... The parameter pgdev allows the user to specify a pgplot device, but, in contrast to the pgplot standard, the file name should not be included, but instead supplied via the parameter plotfile . ... To write a colour postscript file called op.ps: pgdev=/cps plotfile=op.ps . However note that at present, if a colour postscript device ( pgdev = `/cps'), a fits file ( pgdev = `/fits') or a ppm file ( pgdev = `/ppm') are selected, the task in fact bypasses pgplot and writes the postscript file directly. ...

... This calibration approach is recommended when dealing with high frequency data from the old ATCA correlator, especially at 3mm wavelengths. ... The approach described here exploits the dual frequency bands that were available with the old correlator. ... Rather the current approach assumes that you have a single Miriad dataset containing bandpass calibrator, phase calibrator, flux density calibrator and program source. ... MFCAL . ... Input multi-source, dual-band dataset. select=source(1921-293) . ...

Next: Wavelength calibration Up: Reduction using Standard Previous: Order Definition: Methods . ... The algorithm accepts frame which can be mildly contaminated by particle hits, bad columns, order gaps due to absorption lines, as found in FLAT or STD . ... the interorder background is roughly constant over the frame. the slope of the orders is in the range ]0., ... For a background estimate without previous order definition, consider the echelle command BACKGROUND/SMOOTH . ... LOAD/TAB order :X :Y . ...

Next: *pllist* - Look at Up: Regions and Source Parameters Previous: Regions and Source Parameters . ... cl> xray xr> ximages xi> plcreate region description: c 6930 9390 240 reference image file or 2 dims for mask: xdata$rp110590.qp output mask data file [root.pl]: rp110590 # =rp110590.pl file . ... xi> plcreate region descriptor: saoimage # default output file from SAOimage reference image file or 2 dims for mask: xdata$rp110590.qp output mask data file [root.pl]: rp110590 # =rp110590.pl file . ...

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

. Last updated 18 Mar 1999 . The ported software list for XFree86/OS2 is currently under construction. You can find the old pages at this link . In the future, you might find it likely here Trouble that the URLs below are not reachable? Try to look at alternative sites that archive stuff: . set.gmd.de . crydee.sai.msu.su . www.powerusersbbs.com . Reply to: Holger.Veit@gmd.de .

which serves as the electronic discussion forum for this class. ... All assignments will be posted there as well. ... Since the course material is always available, there is no longer a need for students to incessantly take notes in class. ... Grading techniques, however, will be designed so that people with weak math backgrounds or aptitudes will not be penalized. ... 2 Midterms which will total 40% of your grade . ... a few homework assignments which will total 20% of your grade . ...

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Description: . User authentication using MD5 Digest Authentication. Status: . Extension . ... This module implements HTTP Digest Authentication ( RFC2617 ), and provides a more secure alternative to mod_auth_basic . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

. This is the CIMA alternative drift map menu: . The following is the on-line help page for alternative drift map: . You can return to the main CIMA page by clicking here .

... mama/ : STIS UV imaging . ... stis_flank/ STIS Flanking Field imaging . ... Directory name: stis_v1catalog/ stis_v1generic.cat Generic parameters (e.g. numbers, positions) from detect image fuv_v1.cat Photometric parameter from FUVMAMA+F25QTZ observation lp_v1.cat Photometric parameter from CCD+F28X50LP observation nuv_v1.cat Photometric parameter from NUVMAMA+F25QTZ observation s50ccd_v1.cat Photometric parameter from CCD+50CCD observation stis_v1catalog.fits Full Catalog in stsdas table format . ...

NAME httpd - Apache hypertext transfer protocol server SYNOPSIS httpd [ - X ] [ - R libexecdir ] [ - d serverroot ] [ - f config ] [ - C directive ] [ - c directive ] [ - D parameter ] httpd [ - h ] [ - l ] [ - L ] [ - v ] [ - V ] [ - S ] [ - t ] [ - T ] DESCRIPTION httpd is the Apache HyperText Transfer Protocol (HTTP) server program. ... This manual page only lists the command line arguments. ... Paths in this manual may not reflect those compiled into httpd. ... The default is /usr/local/apache . ...

Blackholes Forum Message . Forums: . ... Alternative Idea . ... With the proposal of exotic super dense entities like quark stars and others including black holes, matter on the atomic level can, and most likely does, break down to its most simplist building blocks (photons, leptons, quarks, etc). ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

wcs2dr -- Convert WCS header information into drizzle parameters for image registration wcs2dr image refim . images = "" [file name] . ... The style for the output listing. ... cl wcs2dr @files ref style= para # drizzle .data= test1 drizzle .shft_fr= output drizzle .shft_un= output drizzle .align= center drizzle .xsh= 552.733 drizzle .ysh= 482.749 drizzle .scale= 1.009 drizzle .rot= - 2.871 # drizzle .data= test2 drizzle .shft_fr= output drizzle .shft_un= output ...

. Sergei and keyboard, photo by A.Yuferov .

If you already know the catalogue abbreviation or numbering, enter it below : . Alternatively you can find the catalogue by selecting wavelength or mission or other keys: (More on how to select catalogues) . ... Mission . ... A preliminary list of catalogues available in VizieR (still growing). The acronyms and symbols in use to designate astronomical catalogues in the literature are explained in the Dictionary of Nomenclature of Celestial Objects . Location : CDS Strasbourg, France . ...

grdvector - Plot vector fields from grdfiles grdvector compx . ... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / ...

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

... М: ст.м."Медведково" - Мытищинская ярмарка - расписание . ... 443 (полуэкспресс, бывш. 343к ) - 8руб. ст.м."Алтуфьево" - платф. ... Долгопрудная - Спортивная - 8руб.; по городу Долгопрудному 3руб. ст.м."Домодедовская" - а/п Домодедово - 20руб. ... 313 платф. ... Расторгуево до п-ки) - 4руб. 367 (*) - до Молокова - 7руб., до пос. Володарского - 10руб., по городу - 3руб. 368к (*): платф. ... ст.м."Молодежная" - Барвиха (N101) - 10руб. ст.м."Новогиреево" - г. Балашиха - 16руб. (по городу 6руб.) . ...

Before calibrating the visibility data, we need to plot it and flag the blue channels 21 to 32 because of their low signal-to-noise ratio. Select VisSq, the uncalibrated raw (squared) visibility amplitude, and plot it versus channel. ... The data selection defines which data is to be used to compute the correlation parameters, with the exception that if the Option|Loop parameter is selected in the calibration widget, the channels are calibrated independently, doing every selected channel. ...

... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...