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91 to 100 of 156 Results

2MASS Final Ophiuchus Extinction Map Oct 18, 2012 - COMPLETE Dataverse COMPLETE team, 2011, "2MASS Final Ophiuchus Extinction Map", https://doi.org/10.7910/DVN/VP6WDO, Harvard Dataverse, V2 Description: Extinciton maps made from 2MASS and NICER (Near Infrared Extinction-method Revisited). This map is made from the final 2MASS data release and cover all of Ophiuchus. The data values are magnitudes of visual extinction (Av). At the center of the cloud (high extinction) there is a small hole, and a few other defects are present, includin...
2MASS Final Perseus Extinction Map Oct 18, 2012 - COMPLETE Dataverse COMPLETE team, 2011, "2MASS Final Perseus Extinction Map", https://doi.org/10.7910/DVN/C58EYS, Harvard Dataverse, V2 Description: Extinciton maps made from 2MASS and NICER (Near Infrared Extinction-method Revisited). This map is made from the final 2MASS data release and cover all of Perseus. The data values are magnitudes of visual extinction (Av). Consult the error map and stellar density map to identify any problematic regions (few in this map). Versions in ga...
Replication data for: Second Quadrant, half-beamwidth sampled (DHT17) Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Second Quadrant, half-beamwidth sampled (DHT17)", https://doi.org/10.7910/DVN/VGEG6S, Harvard Dataverse, V3 This survey half-beamwidth (0.0625°) samples the Galactic plane over a range larger than the entire second quadrant. 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 and allows...
Replication data for: Cygnus X (DHT10) Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Leung, H. O.; Thaddeus, P, 2011, "Replication data for: Cygnus X (DHT10)", https://doi.org/10.7910/DVN/SVDGH9, Harvard Dataverse, V3 This survey is also incorporated into the large second quadrant surveys ( DHT17 & DHT18). However, in those surveys the Cygnus spectra are smoothed and interpolated onto a channel spacing of 1.300 km/s. In addition, in DHT18 the data are spat ially smoothed and interpolated onto a 1/4° grid. Thus, the original survey given here, with beamwidth samp...
Replication data for: Aquila South (DHT06) Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Aquila South (DHT06)", https://doi.org/10.7910/DVN/JSVPAN, 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.
Replication data for: Aquila Rift, low b section (DHT04) Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Aquila Rift, low b section (DHT04)", https://doi.org/10.7910/DVN/CBFTKF, Harvard Dataverse, V3 This survey maps two small clouds located about 7° below the Galactic plane. The survey parameters are identical to those of the main Aquila survey above the plane. In Figure 1 of DHT2001, this survey was incorrectly shaded to correspond to the first quadrant survey (DHT08).
Replication data for: Pegasus-East (DHT13) Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Pegasus-East (DHT13)", https://doi.org/10.7910/DVN/DIJ5BF, 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.
Replication data for: Taurus-South (DHT23) Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Taurus-South (DHT23)", https://doi.org/10.7910/DVN/HBZFDF, 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: Panchromatic Observations of SN2011dh Oct 18, 2012 - Supernova Forensics Dataverse Alicia Soderberg, 2012, "Replication data for: Panchromatic Observations of SN2011dh", https://doi.org/10.7910/DVN/IW3ZVX, Harvard Dataverse, V2 We report the discovery and detailed monitoring of X-ray emission associated with the Type IIb SN 2011dh using data from the Swift and Chandra satellites, placing it among the best studied X-ray supernovae to date. We further present millimeter and radio data obtained with the SMA, CARMA, and EVLA during the first three weeks after explosion. Combi...
Replication data for: Whole Galaxy Oct 18, 2012 - 1.2 Meter CO Survey Dataverse Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Whole Galaxy", https://doi.org/10.7910/DVN/WH9OQR, Harvard Dataverse, V3 Available data are raw, interpolated, and moment-masked versions of a large (1.3 GB) FITS cube containing the entire CO archive: all longitudes, all velocities (± 320 km/s), and ± 30° of latitude. While this cube can be very useful for large-scale Galactic studies, one should keep in mind that the component surveys vary somewhat in sensitivity, gri...

2MASS Final Ophiuchus Extinction Map

Oct 18, 2012 - COMPLETE Dataverse

COMPLETE team, 2011, "2MASS Final Ophiuchus Extinction Map", https://doi.org/10.7910/DVN/VP6WDO, Harvard Dataverse, V2

Description: Extinciton maps made from 2MASS and NICER (Near Infrared Extinction-method Revisited). This map is made from the final 2MASS data release and cover all of Ophiuchus. The data values are magnitudes of visual extinction (Av). At the center of the cloud (high extinction) there is a small hole, and a few other defects are present, includin...

2MASS Final Perseus Extinction Map

Oct 18, 2012 - COMPLETE Dataverse

COMPLETE team, 2011, "2MASS Final Perseus Extinction Map", https://doi.org/10.7910/DVN/C58EYS, Harvard Dataverse, V2

Description: Extinciton maps made from 2MASS and NICER (Near Infrared Extinction-method Revisited). This map is made from the final 2MASS data release and cover all of Perseus. The data values are magnitudes of visual extinction (Av). Consult the error map and stellar density map to identify any problematic regions (few in this map). Versions in ga...

Replication data for: Second Quadrant, half-beamwidth sampled (DHT17)

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Second Quadrant, half-beamwidth sampled (DHT17)", https://doi.org/10.7910/DVN/VGEG6S, Harvard Dataverse, V3

This survey half-beamwidth (0.0625°) samples the Galactic plane over a range larger than the entire second quadrant. 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 and allows...

Replication data for: Cygnus X (DHT10)

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

Leung, H. O.; Thaddeus, P, 2011, "Replication data for: Cygnus X (DHT10)", https://doi.org/10.7910/DVN/SVDGH9, Harvard Dataverse, V3

This survey is also incorporated into the large second quadrant surveys ( DHT17 & DHT18). However, in those surveys the Cygnus spectra are smoothed and interpolated onto a channel spacing of 1.300 km/s. In addition, in DHT18 the data are spat ially smoothed and interpolated onto a 1/4° grid. Thus, the original survey given here, with beamwidth samp...

Replication data for: Aquila South (DHT06)

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Aquila South (DHT06)", https://doi.org/10.7910/DVN/JSVPAN, 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.

Replication data for: Aquila Rift, low b section (DHT04)

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

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

This survey maps two small clouds located about 7° below the Galactic plane. The survey parameters are identical to those of the main Aquila survey above the plane. In Figure 1 of DHT2001, this survey was incorrectly shaded to correspond to the first quadrant survey (DHT08).

Replication data for: Pegasus-East (DHT13)

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Pegasus-East (DHT13)", https://doi.org/10.7910/DVN/DIJ5BF, Harvard Dataverse, V3

Replication data for: Taurus-South (DHT23)

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Taurus-South (DHT23)", https://doi.org/10.7910/DVN/HBZFDF, 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: Panchromatic Observations of SN2011dh

Oct 18, 2012 - Supernova Forensics Dataverse

Alicia Soderberg, 2012, "Replication data for: Panchromatic Observations of SN2011dh", https://doi.org/10.7910/DVN/IW3ZVX, Harvard Dataverse, V2

We report the discovery and detailed monitoring of X-ray emission associated with the Type IIb SN 2011dh using data from the Swift and Chandra satellites, placing it among the best studied X-ray supernovae to date. We further present millimeter and radio data obtained with the SMA, CARMA, and EVLA during the first three weeks after explosion. Combi...

Replication data for: Whole Galaxy

Oct 18, 2012 - 1.2 Meter CO Survey Dataverse

Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Whole Galaxy", https://doi.org/10.7910/DVN/WH9OQR, Harvard Dataverse, V3

Available data are raw, interpolated, and moment-masked versions of a large (1.3 GB) FITS cube containing the entire CO archive: all longitudes, all velocities (± 320 km/s), and ± 30° of latitude. While this cube can be very useful for large-scale Galactic studies, one should keep in mind that the component surveys vary somewhat in sensitivity, gri...

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