... Meta Index / Home Page / User-visible functionality The calibration algorithms in the CAL are driven by data in the Current Calibration File (CCF) . A CCF is represented by the contents of a Calibration Index File (CIF) which comprises for each constituent various entries such as the start validity date, issue number, file name etc. ... SAS_CCF . ... A white-space separated list of CCF constituents which should replace the corresponding ones listed in the active CIF. ...

Next: Astrometry Up: Quick Guide Previous: Reduce point data Contents . R EDUCE A VERAGE averages all the data currently contained in the point data arrays. The corresponding scans in the scans array (it will be automatically created when non-existent) will be updated. average will print out messages as to invalid (flagged) data encountered, and non-existing background scans. ... Christian Hummel 2015-04-28 ...

Next: Computation of the Up: Typical Run Previous: Edition of the . This table is used both as an input and output by the main program. The table content is: . INPUT . Parameters relative to the absorption lines . ... OUTPUT . In output, the program will write in this table, for each absorption line, the velocity of the corresponding cloud relative to the source and its redshift (relative to the observer). A template of this table can be found in MID_CLOUD:ABSC.TBL . ...

... The name of each file in an FOC dataset, such as x3l80101t.d0h, has a three-character suffix, in this case the d0h , that uniquely identifies the file's content. ... c1h /. c1d files. ... c1h /. c1d files contain the final calibrated data, which are likely to be of greatest interest to observers. ... trl or trailer file-which comes with each FOC observation-is an ASCII text file that describes the standard processing applied to the images by OPUS. ... Raw Data Files .d0h/.d0d . ... Trailer file .pdq...

... DataљStructures . ... WCSLIB data structures . The WCSLIB routines are based on data structures specific to them: wcsprm for the wcs.h ,c routines, celprm for cel.h ,c, and likewise spcprm, linprm, prjprm and tabprm, with struct definitions contained in the corresponding header files: wcs.h , cel.h , etc. ... In particular, wcsset() analyses the FITS WCS keyvalues provided, fills the required values in the lower-level structs contained in wcsprm, and invokes the setup routine for each of them. ...

The .out files contain the data displayed in plots of the wide spectral scans of High-CAL and the respective bets-fits obtained. Each of the 14 pipelines has a separate file. What to expect inside this file ? ... These files are made available for interested people to download. ... Note: Since the measurements for the beam0-pol_1, beam 5 (both pol.s) were missed from the set on tJD:53228 (due to the pre-amp and WAPP problems respectively), the corresponding fits & .out files missing. ...

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

An example of visual expert system. The program is written on Actor Prolog. -- -- (c) Alexei A. Morozov, March 19, 1999. ... Actually I wrote this program to train myself -- -- in carrying out SADT interview. ... A logical description of the blocks of the SADT model. ... The main purpose of these classes is keeping lists of cooking -- -- battery corresponding to various blocks of the SADT model. ...

authcert . ... The program reads a line from the standard input containing a key, plaintext block and the corresponding encrypted ciphertext block, respectively, as in the following 0000000000000000 0000000000000000 8CA64DE9C1B123A7 FFFFFFFFFFFFFFFF FFFFFFFFFFFFFFFF 7359B2163E4EDC58 3000000000000000 1000000000000001 958E6E627A05557B 1111111111111111 1111111111111111 F40379AB9E0EC533 0123456789ABCDEF 1111111111111111 17668DFC7292532D ...

... This file contains the information about IB_TAIL and IB_AUR (AURORAL) magnetic conjugations as a function of the Universal time. The predicted magnetic conjugations correspond to the less then 5 deg relative geocentric angular distance of the two satellites magnetic footprints. ... the difference between two satellites corrected geomagnetic local times (see as well column 11) . ... the difference between two satellites corrected geomagnetic latitude (see as well column 12) . ... AnD (deg) . ...

... Contains properties describing the display screen and colors. ... JavaScript 1.2 The JavaScript runtime engine creates the screen object for you. ... Specifies the height of the screen, in pixels, minus permanent or semipermanent user interface features displayed by the operating system, such as the Taskbar on Windows. availLeft . ... Specifies the width of the screen, in pixels, minus permanent or semipermanent user interface features displayed by the operating system, such as the Taskbar on...

It is a matter of common knowledge that in processes of genesis and evolution of many solar phenomena participate magnetic fields of sunspots. ... As a basis for formation of the database we take data on magnetic fields, collected by set of observatories during many years of observations. ... Section "Magnetic field data" contains data of magnetic field observation for separate sunspots, presented in standard text format (ASCII). ... Description of structure of these files is presented here . ...

... The user database is traditionally contained in the /etc/passwd љ file. Some systems use shadow passwords , and have moved the passwords to /etc/shadow љ . ... However, installing shadow passwords later onto a system that did not support them can be difficult. ... The crack љ program can be used to crack passwords; any password it can find is by definition not a good one. ... The user group database is kept in /etc/group љ ; for systems with shadow passwords, there can be a /etc/shadow.group љ . ...

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

To proceed to drawing tracks of some objects select Tracks item in menu bar and then select Input Data in drop-down menu. Enter initial and final dates of time interval in corresponding data fields of the Input Data dialog box Input Data . ... The frame with horizontal and vertical scales corresponding to the right ascension and declination axes appears on screen. ... Depending on specifications introduced in the Input Data dialog box the picture represents tracks up to three different objects. ...

... We describe a tool in the PCIPS environment for finishing the job of globular cluster photometry started by DAOPHOT II: starting with the instrumental magnitudes derived by DAOPHOT II, DASHA can automatically produce final color-magnitude diagrams. ... DASHA can automate the whole process of globular cluster photometry, from instrumental magnitude lists produced by DAOPHOT II, to final color-magnitude diagrams. ... DASHA is oriented towards star lists produced by DAOPHOT II as source data. ...

Files do not actually reside inside directories. ... The directory holds two pieces of information about each file: . ... an inode number which acts as a pointer to where the system can find the information it needs about this file. Filenames are only used by the system to locate a file and its corresponding inode number. ... To the system, the file is the inode number. Multiple filenames can be used to refer to the same file by creating a link between an inode and each of the filenames. ...

... Its apparent diameter of 18.0 arc minutes corresponds to a linear extension of about 180 light years; Kenneth Glyn Jones mentions an estimate of even 20 arc minutes from deep photographic plates, corresponding to about 200 light years linear diameter. It appears somewhat smaller in amateur instruments, perhaps about 10 minutes of arc. ... Red: 20x3 minute subs, totaling 1 hour . Green: 20x3 minute subs, totaling 1 hour . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

Download Izmccd (~2.7 MB). ... for 1-5 bytes is number of a numbered minor planet, . ... Positions 1-80 file "mpcreportiz.txt" are similar to positions of file "mpcreport.txt". 83-95 – errors of unit weight, . ... If this tag is " 1 0 " , this record contains results of measurements of an image of object (approximation by "PSF"),  . ... 57-66 – error in X (pixels), for first star in a multicentric image, for subsequent it is error in (distance between first star in the image and this), . ...

... Radio astronomical tests of the engineering model of the space radio telescope (SRT) were completed in Pushchino - see Results . ... Monitoring of the development of the upgrade on-board 1.35-cm receiver (R-SRT-1.35 cm): . ... EM Engineering Model . ... OHCFS-SRT Space Radio Telescope On-board Heterodyne and Clock Frequency Synthesizer set . OHFS-SRT Space Radio Telescope On-board Hydrogen Frequency Standard . ORFS-SRT Space Radio Telescope On-board Rubidium Frequency Standard . ...