1.2 Meter CO Survey Dataverse

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.

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31 to 40 of 305 Results

Replication data for: Gemini (DHT25) Oct 18, 2012 Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Gemini (DHT25)", https://doi.org/10.7910/DVN/ONMHLN, Harvard Dataverse, V3 This is one of about a dozen relatively small surveys carried out to search for molecular clouds predicted by the infrared analysis of DHT2001 (shaded purple in Fig. 1; see Section 3.1.4).
Replication data for: R CrA (DHT03) Oct 18, 2012 Dame, T. M.; Ungerechts, H.; Cohen, R. S.; de Geus, E. J.; Grenier, I. A.; May, J.; Murphy, D. C.; Nyman, L. -A.; Thaddeus, P., 2011, "Replication data for: R CrA (DHT03)", https://doi.org/10.7910/DVN/2IZMNM, Harvard Dataverse, V3 The sampling is fairly tightly constrained to the emission region. The infrared analysis in DHT2001 suggests that there may be a bit more emission at more negative latitudes (see Fig. 8b).
Replication data for: Monoceros (DHT29) Oct 18, 2012 Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Monoceros (DHT29)", https://doi.org/10.7910/DVN/61ZUWZ, Harvard Dataverse, V3 This is one of about a dozen relatively small surveys carried out to search for molecular clouds predicted by the infrared analysis of DHT2001 (shaded purple in Fig. 1; see Section 3.1.4).
Replication data for: Galactic Center (DHT02) Oct 18, 2012 Bitran, M.; Bronfman, L.; May, J.; Thaddeus, P., 2011, "Replication data for: Galactic Center (DHT02)", https://doi.org/10.7910/DVN/7RMW6Q, Harvard Dataverse, V4 This is a high-quality survey of the Galactic center region carried out from Chile, where the center passed almost directly overhead. Users are cautioned of the coarser (1/4 °) sampling at \|b\| > 1 °; the interpolated cube is easier to use for most purposes.
Replication data for: Camelopardalis (DHT19) Oct 18, 2012 Heithausen, A; Stacy, J. G.; de Vries, H. W.; Mebold, U.; Thaddeus, P, 2011, "Replication data for: Camelopardalis (DHT19)", https://doi.org/10.7910/DVN/C4MYI3, Harvard Dataverse, V5 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.
Replication data for: Polaris Flare (DHT16) Oct 18, 2012 Heithausen, A; Stacy, J. G.; de Vries, H. W.; Mebold, U.; Thaddeus, P., 2011, "Replication data for: Polaris Flare (DHT16)", https://doi.org/10.7910/DVN/7H7H30, Harvard Dataverse, V3 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.
Replication data for: Fourth Quadrant (DHT36) Oct 18, 2012 Bronfman, L.; Alvarez, H.; Cohen, R. S.; Thaddeus, P., 2011, "Replication data for: Fourth Quadrant (DHT36)", https://doi.org/10.7910/DVN/OLINEC, Harvard Dataverse, V3 Interpolated cube is recommended owing to the 1/4° sampling at \|b\| > 1°
Replication data for: Lambda-Orionis (DHT24) Oct 18, 2012 Lang, W. J.; Masheder, M. R. W.; Dame, T. M.; Thaddeus, P., 2011, "Replication data for: Lambda-Orionis (DHT24)", https://doi.org/10.7910/DVN/ME5Y7C, Harvard Dataverse, V3 This survey was sampled every half-beamwidth (0.0625°), but for the cube presented here, the data have been spatially smoothed by convolution with a 2d gaussian with fwhm=0.125° and then put on a 0.125° grid. This improves the S/N ratio with only a slight loss of angular resolution.
Replication data for: Aquila Rift, main survey (DHT04) Oct 18, 2012 Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Aquila Rift, main survey (DHT04)", https://doi.org/10.7910/DVN/OQLN0Z, Harvard Dataverse, V3 Sampling is 1/4°. There is additional data for Aquila Rift low latitude section.
Replication data for: Pegasus-West (DHT11) Oct 18, 2012 Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Pegasus-West (DHT11)", https://doi.org/10.7910/DVN/7CLZTL, Harvard Dataverse, V4 This is one of about a dozen relatively small surveys carried out to search for molecular clouds predicted by the infrared analysis of DHT2001. In nearly all cases molecular gas was detected.

Replication data for: Gemini (DHT25)

Oct 18, 2012

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Gemini (DHT25)", https://doi.org/10.7910/DVN/ONMHLN, Harvard Dataverse, V3

This is one of about a dozen relatively small surveys carried out to search for molecular clouds predicted by the infrared analysis of DHT2001 (shaded purple in Fig. 1; see Section 3.1.4).

Replication data for: R CrA (DHT03)

Oct 18, 2012

Dame, T. M.; Ungerechts, H.; Cohen, R. S.; de Geus, E. J.; Grenier, I. A.; May, J.; Murphy, D. C.; Nyman, L. -A.; Thaddeus, P., 2011, "Replication data for: R CrA (DHT03)", https://doi.org/10.7910/DVN/2IZMNM, Harvard Dataverse, V3

The sampling is fairly tightly constrained to the emission region. The infrared analysis in DHT2001 suggests that there may be a bit more emission at more negative latitudes (see Fig. 8b).

Replication data for: Monoceros (DHT29)

Oct 18, 2012

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Monoceros (DHT29)", https://doi.org/10.7910/DVN/61ZUWZ, Harvard Dataverse, V3

This is one of about a dozen relatively small surveys carried out to search for molecular clouds predicted by the infrared analysis of DHT2001 (shaded purple in Fig. 1; see Section 3.1.4).

Replication data for: Galactic Center (DHT02)

Oct 18, 2012

Bitran, M.; Bronfman, L.; May, J.; Thaddeus, P., 2011, "Replication data for: Galactic Center (DHT02)", https://doi.org/10.7910/DVN/7RMW6Q, Harvard Dataverse, V4

This is a high-quality survey of the Galactic center region carried out from Chile, where the center passed almost directly overhead. Users are cautioned of the coarser (1/4 °) sampling at |b| > 1 °; the interpolated cube is easier to use for most purposes.

Replication data for: Camelopardalis (DHT19)

Oct 18, 2012

Heithausen, A; Stacy, J. G.; de Vries, H. W.; Mebold, U.; Thaddeus, P, 2011, "Replication data for: Camelopardalis (DHT19)", https://doi.org/10.7910/DVN/C4MYI3, Harvard Dataverse, V5

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.

Replication data for: Polaris Flare (DHT16)

Oct 18, 2012

Heithausen, A; Stacy, J. G.; de Vries, H. W.; Mebold, U.; Thaddeus, P., 2011, "Replication data for: Polaris Flare (DHT16)", https://doi.org/10.7910/DVN/7H7H30, Harvard Dataverse, V3

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.

Replication data for: Fourth Quadrant (DHT36)

Oct 18, 2012

Bronfman, L.; Alvarez, H.; Cohen, R. S.; Thaddeus, P., 2011, "Replication data for: Fourth Quadrant (DHT36)", https://doi.org/10.7910/DVN/OLINEC, Harvard Dataverse, V3

Interpolated cube is recommended owing to the 1/4° sampling at |b| > 1°

Replication data for: Lambda-Orionis (DHT24)

Oct 18, 2012

Lang, W. J.; Masheder, M. R. W.; Dame, T. M.; Thaddeus, P., 2011, "Replication data for: Lambda-Orionis (DHT24)", https://doi.org/10.7910/DVN/ME5Y7C, Harvard Dataverse, V3

This survey was sampled every half-beamwidth (0.0625°), but for the cube presented here, the data have been spatially smoothed by convolution with a 2d gaussian with fwhm=0.125° and then put on a 0.125° grid. This improves the S/N ratio with only a slight loss of angular resolution.

Replication data for: Aquila Rift, main survey (DHT04)

Oct 18, 2012

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Aquila Rift, main survey (DHT04)", https://doi.org/10.7910/DVN/OQLN0Z, Harvard Dataverse, V3

Sampling is 1/4°. There is additional data for Aquila Rift low latitude section.

Replication data for: Pegasus-West (DHT11)

Oct 18, 2012

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Pegasus-West (DHT11)", https://doi.org/10.7910/DVN/7CLZTL, Harvard Dataverse, V4

This is one of about a dozen relatively small surveys carried out to search for molecular clouds predicted by the infrared analysis of DHT2001. In nearly all cases molecular gas was detected.

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