On/off position switching on continuum sources was done at 2380 Mhz with the sband narrow receiver and the correlator. ... Use the total power information, cal values, and source flux to compute tsys, gain, sefd. Fit the data to a function of (az,za). ... Include losses from pitch, roll, and focus. ... Tsys - fit. ... These plots take a closer look at the average gain fit and how the azimuth terms of the fit compare to the azimuth terms of the gain loss computed from pitch,roll, and focus. ...

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• a2488 dps the 800Mhz rcvr.
• pdev_birdies_25jun07

... NB The next 2 columns will only be present if the parameter usecat has been set to true . ... Source parameters such as count-rates, magnitudes and semi-major axes, are given in sub-tables-eg the column CORR_RATE is actually a vector column containing the values for each filter. ... QUALITY FLAGS Each source has an associated ``quality flag''. ... 0 1 Source lies above one or more bad pixels . ... QFLAG The quality flag for each source in each filter obtained from the input source-lists. ...

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• SourceListFile
• Source Shape Parameterization
• Uniqueness of LABEL and INDEX values.

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

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• harak_e
• Mathematics: <math.h>

... User Guide ] Task: mfboot Purpose: Set the flux scale of a visibility dataset. Categories: calibration MFBOOT is a MIRIAD program that corrects the flux scale in visibility datasets. In doing this, it assumes that the flux density scale is out by a constant scale factor. ... Key: vis Input visibility datasets. ... Key: mode MFBOOT can process the data in one of three modes: "triple", "scalar" and "vector". ... In "triple" mode, MFBOOT compares the triple product of the data and model. ...

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• casacore: casa/Quanta/MVFrequency.h Source File
• casacore: casa/Quanta/MVDoppler.h Source File
• casacore: casa/Quanta/MVRadialVelocity.h Source File

... 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.fm3.html
• covar2ellipse.pro (JWST Pipeline routines in IDL)
• Python T5: 061405 script

... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

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• The COOC Criterion (Criterion of Observations versus Calculations)
• Population synthesis of X-ray sources at the Galactic center
• Evolution of the double neutron star merging rate and the cosmological origin

... SELECT file, title, rank(ts_vec, to_tsquery('create schema')) FROM postgresql_manual WHERE ts_vec @@ to_tsquery('create schema') ORDER BY rank(ts_vec, to_tsquery('create schema')) DESC LIMIT 5; file | title | ... CREATE SCHEMA | ... SELECT file, title, rank('{0, 0, 0.01, 0.99}',ts_vec_tb, to_tsquery('create aggregate')) FROM postgresql_manual WHERE ts_vec_tb @@ to_tsquery('create aggregate') ORDER BY rank('{0, 0, 0.01, 0.99}', ts_vec_tb, to_tsquery('create aggregate')) DESC LIMIT 5; file | ...

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• Lighting plug-in
• GIMP: Channel Ops Tutorial
• Using Channel Ops with GIMP

.

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... Clean . ... 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 | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ... Exposure . ...

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True Color Image Gallery: Galactic SNR | ... nH was dervide from central source. spectrum from central object . does not fit well in the low energy regime. derived nH is rather large compared to the value(2.5~2.6) given by Hughes et al.(1998) . ... reduce chi^2 = . ... DataSet 1: 329 data points -- 326 degrees of freedom. Statistic value = 384.565 . ... DataSet 1: 317 data points -- 314 degrees of freedom. ... Back to SNR J0526.0-6604 Index . Chandra Supernova Remnant Catalog . ...

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• The AstroStat Slog PDF
• The AstroStat Slog background
• Model Spectra for Spectral-Fitting Program

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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• SunSoft
• Explanations for solar physics computing page
• Assigning property values, Cascading, and Inheritance

home education > resources . ... Resources . ... Astronomy Education Bibliography . ... Black Holes: An Introductory Resource List . ... http://hubblesite.org/explore_astronomy/black_holes/home.html . ... The Universe in the Classroom (The ASP's Newsletter on Teaching Astronomy) Issue on Black Holes by John Percy: . ... For a set of black hole information guides and demonstration activities from the ASP's and JPL's Night Sky Network, click on the link below and check the box on black holes: . ...

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• ASP: Book Review
• ASP: Good Astronomy Activities on the WWW
• ASP: Astronomy Education: A Selective Bibliography

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... python . tcc . base . wrapperTestCase.py . ... 7 љ from tcc.base import AxisStateValDict, RotTypeNameDict . ... 13 љ def setUp (self): . ... 55 љ def checkCmdFail (self, cmdVar, shouldFail=False): . ... 64 љ def checkTrackResult (self, cmdVar, axisCmdState, . ... tcc.base.wrapperTestCase.WrapperTestCase.checkTrackResult . ... Definition: wrapperTestCase.py:70 . ... Definition: wrapperTestCase.py:113 . ... Definition: wrapperTestCase.py:100 . ...

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• lsst.tcc: python/tcc/util/runningStats.py Source File
• lsst.tcc: python/tcc/parse/getPVTList.py Source File
• lsst.tcc: python/tcc/parse/getRestart.py Source File

We have designed the laboratory model of static Fourier spectrometer for onboard usage for spectral study of atmosphere and ionosphere. The gain of model is to simulate onboard FS which will not have any moving elements (all its optical elements will be mounted at fused quartz monolithic construction), to compare experimental results with theoretical estimations and to measure MTF of CCD array. ... This fact connected with low frequency response of CCD array due to small format of it. ...

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... The standard science quicklook processing produces over a dozen sky maps at each downlink, and these maps are automatically searched for potential transient point sources. ... We have found that a heuristic modification of a formula derived by Li & Ma (1983) provides reasonably accurate estimates of p -values for point source detections even for very low p -value detections. ... Case 1u. The most straightforward approach uses the signal , where . ... To get a p -value, use . ...

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• ADASS 2003 Conference Proceedings
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• QPSIM: An IRAF/PROS Tool for Source Simulation

... Measured Radio Parameters for 116 extended sources without col.10 (T peak) and col.12(Ref.) ... An asterisk in byte 9 indicates that this line refers to the whole source or major parts of it (same as 'c' in byte 38) (1) (2) (3) (4) (5) (6) (7) (8) (9) (11) source Type RA1950 Dec1950 LAS PA Wmaj Wmin PA S_408 cmp h m s +-s d m s +-" (') deg (') (') comp Jy ----+----1----+----2----+----3----+----4----+----5----+----6----+----7- 0002+12 a M2 000208.1 0.3 +123232 9 3.5 105 1.5 ...

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• The ROSAT All-Sky Survey Faint Source Catalogue
• Optical spectroscopy of radio sources
• WSRT deep surveys

J/MNRAS/429/2080 Lockman Hole 10C sources radio spectral indices (Whittam+ 2013) ================================================================================ The faint source population at 15.7 GHz. ... 2011, Cat. ... 2008, Cat. ... For 10C sources without a counterpart in the GMRT image, three times the local noise is included as an upper limit on the flux density at 610MHz. ... 1.4-GHz flux density value from NVSS catalogue, including upper limits for undetected sources 76 I1 --- f_SNVSS [0/1]? ...

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• Computing dispersive atmospheric delay with AATM
• NVSS Source Search ($Revision: 1.6 $ - running v2.17)
• exchange.h Source File

Stellarium 0.12.3 . ... FileљStructure . FileљList . FileљMembers . core . planetsephems . calc_interpolated_elements.h . ... 6 љ copy of this software and associated documentation files (the "Software"), . ... 26 љ void CalcInterpolatedElements( const double t, double elem[], . ... 36 љ The cache consists of 3 sets of values: . 37 љ e0[0..dim-1] are the cached values at time *t0, . ... 41 љ (*calc_func)(t,elem) calculates the values elem[0..dim-1] at time t, . ...

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• Stellarium: core/renderer/StelGLSLShader.hpp Source File
• Stellarium: core/modules/Landscape.hpp Source File
• Stellarium: core/renderer/StelQGLGLSLShader.hpp Source File

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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• Geomagnetic Indices Kp, ap, Ap, Cp and C9
• ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM
• Pictures/Рисунки

... The actual cross-correlations were done as follows: north of WGACAT was correlated with the GB6 catalog with a correlation radius of one arc minute. ... We therefore cross-correlated WGACAT with the GB6 and PMN radio catalogs with a 1.5 arcmin radius. ... As a result of this experiment, we then added to the WGACAT/PMN candidate list the 29 unclassified sources obtained from the 1.5 arcmin correlation and having PSPC offsets arcmin, ratio between X-ray/radio offset and positional error , and . ...

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• list of DFS Department documentation templates
• ESO - How do I interpret the SEQ TIME keyword values?
• The Browne & March? Effect