Revised photometric distances to nearby dwarf galaxies in the IC 342/Maffei complex J/A+AS/124/559 J/A+AS/124/559 VI photometry of dwarf galaxies Revised photometric distances to nearby dwarf galaxies in the IC 342/Maffei complex I Karanchentsev I Drozdovsky S Kajsin L O Takalo P Heinamaki M Valtonen Astron. Astrophys. Suppl. Ser. 124 559 1997 1997A&AS..124..559K Galaxies, photometry galaxies: distances and redshifts galaxies: irregular galaxies: stellar content Tables show the photometry and colour index for the observed galaxy, with the image parameter SHARP. This parameter is a measure of the difference between the observed width of the object and the psf model.
UGCA 10505 14.3 +62 34 UGCA 9204 32.0 +63 36 UGCA 8603 59.8 +67 08 NGC 156904 30.7 +64 51 Cas 1ZOAG 129.57+07.1102 06.1 +69 01
Photometry of the stars in the galaxy UGCA 105 Photometry of the stars in the galaxy UGCA 92 Photometry of the stars in the galaxy UGCA 86 Photometry of the stars in the galaxy NGC 1569 Photometry of the stars in the galaxy Cas 1 No Star number ----- Xpos X coordinate number=1 The XY positions were calculated from the SW corner (X,Y=0,0) of the image, with +X going to east and +Y to north. This corner is the lower-right corner of the image. pix Ypos Y coordinate number=1 The XY positions were calculated from the SW corner (X,Y=0,0) of the image, with +X going to east and +Y to north. This corner is the lower-right corner of the image. pix Vmag V magnitude mag V-I V-I colour index mag V-R V-R colour index mag SHARP Image parameter SHARP number=2 SHARP is a measure of the difference between the observed width of the object and the width of the psf model. ---- L [01] Marks the stars inside the visible boundary of the galaxy ----- fig6.psGalaxy UGCA 86 fig7.psUGCA 86 V--V-I diagram fig8a.psNGC 1569 Southern part fig8b.psNGC 1569 Northern part fig9.psNGC 1569 V--V-I diagram Patricia Bauer CDS 1997Jan06Leo Takalo <TAKALO@sara.cc.utu.fi> J_A+AS_124_559.xml