ChangeLog for region =============================== Open SPRs: ---------- Nil Version 7.9 - 2005-11-17 (IMS/LUX) ---------------------- - Swapped order of CAL_setState(accuracyLevel=ACCURACY_MEDIUM)and call to CAL_psfValidityRanges(). Fixes SPR 3542/3544. ... Version 7.7 - 2005-06-09 (IMS/LUX) ---------------------- - Added new parameter --tempset (fixes SPR 3471). ... Version 7.1.5 - 2004-02-12 (IMS SSC/LUX) -------------------------- - Fixed SPR 3255. ... Fixes SPR 3178. ...

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

... CCD Parameters table (_ccd) to be placed in the header keyword, CCDTAB, before recalibration. ... Oct 15 1999 . ... INFLIGHT 01/05/1999 02/05/1999 . ... Feb 16 2000 . ... DEC 26 1999 . ... SMOV3A values for Dec 27-29 1999 . ... INFLIGHT 30/12/1999 07/01/2000 . ... INFLIGHT 10/01/2000 25/01/2000 . ... JUL 10 2001 00:00:00 . INFLIGHT 12/07/2001 25/02/2002 . ... Added columns for CTE correction . ... Dec 26 1999 00:00:00 . ... Updated CTE parameters . ... New parameters for improved CTE correction . ...

Stellarium 0.12.3 . ... FileљStructure . ... SphericalRegion . DrawParams . ... SphericalRegion::DrawParams Struct Reference . Parameters specifying how to draw a SphericalRegion . More... #include < StelSphereGeometry.hpp > . DrawParams (class StelProjector *projector) . Construct DrawParams with default parameters and specified projector. ... Do not subdivide the region to follow projection distortions. ... class StelProjector * SphericalRegion::DrawParams::projector_ . ...

Hide Zen home . ... sncat2sntab.pl - convert old catalog to table sn . ... CREATE TABLE cats ( id integer PRIMARY KEY, name text ); -- a list of properties of galaxy CREATE TABLE properties ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy ( id integer PRIMARY KEY, name text ); CREATE TABLE galaxy _property ( gid integer REFERENCES galaxy (id), pid integer REFERENCES properties(id), value float, UNIQUE( gid ,pid) ); CREATE t=# select * from galaxy; id | ...

... The concept of continuous solar wind developed in 1950's. First, Biermann (1951, 1957) observed comet tails as they passed close to the Sun , and explained the observed tail deflection by a continuous flux of protons from the Sun. Then Parker (1959) showed that the solar corona must expand, and called the outward streaming coronal gas 'solar wind'. ... The expanding solar wind drags also the solar magnetic field outward, forming what is called the interplanetary magnetic field (IMF) . ...

... We then updated to PVCam 2.7.4.2, but we still see corrupt images if we don't close and reopen the camera after every exposure sequence, and the camera sometimes fails to respond to a trigger pulse. ... Close and re-init the camera, as follows: ... pl_cam_close(0) pl_pvcam_uninit() pl_pvcam_init() . ... power off camera . ... Call pl_exp_start_cont (to start a continuous exposure sequence into a circular buffer) with a circular buffer that holds too many images and you will hang your computer. ...

The ut1.dat file contains the corrections made to UT1R-TAI time which is used by the Tempo and Tempo2. ... The corrections are published monthly by the International Earth Rotation Service (IERS) in several IERS bulletins Bulletins B, C, D'. ... The script `getut1' extracts UT1R - TAI for every 5th day and places it in the file ut1.tmp. ... Extract the required UT1 - UTC offsets using the script `getut1' %getut1 B.nnn This produces a file ut1.tmp in the iers directory. ...

. Comedi Documentation . Prev . Next . comedi_sv_update -- slowly-varying inputs . #include <comedilib.h> . int comedi_sv_update (comedi_sv_t * sv); . The function comedi_sv_update() updates internal parameters of the slowly varying Comedi structure sv. Prev . Home . Next . comedi_sv_init . Up . comedi_sv_measure

... This is not important for drift observations but poses a problem for any observing mode in which the telescope is moving while taking data, since the ALFA beams then will be rotating on the sky. ... The new mode is called ' sky angle tracking ' and is available for all existing observing modes. ... The next figure shows the distance between the beams in declination as a function of hour angle when the telescope is tracking a source with Dec=+10 from rise to set with a sky angle of 19 degrees. ...

The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...