... It plots visibilities (e.g. amplitude vs time), either one baseline at a time or all together, and allows discrepant points to be flagged with a cursor. ... No default. ... Key: axis Two character strings, giving the X and Y axes of the plot. Possible axis values are: time (the default for the X axis) lst Local apparent sidereal time. uvdistance sqrt(u**2+v**2) hangle (hour angle) channel (implies nofqav) amplitude (the default for the Y axis) phase real imaginary rms Theoretical rms noise. ...

... Focus Model . ... For a given time, this model estimates the amount of defocus at a particular camera. ... If you obtained focus model values from this site prior to May 23rd, for HST observations made after March 29th 2011, then obtaining those values again now will improve agreement with measurements. ... the average focus value over the time period requested (measured and/or modeled values as applicable). a link to a space-delimited text file containing Date, Julian date, Time, and Model value . ...

grdhisteq - Histogram equalization for grd files grdhisteq in _ grdfile [ -G out _ grdfile ] [ -C n _ cells ] [ -D ] [ -N [ norm ] ] [ -Q ] [ -V ] grdhisteq allows the user to find the data values which divide a given grdfile into patches of equal area. ... One could use grdhisteq to write to stdout an ASCII list of those data values which divide the range of the data into n _ cells segments, each of which has an equal area in the image. ... C Sets how many cells (or divisions) of data range to make. ...

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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... This noise can be reduced by replacing the pixels with an average of the surrounding values using a linear filter. ... The effects of applying linear filters to a CCD frame is shown in Figure . Figure: Different digital filters applied on a CCD image: (A) original, (B) block filter, (C) smooth filter, and (D) Laplacian filter. ... To remove stellar images from a picture of comet Halley, the results of applying different non--linear filters to the frame are given in Figure . ...

... FIELD | ... public class RoiDecoder . ... static int . ... Field Detail public static final int VERSION_OFFSET . ... public static final int TYPE . ... public static final int TOP . ... public static final int LEFT . ... public static final int BOTTOM . ... public static final int RIGHT . ... public static final int N_COORDINATES . ... public static final int X1 . ... public static final int STROKE_WIDTH . ... public static final int SHAPE_ROI_SIZE . ... public static final int STROKE_COLOR . ...

NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

... The Multiple Extension FITS (MEF) file interface is an IRAF library providing facilities for general file operations upon FITS multi-extension files. ... The Multiple Extensions FITS (MEF) interface consists of a number of routines to mainly read a FITS Primary Data Unit or an Extension Unit and manipulate the data at a file level. ... Read the FITS header of a MEF file that matches the EXTNAME or EXTVER keyword values or if not specified, read the extension number `group'. ... The header filename. ...

write a simple ASCII file containing pairs of x and y values. write a simple ASCII file containing pairs of x and y values. write a file containing pairs of x and y values in Spectrum format 2, including a header. read a file containing pairs of x and y values in Spectrum format 2, including a header. ... Compute cross-correlation function for functions y1(x1) and y2(x2) The result is returned as ccfy(ccfx) Apply a velocity correction to a wavelength array. v is in units of the speed of light. ...

... radardecode - decode radar data (ao) radardecode [ -dqrt ] [ -b bits ] [ -c codelen ] [ -l decodeFftlen ] [ -n numcodes ] [ -o offset ] [ -p numPol poltoUse ] [ -s samplesPerBaud ] [ -m machine ] [ -f freqShift_NotYetImplemented ] . ... The input data can be ri, cbr, or unpacked data (depending on the -m option). ... If cbr data is input then all polarizations are input to the program and the -p option is used to tell the number of polarizations input, and which polarization should be decoded. ...

... The models provided are: . abs - absorption of x-rays by neutral gas with solar abundances. parameter 1 = . ... parameter 2 = . ... normalization - logarithmic value of the flux density at 1 keV in units of keV cm -2 s -1 keV -1 . ... normalization - logarithmic value of the normalization of the gaussian in units of keV cm -2 s -1 . ... absorption ( params )* model ( params ) . ... A single value for the normalization (i.e., fixed normalization) will force the program to use that value. ...

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

... Module name: fftw_aux . ... This module is meant to be used in conjunction with the Fast Fourier Transform package fftw which comes with the sas. The module contains a header in which some useful variables are declared, as well as the following routine: . function findNextHighest2357multiple(i) result(result) integer, intent(in) :: i end function findNextHighest2357multiple . ... The fftw transform works most efficiently on arrays which have dimensions which are products of small primes. ...

tranback -- Transform an X,Y position from output to input pixel position using the same conventions as drizzle tranback xout yout . xout = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... If "output" the input image center is mapped to the center of the output grid, rotated about that center and then shifted along the grid of the output image. ...

This layer is defined with a <LAYER> tag. You see that the background color is applied to the rectangular region occupied by the layer. The height of the colored area is determined by the height value. This layer is defined in CSS syntax. The style definition sets the position and background color, but doesn't set any values for border characteristics. ... The style definition includes a value for border-width. ... The style definition includes a value for layer-background-color. ...

ntpdate [ -bBdosu ] [ -a key ] [ -e authdelay ] [ -k keyfile ] [ -o version ] [ -p samples ] [ -t timeout ] server [ ... ] . ntpdate sets the local date and time by polling the Network Time Protocol (NTP) server(s) given as the server arguments to determine the correct time. ... A number of samples are obtained from each of the servers specified and a subset of the NTP clock filter and selection algorithms are applied to select the best of these. ... The default is /etc/ntp.keys . ...

Pulkovo NEO Page . ... EPOS Software Package . ... EPOS ( E phemeris P rogram for O bjects of the S olar system) is the Windows PC application for study and ephemeris support of observations of the Solar system objects. ... It controls the part of common data and transfers the control to one of the programs that solve the restricted set of tasks. ... So with the EPOS software package one can calculate the accurate ephemerides for many objects and get the quick illustration of their motion as well. ...

... Source File: mod_negotiation.c . Module Identifier: negotiation_module Content negotiation, or more accurately content selection, is the selection of the document that best matches the clients capabilities, from one of several available documents. ... A type map (a file with the handler type-map ) which explicitly lists the files containing the variants. ... Apache only recognizes encodings that are defined by an AddEncoding directive. ... Content-Language: . ... Module: mod_negotiation . ...