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3.2.3 The Individual Observations

The 64 program galaxies are distributed in 35 of the 43 fields (the 8 fields without program galaxies are the fields 21, 25, 32, 36, 44, 45, 213, and 632). The best seeing Gunn r images of these 35 fields are shown is Appendix [*] (p. [*]) with the 64 program galaxies marked. All 64 galaxies have been observed in Gunn r and Johnson B. 22 galaxies have also been observed in Johnson U. Some of the galaxies have been observed more than once due to field reobservations or due to being located in the overlap region between two fields. A detailed break-down of this is found in Table [*]. The entire list of observations is given in Table [*].


 
Table: Number of Galaxies and Observations
Filter #galaxies #observations #galaxies observed i times
      i=1 i=2 i=3 i=4
GR 64 104 35 20 7 2
JB 64 99 35 24 4 1
JU 22 24 20 2    
Total - 227 - - - -
 


 
Table: Chronological List of Observations
Night fwhm (GR) fwhm (JB) Field Notes Program galaxies
  [arcsec] [arcsec]      
1 1.7 1.7 00   R245, R253, R255, R256, R266, R268, R269, R273, R286, R293
1 1.6 1.7 16   R308
1 1.6 1.7 13   R209, R217, R234, R237, R241
1 1.3 1.4 25   -
1 1.3 1.4 37   R166, R185
1 1.3 1.6 18   R214, R219, R225
1 1.4 1.7 12   R255, R273, R278
1 1.8 2.1 21   -
1 1.7 1.9 33   R317
1 1.9 2.2 45   -
2 1.1 1.4 214   R261
2 1.2 1.4 320   R327
2 1.1 1.4 428   R250
2 1.2 1.3 632   -
2 1.1 1.3 29   R193
2 1.1 1.2 419   R138
2 1.3 1.7 519   R129
2 1.7 1.8 15   R213, R216, R224, R226, R239, R245
3 0.8 0.8 00 a R245, R253, R255, R256, R266, R268, R269, R273, R286, R293
3 0.9 0.8 14   R316, R322
3 0.8 0.9 15 a R213, R216, R224, R226, R239, R245
3 0.9 0.9 13 a, b R209, R217, R234, R237, R241
3 0.9 0.8 27   R188, R194, R209
3 0.9 0.9 23   R243
3 0.9 0.9 43   R338, R343, R347
3 0.9 1.1 18 a R214, R219, R225
3 0.9 1.1 321   R283, R288
3 1.0 1.2 535   R252, R295
3 1.2 1.3 35   R218, R231
4 0.8 0.9 46   R238
4 0.8 0.9 47   R202
4 0.8 0.9 34   R254
4 0.9 1.0 22   R319
4 0.9 0.9 26   R334, R359
4 1.0 1.0 24   R211, R212, R243
4 0.9 1.1 210   R336, R337
4 1.1 1.2 427   R305
4 1.0 1.2 215   R225
4 1.0 1.1 28   R336, R337, R340
4 1.1 1.3 33 a R317
6 1.3 1.3 213   -
6 1.1 1.4 39   R166
6 1.1 1.0 36   -
6 0.9 1.0 44   -
6 0.9 1.0 45   -
6 0.9 0.9 32   -
6 1.0 1.1 64   R389
6 0.9 1.2 66   R307
6 1.3 1.3 615   R112, R120
6 1.1 1.3 16 a R308
6 1.1 1.5 21   -
  fwhm (JU)        
  [arcsec]        
9 1.1   00 c R239, R245, R253, R255, R256, R266, R268, R269, R273, R286, R293
9 1.0   14   R316, R322
9 1.2   15 d R213, R216, R224, (R226), R239, R245
9 1.4   13 e, f R217, R234, R237, (R241)
9 1.6   18   R214, R219, R225
 
Notes: The seeing (`fwhm') is determined to better than the 1 decimal place shown here. $^{\rm a}$ Reobservation of a field containing program galaxies. $^{\rm b}$ Observed twice in GR. $^{\rm c}$ Offset so that R239 is included. $^{\rm d}$ R226 too faint for two-dim. photometry. $^{\rm e}$ Offset so that R209 is excluded and R255 is included - the latter was not fitted, however. $^{\rm f}$ R241 too faint for two-dim. photometry.


next up previous contents
Next: 3.3 The Basic Reductions Up: 3.2 Photometric Observations and Previous: 3.2.2 Selection of the

Properties of E and S0 Galaxies in the Clusters HydraI and Coma
Master's Thesis, University of Copenhagen, July 1997

Bo Milvang-Jensen (milvang@astro.ku.dk)