. Портал | Содержание | О нас | Авторам | Новости | Первая десятка | Дискуссионный клуб | Научный форум | Отправить открытку . Первая десятка "Русского переплета" Темы дня: . | Обращение к Дмитрию Олеговичу Рогозину по теме "космические угрозы": как сделать систему предупреждения? .
... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...
... Observations Com binati on of gridded point s and l ong int egrati on Data Reduction * * * * * * * * * * * * * * * * Map Type Grid Size Pixel Separation Integration Time Switch Frequency Bandwidth Resolution Pointed 8x8 3 45 s 3.125 MHz 12.5 MHz 0.08 km/s * * * * · Have on-sourc e and off-sourc e inform ati on · Sourc es of error Data Reduction (1-e-)=(Tm odel -Tsi gnal )/Ts ource Tspin= Tem/(1-e-) NH=1.823 x 10 18 Tspin (v) dv 1 Results Opaciti es - why di fferent? W esterbork GBT 2 ...
XMMNewton CCF Release Note XMMCCFREL231 EPIC canned response matrices M. Ehle July 11, 2007 1 Purpose The generated EPIC canned response matrix files (RMFs) are described and published on a ded icated web page at http://xmm.esac.esa.int/external/xmm sw cal/calib/epic files.shtml and allow the user to load them (together with source and background spectra of EPIC observations and related ancillary matrices) into spectral analysis packages like XSPEC for model fitting. ...
[
Текст
]
Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0231-1-0.ps.gz -- 61.7 Кб -- 11.07.2007 Похожие документы
This Directory contains mean daily values of geomagnetic field components at the Tbilisi Observatory (1880 - 1991). ... Information on the DUSHETI (TBILISI, GEORGIA) magnetic observatory Geograpic Geomagnetic Latitude 42 05' 36 31' longitude 44 42' 122 12' The long history of magnetic observations of Dusheti observatory is recor- ded on the PC-Disquette. On the floppy disk in the directory DUSHETI are written the elements of the Earth's magnetic field from 1880 to 1991. ...
... Решите систему уравнений м x5 + xy4 = y10 + y6 , п н6 2 3 п x + x = 8 y + 2y. о Решение. ... Функция y = f x возрастает (убывает) на промежутке I тогда и только тогда, когда для любых u и v из этого промежутка знаки чисел f u - f v и u v совпадают (соответственно, противоположны). ... Докажите, что совпадают знаки следующих чисел: б) u - v и u v; а) u - v и u2 - v2 ; в) au - av и u - v a - 1; г) loga u - loga v и u - v a - 1 ; д) a x - b и x - loga b a - 1 ; е) loga x - b и x - ab a - 1 . ...
... casa . ... const Double . ... the minimum single precision floating point number, including denormalised numbers . ... the maximum double precision floating point number . ... Minimum double precision floating point number X such that 1+X does not equal X. const Double . ... Minimum double precision floating point number X such that 1+X does not equal X. const Double casa::C::dbl_max . ... Minimum single precision floating point number X such that 1+X does not equal X. const Double casa::C::flt_max ...
... A printed version of this catalog with B1950 coordinates is available from the NRAO. ... This file b1950 .dat 79 15045 PMN catalog , B1950 coordinates j2000 .dat 79 15045 PMN catalog , J2000 coordinates -------------------------------------------------------------------------------- Byte-per-byte Description of file : b1950 .dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations ---- ...
... This file table1 97 1345 A catalog of positions, radial velocities and proper motions table2 36 19 Coordinates of Kapteyn's areas table3 64 30 List of suspected bynaries and variables ------------------------------------------------------------------- ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- N Kapteyn's area number 6- 18 A13 --- Name Star identification 21- 22 I2 h RAh ...
... E.V. Kazarovets, N.N . Samus , O.V. Durlevich, S.V. Antipin, M.S. Frolov, N.N . Kireeva, E.N. Pastukhova Institute of Astronomy of Russian Academy of Sciences and Sternberg State Astronomical Institute of ... the Moscow State University ================================================================================ The 74th Special Name-list of Variable Stars , A.V. Kazarovets, N.N . Samus , O.V. Durlevich, S.V. Antipin, M.S.,Frolov, ... 3323 Samus, N.N., IBVS, 1997, No. ...
The Texas survey of radio sources covering -35.5{deg} < {delta} < 71.5{deg} at 365MHz . ... We present the Texas Survey of discrete radio sources between -35.5deg and 71.5deg declination (B1950), which was carried out at 365MHz with the Texas Interferometer during 1974-1983. ... The Texas Survey . ... The sources in the simpler model. ... Right Ascension 1950 . ... field separator . ... Some sources came from Version 6 of the Texas Survey ('TS6' in strp field) or Version 7 ('TS7' in strp field) . ...
... Key words: X-rays: stars; stars: neutron; magnetic fields; line: formation. в 1 1+z (n = 0, 1, 2, . ... Line profiles are shown for a continuum spectrum of the form of a power law with a high-energy exponential cutoff f (E ) = const. в E - в exp (-E / ) (XSPECs cutoffpl) and for different cutoff energies. fit (Fig. 4, bottom) was obtained for cylinder geometry, revealing a magnetic field strength of B = 2.95 в 1012 G, a viewing angle of µ = 0.76 and the plasma electron temperature of k Te = 3.4 keV....
[
Текст
]
Ссылки http://hea.iki.rssi.ru/integral06/papers/G41_Schoenherr01-07Feb07_16:54:04.pdf -- 385.0 Кб -- 07.02.2007 Похожие документы
New GCVS Version (GCVS5) FileName Explanations ----------------------------------------------------------------- ReadMe This file GCVS5 The ... ------------------------------------------------------ 1- 2 I2 --- Constell [1/88]Constellation numeric code 3- 6 I4 --- Number Star number within the constellation 7 A1 --- Component *Component identification 9- 18 A10 --- GCVS * Variable ... Field is non-blank if magMin is a magnitude or amplitude given in a system other than that indicated by magCode. ...
A transputer based system for real-time processing of CCD astronomical images A.Balestra1 , C.Cumani1 , G.Sedmak1,2 , R.Smareglia 1 (1) Osservatorio Astronomico di Trieste (OAT), Italy (2) Dipartimento di Astronomia, Universita' di Trieste, Italy Octob er 27, 2006 Abstract A complete transputer based, real-time system has been developed to manage the whole chain of operations from acquisition of CCD images to quick-look, both in on-site observations and in remote observations. ...
... This file clusters .dat 173 32 The 32 clusters in the Southern SHARC sample selfn.dat 20 1092 Selection function for the Southern SHARC survey (as shown in Figure 7) fields.dat 98 66 ROSAT observations used in the Southern SHARC survey (Table A1) extsrcs.dat 112 96 All extended X-ray sources detected by the Southern SHARC survey (Table B1) numflux.dat 21 32 Number- flux points for Southern ... For clusters with pArea = 100, this amounts to multiplying the measured count rate by 1.25. ...