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 Step 3: Generating a list of potential
targets
 
 Before scheduling a night's observations, you need to use program Targets to prepare a 
list of potential targets. This is a text file which summarizes the current information (such as
position, magnitude, rate of motion, etc.) about all potentially observable targets in
TAO's object databases. The list of potential targets
is one of the input files of the TAO scheduler, and
also serves as an aid in the process of selecting targets for observation on a given night based
on a number of criteria.
 
Customizing program Targets 
On the first time you run Targets, you should take some time to customize the program
to suit your particular needs. This may be done by editing the text file
TAO\targets\targets.cfg, which is the default configuration file
for program Targets. The configuration file allows you to specify data about your observing
station and filtering criteria to prevent targets in which you are not interested from 
appearing in the list of potential targets. The contents of this file are shown below: 
 
| STATION DATA:
  Latitude (deg):                                 -23.00056
  Longitude (deg, positive if east of Greenwich): -46.96506
  Range of observable declinations:
    Northern limit (deg):                         +34
    Southern limit (deg):                         -90
OBJECT FILTERS:
  List fixed targets? (yes/no)                    yes
  List moving targets? (yes/no)                   yes
    List asteroids? (yes/no)                      yes
      Exclude numbered asteroids? (yes/no)        yes
      Exclude main belt asteroids? (yes/no)       no
      Limiting magnitude for asteroids:           19.5
    List NEOCP objects? (yes/no)                  yes
      NEOCP ephemeris file:                       NEOCPeph.htm
    List comets? (yes/no)                         yes
  Exclude these priority codes:                   B, N, l
 |  
The various parameters which may be specified in this configuration file are explained 
below: 
 
  Latitude. Specify the latitude of the observing station
      (in degrees; north latitudes are positive).
  Longitude. Specify the longitude of the observing station
      (in degrees; longitudes east of Greenwich are positive).
  Range of observable declinations. Specify the northern
      and southern limits of the range of declinations (in degrees) which you could possibly observe 
      from your station. Note that horizon obstruction, light pollution, and other factors may
      reduce your range of observable declinations with respect to the maximal range determined
      by your latitude.
  List fixed targets? Answer yes
      if you wish that targets belonging to TAO's
      fixed object database appear in the list of potential targets.
  List moving targets? Answer yes
      if you wish that targets belonging to TAO's
      moving object database appear in the list of potential targets.
  List asteroids? Answer yes
      if you wish that minor planets appear in the list of potential targets.
  Exclude numbered asteroids? Answer yes
      if you wish to exclude numbered asteroids from the list of potential targets.
  Exclude main belt asteroids? Answer yes
      if you wish to exclude typical main belt asteroids from the list of potential targets.
      "Main belt asteroids" are here operationally defined as objects whose orbit has
      semi-major axis (a), eccentricity (e), and inclination (i) satisfying the
      inequalities 2.1 AU < a < 3.3 AU, e < 0.2, and  i < 15 deg.
  Limiting magnitude for asteroids. Minor planets whose
      predicted magnitude is fainter than this limit will not appear on the list of potential 
      targets. Due to the uncertainties in minor planet predicted magnitudes, you should set this
      limit to perhaps one magnitude fainter than your actual limiting magnitude.
  List NEOCP objects? Answer yes
      if you wish that objects listed on the 
      NEO Confirmation Page (NEOCP)
      appear on the list of potential targets.
  NEOCP ephemeris file. This is the name of the file
      containing current NEOCP ephemerides. The most convenient (and strongly recommended) way to
      obtain this file is by running script NEOCPMon; in this case,
      the name of the NEOCP ephemerides file will be NEOCPeph.htm.
  List comets? Answer yes
      if you wish that comets appear on the in the list of potential targets.
  
  Exclude these priority codes. Some objects in the
      list of potential targets will have a priority code, a single-character code which
      appears in front of the target name in the list of potential targets. For minor planets,
      the priority code is normally determined by program Targets based on the 
      desirability ratings for further observations which are given in the
      Minor Planet and Comet Ephemeris 
      Service output (click here
      for more details about the standard priority codes for
      minor planets). For fixed targets imported from external 
      catalog files, the priority codes may be assigned by the user when importing the targets,
      and may serve to identify targets imported from different catalogs, or which are of interest
      to different users. One may also manually assign priority codes by editing the text files
      TAO\targets\Fixed.txt (which lists all fixed targets in the database)
      and TAO\targets\Moving.txt (which lists all moving targets in the
      database); the priority code for a given target is specified in the first column of the
      corresponding record of these files. It is possible to exclude targets having certain priority
      codes from the list of potential targets. This is done by specifying a list of
      priority codes which should be excluded. The priority codes to exclude should be separated by
      commas.
 
Notes: 
   Different telescope users may wish to see a list of potential targets containing
       only those targets in which they are interested.
       This is may be achieved by using file TAO\targets\targets.cfg as a 
       template for creating other non-default configuration files for program Targets. For example,
       a user CGD whose sole interest is comets might use a configuration file
       TAO\targets\CGD.cfg with the following contents:
 
| STATION DATA:
  Latitude (deg):                                 -23.00056
  Longitude (deg, positive if east of Greenwich): -46.96506
  Range of observable declinations:
    Northern limit (deg):                         +34
    Southern limit (deg):                         -90
OBJECT FILTERS:
  List fixed targets? (yes/no)                    no
  List moving targets? (yes/no)                   yes
    List asteroids? (yes/no)                      no
      Exclude numbered asteroids? (yes/no)        no
      Exclude main belt asteroids? (yes/no)       no
      Limiting magnitude for asteroids:           19.5
    List NEOCP objects? (yes/no)                  no
      NEOCP ephemeris file:                       NEOCPeph.htm
    List comets? (yes/no)                         yes
  Exclude these priority codes:                   
 |  
       Program Targets could be run multiple times with different configuration files,
       each time producing a list of potential targets tailored to the interests of a particular
       user. 
   The telescope administrator (the person who actually schedules the observations for
       one or more telescope users) should always run Targets with an "all-inclusive"
       configuration file to produce a list of potential targets which includes all targets
       of potential interest to all telescope users. This list of potential targets would be
       one of the input files of the TAO 
       scheduler.
   If you make use of different instruments, which may be located at
       different geographical locations, each instrument might have a separate Targets
       configuration file.
 
 
Previous: Automated monitoring of the NEOCP (continued)Next: Running program Targets
 
 
 
 © 1999-2004 Paulo Holvorcem
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