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Part 1: Document Description
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Citation |
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Title: |
Replication data for: Taurus (DHT21) |
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Identification Number: |
doi:10.7910/DVN/JPZTBQ |
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Distributor: |
Harvard Dataverse |
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Date of Distribution: |
2011-07-06 |
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Version: |
6 |
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Bibliographic Citation: |
Dame, T. M.; Hartmann, Dap; Thaddeus, P., 2011, "Replication data for: Taurus (DHT21)", https://doi.org/10.7910/DVN/JPZTBQ, Harvard Dataverse, V6 |
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Citation |
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Title: |
Replication data for: Taurus (DHT21) |
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Identification Number: |
doi:10.7910/DVN/JPZTBQ |
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Authoring Entity: |
Dame, T. M. (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138) |
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Hartmann, Dap (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; Currently at Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, The Netherlands) |
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Thaddeus, P. (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138) |
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Distributor: |
Harvard Dataverse |
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Date of Deposit: |
2011-07-06 |
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Holdings Information: |
https://doi.org/10.7910/DVN/JPZTBQ |
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Study Scope |
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Abstract: |
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 (<a href="http://dvn1.rc.fas.harvard.edu/dvn/dv/rtdc/faces/study/StudyPage.xhtml?globalId=hdl:TEST/10019">DHT17</a> or <a href="http://dvn1.rc.fas.harvard.edu/dvn/dv/rtdc/faces/study/StudyPage.xhtml?globalId=hdl:TEST/10016">DHT18</a>), which have wider velocity coverage. The interpolated cube is recommended as it fills in a few missing spectra at random locations as well as the 1/4<font face="symbol">°</font> sampling along the bottom. |
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Methodology and Processing |
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Sources Statement |
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Data Access |
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Notes: |
<a href="http://creativecommons.org/publicdomain/zero/1.0">CC0 1.0</a> |
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Other Study Description Materials |
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Related Publications |
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Citation |
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Title: |
<a href="http://adsabs.harvard.edu/abs/2001ApJ...547..792D">The Astrophysical Journal, 2001, Volume 547, Issue 2, pp. 792-813.</a> |
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Identification Number: |
2001ApJ...547..792D |
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Bibliographic Citation: |
<a href="http://adsabs.harvard.edu/abs/2001ApJ...547..792D">The Astrophysical Journal, 2001, Volume 547, Issue 2, pp. 792-813.</a> |
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Label: |
DHT21_big.jpg |
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Text: |
Spatial and longitude-velocity maps of DHT21 |
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Notes: |
image/jpeg |
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Label: |
DHT21_interp.jpg |
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Text: |
Sampling map for DHT21, interpolated |
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Notes: |
image/jpeg |
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Label: |
DHT21_raw.jpg |
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Text: |
Sampling map for DHT21, raw |
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Notes: |
image/jpeg |
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Label: |
DHT21_Taurus_interp.fits |
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Text: |
DHT21 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. |
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Notes: |
text/plain; charset=US-ASCII |
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Label: |
DHT21_Taurus_mom.fits |
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Text: |
DHT21 v-l-b FITS cube, moment masked |
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Notes: |
text/plain; charset=US-ASCII |
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Label: |
DHT21_Taurus_raw.fits |
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Text: |
DHT21 v-l-b FITS cube, raw |
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Notes: |
text/plain; charset=US-ASCII |
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Label: |
DHT21_Taurus_raw.txt |
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Text: |
FITS header for DHT21 |
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Notes: |
text/plain; charset=US-ASCII |