Next: *period* - Period search Up: *fft* - Period search Previous: A summed or incoherent . The distribution of coefficient values for a single FFT is exponential if the original data contain no periodic signal. ... Significant coefficients will appear beyond the high-value end of the normal distributions. ... xt> fft.histogram_bi=0.5 # if necessary, adjust number for an aesthetic plot xt> ftpplot input table file: rp90_ftp The plot will appear on the screen. ...

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... HST . CALCOS v2.13.6 Release Notes . ... Data . ... Press Releases . ... HST Peer Review Process . ... HST Overview . Overview . ... Retrieving HST Data . ... Keyword Dictionary . ... If specified, calcos will search for the target spectrum in the Y direction and use that location to extract the spectrum, rather than relying completely on the offset from the wavecal spectrum. ... For spectroscopic data, calcos now writes WCS keywords to the flt and counts images and to the corrtag table. ...

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XMMґNewton CCF Release Note XMMґCCFґRELґ236 Truncated master o#set maps for epreject M. Kirsch August 16, 2007 1 CCF components Name of CCF VALDATE List of Blocks changed EPN REJECT 0005 2000ґ01ґ01T00:00:00 MASTER OFFSET MAP 2 Changes A problem has turned up in the version v5.9 of epreject, related to the introduction of master o#set maps: some pixels of the master o#set maps contain values which are so high that they may cause the corrected PHA values to leave the allowed range. ...

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Next: Phenomenological Kick Velocity Up: Restrictions on the Scenario Previous: The COOC Criterion (Criterion . ... The results of testing and parameters without kick velocity are presented in the form of "topographical maps" (i.e. as isolines) of constant ``COOC'' criterion in the plane calculated separately for each of the binary species listed in Table? 4 (Figures? 16 - 20 ). The total COOC criterion calculated with equal weights is shown in Figure? 21 . ...

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• Dependence on the Scenario Parameters and Initial Distributions
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Hide Zen home . ... Development version, available from this site, released under the GNU General Public License, version 2 (June 1991). hstore x2192; text - get value , perl analogy $h{key} select 'a=>q, b=>g'->'a'; ? ... akeys(hstore) - returns all keys from hstore as array regression=# select akeys('a=>1,b=>2'); akeys ------- {a,b} . ... delete (hstore,text) - delete (key,value) from hstore if key matches argument. regression=# select delete('a=>1,b=>2','b'); delete ---------- "a"=>"1" . ...

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... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

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... WISE is achieving 5sigma point source sensitivities better than 0.08, 0.11, 1, and 6 mJy in unconfused regions on the ecliptic in bands centered at wavelengths of 3.4, 4.6, 12, and 22 mum. ... The WISE All-Sky Release Source Catalog is available in compressed (gzip or bzip2) ascii form. ... Users should be aware that the Catalog table is extremely large. ... For complete documentation of the WISE All-Sky Release Source Catalog and the All-Sky Data Release, please see the Explanatory Supplement . ...

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OptInt PmWiki . ... Tech Meet 2 . ... Page History | ... PmWiki . ... Return to Tech Meet 2 ( Edit ) . ... 1 pixel independent of pixel scale (avoids aliasing of high frequencies in speckled image) . ... ADR & CAH: Optical image quality tolerancing of OAP-based layout . ... ADR & CAH: Layout and tolerancing of lens-based optical system . ... ADR & CAH: Use tolerancing results to assign image quality and stability budgets by component . ... ADR & CAH: Think about how to apportion image quality budget . ...

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• OptInt PmWiki : Other Variables

... Classes . ... casa . casa::DiscreteUniform . ... DiscreteUniform ( RNG *gen, Int low=-1, Int high=1) . ... low () const . ... range ( Int low, Int high) . ... These function allow you to manipulate the parameters (low & high) described above through the base class. virtual Vector < Double > . ... The DiscreteUniform class implements a quantized uniform random variable over the closed interval ranging from [low..high] . ... Int casa::DiscreteUniform::high . ... Int casa::DiscreteUniform::low . ...

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• Release of 1 July 1999.
• Version 6.0 - Released March 8, 2005

... Kernel . ... This article is part of the LWN Porting Drivers to 2.6 series . The kernel's handling of device interrupts has been massively reworked in the 2.6 series. ... If no interrupt handler for a given IRQ has been registered, the kernel knows that any interrupt on that number is spurious. ... If your interrupt handler recognizes and handles a given interrupt, it should return IRQ_HANDLED . ... can also be used; handled should be nonzero if the handler could deal with the interrupt. ...

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According to Armagh Observatory January was much milder than average. The mean monthly temperature was 6.3 degrees C, that is, 2.4 degrees higher than the average January figure of 3.9 degrees C. The temperature peaked at 13.6 degrees on the 7th January, making it the mildest January day for at least 145 years. ... The total number of hours of sunshine for January was 44.4, compared with the average figure of 46 hours. ...

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• Armagh Observatory Press Release
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09mar04 Measuring the hcorcal . Measuring the ratio of the other cals to the hcorcal . checking the cal values The hcorcal measured values: . ... After this the "other cals" were measured relative to the hcorcal while tracking blank sky. ... Fig 1 plots the cal Values measured the 3 different ways: . ... Fig 2 fits a 12th order polynomial to the cal value. ... The ratio of the "other" cals was then computed relative to the hcorcal (see measuring cals on the telescope using sky and absorber ). ...

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... Public . Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Publications with ESO Data . ... ESO-MIDAS . ... The short statement of the GNU license is included in every MIDAS file; the full text is included as a separate file in the ESO-MIDAS Release. ... Manual pages,installation guides and other documentation are generally released together with the source code and can also be obtained from the ESO-MIDAS ftp account (see below). ...

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... This book explains how to use core and client-side JavaScript for version 1.3. JavaScript is Netscape's cross-platform, object-based scripting language for client and server applications. ... Core, Client-Side, and Server-Side JavaScript . ... Client-Side JavaScript . ... JavaScript and Java . ... Examples . ... Conditional Statements . ... Object Manipulation Statements . ... Defining Functions . ... Objects and Properties . ... Indexing Object Properties . ... Defining an Event Handler . ...

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Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...

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.

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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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... XG Format Daughter Card . ... The MDB50X is a new XG format daughter card that will fit right into the Wave Blaster expansion connector of the Tahiti, SoundBlaster 16 (not the SB 16 Value), AWE-32 , or any sound card with a Wave Blaster compatible connector. ... In addition, extensive DSP effect functions are includes to give you complete control of your computer sound output. 32-note polyphony enables your system to produce all types of music production, sound effects and quality background music. ...

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... In electron-positron colliders, effect of the lattice modification by opposing bunch focusing on the equilibrium radiation emittance is important at high values of the space charge parameter, so one should correctly evaluate this dynamic radiation emittance of the weak beam, which may differ a lot from the nominal emittance, already in the linear beam-beam force model. ... The linearized beam-beam force is equivalent to focusing insertion in linear lattice of the collider. ...

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• Astronomical Catalogues

... ON THE ROLE OF LARGE-SCALE PLASMA IRREGULARITIES AT THE FINAL STAGE OF ANOMALOUS ABSOPTION DEVELOPING UNDER HF HEATING OF THE IONOSPHERE . ... Fig. ... With the aid of numerical statistical modeling based on multiple ray tracing it is shown that in presence of large-scale irregularities the reflected signal amplitude mean value is increased significantly. ... Dependence of the mean amplitude of the reflected from the ionosphere signal on the large-scale (10-50 km) electron density irregularity level...

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