Use the DSS Plate Finder to construct a list of Digitized Sky Survey plates
available for a specific region of the sky
and to select which plates to retrieve images from.
This utility will let you select plates based on the epoch, color, or
location of image on the plate.
Detailed instructions may be found below, but here's how you can get started quickly using the Plate Finder.
Enter either a coordinate pair (RA and Dec) or an object name to be resolved into coordinates.
(If you enter an object name, you can resolve it into coordinates before looking for plates,
or do it all in one step.) Then hit the Find plates button. The Plate Finder
will then look up the position among all the digitized plates currently in our jukebox
(if you entered a target name, it will resolve it into coordinates first) and present
you with a list of the plates from which an image can be extracted at that position, along
with some information about each plate: emulsion, filter, plate epoch, pixel resolution, etc.
You may then select a plate and extract the image from it.
The name of the astronomical object you want coordinates for.
This should be a fixed astronomical target; the name resolvers
cannot resolve moving objects (planets, comets, artificial satellites, etc.) into
their coordinates. The object name should be the name of a star, nebula, galaxy, etc.
If the Resolver (see below) is set to Region,
then the target name should be the name of a DSS plate, as given in the REGION
keyword in the FITS header.
The name resolver you want to use, if you want to get an object's coordinates;
or the name of a specific DSS plate.
To resolve an astronomical object's name into its coordinates (fixed targets only; planets,
comets, asteroids, etc. are not listed in the name resolvers' catalogs),
enter the object name in the Object Name field, select either
NED
or
SIMBAD
for the resolver, and hit the Get coordinates from button. The form will
be redrawn with the object's right ascension and declination entered as defaults in the RA
and Dec fields. Resolving an object name will not change any other choices
made in the form.
Alternatively, you can just hit the Find plates button instead of
Get Coordinates from, and the object name resolution and plate finding
will all be done in one step.
If you select Region for the Name Resolver, then instead of an astronomical
object, the Object Name will be interpreted as the name of a specific DSS plate,
as it appears in the REGION keyword of a DSS FITS header.
For example, an "object name" of XP443 will find the plate XP443.
In this case, pressing Get coordinates will redraw the form with the plate's
coordinates in place, while Find plates will go directly to the platemap
for that plate. (Currently, plate IDs such as A1VA, are not yet recognized.)
You can enter a Right Ascension and Declination in thses fields.
A number of formats are accepted for the RA and Dec. Here are some examples:
Decimal Degrees
185.63325 29.8959861111111
Hours, minutes and Seconds
12 22 31.98 29 53 45.55
12h22m31.98s 29d53m45.55s
12:22:31.98 +29:53:45.55
12h22'31.98" 29d53'45.55"
12h 22m 31.98s 29d 53m 45.55s
12h 22' 31.98" 29d 53' 45.55"
12h 22' 31.98" -29d 53' 45.55"
12h22'31".98 -29d53'45".55
12h22m31s.98 -29o53m45s.55
12h 22' 31".98 -29d 53' 45".55
Hours/Degrees and Minutes (no seconds)
12 22 29 53
12h22m +29d53m
12h22m 29d53m
12:22m 29:53m
12h22' 29d53'
12h 22m 29d 53m
12h 22' 29d 53'
12h 22' -29d 53'
The RA may be given in decimal degrees by indicating
a D or d after the degrees:
12d 22m 29d 53m
Spacing is not important, as long as the value is unambiguous, and that
you can delimit the hours/degrees, minutes, and (optional) seconds with
letters, colons, spaces, or any character that's not a digit or a
decimal point.
Note also that seconds of the form 31".98 or 31s.98 are accepted. This
should make it easy to cut and paste values into these fields from some
electronic publications. However, this is not true for minutes:
31'.98 will be parsed as 31 minutes, 0.98 seconds.
You can select either FITS or GIF for teh format of the data.
If you select FITS, the images will be sent back to your browser
with a MIME type of image/x-fits; if GIF, the MIME type will be image/gif.
The distance in arcminutes between the center of the extracted image
and the edge of the plate. The closer you are to the edge of a plate,
the more distortion you're likely to see. If you're close enough to the
plate edge, it will actually appear in your image as a sudden cutoff
in the astronomical part of the image. When an image center is less than
15.0 arcminutes of a plate edge, the number reported here will be rendered in red.
These are the bugs I know about. Since the Plate Finder is maintained
on a time-available basis (which means I can't spend too much time
working on it), I can't promise a schedule for fixes.
Big bug: Platemaps containing the 00h meridian don't show objects to the east of it.
Zoom in on a platemap.
Extract multiple images at once.
Plot catalogs on extracted images.
Efficiency improvments.
Several improvments to the code internals.
Add choices for catalogs in platemaps (colors, labels, etc).