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

Individual Surveys: Chamaeleon (DHT34)

Boulanger, Bronfman, Dame, & Thaddeus (1998), A&A, 332, 273




Sampling
move cursor over image for interpolated version


FITS Cubes
332 kB each
Raw:    DHT34_Chamaeleon_raw.fits
Raw Header:    DHT34_Chamaeleon_raw.txt
Interpolated*:    DHT34_Chamaeleon_interp.fits
Moment masked:    DHT34_Chamaeleon_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.

Comments

The sampling is tightly constrained to the emission region. The infrared analysis in DHT2001 suggests that there is more emission outside the sampling boundary.

CENTER FOR ASTROPHYSICS | HARVARD & SMITHSONIAN
60 GARDEN STREET, CAMBRIDGE, MA 02138