The RTDC
Processing SMA Data
1.2 m Telescopes
AST/RO
Extra

Individual Surveys: Camelopardalis (DHT19)

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




Sampling
move cursor over image for interpolated version


FITS Cubes
4.5 MB each
Raw:    DHT19_Camelopardalis_raw.fits
Raw Header:    DHT19_Camelopardalis_raw.txt
Interpolated*:    DHT19_Camelopardalis_interp.fits
Moment masked**:    DHT19_Camelopardalis_bw_mom.fits
   DHT19_Camelopardalis_qdeg_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.

Comments

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 this archive, the Camelopardalis spectra were interpolated onto a standard beamwidth spaced grid.

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