Harvard-Smithsonian Center for Astrophysics Harvard Observatory Plate Stacks MC Series Characteristics |
Basics |
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Observatory |
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Online Searchable catalog |
Maps of spatial and temporal distribution |
Histogram by year |
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ASCII
(21983 plates)
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Location |
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Card Catalog: |
complete; there is also an Approach database of the blue plates. | |||||||||||||||||||
Record Books: |
(49) 1-37502 (Catalog)
(2) MC Important Regions (2) MC Long Period Variables (1) MC Photometric Work Online: [01] [02] [03] [04] [05] [06] [07] [08] [09] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22] [23] [24] [25] [26] [27] [28] [29] [30] [31] [32] [33] [34] [35] [36] [37] [38] [39] [40] [41] [42] [43] [44] [45] [46] [47] [48] [49] | |||||||||||||||||||
Record Sheets: |
26154-40591 | |||||||||||||||||||
Comments:[Expanded notes] |
This instrument, the most powerful refractor in the northern station up to 1936,
was especially valuable for faint objects where the large scale was of benefit.
When the plates are used for photometric purposes, it is well to take
precautions, since the color coefficient is large and the distance correction
is both large and variable from one plate to another.
The instrument was refigured after about 3500 plates had been taken; the distance correction was thereby diminished, but the color coefficient was practically unchanged. In general, it is well to avoid plates taken before the refiguring for accurate photometric work. All plates subsequent to 4171 were taken with the curved plate holder, which diminishes the distance correction due to curvature of field. |