... Bojan Nikolic web pages (r. 329) . ... Atmospheric Modelling for ALMA . This is a short and simple illustration of how to use (A)ATM to calculate the dispersive path delay introduced by the atmosphere as well as the non-dispersive parts. ... Compute dispersive delay in the atmosphere This program is part of AATM version 0.06 GPL license -- you have the right to the source code. ... Computing dispersive atmospheric delay with AATM . ... Computing atmospheric absorption with AATM . ...

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• Computing dispersive atmospheric delay with AATM
• Computing atmospheric absorption with AATM Bojan Nikolic web pages (r. 329)
• Computing atmospheric absorption with AATM

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• A Method for Minimizing Background Offset Errors When Creating Mosaics
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• TwoFitlines: An Spectrum and Line Analysis Tool

... Abstract Return the number of radians per degree. Required_Reading None. Brief_I/O The function returns the number of radians per degree. ... Detailed_Output The function returns the number of radians per degree: pi/180. ... Examples The code fragment below illustrates the use of rpd_c . ... Author_and_Institution W.L. Taber (JPL) I.M. Underwood (JPL) E.D. Wright (JPL) . ... Version -CSPICE Version 1.0.0, 08-FEB-1998 (EDW) . Index_Entries radians per degree . Link to routine source . ...

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• CSPICE Routines: OSCELT_C
• CSPICE Routines: HALFPI_C
• CSPICE Routines: PI_C

... CentralProcessor 0.11 documentation . ... It can be run with the following command, where ?config.in? is a file containing the configuration parameters described in the next section. ... Parset parameters understood by ccontsubtract are given in the following table (all parameters must have CContSubtract prefix, i.e. CContSubtract.dataset ). ... A number of other parameters allowing the user to narrow down the data selection are understood. ... Parameter . ... Data set file name to work with. ...

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• Australia Telescope National Facility
• Host Command-Line Interface
• Cosmological Parameter Survey Using the Gravitational Lensing Method

makeprfcorr -- Compute the pixel response function for an image created with asncombine makeprfcorr association . association . ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...

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• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)

Next: Equations of condition Up: Extinction and transformation Previous: Extinction and transformation . Bias can also be introduced by improper fitting procedures. For example, the reduction program known as SNOPY, used for many years at La Silla and also at La Palma, uses a simple iterative technique in which some subsets of the parameters are solved for, while others are held fixed; then the ones last solved for are held fixed, while the ones previously fixed are redetermined. ...

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• Documentation: LEDA: parameter: mod0
• Documentation: LEDA: parameter: vopt
• Line parameter measurements

... Extend the Observation Data File summary file with data extracted from the instrument housekeeping datasets. ... Parameters . ... Errors . ... Input Files . ... Observation/ Slew Record . File Details Record . Instrument Details Record . Exposure Record . EPIC MOS Configuration Record . EPIC p-n Configuration Record . EPIC Radiation Monitor Configuration Record . RGS Configuration Record . OM Configuration Record . Proposal Summary Record . Data Quality Record . ...

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• EPIC source finding thread: step by step

... I determine th as a time period (from some moment in the past till the present moment) during which papers responsible for 1/2 of the total citation index were published. Parameter Nt represents averaging of the citation index over this period: Nt = C.I./2th 1 Intro duction The problem of estimation of an impact of a scientist (or a group of them) is an actual one (see, for example, [1] and references therein). ... One published in 1965 a paper with C.I.=5000, and nothing after that. ...

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• http://xray.sai.msu.ru/~polar/html/publications/citation/citation2.ps
• Parameters of binary compact star evolution
• Initial Distributions of Binary Parameters

System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

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• The Chirplet Transform: Physical Considerations
• The new precision concept
• The Frequency-Frequency (FF) Plane

Find Similar Abstracts (with default settings below ) . ... Also-Read Articles . ... Parameters of the 41 Dra system components . ... 00/2001 . ... Stars: Binaries, Binaries: Fundamental Parameters, Binaries: Individual . ... 61B Based on spectral and speckle-interferometric observations of the system 41 Dra, model atmosphere parameters of the system components have been derived: component Aa - T eff = 6500K, lg g = 3.99, R = 1.87 R solar , component Ab - T eff = 6500K, lg g = 4.11, R = 1.61 R solar . ...

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• Determination of atmospheric parameters and calculation of chemical composition
• Plug-and-Play-HOWTO : Tell the Driver the Configuration
• Spectral energy distribution

... Mokhovaya st., 11, Moscow, 103907, Russia. ... Proceedings of the 6th IEEE International Specialist Workshop on Nonlinear Dynamics of Electronic Systems, Budapest, Hungary, 16-18 July, 1998 , pp. ... The method for synchronization of drive-response systems on conditions of a large mismatch of parameters is considered on example of the system based on modified Chua's circuit. The approach to information transmission using such method is proposed. ...

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• Getting Started in Actor Prolog. Oil Production.
• Getting Started in Actor Prolog. Analyzing Web Sites.

Computer Ephemeris for 2014 from DE200/LE200. Orbital parameters of the Sun. Date Mean Perigee Mean Paral Aberrat Epsilon Nutat longitude longitude anomaly Dec 24 272.6887 283.1787 349.5100 8.941 20.832 2326 6.72 -8.19 Jan 3 282.5451 283.1792 359.3660 8.943 20.837 6.71 -8.18 13 292.4016 283.1796 9.2220 8.942 20.834 6.76 -8.11 23 302.2581 283.1801 19.0780 8.935 20.818 6.87 -7.99 Feb 2 ...

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• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2016 (DE200/LE200).

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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• SCL Sfit SYN Commands
• Sfit Control Language: Classified Listing
• lte-codes: sterne model atmospheres

Detecting Variations in Source Intensity for Poisson Data Y. Yu, XL. Meng, D. van Dyk, V. Kashyap, and A. Zezas Abstract The analysis of light curves is an especially challenging statistical task for low-count Poisson data: Variation in the source intensity may be shadowed by the Poisson variation of the counts. Here we discuss a class of statistical models that are designed to capture trends and autocorrelations in Poisson data that are collected over time. ... Example: A downward trend? . ...

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• Determine a background subtracted radial profile
• The AstroStat Slog nuisance parameter
• Comments on: Grating Dispersion [Equation of the Week] By: vlk By: hlee

Authors: T.V. Borkova , V.A. Marsakov , . ... It is found that dispersions of spatial and kinematics characteristics of field stars change abruptly when the metallicity crosses the boundary [Fe/H] -0.95 . ... По опубликованным прецизионным наземным и спутниковым измерениям собственных движений, компилятивным лучевым скоростям и фотометрическим расстояниям вычислены компоненты пространственных скоростей и элементы галактических орбит для 174 переменных звезд типа ab RR Лиры околосолнечной окрестности. ...

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• MONTE-CARLO
• Population of Galactic globular clusters, tabl

polimplot -- Plot a polarization vector map . ... inpol = "" [name] . Input linear polarization image (in %) to plot. inpopa = "" [name] . Input image for position angle of linear polarization vectors (degrees). poi_err = "" [boolean] . ... Name of corresponding polarization position angle error image (degrees). ... This task is a flexible tool for plotting a polarization vector map from two images of the polarization and the position angle of the polarization vector. ...

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• Preparation of parameter file
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• Beam procedures and functions

The pdev spectrometer dshift parameter (see layout of spectrometer scaling ) down shifts the output of the power computation before accumulating the spectral values in the 40 bit accumulators. ... As an example: a 1 second integrations at 170 MHz with: (A/D=48,pshift=0x1555, dshift=0,ashift=0) has LO feedthrough birdies close to 1.5e9. The maximum allowed value is 4e9. ... The allowable range for dshift had been computed from the spectral mean with dshift = 0 (see page 2 of the plots) . ...

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• AGES Database Search
• Orbits in the period / acceleration plane
• Converting Arecibo Interim Correlator data into a FITS image

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/history.htm
• Determination of the Detector Parameters

ON THE IMPACT OF THE GALACTIC ABERRATION ON VLBI-DERIVED PRECESSION MODEL Z.M. MALKIN Pulkovo Observatory Pulkovskoe Ch. ... Corrections to adopted precession rate are usually computed from the linear trends in long-term time series of celestial pole offset (CPO), which are the differences between the measured and the theoretical coordinates of the celestial pole. ... CONCLUSIONS We have estimated the impact of GA on parameters of precession-nutation model derived from VLBI observations. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm09b.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm09a.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/huang.pdf

... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...

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• Further Information and Bibliography
• CREATE FULLTEXT CONFIGURATION
• ALTER FULLTEXT ... OWNER