The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus 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. Iv Lupus observed with MIPS Nicholas L. Chapman, Shih Ping Lai, Lee G. Mundy, Neal J. Evans, Timothy Y. Brooke, Lucas A. Cieza, William J. Spiesman, Luisa M. Rebull, Karl R. Stapelfeldt, Alberto Noriega-Crespo, Lauranne Lanz, Lori E. Allen, Geoffrey A. Blake, Tyler L. Bourke, Paul M. Harvey, Tracy L. Huard, Jes K. Jørgensen, David W. Koerner, Philip C. Myers, Deborah L. PadgettShow 5 othersShow lessAnnelia I. Sargent, Peter Teuben, Ewine F. Van Dishoeck, Zahed Wahhaj, Kaisa E. Young Astronomy and Planetary Sciences Research output: Contribution to journal › Article › peer-review 29 Scopus citations Overview Fingerprint Abstract We present maps of 7.78 deg2 of the Lupus molecular cloud complex at 24, 70, and 160 μm. They were made with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) instrument as part of the Spitzer Legacy Program "From Molecular Cores to Planet-Forming Disks" (c2d). The maps cover three separate regions in Lupus, denoted I, III, and IV. We discuss the c2d pipeline and how our data processing differs from it. We compare source counts in the three regions with two other data sets and predicted star counts from the Wainscoat model. This comparison shows the contribution from background galaxies in Lupus I. We also create two color-magnitude diagrams using the 2MASS and MIPS data. From these results, we can identify background galaxies and distinguish them from probable young stellar objects. The sources in our catalogs are classified based on their spectral energy distribution (SED) from 2MASS and Spitzer wavelengths to create a sample of young stellar object candidates. From 2M ASS data, we create extinction maps for each region and note a strong correspondence between the extinction and the 160 μm emission. The masses we derived in each Lupus cloud from our extinction maps are compared to masses estimated from 13CO and C18 O and found to be similar to our extinction masses in some regions, but significantly different in others. Finally, based on our color-magnitude diagrams, we selected 12 of our reddest candidate young stellar objects for individual discussion. Five of the 12 appear to be newly discovered YSOs. Original language English (US) Pages (from-to) 288-302 Number of pages 15 Journal Astrophysical Journal Volume 667 Issue number 1 I DOIs https://doi.org/10.1086/520790 State Published - 2007 Keywords ISM: clouds Infrared: stars Stars: formation ASJC Scopus subject areas Astronomy and Astrophysics Space and Planetary Science Access to Document 10.1086/520790 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. Iv Lupus observed with MIPS'. Together they form a unique fingerprint. photometer Earth & Environmental Sciences 100% photometers Physics & Astronomy 75% extinction Physics & Astronomy 71% color-magnitude diagram Physics & Astronomy 52% young Earth & Environmental Sciences 43% diagram Earth & Environmental Sciences 33% galaxies Physics & Astronomy 30% Space Infrared Telescope Facility Physics & Astronomy 27% View full fingerprint Cite this APA Standard Harvard Vancouver Author BIBTEX RIS Chapman, N. L., Lai, S. P., Mundy, L. G., Evans, N. J., Brooke, T. Y., Cieza, L. A., Spiesman, W. J., Rebull, L. M., Stapelfeldt, K. R., Noriega-Crespo, A., Lanz, L., Allen, L. E., Blake, G. A., Bourke, T. L., Harvey, P. M., Huard, T. L., Jørgensen, J. K., Koerner, D. W., Myers, P. C., ... Young, K. E. (2007). The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS. Astrophysical Journal, 667(1 I), 288-302. https://doi.org/10.1086/520790 The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS. / Chapman, Nicholas L.; Lai, Shih Ping; Mundy, Lee G.; Evans, Neal J.; Brooke, Timothy Y.; Cieza, Lucas A.; Spiesman, William J.; Rebull, Luisa M.; Stapelfeldt, Karl R.; Noriega-Crespo, Alberto; Lanz, Lauranne; Allen, Lori E.; Blake, Geoffrey A.; Bourke, Tyler L.; Harvey, Paul M.; Huard, Tracy L.; Jørgensen, Jes K.; Koerner, David W.; Myers, Philip C.; Padgett, Deborah L.; Sargent, Annelia I.; Teuben, Peter; Van Dishoeck, Ewine F.; Wahhaj, Zahed; Young, Kaisa E. In: Astrophysical Journal, Vol. 667, No. 1 I, 2007, p. 288-302. Research output: Contribution to journal › Article › peer-review Chapman, NL, Lai, SP, Mundy, LG, Evans, NJ, Brooke, TY, Cieza, LA, Spiesman, WJ, Rebull, LM, Stapelfeldt, KR, Noriega-Crespo, A, Lanz, L, Allen, LE, Blake, GA, Bourke, TL, Harvey, PM, Huard, TL, Jørgensen, JK, Koerner, DW, Myers, PC, Padgett, DL, Sargent, AI, Teuben, P, Van Dishoeck, EF, Wahhaj, Z & Young, KE 2007, 'The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS', Astrophysical Journal, vol. 667, no. 1 I, pp. 288-302. https://doi.org/10.1086/520790 Chapman NL, Lai SP, Mundy LG, Evans NJ, Brooke TY, Cieza LA et al. The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS. Astrophysical Journal. 2007;667(1 I):288-302. https://doi.org/10.1086/520790 Chapman, Nicholas L. ; Lai, Shih Ping ; Mundy, Lee G. ; Evans, Neal J. ; Brooke, Timothy Y. ; Cieza, Lucas A. ; Spiesman, William J. ; Rebull, Luisa M. ; Stapelfeldt, Karl R. ; Noriega-Crespo, Alberto ; Lanz, Lauranne ; Allen, Lori E. ; Blake, Geoffrey A. ; Bourke, Tyler L. ; Harvey, Paul M. ; Huard, Tracy L. ; Jørgensen, Jes K. ; Koerner, David W. ; Myers, Philip C. ; Padgett, Deborah L. ; Sargent, Annelia I. ; Teuben, Peter ; Van Dishoeck, Ewine F. ; Wahhaj, Zahed ; Young, Kaisa E. / The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS. In: Astrophysical Journal. 2007 ; Vol. 667, No. 1 I. pp. 288-302. @article{70b97d81b5bb4d82a3cd90aa4a8b330b, title = "The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS", abstract = "We present maps of 7.78 deg2 of the Lupus molecular cloud complex at 24, 70, and 160 μm. They were made with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) instrument as part of the Spitzer Legacy Program {"}From Molecular Cores to Planet-Forming Disks{"} (c2d). The maps cover three separate regions in Lupus, denoted I, III, and IV. We discuss the c2d pipeline and how our data processing differs from it. We compare source counts in the three regions with two other data sets and predicted star counts from the Wainscoat model. This comparison shows the contribution from background galaxies in Lupus I. We also create two color-magnitude diagrams using the 2MASS and MIPS data. From these results, we can identify background galaxies and distinguish them from probable young stellar objects. The sources in our catalogs are classified based on their spectral energy distribution (SED) from 2MASS and Spitzer wavelengths to create a sample of young stellar object candidates. From 2M ASS data, we create extinction maps for each region and note a strong correspondence between the extinction and the 160 μm emission. The masses we derived in each Lupus cloud from our extinction maps are compared to masses estimated from 13CO and C18 O and found to be similar to our extinction masses in some regions, but significantly different in others. Finally, based on our color-magnitude diagrams, we selected 12 of our reddest candidate young stellar objects for individual discussion. Five of the 12 appear to be newly discovered YSOs.", keywords = "ISM: clouds, Infrared: stars, Stars: formation", author = "Chapman, {Nicholas L.} and Lai, {Shih Ping} and Mundy, {Lee G.} and Evans, {Neal J.} and Brooke, {Timothy Y.} and Cieza, {Lucas A.} and Spiesman, {William J.} and Rebull, {Luisa M.} and Stapelfeldt, {Karl R.} and Alberto Noriega-Crespo and Lauranne Lanz and Allen, {Lori E.} and Blake, {Geoffrey A.} and Bourke, {Tyler L.} and Harvey, {Paul M.} and Huard, {Tracy L.} and J{\o}rgensen, {Jes K.} and Koerner, {David W.} and Myers, {Philip C.} and Padgett, {Deborah L.} and Sargent, {Annelia I.} and Peter Teuben and {Van Dishoeck}, {Ewine F.} and Zahed Wahhaj and Young, {Kaisa E.}", year = "2007", doi = "10.1086/520790", language = "English (US)", volume = "667", pages = "288--302", journal = "Astrophysical Journal", issn = "0004-637X", publisher = "IOP Publishing Ltd.", number = "1 I", } TY - JOUR T1 - The spitzer c2d survey of large, nearby, interstellar clouds. Iv Lupus observed with MIPS AU - Chapman, Nicholas L. AU - Lai, Shih Ping AU - Mundy, Lee G. AU - Evans, Neal J. AU - Brooke, Timothy Y. AU - Cieza, Lucas A. AU - Spiesman, William J. AU - Rebull, Luisa M. AU - Stapelfeldt, Karl R. AU - Noriega-Crespo, Alberto AU - Lanz, Lauranne AU - Allen, Lori E. AU - Blake, Geoffrey A. AU - Bourke, Tyler L. AU - Harvey, Paul M. AU - Huard, Tracy L. AU - Jørgensen, Jes K. AU - Koerner, David W. AU - Myers, Philip C. AU - Padgett, Deborah L. AU - Sargent, Annelia I. AU - Teuben, Peter AU - Van Dishoeck, Ewine F. AU - Wahhaj, Zahed AU - Young, Kaisa E. PY - 2007 Y1 - 2007 N2 - We present maps of 7.78 deg2 of the Lupus molecular cloud complex at 24, 70, and 160 μm. They were made with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) instrument as part of the Spitzer Legacy Program "From Molecular Cores to Planet-Forming Disks" (c2d). The maps cover three separate regions in Lupus, denoted I, III, and IV. We discuss the c2d pipeline and how our data processing differs from it. We compare source counts in the three regions with two other data sets and predicted star counts from the Wainscoat model. This comparison shows the contribution from background galaxies in Lupus I. We also create two color-magnitude diagrams using the 2MASS and MIPS data. From these results, we can identify background galaxies and distinguish them from probable young stellar objects. The sources in our catalogs are classified based on their spectral energy distribution (SED) from 2MASS and Spitzer wavelengths to create a sample of young stellar object candidates. From 2M ASS data, we create extinction maps for each region and note a strong correspondence between the extinction and the 160 μm emission. The masses we derived in each Lupus cloud from our extinction maps are compared to masses estimated from 13CO and C18 O and found to be similar to our extinction masses in some regions, but significantly different in others. Finally, based on our color-magnitude diagrams, we selected 12 of our reddest candidate young stellar objects for individual discussion. Five of the 12 appear to be newly discovered YSOs. AB - We present maps of 7.78 deg2 of the Lupus molecular cloud complex at 24, 70, and 160 μm. They were made with the Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) instrument as part of the Spitzer Legacy Program "From Molecular Cores to Planet-Forming Disks" (c2d). The maps cover three separate regions in Lupus, denoted I, III, and IV. We discuss the c2d pipeline and how our data processing differs from it. We compare source counts in the three regions with two other data sets and predicted star counts from the Wainscoat model. This comparison shows the contribution from background galaxies in Lupus I. We also create two color-magnitude diagrams using the 2MASS and MIPS data. From these results, we can identify background galaxies and distinguish them from probable young stellar objects. The sources in our catalogs are classified based on their spectral energy distribution (SED) from 2MASS and Spitzer wavelengths to create a sample of young stellar object candidates. From 2M ASS data, we create extinction maps for each region and note a strong correspondence between the extinction and the 160 μm emission. The masses we derived in each Lupus cloud from our extinction maps are compared to masses estimated from 13CO and C18 O and found to be similar to our extinction masses in some regions, but significantly different in others. Finally, based on our color-magnitude diagrams, we selected 12 of our reddest candidate young stellar objects for individual discussion. Five of the 12 appear to be newly discovered YSOs. KW - ISM: clouds KW - Infrared: stars KW - Stars: formation UR - http://www.scopus.com/inward/record.url?scp=35348860069&partnerID=8YFLogxK UR - http://www.scopus.com/inward/citedby.url?scp=35348860069&partnerID=8YFLogxK U2 - 10.1086/520790 DO - 10.1086/520790 M3 - Article AN - SCOPUS:35348860069 VL - 667 SP - 288 EP - 302 JO - Astrophysical Journal JF - Astrophysical Journal SN - 0004-637X IS - 1 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
