The Spitzer Mapping of the Outer Galaxy (SMOG; Carey et al. 2008) project mapped a 21 square degree area with IRAC & MIPS (l=102d to 109d , b=0d to 3d) of the Outer Galaxy. The SMOG IRAC data have been processed by the Wisconsin GLIMPSE IRAC pipeline. There are two types of source lists: a high reliability point source Catalog and a more complete point source Archive.
The Spitzer Mapping of the Outer Galaxy (SMOG; Carey et al. 2008) project mapped a 21 square degree area with IRAC & MIPS (l=102d to 109d , b=0d to 3d) of the Outer Galaxy. The SMOG IRAC data have been processed by the Wisconsin GLIMPSE IRAC pipeline. There are two types of source lists: a high reliability point source Catalog and a more complete point source Archive.
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.
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.
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.
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.
The Galactic Plane Infrared Polarization Survey (GPIPS) covers 76 sq. deg. of the first Galactic quadrant midplane, 18<l<56 deg and -1<b<+1 deg, in H-band (1.6 micron) linear polarimetry to reveal the plane-of-the-sky orientation of the magnetic field in diffuse and denser atomic and molecular clouds. The Survey consists of 3234 overlapping 10x10 arcmin fields observed using the Mimir instrument on the 1.8 m Perkins telescope.
The unique star data file (Clemens et al. 2020) collects all GPIPS photometry and polarimetry and all matching stellar data appropriate to each GPIPS star. The unique star file contains entries for 13,861,329 GPIPS stars.
The GOALS sample consists of a total of 179 LIRGs (log (L_IR/L_sun) = 11.0-11.99) and 22 ultra-luminous infrared galaxies (ULIRGs: log (L_IR/L_sun) > 12.0) selected from the IRAS Revised Bright Galaxy Sample; these 201 objects comprise a statistically complete flux-limited sample of infrared-luminous galaxies in the local universe. The GOALS objects have been the subject of an intense multi-wavelength observing campaign, including space-based imaging and spectroscopy from Spitzer and Herschel.
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.
HERON used a dedicated 0.7-m telescope to image the haloes of 124 galaxies in the Local Volume to surface brightnesses of 28-30 mag/arcsec^2. The sample is primarily from the Two Micron All Sky Survey Large Galaxy Atlas and extended to include nearby dwarf galaxies and more distant giant ellipticals, and spans fully the galaxy color-magnitude diagram including the blue cloud and red sequence
