define N 1024 set x=1,$N # dummy call to get ws dimensioned right get_hist x v ws -.5 .5 .02 set ws=ws*0 erase window 1 1 1 1 set y=x*0 limits 0 $N -.7 0.7 box ptype 1 1 # generate a lot of points to uniformly cover - 0.5 to 0.5 # -and- at the same time do averages of 10 samples = pseudo-gaussian do i=1,10 { set t=random($N)- 0.5 set y=y+t # keep plotting the uniform points points x t get_hist t v w -.5 .5 .02 set ws=ws+w } ...

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• http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/build_data.5.sm
• http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/build_data.3.sm
• http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/build_data.1.sm

... For those users of Mongo intimidated by change, we note that in most cases it is possible to ignore the enhancements by using a macro presented in the next section. This macro redefines commands to reproduce the old syntax; for example limits is defined to mean LIMITS x y . It is also possible to read Mongo files using the READ OLD command, and the macros input and read_old based upon it. ... Vectors may be defined from the keyboard using DO loops or expressions. ...

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• casacore: casa::Dummy_Constants_class Class Reference
• blflag
• The SM Tutorial - How do I define variables, and how can I use them?

... Height from the galactic plane 65- 75 A11 --- IRAS IRAS name 81 A1 --- l_F12 limit flag on F12 (upper limit ) 83- 90 E8.2 Jy F12 IRAS flux density at 12 micron 92 A1 --- l_F25 limit flag on F25 (upper limit ) 94-101 E8.2 Jy F25 IRAS flux density at 25 micron 103 A1 --- l_F60 limit flag on F60 (upper limit ) 105-112 E8.2 Jy F60 IRAS flux density at 60 micron 114 A1 --- l_F100 limit ...

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• Big Pixels
• Sky subtraction and object extraction
• Entry points

... The integration time (INT_TIME) is defined as the length of time over which the data were averaged to yield the given data point. ... Taking the system variable !int_time to specify an upper limit for the integration time in seconds which will not require integrating the model visibilities, will compare the actual integration times to this limit and determine the maximum number of computations required to cover the largest integration interval. ...

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• FORS Sec Std and Abs Phot Project
• The Criteria

Composition and cartesian product of continuous maps is continuous. A set is closed iff it contains all its limit points. ... Completeness of R and its corollaries (existence of the supremum, etc.) The segment is a connected set. ... Compacts in R n (the Heine?ndash;Borel lemma). An infinite subset of a compact has a limit point. ... A uniform limit of a family of continuous maps is continuous. ... A continuous map on a compact set is uniformly continuous. ... The completeness of $C(X)$. ...

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... The performance of the task is directly proportional to the number of bins in the energy grid (ie the number of rows of the matrix), while the scientific accuracy of the results of using the matrix improves (to the limit of the energy resolution of the instrument) the more rows there are in the matrix. ... A user-defined grid can at present be only such that the grid points are evenly distributed across the energy range. ...

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• Description
• Limits on attitude wander

... 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 2002 Conference Proceedings
• Simulations of Pinhole Imaging for AXAF: Distributed Processing Using the MPI
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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... 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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• Astrophysical Research Consortium - Apache Point Observatory
• lsst.tcc: python/tcc/mov/checkSegment.py Source File
• lsst.tcc: tcc.mov.checkSegment Namespace Reference

NStars 1: photometric surveyse --- | ... The second incremental release of 2MASS data provides accurate JHK S photometry for hundreds of millions of point sources covering 47% of the sky. ... The simple colour-magnitude limits outlined in Figure A1.2 encompass a wide range of astronomical sources: red giants, carbon stars, reddened Galactic stars, T Tauris and dusty QSOs, besides the targeted ultracool dwarfs. ... Figure A1.6: 9 are sources eliminated from the sample based on optical photometry. ...

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• Comments
• Stellar Photometry
• Method

... Re : Can you block or ignore ICMP packets? ... While adding that #define CONFIG_IP_IGNORE_ECHO_REQUESTS into linux/net/ipv4/icmp.c will work fine for now, I'd suggest putting it into the configuration-headers so it doesn't tangle up with further patches, or, should that define later move into different file(s), lose it's efficiency. ... Meanwhile, if you're worried that ignoring _all_ echo-requests may be a bit too rough move, there's a way to make the kernel ignore them selectively. ...

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• LASG - Limiting and monitoring users
• mod_dialup - Apache HTTP Server
• LASG - License and Warranty

Blackholes Forum Message . ... Quicksand As Black Hole Model? ... For the hole to be black it must have a fuzzy edge i.e. something one is sinking into (like a black hole is like quicksand that you discover by sinking partly into it?) ... A number of oranges "probes" what it is to be an orange so "black hole" = "number" you might suppose. ... The rest of their body not in the quicksand (i.e. not in the black hole) equates to the "collection of anti-matter near the blackhole"? ... www.astronomy.net . ...

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• Diffraction Limited, AstroGuide Listing
• Floating Factorisation - an Astronomy Net Blackholes Forum Message

... Hide Zen home . ... GIN . ... contains: value_array @ query_array . ... An example for a Gin opclass can be found in ginarayproc.c. Datum * extractValue( Datum inputValue, uint32* nentries) Returns an array of Datum of entries of the value to be indexed. nentries should contain the number of returned entries . int compareEntry( Datum a, Datum b) Compares two entries (not the indexing values) Datum * extractQuery( Datum query , uint32* nentries, StrategyNumber n) Returns an ...

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• Access Control Options
• Zen: knngist
• Zen: Tsearch V2 in Brief

The above image is a computer simulation of the distribution of mass in a Dark Matter dominated Universe. ... Structure (\eg density enhancements) clearly forms at the intersection of these filaments. ... What is Dark Matter? ... Testing for the presence of dark matter in the solar neighborhood now becomes an accounting problem The possible sources of this mass in the solar neighborhood are 1) luminous stars, 2) interstellar gas, 3) stellar remnants (mostly white dwarfs) and 4) dark matter: . ...

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• CCDs for Material Scientists
• Comparing Means and Deviations

... Posts tagged ?point spread function? ... Thus, a major contributor to the LRF (Line Response Function) is the aforementioned scattering. ... controls the sharpness of the function ? ... Tags: beta profile , Chandra , EotW , Equation , Equation of the Week , Line Response Function , Lorentzian , LRF , point spread function , PSF , response matrix , RMF , XMM . ... Tags: ARF , effective area , EotW , Equation , Equation of the Week , LRF , point spread function , PSF , response matrix , RMF , source ....

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• PINTofALE EXAMPLE : Simulation for Chandra ACIS-I
• The AstroStat Slog RMF
• *qpspec* - Extraction of Photon Distributions from QPOE files

... Arithmetic Functions . Random Numbers . String Conversion . Searching and Sorting . ... There are 4 basic integer functions: . int abs(int number); long int labs(long int number); div_t div(int numerator,int denominator); ldiv_t ldiv(long int numerator, long int denominator); . ... In practice no functions produce truly random data -- they produce pseudo-random numbers. ... The stdlib.h provides 2 useful functions to perform general searching and sorting of data on any type. ...

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• Advanced Pointer Topics
• harak_e
• Arrays and Strings

. 1. Move the cursor to the start of the text block you want to define. 2. Type M-space (the META character followed by a space). This sets a 'mark' at the start of the 'region'. 3. Move the cursor to the end of the text block you want to define as the 'region'. This sets the 'point' at the end of the 'region'. You do not have to type anything to set this 'point', the 'point' is the location of the cursor.

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• Hypertext Links

... 07feb11: cband receiver, za limits still 16 degrees . 08feb11: lband receiver, za limits 19.69 degrees. 09feb11: lband receiver, za limits 19.69 . The plots show the results of the pointing runs (.ps) ( .pdf ): . ... Page 2: 01dec10 thru 31jan11 pointing results: . ... Page 3: 01dec10 thru 09feb11. all data separating out before after 01feb11 . ... Page 4: 01dec10 thru 09feb11. all data separating out lband and cband. The black points are lband, the red points are cband. ... data set . ...

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• rotaPlatToSky
• Pulsar ALFA Surveys
• pntModelGradients

SAVE_PHOTO_WHEN_TERMINATE=T, CREATE_PRE_MAIN_SEQUENCE_MODEL=T, PRE_MS_RELAX_NUM_STEPS= 200, LOAD_SAVED_MODEL=F, SAVED_MODEL_NAME=' undefined ', CREATE_INITIAL_MODEL=F, INITIAL_MODEL_RELAX_NUM_STEPS= 10, INITIAL_MODEL_EPS= 5.0000000745058060E-002, RADIUS_IN_CM_FOR_CREATE_INITIAL_MODEL= 0.0000000000000000 , MASS_IN_GM_FOR_CREATE_INITIAL_MODEL= 0.0000000000000000 , STEPS_TO_TAKE_BEFORE_TERMINATE= -1, STOP_IF_THIS_FILE_EXISTS=' ', SET_INITIAL_AGE=F, INITIAL_AGE= ...

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• Relationship Between Auto Chirplet FF Plane and Radon Transform
• Conformance: requirements and recommendations
• Peculiarities in the language Fortran 90

SINGULAR POINTS IN THE SOLAR CHROMOSPHERE . ... In the structure of the solar chromosphere, containing information on the configuration of the magnetic field, we have found and identified all the main types of the singular points ( see Fig. 1 ), which are known as inherent features of the 2-D vector field. ... The main types of the singular points are the node, the focus, the center, and the saddle. ... Singular point of the focus type in the solar chromosphere. ...

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