Difference: ZTFOpsCGI01 (1 vs. 2)

• Gal_Lat : Galactic latitude of center of field in degrees.
• Ecl_Lat : Ecliptic latitude of center of field in degrees.
• Moon_Sep : Separation between center of field and Moon position (middle of night) in degrees.

Create a list of fields visible on a given night

Give the UT date (YYYY-MM-DD) of the night of the observations, for example, 2017-10-16 (UT) would be for the night of Sunday, October 15, 2017 (Pacific Time). This list of fields will include all fields visible for the given minimal number of hours to the given maximum airmass. Choose the primary grid (IDs 1 to 879) or the secondary grid (IDs 1001 to 1895) or both. For more information on the ZTF grids see ZTFFieldGrid.

The output will be an ASCII text file with 5 columns:

• ID : ZTF field ID number
• RA : Right Ascension of field center (J2000).
• Dec : Declination of field center (J2000).
• Visible : the number of hours a field is visible on the given night to the maximum airmass.
• HA_limit : the hour angle limit in degrees that this field can be observed to the maximum airmass.

Go to CGI page: ZTF Operations CGI ..(username and password are the same as for transient marshal)

-- TomBarlow - 02 Oct 2017