The whole-Galaxy CO survey presented in Dame et al. (2001) is a composite of 37 separate surveys that are described and numbered in Table 1 of the paper. The data from most of these surveys can be accessed by clicking on the survey number in the map below, which is Figure 1 from the paper. Larger composites of these individual surveys are available from the link below. Galactic Center (DHT02) Galactic Center (DHT02) Camelopardalis (DHT19) Lambda-Orionis (DHT24) Pegasus-West (DHT11) Taurus (DHT21) Taurus (DHT21) Polaris Flare (DHT16) Chamaeleon (DHT34) Fourth Quadrant (DHT36) Carina (DHT33) Third Quadrant (DHT31) Orion (DHT27) Canis Major (DHT30) Gum Nebula (DHT32) Cygnus X (DHT10) Lacerta (DHT12) Cassiopeia A (DHT14) SNR CTA 1 (DHT15) Second Quadrant, half-beamwidth sampled (DHT17) Second Quadrant, half-beamwidth sampled (DHT17) Second Quadrant, half-beamwidth sampled (DHT17) Second Quadrant, half-beamwidth sampled (DHT17) Second Quadrant, 1/4° sampled (DHT18) Second Quadrant, 1/4° sampled (DHT18) Second Quadrant, 1/4° sampled (DHT18) Second Quadrant, 1/4° sampled (DHT18) Second Quadrant, 1/4° sampled (DHT18) Second Quadrant, 1/4° sampled (DHT18) Second Quadrant, 1/4° sampled (DHT18) Gem OB1 (DHT22) Monoceros OB1 (DHT26) Canis Major (DHT30) Hercules (DHT09) Aquila Rift, main survey (DHT04) Aquila Rift, low b section (DHT04) Ophiuchus (DHT37) Ophiuchus (DHT37) Gemini (DHT25) Canis Minor (DHT28) Monoceros (DHT29) Coalsack (DHT35) First Quadrant, high z search (DHT07) First Quadrant, high z search (DHT07) First Quadrant, high z search (DHT07) First Quadrant, high z search (DHT07) First Quadrant, high z search (DHT07) First Quadrant, main survey (DHT08) First Quadrant, main survey (DHT08) First Quadrant, main survey (DHT08) First Quadrant, main survey (DHT08) First Quadrant, main survey (DHT08) First Quadrant, main survey (DHT08) Sagittarius South (DHT05) Aquila South (DHT06) R CrA (DHT03) R CrA (DHT03) Pegasus-East (DHT13) Ursa Major, Heithausen (DHT20) Ursa Major, de Vries (DHT20) Taurus-South (DHT23) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01) Superbeam (DHT01)
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DHT13_Pegasus-East_raw.txt
Jul 17, 2011 - Replication data for: Pegasus-East (DHT13)
Plain Text - 2.7 KB - MD5: 8938716755e67c0b76c9090b651c5345
FITS Header File
FITS header for DHT13
DHT13_raw.jpg
DHT13_raw.jpg
Jul 17, 2011 - Replication data for: Pegasus-East (DHT13)
JPEG Image - 88.8 KB - MD5: 6e6bb20f8b3e8e359cf660416de39a7f
Image File
Sampling map for DHT13, raw
DHT23.jpg
DHT23.jpg
Jul 17, 2011 - Replication data for: Taurus-South (DHT23)
JPEG Image - 83.0 KB - MD5: 499cdb57baeb134dffee3bdb78e3554e
Image File
Spatial and longitude-velocity maps of DHT23
DHT23_raw.jpg
DHT23_raw.jpg
Jul 17, 2011 - Replication data for: Taurus-South (DHT23)
JPEG Image - 135.5 KB - MD5: 031c32cde69d9fa5292f93186330cfd1
Image File
Sampling map for DHT23, raw
DHT23_Taurus-South_interp.fits
Jul 17, 2011 - Replication data for: Taurus-South (DHT23)
Plain Text - 47.8 KB - MD5: 917a727055160447d9a20c3274c144f2
FITS File
DHT23 v-l-b FITS cube, interpolated. 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.
DHT23_Taurus-South_mom.fits
Jul 17, 2011 - Replication data for: Taurus-South (DHT23)
Plain Text - 47.8 KB - MD5: c7a5e40da3e413b8a3f98ab456afa4c1
FITS File
DHT23 v-l-b FITS cube, moment masked
DHT23_Taurus-South_raw.fits
Jul 17, 2011 - Replication data for: Taurus-South (DHT23)
Plain Text - 47.8 KB - MD5: 14b7c5ec2c6ee91cfcf5fb4b99d58e5e
FITS File
DHT23 v-l-b FITS cube, raw
DHT23_Taurus-South_raw.txt
Jul 17, 2011 - Replication data for: Taurus-South (DHT23)
Plain Text - 2.7 KB - MD5: 31c575f62a684505647ea39754625ea3
FITS Header File
FITS header for DHT23
DHT28_CanisMinor_interp.fits
Jul 17, 2011 - Replication data for: Canis Minor (DHT28)
Plain Text - 978.8 KB - MD5: c401f6c3ec1a74e41dd04baeacc61c88
FITS File
DHT28 v-l-b FITS cube, interpolated. 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.
DHT28_CanisMinor_mom.fits
Jul 17, 2011 - Replication data for: Canis Minor (DHT28)
Plain Text - 978.8 KB - MD5: 36118db497ca2a64adf7440aeedd58d3
FITS File
DHT28 v-l-b FITS cube, moment masked
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