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This page gives you easy access to individual images. Select a run, camcol and a field, as well as the image size from the form below. If you want to save an image to a disk, use this service. If you want to use this image on your website, feel free to do so, but please give us an acknowledgement.
Run
Camcol
Field   
Size

StripeRunField minField max
72483611271
4836345455
484368242
4843242343
484411168
485111119
487921193
488022110
647557158
79506511255
559811203
563611161
564011284
564111160
565511263
565611167
571411256
1020538411122
539676187
106261051177
540915125
54151190
53781154
5421155234
1100483234154
4832154203
4832203504
482851172
4828172221
4828221522
1140540311203
5403203306
541611203
617756309
685032182
1188618211197
6182197304
635430323
636115169
636658172
637128156
637235124
641322135
61691154
612211131
61231196
616214448
1220413457398
413516297
414412166
415225119
1260480011215
482927235
4829235320
581414163
60741159
60751164
595949188
596046153
5960153209
1300581711350
593411280
488711290
504411149
506041202
135650663445
600311289
648511213
650536192
650938173
657211127
657329233
659125141
1374658137216
658523202
67091188
672735114
651417205
651911199
1406717811226
659712166
660511165
670843258
1458657411209
674911208
1540678112138
597333159
597611145
598262142
59992276
1600600512220
612111219
1660617411229
61765292
616618276

Table for field ranges

The images from the SDSS project are organized into stripes. These are long images, 24,000 pixels wide (2.5 degrees), and typically over 1 million pixels long (120 degrees). The SDSS covers the northern sky with 45 overlapping stripes. The stripes are designed to avoid the dust in the plane of the Milky Way, shown as the red areas in the diagram at right.
Each stripe is merged from two runs, taken on separate nights. The telescope can complete only a single 8-hour run in any given night. Each run consists of 6 camcols (camera columns); each camcol corresponds to each array of CCD detectors of our camera. Each camcol takes images in five colors.