Instrument Overview . ... Spectral Filters . Quantum Efficiency and Exposure Limits . ... Which Instrument to Use: WFPC2, ACS, NICMOS, or STIS? Comparison of WFPC2 and ACS . Comparison of WFPC2 and NICMOS . Comparison of WFPC2 and STIS . History of WFPC2 . ... WFPC2 . ... What's New in Version 5.0 for Cycle 10 . ... Calibration Channel . ... LRF Photometric Calibration . ... Wood's Filters . ... Sources of Dark Current . ... Calibration Plan Summary . Cycle 4 Calibration Plan . ...

... List of Tables . ... How to use the MIDAS Manual . ... Commands . ... Executing System Commands . Some Useful Commands . Monitor and Command Language . ... MIDAS Data Structures . ... Specifying Pixels in an Image . ... Command Syntax . Command Recalling . Command Line Editing . ... MIDAS Command Language . ... Command Overview . ... Table Format Files . ... Graphic and Image Display . ... PLOT and OVERPLOT commands for plotting data . ... Graphic Cursor Commands . ... FITS Format . ...

... This paper describes recent improvements to the FITSIO subroutine library and the fv FITS file viewer and editor, both of which were initially described at previous ADASS conferences. ... Since the time of the last FITSIO update (Pence 1995) a new CFITSIO library has been developed, written entirely in C. CFITSIO is easier for C programmers to build and call than the previously available C wrapper routines built on top of the FORTRAN FITSIO library. ...

... Routines for accessing I/O ports are in /usr/include/asm/io.h (or linux/include/asm-i386/io.h in the kernel source distribution). ... Before you access any ports, you must give your program permission to do so. This is done by calling the ioperm() function (declared in unistd.h , and defined in the kernel) somewhere near the start of your program (before any I/O port accesses). ... For example, ioperm(0x300, 5, 1) would give access to ports 0x300 through 0x304 (a total of 5 ports). ...

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

... In addition to the help files associated with each task and package, there are a number of more general descriptions which give information about algorithms or about topics which affect more than one task. ... The source tree is contained in a compressed tar file called saord.tar.Z. The unpacked tar file requires approximately 45 Mb of disk space. ... QPOE Files . ... rarc2pros* - Converting Archived Data to PROS files . ... qpcopy* - Manipulation of PROS/IRAF data files . ... Image Display . ...

Next: Up: Optical Interferometer Script Data Previous: Optical Interferometer Script Data . ... Programmer's reference . ... The plot selection widget . ... Astrometry . ... Script library files . ... Introduction . ... Data files . ... Basic widget procedures . Load data . ... File usage . ... Data and auxilliary files . ... Output files . ... Open the data file . ... Open a data file . Access a data file . ... Accessing data files . ... NPOI raw data files . ... NPOI raw packet data files . ...

. ОГЛАВЛЕНИЕ . Предисловие к четвертому изданию . Введение . § 1. Предмет и задачи астрономии . § 2. Подразделение астрономии . § 3. Возникновение и основные этапы развития астрономии . § 4. Практическое и идеологическое значение астрономии . § 5. Основа и источник астрономических исследований . § 6. Краткий очерк строения Вселенной . Глава I . Основные сведения из сферической астрономии . § 7. Видимые положения светил. Созвездия . § 8. Видимые движения звезд, Солнца, Луны и планет . § 9. Географические

... The PSF is stored as a radial distribution in the CCF component PSF1DRB. ... The radial width of the PSF is stretched by the factor f by multiplying the radial bin limits with f : . The stretching factor f is calculated for the specified field position (rawX, rawY) from a 3rd order polynomial. (35) . ... calculate the minimum distance r of the pixel to the PSF centre (rawX, rawY) . calculate the maximum distance r of the pixel to the PSF centre (rawX, rawY) . ... normalize PSF map to 1 . ...

... Bojan Nikolic web pages (r. 329) . See ALMA WVR phase correction algorithms and software for information regarding the wvrgcal program, libAIR C++ library and download of software for atmospheric phase correction for ALMA . This is the contents page for my ALMA related work, which is currently focused primarily on techniques for correction of atmospheric phase errors using 183GHZ water vapour radiometers. ... ALMA Goals . ... ALMA WVR phase correction algorithms and software . ... Software . ...