- ID:
- ivo://irsa.ipac/Spitzer/Catalog/DeepDrill/DeepDrillPhot
- Title:
- DeepDrill Forced Photometry Catalog
- Short Name:
- DeepDrillPhot
- Date:
- 01 Apr 2023 01:07:04
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The DeepDrill team presents a catalog of multi-band forced photometry in the CDFS and XMM-LSS fields. They used The Tractor image-modeling software to produce de-blended photometry across 13 to 15 optical/infrared bands and determine photometric redshifts. The Catalog contains ~1.5 million sources covering a total area of ~9 square degrees.
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- ID:
- ivo://irsa.ipac/Spitzer/Catalog/DeepDrillXMMI12
- Title:
- DeepDrill XMM-LSS 2-band Catalog
- Short Name:
- DeepDrillXMMI12
- Date:
- 07 May 2021 01:52:01
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. The "DeepDrill" survey (Program ID 11086, P.I. Lacy) used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centered on 3.6 um and 4.5 um. These observations expand the area which was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South field (ECDFS), the ELAIS-S1 field (ES1), and the XMM-Large-Scale Structure Survey field (XMM-LSS).
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/DeepDrillXMMI2
- Title:
- DeepDrill XMM-LSS 4.5 micron Catalog
- Short Name:
- DeepDrillXMMI2
- Date:
- 07 May 2021 01:52:01
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. The "DeepDrill" survey (Program ID 11086, P.I. Lacy) used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centered on 3.6 um and 4.5 um. These observations expand the area which was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South field (ECDFS), the ELAIS-S1 field (ES1), and the XMM-Large-Scale Structure Survey field (XMM-LSS).
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/DeepDrillXMMI1
- Title:
- DeepDrill XMM-LSS 3.6 micron Catalog
- Short Name:
- DeepDrillXMMI1
- Date:
- 07 May 2021 01:52:01
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. The "DeepDrill" survey (Program ID 11086, P.I. Lacy) used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centered on 3.6 um and 4.5 um. These observations expand the area which was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South field (ECDFS), the ELAIS-S1 field (ES1), and the XMM-Large-Scale Structure Survey field (XMM-LSS).
- ID:
- ivo://irsa.ipac/Herschel/Catalog/eHOPS/eHOPSAquilaPhot
- Title:
- eHOPS Aquila SED Data Catalog
- Short Name:
- eHOPSAquilaPhot
- Date:
- 01 Apr 2023 01:07:05
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- 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). For every source detected in the Herschel/PACS bands, the eHOPS-Aquila catalog contains 1-850 micron SEDs assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data. A total of 172 protostars are found in Aquila, tightly concentrated in the molecular filaments that thread the clouds. Of these, 72 (42%) are Class 0 protostars, 53 (31%) Class I protostars, 43 (25%) are flat-spectrum protostars, and 4 (2%) are Class II sources. Ten of the Class 0 protostars are young PACS Bright Red Sources similar to those discovered in Orion. eHOPS compares the SEDs to a grid of radiative transfer models to constrain the luminosities, envelope densities, and envelope masses of the protostars.
- ID:
- ivo://irsa.ipac/Herschel/Catalog/eHOPS/eHOPSAquilaFits
- Title:
- eHOPS Aquila SED Fits Catalog
- Short Name:
- eHOPSAquilaFits
- Date:
- 01 Apr 2023 01:07:05
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- 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). For every source detected in the Herschel/PACS bands, the eHOPS-Aquila catalog contains 1-850 micron SEDs assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data. A total of 172 protostars are found in Aquila, tightly concentrated in the molecular filaments that thread the clouds. Of these, 72 (42%) are Class 0 protostars, 53 (31%) Class I protostars, 43 (25%) are flat-spectrum protostars, and 4 (2%) are Class II sources. Ten of the Class 0 protostars are young PACS Bright Red Sources similar to those discovered in Orion. eHOPS compares the SEDs to a grid of radiative transfer models to constrain the luminosities, envelope densities, and envelope masses of the protostars.
- ID:
- ivo://sdss.jhu/services/CONE
- Title:
- Sloan Digital Sky Survey Cone Search (Latest Release)
- Short Name:
- SDSS-CONE
- Date:
- 05 Feb 2015 21:18:36
- Publisher:
- The Johns Hopkins University
- Description:
- The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
- ID:
- ivo://sdss.jhu/services/DR5CONE
- Title:
- Sloan Digital Sky Survey (DR5)
- Short Name:
- SDSS-DR5
- Date:
- 05 Dec 2018 20:08:59
- Publisher:
- The Johns Hopkins Univer
- Description:
- The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
- ID:
- ivo://sdss.jhu/services/DR9CONE
- Title:
- Sloan Digital Sky Survey (DR9)
- Short Name:
- SDSS-DR9
- Date:
- 05 Feb 2015 20:33:12
- Publisher:
- The Johns Hopkins University
- Description:
- The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
- ID:
- ivo://sdss.jhu/services/DR8CONE
- Title:
- Sloan Digital Sky Survey (DR8)
- Short Name:
- SDSS-DR8
- Date:
- 05 Feb 2015 20:32:31
- Publisher:
- The Johns Hopkins University
- Description:
- The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
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