The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. IX. The Serpens YSO Population as Observed with IRAC and MIPS

By P. Harvey, B. Mer'in, T. Huard, L. Rebull, N. Chapman, N. Evans II, P. Myers. 2007

161 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/96c38bb9d5e8c92b6f8630d3ac1b7c7139959a57

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Citations in the corpus

Probing dust grain evolution in IM Lupi's circumstellar disc. Multi-wavelength observations and mo (2008, methodology): “A detailed description of the reduction and source extraction procedures used for the IRAC and MIPS measurements can be found in Harvey et al. (2006, 2007) and in the c2d delivery document (Evans et al. 2007).”
STAR FORMATION RELATIONS IN NEARBY MOLECULAR CLOUDS (2014, methodology): “The detailed descriptions of this process are in Harvey et al. 2007; Evans 2007; Evans et al. 2009.”
THE TAURUS SPITZER SURVEY: NEW CANDIDATE TAURUS MEMBERS SELECTED USING SENSITIVE MID-INFRARED PHOTOMETRY (2009, methodology): “We compare our search method to others in the literature in §4.7 below; in preparation for that, Tables 6 and 7 indicate, for each of the previously identified Taurus members, how (or if) the c2d (Harvey et al. 2007) or Gutermuth et al. (2008) criteria for YSOs identified the object.”
A SPITZER SURVEY OF YOUNG STELLAR CLUSTERS WITHIN ONE KILOPARSEC OF THE SUN: CLUSTER CORE EXTRACTION AND BASIC STRUCTURAL ANALYSIS (2009, background): “Also, the Serpens Core as isolated in Section 7 is a structure of nearly identical area (0.2 pc2) to “Cluster A” as described in Harvey et al. (2007), another paper from the c2d Legacy Survey.”
Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores (2007, methodology): “The observations of Serpens, Lupus, Chamaeleon II, Ophiuchus, and Perseus were obtained in Program IDs (PIDs) 174, 175, 176, 177, and 178, respectively.”
The Mass Distribution and Lifetime of Prestellar Cores in Perseus, Serpens, and Ophiuchus (2008, methodology): “…to eliminate most extragalactic interlopers and sources with SEDs 8 Note that this limit is considerably higher than the S24µm & 0.7 mJy limit imposed by Harvey et al. (2007b), together with several other criteria, to help eliminate galaxies. that are clearly inconsistent with an embedded nature…”
YOUNG STELLAR OBJECTS IN THE GOULD BELT (2015, methodology): “Since it is unnormalized, this quantity is not a true probability but a relative parameter expressing the likelihood of being a background galaxy (higher values indicate higher likelihood of being galaxies; see Harvey et al. 2007a, for details).”
THE SPITZER c2d LEGACY RESULTS: STAR-FORMATION RATES AND EFFICIENCIES; EVOLUTION AND LIFETIMES (2008, methodology): “Compared to earlier catalogs, advances in distinguishing YSOs from background galaxies (Harvey et al. 2007b) have provided much cleaner samples.”
A CORRELATION BETWEEN SURFACE DENSITIES OF YOUNG STELLAR OBJECTS AND GAS IN EIGHT NEARBY MOLECULAR CLOUDS (2011, methodology): “…(Pearson coefficients of the log-log data are 0.87 and 0.83, respectively), thus we use 1This value is higher than the value reported for c2d (e.g. Harvey et al. 2007), but we apply it across all clouds for consistency in treatment. their correlation data to characterize the trend in detail.”
PROPERTIES OF THE YOUNGEST PROTOSTARS IN PERSEUS, SERPENS, AND OPHIUCHUS (2008, methodology): “This criteria is motivated by a comparison to the carefully vetted Serpens YSO sample of Harvey et al. (2007a).”
SPITZER SAGE SURVEY OF THE LARGE MAGELLANIC CLOUD. III. STAR FORMATION AND ∼1000 NEW CANDIDATE YOUNG STELLAR OBJECTS (2008, methodology): “A similar comparison of our model CMDs and CCDs in the Perseus starformation region found good agreement between the models and data (Harvey et al. 2007).”
THE MID-INFRARED EXTINCTION LAW IN THE OPHIUCHUS, PERSEUS, AND SERPENS MOLECULAR CLOUDS (2008, methodology): “Readers interested in the YSO/Galc content of the full clouds should consult Padgett et al. (2007) (Ophiuchus), Jørgensen et al. (2006) and Rebull et al. (2007) (Perseus), and Harvey et al. (2007a) (Serpens).”