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DAFTAR ISIImplementasi Content-Based Retrieval Pada Perpustakaan Digital Berbasis Open Source Menggunakan Apache Lucene David Pages: 1-13Perancangan Sistem Kendali Otomatik Proses Pengolahan Limbah Cair Tahu Berbasis Mikrokontroler AT89S52Barita Bram Ardiwinata Putra Pages: 14-25Analisis Penerapan Arsitektur Wireless LAN Menggunakan Top Down Approach pada PT. Telkom Pontianak Sandy Kosasi Pages: 26-42Sistem Intelijen Bisnis Global untuk Perencanaan e-commerce Budi Susilo Pages: 43-52Understanding e-Business & e-Commerce and Their Relation to the Conceptual framework of e-Marketing: Case Study Alexander Harsono Pages: 53-68Analisis dan Perancangan Aplikasi Persediaan pada CV. Fajar Khatulistiwa Motor PontianakSusanti Margaretha Kuway Pages: 69-79Analisis Penerapan Aplikasi Sistem Akuntansi Persediaan Menggunakan Technology Acceptance Model (TAM) pada Distrik Navigasi Kelas III PontianakSlamet Sugiarto, Rusmanto Lianto Pages: 80-94Implementasi Web Services Sistem Integrasi Data Menggunakan Teknik Replikasi Data Pada Inventarisasi Bangunan Pemerintah Ilhamsyah Pages: 95-10

Extreme multiplex spectroscopy at wide-field 4-m telescopes

We describe the design and science case for a spectrograph for the prime focus of classical 4-m wide-field telescopes that can deliver at least 4000 MOS slits over a 1 degree field. This extreme multiplex capability means that 25000 galaxy redshifts can be measured in a single night, opening up the possibilities for large galaxy redshift surveys out to z~0.7 and beyond for the purpose of measuring the Baryon Acoustic Oscillation (BAO) scale and for many other science goals. The design features four cloned spectrographs and exploits the exclusive possibility of tiling the focal plane of wide-field 4-m telescopes with CCDs for multi-object spectroscopic purposes. In ~200 night projects, such spectrographs have the potential to make galaxy redshift surveys of ~6 million galaxies over a wide redshift range and thus may provide a low-cost alternative to other survey routes such as WFMOS and SKA. Two of these extreme multiplex spectrographs are currently being designed for the AAT (NG1dF) and Calar Alto (XMS) 4-m class telescopes. NG2dF, a larger version for the AAT 2 degree field, would have 12 clones and at least 12000 slits. The clones use a transparent design including a grism in which all optics are smaller than the clone square subfield so that the clones can be tightly packed with little gaps between the contiguous fields. Only low cost glasses are used; the variations in chromatic aberrations between bands are compensated by changing one or two of the lenses adjacent to the grism. The total weight and length is smaller with a few clones than a unique spectrograph which makes it feasible to place the spectrograph at the prime focus.Comment: 8 pages, 4 figures, to appear in proceedings of Astronomical Telescopes and Instrumentation, SPIE conference, Marseille, 23-28 June, 200

Human fibroblast interferon RNA transcripts of different sizes in poly(I).poly(C) induced cells

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Photonic lantern behaviour and implications for instrument design

Photonic lanterns are an important enabling technology for astrophotonics with a wide range of potential applications including fibre Bragg grating OH suppression, integrated photonic spectrographs and fibre scramblers for high resolution spectroscopy. The behaviour of photonic lanterns differs in several important respects from the conventional fibre systems more frequently used in astronomical instruments and a detailed understanding of this behaviour is required in order to make the most effective use of this promising technology. To this end we have undertaken a laboratory study of photonic lanterns with the aim of developing an empirical model for the mapping from input to output illumination distributions. We have measured overall transmission and near field output light distributions as a function of input angle of incidence for photonic lanterns with between 19 and 61 cores. We present the results of this work, highlight the key differences between photonic lanterns and conventional fibres, and illustrate the implications for instrument design via a case study, the design of the PRAXIS spectrograph. The empirical photonic lantern model was incorporated into an end-to-end PRAXIS performance model which was used to optimise the design parameters of the instrument. We describe the methods used and the resulting conclusions. The details of photonic lantern behaviour proved particularly important in selecting the optimum on sky field of view per fibre and in modelling of the instrument thermal background.Comment: 18 pages, 14 figures, presented at SPIE Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation 2014, to be published in Proc. SPIE 915

Design and construction of the IMACS-IFU, a 2000-element integral field unit

The IMACS-IFU is an Integral Field Unit built for the IMACS spectrograph at the Magellan-I-Telescope at Las Campanas Observatory. It consists of two rectangular fields of 5 by 7 arcseconds, separated by roughly one arcminute. With a total number of 2000 spatial elements it is the second largest fiber-lenslet based IFU worldwide, working in a wavelength range between 400 and 900 nm. Due to the equally sized fields classical background subtraction, beam switching and shuffling are possible observation techniques. One particular design challenge was the single, half a metre long curved slit in combination with a non telecentric output. Besides the construction some preliminary results are described.Comment: 10 pages, 7 figures, 1 table. Proceedings for SPIE poster 5492-175 of SPIE Symposium "Astronomical Telescopes and Instrumentation", June 2004, Glasgo

Introduction of a pseudo-6th order ISDN splitter with bandstop topology

A newly developed ‘integrated services digital network’ (ISDN) splitter with bandstop (BS) topology is presented and compared to an actual ISDN splitter with a traditional lowpass (LP) topology. The LP-to-BS topology change reduced the amount of filter stages: a LP ISDN splitter requires an 8th order elliptic-like filter in order to be compliant to the standard ‘TS 101 952-1-4 V1.1.1’ [1] of the European Telecommunications Standards Institute (ETSI), whereas the BS ISDN splitter only needs a pseudo-6th order elliptic-like filter. The design of the new BS ISDN filter is discussed in the light of the enforced ETSI specifications. Furthermore, both the ISDN splitters are compared in the field of their specific stopband performance and their physical implementation. The area reduction that comes together with the introduction of the new ISDN splitter with BS topology is more than 25%

Rainforests : seqüència didàctica per l'aula AICLE inclusiva

La Seqüència Didàctica Rainforests va ser dissenyada i experimentada per l'equip col·laboratiu CLIL-SI dins dels projectes ARIE2004-00058 i ARIE2005-10056 (ArtICLE), finançats pel DURSI (Generalitat de Catalunya). El treball de disseny i recerca a l'aula desenvolupat ha donar lloc a un conjunt de material didàctic, treballs de recerca i publicacions

Dual-Channel Multi-Purpose Telescope

A dual-channel telescope allows for a wide-field telescope design wit h a good, narrow field channel of fewer surfaces for shorter-wavelen gth or planet-finding applications. The design starts with a Korsch three-mirror-anastigmat (TMA) telescope that meets the mission criter ia for image quality over a wide field of view. The internal image a t the Cassegrain focus is typically blurry due to the aberration bala ncing among the three mirrors. The Cassegrain focus is then re-optim ized on the axis of the system where the narrow field channel instru ment is picked off by bending the primary mirror

Replica Placement on Bounded Treewidth Graphs

We consider the replica placement problem: given a graph with clients and nodes, place replicas on a minimum set of nodes to serve all the clients; each client is associated with a request and maximum distance that it can travel to get served and there is a maximum limit (capacity) on the amount of request a replica can serve. The problem falls under the general framework of capacitated set covering. It admits an O(\log n)-approximation and it is NP-hard to approximate within a factor of $o(\log n)$. We study the problem in terms of the treewidth $t$ of the graph and present an O(t)-approximation algorithm.Comment: An abridged version of this paper is to appear in the proceedings of WADS'1