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The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. VIII. Serpens Observed with MIPS

Harvey, Paul M. and Rebull, Luisa M. and Brooke, Tim and Spiesman, William J. and Chapman, Nicholas and Huard, Tracy L. and Evans, Neal J., II and Cieza, Lucas and Lai, Shih-Ping and Allen, Lori E. and Mundy, Lee G. and Padgett, Deborah L. and Sargent, Anneila I. and Stapelfeldt, Karl R. and Myers, Philip C. and van Dishoeck, Ewine F. and Blake, Geoffrey A. and Koerner, David W. (2007) The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. VIII. Serpens Observed with MIPS. Astrophysical Journal, 663 (2). pp. 1139-1148. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20100917-094755422

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Abstract

We present maps of 1.5 deg^2 of the Serpens dark cloud at 24, 70, and 160 μm observed with the Spitzer Space Telescope MIPS camera. We describe the observations and briefly discuss the data processing carried out by the c2d team on these data. More than 2400 compact sources have been extracted at 24 μm, nearly 100 at 70 μm, and four at 160 μm. We estimate completeness limits for our 24 μm survey from Monte Carlo tests with artificial sources inserted into the Spitzer maps. We compare source counts, colors, and magnitudes in the Serpens cloud to two reference data sets: a 0.50 deg^2 set on a low-extinction region near the dark cloud, and a 5.3 deg^2 subset of the SWIRE ELAIS N1 data that was processed through our pipeline. These results show that there is an easily identifiable population of young stellar object candidates in the Serpens cloud that is not present in either of the reference data sets. We also show a comparison of visual extinction and cool dust emission illustrating a close correlation between the two and find that the most embedded YSO candidates are located in the areas of highest visual extinction.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/518647DOIArticle
http://iopscience.iop.org/0004-637X/663/2/1139PublisherArticle
ORCID:
AuthorORCID
Rebull, Luisa M.0000-0001-6381-515X
Padgett, Deborah L.0000-0001-5334-5107
Sargent, Anneila I.0000-0002-4633-5098
van Dishoeck, Ewine F.0000-0001-7591-1907
Blake, Geoffrey A.0000-0003-0787-1610
Additional Information:© 2007 American Astronomical Society. Received 2007 February 3; accepted 2007 March 16. Support for this work, part of the Spitzer Legacy Science Program, was provided by NASA through contracts 1224608, 1230782, and 1230779 issued by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407. Astrochemistry in Leiden is supported by an NWO Spinoza grant and a NOVA grant. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by NASA and the National Science Foundation. We also acknowledge extensive use of the SIMBAD database.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA1224608
NASA1230782
NASA1230779
NASA/JPL/CaltechUNSPECIFIED
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)UNSPECIFIED
Nederlandse Onderzoekschool voor de Astronomie (NOVA)UNSPECIFIED
Subject Keywords:infrared: general
Record Number:CaltechAUTHORS:20100917-094755422
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20100917-094755422
Official Citation:Paul M. Harvey et al 2007 ApJ 663 1139 doi: 10.1086/518647
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:20009
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:17 Sep 2010 18:00
Last Modified:29 Nov 2017 05:57

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