ALMA TST2.0

Note: The published or PI-provided results are available with the test data for comparison; remember that fits cubes/images can be viewed directly in the viewer tool without conversion.

Orion NGC 4826
The BIMA Survey of Nearby Galaxies (BIMA SONG). II. The CO Data
AIPS++ reduced image (feather)
300x300 image, 2.0" grid; Maximum value 1.645553e+00 at [161, 133, 1, 1] (05:35:16.131, -05.23.42.790, I, 8.4351e+09Hz); Rms = 2.970394e-01
AIPS++ reduced image
256x256 image, 1" grid, 0th moment; Maximum value 1.501140e+02 at [138, 123, 1] (12:56:43.594, +21.40.59.100, I); Rms = 1.470170e+01
PI reduced image (AIPS++)
300x300 image, 2.0" grid;Maximum value 1.645553e+00 at [161, 133, 1, 1] (05:35:16.131, -05.23.42.790, I, 8.4351e+09Hz); Rms = 2.970394e-01
MIRIAD reduced image
343x333 image , 1" grid, 0th moment; Maximum value 1.511604e+02 at [182, 161, 1, 1] (12:56:43.521, +21.40.59.098, 1.15112e+11Hz, I); Rms = 1.873132e+01