247 research outputs found
The Functioning of the Mufti Institution in Bulgaria at the Beginning of the 20th Century. A Case Study
Autor analizuje działalność muftich, jednej z najważniejszych instytucji administracji muzułmańskiej w Bułgarii w okresie Trzeciego stanu (1878–1944). Przedstawione zostały trzy przypadki: Afiza M. Mustafowa, Afiz Suleymanova i Sali Effendiego, które ilustrują szereg zjawisk związanych z funkcjonowaniem muzułmańskich autonomicznych instytucji w Bułgarii na przełomie XIX i XX w. Studia przypadków oparte są na materiałach z Centralnego Archiwum Państwowego Bułgarii w Sofii. The author analyses the functioning of the muftis in Bulgaria, one of the most important institution of the Muslim religious-administrative autonomy in that Balkan country during the Third State period (1878–1944). The presented three cases of Afiz M. Mustafow, Afiz Suleymanov, and Sali Effendi illustrated series of phenomenon linked to the functioning of mufti and Muslim autonomous institutions in Bulgaria in the turn of the 19th and 20th century. The case studies are based on the materials from the Central State Archive of Bulgaria in Sofia
The Functioning of the Mufti Institution in Bulgaria at the Beginning of the 20th Century. A Case Study
Autor analizuje działalność muftich, jednej z najważniejszych instytucji administracji muzułmańskiej w Bułgarii w okresie Trzeciego stanu (1878–1944). Przedstawione zostały trzy przypadki: Afiza M. Mustafowa, Afiz Suleymanova i Sali Effendiego, które ilustrują szereg zjawisk związanych z funkcjonowaniem muzułmańskich autonomicznych instytucji w Bułgarii na przełomie XIX i XX w. Studia przypadków oparte są na materiałach z Centralnego Archiwum Państwowego Bułgarii w Sofii. The author analyses the functioning of the muftis in Bulgaria, one of the most important institution of the Muslim religious-administrative autonomy in that Balkan country during the Third State period (1878–1944). The presented three cases of Afiz M. Mustafow, Afiz Suleymanov, and Sali Effendi illustrated series of phenomenon linked to the functioning of mufti and Muslim autonomous institutions in Bulgaria in the turn of the 19th and 20th century. The case studies are based on the materials from the Central State Archive of Bulgaria in Sofia
A Computational Network Model for Shared Mental Models in Hospital Operation Rooms
This paper describes a network model for mental processes making use of shared mental models (SMM) of team performance. The paper illustrates the value of adequate SMM’s for safe and efficient team performance. The addressed application context is that of a medical team performing a tracheal intubation executed by a nurse and a medical specialist. Simulations of successful and unsuccessful team performance have been performed, some of which are presented. The paper discusses potential further elaborations for future research as well as implications for other domains of team performance.Information managementSafety and Security Scienc
ديوان باقی. Le recueil des poésies de Baki, ou ʿAbd el-Baki, qui fut successivement kadi de la Mecque, de Constantinople, sadr d'Anatolie, de Roumélie (m. 23 Ramadhan 1008 de l'hégire = 7 avril 1600).
Numérisation effectuée à partir d'un document original.Ce divan contient des kaside dédiées au sultan Soleïman II, à ʿAli Pacha, à Kobad Pacha, au mufti Abous-Soʿoud, les ghazels rangés alphabétiquement, suivis de kitʿa et de pièces mineures. Manuscrit de luxe, orné de deux sarlohs enluminés en or et en bleu.Gaulmin
ein Beitrag zum Dialog im Offenen Brief an Papst Benedikt XVI
In der vorliegenden Arbeit begibt sich die Autorin auf eine einzigartige Tauchreise in das islamische Denken. Sie betrachtet die größeren Fragen des interreligiösen und kulturellen Dialogs zwischen Christentum und Islam, sowie die Grundlagen, auf denen dieser Dialog nach Vorstellungen muslimischer Religionsexperten geführt werden sollte. Der Reiseführer ist Prof. Dr. Peter Heine, deutscher Islamwissenschaftler. Um die Wende des interreligiösen und kulturellen Dialogs einzuleiten, legen die berühmtesten Gelehrten der islamischen Welt, darunter Großscheich von Al-Azhar Prof. Dr. Tantawi, der ägyptische Gelehrte und Politiker Dr. Zakzouk, Großmufti von Ägypten Dr. Ali Gomaa, Großmufti von Mauretanien Dr. Ibn Bayyah, sowie Großmufti von Syrien Dr. Hassoun, zum ersten Mal die Grundzüge eines wahrhaften, ernsten und erfolgreichen Dialogs zwischen der westlichen und islamischen Welt nieder. Die „Regensburger Rede“ des Papst Benedikt XVI im Jahr 2006, der darauffolgende offene Brief von 38 muslimischen Gelehrten an den Papst, sowie der Text der Botschaft aus Amman sind die Grundsteine zur Herstellung einer friedlichen, solidarischen Welt, in der ein offener geistiger Austausch gefördert und gegenseitiges Verständnis gefordert wird.An unique trip into the Islamic thought. Using the ship of humanity the present work dives into the largest issues of the inter-religious and cultural dialogue between Christianity and Islam, as well as the basics on which this dialog should be conducted according to the ideas of famous Muslim religious experts. The guide is Dr. Peter Heine, the famous German Islamic scholar. For the first time, the most famous scholars of the Islamic world, including Grand Sheikh of Al-Azhar, Grand Mufti of Egypt Dr. Ali Gomaa, Dr. Zazouk, minister of higher religious organization, Grand Mufti of Mauritania Dr. Ibn Bayyah, Grand Mufti of Syria Dr. Hassoun and others draw the basic principles of a successful and honest dialogue between the Western and Islamic world in order to live in a solidaric and peaceful world to restore the turn of interreligious and intercultural dialog
TOI 560 : Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS and HIRES RVs
We validate the presence of a two-planet system orbiting the 0.15--1.4 Gyr K4 dwarf TOI 560 (HD 73583). The system consists of an inner moderately eccentric transiting mini-Neptune (TOI 560 b, days, ) initially discovered in the Sector 8 \tess\ mission observations, and a transiting mini-Neptune (TOI 560 c, days) discovered in the Sector 34 observations, in a rare 1:3 orbital resonance. This moderate eccentricity for TOI 560 b is from the detection of the photoeccentric effect in the spitzer light curve. We utilize photometric data from \tess\, \textit{Spitzer}, and ground-based follow-up observations to confirm the ephemerides and period of the transiting planets and vet false positive scenarios. We obtain follow-up spectroscopy and corresponding precise radial velocities (RVs) with the iSHELL spectrograph at the NASA Infrared Telescope Facility and the HIRES Spectrograph at Keck Observatory to validate the planetary nature of these signals, which we combine with published PFS RVs from Magellan Observatory. We place upper limits on the masses of both planets of 2.1 and 4.1 M for b and c, respectively. We apply a Gaussian Processes (GP) model to the \tess\ light curves to place priors on a chromatic radial velocity GP model to constrain the stellar activity of the TOI 560 host star. TOI 560 is a nearby moderately young multi-planet system with two planets suitable for atmospheric characterization with James Webb Space Telescope (JWST) and other upcoming missions. In particular, it will undergo six transit pairs separated by 6 hours before June 2027
Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: A planet in the radius gap?
Bluhm, P., Luque, R., Espinoza, N., Pallé, E., Caballero, J.A., Dreizler, S., Livingston, J.H., Mathur, S., Quirrenbach, A., Stock, S., Van Eylen, V., Nowak, G., López, E.D., Csizmadia, S., Zapatero Osorio, M.R., Schöfer, P., Lillo-Box, J., Oshagh, M., González-Álvarez, E., Amado, P.J., Barrado, D., Béjar, V.J.S., Cale, B., Chaturvedi, P., Cifuentes, C., Cochran, W.D., Collins, K.A., Collins, K.I., Cortés-Contreras, M., Díez Alonso, E., El Mufti, M., Ercolino, A., Fridlund, M., Gaidos, E., García, R.A., Georgieva, I., González-Cuesta, L., Guerra, P., Hatzes, A.P., Henning, T., Herrero, E., Hidalgo, D., Isopi, G., Jeffers, S.V., Jenkins, J.M., Jensen, E.L.N., Kábath, P., Kaminski, A., Kemmer, J., Korth, J., Kossakowski, D., Kürster, M., Lafarga, M., Mallia, F., Montes, D., Morales, J.C., Morales-Calderón, M., Murgas, F., Narita, N., Passegger, V.M., Pedraz, S., Persson, C.M., Plavchan, P., Rauer, H., Redfield, S., Reffert, S., Reiners, A., Ribas, I., Ricker, G.R., Rodríguez-López, C., Santos, A.R.G., Seager, S., Schlecker, M., Schweitzer, A., Shan, Y., Soto, M.G., Subjak, J., Tal-Or, L., Trifonov, T., Vanaverbeke, S., Vanderspek, R., Wittrock, J., Zechmeister, M., Zohrabi, F
Transit Timing Variations for AU Microscopii b & c
We explore the transit timing variations (TTVs) of the young (22 Myr) nearby
AU Mic planetary system. For AU Mic b, we introduce three Spitzer (4.5 m)
transits, five TESS transits, 11 LCO transits, one PEST transit, one Brierfield
transit, and two transit timing measurements from Rossiter-McLaughlin
observations; for AU Mic c, we introduce three TESS transits. We present two
independent TTV analyses. First, we use EXOFASTv2 to jointly model the Spitzer
and ground-based transits and to obtain the midpoint transit times. We then
construct an O--C diagram and model the TTVs with Exo-Striker. Second, we
reproduce our results with an independent photodynamical analysis. We recover a
TTV mass for AU Mic c of 10.8 M. We compare the
TTV-derived constraints to a recent radial-velocity (RV) mass determination. We
also observe excess TTVs that do not appear to be consistent with the dynamical
interactions of b and c alone, and do not appear to be due to spots or flares.
Thus, we present a hypothetical non-transiting "middle-d" candidate exoplanet
that is consistent with the observed TTVs, the candidate RV signal, and would
establish the AU Mic system as a compact resonant multi-planet chain in a 4:6:9
period commensurability. These results demonstrate that the AU Mic planetary
system is dynamically interacting producing detectable TTVs, and the implied
orbital dynamics may inform the formation mechanisms for this young system. We
recommend future RV and TTV observations of AU Mic b and c to further constrain
the masses and to confirm the existence of possible additional planet(s).Comment: Corrected typos; revised Section 3, 4, and 5 to reflect reanalysis,
results unchanged. Submitted to AAS Journals Nov 11th, 2020; favorable
referee report received Jan 3rd; final draft accepted for publication in the
AJ Apr 19t
Advances in Tagging Methods for Lifetimes of Isomeric-and Proton-Unbound States
This paper summarises the programme of Recoil-isomer tagging that has been performed over the last ten years at the University of Jyvaskyla, Finland. The nuclei studied lie in the mass 130-140 region of the Segre chart very close to the proton drip line. The evolution of the isomer character is seen to change from K-isomers, at N=74, to shape-isomers in the gamma soft N=77 nuclei to seniority-isomers around N=82. The influence of the proton drip line on the N=74 isomers and possible critical-point symmetries in the N=77 nuclei are discussed and the latest results presented. Developments of the isomer-tagging technique, using large beam currents with a dual Mufti-Wire Proportional Counter setup, and an Isomer-tagged Differential-Plunger setup are discussed along with a future programme of work at Jyvaskyla
Advances in Tagging Methods for Lifetimes of Isomeric-and Proton-Unbound States
This paper summarises the programme of Recoil-isomer tagging that has been performed over the last ten years at the University of Jyvaskyla, Finland. The nuclei studied lie in the mass 130-140 region of the Segre chart very close to the proton drip line. The evolution of the isomer character is seen to change from K-isomers, at N=74, to shape-isomers in the gamma soft N=77 nuclei to seniority-isomers around N=82. The influence of the proton drip line on the N=74 isomers and possible critical-point symmetries in the N=77 nuclei are discussed and the latest results presented. Developments of the isomer-tagging technique, using large beam currents with a dual Mufti-Wire Proportional Counter setup, and an Isomer-tagged Differential-Plunger setup are discussed along with a future programme of work at Jyvaskyla
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