{ "aliases": {}, "cgroups": [ [ "auto001", { "columns": [ [ "_id", "u8" ], [ "obj_id", "u8" ], [ "ra", #The mean RA of all detections of the object "f8" ], [ "dec", #The mean DEC of all detections of the object "f8" ], [ "posstdev", # The standard deviation of positional errors in all detections "f4" ], [ "ra_ok", #The mean RA of all *good* detections of the object "f8" ], [ "dec_ok", #The mean DEC of all *good* detections of the object "f8" ], [ "posstdev_ok", # The standard deviation of positional errors in all *good* detections "f4" ], [ "ndet", #The total number of detections of this object in all filters "i2" ], [ "ndet_ok", #The total number of all good detections of this object in all filters. "i2" ], [ "nmag", #The total number of detections of this object in each filter "5i2" ], [ "nmag_ok", #The total number of *good* detections of this object in each filter "5i2" ], [ "mean", #The mean flux in each filter "5f4" ], [ "stdev", #The standard deviation of good detections of this object's flux in each filter "5f4" ], [ "err", #The formal uncertainty in the inverse variance weighted mean "5f4" ], [ "median", #The median flux in each filter "5f4" ], [ "q25", #The 25th percentile flux in each filter "5f4" ], [ "q75", #The 75th percentile flux in each filter "5f4" ], [ "ndet_ap", #Same as ndet but for aperture magnitudes (not recommended for stars, use psf magnitudes instead). "i2" ], [ "ndet_ap_ok", #Same as ndet_ok but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "i2" ], [ "nmag_ap", #Same as nmag but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5i2" ], [ "nmag_ap_ok", #Same as nmag_ok but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5i2" ], [ "mean_ap", #Same as mean but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5f4" ], [ "stdev_ap", #Same as stdev but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5f4" ], [ "err_ap", #Same as err but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5f4" ], [ "median_ap", #Same as median but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5f4" ], [ "q25_ap", #Same as q25 but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5f4" ], [ "q75_ap", #Same as q75 but for aperture magnitudes (not recommended for stars, use psf magnitudes instead) "5f4" ], [ "maglimit", #The magnitude limit of the deepest exposure in which a given object was taken, at the given location in the exposure "5f4" ], [ "epochrange", #The difference in time (in days) between the first and last detection of an object "f8" ], [ "epochrange_ok", #The difference in time (in days) between the first and last *good* detection of an object "f8" ], [ "epochmean", # Mean epoch (MJD) of detections of this object "f8" ], [ "epochmean_ok", # Mean epoch (MJD) of *good* detections of this object "f8" ] ], "commit_hooks": [ [ "Updating neighbors", 0, "lsd.tasks", "build_neighbor_cache" ] ], "primary_key": "_id", "spatial_keys": [ "ra", "dec" ] } ] ], "commit_hooks": [ [ "Updating neighbors", 0, "lsd.tasks", "build_neighbor_cache" ] ], "dt": 1, "fgroups": {}, "filters": { "complevel": 5, "complib": "blosc", "fletcher32": false }, "level": 6, "name": "ucal_fluxqz", "nrows": 0, "t0": 54335 }