... The system was recalibrated on 29may06 using 3C286 (24.3Jy at 430Mhz). 24 cross scans were done on the 430 yagi and 4 cross scans on the linefeed. ... The yagi feed adds the polarizations together. ... At the beginning of a set of crosses, the cal was fired for two seconds to measure Tsys. ... Fig 3 has the Gain and Tsys. ... The yagi gain on 12feb06 was about 8% higher than 29may06. ... Both the gain and Tsys being higher on 12feb06 points to the cal value changing by 8% from the 29may06 value. ...

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• http://www.naic.edu/~phil/calcb/meascalMay03/meascalMay03.html
• http://www.naic.edu/~phil/mbeam/ohspider/ohspiderscans_jul04.html
• http://www.naic.edu/~phil/calsbw/meascalSep01/meascalsep01.html

... This chapter discusses values that JavaScript recognizes and describes the fundamental building blocks of JavaScript expressions: variables and literals. ... So, for example, you could define a variable as follows: . var answer = 42 And later, you could assign the same variable a string value, for example, . ... These are fixed values, not variables, that you literally provide in your script. ... A string literal is zero or more characters enclosed in double ( " ) or single ( ' ) quotation marks. ...

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• Standard values
• worldCoords(3)
• Order Definition

... There are two types of STIS target acquisition: ACQ and ACQ/PEAK; for more details on target acquisition, see STIS ISR 97-03. ... The first is an image of the target in the target acquisition sub-array (100 x 100 pixels for POINT sources, user-defined for DIFFUSE sources) based on the initial pointing (see Figure 23.1 a), image_raw.fits[sci,1]. ... To verify that the ACQ/PEAK worked, examine the flux values at each stage of the peakup (listed in the paper products or in the data file). ...

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• http://www.stsci.edu/documents/dhb/webvol2/c15_hspdata.fm1.html
• CSPICE Routines: SCE2C_C
• COS Instrument Handbook

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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• Trigonometry beyond 90 degrees

Program: CORMAP Purpose: Check whether there is a correlation between two maps Category: ANALYSIS, CALCULATION File: cormap.c Author: M. Vogelaar Keywords: INSET= Give set, subsets: Maximum number of subsets is 2048. BOX= Give box: [entire subset] RANGE= Give range of levels to include in calculation: [all] Input consists of two values. The first value may be greater than the second. See the description for the correct use of this keyword. ... PGCOLOR= Give color 1.. ...

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• casacore: casa::Dummy_Constants_class Class Reference
• difx:vdifio [ATNF VLBI Wiki]
• mbspect

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• Comparing Means and Deviations
• Potential Energy

... static int . ... Plot (java.lang.String title, java.lang.String xLabel, java.lang.String yLabel, double[] xValues, double[] yValues) . ... void . ... This version of the constructor uses the default flags. public Plot (java.lang.String title, java.lang.String xLabel, java.lang.String yLabel, double[] xValues, double[] yValues, int flags) . ... public void addPoints (double[] x, double[] y, int shape) . ... Adds error bars to the plot. public void addLabel (double x, double y, java.lang.String label)...

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• FileInfo (ImageJ API)
• RoiDecoder (ImageJ API)
• CurveFitter (ImageJ API)

... XMM-Newton CCF Release XMM- CCF -REL-331 Page: 4 Table 1: Ratio of number of events in extracted spectra ( New /Current) Ob ject Obsid Rev RGS1 o1 RGS1 o2 RGS2 o1 RGS2 o2 PKS 2155-304 0411780301 1543 1.02 1.08 1.02 1.08 Mkn 421 0560980101 1640 1.02 1.08 1.02 1.08 Mkn 421 0560983301 1732 1.02 1.08 1.02 1.08 PKS 2155-304 0411780401 1734 1.03 1.09 ... XMM-Newton CCF Release XMM-CCF-REL-331 Page: 8 Figure 6: Evolution of the Parallel CTI (left RGS1, right RGS2...

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• Description
• Output Files

... Here is an example of the output header of CATS data. ... SIMPLE=T / BITPIX=8 / character information NAXIS=0 / no image data array present EXTEND=T / may be standard extensions OBJECT= CATS SEARCH / CATS search result ORIGIN=SAO RAS DATE=01/01/1997 / date of file creation END XTENSION=TABLE / F-file table extension BITPIX=8 / 8-bits ... NAXIS1=93 / No. of characters per row NAXIS2=1000 / the number of lines (sources) TFIELDS=10 / there are 16 fields per row EXTNAME= CATS / object name: ...

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• Advanced Pointer Topics
• Times Up!!
• di_eks

... Sea Surface Temperature, restored from NOAA satellite data . You may use Java applet to view temperature maps in more detail. Using the applet, you can build "accumulated" temperature maps from selected data, get temperature values in any point and save the resulting image to your local disk. Date and time of the data . ... 3.11.2007 . 19:10 (GMT) . ... For information send a mail to: info@sputnik.infospace.ru . ...

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• SPUTNIK, SST Black Sea . (Novorossiysk Region)

Ballistic life-time . ... The orbit inclination to the equatorial plane (black line) and to the ecliptic plane (red line) are shown on the third panel. ... The launch orbital elements value and its evolution during flight is shown on the plot for the time interval (August 3, 1995 - October 16 2000). ... The critical parameter is perigee altitude shown on the first panel. ... This parameter determine the IB_Tail ballistic lifetime up to October 16, 2000. ... Dated 25 May, 2000 . ... INTERBALL mission ...

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• Trigonometry beyond 90 degrees
• More on Kepler's Second Law
• Kepler's First Law of Planetary Motion

... This plug-in enables you to add various types of lighting effects to your (RGB) image. ... Directional light . ... Well, you get the idea :) The default settings for this light-type is [-0.5,-0.5,-1.0]. ... Higher values makes your image reflect a lot of light (appear lighter or more intense), while smaller values makes it appear more dull or matte. ... A value of 1.0 makes your image very shiny (bright high-lights) while smaller values makes you image less shiny, making the high-lights dimmer. ...

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• The Sparkle Plug-In: The Sparkle Dialog Box
• Creating a watermark effect
• GIMP: Channel Ops Tutorial

... The grid of values can be built around any parameter by explicitly giving the center point of the grid (in response to the model descriptor prompt). ... Please choose the grid axes: model componet number for the first axis (1): cr first axis parameter (norm|index|temp|galacticNh|intrinsicNh): temp half range of first axis parameter (0.4): 0.25 number of steps in the first axis (1:) (7): 5 model component number for the second axis (1): 2 second axis ...

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• Getting Common Information About Access Points
• Mapping Pixel Values to Screen Intensity
• The AstroStat Slog Blog Archive P Values: What They Are and How to Use Them

Next: Cyg X-1 as a Up: Black Holes in Binaries Previous: Black Hole Creation in . The discovery of binary radiopulsars with massive unseen companions ( >3- ) would be of great importance to fundamental physics and modern theory of stellar evolution, providing a compelling evidence for the existence of BH in nature. The formation of binaries consisting of a BH in a pair with a radiopulsar (PSR) has been discussed previously by Narayan et al. ... Здесь должна быть Table 11 (Note к Table 11) . ...

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... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Developer Documentation . ... In general, a hook function is one that Apache will call at some point during the processing of a request. ... Use the AP_DECLARE_HOOK macro, which needs to be given the return type of the hook function, the name of the hook, and the arguments. ... During initialisation, the server will call each modules hook registering function, which is included in the module structure: . ...

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• Hook Functions in the Apache HTTP Server 2.x - Apache HTTP Server
• Color Values
• mod_reqtimeout - Apache HTTP Server

Underdetermined sets is a new type of data structures (terms) developed in Actor Prolog . ... The point is that an underdetermined set can include some indefinite rest (a tail) like a list in usual Prolog . At the same time, the order of elements of an underdetermined set can be arbitrary one and it does not affect results of unification of underdetermined sets. Moreover, Actor Prolog guarantees that a rest of an underdetermined set never contains elements that are explicitly given in the set. ...

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• EIT Server Input File Format
• Online EIT reconstruction server
• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM-E\JAM-E.A"

... Flux Sign Expo . ... The map above is movable . The image is shown in significance with a squared root color map ranging from 0 to 25. ... Original shows mosaics with all data available. Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. ... Exposure maps are in ksec. INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... Galactic Bulge . ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ...

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Stellarium 0.12.3 . ... Classes . ... AngleSpinBox Class Reference . A spin box for displaying/entering angular values. More... #include < AngleSpinBox.hpp > . ... virtual voidљ . ... Set the value to default 0 angle. ... AngleSpinBox (QWidget *parent=0, DisplayFormat format= DMSSymbols , PrefixType prefix= Normal ) . ... Set the display format. ... the value to set, in decimal degrees. void AngleSpinBox::setDisplayFormat . ... the value to set, in radians. void AngleSpinBox::valueChanged . ...

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• Stellarium: gTime Class Reference
• Stellarium: Triplet< T > Struct Template Reference

Magnetic Stars, 2011, pp. 153 ­ 156 Ab out the Dep endence of the Rotation Velo city of CP Stars on the Magnetic Field Glagolevskij Yu. ... Based on the observational data of the average magnitudes of the surface magnetic field strength Bs for a number of chemically peculiar stars we investigate the dependence of the rotation period on the magnetic field. ... Now the periods of rotation P and the average values of the surface magnetic field Bs are known for more than 50 magnetic stars. ...

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• Detection of radio pulsar pairs
• Evidences of supercritical accretion onto black hole in SS433

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• Pointing error budget
• TUI:Telescope:Offset window
• TUI:Telescope:Slew Window:Options:Calibrate