and the effect of pyrite -- influencing the rate of leaching of the Britannia copper ore. The natural leaching phenomenon at the Britannia Mine is described and brief geological descriptions are listed of other mines from which copper recovery is made from the mine water. The general chemical and physical principles involved in the leaching of copper sulphide ores are reviewed. Samples taken from the Britannia Mine are crushed, sorted according to size, oven heated to destroy any bacteria, packed in glass tubes, and leached with different chemical solutions at various rates of flow. The chemical character of the attacking solutions is the key factor in determining the rate of leaching. Ferric sulphate and sulphuric acid increase the rate of leaching up to 600 times and 33 times that of pure water respectively. Changes in the rate of flow are of secondary importance and determine the range of fluctuations in the rate of leaching around an order of magnitude dependent on the chemical character of the attacking solutions. The ore with the smaller chalcopyrite to pyrite ratio is more readily attacked than the one with the greater ratio. Leaching of copper ores in place may be increased by attacking them with solutions of sulphuric acid and/or ferric sulphate. This may be accomplished by the recirculating of the conditioned mine waters after the extraction of the copper.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð² Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½ÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸ÑÑ
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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: Ð±ÑÑÐ¾Ð²Ð¾Ðµ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ðµ
Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ
Ð»Ð¸ÑÐµÐ½Ð·Ð¸ÑÐ¾Ð²Ð½Ð¸Ðµ
ÑÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ
ÑÑÐ»ÑÐ³Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ðµ ÑÐµÐ»Ð¸ Ð¿ÑÐµÐ´ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð² Ð¿Ð¾Ð½ÑÑÐ¸Ñ Â«Ð±ÑÑÐ¾Ð²Ð¾Ðµ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸ÐµÂ», Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð¼ÐµÑÐ½Ð¾ÑÑÐµÐ¹ ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð±Ð°Ð·Ñ, Ð½Ð° ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð´Ð°Ð½Ð½Ð°Ñ ÑÑÐµÑÐ° ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐµÐ»ÑÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð´Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°ÑÐ¿ÐµÐºÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð¢ÑÐ°Ð¿ÑÐ¸Ð½ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ, ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð±ÑÐ´ÐµÑ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²Ð¾Ð²Ð°ÑÑ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð±ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÐµÑÐµÑÐ½Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð±ÑÑÐ¾Ð²ÑÑ ÑÑÐ»ÑÐ³, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¼Ð¾Ð¶ÐµÑ Ð¾ÑÐ²Ð°ÑÐ¸ÑÑ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ðµ, Ð¿ÑÐ¾Ð¶Ð¸Ð²Ð°ÑÑÐµÐµ Ð² ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð¼ÐµÑÑÐ½Ð¾ÑÑÐ¸. Ð£ÑÐ¸ÑÑÐ²Ð°Ñ ÑÐ¾Ñ ÑÐ°ÐºÑ, ÑÑÐ¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð±ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ â ÑÑÐµÑÐ° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð¾Ð»Ð¾Ð´ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸Ð½Ð¸Ð¼Ð°ÑÐµÐ»ÐµÐ¹ Ð±ÑÐ» Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¸Ð½ÐºÑÐ±Ð°ÑÐ¾ÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð±ÑÐ´ÐµÑ ÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¼Ð°Ð»ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¸ Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð² ÑÑÐµÑÐµ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±ÑÑÐ¾Ð²ÑÑ ÑÑÐ»ÑÐ³.
RHIC data and small x physics
Creators: name: Lappi, T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: This is a short review of some RHIC results that have been most important for the small x physics community. We discuss saturation effects in deuteron-gold collisions, particle production in gold-gold collisions and some effects of the large "glasma" field configurations in the early stages of the collision.
description: 6 pages, 7 figures, uses espcrc2.sty. Talk at the International Symposium on Very High Energy Cosmic Ray Interactions, Paris, France, September 2008
Cost-effectiveness of toripalimab plus chemotherapy versus chemotherapy as first-line treatment for advanced non-small cell lung cancer in China: a societal perspective
Creators: name: Lian, Dai
name: Yang, Yi
name: Gan, Yuling
name: Xiao, Dunming
name: Xiang, Yuliang
name: Jiang, Shan
name: Gu, Yuanyuan
name: Chen, Yingyao
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: To investigate the cost-effectiveness of toripalimab plus chemotherapy versus chemotherapy alone for advanced non-small cell lung cancer (NSCLC) patients from a societal perspective. A partitioned-survival model estimated the costs and cost-effectiveness of toripalimab plus chemotherapy versus standard chemotherapy for advanced NSCLC over 20 years. Clinical data were derived from the CHOICE-01 trial, and cost and utility inputs were gathered from Yaozh.com, expert interviews, and a nationwide hospital-based survey. Costs were reported in 2022 US dollars, and outcomes included quality-adjusted life-years (QALYs) and incremental cost-effectiveness ratios (ICERs), with a 5% discount rate was applied. Sensitivity, subgroup, and scenario analyses verified the robustness of results. Toripalimab plus chemotherapy resulted in 3.048 QALYs and a total cost of $60,813, with an ICER of $19,066 per QALY gained, below China’s 3 times GDP per capita threshold ($38,223). Robustness is confirmed through sensitivity, subgroup and scenario analyses. Toripalimab plus chemotherapy is a cost-effective option for treatment-naive advanced NSCLC compared to chemotherapy alone, providing valuable evidence for clinical and reimbursement decision-making.
La nova che non ti aspetti
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

Le osservazioni in banda radio condotte con vari radiotelescopi hanno permesso a un team internazionale di ricercatori di individuare i meccanismi alla base della inattesa produzione di raggi gamma associati alla nova V 959 Mon e identificati nel 2012 dal satellite Fermi. Il commento di Luigina Feretti (INAF)
title: ÐÐ¸Ð´ÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ ÑÑÐ¾Ð»Ð° ÑÑÐ°Ð½ÐºÐ° Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼
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Ð¾ÑÐ¸ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
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¿ÑÐ¸Ð²Ð¾Ð´
Ð·Ð¾Ð»Ð¾ÑÐ½Ð¸Ðº
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Ð³Ð¸Ð´ÑÐ¾ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»Ñ
"ÑÐ¾Ð¿Ð»Ð¾-Ð·Ð°ÑÐ»Ð¾Ð½ÐºÐ°"

description: Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° â Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÑÐ¾Ð»Ð° ÑÑÐ°Ð½ÐºÐ° Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼.
Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ Ð³Ð¸Ð´ÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¸ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸Ð´ÐµÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð¾Ð»Ð¾ÑÐ½Ð¸ÐºÐ° Ð¸ Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ ÐºÐ°ÑÐºÐ°Ð´Ð° ÑÑÐ¸Ð»ÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð³Ð¸Ð´ÑÐ¾ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¿Ð¾Ð´Ð±Ð¾Ñ Ð³Ð¸Ð´ÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð³Ð»Ð°ÑÐ½Ð¾ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ¼Ðµ.
Empirical H-alpha emitter count predictions for dark energy surveys
Creators: name: Geach, J. E.
name: Cimatti, A.
name: Percival, W.
name: Wang, Y.
name: Guzzo, L.
name: Zamorani, G.
name: Rosati, P.
name: Pozzetti, L.
name: Orsi, A.
name: Baugh, C. M.
name: Lacey, C. G.
name: Garilli, B.
name: Franzetti, P.
name: Walsh, J. R.
name: Kümmel, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Future galaxy redshift surveys aim to measure cosmological quantities from the galaxy power spectrum. A prime example is the detection of baryonic acoustic oscillations (BAOs), providing a standard ruler to measure the dark energy equation of state, w(z), to high precision. The strongest practical limitation for these experiments is how quickly accurate redshifts can be measured for sufficient galaxies to map the large-scale structure. A promising strategy is to target emission-line (i.e. star-forming) galaxies at high-redshift (z~0.5-2); not only is the space density of this population increasing out to z~2, but also emission-lines provide an efficient method of redshift determination. Motivated by the prospect of future dark energy surveys targeting H-alpha emitters at near-infrared wavelengths (i.e. z>0.5), we use the latest empirical data to model the evolution of the H-alpha luminosity function out to z~2, and thus provide predictions for the abundance of H-alpha emitters for practical limiting fluxes. We caution that the estimates presented in this work must be tempered by an efficiency factor, epsilon, giving the redshift success rate from these potential targets. For a range of practical efficiencies and limiting fluxes, we provide an estimate of nP_{0.2}, where n is the 3D galaxy number density and P_{0.2} is the galaxy power spectrum evaluated at k=0.2h/Mpc. Ideal surveys must provide nP_{0.2}>1 in order to balance shot-noise and cosmic variance errors. We show that a realistic emission-line survey (epsilon=0.5) could achieve nP_{0.2}=1 out to z~1.5 with a limiting flux of 10^{-16} erg/s/cm^{-2}. If the limiting flux is a factor 5 brighter, then this goal can only be achieved out to z~0.5, highlighting the importance of survey depth and efficiency in cosmological redshift surveys.
description: 9 pages, 5 figures, 2 tables. Accepted for publication in MNRAS
title: Ð¢ÑÐ¸Ð±Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¼Ð¸Ð½Ñ, Ð¿Ð¾Ð»ÐµÐ·Ð½ÑÐµ ÑÐ»Ð¾Ð²Ð°, Ð²ÑÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ°Ñ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐ°
Creators: name: ÐÐ¾Ð¹Ð½Ð¾Ð², Ð.
Publisher: name: ÐÑÐ´ÑÑÐµÐµ
Year: 2005
Subjects: Ð¢ÑÐ¸Ð±Ð¾Ð½Ð¸ÐºÐ°
Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº

description: ÐÑÐ¾ÑÑÑÐ° Ð½Ð° Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐµ, ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¼Ð½Ð¾Ð³Ð¾ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÐµ ÑÐµÑÐ¼Ð¸Ð½Ñ, ÑÐ»Ð¾Ð²Ð° Ð¸ Ð²ÑÑÐ°Ð¶ÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾ ÑÐ°ÑÑÐ¾ Ð²ÑÑÑÐµÑÐ°ÑÑÑÑ Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐµÐ¹ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÑÑÐ¸Ð±Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ. ÐÐ½Ð¾Ð³Ð¸Ðµ Ð¸Ð· Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ð¼ÑÑ ÑÐ»Ð¾Ð² Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð°Ð²ÑÐ¾ÑÐ°Ð¼Ð¸ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð² Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸ÑÑ Ð¸ ÑÐµÐ¼Ð¸Ð½Ð°ÑÐ°Ñ. Ð Ð·Ð°ÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð±ÑÐ¾ÑÑÑÑ Ð´Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð²ÑÐµÐ¼ÐµÐ½Ð° Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð±ÑÐ¾ÑÑÑÑ Ð±ÑÐ´ÐµÑ Ð¿Ð¾Ð»ÐµÐ·ÐµÐ½ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 071200, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÑÐµÐ½Ð¸Ñ, ÑÐ¼Ð°Ð·ÐºÐ¸, Ð¸Ð·Ð½Ð°ÑÐ¸Ð²Ð°Ð½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼, Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼ Ð¸ Ð»Ð¸ÑÐ°Ð¼, Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸Ð¼ÑÑ ÑÐµÑÑÑÐ·Ð½ÑÐ¼ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ²Ð¾ÐµÐ³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð·Ð½Ð°Ð½Ð¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°. ÐÐ²ÑÐ¾Ñ Ð²ÑÑÐ°Ð¶Ð°ÐµÑ Ð¸ÑÐºÑÐµÐ½Ð½ÑÑ Ð±Ð»Ð°Ð³Ð¾Ð´Ð°ÑÐ½Ð¾ÑÑÑ ÑÐµÑÐµÐ½Ð·ÐµÐ½ÑÑ, ÑÑÐ¸ÑÐµÐ»Ñ Ð²ÑÑÑÐµÐ¹ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÑ Ð¿Ð¾ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° ÐÐ¾ÐºÑÑÐ°ÐµÐ²Ð¾Ð¹ ÐÐ¾Ðµ ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ¾Ð²Ð½Ðµ Ð·Ð° Ð¾ÐºÐ°Ð·Ð°Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÐ»ÑÑÐ°ÑÐ¸Ð¸ Ð¸ Ð²Ð½Ð¸Ð¼Ð°ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ ÑÑÐºÐ¾Ð¿Ð¸ÑÐ¸ Ð½Ð° ÑÑÐ°Ð¿Ðµ ÐµÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
Come dieci milioni di Soli
Creators: Silvia Casu
Publisher: name: Media Inaf
Year: 2014

Uno studio su Nature, guidato dal giovane Matteo Bachetti, ora in forza all'INAF-Osservatorio Astronomico di Cagliari, illustra, grazie ai dati del telescopio Nustar, la pulsar più luminosa mai registrata
On reconstruction of inclusions in a heat conductive body from dynamical boundary data over a finite time interval
Creators: name: Ikehata, Masaru
name: Kawashita, Mishio
Publisher: name: arXiv
Year: 2010
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 35R30, 80A23

description: The enclosure method was originally introduced for inverse problems of concerning non-destructive evaluation governed by elliptic equations. It was developed as one of useful approaches in inverse problems and applied for various equations. In this paper, an application of the enclosure method to an inverse initial boundary value problem for a parabolic equation with a discontinuous coefficient is given. A simple method to extract the depth of unknown inclusions in a heat conductive body from a single set of the temperature and heat flux on the boundary observed over a finite time interval is introduced. Other related results with infinitely many data are also reported. One of them gives the minimum radius of the open ball centered at a given point that contains the inclusions. The formula for the minimum radius is newly discovered.
description: 18pages. This is the final version
title: ÐÐ±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾-Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¿ÐµÑÐµÐ´Ð¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð¼Ð¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ
ERP-ÑÐ¸ÑÑÐµÐ¼Ð°
Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ
ERP-system
control
management

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ERP-ÑÐ¸ÑÑÐµÐ¼ Ð½Ð° ÑÑÐ°Ð¿Ðµ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ñ Ð¡ÐÐ  ÑÐ°Ð±Ð¾Ñ ÐºÐ°Ðº ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ð¼Ð¸ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ°Ñ. ÐÐ¾ÑÐ»Ðµ ÑÑÐ¿ÐµÑÐ½Ð¾Ð³Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ERP-ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾-Ð´ÐµÐ»Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ½ÑÑÐ°, ÑÐ¸ÑÐºÐ¸ Ð½ÐµÑÐ²Ð¾ÐµÐ²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð²ÐµÑÑÐµÐ½Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð½Ðµ ÑÐ´Ð°ÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ° Ñ ÑÑÐµÐ±ÑÐµÐ¼ÑÐ¼ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð¸ Ñ Ð¿ÑÐµÐ²ÑÑÐµÐ½Ð¸ÐµÐ¼ ÑÐ¼ÐµÑÐ½Ð¾Ð¹ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÑÐ½Ð¸Ð·Ð¸Ð»Ð¸ÑÑ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐµÐ³Ð¾ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐ´ÐµÐ»Ð°ÑÑ Ð²ÑÐ²Ð¾Ð´ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ ERP-ÑÐ¸ÑÑÐµÐ¼Ð° Ð´Ð°ÑÑ Ð·Ð°ÐºÐ°Ð·ÑÐ¸ÐºÑ Ð¾Ð±ÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾Ñ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐµ, Ð¸Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐµ Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ðµ ÐºÐ¾Ð½ÐµÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ°. Ð­ÑÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ñ ÑÑÑÐ¾Ð¹ÐºÐ¸ Ð¿ÑÐ¸Ð½Ð¸Ð¼Ð°ÑÑ Ð³ÑÐ°Ð¼Ð¾ÑÐ½ÑÐµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð½Ð° Ð¾Ð±ÑÐµÐºÑÐµ.
A caccia di raggi cosmici con lo smartphone
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Un telefono cellulare di ultima generazione, una striscia di nastro adesivo, ed è fatta: arriva rilevatore di raggi cosmici prêt-à-porter, progettato dai ricercatori del Wisconsin IceCube Particle Astrophysics Center e disponibile per dispositivi Android
title: Evaluating the Impact of Socioeconomic Factors on Timing and Quality of Autism Diagnosis in Maryland
Creators: name: Alagarsamy, Darsana
name: Adefisan, Olutobi
name: Bowman, Raquel
name: Esteves, Amanda
name: O’Hara, Nell
name: Serrano, Abigail
name: Valenzuela, Melannie
name: Yonas, Kalkidan
Publisher: name: Digital Repository at the University of Maryland
Year: 2025
Subjects: subject: Special Education
subject: Gemstone Honors College
subject: EDU
subject: Autism Diagnosis
subject: Socioeconomic Factors
subject: Parent Reports

description: Previous research has established that early diagnosis and intervention for Autism Spectrum Disorder (ASD) significantly improve the effectiveness of interventions. However, obtaining a diagnosis can be challenging for some families. This study aims to explore whether socioeconomic status (SES) and related factors contribute to delays in receiving an ASD diagnosis, and if so, how. A mixed-methods approach is used, combining surveys and interviews with a subset of participants. The goal is to provide a comprehensive understanding of the obstacles parents and caregivers in Maryland face when seeking an ASD diagnosis for their child. The study begins with an initial survey and interviewees are randomly selected from participants who express interest in further involvement. As the survey is currently ongoing, preliminary results are not yet available. If specific obstacles are identified, future research can validate these findings and help inform strategies to reduce barriers, making the diagnostic process more accessible for families.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐ´Ð¾ÑÑÑÐ¿Ð½Ð¾Ð¹ ÑÑÐ¾Ð»Ð¾Ð²Ð¾Ð¹ Ð½Ð° 75 Ð¼ÐµÑÑ Ð² ÐÑÐ±Ð¾ÑÐ³ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ - ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»Ð¾Ð²-ÐÐµÐ¾Ð½ÑÑÐµÐ², 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: Ð¾Ð±ÑÐµÐ´Ð¾ÑÑÑÐ¿Ð½Ð°Ñ ÑÑÐ¾Ð»Ð¾Ð²Ð°Ñ
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ
Ð¼ÐµÐ½Ñ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐµÐ´Ð¾ÑÑÑÐ¿Ð½Ð¾Ð¹ ÑÑÐ¾Ð»Ð¾Ð²Ð¾Ð¹, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Deterministic Ultracold Ion Source targeting the Heisenberg Limit
Creators: name: Schnitzler, W.
name: Linke, N. M.
name: Fickler, R.
name: Meijer, J.
name: Schmidt-Kaler, F.
name: Singer, K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The major challenges to fabricate quantum processors and future nano solid state devices are material modification techniques with nanometre resolution and suppression of statistical fluctuations of dopants or qubit carriers. Based on a segmented ion trap with mK laser cooled ions we have realized a deterministic single ion source which could operate with a huge range of sympathetically cooled ion species, isotopes or ionic molecules. We have deterministically extracted a predetermined number of ions on demand and have measured a longitudinal velocity uncertainty of 6.3m/s and a spatial beam divergence of 0.6 mrad. We show in numerical simulations that if the ions are cooled to the motional ground state (Heisenberg limit) nanometre spatial resolution can be achieved.
description: 4 pages 4 figures. to be published in prl
title: Query sampling method for estimating local cost parameters in a multidatabase system
Creators: name: Zhu, Q
name: Larson, PA
Publisher: name: Institute of Electrical and Electronics Engineers (IEEE)
Year: 1994
Subjects: subject: 4605 Data Management and Data Science
subject: 46 Information and Computing Sciences
subject: 4609 Information Systems

description: In a multidatabase system (MDBS), some query optimization information related to local database systems may not be available at the global level because of local autonomy. To perform global query optimization, a method is required to derive the necessary local information. This paper presents a new method that employs a query sampling technique to estimate the cost parameters of an autonomous local database system. We introduce a classification for grouping local queries and suggest a cost estimation formula for the queries in each class. We present a procedure to draw a sample of queries from each class and use the observed costs of sample queries to determine the cost parameters by multiple regression. Experimental results indicate that the method is quite promising for estimating the cost of local queries in an MDBS.
title: Ð Ð°ÑÑÐµÑ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°Ð½ÐºÐ¾Ð². Ð¨Ð¿Ð¸Ð½Ð´ÐµÐ»ÑÐ½ÑÐµ ÑÐ·Ð»Ñ Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ½Ð´ÑÑ, ÐÐ¸ÑÐ°Ð¸Ð»
name: Ð¨Ð¼Ð°ÐºÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: ÐÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ðµ ÑÑÐ°Ð½ÐºÐ¸
Ð¨Ð¿Ð¸Ð½Ð´ÐµÐ»Ð¸

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¼Ñ ÑÑÐµÐ±Ð½Ð¾Ð¼Ñ Ð¿Ð»Ð°Ð½Ñ ÐÐÐ¤, Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð Ð°ÑÑÐµÑ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°Ð½ÐºÐ¾Ð²Â» ÑÐ¸ÐºÐ»Ð° ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½, ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÐµÐ¼ÑÑ Ð¡Ð¾Ð²ÐµÑÐ¾Ð¼ Ð²ÑÐ·Ð° (ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°), Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«ÐÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ðµ ÑÑÐ°Ð½ÐºÐ¸Â». Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ Ð¿Ð¾ ÑÐ¸Ð¿Ð¾Ð²ÑÐ¼ ÑÑÐµÐ¼Ð°Ð¼ ÑÐ¿Ð¸Ð½Ð´ÐµÐ»ÑÐ½ÑÑ ÑÐ·Ð»Ð¾Ð² Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ¾Ð² Ñ Ð¾Ð¿Ð¾ÑÐ°Ð¼Ð¸ ÐºÐ°ÑÐµÐ½Ð¸Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¸ Ð¸Ð¼Ð¿Ð¾ÑÑÐ½ÑÑ Ð¿Ð¾Ð´ÑÐ¸Ð¿Ð½Ð¸ÐºÐ¾Ð² ÐºÐ°ÑÐµÐ½Ð¸Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð² ÑÐ¿Ð¸Ð½Ð´ÐµÐ»ÑÐ½ÑÑ ÑÐ·Ð»Ð°Ñ, Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸Ñ Ð¼Ð¾Ð½ÑÐ°Ð¶Ð° Ð¸ ÑÐ¼Ð°Ð·ÑÐ²Ð°Ð½Ð¸Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°ÑÑÐµÑÐ° ÑÐ¿Ð¸Ð½Ð´ÐµÐ»ÑÐ½ÑÑ ÑÐ·Ð»Ð¾Ð² Ð½Ð° Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ Ð¸ Ð¶ÐµÑÑÐºÐ¾ÑÑÑ. ÐÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐ¿Ð¸Ð½Ð´ÐµÐ»ÑÐ½ÑÑ ÑÐ·Ð»Ð¾Ð² Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ¾Ð². Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¸Ð¼ÐµÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÐ¿Ð¸Ð½Ð´ÐµÐ»ÑÐ½ÑÑ ÑÐ·Ð»Ð¾Ð² Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ¾Ð², ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð² ÑÑÐ°Ð½ÐºÐ°Ñ Ð²ÐµÐ´ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¸ÑÐ¼ ÐÐµÑÐ¼Ð°Ð½Ð¸Ð¸, Ð¯Ð¿Ð¾Ð½Ð¸Ð¸, Ð¨Ð²ÐµÑÐ¸Ð¸, ÐÑÐ°Ð»Ð¸Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹ Ð¸ Ð²ÐµÑÐµÑÐ½ÐµÐ¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 151002 Â«ÐÐµÑÐ°Ð»Ð»Ð¾Ð¾Ð±ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑÐ¸Ðµ ÑÑÐ°Ð½ÐºÐ¸ Ð¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÂ» Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ, ÐºÑÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÐÐÐ  Ð¸ ÐÐÐÐÐ , ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
National Astronomical Observatory of Japan
Creators: name: Iye, Masanori
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: National Astronomical Observatory is an inter-university institute serving as the national center for ground based astronomy offering observational facilities covering the optical, infrared, radio wavelength domain. NAOJ also has solar physics and geo-lunar science groups collaborating with JAXA for space missions and a theoretical group with computer simulation facilities. The outline of NAOJ, its various unique facilities, and some highlights of recent science achievements are reviewed.
description: Invited paper to introduce the activities at NAOJ
The non-symmetric operad pre-Lie is free
Creators: name: Bergeron, Nantel
name: Livernet, Muriel
Publisher: name: arXiv
Year: 2008
Subjects: subject: Rings and Algebras (math.RA)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 18D, 05E, 17B

description: We prove that the pre-Lie operad is a free non-symmetric operad.
description: 12 pages. Details on the trees used added in definition 1.2. The proof of corollary 3.6 has been changed
Effect of packing geometry on heat and mass transfer in stacked beds of spheres
Creators: name: Komarnicky, Walter
Publisher: name: University of British Columbia
Year: 2012

description: Experimental measurements have been made of the simultaneous rates of mass and heat transfer for the surface evaporation of water into air from a simple cubic, a rhombohedral, and two orthorhombic assemblages of uniform celite spheres, in the particle Reynolds number range 300-1200. The measurements were confined to the pre-determined constant rate drying period of the spheres. No appreciable differences in mass and heat transfer factors were found for the various assemblages, except for the cubic, which exhibited lower transfer factors at the higher Reynolds numbers. This is explained qualitatively by the fact that the cubic configuration shows a considerably larger free projected cross-sectional area than the others, thus allowing for greater fluid channelling. Various methods proposed by investigators of randomly packed beds for correlating mass transfer by the inclusion of fractional void volume functions in the mass transfer factor and/or the Reynolds number were tested for the stacked assemblages. None of these methods completely correlated the results. Galloway's fluid friction data for the two orthorhombic assemblages were recalculated and showed similar friction factors to those obtained by Martin for identical packings of brass spheres. Ergun's criteria for complete and for no longitudinal fluid mixing were applied to the various assemblages. The results for the cubic assemblage suggest the possibility of considerable air mixing therein.
NASA: finisce in tribunale il dopo Soyuz
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Boeing e SpaceX hanno appena ricevuto un finanziamento miliardario per mandare avanti i lavori sulla nuova astronave taxi per raggiungere l’orbita terrestre bassa, ma è tutto da rifare: la Sierra Nevada Corporation non accetta l'esclusione dalla Commercial Crew Transportation Capability e trascina  in tribunale l'agenzia spaziale statunitense
The Local Hosts of Type Ia Supernovae
Creators: name: Neill, James D.
name: Sullivan, Mark
name: Howell, D. Andy
name: Conley, Alex
name: Seibert, Mark
name: Martin, D. Christopher
name: Barlow, Tom A.
name: Foster, Karl
name: Friedman, Peter G.
name: Morrissey, Patrick
name: Neff, Susan G.
name: Schiminovich, David
name: Wyder, Ted K.
name: Bianchi, Luciana
name: Donas, José
name: Heckman, Timothy M.
name: Lee, Young-Wook
name: Madore, Barry F.
name: Milliard, Bruno
name: Rich, R. Michael
name: Szalay, Alex S.
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 use multi-wavelength, matched aperture, integrated photometry from GALEX, SDSS and the RC3 to estimate the physical properties of 166 nearby galaxies hosting 168 well-observed Type Ia supernovae (SNe Ia). Our data corroborate well-known features that have been seen in other SN Ia samples. Specifically, hosts with active star formation produce brighter and slower SNe Ia on average, and hosts with luminosity-weighted ages older than 1 Gyr produce on average more faint, fast and fewer bright, slow SNe Ia than younger hosts. New results include that in our sample, the faintest and fastest SNe Ia occur only in galaxies exceeding a stellar mass threshhold of ~10^10 M_sun, indicating that their progenitors must arise in populations that are older and/or more metal rich than the general SN Ia population. A low host extinction sub-sample hints at a residual trend in peak luminosity with host age, after correcting for light-curve shape, giving the appearance that older hosts produce less-extincted SNe Ia on average. This has implications for cosmological fitting of SNe Ia and suggests that host age could be useful as a parameter in the fitting. Converting host mass to metallicity and computing 56Ni mass from the supernova light curves, we find that our local sample is consistent with a model that predicts a shallow trend between stellar metallicity and the 56Ni mass that powers the explosion, but we cannot rule out the absence of a trend. We measure a correlation between 56Ni mass and host age in the local universe that is shallower and not as significant as that seen at higher redshifts. The details of the age -- 56Ni mass correlations at low and higher redshift imply a luminosity-weighted age threshhold of ~3 Gyr for SN Ia hosts, above which they are less likely to produce SNe Ia with 56Ni masses above ~0.5 M_sun. (Abridged)
description: 21 pages, 15 figures, accepted for ApJ
A retrospective observational analysis of the real-world care pathway of people with hereditary transthyretin amyloidosis with polyneuropathy in Italy
Creators: name: Calabria, Silvia
name: Ronconi, Giulia
name: Dondi, Letizia
name: Dondi, Leonardo
name: Dell’anno, Irene
name: Piccinni, Carlo
name: Esposito, Immacolata
name: Addesi, Alice
name: Gnesi, Marco
name: Cosentino, Nicola
name: D’Amelio, Marco
name: Martini, Nello
name: Maggioni, Aldo Pietro
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: This retrospective observational study described the epidemiology and the burden on the Italian healthcare service (SSN) of patients with polyneuropathy (PN) associated to the hereditary transthyretin amyloidosis (ATTRv). From the Fondazione ReS (Ricerca e Salute) administrative healthcare database (~5.5 million inhabitants in 2021), patients were identified as having ATTRv-PN in 2021 if they had received treatments for ATTRv-PN under SSN reimbursement (i.e. tafamidis, patisiran or inotersen) from 1 January 2014 to 12/31/2021 (index date in 2021). Demographics and comorbidities at baseline, healthcare resource consumptions and related direct costs reimbursed by the SSN throughout one-year follow-up were described. In 2021, 36 patients with ATTRv-PN (prevalence: 7.4/1,000,000) were identified (males were 83.3%; patients with ≥ 2 comorbidities were 61.1%; mean age was 73 ± 8 years). During follow-up, of patients: 91.7% received drugs for ATTRv-PN; >50% received antiepileptics and acid suppressants; 22.2% were admitted to overnight hospitalizations; 30.6% accessed the emergency department; 97.2% received local outpatient specialist care. The per patient mean annual cost was € 122,017; drugs for ATTRv-PN accounted for 94.7% of the total expenditure. This study of real-world patients with ATTRv-PN showed a high rate of comorbidities, and substantial direct healthcare and economic burdens on the SSN.
Quel neutrino che gioca a nascondino
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2014

Gli scienziati che studiano le sottili trasformazioni dei neutrini  hanno pubblicato i primi risultati di un nuovo studio sulla ricerca del cosiddetto “neutrino sterile” un ipotetico nuovo tipo di neutrino che si andrebbe ad aggiungere ai tre tipi, o “sapori” ad oggi conosciuti. L’esistenza di queste particelle così sfuggenti, se provata, avrebbe un profondo impatto sulla nostra comprensione dell’universo e influirebbe in modo determinante nell’ideazione dei futuri esperimenti sui neutrini
Cost effectiveness of obstructive sleep apnea therapies: a systematic review and meta-analysis of cost utility studies
Creators: name: Kumar, S. Sajith
name: Lakshmi, G. Suchitra
name: Sohail, Aamir
name: Jagadeesh, Kayala Venkata
name: Bagepally, Bhavani Shankara
Publisher: name: Taylor & Francis
Year: 2025
Subjects: Medicine
Pharmacology
Science Policy

description: Obstructive sleep apnea (OSA) is a sleep-related breathing disorder characterized by recurrent episodes of nocturnal breathing cessation resulting from upper airway collapse. Given the absence of a comprehensive review of the cost-effectiveness of OSA treatments, we undertook an extensive systematic review and meta-analysis to calculate the pooled incremental net benefit (INBp). A systematic search of PubMed, Embase, Scopus, and Tufts cost-effectiveness analysis registry was conducted. INBp with 95% confidence intervals (CI) was estimated using a random-effects model, and heterogeneity was assessed through the Cochrane-Q test and I2 statistic. Study quality was evaluated using the modified ECOBIAS Checklist, and GRADE framework was applied to assess the certainty of outcomes. Thirty-four studies were included in the systematic review, fifteen qualifying for meta-analysis. CPAP was cost-effective compared to other treatments, with a INBp of $13,024 (95%CI $6,813 to $19,236), and substantial heterogeneity (I2 = 97.48%). Compared to no treatment and oral appliances (OAs), CPAP showed cost-effective INB values of $30,834 ($21,325 to $40,343) and $2,708 ($645 to $4,771) respectively. CPAP is cost effective compared to all treatments collectively, as well as specifically to OAs and no treatment though with low certainty.
title: ÐÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, ÐÐ»Ð¸Ð·Ð°Ð²ÐµÑ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: ÑÑÐ´ÐµÐ±Ð½Ð°Ñ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð°
ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð°
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description: ÐÐ°Ð½Ð½Ð°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÑÐµÐ½Ð¸Ñ Ð¾ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ, Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ, ÐµÑ Ð²Ð¸Ð´Ð°Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ°Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐ°Ð·ÑÐµÑÐµÐ½Ð¸Ñ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ, ÑÐ°Ðº ÐºÐ°Ðº ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¼ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð¼ Ð¿ÑÐ¾ÑÐµÐºÑÐ¸Ð¸ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ Ð¸ Ð¿ÑÐµÐ´ÑÐ¿ÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½Ð¸Ñ Ð½Ð¾Ð²ÑÑ Ð¿ÑÐ°Ð²Ð¾Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹ Ð² ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÐºÐ°Ðº Ð½Ð° Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÑÐ¾Ð²Ð½Ðµ, ÑÐ°Ðº Ð¸ Ð² Ð½Ð°ÑÑÐ½Ð¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸. ÐÐ¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð² ÑÐ°Ð±Ð¾ÑÐµ.
Il paso doble delle correnti di Birkeland
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2014

Grazie ai satelliti Iridium, un gruppo di scienziati ha studiato le correnti elettriche generate dall’interazione tra vento solare e campo magnetico, alla base delle aurore polari, scoprendo che si formano in due fasi. Un fatto che può essere utile per limitare i danni di una tempesta geomagnetica
Discovery of an old photoevaporating disk in sigma Orionis
Creators: name: Rigliaco, E.
name: Natta, A.
name: Randich, S.
name: Sacco, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The photoevaporation of circumstellar disks is a powerful process in the disk dissipation at the origin of the Orion proplyds. This Letter reports the first detection of a photoevaporating disk in the final but long-lasting phase of its evolution. The disk is associated to a low-mass T Tauri member of the sigma Orionis Cluster. It is characterized by a very low (if any) accretion rate and by a tenuous (Mloss ~ 10^{-9} Msun/yr) photoevaporation wind, which is unambiguously detected in the optical spectrum of the object. The wind emits strong forbidden lines of [SII] and [NII] because the low-mass star is close to a powerful source of ionizing photons, the O9.5 star sigma Ori.
description: Accepted by A&A; 4 pages, 2 figures
title: Ð ÐµÐºÐ»Ð°Ð¼Ð° Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐ¼ Ð¸Ð¼Ð¸Ð´Ð¶ÐµÐ¼ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð¤ÑÐµÐ³Ð°ÑÂ»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¸Ð¿Ð¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐ¹ Ð¸Ð¼Ð¸Ð´Ð¶
Ð¸Ð¼Ð¸Ð´Ð¶ÐµÐ²Ð°Ñ ÑÐµÐºÐ»Ð°Ð¼Ð°
ÑÐ¸ÑÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¸Ð»Ñ
ÑÑÐµÐ´ÑÑÐ²Ð° ÑÐµÐºÐ»Ð°Ð¼Ñ

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð»Ð¸ ÑÐµÐºÐ»Ð°Ð¼Ñ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐ¼ Ð¸Ð¼Ð¸Ð´Ð¶ÐµÐ¼ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐ¼ Ð¸Ð¼Ð¸Ð´Ð¶ÐµÐ¼ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÑÐ¸ÑÑÐµÐ¼Ð° Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÑÐµÐ´ÑÑÐ² ÑÐµÐºÐ»Ð°Ð¼Ñ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼ÐµÐ±ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Â«Ð¤ÑÐµÐ³Ð°ÑÂ». Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð±ÑÐ» Ð²ÑÑÐ²Ð»ÐµÐ½ ÑÑÐ´ Ð½ÐµÐ´Ð¾ÑÐ°Ð±Ð¾ÑÐ¾Ðº Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÑÐ´ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð´Ð»Ñ ÐµÐ³Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ ÑÑÐµÐ´ÑÑÐ²Ð° ÑÐµÐºÐ»Ð°Ð¼Ñ Ð¸Ð³ÑÐ°ÑÑ Ð³Ð»Ð°Ð²Ð½ÑÑ ÑÐ¾Ð»Ñ.
Cost-effectiveness of toripalimab plus chemotherapy versus chemotherapy as first-line treatment for advanced non-small cell lung cancer in China: a societal perspective
Creators: name: Lian, Dai
name: Yang, Yi
name: Gan, Yuling
name: Xiao, Dunming
name: Xiang, Yuliang
name: Jiang, Shan
name: Gu, Yuanyuan
name: Chen, Yingyao
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: To investigate the cost-effectiveness of toripalimab plus chemotherapy versus chemotherapy alone for advanced non-small cell lung cancer (NSCLC) patients from a societal perspective. A partitioned-survival model estimated the costs and cost-effectiveness of toripalimab plus chemotherapy versus standard chemotherapy for advanced NSCLC over 20 years. Clinical data were derived from the CHOICE-01 trial, and cost and utility inputs were gathered from Yaozh.com, expert interviews, and a nationwide hospital-based survey. Costs were reported in 2022 US dollars, and outcomes included quality-adjusted life-years (QALYs) and incremental cost-effectiveness ratios (ICERs), with a 5% discount rate was applied. Sensitivity, subgroup, and scenario analyses verified the robustness of results. Toripalimab plus chemotherapy resulted in 3.052 QALYs and a total cost of $60,813, with an ICER of $19,066 per QALY, below China’s 3 times GDP per capita threshold ($38,223). Robustness is confirmed through sensitivity, subgroup and scenario analyses. Toripalimab plus chemotherapy is a cost-effective option for treatment-naive advanced NSCLC compared to chemotherapy alone, providing valuable evidence for clinical and reimbursement decision-making.
A Reflection on the Structure and Process of the Web of Data
Creators: name: Rodriguez, Marko A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Digital Libraries (cs.DL)
subject: General Literature (cs.GL)
subject: FOS: Computer and information sciences
subject: E.1; C.2.4

description: The Web community has introduced a set of standards and technologies for representing, querying, and manipulating a globally distributed data structure known as the Web of Data. The proponents of the Web of Data envision much of the world's data being interrelated and openly accessible to the general public. This vision is analogous in many ways to the Web of Documents of common knowledge, but instead of making documents and media openly accessible, the focus is on making data openly accessible. In providing data for public use, there has been a stimulated interest in a movement dubbed Open Data. Open Data is analogous in many ways to the Open Source movement. However, instead of focusing on software, Open Data is focused on the legal and licensing issues around publicly exposed data. Together, various technological and legal tools are laying the groundwork for the future of global-scale data management on the Web. As of today, in its early form, the Web of Data hosts a variety of data sets that include encyclopedic facts, drug and protein data, metadata on music, books and scholarly articles, social network representations, geospatial information, and many other types of information. The size and diversity of the Web of Data is a demonstration of the flexibility of the underlying standards and the overall feasibility of the project as a whole. The purpose of this article is to provide a review of the technological underpinnings of the Web of Data as well as some of the hurdles that need to be overcome if the Web of Data is to emerge as the defacto medium for data representation, distribution, and ultimately, processing.
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾-Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð²ÐµÐ±-ÑÑÐ°Ð½ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶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ÐºÐ¸Ð½, ÐÐ°ÐºÑÐ¸Ð¼
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: ANDROID
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OPENGL
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description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾-Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°, Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð´Ð»Ñ Ð¿ÑÐ¸ÑÐ¼Ð°, Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ ÑÑÐ°Ð½ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¸Ð´ÐµÐ¾-Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¿Ð¾Ð¿ÑÐ»ÑÑÐ½ÑÐ¹ Ð²Ð¸Ð´ÐµÐ¾ÑÑÑÐ¸Ð¼Ð¸Ð½Ð³Ð¾Ð²ÑÐ¹ Ð¸Ð½ÑÐµÑÐ½ÐµÑ ÑÐµÑÐ²Ð¸Ñ YouTube Ð² ÑÐµÐ¶Ð¸Ð¼Ðµ ÑÐµÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹, ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð½Ð°Ð±Ð¾Ñ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÐ¿Ð¸ÑÐ°Ð½ Ð¿ÑÐ¾ÑÐµÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÐ°Ð±Ð¾ÑÑ.