eHOPS SEDs | eHOPS Auxiliary Photometry Table | IRSA Catalog Search Tool: eHOPS |
Overview
The Extension of HOPS Out
to 500 ParSecs (eHOPS) project used archival data to survey all the major star
forming molecular clouds within 500 pc of the Sun, except Orion (which was
surveyed by HOPS). The first eHOPS data release covers the Aquila
molecular clouds (d ~ 436 pc), and the second eHOPS data release adds the Auriga, Cepheus, Chamaeleon, CrA, Lupus, Musca, Ophiuchus, Perseus, and Pipe molecular clouds. For every source detected in the
Herschel/PACS bands, the eHOPS catalog contains 1-850 micron SEDs
assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data.
eHOPS compares the SEDs to a grid of radiative transfer models to constrain
the luminosities, envelope densities, and envelope masses of the protostars.
If you use eHOPS data, please cite both the journal article Pokhrel et al. (2023) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA553. Last updated: 2023-10-24 |
Data Set Characteristics
Data Product | Description | Data Access |
---|---|---|
SED Data Catalog | 2MASS JHK_s Spitzer/IRAC 3.6, 4.5, 5.8, 8 micron Spitzer/MIPS 24 micron Herschel/PACS 70, 100, 160 micron WISE 3.4, 4.6, 12, 22 micron JCMT/SCUBA2 850 micron Spitzer/IRS 5.4-35 micron |
SED Fits Catalog | Best-fit parameters, including SED class, luminosity, temperature, disk radius, envelope mass, inclination angle, etc. |
eHOPS Documentation
General | Catalogs |
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Data Delivery Document |