#1 VELOCITY FRAMES and SOURCE CATALOGS Files named 'anything'.cat may be used to list sources and coordinates. Your area contains the example dummy.cat. Use any text editor to prepare similar catalogs for your observing run. If you wish, simply modify dummy.cat and rename it using the UNIX command mv dummy.cat `anything'.cat where 'anything' is the catalog name convenient for you. Permitted coordinate frames include B1950.0--the usual reference frame (B stands for Besselian), J2000.0 and GALACTIC. Velocities are in units of km/s. The telescope control system supports four spectral line velocity frames: Local Standard of Rest (LSR), Heliocentric (HEL), Geocentric (GEO), and Topocentric (TOP). The velocity frame abbreviation is shown on the on-line status monitor. The default frame when the entire system is reloaded is LSR. Also shown on the status monitor is the Velocity Type, or definition, which can be Radio (RAD), Optical (OPT), or Relativisitic (REL). The system default is RAD. For extragalactic sources, observers may want to consult Section 6.1 of the paper "Observations of radio lines from unresolved sources:telescope coupling, Doppler effects, and cosmological corrections" by Gordon, Baars, and Cocke 1992 A&A October for information on the meaning of the Doppler velocities. (The Millimeter-Wave Calibration notebook contains a copy of the paper.) Observers should indicate the velocity frame explicitly on their source catalog entries. Although blank field is interpreted as LSR, we recommend that you explicitly type LSR to leave no doubt as to what was intended. The system will not accept the old FORTH designation of KM/S; if the entry contains KM/S, an error message will be printed on the operator's console and the existing velocity will not be changed. Observers may also indicate the velocity type (RAD, OPT, or REL) on their source catalog entries. A blank field will be interpreted as RAD. The general format for RA/DEC coordinates is HH:MM:SS.SS sDD:MM:SS.S Coord-frame Name sVV.V Vel-frame Vel-Type Example: 09:45:14.80 13:30:41.0 B1950 IRC+10216 -26.0 LSR RAD P. R. Jewell and M. A. Gordon 24 October 1992