... Archives . ... ArXiv] Kernel Regression, June 20, 2007 . Quote of the Week, June 27, 2007 . Jun 27th, 2007| 02:23 pm | ... Comments on the unified approach to the construction of classical confidence intervals . ... I?ve heard a few discussions about classical confidence intervals and upper limits from particle physicists and theoretical statisticians. ... Tags: confidence interval , coverage , flip-flopping problem , upper limit . ... Chandra Blog . ... SAMSI AstroStat Prog. ...

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• *timfilter* - List start & stop times of good data intervals
• The AstroStat Slog interval
• Extraction of limited time intervals

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

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• Meteo :: Kislovodsk Database ::

MODULE INTERVAL _ARITHMETICS TYPE INTERVAL REAL LOWER , UPPER END TYPE INTERVAL INTERFACE OPERATOR (+) MODULE PROCEDURE INTERVAL_ADDITION END INTERFACE INTERFACE OPERATOR (-) MODULE PROCEDURE INTERVAL _SUBTRACTION END INTERFACE INTERFACE OPERATOR (*) MODULE PROCEDURE INTERVAL_MULTIPLICATION END INTERFACE INTERFACE OPERATOR (/) MODULE PROCEDURE ...

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• Program units

... 20 Hz ------------------------------------------------------------------------- Total CTO frame = 51008 Cnt_ION frame = 123 Cnt_IESP frame = 51008 Cnt_POL frame = 45581 Cnt_DOK frame = 51008 Total frame: 51008 Error_de 10, Error_dp 1 Error_Teta 0 Error_marker 13, Error_cycle 31 Er_h 0, Er_min 0, Er_sec 0 Total frame: 51008 Error_de 10, Error_dp 1 Error_Teta 0 Error_marker 13, Error_cycle 31 Er_h 0, Er_min 0, Er_sec 0 ...

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• http://www.cosmos.ru/da/interball/auroral/passport/sto7_07/a71991c1.tx1
• http://www.cosmos.ru/da/interball/auroral/passport/sto7_10/a72861c1.tx1
• http://www.cosmos.ru/da/interball/auroral/passport/sto7_07/a71951c1.tx1

... Connecting the planned observations and the actual status of the Chandra X-ray Observatory is the observation interval determination pipeline ( OBIDET ). This collection of tools allows the Chandra X-Ray Center Data System automated processing to process the data through the necessary pipelines based on what was actually observed. ... In the case of the Chandra X-ray Observatory, the observation interval determination pipeline ( OBIDET ) is used for this task. ...

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... User Guide ] Task: mfcal Purpose: Multifrequency antenna and passband calibration. ... No default. This can (indeed should) contain multiple channels and spectral windows. ... Key: flux Three to five numbers, giving the source flux density, a reference frequency (in GHz) and the source spectral index parameters. ... Key: interval This gives one, two or three numbers, all in units of minutes, being used to determine the lengths of the antenna gain and passband calibration solution interval. ...

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• casacore: casa::MSInterval Class Reference
• casacore: casa::TableLock Class Reference
• Summary

This module provides for the generation of Expires HTTP headers according to user-specified criteria. ... This module controls the setting of the Expires HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... ExpiresByType . ExpiresDefault . The ExpiresDefault and ExpiresByType directives can also be defined in a more readable syntax of the form: . ... Module: mod_expires . ...

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• Other Programs - Apache HTTP Server

1) Find the variable star and the comparison stars marked in the map. 2) Seeing the the variable star, try to imagine its location in the brightness interval between the reference stars. 3) Looking at the specially prepared scale, try to reproduce the location of variable in the brightness scale from memory. ... The grades of arbitrary scale are marked relative to brightness intervals between the reference stars. ...

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• http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p78-p78.pdf
• http://mavr.sao.ru/hq/lizm/conferences/pdf/1996/1996_p93.pdf
• Description of algorithm

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Timers don't work?? ( Joshua Liew ) . Keywords: timer . Date: Wed, 03 Dec 1997 01:25:06 GMT . From: Balaji Srinivasan < balaji@hegel.ittc.ukans.edu > . The mistake with your code is that you need to . update INTERVAL every time you add_timer. The expires field in timer_list is an absolute . time not a relative time. for example: . irq() { . timer.expires = jiffies + INTERVAL; . add_timer(&timer); . } .

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• mod_expires - Apache HTTP Server
• htcacheclean - Clean up the disk cache - Apache HTTP Server
• rotatelogs - Piped logging program to rotate Apache logs - Apache HTTP Server

initial data . mean 1990-2012 . mean 1970-2012 . PC 1 (1+2) mean . PC 2 (3+4) annual . ... PC 5 (9+10) 1/3 year . ... PC 4 (7+10) quasi-biannual . ... Sum of nine first PCs 2-10 without mean (1st PC) . Difference between the initial signal and ten first PCs 1-10 . ... Sum of ten first PCs 1-10 . ...

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In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

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• More about shutdowns
• Planetary positions
• SPECTRUM v3 - Examples

The maps show how the sky looks at gamma-ray energies above 100 million electron volts (MeV) with a view centered on the north galactic pole. The first frame shows the sky during a three-hour interval prior to GRB 130427A. The second frame shows a three-hour interval starting 2.5 hours before the burst, and ending 30 minutes into the event. The Fermi team chose this interval to demonstrate how bright the burst was relative to the rest of the gamma-ray sky. ... NASA/DOE/Fermi LAT Collaboration ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B187D1259-28D4-45C0-A2E7-9A63626C913B%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2E8BCE16-51D9-439D-8B7E-FCA707D63559%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3B5A7929-AF93-4A52-A0E0-251DD777564C%7D

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• Current state

... SEARCH ASP SITE: Match ALL words Match ANY word . ... Comet Hyakutake wowed us this spring [see Guest Observer, May/June, p. 11]. ... The best time to observe a meteor shower is after midnight, as your nighttime location moves head-on into the path of the cometary debris. ... As observers, we are interested in the number of Perseids per time interval. ... Tabulate the number of meteors observed per interval, and make sure to label the table with the local time and date of each interval. ...

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• ASP: The Music of the New Spheres?

. Please, enter light elements for your star and Julian Day interval. HJD0: . Period: . JD1: . JD2: .

16. Guidelines for creating a password

17. Vertical Structure, figures

18. East Siberian Center for the Earth's Ionosphere Research. Maximum usable

19. Reduction quantities for Dynamical time. Explanations for Computer Ephemeris.

20. lsst.tcc: python/tcc/base/tune.py Source File