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1 H THumaniora & Teologi Pedagogisk inspirationskonferens för ht-områdets lärare 21 september 2010 TEXTKOMPENDIUM 2 FÖRORD: Förord ..................................................................................................................................................................................... 3 av Lynn Åkesson - Dekanus område humaniora och teologi, Lunds universitet. PROGRAM: P
1 A History of A4. A History of Automatic Control C.C. Bissell Automatic control, particularly the application of feedback, has been fundamental to the devel- opment of automation. Its origins lie in the level control, water clocks, and pneumatics/hydraulics of the ancient world. From the 17th century on- wards, systems were designed for temperature control, the mechanical control of mills, and th
Total pages of required readings (marked with *): 746 Total pages of student-selected readings (chosen from the below list): 350 Total pages of reading required by students in the course: 1096 Abraham, I. 2020. “Host Communities and Refugees in Southeast Asia: Report on a Workshop held at the National University of Singapore (NUS), 10-11 May 2019.” Sojourn: Journal of Social Issues in Southeast As
https://www.historiska.lu.se/media/utbildning/dokument/kurser/COSM33/20242/COSM33_literature_list.pdf - 2026-05-03
The Judiciary and the Zimbabwean Constitution Edited by James Tsabora The Judiciary and the Zimbabwean Constitution Edited by James Tsabora University of Zimbabwe Press Supported by: © University of Zimbabwe Press, 2022 Editor: James Tsabora (PhD) Assistant Editors: Professor Julie Stewart and Dr Innocent Maja Main Funding Organisation: Swedish International Development Cooperation Agency through
https://rwi.lu.se/wp-content/uploads/2022/09/The-Judiciary-and-the-Zimbabwean-Constitution.pdf - 2026-05-03
We present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed when at least two of the three LIGO-Virgo detectors are in coincident operation, with a total observation time of 207 days. The analysis searches for transients of duration less than or similar to 1 s over the frequency ba
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo observations between July 7, 2009, and October 20, 2010. We searched for signals from binaries with total mass between 2 and 25M(circle dot); this includes binary neutron stars, binary black holes, and binaries consisting of a black hole and neutron star. The detectors were sensitive to systems up t
We present the results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs. We perform two distinct searches: a modeled search for coalescences of either two neutron stars or a neutron star and black hole, and a search f
We present the first multi-wavelength follow-up observations of two candidate gravitational-wave (GW) transient events recorded by LIGO and Virgo in their 2009-2010 science run. The events were selected with low latency by the network of GW detectors (within less than 10 minutes) and their candidate sky locations were observed by the Swift observatory (within 12 hr). Image transient detection was
Aims. The detection and measurement of gravitational-waves from coalescing neutron-star binary systems is an important science goal for ground-based gravitational-wave detectors. In addition to emitting gravitational-waves at frequencies that span the most sensitive bands of the LIGO and Virgo detectors, these sources are also amongst the most likely to produce an electromagnetic counterpart to th
Aims. A transient astrophysical event observed in both gravitational wave (GW) and electromagnetic (EM) channels would yield rich scientific rewards. A first program initiating EM follow-ups to possible transient GW events has been developed and exercised by the LIGO and Virgo community in association with several partners. In this paper, we describe and evaluate the methods used to promptly ident
This paper presents results of an all-sky search for periodic gravitational waves in the frequency range [50, 1190] Hz and with frequency derivative range of similar to[-20, 1.1] x 10(-10) Hz s(-1) for the fifth LIGO science run (S5). The search uses a noncoherent Hough-transform method to combine the information from coherent searches on time scales of about one day. Because these searches are ve
We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20, 20)M-circle dot coalescence was 300 Mpc. No gravitational wave signals w
A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical origin. This background is a target for the current generation of ground-based detectors. In this article we present the first joint search for a stochastic background using data from the LIGO and Virgo interferometers.
We present the results of a weakly modeled burst search for gravitational waves from mergers of nonspinning intermediate mass black holes in the total mass range 100-450 M-circle dot and with the component mass ratios between 1: and 4:1. The search was conducted on data collected by the LIGO and Virgo detectors between November of 2005 and October of 2007. No plausible signals were observed by the
We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6 x 10(-9) Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10x increase in computational efficienc
Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational-wave detectors. Gravitational radiation encodes rich information about source physics; thus parameter estimation and model selection are crucial analysis steps for any detection candidate events. Detailed models of the anticipated waveforms enable inference on several param
Between 2007 and 2010 Virgo collected data in coincidence with the LIGO and GEO gravitational-wave (GW) detectors. These data have been searched for GWs emitted by cataclysmic phenomena in the universe, by non-axisymmetric rotating neutron stars or from a stochastic background in the frequency band of the detectors. The sensitivity of GW searches is limited by noise produced by the detector or its
Microsoft Word - kappan060807.doc Karlstad University Studies ISSN 1403-8099 ISBN 91-7063-059-3 Faculty of Social and Life Sciences Nursing science DISSERTATION Karlstad University Studies 2006:28 Linda J. Kvist Care and treatment of women with inflammatory symptoms of the breast during lactation Care and treatment of women with inflammatory symptoms of the breast during lactation Inflammation of
https://www.vetenskaphalsa.se/wp-content/uploads/2011/07/Linda-Kvist-doktoravhandling.pdf - 2026-05-03
Microsoft Word - Katarina_Dahlenborg.doc Cellular and Molecular Aspects of the Germinal Centre Reaction Katarina Dahlenborg Lund 1998 Katarina Dahlenborg Dept. of Immunotechnology Lund University PO Box 7031 S-220 07 Lund, Sweden © 1998 Katarina Dahlenborg ISBN 91-628-3080-5 Printed by Bloms i Lund Tryckeri AB, Lund, Sweden ”At ville forstå naturens finmekanik ved hjælp af vores praktiske tankevan
https://www.immun.lth.se/fileadmin/immun/Avhandlingar/Katarina_Dahlenborg.pdf - 2026-05-02
We present the results of the first search for gravitational wave bursts associated with high energy neutrinos. Together, these messengers could reveal new, hidden sources that are not observed by conventional photon astronomy, particularly at high energy. Our search uses neutrinos detected by the underwater neutrino telescope ANTARES in its 5 line configuration during the period January - Septemb
