Individual Surveys: Polaris Flare (DHT16)

Heithausen, Stacy, de Vries, Mebold, & Thaddeus (1993), A&A, 268, 265

move cursor over image for interpolated version

FITS Cubes
2.0 MB each
Raw:    DHT16_Polaris_raw.fits
Raw Header:    DHT16_Polaris_raw.txt
Interpolated*:    DHT16_Polaris_interp.fits
Moment masked**:    DHT16_Polaris_bw_mom.fits

* In each spectrum, <= 2 missing channels are filled by linear interpolation. In each spatial
plane, single missing pixels are filled by linear interpolation, first in l direction, then b.

** Two moment masked cubes are provided, one covering the smaller area with uniform
beamwidth sampling and the other covering the whole area with 1/4° sampling.


Owing to the high latitude of this survey, the longitude spacing of the observations is 0.1429°, slightly larger than our normal "beamwidth" spacing of 0.125°. For incorporation into the whole-Galaxy cubes presented elsewhere in the archive, the Polaris spectra were interpolated onto a standard beamwidth spaced grid.