THIS IS THE TASSBETA README AND DESCRIPTION FILE AND SHOULD BE STORED tassbeta.dat consists of over 380,000 TASS V and Ic measures. The data is courtesy of Tom Droege, taken on his own self made cameras, and the reference to the online database is http://sallman.tass-survey.org/servlet/markiv/ which is the reference to be used when measures are used. Positions are good to the arcsec or better. The V and Ic measures are averages of observations of at least ten and often far more V and Ic observations and the individual V and Ic observations are made simultaneously. Individual observations can be downloaded and plots of them examined at the above reference url. This particular list has been filtered in the hope of providing good quality V measures of standard stars. V-Ic is also included to help with colour determination. This is a beta catalogue, and as such a problem with preceding zeros in the sexagesimal position has not been resolved, although column integrity has been maintained. This can lead to declinations like -00 being written as - 0 for example. The Welch Stetson index is a means of assessing variation and variability in a data set of two colour photometry. Negative values show problematic photometry. Large values show variability if observations are large, and either star variability or data variation if less large values. This data set has been truncated at WS index values of 10 or less. WS indices of 50 or more are likely variables, when there are no data problems. The lower the WS index value the more likely there is no variation in the data. Assessment of WS index in relation to TASS data is still ongoing, and on occasion values of 9 may be better than values of 0.1. Clues and evidence on this is part of the beta test objectives. Assessment of WS index use in this could lead to either more strict limits, eg WS index <5 or lower, giving better quality data, or if alternatively most data with WS index < 10 was in fact of use and of usually good quality, the level may be increased to eg 20, thus allowing far more stars in the catalogue. COLUMNS 1 RA hours 2 RA minutes 3 RA seconds 4 Dec degrees 5 Dec minutes 6 Dec seconds 7 RA in decimal degrees (for use with TASS database interface, to check plots) 8 Dec in decimal degrees (for use with TASS database interface, to check plots) 9 Johnson V magnitude, given to 3 decimals so the user can decide on rounding The mean V magnitude from all measures of V 10 Error in V. Errors are root mean square means of each observational error and are _not_ standard deviations of all observations 11 Cousins Ic magnitude, given to 3 decimals so the user can decide on rounding The mean Ic magnitude from all measures of Ic 12 Error in Ic. Errors are root mean square means of each observational error and are _not_ standard deviations of all means 13 V-Ic. Colour (use Pickles' table for conversions) 14 Error on V-Ic. Calculated by square_root(meanV^2 + meanIc^2) 15 The number of observations that went in to the mean V and Ic values 16 How many nights the observations of V and Ic were taken over 17 The Welch-Stetson Index (an indicator of variation and variability) Data is courtesy of Tom Droege's observations, as processed by Michael Richmond's pipeline (www.tass-survey.org and links thereunder). J Greaves