High-resolution imaging of Virgo cluster galaxies. I - Observational techniques and first results

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photography, Imaging Techniques, Virgo Galactic Cluster, Charge Coupled Devices, Contrast, High Resolution

Scientific paper

The potential of the image sharpening technique for making high-resolution images of Virgo cluster galaxies is investigated in order to obtain new estimates of this cluster's distance. Both the Galway Image Sharpening Camera and the MARTINI instrument at the William Herschel Telescope have been used to confirm Fried's 4r0 optimum aperture for image sharpening. Further, the MARTINI image sharpening instrument has been used to observe the Virgo galaxy, IC 3583. The resulting image has 0.60-arcsec FWHM seeing, but to a limiting magnitude of R = 21.7 mag the brightest stars in IC 3583 are not resolved. This tentatively suggests a lower limit to the Virgo distance modulus of m - M greater than 30.7 mag.

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