Chapter 10 Integrated Submm Wave Receiver : Development and Applications Valery P. Koshelets, Manfred Birk, Dick Boersma, Johannes Dercksen, Pavel Dmitriev, Andrey B. Ermakov ... S. Sobolev, Mikhail Yu Torgashin, Vladimir L. Vaks, Ed de Vries, Georg Wagner, and Pavel A. Yagoubov Abstract A superconducting integrated receiver ( SIR ) comprises in a single chip a planar antenna combined with a superconductor-insulator-superconductor (SIS) mixer, a superconducting ... 700 GHz/. ... Fig. ...
; Model file automatically generated from fm1.config medium gold begin ; gold index of refraction table ; < 100 eV from D.W. Lynch and W.R. Hunter, Optical Constants of Metals, ; in Handbook op Optical Constants of Solids, ed. E.D. Palik, ; Academic Press, Orlando, 1985. ; > 100 eV from an updated table from E. Gullikson ; E (eV) n k delta=1-n 0.125 12.24 54.7 -11.24 0.13 11.51 53.1 -10.51 0.135 10.84 51.6 -9.84 0.14 10.21 50.2 -9.21 0.145 9.582 48.8 -8.582 0.15 9.016 47.6 -8.016 0.155 8.5 46.4 -7.5 0.16
Computer Ephemeris for 2016 from DE200/LE200. Fundamental ephemeris of Mercury. Date alpha dif delta dif paral. radius distance dif upper_culm. h m s s o ' h m s Jan 1 200624.633 187.005 -210244.80 1327.58 9.55 3.65 0.92063901 -2609373 Date alpha dif delta dif paral. radius distance dif upper_culm. h m s s o ' h m s Feb 1 191255.610 158.680 -203521.55 -387.25 9.93 3.80 0.88570120 1813044 ...
... ARC 3.5m | TripleSpec . ... Fowler sampling, read noise, and minimum integration time . ... The integration time for the slit viewer is adjustable, but 30 seconds represents a maximum practical integration for positioning the source and for guiding. Longer integration times are possible, but the delay between exposures makes guiding and/or positioning the source on the slit tedious. ... Decide on your guider integration time and acquire a frame to serve as the background image with "Expose". ...
... 2006, A&A, 455, 107) are attributed to both an improvement of the local TFR and the more detailed accurate measurement of the rotation velocities in the distant sample. ... 2007). ... Results We compare both the distant and local K -band TFR in Fig. ... We reiterate that we assume no evolution in slope (see Sect. 4.1): a larger sample would be required to tackle directly the possible evolution in slope of the TFR and determine the details of the evolutionary path between distant and local RDs. ...
... For the first time this year, I have an image of EVERY supernova above magnitude 18.0. 2005nc (= GRB 050525A ), IAUC 8696 discovered 2005/05/30.28 by ESO type Ic Mag 24. 2005nb , IAUC 8657 discovered 2005/12/17.38 by Texas Supernova Search . ... 2005ky , IAUC 8636 discovered 2005/11/24.3 by Supernova Legacy Survey type Ia at mag 21.0 ( CSP/LCO image ) . ... 2005mx , ATEL 556 discovered 2005/07/01.5 by Nearby Supernova Factory type II Mag 19.4 ( Discovery image ) (References: CBET 344 , IAUC 8651 ) ....
... Structural Analysis of Disk Galaxies of the NGC 524 Group M. A. Il'ina and O. K. Sil'chenko * Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia Received February 24, 2012; in final form, March 2, 2012 Abstract--Members of the NGC 524 group of galaxies are studied using data obtained on the 6m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, with the SCORPIO reducer in an imaging mode. ... NGC 502. ... NGC 524. ... Rev. Astron. ...
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: 05 (08.01.1; 11.01.1; 11.05.2; 11.13.1; 11.19.4; 11.19.5) ASTRONOMY AND ASTROPHYSICS Age and metallicity for six LMC clusters and their surrounding field population B. Dirsch1 , T. Richtler2, W.P. Gieren2 , M. Hilker 1 2 3 3 Sternwarte der Universitat Bonn, Auf dem Hugel 71, 53121 Bonn, Germany ? ? Universidad de Concepcion, Departamento de FЄ Є isica, Casilla 160-C, Concepcion, Chile Є P. Universidad Catolica, Departamento de
Acta Materialia 53 (2005) 1597-1609 www.actamat-journals.com Comparative study of grain-boundary migration and grain-boundary self-diffusion of [0 0 1] twist-grain boundaries in copper by atomistic simulations B. Schonfelder a, G. Gottstein ? ... The behavior of atoms during grainboundary migration was analyzed for all studied GBs. ... case of [0 0 1] twist GBs in cubic materials recently. ... Misorientation dependence of the activation enthalpy of GB migration of the studied [0 0 1] twist GBs. ...
. 1. Цель работы . 2. Обновление исходных данных по сравнению с 1этапом . 2.1. Данные по источникам выброса . 2.2. Данные по метеорологии . 3. Методика . 3.1. Проблемы агрегации результатов . 3.1.1.Способы характеристики средней и максимальной опасности . 3.1.2.Влияние порядка агрегации на результат . 3.1.3.Проблема учета нулей и отсутствующих данных при агрегации . 3.2. Проблемы сшивки разных вариантов модели . 3.2.1.Сшивка расчетов по ОНД и ISC . 3.2.2.Сшивка разных пространственных и временных масштабов
EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH CERN-EP-2000-148 OPAL PR 328 30 Novemb er 2000 Precise Determination of the Z Resonance Parameters at LEP: "Zedometry" The OPAL Collaboration Abstract This final analysis of hadronic and leptonic cross-sections and of leptonic forward-backward asymmetries in e+ e- collisions with the OPAL detector makes use of the full LEP 1 data sample comprising 161 pb-1 of integrated luminosity and 4.5 Ч 106 selected Z decays. An interpretation of the data in terms of
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Ссылки http://zebu.uoregon.edu/~uochep/docs/docs00/pr328_journal.pdf -- 1264.4 Кб -- 23.05.2005 Похожие документы
# IBVS 5721-t1.txt #Author: Kazarovets, E.V.; Samus, N.N.; Durlevich, O.V.; Kireeva, N.N.; Pastukhova, E.N. #Comment: The 78th Name-List of Variable Stars, Table 1 #IBVSdataKey: name-list No. Name R.A., Decl., 2000.0 Max Min Type References h m s o ' " m m 780001 V956 Cas 00 05 05.4 +59 39 01 14.2 17.2 B IS: 001 002 780002 CD Scl 00 06 20.8 -35 17 13 12.7 14.2 V RRAB 130 004 780003 V439 And 00 06 36.8 +29 01 17 6.13 ( 0.04 ) V BY 005 DM 780004 V957 Cas 00 09 45.7 +50 30 39 11.6 12.8 * SR: 006 USNO 780005
RT And * CB EA RS 8.97 0.41 0.31 V 0.6289 v 170 000 170 000 F8V+K1 a 231110.1 +530133 SY And SA * EA 10.70 1.50 V 34.9085 060 027 A0+K1 001316.4 +434241 TT And * SA EA 11.50 1.50 0.10 V 2.7651 v 140 000 A+G7IV 231322.9 +460851 TW And * SA EA 8.98 2.06 0.15 V 4.1228 v 130 020 F0V+K0 000318.2 +325045 UU And SA EA 11.20 3.00 0.20 V 1.4863 v 170 000 A8IV/V 004345.1 +305620 WW And * SA EA 10.92 0.67 0.16 V 23.2852 050 000 000 A0:+G5-K0III 234453.5 +454112 WX And SA * EA 12.10 1.70 V 3.0011 d 120 030 F5IV
Mon. Not. R. Astron. Soc. 000, 1-?? (2002) Printed 16 novembre 2012 A (MN LTEX style file v2.2) A high-resolution spectropolarimetric survey of Herbig Ae/Be stars I. Observations and measurements E. Alecian1,2 , G.A. Wade2 , C. Catala1 , J.H. Grunhut ? T. Bohm6,7, C.P. Folsom5, S. Marsden8,9, I. Waite9 1 2 3 4 5 6 7 8 9 2,3 , J.D. Landstreet4,5 , S. Bagnulo5, LESIA-Observatoire de Paris, CNRS, UPMC Univ., Univ. Paris-Diderot, 5 place Jules Janssen, F-92195 Meudon Principal Cedex, France, Dept. of Physics,
ОСНОВНЫЕ ОРТОГОНАЛЬНЫЕ ФУНКЦИИ И ИХ ПРИЛОЖЕНИЯ ЧАСТЬ I. ОРТОГОНАЛЬНЫЕ ФУНКЦИИ ЭКСПОНЕНЦИАЛЬНОГО ТИПА УДК 517.587:519.216 Прохоров С.А., Куликовских И.М. Основные ортогональные функции и их приложения. Часть I. Ортогональные функции экспоненциального типа. Самара: Издательство Самарского научного центра РАН, 2013. 200 с. ISBN 978-5-93424-652-6 В первой части предлагаемой монографии рассматриваются ортогональные функции экспоненциального типа. Структура монографии разработана с учетом дальнейшего приложения к
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Ссылки http://www.ssau.ru/files/resources/sotrudniki/prohorov/osn_ortog_func.pdf -- 1658.8 Кб -- 09.09.2015 Похожие документы