cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Imaging of tumour microvasculature using high-resolution contrast-enhanced ultrasound together with markers of proliferation, angiogenesis and vascular mimicry to characterise the response to neoadjuvant chemotherapy in triple-negative breast cancer
Creators: name: Rait, Jaideep Singh
Publisher: name: University of Kent
Year: 2024

description: Triple-negative breast cancer (TNBC) represents 10-15% of all breast cancer cases diagnosed annually in the UK. Treatment frequently involves neoadjuvant chemotherapy, immunotherapy and surgical excision. Current imaging techniques to monitor and predict disease response have limited accuracy. New high-resolution contrast-enhanced ultrasound (CEUS) techniques have the ability to image gross tumour morphology and its microvasculature to visualise angiogenesis.
This research aimed to characterise microvessel density (a surrogate marker for angiogenic activity) as quantified by imaging features using high-resolution CEUS and biomarkers of proliferation, angiogenesis and vasculogenic mimicry during neoadjuvant chemotherapy (NACT). The study also investigated whether germline mutations, as well as the basal type phenotype, correlated with microvessel density and tumour response.
Two patients with triple-negative breast cancer and planned neoadjuvant treatment were recruited and, at specific points of NACT, underwent high-resolution CEUS and immunohistochemistry of tissue samples to assess their response to NACT. Both patients (TNBC001 and TNBC002) demonstrated an encouraging response during neoadjuvant treatment radiologically and histologically. TNBC001 has been found to have complete pathological response, and TNBC002 is awaiting completion of the research study.
This preliminary study indicates that high-resolution CEUS is a potentially valuable tool to monitor treatment response during NACT in patients with TNBC with a demonstrable reduction in microvessel density. The results presented here provide the evidence required to initiate a larger-scale study, which will be needed to change clinical practice.
title: ÐÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ°Ñ (ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ) Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÐµÐ»Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ
Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ°Ñ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080100.62 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â». Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "ÐÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ°Ñ (ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ) Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ" Ð¸ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½ÑÐµ Ð´Ð»Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080100.62 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð¿ÑÐ¾ÑÐ¸Ð»Ñ âÐÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð°ÑÐ´Ð¸Ñâ. ÐÐ»Ñ Ð»ÑÑÑÐµÐ³Ð¾ ÑÑÐ²Ð¾ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð² Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð²ÐºÐ»ÑÑÐµÐ½Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¸ Ð¼Ð¸Ð½Ð¸-ÑÐµÑÑÑ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑ Ð² ÑÐ°Ð¼Ð¾Ð¼ ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸, Ð´Ð»Ñ ÑÐµÐ³Ð¾ Ð² Ð½ÐµÐ¼ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ ÑÐ°Ð±Ð»Ð¸ÑÑ, ÑÐ¾ÑÐ¼Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¸ Ñ.Ð¿. Ð¢Ð°ÐºÐ¾Ðµ ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¸Ð·ÑÑÐ¸ÑÑ Ð±Ð¾Ð»ÑÑÐ¸Ð¹ Ð¾Ð±ÑÐµÐ¼ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð½Ð° Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ½ÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÑÐ°Ð²Ð»ÑÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð´Ð¾Ð¼Ð°ÑÐ½ÐµÐ¹ ÑÐ°Ð±Ð¾ÑÑ Ð¸ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸. ÐÑÑÐ¾Ð´Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ Ð² Ð·Ð°Ð´Ð°Ð½Ð¸ÑÑ ÑÑÐ»Ð¾Ð²Ð½ÑÐµ Ð¸ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐ¼ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð¼ ÑÐ»ÑÐ¶Ð¸ÑÑ Ð½Ðµ Ð¼Ð¾Ð³Ñ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°.
Tip vortex cavitation in marine propellers : mechanism and morphing concept
Creators: name: Lak, Saman
Publisher: name: University of British Columbia
Year: 2024

description: Tip vortex cavitation (TVC) is a complex phenomenon that occurs during the operation of marine propellers, contributing to the underwater radiated noise (URN) of marine vessels. The urgent need for alleviation of the URN levels of marine vessels due to its detrimental impact on marine ecosystems necessitates a thorough investigation of this phenomenon and development of mitigation strategies. In this thesis, due to the challenges associated with the numerical simulation of this phenomenon, a comprehensive validation of large eddy simulation of tip vortex cavitating flow past a hydrofoil is conducted, followed by a detailed analysis of the oscillatory dynamics of TVC and its contribution to the near-field pressure fluctuations. In the next stage, geometric modifications of bending and twisting types are proposed and studied as a strategy for the mitigation of tip vortex cavitation. An investigation of modified hydrofoils in various bending and twisting configurations is conducted demonstrating the potential of these strategies for TVC mitigation without adversely affecting the hydrodynamic performance. A detailed analysis of the flow field in various modified configurations is carried out to reveal the mechanisms involved in the TVC mitigation achieved through these geometric modifications. The thesis is concluded with the development of a toolbox for the application of chord-normal bending and twisting modifications to marine propellers. Preliminary simulations of flow past a conventional and a modified propeller are conducted, which demonstrate that the TVC mitigation strategies proposed in the present work are promising methods for reducing the footprints of human activities on the ocean soundscape.
title: ÐÐµÑÐ¿ÐµÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð°ÑÐ°Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð¾Ð²ÑÐ°
title: Non-specific criteria for hydrodynamic training of a paralympic swimmer
Creators: name: ÐÐ¸Ð½Ð¾ÐºÑÑÐ¾Ð², ÐÐµÐ¾Ð½Ð¸Ð´
name: ÐÐµÐ±ÐµÐ´ÐµÐ²Ð°, ÐÐ½Ð½Ð°
name: ÐÐ°ÑÑÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: Ð¿Ð°ÑÐ°Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ðµ Ð¿Ð»Ð°Ð²Ð°Ð½Ð¸Ðµ
Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
ÑÐµÑ Ð½Ð¸ÐºÐ¾-ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
Ð½ÐµÑÐ¿ÐµÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸
ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹
Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸-Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
Ð¿Ð»Ð¾Ð²ÐµÑ-Ð¿Ð°ÑÐ°Ð»Ð¸Ð¼Ð¿Ð¸ÐµÑ
Paralympic swimming
hydrodynamic training
technical and tactical training
non-specific criteria
comprehensive
trait-indicators
Paralympic swimmer

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð½ÐµÑÐ¿ÐµÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ½Ð¾Ð¼ÐµÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ (Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹) ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð»Ð¾Ð²ÑÐ°. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð½Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ ÑÐ°ÑÑÐ¸ÑÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ð¹ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ ÑÑÐ±ÑÐµÐºÑÐ° Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Â«Ð¿Ð»Ð¾Ð²ÐµÑ â Ð²Ð¾Ð´Ð°Â», ÑÐ°Ðº ÐºÐ°Ðº Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐµ Ð¿Ð¾ ÐºÐ°Ð¶Ð´Ð¾Ð¼Ñ ÐºÑÐ¸ÑÐµÑÐ¸Ñ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸-Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑ ÑÐ°Ð·Ð½Ð¾ÑÑÐ¾ÑÐ¾Ð½Ð½Ð¸Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐµÐ·ÐµÑÐ²Ð¾Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð»Ð¾Ð²ÑÐ°-Ð¿Ð°ÑÐ°Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐ°.
description: Non-specific complex criteria of hydrodynamic phenomenology evaluation used in the process of special (hydrodynamic) technical and tactical training of a swimmer are considered. It is shown that the new complex criteria significantly expand the possibilities of quantitative assessment of the manifestations of hydrodynamics of the subject in the system âswimmer - waterâ, as the signs-indicators proposed for each criterion provide a versatile control of the main reserves of the Paralympic swimmerâs training.
A Conversation on Sustainability in Teaching Practice
Creators: name: Perry, Mia
name: Rodolico, Gabriella
name: Thompson, Karen
name: MacEachern, Karen
name: Huser, Camille
Publisher: name: Edge Hill University
Year: 2021
Subjects: Education

description: The recently launched Community of Practice in Sustainability in Teaching and Learning is a group of committed staff who bring both questions and solutions to the issue of sustainability in our teaching practices. The question that we heard most frequently from our colleagues both inside and outside this Community of Practice was “what can I do?” In this context, we decided to open up a space to share accessible tips and encourage discussion at the 14TH ANNUAL LEARNING AND TEACHING CONFERENCE. The interactive workshop was the second in a series of practice-based workshops offered by the Community of Practice. aimed to initiate and support an exchange of ideas on how to embed sustainability into the foundation of all of our teaching, regardless of the discipline, level, or content. We did this through workshopping four essential and adaptable strategies with a range of existing course curricula and contexts.
Forward Physics at the LHC
Creators: name: Martin, A. D.
name: Ryskin, M. G.
name: Khoze, V. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We review two inter-related topics. First, we consider the behaviour of "soft" scattering observables, such as sigma_{tot}, dsigma_{el}/dt, dsigma_{SD}/dtdM^2, particle multiplicities etc., at high-energy proton-(anti)proton colliders. We emphasize the sizeable effects of absorption on high-energy `soft' processes, and, hence, the necessity to include multi-Pomeron-Pomeron interactions in the usual multi-channel eikonal description. We describe a multi-component model which has been tuned to the available data for soft processes in the CERN-ISR to Tevatron energy range, and which therefore allows predictions to be made for `soft' observables at the LHC. The second topic concerns the calculation of the rate of exclusive processes of the form pp --> p+A+p at high energy colliders, where A is a heavy system. In particular, we discuss the survival probability of the rapidity gaps (denoted by the + signs) to both eikonal and enhanced soft rescattering effects. At the LHC energy, the most topical case is when A is a Higgs boson. At the Tevatron, measurements have been made for the exclusive diffractive production of various systems: A being either gamma-gamma, dijet, or a chi_c meson. We compare the observed rates with the expectations. Finally, we describe how predictions for exclusive processes may be checked in the early runs of the LHC.
description: 34 pagers, 16 figures; based on a talk by Alan Martin at the Cracow Epiphany Conference on ``Hadron interactions at the dawn of the LHC, 5-7 January 2009; dedicated to the memory of Jan Kwiecinski, to be published in Acta Physica Polonica, new subsection 3.5 added
title: Ð¡Ð¸ÑÑÐµÐ¼Ð° ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ Ð´Ð°ÐºÑÐ¸Ð»ÑÐ½ÑÑ Ð¶ÐµÑÑÐ¾Ð² ÑÐ·ÑÐºÐ° Ð³Ð»ÑÑ Ð¾Ð½ÐµÐ¼Ñ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Ð¾ÑÐµÐ²Ð°, 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´Ð°ÐºÑÐ¸Ð»ÑÐ½ÑÐµ Ð¶ÐµÑÑÑ
ÑÐ·ÑÐº Ð³Ð»ÑÑ Ð¾Ð½ÐµÐ¼ÑÑ
ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð½Ð° Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¸
ÑÐ²ÐµÑÑÐ¾ÑÐ½ÑÐµ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸

description: Ð¢ÐµÐ¼Ð° Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¾ÑÐ½Ð¾ÑÐ¸ÑÑÑ Ðº Ð·Ð°Ð´Ð°ÑÐ°Ð¼ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð½Ð° Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸ÑÑ.
Ð ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð½Ð° ÑÐµÐ³Ð¾Ð´Ð½ÑÑÐ½Ð¸Ð¹ Ð´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð´ÐµÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¶ÐµÑÑÐ¾Ð² ÑÑÐº ÑÐ·ÑÐºÐ° Ð³Ð»ÑÑÐ¾Ð½ÐµÐ¼ÑÑ, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð±ÑÐ» ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ Ð² Ð²Ð¸Ð´Ðµ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Android. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¾ÑÐ° Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð½Ð° Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¸ Ð±ÑÐ»Ð° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð° Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ ÑÐ²ÐµÑÑÐ¾ÑÐ½Ð°Ñ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð°Ñ ÑÐµÑÑ Inception v3, Ð¿Ð¾Ð´Ð²ÐµÑÐ³ÑÐ°ÑÑÑ Ð¿ÐµÑÐµÐ¾Ð±ÑÑÐµÐ½Ð¸Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ TensorFlow. Ð¢ÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¹ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð´Ð¾ÐºÐ°Ð·Ð°Ð»Ð¾ ÑÑÐ¿ÐµÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð°.
The Hardness-Intensity Diagram of Cygnus X-3: Revisiting the Radio/X-Ray States
Creators: name: Koljonen, K. I. I.
name: Hannikainen, D. C.
name: McCollough, M. L.
name: Pooley, G. G.
name: Trushkin, S. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Cygnus X-3 is one of the brightest X-ray and radio sources in the Galaxy, and is well known for its erratic behaviour in X-rays as well as in the radio, occasionally producing major radio flares associated with relativistic ejections. However, even after many years of observations in various wavelength bands Cyg X-3 still eludes clear physical understanding. Studying different emission bands simultaneously in microquasars has proved to be a fruitful approach towards understanding these systems, especially by shedding light on the accretion disc/jet connection. We continue this legacy by constructing a hardness-intensity diagram (HID) from archival Rossi X-ray Timing Explorer data and linking simultaneous radio observations to it. We find that surprisingly Cyg X-3 sketches a similar shape in the HID to that seen in other transient black hole X-ray binaries during outburst but with distinct differences. Together with the results of this analysis and previous studies of Cyg X-3 we conclude that the X-ray states can be assigned to six distinct states. This categorization relies heavily on the simultaneous radio observations and we identify one new X-ray state, the hypersoft state, similar to the ultrasoft state, which is associated to the quenched radio state during which there is no or very faint radio emission. Recent observations of GeV flux observed from Cyg X-3 (Tavani et al. 2009; Fermi LAT Collaboration et al. 2009) during a soft X-ray and/or radio quenched state at the onset of a major radio flare hint that a very energetic process is at work during this time, which is also when the hypersoft X-ray state is observed. In addition, Cyg X-3 shows flaring with a wide range of hardness.
description: 17 pages, 9 figures, accepted for publication in MNRAS
title: Ð¡ÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ¾Ð²Ð½Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐµÐ½ÐµÑÐ¾Ð² ÑÐµÑÐ¸ ÑÐ¸ÑÐ½ÐµÑ-ÐºÐ»ÑÐ±Ð¾Ð² Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³
title: Comparative analysis of the level of professional preparedness of trainers in the network of fitness clubs in St. Petersburg
Creators: name: ÐÐ¾Ð»ÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
name: ÐÐ¾Ð½Ð¾Ð¼Ð°ÑÐµÐ², ÐÐµÐ½Ð½Ð°Ð´Ð¸Ð¹
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¸ÑÐ½ÐµÑ
ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¸Ð·ÐºÑÐ»ÑÑÑÑÐ½Ð¾-Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÑÐµÐ½ÐµÑ ÑÑÐµÐ½Ð°Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ð»Ð°
Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð·Ð½Ð°Ð½Ð¸Ñ
ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¾ÑÐ¼Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ
fitness
level of education
health-improving activity
gym trainer
professional knowledge
specially organized forms of physical culture

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐ½ÐµÑ-ÑÑÐ»ÑÐ³ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐµÐ½ÐµÑÐ¾Ð² ÑÑÐµÐ½Ð°Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ð»Ð° Ñ ÑÐ°Ð·Ð½ÑÐ¼ ÑÑÐ¾Ð²Ð½ÐµÐ¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð·ÐºÑÐ»ÑÑÑÑÐ½Ð¾-Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸ÐµÐ¼. Ð¡Ð´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¾ ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÐºÑÑÑÐ¾Ð² Ð¿ÐµÑÐµÐ¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð´Ð»Ñ ÑÐ¸ÑÐ½ÐµÑ-Ð¸Ð½ÑÑÑÑÐºÑÐ¾ÑÐ¾Ð².
description: The article touches upon the issues of the quality of the provision of fitness services to the population. A comparative analysis of the theoretical preparedness of gym trainers with different levels of education was carried out. The effectiveness of the implementation of physical culture and health work with the population has been revealed. Conclusions are drawn about the quality of education in the framework of retraining courses for fitness instructors.
SuperIso program and flavor data constraints
Creators: name: Mahmoudi, F.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present here an overview of the SuperIso program which is a public code dedicated to the calculation of flavor physics observables in supersymmetry. The main purpose of the SuperIso program is to provide, by confronting the theoretical predictions to the experimental data for flavor observables, indirect constraints on the parameters of supersymmetry. These constraints can then provide limits on physical masses of yet undiscovered new particles, such as charged Higgs bosons.
description: 6 pages, 1 figure. To appear in the proceedings of "cHarged 2008", Uppsala, Sweden, September 2008
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ. Ð Ð°Ð±Ð¾ÑÐ° Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¼Ð¸ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð² ÑÑÐµÐ´Ðµ Microsoft Office'2013
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð·ÐµÐ»ÐµÑÐºÐ°Ñ, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2016
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð² Ð¿Ð¾Ð»Ð½Ð¾Ð¼ Ð¾Ð±ÑÐµÐ¼Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐµÐºÑÑÐ¾Ð²ÑÐ¹ ÑÐµÐ´Ð°ÐºÑÐ¾Ñ MS Word. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¾Ñ Ð¿ÑÐ¾ÑÑÐµÐ¹ÑÐ¸Ñ Ð´Ð¾ ÑÐ°Ð¼ÑÑ ÑÐ»Ð¾Ð¶Ð½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð², Ð¿ÑÐ¸ÐµÐ¼Ñ Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°Ð±Ð¾ÑÐµ Ð² MS Word. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Microsoft Office Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐµÑÐµÐ½Ð¸Ðµ ÑÑÐ´Ð° Ð¾ÑÐ¸ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð¸ Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ», Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸ÐµÂ» Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
Sharing Christian Faith Through Social Media: Effects on College Students
Creators: name: BOWMAN, GLEN
name: Sheppard, Tyler
Publisher: name: figshare
Year: 2021
Subjects: subject: 170111 Psychology of Religion
subject: FOS: Psychology
subject: 170113 Social and Community Psychology
subject: Sociology
subject: FOS: Sociology

description: This qualitative descriptive study explored how college students describe the influence that encountering Christian faith sharing through social media has on their thoughts, emotions, and behaviors. Data collection took place through interviews and focus groups followed by thematic analysis of the data, which resulted in six themes. Three themes described the influence on college students’ thoughts and emotions: a) the message contents and delivery methods influence college students’ thoughts and emotions, b) positive or negative influences on their thoughts and emotions can occur based on their perception of the posts, and c) people who practice Christian faith sharing through social media but live a sinful lifestyle negatively influence their thoughts and emotions. Three themes described the corresponding influence on behaviors: a) positive thoughts produce positive interpersonal and spiritual behaviors, b) negative thoughts typically decrease interpersonal interactions but also prompt negative or positive behaviors, and c) thinking changes produce greater behavioral changes than college students typically recognize. Using these findings, Christians could learn to share their faith online more effectively and less offensively.
Single-ended Coherent Receiver
Creators: name: Le, Son Thai
name: Aref, Vahid
name: Cho, Junho
Publisher: name: arXiv
Year: 2021
Subjects: subject: Signal Processing (eess.SP)
subject: Information Theory (cs.IT)
subject: Optics (physics.optics)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: Commercial coherent receivers utilize balanced photodetectors (PDs) with high single-port rejection ratio (SPRR) to mitigate the signal-signal beat interference (SSBI) due to the square-law detection process. As the symbol rates of coherent transponders are increased to 100 Gbaud and beyond, maintaining a high SPRR in a cost-effective manner becomes more and more challenging. One potential approach for solving this problem is to leverage the concept of single-ended coherent receiver (SER) where single-ended PDs are used instead of the balanced PDs. In this case, the resulting SSBI should be mitigated in the digital domain. In this paper, we show that SSBI can be effectively mitigated using various low-complexity techniques, such as the direct filed reconstruction (DFR), clipped iterative SSBI cancellation (CIC) and gradient decent (GD). In addition, we present a self-calibration technique for SERs which can be extended for characterizing the optical-to-electrical (O/E) response of a conventional balanced coherent receiver (BR). Using the developed techniques, we then experimentally demonstrate a 90 Gbaud probabilistically constellation shaped 64-QAM (PCS-64QAM) transmission using a SER, achieving a net data rate of 882 Gb/s over 100 km of standard single mode fiber (SSMF). The sensitivity penalty compared to the BR is below 0.5 dB. We expect that when the symbol rate is increased further, a SER can potentially outperform a BR, especially when applied to cost-sensitive commercial pluggable coherent transceivers
title: Smoke Particle Size Distribution in Pine Wood Fires
Creators: name: Mustafa, B.
name: Mat Kiah, M.
name: Andrews, G.
name: Phylaktou, H.
name: Li, H.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019

description: There is a growing concern about the impact of ultra- fine particulates released from fires on the health of
humans in fires and the related environmental pollution. However, there is no requirement to measure
particle mass or number from legislated test fires and hence there is minimum information in the literature
on this toxic hazard in fires. This work compares particulates generated from freely ventilated and
restricted ventilation pine wood fires using the cone calorimeter. The standard cone calorimeter with
freely ventilated combustion was modified by adding a discharge pipe to the cone heater that enabled
direct fire product sampling from the cone outlet. The controlled atmosphere cone calorimeter was used
for the restricted ventilation fire with metered air fed to the enclosure around the test area. Both tests used
a radiant heat flux of 35kW/m2. Real-time particulate number and size distribution were measured using
the Cambustion DMS 500 particle electrical mobility spectrometer. The particulate size distribution
showed a peak of ultra-fine aerosol particles of <100 nm in the early stage of the fire development and
then changed to the larger size (100-1000 nm) with a peak of 200 nm as the fire progressed. The restricted
ventilation fire generated more particles. There were high numbers of 20 nm particles throughout the fire
and these have the greatest health risks. Toxic gases were also measured from the raw exhaust gases using
a heated Gasmet FTIR gas analyser.
Energy Spectra of the Soft X-ray Diffuse Emission in Fourteen Fields Observed with Suzaku
Creators: name: Yoshino, T.
name: Mitsuda, K.
name: Yamasaki, N. Y.
name: Takei, Y.
name: Hagihara, T.
name: Masui, K.
name: Bauer, M.
name: McCammon, D.
name: Fujimoto, R.
name: Wang, Q. D.
name: Yao, Y.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The soft diffuse X-ray emission of twelve fields observed with Suzaku are presented together with two additional fields from previous analyses. All have galactic longitudes 65 deg < l < 295 deg to avoid contributions from the very bright diffuse source that extends at least 30 deg from the Galactic center. The surface brightnesses of the Suzaku nine fields for which apparently uncontaminated ROSAT All Sky Survey (RASS) were available were statistically consistent with the RASS values, with an upper limit for differences of 17 x 10^{-6} c s^{-1} amin^{-2} in R45}-band. The Ovii and Oviii intensities are well correlated to each other, and Ovii emission shows an intensity floor at ~2 photons s^{-1} cm^{-2 str^{-1} (LU). The high-latitude Oviii emission shows a tight correlation with excess of Ovii emission above the floor, with (Oviii intensity) = 0.5 x [(Ovii intensity) -2 LU], suggesting that temperatures averaged over different line-of-sight show a narrow distribution around ~0.2 keV. We consider that the offset intensity of Ovii arises from the Heliospheric solar wind charge exchange and perhaps from the local hot bubble, and that the excess Ovii (2-7 LU) is emission from more distant parts of the Galaxy. The total bolometric luminosity of this galactic emission is estimated to be 4 x 10^{39} erg s^{-1}, and its characteristic temperature may be related to the virial temperature of the Galaxy.
description: 22 Pages, 8 figures, to appear in PASJ (Vol.61 No.4)
title: ÐÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ Ð¿ÑÐ¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÐºÑÑÐ±Ð¸Ð½Ð°, ÐÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ
ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¹ Ð¾Ð±Ð¼ÐµÐ½ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐÐ Ð£Ð¡ ÐÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³ Ð¡ÐÐÂ». ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¾Ð±ÑÐ¸Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¸ ÑÑÐµÐ¼Ñ ÑÐ°Ð±Ð¾ÑÑ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð½Ð° ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐµ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÑ. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð¸Ð·ÑÑÐ¸ÑÑ Ð¸ Ð´Ð°ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÑ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¼ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼, Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÐ¼ Ð² Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð¼ ÑÑÐµÑÐµ Ð² Ð Ð¾ÑÑÐ¸Ð¸.
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ ÐÐ­Ð¡ Ñ ÑÐµÐ°ÐºÑÐ¾ÑÐ°Ð¼Ð¸ ÐÐÐ­Ð - 1000 Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 2*1000 ÐÐ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 Ð¾ÑÐºÐ¾Ð²Ð°Ð½Ð¾Ð², ÐÐ¸ÑÐ°Ð¸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: 2018
Subjects: Ð°ÑÐ¾Ð¼Ð½Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ñ (ÐÐ­Ð¡)
ÑÐ¸Ð»Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¾Ðº ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ (Ð¢ÐÐ)
ÐÐÐ­Ð -1000
ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÐÐ­Ð¡ Ñ 2 Ð±Ð»Ð¾ÐºÐ°Ð¼Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 1000 ÐÐÑ. ÐÑÐ»Ð¾ Ð²ÑÐ±ÑÐ°Ð½Ð¾ ÑÐ¸Ð»Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ: Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÑ, ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ Ð¸ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° ÐÐ­Ð¡, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ¾ÐºÐ° ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ Ð² Ð¾ÑÐ¾Ð±ÑÑ ÑÐ¾ÑÐºÐ°Ñ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÑÐµÐ¼Ñ. ÐÐ°Ð»ÐµÐµ Ð±ÑÐ»Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ, ÑÐ¸Ð½Ñ, ÐºÐ°Ð±ÐµÐ»Ð¸, ÑÐ¾ÐºÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ñ Ð¸ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ ÑÐ¾ÐºÐ° Ð¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹, ÑÐ°Ð·ÑÐµÐ· Ð¸ ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° 500 ÐºÐ.
ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim4$
Creators: name: García-Vergara, Cristina
name: Rybak, Matus
name: Hodge, Jacqueline
name: Hennawi, Joseph F.
name: Decarli, Roberto
name: González-López, Jorge
name: Arrigoni-Battaia, Fabrizio
name: Aravena, Manuel
name: Farina, Emanuele P.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present an Atacama Large Millimeter/submillimeter Array (ALMA) survey of CO(4--3) line emitting galaxies in 17 quasar fields at $z\sim4$ aimed to perform the first systematic search of dusty galaxies in high$-z$ quasar environments. Our blind search of galaxies around the quasars results in 5 CO emitters with S/N$\geq5.6$ within a projected radius of $R\lesssim1.5\,h^{-1}\,$cMpc and a velocity range of $\rmΔ\,v=\pm1000\,$km\,s$^{-1}$ around the quasar. In blank fields, we expect to detect only 0.28 CO emitters within the same volume, implying a total overdensity of $17.6^{+11.9}_{-7.6}$ in our fields, and indicating that quasars trace massive structures in the early universe. We quantify this overdensity by measuring the small-scale clustering of CO emitters around quasars, resulting in a cross-correlation length of $r_{\rm 0,QG}=8.37^{+2.42}_{-2.04}\,h^{-1}\,$cMpc, assuming a fixed slope $γ=1.8$. This contradicts the reported mild overdensities (x1.4) of Lyman alpha emitters (LAEs) in the same fields at scales of $R\lesssim7\,h^{-1}\,$cMpc which is well described by a cross-correlation length 3 times lower than that measured for CO emitters. We discuss some possibilities to explain this discrepancy, including low star formation efficiency, and excess of dust in galaxies around quasars. Finally, we constrain, for the first time, the clustering of CO emitters at $z\sim4$, finding an auto-correlation length of $r_{\rm 0,CO}=3.14\pm1.71\,h^{-1}\,$cMpc (with $γ=1.8$). Our work together with the previous study of LAEs around quasars traces simultaneously the clustering properties of both optical and dusty galaxy populations in quasars fields, stressing the importance of multi-wavelength studies, and highlighting important questions about galaxy properties in high$-z$ dense environments.
description: 17 pages, 8 figures, submitted to the ApJ
title: Ð¡ÐµÐ¼ÐµÐ¹Ð½Ð¾Ðµ Ð¿ÑÐ°Ð²Ð¾ Ð¸ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ° ÑÐµÐ¼ÑÐ¸ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ»ÑÐ½ÐµÐ²Ð° , ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÐ¼ÑÑ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸
ÑÐµÐ¼ÐµÐ¹Ð½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° ÐÑÐ¿Ð°Ð½Ð¸Ð¸
ÑÐµÐ³Ð¸ÑÑÑÐ°ÑÐ¸Ñ Ð±ÑÐ°ÐºÐ°
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐµÐ¼ÐµÐ¹Ð½Ð¾Ð¼Ñ Ð¿ÑÐ°Ð²Ñ ÐÑÐ¿Ð°Ð½Ð¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÐµÐ¼ÑÐµ Ð¸ ÑÐµÐ¼ÐµÐ¹Ð½Ð¾Ð¼ Ð¿ÑÐ°Ð²Ðµ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾: Ð¸ÑÑÐ¾ÑÐ¸Ñ ÑÐµÐ¼ÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð°, ÑÐµÐ»Ð¸Ð³Ð¸Ð¾Ð·Ð½Ð¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÐµÐ¼ÐµÐ¹Ð½ÑÑ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÑ, ÑÐµÐ¼ÐµÐ¹Ð½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð¸ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÑ, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ¸Ðµ ÑÐµÐ¼ÐµÐ¹Ð½Ð¾Ðµ Ð¿ÑÐ°Ð²Ð¾, Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ Ð±ÑÐ°ÐºÐ° Ð¸ ÐµÐ³Ð¾ ÑÐ¾ÑÐ¼Ñ, Ð¿ÑÐ°Ð²Ð¾ Ð½Ð° ÑÐµÐ³Ð¸ÑÑÑÐ°ÑÐ¸Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¶Ð¸Ð²Ð°Ð½Ð¸Ñ, ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÐ°Ð·Ð²Ð¾Ð´Ð° Ð¸ ÐµÐ³Ð¾ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ. ÐÐ·ÑÑÐµÐ½Ð° ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° ÐÑÐ¿Ð°Ð½Ð¸Ð¸, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¾ÑÐµÐ½Ñ Ð²Ð°Ð¶Ð½Ð° Ð´Ð»Ñ Ð¼Ð°Ð»Ð¾Ð¸Ð¼ÑÑÐ¸Ñ ÑÐµÐ¼ÐµÐ¹, ÑÐµÐ¼ÐµÐ¹ Ñ Ð¾Ð´Ð½Ð¸Ð¼ ÑÐ¾Ð´Ð¸ÑÐµÐ»ÐµÐ¼, Ð¼Ð½Ð¾Ð³Ð¾Ð´ÐµÑÐ½ÑÑ ÑÐµÐ¼ÐµÐ¹, Ð´ÐµÑÐµÐ¹ Ð¸Ð½Ð²Ð°Ð»Ð¸Ð´Ð¾Ð², ÑÐ°ÐºÐ¶Ðµ Ð±ÑÐ»Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ° Ð² ÑÐ»ÑÑÐ°Ðµ Ð½Ðµ Ð²ÑÐ¿Ð»Ð°ÑÑ Ð°Ð»Ð¸Ð¼ÐµÐ½ÑÐ¾Ð² Ð¸ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ° Ð¿Ð¾ÑÐ»Ðµ ÑÐ°Ð·Ð²Ð¾Ð´Ð° ÑÐµÐ¼, ÐºÑÐ¾ Ð¾ÑÑÐ°ÐµÑÑÑ Ð² ÑÐ»Ð¾Ð¶Ð½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾ÑÐ»Ðµ ÑÐ°ÑÑÐ¾ÑÐ¶ÐµÐ½Ð¸Ñ Ð±ÑÐ°ÐºÐ°. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ° ÑÐ¾ÑÐ¼ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ Ð±ÑÐ°ÐºÐ°, ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ° ÑÐ°Ð·Ð²Ð¾Ð´Ð¾Ð². ÐÑÑÐ²Ð»ÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð² ÑÑÐµÑÐµ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐµ ÑÐµÐ¼ÑÐ¸, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ Ð½Ðµ Ð² Ð»ÑÑÑÐµÐ¼ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸ Ð¸Ð· Ð²ÑÐµÑ ÑÑÑÐ°Ð½ ÐÐ²ÑÐ¾Ð¿Ñ.
title: Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ Ð¼Ð¾Ð½Ð°ÑÑ Ð¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¾Ð²ÑÐºÐ¸Ð¹ , ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸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°Ð±ÑÐ¾Ð»ÑÑÐ½Ð°Ñ Ð¼Ð¾Ð½Ð°ÑÑ Ð¸Ñ
Ð¿Ð°ÑÐ»Ð°Ð¼ÐµÐ½ÑÑÐºÐ°Ñ Ð¼Ð¾Ð½Ð°ÑÑ Ð¸Ñ
Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½Ð°Ñ Ð¼Ð¾Ð½Ð°ÑÑ Ð¸Ñ
ÐºÐ¾Ð½ÑÑÐ¸ÑÑÑÐ¸Ñ
Ð¿Ð°ÑÐ»Ð°Ð¼ÐµÐ½Ñ

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° (Ð´Ð¸Ð¿Ð»Ð¾Ð¼) Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹ Ð¼Ð¾Ð½Ð°ÑÑÐ¸Ð¸ Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¼Ð¾Ð½Ð°ÑÑÐ¸Ð¸ ÐºÐ°Ðº ÑÐ¾ÑÐ¼Ñ Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÐµÐµ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°Ð·Ð½Ð¾Ð²Ð¸Ð´Ð½Ð¾ÑÑÐ¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð¾Ð½Ð°ÑÑÐ¸Ð¹. ÐÐ¾Ð½Ð°ÑÑÐ¸Ñ - ÑÑÐ¾ ÑÐ°ÐºÐ°Ñ ÑÐ¾ÑÐ¼Ð° Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¸ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð²ÐµÑÑÐ¾Ð²Ð½Ð°Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð²Ð»Ð°ÑÑÑ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐµÑÑÑ ÐµÐ´Ð¸Ð½Ð¾Ð»Ð¸ÑÐ½Ð¾ Ð¸ Ð¿ÐµÑÐµÑÐ¾Ð´Ð¸Ñ, ÐºÐ°Ðº Ð¿ÑÐ°Ð²Ð¸Ð»Ð¾, Ð¿Ð¾ Ð½Ð°ÑÐ»ÐµÐ´ÑÑÐ²Ñ. ÐÐ³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½Ð°Ñ (ÐºÐ¾Ð½ÑÑÐ¸ÑÑÑÐ¸Ð¾Ð½Ð½Ð°Ñ) Ð¼Ð¾Ð½Ð°ÑÑÐ¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ°ÐºÑÑ ÑÐ¾ÑÐ¼Ñ Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¸ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð²Ð»Ð°ÑÑÑ Ð¼Ð¾Ð½Ð°ÑÑÐ° Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÑÐ½ÑÐ¼ Ð¾ÑÐ³Ð°Ð½Ð¾Ð¼. ÐÐ±ÑÑÐ½Ð¾ ÑÑÐ¾ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ ÐºÐ¾Ð½ÑÑÐ¸ÑÑÑÐ¸ÐµÐ¹, ÑÑÐ²ÐµÑÐ¶Ð´Ð°ÐµÐ¼Ð¾Ð¹ Ð¿Ð°ÑÐ»Ð°Ð¼ÐµÐ½ÑÐ¾Ð¼. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐ¾ÑÐ¼ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ Ð¼Ð¾Ð½Ð°ÑÑÐ¸Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð¾Ð½Ð°ÑÑÐ¸Ð¹.
Theory of finite-entanglement scaling at one-dimensional quantum critical points
Creators: name: Pollmann, Frank
name: Mukerjee, Subroto
name: Turner, Ari
name: Moore, Joel E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Studies of entanglement in many-particle systems suggest that most quantum critical ground states have infinitely more entanglement than non-critical states. Standard algorithms for one-dimensional many-particle systems construct model states with limited entanglement, which are a worse approximation to quantum critical states than to others. We give a quantitative theory of previously observed scaling behavior resulting from finite entanglement at quantum criticality: the scaling theory of finite entanglement is only superficially similar to finite-size scaling, and has a different physical origin. We find that finite-entanglement scaling is governed not by the scaling dimension of an operator but by the "central charge" of the critical point, which counts its universal degrees of freedom. An important ingredient is the recently obtained universal distribution of density-matrix eigenvalues at a critical point\cite{calabrese1}. The parameter-free theory is checked against numerical scaling at several quantum critical points.
description: 4 pages + 2 pages supplementary information
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð±Ð¾ÑÑ Service Desk Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ "ÐÐµÐ½ÑÐ°" Ð·Ð° ÑÑÐµÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÑÐ»Ñ Ð¼Ð°ÑÑÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð°Ð¿ÑÐ¾ÑÐ¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ´ÑÑÑÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ° Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹
sevise desk
sla
Ð±Ð°Ð·Ð° Ð·Ð½Ð°Ð½Ð¸Ð¹

description: Ð¦ÐµÐ»Ñ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° ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð·, Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ Ð¾Ð±Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¾ÑÐ´ÐµÐ»Ð° Service Desk ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐµÐ½ÑÐ°Â».
ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ Ð±ÑÐ´ÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ: Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° ÑÐ°Ð±Ð¾ÑÑ Service Desk; ÑÐ´ÐµÐ»Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ðµ Ð·Ð°Ð´Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾Ð±Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Service Desk; Ð¿ÑÐ¾Ð´ÐµÐ»Ð°Ð½Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÑÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸, Ð´Ð»Ñ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÑ Ð·Ð°Ð¿ÑÐ¾ÑÐ¾Ð²; ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´ÐµÐ»Ð°Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ.
ÐÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ, ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ðµ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÑ Ð·Ð°Ð¿ÑÐ¾ÑÐ¾Ð² Ð¾Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹. Ð¢Ð°Ðº Ð¶Ðµ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÑ Ð·Ð°Ð¿ÑÐ¾ÑÐ¾Ð², ÑÐ¾ÑÐ¾ÑÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð¾ÑÐ´ÐµÐ»Ð° Service Desk.
Additional file 1 of Gut microbiota profiling variated during colorectal cancer development in mouse
Creators: name: Liu, Jingjing
name: Dong, Wei
name: Zhao, Jian
name: Wu, Jing
name: Xia, Jinqiang
name: Xie, Shaofei
name: Song, Xiaofeng
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 1.
Ray-Tracing Analysis of Anisotropic Neutrino Radiation for Estimating Gravitational Waves in Core-Collapse Supernovae
Creators: name: Kotake, Kei
name: Iwakami, Wakana
name: Ohnishi, Naofumi
name: Yamada, Shoichi
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We propose a ray-tracing method to estimate gravitational waves (GWs) generated by anisotropic neutrino emission in supernova cores. To calculate the gravitational waveforms, we derive analytic formulae in a useful form, which are applicable also for three-dimensional computations. Pushed by evidence of slow rotation prior to core-collapse, we focus on asphericities in neutrino emission and matter motions outside the protoneutron star. Based on the two-dimensional (2D) models, which mimic SASI-aided neutrino heating explosions, we compute the neutrino anisotropies via the ray-tracing method in a post-processing manner and calculate the resulting waveforms. With these computations, it is found that the waveforms exhibit more variety in contrast to the ones previously estimated by the ray-by-ray analysis (e.g., Kotake et al. (2007)). In addition to a positively growing feature, which was predicted to determine the total wave amplitudes predominantly, the waveforms are shown to exhibit large negative growth for some epochs during the growth of SASI. These features are found to stem from the excess of neutrino emission in lateral directions, which can be precisely captured by the ray-tracing calculation. Due to the negative contributions and the neutrino absorptions appropriately taken into account by the ray-tracing method, the wave amplitudes become more than one-order-of magnitude smaller than the previous estimation, thus making their detections very hard for a galactic source.On the other hand, it is pointed out that the GW spectrum from matter motions have its peak near $\sim 100$ Hz, which could be characteristic for the SASI-induced supernova explosions.(abridged)
description: 30 pages, 17 figures, ApJ in press
title: ÐÐ¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° ÐÐÐ "ÐÐ½ÑÑÐ¸ÑÑÑ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÐ¾ÑÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¿ÑÐ¾ÐµÐºÑÐ½Ð°Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ
Ð´Ð¾Ð³Ð¾Ð²Ð¾ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ°

description: Ð¦ÐµÐ»Ñ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° ÑÐ²Ð»ÑÐµÑÑÑ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÑÐ° Ð² ÐÐÐ Â«ÐÐ½ÑÑÐ¸ÑÑÑ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸ÑÂ» Ð² ÑÐ¾Ð´Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ñ ÑÑÐµÑÐ¾Ð¼ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð´Ð¾Ð³Ð¾Ð²Ð¾ÑÐ½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ Ð±ÑÐ» ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ Ð´Ð¾Ð³Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð²Ð°Ð¶Ð½Ñ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÑÐ°. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ» Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½ Ð³Ð»Ð°Ð²Ð½ÑÐ¹ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐ¾Ðº Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð·Ð°ÐºÐ»ÑÑÐ°ÑÑÐ¸ÐµÑÑ Ð² Ð¾ÑÑÑÑÑÑÐ²Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾Ñ Ð²Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð² ÑÐ¾ÑÐ½Ð¾ ÑÑÐ¾Ðº Ñ ÑÑÑÑÐ¾Ð¼ ÑÐµÑÑÑÑÐ½ÑÑ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð¾ÑÐ´ÐµÐ»Ð°Ð¼ Ð¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ°Ð¼. ÐÐ»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÑÐµÐ¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð±ÑÐ» Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð±Ð¾Ð»ÐµÐµ Ð´ÐµÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°. ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð´Ð¾Ð»Ð¶Ð½Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸ÑÑ Ð»ÑÑÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÑÐµÐ¼Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð·Ð° ÑÑÑÑ ÐµÐ³Ð¾ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ¾ ÐµÑÑÑ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð¿Ð¾ ÑÑÐ°Ð¿Ð°Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð½Ð¾ Ð¸ Ð¿Ð¾ ÐºÐ°Ð¶Ð´Ð¾Ð¹ Ð¸Ð· ÑÐ°Ð±Ð¾Ñ ÑÑÐ°Ð¿Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½ÐµÐ·Ð°Ð¼ÐµÐ´Ð»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ°Ð³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¾ÑÐºÐ»Ð¾Ð½ÐµÐ½Ð¸Ñ Ð² ÑÐ¾Ð´Ðµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°.
On the Initial Mass Function and tilt of the Fundamental Plane of massive early-type galaxies
Creators: name: Grillo, C.
name: Gobat, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the most plausible stellar Initial Mass Function (IMF) and the main origin of the tilt of the Fundamental Plane (FP) for old, massive early-type galaxies. We consider a sample of 13 bright galaxies of the Coma cluster and combine our results with those obtained from a sample of 57 lens galaxies in the same luminous mass range. We estimate the luminous mass and stellar mass-to-light ratio values of the sample galaxies by fitting their SDSS multi-band photometry with composite stellar population models computed with different dust-free, solar-metallicity templates and IMFs. We compare these measurements and those derived from two-component orbit-based dynamical modelling. The photometric and dynamical luminous mass estimates of the galaxies in our sample are consistent, within the errors, if a Salpeter IMF is adopted. On the contrary, with a Kroupa or Chabrier IMF the two luminous mass diagnostics differ at a more than 4 σlevel. For the massive Coma galaxies, their stellar mass-to-light ratio scales with luminous mass as the corresponding effective quantities are observed to scale on the FP. This indicates that the tilt of the FP is primarily caused by stellar population properties. We conclude that old, massive lens and non-lens early-type galaxies obey the same luminous and dynamical scaling relations, favour a Salpeter IMF, and suggest a stellar population origin for the tilt of the FP. The validity of these results for samples of early-type galaxies with different age and mass properties still remains to be tested.
description: 5 pages, 2 figures, accepted by MNRAS