The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS
— Northern Arizona University Skip to main navigation Skip to search Skip to main content Northern Arizona University Home Home Profiles Departments and Centers Scholarly Works Activities Grants Datasets Prizes Search by expertise, name or affiliation The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS Paul M. Harvey, Luisa M. Rebull, Tim Brooke, William J. Spiesman, Nicholas Chapman, Tracy L. Huard, Neal J. Evans, Lucas Cieza, Shih Ping Lai, Lori E. Allen, Lee G. Mundy, Deborah L. Padgett, Anneila I. Sargent, Karl R. Stapelfeldt, Philip C. Myers, Ewine F. Van Dishoeck, Geoffrey A. Blake, David W. Koerner Astronomy and Planetary Sciences Research output: Contribution to journal › Article › peer-review 44 Scopus citations Overview Fingerprint Abstract We present maps of 1.5 deg2 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 deg2 set on a low-extinction region near the dark cloud, and a 5.3 deg2 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. Original language English (US) Pages (from-to) 1139-1148 Number of pages 10 Journal Astrophysical Journal Volume 663 Issue number 2 I DOIs https://doi.org/10.1086/518647 State Published - Jul 10 2007 Keywords Infrared: general ASJC Scopus subject areas Astronomy and Astrophysics Space and Planetary Science Access to Document 10.1086/518647 Other files and links Link to publication in Scopus Fingerprint Dive into the research topics of 'The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS'. Together they form a unique fingerprint. extinction Physics & Astronomy 100% Space Infrared Telescope Facility Physics & Astronomy 51% completeness Physics & Astronomy 45% set theory Physics & Astronomy 40% dust Physics & Astronomy 32% cameras Physics & Astronomy 30% color Physics & Astronomy 27% young Earth & Environmental Sciences 27% View full fingerprint Cite this APA Standard Harvard Vancouver Author BIBTEX RIS Harvey, P. M., Rebull, L. M., Brooke, T., Spiesman, W. J., Chapman, N., Huard, T. L., Evans, N. J., Cieza, L., Lai, S. P., Allen, L. E., Mundy, L. G., Padgett, D. L., Sargent, A. I., Stapelfeldt, K. R., Myers, P. C., Van Dishoeck, E. F., Blake, G. A., & Koerner, D. W. (2007). The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS. Astrophysical Journal, 663(2 I), 1139-1148. https://doi.org/10.1086/518647 The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS. / Harvey, Paul M.; Rebull, Luisa M.; Brooke, Tim; Spiesman, William J.; Chapman, Nicholas; Huard, Tracy L.; Evans, Neal J.; Cieza, Lucas; Lai, Shih Ping; Allen, Lori E.; Mundy, Lee G.; Padgett, Deborah L.; Sargent, Anneila I.; Stapelfeldt, Karl R.; Myers, Philip C.; Van Dishoeck, Ewine F.; Blake, Geoffrey A.; Koerner, David W. In: Astrophysical Journal, Vol. 663, No. 2 I, 10.07.2007, p. 1139-1148. Research output: Contribution to journal › Article › peer-review Harvey, PM, Rebull, LM, Brooke, T, Spiesman, WJ, Chapman, N, Huard, TL, Evans, NJ, Cieza, L, Lai, SP, Allen, LE, Mundy, LG, Padgett, DL, Sargent, AI, Stapelfeldt, KR, Myers, PC, Van Dishoeck, EF, Blake, GA & Koerner, DW 2007, 'The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS', Astrophysical Journal, vol. 663, no. 2 I, pp. 1139-1148. https://doi.org/10.1086/518647 Harvey PM, Rebull LM, Brooke T, Spiesman WJ, Chapman N, Huard TL et al. The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS. Astrophysical Journal. 2007 Jul 10;663(2 I):1139-1148. https://doi.org/10.1086/518647 Harvey, Paul M. ; Rebull, Luisa M. ; Brooke, Tim ; Spiesman, William J. ; Chapman, Nicholas ; Huard, Tracy L. ; Evans, Neal J. ; Cieza, Lucas ; Lai, Shih Ping ; Allen, Lori E. ; Mundy, Lee G. ; Padgett, Deborah L. ; Sargent, Anneila I. ; Stapelfeldt, Karl R. ; Myers, Philip C. ; Van Dishoeck, Ewine F. ; Blake, Geoffrey A. ; Koerner, David W. / The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS. In: Astrophysical Journal. 2007 ; Vol. 663, No. 2 I. pp. 1139-1148. @article{4d7bd1eec9d847258420e719b8bd6c6f, title = "The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS", abstract = "We present maps of 1.5 deg2 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 deg2 set on a low-extinction region near the dark cloud, and a 5.3 deg2 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.", keywords = "Infrared: general", author = "Harvey, {Paul M.} and Rebull, {Luisa M.} and Tim Brooke and Spiesman, {William J.} and Nicholas Chapman and Huard, {Tracy L.} and Evans, {Neal J.} and Lucas Cieza 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.}", year = "2007", month = jul, day = "10", doi = "10.1086/518647", language = "English (US)", volume = "663", pages = "1139--1148", journal = "Astrophysical Journal", issn = "0004-637X", publisher = "IOP Publishing Ltd.", number = "2 I", } TY - JOUR T1 - The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS AU - Harvey, Paul M. AU - Rebull, Luisa M. AU - Brooke, Tim AU - Spiesman, William J. AU - Chapman, Nicholas AU - Huard, Tracy L. AU - Evans, Neal J. AU - Cieza, Lucas AU - Lai, Shih Ping AU - Allen, Lori E. AU - Mundy, Lee G. AU - Padgett, Deborah L. AU - Sargent, Anneila I. AU - Stapelfeldt, Karl R. AU - Myers, Philip C. AU - Van Dishoeck, Ewine F. AU - Blake, Geoffrey A. AU - Koerner, David W. PY - 2007/7/10 Y1 - 2007/7/10 N2 - We present maps of 1.5 deg2 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 deg2 set on a low-extinction region near the dark cloud, and a 5.3 deg2 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. AB - We present maps of 1.5 deg2 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 deg2 set on a low-extinction region near the dark cloud, and a 5.3 deg2 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. KW - Infrared: general UR - http://www.scopus.com/inward/record.url?scp=34547433622&partnerID=8YFLogxK UR - http://www.scopus.com/inward/citedby.url?scp=34547433622&partnerID=8YFLogxK U2 - 10.1086/518647 DO - 10.1086/518647 M3 - Article AN - SCOPUS:34547433622 VL - 663 SP - 1139 EP - 1148 JO - Astrophysical Journal JF - Astrophysical Journal SN - 0004-637X IS - 2 I ER - Powered by Pure, Scopus & Elsevier Fingerprint Engine™ © 2022 Elsevier B.V We use cookies to help provide and enhance our service and tailor content. By continuing you agree to the use of cookies Log in to Pure About web accessibility Contact us
