- ID:
- ivo://irsa.ipac/Spitzer/Catalog/GOODS/GOODSN_IRS16
- Title:
- GOODS-N IRS 16 micron Catalog
- Short Name:
- GOODSN_IRS16
- Date:
- 01 Oct 2018 20:27:17
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS Spitzer IRS 16 micron observations surveyed 150 square arcminutes in each of the two GOODS fields (North and South), to an average 3 sigma depth of 40 and 65 microJy, respectively. These sources have been cross-correlated with Spitzer, Chandra, and HST measurements in other bands.
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- ID:
- ivo://irsa.ipac/Spitzer/Catalog/GOODS/GOODS-N_MIPS24
- Title:
- GOODS-N MIPS 24 micron Photometry Catalog
- Short Name:
- GOODS-N MIPS24
- Date:
- 01 Oct 2018 20:27:17
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. This catalog provides a list of sources for the MIPS 24 micron imaging of the GOODS-N field. It is limited to flux densities greater than 80 microJy, where the source extraction is highly complete and reliable.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/GOODS/GOODSS_IRS16
- Title:
- GOODS-S IRS 16 micron Catalog
- Short Name:
- GOODSS_IRS16
- Date:
- 01 Oct 2018 20:27:17
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS Spitzer IRS 16 micron observations surveyed 150 square arcminutes in each of the two GOODS fields (North and South), to an average 3 sigma depth of 40 and 65 microJy, respectively. These sources have been cross-correlated with Spitzer, Chandra, and HST measurements in other bands.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/GOODS/GOODS-S_MIPS24
- Title:
- GOODS-S MIPS 24 micron Photometry Catalog
- Short Name:
- GOODS-S MIPS24
- Date:
- 01 Oct 2018 20:27:17
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. This catalog provides a list of sources for the MIPS 24 micron imaging of the GOODS-S field. It is limited to flux densities greater than 80 microJy, where the source extraction is highly complete and reliable.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/SEP/SEP_MW
- Title:
- SEP Multiwavelength Photometric Catalog
- Short Name:
- SEP_MW
- Date:
- 01 Oct 2018 20:27:18
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field (SEP) covers an area of 7.74 sq. deg to a depth of ~5.80 microJy (3sigma) at 3.6 microns and 5.25 microJy at 4.5 microns. The 90% and 50% completeness limits are at 14 and 9 microJy, respectively. The multiwavelength catalog includes the WFI-Rc, MIPS-24 micron, SPIRE 250, 350 and 500 micron fluxes of the counterparts that were identified by searching for the closest neighbor.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/SIMPLE
- Title:
- SIMPLE Photometry Catalog
- Short Name:
- SIMPLE Catalog
- Date:
- 01 Oct 2018 20:27:19
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Spitzer IRAC/MUSYC Public Legacy Survey in the Extended Chandra Deep Field South (SIMPLE) consists of deep IRAC observations (several hours per pointing) covering the 0.5 x 0.5 deg area surrounding the GOODS CDF-South. This low-background region of the sky has by far the best supporting data of any cosmological survey field of comparable area, with deep observations from the X-rays to the thermal infrared.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/SAFIRES/SAFIRES160
- Title:
- Spitzer Archival Far-Infrared Extragalactic Survey (SAFIRES) MIPS 160 micron Catalog
- Short Name:
- SAFIRES160
- Date:
- 01 Oct 2018 20:27:18
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Spitzer Archival FIR Extragalactic Survey (SAFIRES) is an offshoot of the Spitzer Space Telescope Enhanced Imaging Products (SEIP). SAFIRES applies the SEIP project's methods to the remaining two MIPS bands, located at far-infrared wavelengths of 70 and 160 microns. Due to the complexity of far-infrared observations, these bands require an expansion of SEIP's standard pipeline through the addition of reprocessing tools. These additional steps are required to remove obvious artifacts before extracting useful measurements. As a result, these bands were not included in the SEIP project, but were later funded through an additional NASA Astrophysics Data Analysis Program (ADAP) grant. To ensure high reliability, the SAFIRES sample includes no fields near the Galactic disk; these observations comprised more than half of the area observed by Spitzer, but the practical drawbacks of Galactic contamination would inhibit the ability to maintain the level of reliability desired in the SAFIRES products. As with SEIP, the SAFIRES source lists contains no extended sources. The remaining sample comprises nearly 1132 fields spanning almost 180 square degrees of sky.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/SAFIRES/SAFIRES70
- Title:
- Spitzer Archival Far-Infrared Extragalactic Survey (SAFIRES) MIPS 70 micron Catalog
- Short Name:
- SAFIRES70
- Date:
- 01 Oct 2018 20:27:18
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Spitzer Archival FIR Extragalactic Survey (SAFIRES) is an offshoot of the Spitzer Space Telescope Enhanced Imaging Products (SEIP). SAFIRES applies the SEIP project's methods to the remaining two MIPS bands, located at far-infrared wavelengths of 70 and 160 microns. Due to the complexity of far-infrared observations, these bands require an expansion of SEIP's standard pipeline through the addition of reprocessing tools. These additional steps are required to remove obvious artifacts before extracting useful measurements. As a result, these bands were not included in the SEIP project, but were later funded through an additional NASA Astrophysics Data Analysis Program (ADAP) grant. To ensure high reliability, the SAFIRES sample includes no fields near the Galactic disk; these observations comprised more than half of the area observed by Spitzer, but the practical drawbacks of Galactic contamination would inhibit the ability to maintain the level of reliability desired in the SAFIRES products. As with SEIP, the SAFIRES source lists contains no extended sources. The remaining sample comprises nearly 1132 fields spanning almost 180 square degrees of sky.
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/SDWFS/SDWFS-LCurve
- Title:
- Spitzer Deep Wide-Field Survey Light Curve Catalog
- Short Name:
- SDWFS-LCurve
- Date:
- 01 Oct 2018 20:27:18
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Spitzer Deep, Wide-Field Survey (SDWFS) is a four-epoch infrared survey of 10 square degrees in the Boötes field of the NOAO Deep Wide-Field Survey using the IRAC instrument on the Spitzer Space Telescope. SDWFS, a Spitzer Cycle 4 Legacy project, occupies a unique position in the area-depth survey space defined by other Spitzer surveys. The four epochs that make up SDWFS permit - for the first time - the selection of infrared-variable and high proper motion objects over a wide field on timescales of years. Because of its large survey volume, SDWFS is sensitive to galaxies out to z ~ 3 with relatively little impact from cosmic variance for all but the richest systems. The SDWFS data sets will thus be especially useful for characterizing galaxy evolution beyond z ~ 1.5. The SDWFS Light Curve Catalog presents the 3.6 and 4.5 micron magnitudes for each SDWFS source in each of the four epochs. For more details see Kozlowski et al. (2010).
- ID:
- ivo://irsa.ipac/Spitzer/Catalog/SDWFS/SDWFSI1C
- Title:
- Spitzer Deep Wide-Field Survey 3.6 micron Combined Catalog
- Short Name:
- SDWFSI1C
- Date:
- 01 Oct 2018 20:27:18
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The Spitzer Deep, Wide-Field Survey (SDWFS) is a four-epoch infrared survey of 10 square degrees in the Boötes field of the NOAO Deep Wide-Field Survey using the IRAC instrument on the Spitzer Space Telescope. SDWFS, a Spitzer Cycle 4 Legacy project, occupies a unique position in the area-depth survey space defined by other Spitzer surveys. The four epochs that make up SDWFS permit - for the first time - the selection of infrared-variable and high proper motion objects over a wide field on timescales of years. Because of its large survey volume, SDWFS is sensitive to galaxies out to z ~ 3 with relatively little impact from cosmic variance for all but the richest systems. The SDWFS data sets will thus be especially useful for characterizing galaxy evolution beyond z ~ 1.5. The delivery consists of four band-matched catalogs for each of the four epochs and for the total SDWFS coadd data, a total of 20 catalogs. Vega magnitudes are reported for each IRAC band: 3.6, 4.5, 5.8, and 8 microns. Each source was measured three ways: 4 arcsec diameter aperture, 6 arcsec diameter aperture, and Kron radius aperture (MAG_AUTO in SExtractor). Source coordinates correspond to 2MASS catalog positions to within 0.2 arcsec. The tabulated uncertainties are twice the SExtractor (statistical only) uncertainties as an attempt to account for systematic uncertainties.
