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7.1 HST WFPC2 Image
The HST WFPC2 image on which the simulations presented in this Chapter are
based is a Planetary Camera (PC, see Section 6.1) image of the
central regions of the M100 spiral galaxy, obtained with a 900 s exposure
with the F555W filter.
This image was chosen because it contains most interesting features one would
like to observe in bright galaxies: a conspicuous core, large surface
brightness variations on short space scales, spiral arms and HII
regions7.1.
The central part of this image, namely a square of about 16 arcsec
side whose flux map was reconstructed from the simulated observations, is
shown in Figure 7.1.
Figure 7.1:
HST WFPC2 PC image of M100. Central part of a WFPC2 PC image of the spiral
galaxy M100, obtained with a 900 s exposure with the F555W filter, similar to
.
Encircled on the right image is the position of the eight zones used to
calculate the median surface brightness in Table 7.1 (letters
-) and of the five HII regions of which aperture photometry is carried
out in Section 7.7 (numbers 1-5).
The image side is about 16 arcsec and the circles have a diameter
of about 0.7 arcsec.
|
The median surface brightness in inside the eight circles marked by
letters is given in Table 7.1.
These values were calculated following the WFPC2 photometric calibration
obtained by [Holtzman et al. 1995b], and indicate the surface brightness range
spanned by the image.
Note that the median surface brightness of the whole image is
mag/arcsec.
M100 is classified as Sc(s)I in [Sandage and Bedke 1994] and the [de Vaucouleurs et al. 1991] report a
photoelectric total magnitude and an effective radius of about 104
arcsec, meaning that the sky region shown in Figure 7.1
covers its very central parts only.
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Mattia Vaccari
2000-12-05