macro into sm # : noisedemo 1000 0 = runs macro with 1000 pts # = 0 means no errorbars define N $1 define DOERR $2 set x=1,$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 { ...

... 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. ...

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 $C(X)$. ...

... 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 ...

... 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. ...

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. ...

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. ...

... 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. ...

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 . ...

... 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) . ...

... 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 . ...

Next: Spectral Extraction of Point Up: Spectral Analysis Previous: Structure of the Spectral . A pulse height distribution can be extracted from a QPOE file only if the event structure is `large', `region', or `full'. ... With the new RDF format files, the output from qpspec for most instruments is split into three files: . ... source off-axis histogram . ... background off-axis histogram . For Einstein IPC, there are no off-axis histogram files, but there is a BAL histogram file, _bal.tab. ...

... 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. ...

... 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 ...

. 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.

... 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 . ...

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= ...

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. ...

OptInt PmWiki : Pm Wiki / Wiki Group . ... PmWiki pages are organized into groups of related pages. ... By default, page links are between pages of the same group; to create a link to a page in another group, add the name of the other group and a dot or slash to the page name. ... To link to the default home page of a group, the name of the page can be omitted, like this: . ... For example, to make a default page in the group Foo, create a link to [[Foo/]] (or [[Foo.] ... Main : The default group. ...

... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...