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Table 1

Observed fields.

Galaxy α and δ PAmaj q Distance ′/kpc scale Prog./field Filter Frames Exptime r/m
(h, o) (o) (Mpc) (s) (′)

NGC 4 30 48.8 117.0 0.43 3.041 1/0.885 10885/1 F606W 32 33 600 7.00/14.23
1569 +64 50 56.1 10885/1 F814W 16 17 600
10885/2 F606W 24 25 600 7.17/13.33
10885/2 F814W 4 4000
8059/1 F606W 3 1800 5.16/12.03
8059/1 F814W 5 3200
8059/2 F606W 5 5600 5.16/7.50
8059/2 F814W 6 4100

NGC 12 28 11.2 42.4 0.50 3.822 1/1.111 10585/1 F606W 4 3600 5.67/8.29
4449 +44 05 36.9 10585/1 F814W 4 6000
10585/2 F606W 4 3600 7.83/10.22
10585/2 F814W 4 5793

Notes. Adopted galaxy center coordinates (α and δ), major axis position angles (PAmaj), axial ratios (q), distances and corresponding arcmin/kpc scales; number of frames, total exposure times and galactocentric radii (r) and elliptical radii (m) for each WFPC2 pointing. The axial ratios and position angles were calculated by taking typical values from the IRAF ellipse task isophote fits at 2 arcmin radii. Elliptical radii m were calculated according to the following formula: m2 = x2 + (y2/q2) where x and y are projected major and minor axis distances, respectively.

References. 

(1)

Grocholski et al. (in prep.);

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