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Part 1: Document Description
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Citation |
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Title: |
Replication data for: Spitzer/MIPS Column Density and Temperature maps |
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Identification Number: |
doi:10.7910/DVN/6IGXPU |
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Distributor: |
Harvard Dataverse |
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Date of Distribution: |
2011-09-27 |
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Version: |
2 |
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Bibliographic Citation: |
S. Schnee; A. A. Goodman; A. I. Sargent, 2011, "Replication data for: Spitzer/MIPS Column Density and Temperature maps", https://doi.org/10.7910/DVN/6IGXPU, Harvard Dataverse, V2 |
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Citation |
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Title: |
Replication data for: Spitzer/MIPS Column Density and Temperature maps |
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Identification Number: |
doi:10.7910/DVN/6IGXPU |
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Authoring Entity: |
S. Schnee (Division of Physics, Mathematics and Astronomy, California Institute of Technology, 770 South Wilson Avenue, Pasadena, CA 91125) |
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A. A. Goodman (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138) |
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A. I. Sargent (Division of Physics, Mathematics and Astronomy, California Institute of Technology, 770 South Wilson Avenue, Pasadena, CA 91125) |
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Distributor: |
Harvard Dataverse |
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Access Authority: |
Scott Schnee |
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Date of Deposit: |
2011-09-23 |
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Holdings Information: |
https://doi.org/10.7910/DVN/6IGXPU |
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Study Scope |
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Abstract: |
<p><b>Description:</b><br /> Combining Spitzer/MIPS maps at 70 and 160 microns with IRAS maps at 60 and 100 microns we have produced high-resolution column density and temperature maps of Perseus. The emission maps at 60 and 70 microns are statistically corrected for emission from Very Small Grains (VSG's), and the dust emissivity is seen to increase in colder and denser regions within the molecular cloud. The resolution of the map is 40", set by the resolution of the Spitzer 160 micron map. < /p> <p><b>Telescope Information</b><br /> <a href="http://www.spitzer.caltech.edu/">Spitzer Space Telescope</a></p> <p><b>Status:</b><br /> Final</p> <p><b>Sampling:</b><br /> Wavebands: 70 and 160 microns<br /> Resolution: 40 arcseconds</p> <p><b>Areal Coverage:</b><br /> Roughly 8 square degrees</p> <p><b>Map Center (J2000):</b><br /> RA = 03:35:00 <br /> Dec = 31:00:00 </p> |
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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: |
Scott Schnee et al., <i>Dust Emission from the Perseus Molecular Cloud</i>, <a href="http://arxiv.org/abs/0805.4215">astro-ph</a> |
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Identification Number: |
2008ApJ...684.1228S |
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Bibliographic Citation: |
Scott Schnee et al., <i>Dust Emission from the Perseus Molecular Cloud</i>, <a href="http://arxiv.org/abs/0805.4215">astro-ph</a> |
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Label: |
PerA_AvTemMIPS_F_Av.fits |
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Text: |
Column density map of Perseus in FITS cube |
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Notes: |
text/plain; charset=US-ASCII |
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Label: |
PerA_AvTemMIPS_F_Av.jpg |
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Text: |
Emission map of Perseus |
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Notes: |
image/jpeg |
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Label: |
PerA_AvTemMIPS_F_T.fits |
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Text: |
Temperature map of Perseus in FITS cube |
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Notes: |
text/plain; charset=US-ASCII |