cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Large-scale collective properties of self-propelled rods
Creators: name: Ginelli, F.
name: Peruani, F.
name: Baer, M.
name: Chate, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study, in two space dimensions, the large-scale properties of collections of constant-speed polar point particles interacting locally by nematic alignment in the presence of noise. This minimal approach to self-propelled rods allows one to deal with large numbers of particles, revealing a phenomenology previously unseen in more complicated models, and moreover distinctively different from both that of the purely polar case (e.g. the Vicsek model) and of active nematics.
description: Submitted to Phys. Rev. Lett
Mosu huogou Miller, Griswold & Yin 2009, sp. n.
Creators: name: Miller, Jeremy
name: Griswold, Charles
name: Yin, Chang
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Mysmenidae
Mosu
Mosu huogou

description: Mosu huogou Miller, Griswold & Yin, sp. n. urn:lsid:zoobank.org:act: 045120B5-85D4-4A79-8B2F-26FE9B340702 Figs 43 H-I, 96 Material Examined. Holotype: CHINA: Yunnan: Gongshan Co. Dulongjiang Township, Haban Falls 0.5 airkm from Qinlangdang village along Dulong Jiang, 27.67934°N, 98.27291°E, 1265 m, 1 September 2006, subtropical evergreen broadleaf forest, sifting leaf litter, J.A. Miller, D.H. Kavanaugh, JM06090105 (CASENT 9024389, HNU), 1 ♀. Etymology. Formed from the Chinese words for fire (huǒ) and dog (gǒu), referring to the element and animal of the Chinese zodiac when this species was collected. Diagnosis. Distinguished from M. nujiang by the shape of the spermathecae, transversely ovoid in M. huogou (Fig. 43I), bulbous in M. nujiang (Fig. 43G), by the separation of the membranous copulatory ducts in the posteromedial region (Fig. 43I; justaposed in M. nujiang, Fig. 43G), and by the presence of a posterior abdominal tubercle in M. nujiang, absent in M. huogou. Description. Carapace brown. Sternum dark gray with lighter patches down midline and anterolaterally. Legs light brown, darker distally on tibiae, metatarsi, and tarsi. Abdomen dark gray with tan and white spots; posterior tubercle absent. Vulva: Spermathecae transversely ovoid, copulatory duct adjacent to spermathecae less strongly sclerotized than spermathecae. Fertilization ducts run posteromesally then turn anteriorly. Membranous copulatory ducts in posteriomedian region separated (Fig. 43I). Female (holotype): Total length 0.92, carapace 0.44 long, 0.39 wide, clypeus 0.09, sternum 0.26 long, 0.27 wide, coxa IV separated by 2.08 times their width. Macrosetae: Leg I: patella d1, tibia d1; Leg II: patella d1, tibia d1; Leg III: patella d1, tibia d1; Leg IV: patella d1, tibia d1. Metatarsal trichobothria: TmI: 0.31; TmII: 0.31; TmIII: 0.33. Leg measurements: see Appendix A. Male unknown.
description: Published as part of Miller, Jeremy, Griswold, Charles & Yin, Chang, 2009, The symphytognathoid spiders of the Gaoligongshan, Yunnan, China (Araneae: Araneoidea): Systematics and diversity of micro-orbweavers, pp. 9-195 in ZooKeys 11 (11) on page 53, DOI: 10.3897/zookeys.11.160, http://zenodo.org/record/576459
title: Ð¡Ð¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ ÑÐ²ÑÐ·ÑÐ¼ Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Novus)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð»ÐµÑÐ±Ð°Ñ , ÐÐµÑÑ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: 2016
Subjects: PR
ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÑÐ¾Ð±ÑÑÐ¸Ð¹Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
special events
event management

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°ÐºÐ¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, ÐºÐ°Ðº ÑÐ¾Ð»Ñ Ð¸ Ð¼ÐµÑÑÐ¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ ÑÐ²ÑÐ·ÑÐ¼ Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÑ, Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ ÑÐµÐ»Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð¼ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÐ¾Ð¼Ð¸Ð¼Ð¾ ÑÑÐ¾Ð³Ð¾ Ð² ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÐµÑÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿Ð¾ ÑÐ²ÑÐ·ÑÐ¼ Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐµÐ¹ÑÑ Ð½Ð° Ð¾ÑÐ´ÐµÐ»Ð¾ÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ñ Ð¸ Ð¸Ð½ÑÐµÑÑÐµÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸ÑÑ, Novus. ÐÐ°ÐµÑÑÑ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð»Ð¾ÑÐ»ÑÐ½Ð¾ÑÑÐ¸ Novus Design Community. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÑÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
description: This bachelor work is devoted to special events in the public relations work on the example of company Novus. The research issued such theoretical aspects of special events organization as the role and the place of special events in the public relations work, its concept and objectives, and an assessment of special events effectiveness. Moreover it is characterized PR activities of the company specializing in finishing materials and interior solutions - Novus. It describes the characteristics of the special event organization and realization as part of the loyalty program Novus Design Community. There are some recommendations for Public Relations strategy in the key of special events.
Magnetic layers and neutral points near rotating black hole
Creators: name: Karas, V.
name: Kopacek, O.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Magnetic layers are narrow regions where the field direction changes sharply. They often occur in the association with neutral points of the magnetic field. We show that an organised field can produce these structures near a rotating black hole, and we identify them as potential sites of magnetic reconnection. To that end we study the field lines affected by the frame-dragging effect, twisting the magnetic structure and changing the position of neutral points. We consider oblique fields in vacuum. We also include the possibility of translational motion of the black hole which may be relevant when the black hole is ejected from the system. The model settings apply to the innermost regions around black holes with the ergosphere dominated by a super-equipartition magnetic field and loaded with a negligible gas content.
description: 10 pages, 3 figures, Classical and Quantum Gravity accepted
Realistic first-principles calculations of the magnetocaloric effect: applications to hcp Gd
Creators: name: Vieira, R. Martinho
name: Eriksson, O.
name: Björkman, T.
name: Bergman, A.
name: Herper, H. C.
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: We present an efficient computational approach to evaluate field-dependent entropy of magnetocaloric materials from ab-initio methods. The temperature dependence is reported for the entropy change, specific heat and magnetization for hcp Gd. To obtain optimal accuracy in the calculations, a mixed-scheme for magnetic Monte Carlo simulations is proposed and found to be superior to using pure quantum or classic statistics. It is demonstrated that lattice and magnetic contributions play a role in the entropy change and that the dominating contribution comes from the magnetic contribution. The total calculated entropy change agrees with measurements at room temperature. Demonstration of the accuracy of ab-initio theory, coupled to statistical methods, for accurate calculations of the total entropy variation associated with the magnetic transition of Gd. Reproduction of experimental data of entropy change.
Chanea Miller, Griswold & Yin 2009, gen. n.
Creators: name: Miller, Jeremy
name: Griswold, Charles
name: Yin, Chang
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Mysmenidae
Chanea

description: Genus Chanea Miller, Griswold & Yin, gen. n. urn:lsid:zoobank.org:act: E6C9BD88-D0C8-4915-9C4C-EC945E2F0F99 Type species. Chanea suukyii Miller, Griswold & Yin, sp. n. Etymology. Derived from the Chinese word for coil (chán). The gender is feminine. Diagnosis. Male distinguished from other mysmenids by the long coiled embolus (Figs 49A, 51B), the entire distal part of the cymbium (Fig. 49A), the widely spaced anterior median eyes, and pair of macrosetae on the clypeus (Fig. 52B). Female distinguished by the long copulatory ducts coiled around the fertilization ducts (Fig. 49C). Species. Chanea suukyii, sp. n.
description: Published as part of Miller, Jeremy, Griswold, Charles & Yin, Chang, 2009, The symphytognathoid spiders of the Gaoligongshan, Yunnan, China (Araneae: Araneoidea): Systematics and diversity of micro-orbweavers, pp. 9-195 in ZooKeys 11 (11) on page 54, DOI: 10.3897/zookeys.11.160, http://zenodo.org/record/576459
Francis Ponge, artisan du langage
Creators: name: Coope, Renee A.G.
Publisher: name: University of British Columbia
Year: 2011

description: Seuls qualquee écrivains et amis de Francis Ponge ont remarqué son oeuvre et lui ont consacré, entre autres, divers articles dans des revues littéraires telles que les Cahiers du Sud, les Cahiera de la Pléiade et la N.N.R.F. qui a voulu attirer l’attention du grand public en la presentant dans un numéro ("Hammage à Francis Ponge"). Tirés à pou d’exemplaires, les ouvrages de Ponge paraissent surtout chez Gallimard, ce qui donne une idée de l'importance de ce poete presque inconnu. De très belles éditions aux illustratins précieuses ont paru chez Mermod, Louise Leiris, Pro-Francis… Seul Le Parti pris des choses a connu une réédition. Quelques poemes furent publiés dan des revues ou séparérement, avant d’être recueillis dans la Rage de l’expressions. Francis Ponge est né en 1899. Comme il s'agit d’une oeuvre inachevée, cette étude ne peut être au fond que proviso ire. II est à noter qu’après un silence de vingt ans, cette oeuvre fut lancée vers 1942, publication qui a profité d’une certaine accalmie littéraire sous I'Occupation Allemande. Sana renier see premiere poèmes hermétiques, Ponge a pensé qu’il avait alors quelque chose à dire. Découvert par Jean Paulhan, Ponge a été ensuite vivement encouragé par Sartre et Camus à continuer sa tentative poétique. Il n’est pas aisé de trouver, même chez un libraire parisien, les minces plaquettes de Ponge. Nous tenons, à ce sujet, à remercier Mile Elisabeth Walter qui a bien voulu nous communiquer, avec d'autres renseignemente, le texte inédit d’une conference de l’auteur. M. Gordon Andison du Département de Francais nous a soutenue de ses encouragements au long do notre travail, cependant que M. Kurt Weinberg du Département de Francaio nous a tout particulièrement aidée de ses conseils, de ses suggestions et de ses oritques amicales. Je leur adresse à tous deux mes très sinoères remerciemants.
Impact of Infarct Size on Blood Pressure in Young Patients with Acute Stroke
Creators: name: Zeenat Qureshi Stroke Institutes
Publisher: name: Zenodo
Year: 2023

description: Background

Hypertension can be found in up to 80% of patients with acute stroke. Many factors have been related to this phenomenon such as age, history of hypertension, and stroke severity. The aim of our study was to determine the relationship between infarct volume and blood pressure, at admission, in young patients with acute ischemic stroke.

Materials and Methods

Patients younger than 55 years old admitted within 24 hours of ischemic stroke were included. Socio-demographic variables, systolic blood pressure, diastolic blood pressure, and infarct volume at admission were assessed. Statistical analysis: mean and SEM for quantitative variables, percentages for qualitative, and Spearman correlations (p value < 0.05 was considered statistically significant).

Results

Twenty-two patients (12 men), mean age: 44.64 ± 1.62 years. The most frequent vascular risk factors were: hypertension, smoking, and overweight (40.9%). Mean systolic and diastolic blood pressure on admission were: 143.27 ± 6.57 mmHg and 85.14 ± 3.62 mmHg, respectively. Infarct volume: 11.55 ± 4.74 ml. Spearman correlations: systolic blood pressure and infarct volume: p = 0.15 r: –0.317; diastolic blood pressure and infarct volume: p = 0.738 r: –0.76.
Supplementary Material to accompany: Traffic Noise Inhibits Cognitive Performance in a Songbird from Traffic noise inhibits cognitive performance in a songbird
Creators: name: Osbrink, Alison
name: Meatte, Megan A.
name: Tran, Alan
name: Herranen, Katri K.
name: Lilliann Meek
name: Murakami-Smith, May
name: Jacelyn Ito
name: Some Bhadra
name: Nunnenkamp, Carrie
name: Templeton, Christopher N.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 170299 Cognitive Science not elsewhere classified
subject: FOS: Psychology
subject: 60801 Animal Behaviour

description: Additional data tables, and figures showing photos of the methods used for each type of cognitive task
Microstructure evolution and composition redistribution of FeCoNiCrMn high entropy alloy under extreme plastic deformation
Creators: name: Yu, Pengfei
name: Fan, Ningsong
name: Zhang, Yongyun
name: Wang, Zhijun
name: Li, Wenya
name: Lupoi, Rocco
name: Yin, Shuo
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: The microstructure and composition evolution of FeCoNiCrMn high entropy alloy during extreme deformation with a strain rate of 108–109 s−1 induced by cold spray technology was investigated. In the region experiencing extremely large strain and high strain rate deformation, ultrafine nanograins with an average size of smaller than 100 nm were formed due to the occurrence of dynamic recrystallization. Additionally, the rapid redistribution of segregated Mn and Ni elements in extremely deformed FeCoNiCrMn was found for the first time. The reason for this phenomenon is the increased grain boundary area and dislocation density caused by extreme plastic deformation. The redistribution of Mn and Ni elements was found in extremely deformed FeCoNiCrMn. This finding enriches our knowledge on the microstructure evolution mechanism of high entropy alloys under extreme deformation.
title: ÐÐµÑÐ¾Ð´Ñ ÑÐ°ÑÐºÑÑÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐ¸ÑÐºÐ°Ñ Ð² ÑÐ¾ÑÑÐ°Ð²Ðµ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð³Ð¾ Ñ Ð¾Ð»Ð´Ð¸Ð½Ð³Ð°
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, Ð.
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (Ð ÐÐ¡ÐâÐ­â2018) (2018; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2018

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title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ³Ð¸Ð½Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±ÑÐµÐºÑ
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Search for very low-mass brown dwarfs and free-floating planetary-mass objects in Taurus
Creators: name: Quanz, Sascha P.
name: Goldman, Bertrand
name: Henning, Thomas
name: Brandner, Wolfgang
name: Burrows, Adam
name: Hofstetter, Lorne W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The number of low-mass brown dwarfs and even free floating planetary mass objects in young nearby star-forming regions and associations is continuously increasing, offering the possibility to study the low-mass end of the IMF in greater detail. In this paper, we present six new candidates for (very) low-mass objects in the Taurus star-forming region one of which was recently discovered in parallel by Luhman et al. (2009). The underlying data we use is part of a new database from a deep near-infrared survey at the Calar Alto observatory. The survey is more than four magnitudes deeper than the 2MASS survey and covers currently ~1.5 square degree. Complementary optical photometry from SDSS were available for roughly 1.0 square degree. After selection of the candidates using different color indices, additional photometry from Spitzer/IRAC was included in the analysis. In greater detail we focus on two very faint objects for which we obtained J-band spectra. Based on comparison with reference spectra we derive a spectral type of L2+/-0.5 for one object, making it the object with the latest spectral type in Taurus known today. From models we find the effective temperature to be 2080+/-140 K and the mass 5-15 Jupiter masses. For the second source the J-band spectrum does not provide a definite proof of the young, low-mass nature of the object as the expected steep water vapor absorption at 1.33 micron is not present in the data. We discuss the probability that this object might be a background giant or carbon star. If it were a young Taurus member, however, a comparison to theoretical models suggests that it lies close to or even below the deuterium burning limit (<13 Jupiter masses) as well. A first proper motion analysis for both objects shows that they are good candidates for being Taurus members.
description: 32 pages incl. 9 Tables, 12 Figures, accepted for publication by ApJ
title: Standing Committee on the Law of Trademarks, Industrial Designs and Geographical Indications :
title: Report adopted by the Special Session of the Standing Committee.
titleType: Subtitle
Creators: name: (:Unas)
Publisher: name: Unknown
Year: 0

description: In accordance with the decision of the WIPO General Assembly at its meeting in September 2001 (document WO/GA/27/8) that the Standing Committee on the Law of Trademarks, Industrial Designs and Geographical Indications (SCT) hold two special sessions on the Report of the Second WIPO Internet Domain Name Process (the “Special Sessions”), the first such Special Session was held in Geneva from November 29, 2001, to December 4, 2001.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð² Ð³. ÐÐµÑÑÐ¾Ð·Ð°Ð²Ð¾Ð´ÑÐºÐµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð°Ð»Ð°ÐµÐ²Ð°, ÐÐ°ÑÑ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: Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ð°
ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ
Ð¾ÑÐºÐ»Ð¾Ð½ÐµÐ½Ð¸Ðµ ÑÐ°ÑÑÐ¾ÑÑ
Ð¾ÑÐºÐ»Ð¾Ð½ÐµÐ½Ð¸Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
Ð½ÐµÑÐ¸Ð¼Ð¼ÐµÑÑÐ¸Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
ÐºÐ¾Ð¼Ð¿ÐµÐ½ÑÐ°ÑÐ¾Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð² Ð³. ÐÐµÑÑÐ¾Ð·Ð°Ð²Ð¾Ð´ÑÐºÐµ. ÐÐ»Ñ ÑÑÐ¾Ð³Ð¾ ÑÐºÐ°Ð·Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð² Ð³. ÐÐµÑÑÐ¾Ð·Ð°Ð²Ð¾Ð´ÑÐºÐµ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³Ð¸Ð¸ ÑÐ¸ÑÑÐµÐ¼ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ°ÑÐµÑÑÐ²Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿ÐµÐ½ÑÐ°ÑÐ¾ÑÐ¾Ð² ÑÐµÐ°ÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸.
The Evolution of the Stellar Mass Function of Galaxies from z=4.0 and the First Comprehensive Analysis of its Uncertainties: Evidence for Mass-dependent Evolution
Creators: name: Marchesini, Danilo
name: van Dokkum, Pieter G.
name: Schreiber, Natascha M. Forster
name: Franx, Marijn
name: Labbe', Ivo
name: Wuyts, Stijn
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: [Abridged] We present the evolution of the stellar mass function (SMF) of galaxies from z=4.0 to z=1.3 measured from a sample constructed from the deep NIR MUSYC, the FIRES, and the GOODS-CDFS surveys, all having very high-quality optical to mid-infrared data. This sample, unique in that it combines data from surveys with a large range of depths and areas in a self-consistent way, allowed us to 1) minimize the uncertainty due to cosmic variance and empirically quantify its contribution to the total error budget; 2) simultaneously probe the high-mass end and the low-mass end (down to ~0.05 times the characteristic stellar mass) of the SMF with good statistics; and 3) empirically derive the redshift-dependent completeness limits in stellar mass. We provide, for the first time, a comprehensive analysis of random and systematic uncertainties affecting the derived SMFs. We find that the mass density evolves by a factor of ~17(+7,-10) since z=4.0, mostly driven by a change in the normalization Phi*. If only random errors are taken into account, we find evidence for mass-dependent evolution, with the low-mass end evolving more rapidly than the high-mass end. However, we show that this result is no longer robust when systematic uncertainties due to the SED-modeling assumptions are taken into account. Taking our results at face value, we find that they are in conflict with semi-analytic models of galaxy formation. The models predict SMFs that are in general too steep, with too many low-mass galaxies and too few high-mass galaxies. The discrepancy at the high-mass end is susceptible to uncertainties in the models and the data, but the discrepancy at the low-mass end may be more difficult to explain.
description: 33 pages, 22 figures. Accepted for publication in the Astrophysical Journal. Version revised according to referee's comments; figures updated accordingly
Confinement Mechanism in the Field Correlator Method
Creators: name: Simonov, Yu. A.
name: Shevchenko, V. I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Confinement in QCD is caused by vacuum fluctuations of gluon fields. There are two numerically different scales, characterizing nonperturbative QCD vacuum dynamics: a "small" scale, corresponding to gluon condensate, critical temperature etc, which is about 0.2-0.3 GeV, and a "large" one, given by inverse confining string width, glueball and gluelump masses etc, which is about 1.5-2.5 GeV. We discuss this mismatch in a picture where confinement is ensured by two-point gauge-invariant field strength correlator of special type. It supports most of perturbative and nonperturbative dynamics, while contribution of other terms is argued to be small. This object, on the other hand, can be expressed via gluelump Green's function, whose dynamics is defined in terms of the same correlator. In this way one obtains a self-consistent scheme of mean-field type leading to permanent confinement at temperatures less than the critical one.
description: LaTeX, 33 pages, 6 figures
title: ÐÐ¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ° Ð½Ð° ÑÐ·ÑÐºÐµ C# Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ð¾Ð² Ð½Ð° Ð±Ð¸Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸ÑÑ
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´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¸Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ðµ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ðµ
ÐºÑÐ¸Ð¿ÑÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»
ÑÐ·ÑÐº C#

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ð±Ð·Ð¾ÑÐ° ÐºÑÐ¸Ð¿ÑÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ð¾Ð², Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð½ÑÑ Ð½Ð° Ð±Ð¸Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸ÑÑ, Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð½Ð° ÑÐ·ÑÐºÐµ Ð¡# Ð´Ð»Ñ Ð¸Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ°Ð»ÐµÐµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÐºÑÐ°ÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ.
Hot stars observed by XMM-Newton I. The catalog and the properties of OB stars
Creators: name: Naze, Yael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Aims : Following the advent of increasingly sensitive X-ray observatories, deep observations of early-type stars became possible. However, the results for only a few objects or clusters have until now been reported and there has been no large survey comparable to that based upon the ROSAT All-Sky Survey (RASS). Methods : A limited survey of X-ray sources, consisting of all public XMM observations (2XMMi) and slew survey data (XMMSL1), is now available. The X-ray counterparts to hot, massive stars have been searched for in these catalogs. Results : About 300 OB stars were detected with XMM. Half of them were bright enough for a spectral analysis to be possible, and we make available the detailed spectral properties that were derived. The X-ray spectra of O stars are represented well by low (<1keV) temperature components and seem to indicate that an absorption column is present in addition to the interstellar contribution. The X-ray fluxes are well correlated with the bolometric fluxes, with a scatter comparable to that of the RASS studies and thus larger than found previously with XMM for some individual clusters. These results contrast with those of B stars that exhibit a large scatter in the L_X-L_BOL relation, no additional absorption being found, and the fits indicate a plasma at higher temperatures. Variability (either within one exposure or between multiple exposures) was also investigated whenever possible: short-term variations are far more rare than long-term ones (the former affects a few percent of the sample, while the latter concerns between one third and two thirds of the sources). Conclusions : This paper presents the results of the first high-sensitivity investigation of the overall high-energy properties of a sizable sample of hot stars.
description: 10 pages, 4 figures, accepted for publication by A&A
Nano-bio interactions in mRNA nanomedicine: Challenges and opportunities for targeted mRNA delivery
Creators: name: Tao, Wei
Publisher: name: Health Research Alliance
Year: 2025
Subjects: classificationCode: 400302
subject: Biomaterials

description: Upon entering the biological milieu, nanomedicines swiftly interact with the surrounding tissue fluid, subsequently
being enveloped by a dynamic interplay of biomacromolecules, such as carbohydrates, nucleic acids, and cellular metabolites, but with predominant serum proteins within the biological corona. A notable consequence of the protein corona phenomenon is the unintentional loss of targeting ligands initially designed to direct nanomedicines toward particular cells or organs within the in vivo environment. mRNA nanomedicine displays high demand for specific cell and tissue-targeted delivery to effectively transport mRNA molecules into target cells, where they can exert their therapeutic effects with utmost efficacy. In this review, focusing on the delivery systems and tissue-specific applications, we aim to update the nanomedicine population with the prevailing and still enigmatic paradigm of nano-bio interactions, a formidable hurdle in the pursuit of targeted mRNA delivery.
We also elucidate the current impediments faced in mRNA therapeutics and, by contemplating prospective
avenues—either to modulate the corona or to adopt an ’ally from adversary’ approach—aim to chart a course for
advancing mRNA nanomedicine.
Quantum quenches in the anisotropic spin-1/2 Heisenberg chain: different approaches to many-body dynamics far from equilibrium
Creators: name: Barmettler, Peter
name: Punk, Matthias
name: Gritsev, Vladimir
name: Demler, Eugene
name: Altman, Ehud
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: Recent experimental achievements in controlling ultracold gases in optical lattices open a new perspective on quantum many-body physics. In these experimental setups it is possible to study coherent time evolution of isolated quantum systems. These dynamics reveal new physics beyond the low-energy properties usually relevant in solid-state many-body systems. In this paper we study the time evolution of antiferromagnetic order in the Heisenberg chain after a sudden change of the anisotropy parameter, using various numerical and analytical methods. As a generic result we find that the order parameter, which can show oscillatory or non-oscillatory dynamics, decays exponentially except for the effectively non-interacting case of the XX limit. For weakly ordered initial states we also find evidence for an algebraic correction to the exponential law. The study is based on numerical simulations using a numerical matrix product method for infinite system sizes (iMPS), for which we provide a detailed description and an error analysis. Additionally, we investigate in detail the exactly solvable XX limit. These results are compared to approximative analytical approaches including an effective description by the XZ-model as well as by mean-field, Luttinger-liquid and sine-Gordon theories. This reveals which aspects of non-equilibrium dynamics can as in equilibrium be described by low-energy theories and which are the novel phenomena specific to quantum quench dynamics. The relevance of the energetically high part of the spectrum is illustrated by means of a full numerical diagonalization of the Hamiltonian.
description: 28 pages
title: Investigating the impact of lung cancer cell-of-origin on tumour metabolic phenotype and heterogeneity
Creators: name: Caldera-Quevedo, Irene
Publisher: name: University of Glasgow
Year: 2024

description: Non-small-cell lung cancer has been described as highly heterogenous which results in different metabolic phenotypes. There are multiple factors which contribute to this heterogeneity, one of which is the tumour cell-of-origin. In the lung, there are five cell types reported to be cells-of-origin: alveolar epithelial type 2, club, basal, neuroendocrine and bronchioalveolar stem cells. This project focuses on the interaction between the cell-of-origin and the metabolic phenotype of lung cancer, and we aim to assess the contribution of the cell-of-origin to lung cancer metabolic resultant phenotype and heterogeneity.

To accomplish this, we have established two complementary model systems, one in vitro and one in vivo. In our in vitro model, we isolated specific lung cell types, including AT2 cells, basal cells, and club cells, utilising their unique cell surface markers. By introducing oncogenic KRAS mutations and deleting the P53 gene, we are creating lineage-restricted organoids. These organoids will serve as valuable tools for characterizing the metabolic aspects of tumours arising from different cell-of-origin backgrounds within an in vitro setting.

In our in vivo model, we induced NSCLC tumours in mice with genetic modifications using viral vectors, namely Ad5-mSPC-Cre, Ad5-CC10-Cre, and Ad5- bk5-Cre. These vectors are selectively expressed in AT2, club, and basal cells, respectively. To ensure the validity of our comparisons, we have carefully monitored tumour growth dynamics and burden in these mouse models. Our comprehensive analysis has revealed three distinct transcriptomic subtypes (S1, S2, and Acetate) within these NSCLC tumours. Notably, S1 and Acetate subtypes are enriched in tumours originating from specific cell types. Positron emission tomography (PET) imaging has unveiled metabolic variations, with S1 tumours displaying heightened [18F]FDG uptake and the Acetate subtype exhibiting increased [11C]acetate uptake. Furthermore, our multi-omics approach, encompassing transcriptomics, proteomics, and metabolomics, has exposed disparities in critical metabolic pathways, such as glycolysis, hypoxia response, and apoptosis.

In summary, our research provides a comprehensive examination of the metabolic heterogeneity of NSCLC based on the cell-of-origin independently of genomic alterations.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¾ÑÐ° Ð¼ÐµÑÐµÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÐ°Ð½Ð°Ð»Ð° ÑÐ°Ð´Ð¸Ð¾ÑÐ²ÑÐ·Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°ÐºÑÐ¾Ð½Ð¾Ð²Ð°, 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: 2018
Subjects: Ð Ð°Ð´Ð¸Ð¾ÑÐ²ÑÐ·Ñ Ð¼ÐµÑÐµÐ¾ÑÐ½Ð°Ñ
ÐÐ¾Ð´Ñ
Ð¢ÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸

description: Ð ÑÐ¾Ð´Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ Ð¼Ð¾Ð´ÐµÐ¼ Ð´Ð»Ñ Ð¼ÐµÑÐµÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°Ð´Ð¸Ð¾ÑÐ²ÑÐ·Ð¸. ÐÑÐ¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐµ Ð² ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½Ð¾Ð¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÐµÑÑÑ Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ°Ð´ÑÐ¾Ð² ÐºÐ°Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð¸ Ð¿Ð°ÐºÐµÑÐ¾Ð² ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ. ÐÐ»Ñ ÐºÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ Ð¿Ð¾Ð»ÑÑÐ½ÑÐµ ÐºÐ¾Ð´Ñ ÑÐµÑÑÑÐµÑ Ð²Ð¸Ð´Ð¾Ð² ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸. ÐÐ°Ð»ÐµÐµ ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑÑÑ ÐºÐ²Ð°Ð´ÑÐ°ÑÑÑÐ½ÑÐµ Ð¾ÑÑÑÑÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÑÑ Ð½Ð° Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ SDR-Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ. ÐÐ¾Ð·Ð¼Ð¾Ð¶Ð½Ð° Ð¿ÐµÑÐµÐ´Ð°ÑÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ñ ÐºÐ°Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾ÑÐ¾ÑÑÑÑ Ð´Ð¾ 10 ÐÐ±Ð¸Ñ/Ñ. ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»ÑÑ Ð²ÐµÑÐ°ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÐµÐ¶Ð¸Ð¼ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Â«ÑÐ¾ÑÐºÐ°-ÑÐ¾ÑÐºÐ°Â». Ð Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¾ÑÐ° ÐºÐ°Ð½Ð°Ð»Ð° Ð¼ÐµÑÐµÐ¾ÑÐ½Ð¾Ð¹ ÑÐ²ÑÐ·Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐ¸Ð¹ Ð½Ð°ÐºÐ¾Ð¿Ð»ÐµÐ½Ð½ÑÐµ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð´Ð°Ð½Ð½ÑÐµ Ð¾Ð± Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°Ñ ÑÐ»ÐµÐ´Ð¾Ð². ÐÐ°ÑÐµÐ¼ Ðº Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼Ñ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¾ÑÑ Ð¿Ð¾Ð´ÐºÐ»ÑÑÐ°Ð»Ð¸ÑÑ Ð´Ð°Ð½Ð½ÑÐµ Ñ ÑÑÐ°ÑÑÐ¾Ð²ÑÑ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹, ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ðµ Ð´Ð°Ð½Ð½ÑÐµ Ð¾Ð± Ð¸Ð½ÑÐµÑÐ²Ð°Ð»Ðµ Ð¼ÐµÐ¶Ð´Ñ ÑÐ»ÐµÐ´Ð°Ð¼Ð¸, Ð¸Ñ Ð´Ð»Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð¸ÐºÐ¾Ð²Ð¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸, Ð¸ ÑÐ°ÐºÐ¶Ðµ Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¾ÑÐ°.
Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼Ð¸ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾ Ð¿ÑÐ¸Ð½ÑÑÑÑ Ð¿Ð°ÐºÐµÑÐ¾Ð², ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿Ð°ÐºÐµÑÐ¾Ð² Ñ Ð¾ÑÐ¸Ð±ÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾Ð¹ ÑÑÐ¼Ð¼Ñ Ð¸ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿Ð°ÐºÐµÑÐ¾Ð² Ñ Ð¾ÑÐ¸Ð±ÐºÐ¾Ð¹ Ð´ÐµÐºÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¸ÑÑÐ¼ Ð´Ð°Ð½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð´Ð»Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¹ ÐºÐ°Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾ÑÐ¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÐºÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑ Ð²ÑÐ±ÑÐ°ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¼ÐµÑÐµÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°Ð´Ð¸Ð¾ÑÐ²ÑÐ·Ð¸ Ð´Ð»Ñ Ð¼Ð°ÐºÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ¸ÑÑÑÑÐµÐ¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐºÐ¾ÑÐ¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸.
Vacuum polarization by a cosmic string in de Sitter spacetime
Creators: name: de Mello, E. R. Bezerra
name: Saharian, A. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this paper we investigate the vacuum polarization effect associated with a quantum massive scalar field in a higher dimensional de Sitter spacetime in the presence of a cosmic string. Because this investigation has been developed in a pure de Sitter space, here we are mainly interested on the effects induced by the presence of the string. So this analysis is developed by expressing the complete Wightman function as the sum of two terms: The first one corresponds to the bulk where the cosmic string is absent and the second one is induced by the presence of the string. By using the Abel-Plana summation formula, we show that for points away from the string the latter is finite at the coincidence limit and it is used to evaluate the vacuum averages of the square of the field and the energy-momentum tensor induced by the cosmic string. Simple asymptotic formulae are obtained for these expectation values for points near the string and at large distances from it. It is shown that, depending on the curvature radius of de Sitter spacetime, two regimes are realized with monotonic and oscillatory behavior of the vacuum expectation values at large distances.
description: 18 pages, 2 figures, discussion on string metric in static coordinates is added
title: ÐÐ¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° ÐºÐ°Ðº ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼Ñ ÑÐ·ÑÐºÑ Ð² Ð²ÑÐ·Ðµ
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¡ÐµÐ²Ð¾ÑÑÑÑÐ½Ð¾Ð²Ð°, 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Ð¸Ð½ÑÐ¸Ð¿ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ÑÑÐ¸
ÑÐµÐ¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ð²Ð½Ð°Ñ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ÑÑÑ
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ÑÑÐµÐ´ÑÑÐ²Ð° Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ÑÑÐ¸ ÑÑÐµÐ±Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÑÐµÐ´ÑÑÐ² Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð£ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ñ Ð²Ð¸Ð·ÑÐ°Ð»ÑÐ½ÑÐµ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, ÑÑÐµÐ´ÑÑÐ²Ð°, ÑÑÐ½ÐºÑÐ¸Ð¸ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð° Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ðµ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿Ð¾ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼Ñ ÑÐ·ÑÐºÑ.
Manuel de l'observateur en criées et sur les lieux de débarquement
Creators: name: Ifremer, Equipe ObsVentes
Publisher: name: Ifremer
Year: 2025

description: Ce manuel détaille les missions d’observation dans les criées et sur les lieux de débarquement et se veut un guide opérationnel pour l’observateur sur le terrain. Il décrit les tâches à réaliser et les résultats attendus
ALSPAC Mother during pregnancy and the puerperium_data abstraction instructions
Creators: name: Birmingham, Karen
name: Gregory, Steven
name: Iles-Caven, Yasmin
name: Fraser, Abigail
name: Lawlor, Deborah
name: Boyd, Andrew
name: Northstone, Kate
name: Golding, Jean
Publisher: name: figshare
Year: 2021
Subjects: subject: 111706 Epidemiology
subject: FOS: Health sciences

description: ALSPAC Obstetric data abstraction instructions
Metal-Absorption Column Densities in Fast Radiative Shocks
Creators: name: Gnat, Orly
name: Sternberg, Amiel
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we present computations of the integrated metal-ion column densities produced in the post-shock cooling layers behind fast, radiative shock-waves. For this purpose, we have constructed a new shock code that calculates the non-equilibrium ionization and cooling; follows the radiative transfer of the shock self-radiation through the post-shock cooling layers; takes into account the resulting photoionization and heating rates; follows the dynamics of the cooling gas; and self-consistently computes the initial photoionization state of the precursor gas. We discuss the shock structure and emitted radiation, and study the dependence on the shock velocity, magnetic field, and gas metallicity. We present a complete set of integrated post-shock and precursor metal-ion column densities of all ionization stages of the elements H, He, C, N, O, Ne, Mg, Si, S, and Fe, for shocks with velocities of 600 and ~2000 km/s, corresponding to initial post-shock temperatures of 5e6 and 5e7 K, cooling down to 1000 K. We consider shocks in which the magnetic field is negligible (B=0) so that the cooling occurs at approximately constant pressure ("isobaric"), and shocks in which the magnetic pressure dominates everywhere such that the cooling occurs at constant density (isochoric). We present results for gas metallicities Z ranging from 1e-3 to twice the solar abundance of heavy elements, and we study how the observational signatures of fast radiative shocks depend on Z. We present our numerical results in convenient online figures and tables, available at http://wise-obs.tau.ac.il/~orlyg/shocks/
description: 32 pages, 29 figures. ApJ in press. Electronic data available at http://wise-obs.tau.ac.il/~orlyg/shocks/
Simulation dynamique du voilier
Creators: name: Roncin, Kostia
name: Kobus, Jean-Michel
Publisher: name: arXiv
Year: 2010
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: A sailing simulator has been developed from a new point of view. It will rather be for the sailor to use it than for the architect. One boat which characteristics were already known has been chosen. The whole coupled mechanic equations system has been solved. Heave and pitch equations, usually neglected, have been introduced to evaluate each trim of the crew and provide an optimal ride analysis tool. In this paper, efforts models and their determination's method are briefly presented. A tack simulation is shown as a brief overview on the simulator possibilities.
Maymena Gertsch 1960
Creators: name: Miller, Jeremy
name: Griswold, Charles
name: Yin, Chang
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Mysmenidae
Maymena

description: Genus Maymena Gertsch, 1960 Maymena Gertsch, 1960: 30. Type species Nesticus mayanus Chamberlin & Ivie, 1938 (= Maymena mayana (Chamberlin & Ivie, 1938)). Natural History. Chinese Maymena build horizontal orb webs with some extraplanar lines, similar to those known from the Appalachian region of North America (P. Paquin, pers comm.; see Coddington 1986b, fig. 22; Griswold et al. 1998, fig. 3B; Lopardo and Coddington 2005, fig. 40.16). This is the first record of Maymena from beyond the Americas. Paracymbium homology. Theridiosomatids are the only symphytognathoids with a distinct paracymbium (Griswold et al. 1998, but see Schütt 2003, Wunderlich 2004). The basal apophysis in some mysmenids (Figs 17B, 24C) and the hook-like cymbial apophysis in Maymena (Fig. 55) resemble a paracymbium, but are on the prolateral side, not the retrolateral side. However, the mysmenid palp is rotated so that the bulb sits on top of the cymbium rather than hanging down from it (i.e., the apophysis arises from the morphologically retrolateral face of the cymbium). Thus, the mysmenid cymbial apophyses could arise from the same part of the cymbium as the paracymbium after all. Possible paracymbium homologues in the Mysmenidae should be investigated as the phylogenetic structure of the family becomes better understood.
description: Published as part of Miller, Jeremy, Griswold, Charles & Yin, Chang, 2009, The symphytognathoid spiders of the Gaoligongshan, Yunnan, China (Araneae: Araneoidea): Systematics and diversity of micro-orbweavers, pp. 9-195 in ZooKeys 11 (11) on page 55, DOI: 10.3897/zookeys.11.160, http://zenodo.org/record/576459
description: {"references": ["Gertsch WJ (1960) Descriptions of American spiders of the family Symphytognathidae. American Museum Novitates 1981: 1 - 40.", "Coddington JA (1986 b) The monophyletic origin of the orb web. In Shear, WA (Ed) Spiders. Webs. Behavior, and Evolution. Stanford University Press, Stanford, 319 - 363.", "Griswold CE, Coddington JA, Hormiga G, Scharff N (1998) Phylogeny of the orb-web building spiders (Araneae, Orbiculariae: Deinopoidea, Araneoidea). Zoological Journal of the Linnean Society 123: 1 - 99.", "Lopardo L, Coddington JA (2005) Mysmenidae. In Ubick, D, P Paquin, CE CushingV Roth (Ed) Spiders of North America: An Identification Manual. American Arachnological Society, 377.", "Schutt K (2003) Phylogeny of Symphytognathidae s. l. (Araneae, Araneoidea). Zoologica Scripta 32: 129 - 151.", "Wunderlich J (2004) The fossil spiders of the family Anapidae s. l. (Aeaneae) [sic] in Baltic, Dominican and Mexican amber and their extant relatives, with the description of the new subfamily Comarominae. Beitrage zur Araneologie 3: 1020 - 1111."]}