11 to 20 of 305 Results
Ungerechts, H.; Umbanhowar, P.; Thaddeus, P., 2011, "Replication data for: Cassiopeia A (DHT14)", https://doi.org/10.7910/DVN/FT2MEO, Harvard Dataverse, V3
This survey is also incorporated into the large second quadrant surveys ( DHT17 & DHT18). However, in those surveys the CasA spectra are smoothed and interpolated onto a channel spacing of 1.300 km/s. In addition, in DHT18 the data are spatia lly smoothed and interpolated onto a 1/4° grid. Thus, the original survey given here, with beamwidth sampli... |
Wilson, B. A.; Dame, T. M.; Masheder, M. R. W.; Thaddeus, P., 2011, "Replication data for: Orion (DHT27)", https://doi.org/10.7910/DVN/MW6HM7, Harvard Dataverse, V3
The sampling of this survey was unique among those in the archive -- two interleaved 0.125 ° grids. For the cubes presented here, the data were spatially smoothed and placed on a single 0.125° grid. The interpolated cube is recommended as it fills in a small number of missing spectra at random locations as well as the 1/4° sampling on the survey's... |
Oliver, R. J.; Masheder, M. R. W.; Thaddeus, P., 2011, "Replication data for: Monoceros OB1 (DHT26)", https://doi.org/10.7910/DVN/SWIR8K, Harvard Dataverse, V3
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Boulanger, F.; Bronfman, L.; Dame, T. M.; Thaddeus, P., 2011, "Replication data for: Chamaeleon (DHT34)", https://doi.org/10.7910/DVN/S2RDTX, Harvard Dataverse, V3
The sampling is tightly constrained to the emission region. The infrared analysis in DHT2001 suggests that there is more emission outside the sampling boundary. |
Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Lacerta (DHT12)", https://doi.org/10.7910/DVN/OSOE1E, 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). In nearly all cases molecular gas was detected. |
Stacy, J. A.; Thaddeus, P., 2011, "Replication data for: Gem OB1 (DHT22)", https://doi.org/10.7910/DVN/83LWX5, Harvard Dataverse, V3
The user is cautioned on the odd sampling pattern outside the limits of the main cloud, a pattern that is not substantially improved in the interpolated cube. |
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: Superbeam (DHT01)", https://doi.org/10.7910/DVN/G623C8, Harvard Dataverse, V3
This is a composite of four of the so-called "superbeam" surveys published in the original "Composite CO Survey of the Entire Milky Way" (Dame et al. 1987). The effective angular resolution and grid spacing of these surveys is 1/2 °, so they should only be used as a last resort. The area covered by the other superbeam surveys has largely been reobs... |
Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Taurus (DHT21)", https://doi.org/10.7910/DVN/JPZTBQ, Harvard Dataverse, V6
Owing to the frequency switching mode used for this survey, its velocity range is relatively small, -22 to 30 km/s. This range is adequate to cover essentially all the CO emission at b < -5, but not so at higher latitudes closer to the Galactic plane. In the range b = -5 to -2 it is better to use one of the second quadrant surveys (DHT17 or DHT18),... |
Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Second Quadrant, 1/4° sampled (DHT18)", https://doi.org/10.7910/DVN/MVX68A, Harvard Dataverse, V5
This is the single survey with the largest angular extent, covering more than the entire second quadrant over a wide latitude range. The sampling is 1/4 °. Spectra spaced every 1/4° were extracted from the Cygnus, CasA, and MonOB1 surveys and included in the cubes presented here. All the spectra were interpolated to a channel spacing of exactly 1.3... |
Nyman, L. -A.; Bronfman, L.; Thaddeus, P., 2011, "Replication data for: Coalsack (DHT35)", https://doi.org/10.7910/DVN/FJTHAH, Harvard Dataverse, V3
The survey was conducted with the 100 kHz filterbank on the southern telescope, providing a velocity resolution of 0.26 km/s over 67 km/s. The velocity range in the cube is narrow, -10 to 8 km/s, but apparently adequate to cover all the emission from the Coalsack cloud. |
