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OF THE ROGER N. CLARK

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Appendix E<br />

A catalog of deep-sky objects<br />

This appendix lists the 611 deep-sky objects<br />

that, in the author's opinion, are the most<br />

interesting for amateur astronomers. The list<br />

represents a search of the literature for objects<br />

that are both interesting to observe and<br />

also have photographs widely available. I<br />

culled the information from many sources:<br />

Burnham's Celestial Handbook, magazines such<br />

as Sky & Telescope, Astronomy, and Deep Sky; Sky<br />

Catalog 2000.0 (Volume 2) , and professional<br />

journals such as the Astrophysical Journal.<br />

In compiling this catalog, the first step was<br />

to check that an object might be seen through<br />

average amateur telescopes. Then I searched<br />

for those that might show some features.<br />

Many objects within range of small telescopes<br />

were left out because they are so near<br />

the limits that most would just look like<br />

another fuzzy patch. The present list still has<br />

many of these (depending on your telescope<br />

size an sy quality), but many others clearly<br />

show slgmficant detail and have much text<br />

devoted to them in books like Burnham's.<br />

When going out for an observing session,<br />

one wants to know which objects will be visible<br />

that n .<br />

ight. Some books (e.g. Burnham's)<br />

are orgamzed alphabetically by constellation,<br />

so a search through the entire work is required<br />

in order to find out what there is to<br />

s <br />

e. This list, on the other hand, is ordered by<br />

nght ascension. For any given night, one can<br />

start at some point on the list and work<br />

downward.<br />

The following data are tabulated:<br />

ID: The NGC number of the object, or other<br />

atalog number if the object has no NGC<br />

:slgnation. The Messier number is also<br />

glv<br />

d<br />

en If appropriate. Before the ID several<br />

ax appear. An astensk (*) means the<br />

IS .<br />

Iscussed m the book and a drawing<br />

co es m . '<br />

obj ect '<br />

and<br />

Con: The constellation in which the object is<br />

located. The following standard abbrevia-<br />

tions are used:<br />

photograph are presented in Chapter 7.<br />

An S indicates the object is a star cluster with<br />

star magnitudes given in Appendix B. Exclamation<br />

points indicate the object is an<br />

es ecially fine-looking one, with four (!!!!)<br />

bemg the most spectacular visually.<br />

Positions: Positions in right ascension (RA)<br />

and declination (DEC) are tabulated fo r<br />

equinoxes 1950.0 and 2000.0. Both are given<br />

because star charts for both equinoxes are<br />

common. The RA is given in hours and de­<br />

imal minutes of time, and the DEC is given<br />

m degrees and arc-minutes. The objects are<br />

sorted by increasing 1950.0 RA. The positions<br />

in the catalog have been checked<br />

a ainst se eral other catalogs, and as many<br />

discrepanCIes as possible have been eliminated.<br />

One good reference is Sky Catalog 2000.0,<br />

Vo lume 2, by Hirshfeld and Sinnott (1985).<br />

The 2000.0 positions in this list have all been<br />

che ed ag inst Hirshfeld and Sinnott. Many<br />

pOSitIOns disagree in the last digit between<br />

the two catalogs, but the differences are not<br />

significant and can be attributed to round-off<br />

error, or to where the exact center of a large<br />

object was chosen (a center may not be obvious<br />

in open clusters and nebulae in particular)<br />

. When the position disagreement was<br />

significant, I investigated and chose the best<br />

position. In some cases that meant measuring<br />

photographs. Several small galaxies in the<br />

c uple-o:-arc-minute size range had positions<br />

dlsagreemg by about an arc minute or two.<br />

However, the coordinates are always accur<br />

te enough to find an object with setting<br />

CI rcles or by plotting on star charts, even at<br />

.<br />

high power.<br />

283

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