... Finally at upper right is shown an ISO spectrum of another PPN candidate object, and in this case one sees both crystalline silicate dust and the aromatic/UIR features in the spectrum. ...
... The solar reference spectrum combines absolute flux measurements from satellites and from the ground with a model spectrum for the near-infrared (Colina, Bohlin, & Castelli 1996). ...
... SLITLESS displays the extracted, background subtracted spectrum, produces a text file listing the extracted spectrum (and background) and can optionally produce a FITS image of the background subtracted spectrum. ...
... Unfortunately, PSFs vary considerably from one end of the spectrum to the other, possibly introducing errors on the order of 10% in the photometry of the spectrum at any given wavelength for f /96 spectra. ...
... Figure 8.1: Spectrum resolving power as a function of wavelength for the GHRS medium ... one can expect, the range being from the blue end of the spectrum to the red ... FWHM) of lines from an exposure of a spectrum calibration lamp ...
... But time is also a dimension of the spectrum, in the sense of when the spectrum was obtained, how long the exposure lasted, and the extent of interruptions of that exposure. ...
... ASCA Observations of the GHz Peaked Spectrum Radio Galaxies 1345+125 and 2352+495. ... and GIS observations of two GHz peaked spectrum (GPS) radio galaxies, PKS 1345+125 ...
... 1 Fig. 2 Fig. 3 + Figure 1. JBand spectrum of Edd1 taken with IRTF. ... HBand spectrum of Edd1 taken with IRTF. The 2MASS magnitude in H is 12.107 +/0.060. ... KBand spectrum of Edd1 taken with IRTF. The 2MASS magnitude in K is 10.325 +/0.072. ...
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