... GPI Data Pipeline 1.0 documentation . GPI IFS Data Handbook . ... GPI Data Formats . Multi-Extension FITS format . ... Data quality flags extension ?DQ? ... This extension will contain a 8-bit integer flag for each pixel in the main image array. ... Bit 5 may be written by the data pipeline, which can also modify bit 0. bit 0: bad pixel, do not use if set. ... bit 5: [work in progress] flagged as bad pixel by data pipeline using time-dependent bad pixel map from calibration database. ...

SAOtng can load array files containing "raw" images. ... skip -- the size of the header to skip (in bytes) . ... This information is added to an array filename using the IRAF bracket specification: foo.array[xdim= xdim ,ydim= ydim ,bitpix= bitpix ,skip= skip ] . ... Thus, a 512 x 512 array of any type without a header can be specified as: foo.arr 512 while a 600 x 700 double array with a 1024-byte header can be specified as: foo.arr 600 700 -64 1024 . ... r512 -- bitpix=-32 xdim=512 ydim=512 . ...

WCSLIB љ 5.15 . ... fitshdr.h File Reference . ... fitshdr (const char header[], int nkeyrec, int nkeyids, struct fitskeyid keyids[], int *nreject, struct fitskey **keys) . ... Typically the latter may be set to remove WCS keyrecords from a header leaving fitshdr() to handle the remainder. #define FITSHDR_KEYWORDљљљ0x01 . ... Bit mask for the status flag bit-vector returned by fitshdr() indicating a keyrecord following a valid END keyrecord. #define KEYIDLENљљљ(sizeof(struct fitskeyid )/sizeof(int)) . ...

... We propose a set of standard character strings to be used in FITS files generated by data from the ALEXIS (Array of Low Energy X-ray Imaging Sensors) satellite mission. ... The following is our current proposal for keywords to use for storing raw and processed ALEXIS mission data in FITS format. TELESCOP= 'ALEXIS ' . ... In migrating these existing files to FITS formats, we propose the following non-inclusive list of generic column headers (these will be of the form TTYPE n = ' header ' ). ...

The following list contains links to examples of the FITS-headers used in various versions of CIMAFITS: . CIMAFITS pre-1.00 version - used 16 September 2004 - 3 February 2005 . ... CIMAFITS version 1.01 ( bug fix only - no format change) - used 22 February 2005 - 25 May 2005 . ... CIMAFITS version 1.04 ( bug fix only - no format change) - used 10 May 2006 - 8 February 2007 . CIMAFITS version 1.05 ( bug fix only - no format change) - used 8 February 2007 - 15 February 2007 . ...

... source code A class to hold all the information from a NIFS-produced data cube. ... Returns the data content of scidata as a numpy array. source code . ... Returns a spectrum from the specified spaxel, over the designated wavelength or velocity range. source code . ... source code Returns the data content of scidata as a numpy array. ... The fitscube instance is updated in-situ. source code Returns a spectrum from the specified spaxel, over the designated wavelength or velocity range. ...

... Now click on HIDE and all non-PRISM observations should disappear. ... Can be accessed with visTable = oirGetVis(filename, wave=wave) with wave optional visTable.visamp is an array of (nWave) correlated fluxes (Jy) visTable.visphi is an array of (nWave) differential phases (degree) visTable.visamperr contains the estimated rms of visamp visTable.visphierr contains the estimated rms of visphi wave contains nWave values of the wavelength (microns) .photometry Produced by oirChopPhotometry. ...

Next: Restrictions Up: IHAP Format Previous: IHAP Format . The IHAP header contains the description of the data in a fixed, binary format. With reference to the IHAP manual, the translation of this information into MIDAS descriptors are given in Table . IHAP defines the end of exposure which is converted to exposure time. Also, start and end are given for image axes instead of start and number of pixels . Table: Name translation between IHAP header and MIDAS descriptors. ...

write a simple ASCII file containing pairs of x and y values. write a simple ASCII file containing pairs of x and y values. write a file containing pairs of x and y values in Spectrum format 2, including a header. read a file containing pairs of x and y values in Spectrum format 2, including a header. ... Compute cross-correlation function for functions y1(x1) and y2(x2) The result is returned as ccfy(ccfx) Apply a velocity correction to a wavelength array. v is in units of the speed of light. ...

This module provides for the customization of HTTP response headers. ... This module provides a directive to control the sending of HTTP headers. ... Header . ... Syntax: Header set|append|add header value . ... Module: mod_headers . This directive can replace, merge or remove HTTP response headers during 1xx and 2xx series replies. ... set . The response header is set, replacing any previous header with this name . ... The response header is appended to any existing header of the same name. ...

... This appendix tells you how you can use JavaScript to filter your incoming mail and news when you use Netscape Messenger. ... Write a JavaScript function to serve as a filter and put it in your filters file. This function takes one argument, a message object, and can make changes to that message. ... News Filters . ... This file contains the JavaScript functions that perform the mail filtering. ... For news filters it is a News Message object and for mail filters it is a Mail Message object. ...