5 The Functionality of catremote
The purpose of catremote
is to query remote astronomical databases. It has a number of separate
functions to realise this purpose, and each function corresponds to a mode of the program. The mode
to be used is specified when catremote
is run. The various modes are listed in Table 2 and described
briefly below. Running catremote
to invoke the various modes is described in detail in Section 6,
below.
-
list
- list all the databases which are currently available.
-
details
- show details of a named database.
-
query
- submit a query to a named database and retrieve the results. The basic type of query
supported is the ‘cone search’ or ‘circular area search’ which returns all the objects found
in a given circular area of sky. This area is specified by its central Right Ascension and
Declination and angular radius. The objects returned are formatted as a catalogue and
written to a local file.
-
name
- submit a name of an astronomical object to a remote name-resolver database. If the
name-resolver finds this name in its database then the Right Ascension and Declination
of the object are returned and displayed.
-
help
- list the modes available.
Mode | Description |
|
|
list | list the databases currently available |
details | show details of a named database |
query | submit a query to a remote database and retrieve the results |
name | resolve an object name into coordinates |
help | list the modes available |
|
Table 2: The modes of catremote
Copyright © 2001 Council for the Central Laboratory of the Research Councils