... Meta Index / Home Page This section documents warnings and errors generated by this task (if any). ... error . checkframes =yes and no input events file . ... invalid input events file . ... corrective action: restart from auxiliary file if you wish to reapply FRAMES . ... corrective action: check input events file . ... duplicate frame numbers found in the input file, all but one were dropped. corrective action: check in the input auxiliary file that the proper frames were selected for analysis . ...

... Classes . ... Class List . ... casa . casa::SolarPos . ... Solar position class and calculations. ... SolarPos (const SolarPos &other) . ... operator() ( Double epoch) . ... Barycentric position of Earth. const MVPosition & casa::SolarPos::baryEarthDerivative . ... Barycentric position of Sun. const MVPosition & casa::SolarPos::barySunDerivative . ... Double casa::SolarPos::checkEpoch [private] . ... Double casa::SolarPos::checkSunEpoch [private] . ... Double casa::SolarPos::deval [3] [private] . ...

... APPLY/DISPERSION in out [y] [coef] . Apply the dispersion relation to a 1D spectrum and generates a table . BATCH/LONG . ... CALIBRA/FLUX in out [resp] . Correct an image for the instrumental response function . ... Wavelength calibration of 1D and long-slit spectra . ... LINADD/LONG in w,bin [y] [mtd] [mode] [line] . ... PLOT/CALIBRATE [mode] . ... Plots a 1D spectrum in table format, as supplied by APPLY/DISPERSION . ... RESPONSE/LONG [plot] [fit] [deg] [smo] [table] [image] [visu] . ...

... Some users may wish to create their own calibration reference files or tables for certain parts of the pipeline calibration. IRAF/STSDAS tools exist to generate certain types of user reference files. ... Wavelengths : IRAF/STADAS tasks hst_calib.fos.y_calib.linefind and .hst_calib.fos.y_calib.dispfity are required. linefind is used to find the positions in a WAVE spectrum of candidate comparison lines from a template list of lines. ... In general, a spectrum of an object with few lines is used. ...

... A simulated HRI event list is generated from a set of user-specified source intensities, shapes and positions. ... Once this table has been created, qpsim is run to generate the qpoe file: Note that the ``bad attribute name `time''' message can be ignored, see help file. tt> qpsim Input source table file: source Reference QPOE file (xspatial$data/hdummy.qp): Root name for output files: simul ### Generating simulated data ### Beginning run of SIMEVT .. ... Skipping this source .. ...

To: file From: Jon Hagen Date: 12-22-00 Subject: Azimuth (or other axis) Encoder calibration When an encoder assembly (pinion gear, arbor, flex coupling, and encoder) has been removed and repaired, the encoder position must be recalibrated (reset to its standard position). The most obvious procedure is as follows: Procedure I Move the azimuth arm to a known "cal" position, identified by a pair of scribe marks or other prearranged hardware pointers. Suppose the cal position is 360.000 degrees. ...

Next: Determination of atmospheric parameters Up: Optical spectrum of IRAS04296 Previous: Radial velocity of the . From comparison of observed and synthetic spectra of IRAS04296 we revealed some strong absorptional features whose positions coincide with known diffuse interstellar bands (DIBs) (Jenniskens et al., ... In Fig. 5 we illustrate the presence of DIB's by showing a spectral region of IRAS04296 . ...

... The Advanced X-ray Astrophysics Facility's (AXAF) High and Low energy transmission gratings (HETG, LETG) data require new tools and data structures to support x-ray dispersive spectroscopy. ... The sky coordinates, which are referenced to the telescope mirror node and therefore independent of the grating reference node, are only useful for the imaging of zero order and the filtering of grating arm photons. ... For more details on the AXAF grating flight processing software, see: . ...

Next: Who We Are Up: annrep2004 Previous: Identified Media Mentions 2004 Contents . Armagh Observatory . New Targeting Social Need (New TSN) Action Plan 2005 . The Vision of the Armagh Observatory is: . To maintain and build on its position as a thriving astronomical research institute, and to continue to expand our understanding of the Universe and of humanity's place in it.' ... How We Contribute to New TSN . ...

Next: Identifications and Efficiency Up: THE DEEP X-RAY RADIO Previous: Source Classification . ... For some sources which did not have NVSS positions before the time of optical observations, arcsecond positions from the Texas survey (Douglas et al. 1996) and NED (typically based on VLA data) were used. ... All X-ray/radio sources without counterparts on the survey plates were imaged at either the KPNO 0.9m or the CTIO 0.9m telescopes. ... Previously Identified Sources . Sample Properties . ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...