Summary of Data Sets in IRSA Viewer Summary of Data Sets in IRSA Viewer This page provides a reference for data sets currently in (or planned to be in) IRSA Viewer. Words in green can be used on the main IRSA Viewer search page to whittle down the number of programs shown in the search page. IRSA Viewer does not necessarily provide all data products from a project; it returns the most centered science image it can find. Follow the 'Website for more information' link if you need all data products (for example uncertainty maps, coverage maps, alternate mosaic algorithms, models, PSFs, etc.) instead of just a single image. Mission/ Survey Name Mission/ Survey Description Website for More Infor- mation Wavelengths Project Type Resolution Date Space/ Ground Primary Funding Agencies DSS: Digitized Sky Survey DSS Digitization of the photographic sky survey plates from the Palomar and UK Schmidt telescopes. Optical: filters covering roughly 3950 Angstroms to 9000 Angstroms All-sky: Over all DSS data, all-sky. Multiple image sets taken at different times using different instruments. one arcsec pixels 1950s-1990s ground US SDSS: Sloan Digital Sky Survey SDSS Survey of about a quarter of the sky in 5 bands. Optical: five filters (from ~2100 to ~9100 Angstroms) All-sky: While not technically an all-sky survey, it covers more than a quarter of the sky. about 1.5 arcsecond resolution 2000-2020 ground Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. PTF: Palomar Transient Facility PTF A fully-automated, wide-field survey for a systematic exploration of the optical transient sky. Optical: g and R (~4800 and ~6250 Angstroms) Northern Sky: the sky available from Palomar about 1.5 arcsecond resolution 2009-2016 ground U.S. National Science Foundation and the Participating Institutions. ZTF: Zwicky Transient Facility ZTF Building on PTF, ZTF uses a new camera with a 47 square degree field of view, looking for anything that explodes, moves, or changes in brightness. Optical: g and r (~4720 and ~6340 Angstroms) Northern Sky: the sky available from Palomar about 1.5 arcsecond resolution 2017-date ground U.S. National Science Foundation and the Participating Institutions. P60 GRBCam: Palomar 60inch Gamma Ray Burst CAMera P60:GRBCam During the years 2004 to 2017, the Palomar 60 inch telescope (P60) operated as a fully robotic facility to obtain targeted optical observations of gamma-ray burst (GRB) afterglows and other transient events. Optical: many (~4898 to ~9038 Angstroms) Northern Sky: the sky available from Palomar about 1.5 arcsecond resolution 2004-2017 ground NASA, NSF. 2MASS All-Sky 2MASS All-sky NIR survey. The All-Sky release includes the best data in three bands over the whole sky. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) All-sky pixel size of 2 arcsec 1997-2001 ground NASA 2MASS Full 2MASS All-sky NIR survey. The Full release includes all of the data over the whole sky. IRSA Viewer will pick the most centered image for you. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) All-sky pixel size of 2 arcsec 1997-2001 ground NASA 2MASS 6 degree images 2MASS All-sky NIR survey. The original 2MASS tiles are tiny by modern standards. These images are 6 degree tiles compsed from the smaller tiles. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) All-sky pixel size of 2 arcsec 1997-2001 ground NASA 2MASS 6x Catalog 2MASS All-sky NIR survey. During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These regions were imaged for 6x as long as the main survey. The 6x Catalog images are the best frames of the 6x data. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) All-sky pixel size of 2 arcsec 1997-2001 ground NASA 2MASS Full 6x 2MASS All-sky NIR survey. During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These regions were imaged for 6x as long as the main survey. The Full 6x images are all of the frames of the 6x data. IRSA Viewer will pick the most centered image for you. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) All-sky pixel size of 2 arcsec 1997-2001 ground NASA 2MASS Calib 2MASS All-sky NIR survey. The 2MASS Calib(ration) images are those used for calibration. IRSA Viewer will pick the most centered image for you. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) All-sky pixel size of 2 arcsec 1997-2001 ground NASA 2MASS Large Galaxy Atlas 2MASS The 2MASS Large Galaxy Atlas is a collection of custom-made mosaics and data products for 649 extended objects. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) Extragalactic: various pixel size of 2 arcsec 1997-2001 ground NASA LH: Lockman Hole 2MASS 6x Ancillary Data 2MASS The 2MASS Lockman Hole data are deep 2MASS observations of this region, and are not a product endorsed by the 2MASS project. Near-IR: J (1.235 �m), H (1.662 �m), K (2.159 �m) Extragalactic: various pixel size of 2 arcsec 2000 ground NASA AllWISE WISE Widefield Infrared Survey Explorer (WISE). The AllWISE release represents products derived from all the data taken between 14 Dec 2009 and 1 Feb 2011. Mid-IR: WISE1 (3.4 �m), WISE2 (4.6 �m), WISE3 (12 �m), WISE4 (22 �m) All-sky about 6.1, 6.4, 6.5, and 12.0 arcseconds 14 Dec 2009 to 1 Feb 2011 space NASA WISE All-Sky WISE Widefield Infrared Survey Explorer (WISE). The All-Sky release represents products derived from all the data taken between 7 Jan 2010 to 6 Aug 2010, before exhaustion of cryogen. Mid-IR: WISE1 (3.4 �m), WISE2 (4.6 �m), WISE3 (12 �m), WISE4 (22 �m) All-sky about 6.1, 6.4, 6.5, and 12.0 arcseconds 7 Jan 2010 to 6 Aug 2010 space NASA unWISE WISE Widefield Infrared Survey Explorer (WISE). The unWISE coadds are contributed data products; we serve just one of their datasets (NEOWISE3). Mid-IR: WISE1 (3.4 �m), WISE2 (4.6 �m) All-sky about 6.1, and 6.4 arcseconds 2010 to date of release space NASA z0MGS: The z=0 Multiwavelength Galaxy Synthesis WISE Z0MGS is an archival project combining WISE and GALEX images of nearby galaxies.. UV: GALEX NUV, FUV; Mid-IR: WISE1 (3.4 �m), WISE2 (4.6 �m), WISE3 (12 �m), WISE4 (22 �m) Extragalactic: nearby galaxies about 6.1, 6.4, 6.5, and 12.0 arcseconds various, 2009-2012 space NASA AKARI Far-Infrared All-sky Maps AKARI AKARI was a Japanese satellite. FIS images are in IRSA Viewer; IRC images have not yet been released. Mid-IR: Infrared Camera (IRC): Nine bands between 1.8-26 �m; far IR : Far-Infrared Surveyor (FIS): Four bands between 50-180 �m. All-sky 1.5 arcseconds to 1 arcminute 2006-2007 space JAXA SEIP: Spitzer Enhanced Imaging Products Spitzer Much of the most popular regions of the sky have Spitzer data. The Spitzer Enhanced Imaging Products (SEIP) combines all of the data taken during the cryogenic era. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m) Compilation: Sum of all pointed data taken during the cryogenic mission. about 1.2 arcsec to 6 arcsec 2004-2009 space NASA Abell 1763 Spitzer The galaxy cluster Abell 1763 was observed at several visible and infrared wavelengths. Optical: r (6255 �); near-IR: J (1.25 �m), H (1.635 �m), K (2.15 �m), mid-IR: IRAC1 (3.6 �m); IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: Abell 1763 About 1 arcsec to 40 arcsec various, 2004-2009 space NASA C2D: From Molecular Cores to Planet-Forming Disks Spitzer The Cores-to-Disks (c2d) project observed several star forming regions and young stars with Spitzer and Bolocam. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); Far IR: MIPS70 (70 �m), MIPS160 (160 �m); millimeter: Bolocam (1.1 mm) Galactic: several star-forming regions and young stars About 1 arcsec to 40 arcsec various, 2004-2009 space (ground for Bolocam) NASA CLASH: Cluster Lensing And Supernova survey with Hubble Spitzer The Cluster Lensing And Supernova survey with Hubble (CLASH) project surveyed 25 massive galaxy clusters. Mosaics from Spitzer are available here; additional data are located at other archives. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m) Extragalactic: several massive galaxy clusters About 1 arcsec various, 2004-2009 space NASA A Spitzer Legacy Survey of the Cygnus-X Complex Spitzer The Cygnus-X project surveyed the Cygnus X star forming region. Mosaics from Spitzer are available here. Two versions of these data were delivered to IRSA, one as part of the Cygnus X delivery, and one as part of the GLIMPSE deliveries. Both versions can be obtained via IRSA Viewer. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m) Galactic: Cygnus X About 1 to 6 arcsec various, 2004-2009 space NASA DUSTiNGS: Dust in Nearby Galaxies with Spitzer Spitzer The Dust in Nearby Galaxies with Spitzer (DUSTiNGS) project surveyed 50 dwarf galaxies. Mosaics from Spitzer are available here. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: 50 dwarf galaxies About 1 arcsec various, 2009-2017 space NASA DeepDrill: Spitzer Survey of Deep Drilling Fields Spitzer The Spitzer Survey of Deep Drilling Fields (DeepDrill) project surveyed fields anticipated to be observed at a high cadence by Rubin. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: 3 fields About 1 arcsec various, 2009-2017 space NASA ELFLock: The Eureka Lawrence Berkeley National Laboratory (LBNL) Far-Infrared Lockman Hole Map Spitzer The Eureka Lawrence Berkeley National Laboratory (LBNL) Far-Infrared Lockman Hole Map (ELFLock) project surveyed the Lockman Hole at 160 microns with Spitzer. Far IR: MIPS160 (160 �m) Extragalactic: Lockman Hole About 40 arcsec various, 2004-2009 space NASA FEPS: The Formation and Evolution of Planetary Systems Spitzer The Formation and Evolution of Planetary Systems (FEPS) project observed more than 300 young stars with Spitzer. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Galactic: young stars About 1 to 40 arcsec. various, 2004-2009 space NASA FIDEL: Far-Infrared Deep Extragalactic Legacy Survey Spitzer The Far-Infrared Deep Extragalactic Legacy Survey (FIDEL) project observed several extragalactic survey regions with Spitzer. Mid-IR: MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: Several survey regions About 6 to 40 arcsec various, 2004-2009 space NASA Spitzer FLS Spitzer The Spitzer First Look Survey (FLS) observed several representative regions with Spitzer very early in the mission. Images of the extragalactic region are available at several bands, including many bands beyond Spitzer. Optical: u (3543 �), g (4770 �), r (6231 �), R (6440 �), i (7625 �), z (9134 �); mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m); radio: 21 cm, 1.4 GHz Extragalactic: Several survey regions About 1 to 40 arcsec various, 2004-2009 space, ground NASA Frontier Fields Spitzer Spitzer imaged the Frontier Fields; HST data are also available as part of this program but at other archives. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m) Extragalactic: Frontier Fields about 1 to 6 arcsec various, 2004-2009 space NASA GLIMPSE: Galactic Legacy Infrared Midplane Survey Extraordinaire Spitzer The Galactic Legacy Infrared Midplane Survey Extraordinaire (GLIMPSE) surveyed the Galactic plane in several different projects in successive cycles. IRAC images are available, though only the shortest two bands are available for projects executed after cryogen exhaustion. These images are relatively shallow to enable coverage of a larger area. This project also delivered versions of data from two other projects: Cygnus X and SMOG. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m) Galactic: galactic plane about 1-6 arcsec various, 2004-2009 space NASA GOALS: Great Observatories All-sky LIRG Survey Spitzer and Herschel The Great Observatories All-sky LIRG Survey (GOALS) observed more than 200 galaxies with several observatories. Data from Spitzer and Herschel are both available in IRSA Viewer. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), PACS70 (70 �m), PACS100 (100 �m), MIPS160 (160 �m), PACS160 (160 �m), SPIRE250 (250 �m), SPIRE350 (350 �m), SPIRE500 (500 �m) Extragalactic: More than 200 nearby galaxies about 1 to 35 arcsec various, 2004-2013 space NASA/ESA GOODS: Great Observatories Origins Deep Survey Spitzer and Herschel The Great Observatories Origins Deep Survey (GOODS) observed two extragalactic fields with several observatories. Data from Spitzer and Herschel are both available in IRSA Viewer. and optical: B (4328 �), V (5921 �), I (7692 �), z (9033 �), Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), IRS16 (16 �m), MIPS24 (24 �m), Far IR: PACS100 (100 �m), PACS160 (160 �m), SPIRE250 (250 �m), SPIRE350 (350 �m), SPIRE500 (500 �m) Extragalactic: GOODS fields about 1 to 35 arcsec various, 2004-2013 space NASA HOPS: Herschel Orion Protostar Survey Spitzer and Herschel The Herschel Orion Protostar Survey (HOPS) observed Orion. Data from Spitzer and Herschel are both available in IRSA Viewer. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: PACS70 (70 �m), PACS160 (160 �m) Galactic: Orion about 1 to 10 arcsec various, 2004-2013 space NASA, ESA IUDF: IRAC Ultradeep Field Spitzer The IRAC Ultradeep Field (IUDF) combines IRAC data from several programs. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: Several survey regions about 1 arcsec various, 2009-2017 space NASA LVL: Spitzer Local Volume Legacy Survey Spitzer The Spitzer Local Volume Legacy Survey (LVL) observed nearly 300 galaxies with several observatories. Optical, UV, and Spitzer are available in IRSA Viewer. UV: FUV (1528 �), NUV (2271 �); optical: R (6451 �), Halpha (6585 �); mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far-IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: nearly 300 nearby galaxies about 1 to 40 arcsec various, 2004-2009 space NASA M31IRAC: IRAC Observations of the Extended Disk and Halo of M31 Spitzer The IRAC Observations of the Extended Disk and Halo of M31 (M31IRAC) project observed M31 with IRAC. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: M31 about 1 arcsec various, 2009-2017 space NASA MIPS Local Galaxies Spitzer The MIPS Local Galaxies program (MIPS_LG) compiles the Spitzer MIPS observations of all available galaxies in several Herschel programs. Mid-IR: MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: several nearby galaxies about 6 to 40 arcsec various, 2004-2009 space NASA MIPSGAL: A 24 and 70 Micron Survey of the Inner Galactic Disk with MIPS Spitzer The 24 and 70 Micron Survey of the Inner Galactic Disk with MIPS (MIPSGAL) program surveyed the Galactic plane with Spitzer MIPS observations. Only the 24 micron data were delivered back to IRSA. Mid-IR: MIPS24 (24 �m) Galactic: galactic plane about 6 arcsec various, 2004-2009 space NASA S-CANDELS: Spitzer-Cosmic Assembly Deep Near-Infrared Extragalactic Legacy Survey Spitzer The Spitzer-Cosmic Assembly Deep Near-Infrared Extragalactic Legacy Survey (S-CANDELS) surveyed several extragalactic regions in IRAC-1 and 2. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: several survey regions about 1 arcsec various, 2009-2017 space NASA S4G: The Spitzer Survey of Stellar Structure in Galaxies Spitzer The Spitzer Survey of Stellar Structure in Galaxies (S4G) surveyed almost 2400 nearby galaxies in IRAC-1 and 2. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: extragalactic: almost 2400 nearby galaxies about 1 arcsec various, 2009-2017 space NASA SAFIRES: Spitzer Archival FIR Extragalactic Survey Spitzer The Spitzer Archival FIR Extragalactic Survey (SAFIRES) is an offshoot of SEIP; it delivered MIPS-70 and 160 micron images of extragalactic regions. Far-IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: several survey regions about 20 to 40 arcsec various, 2004-2009 space NASA SAGE: Surveying the Agents of a Galaxy's Evolution Spitzer The Surveying the Agents of a Galaxy's Evolution (SAGE) project observed the LMC with IRAC and MIPS. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: extragalactic: LMC about 1 to 40 arcsec various, 2004-2009 space NASA SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally-Disrupted, Low-Metallicity Small Magellanic Cloud Spitzer The Surveying the Agents of Galaxy Evolution in the Tidally-Disrupted, Low-Metallicity Small Magellanic Cloud (SAGE-SMC) project observed the SMC with IRAC and MIPS. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: extragalactic: SMC about 1 to 40 arcsec various, 2004-2009 space NASA SDWFS: Spitzer Deep, Wide-Field Survey Spitzer The Spitzer Deep, Wide-Field Survey (SDWFS) surveyed the NOAO Deep Wide-Field Survey Bootes field in IRAC. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m) Extragalactic: extragalactic: NOAO Deep Wide-Field Survey Bootes field about 1 arcsec various, 2004-2009 space NASA SEP: Spitzer MIPS 24 and 70 micron Imaging of the South Ecliptic Pole Spitzer SEP observed the South Ecliptic Pole (SEP) with several observatories, but MIPS-24 and 70 microns are available here. Mid-IR: MIPS24 (24 �m); far IR: MIPS70 (70 �m) Extragalactic: extragalactic: South Ecliptic Pole about 6-20 arcsec various, 2004-2009 space NASA SERVS: Spitzer Extragalactic Representative Volume Survey Spitzer The Spitzer Extragalactic Representative Volume Survey (SERVS) surveyed several extragalactic regions in IRAC-1 and 2. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: several survey regions about 1 arcsec various, 2009-2017 space NASA SHELA: Spitzer/HETDEX Exploratory Large-Area survey Spitzer The Spitzer/HETDEX Exploratory Large-Area survey (SHELA) surveyed an extragalactic region with HETDEX and Spitzer (in IRAC-1 and 2); only the Spitzer data are available here. (SHELA+SpIES is Stripe 82.) Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: survey region about 1 arcsec various, 2009-2017 space NASA SIMPLE: Spitzer IRAC/MUSYC Public Legacy Survey in the Extended Chandra Deep Field South Spitzer Spitzer IRAC/MUSYC Public Legacy Survey in the Extended Chandra Deep Field South (SIMPLE) is part of the larger MUSYC project. The Spitzer data are available here (see MUSYC, below, for additional wavelengths). Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m) Extragalactic: CDFS about 1 arcsec various, 2004-2009 space NASA SINGS: The Spitzer Infrared Nearby Galaxies Survey - Spitzer and Ancillary Data Spitzer The Spitzer Infrared Nearby Galaxies Survey (SINGS) observed 75 nearby galaxies with several observatories. Optical, NIR, and Spitzer data are available here. Optical: B (4300 �), V (5480 �), Halpha (6585 �), NII (6618 �), R (7000 �), I (9000 �); mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: 75 nearby galaxies about 1 to 40 arcsec various, 2004-2009 space NASA SMUVS: Spitzer Matching Survey of the Ultra-VISTA Deep Stripes Spitzer The Spitzer Matching Survey of the Ultra-VISTA Deep Stripes (SMUVS) surveyed three Ultra-VISTA near-infrared survey stripes in the COSMOS region with Spitzer (in IRAC-1 and 2); only the Spitzer data are available here. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: COSMOS region about 1 arcsec various, 2009-2017 space/ground NASA SpIES: Spitzer IRAC Equatorial Survey Spitzer The Spitzer IRAC Equatorial Survey (SpIES) is a large-area survey of 115 sq. degrees in the Equatorial SDSS Stripe 82 field with Spitzer (in IRAC-1 and 2); only the Spitzer data are available here. (Also see SHELA.) Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: Stripe 82 about 1 arcsec various, 2009-2017 space NASA SpUDS: Spitzer Public Legacy Survey of the UKIDSS Ultra Deep Survey Spitzer The Spitzer UKIDSS Ultra Deep Survey (SpUDS) surveyed the UKIDSS Ultra Deep Survey region with Spitzer; only the Spitzer data are available here. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m) Extragalactic: survey region about 1 to 6 arcsec various, 2004-2009 space NASA SRELICS: Spitzer Reionization Lensing Cluster Survey Spitzer The Spitzer Reionization Lensing Cluster Survey (SRELICS) is the Spitzer counterpart to the RELICS HST Treasury program (PI: Coe) to survey 41 massive galaxy clusters. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: 41 clusters about 1 arcsec various, 2015-2019 space NASA SSDF: The SPT-Spitzer Deep Field Spitzer The Spitzer-South Pole Telescope Deep Field (SSDF) surveyed a deep field with Spitzer (in IRAC-1 and 2); only the Spitzer data are available here. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m) Extragalactic: survey region about 1 arcsec various, 2009-2017 space NASA SWIRE: Spitzer Wide-area InfraRed Extragalactic Survey Spitzer The Spitzer Wide-area InfraRed Extragalactic Survey (SWIRE) surveyed several extragalactic regions Spitzer as well as other observatories. Spitzer data as well as optical data are available here. Optical: U (3552 �), u (3624 �), g (4750 �), g (4885 �), r (6240 �), r (6292 �), i (7696 �), i (7726 �), z (9120 �); mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), ISO14 (14.3 �m), MIPS24 (24 �m); far-IR: MIPS70 (70 �m), MIPS160 (160 �m) Extragalactic: several survey regions about 1 to 40 arcsec various, 2004-2009 space/ground NASA Taurus 2: Finishing the Spitzer Map of the Taurus Molecular Clouds Spitzer The Taurus project observed the Taurus molecular clouds with Spitzer as well as other observatories. Data from Spitzer are available here. Mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m), MIPS24 (24 �m); far IR: MIPS70 (70 �m), MIPS160 (160 �m) Galactic: Taurus molecular cloud about 1 to 40 arcsec various, 2004-2009 space NASA IRIS: Improved Reprocessing of the IRAS Survey IRAS IRAS was the first all-sky IR survey; the satellite flew in 1983. The Improved Reprocessing of the IRAS Survey (IRIS) data are available here. Mid-IR: IRAS1 (12 �m), IRAS2 (25 �m); far IR: IRAS3 (60 �m), IRAS4 (100 �m) All-sky about 0.5 to 5 arcminutes 1983 space US, UK and the Netherlands. ISSA: IRAS Sky Survey Atlas IRAS IRAS was the first all-sky IR survey; the satellite flew in 1983. The IRAS Sky Survey Atlas (ISSA) data are available here. Mid-IR: IRAS1 (12 �m), IRAS2 (25 �m); far IR: IRAS3 (60 �m), IRAS4 (100 �m) All-sky about 0.5 to 5 arcminutes 1983 space US, UK and the Netherlands. IGA: IRAS Galaxy Atlas IRAS The IRAS Galaxy Atlas (IGA) is a high resolution atlas of the Galactic plane at 60 and 100 microns. far IR: IRAS3 (60 �m), IRAS4 (100 �m) Galactic about 1 arcminute 1983 space US, UK and the Netherlands. EIGA: Extended IRAS Galaxy Atlas IRAS The Extended IRAS Galaxy Atlas (EIGA) is an extension of the original IGA to more northerly galactic latitudes, still at 60 and 100 microns. far IR: IRAS3 (60 �m), IRAS4 (100 �m) Galactic about 1 arcminute 1983 space US, UK and the Netherlands. MIGA: Mid-Infrared Galaxy Atlas IRAS The Mid-Infrared Galaxy Atlas (MIGA) is a high resolution atlas of the Galactc plane at 12 and 25 microns. Mid-IR: IRAS1 (12 �m), IRAS2 (25 �m) Galactic about 0.5 arcminute 1983 space US, UK and the Netherlands. MSX: Midcourse Space Experiment MSX The Midcourse Space Experiment (MSX), a Ballistic Missile Defense Organization satellite, surveyed the Galactic plane and IRAS gap regions. Mid-IR: A (8.28 �m), C (12.13 �m), D (14.65 �m), E (21.3 �m) Galactic: galactic plane about 20 to 70 arcsec 1996-1997 space US Air Force COSMOS: Cosmic Evolution Survey Herschel The Cosmic Evolution Survey (COSMOS) project observed the same field with many, many observatories. The data from this project are available in IRSA Viewer. X-rays: 4.5-10 keV, 2.0-8 keV, 2.0-7.0 keV, 0.5-7.0 keV, 0.5-2.0 keV; UV: FUV (0.1528 �m), NUV (0.2271 �m); optical: U (0.2987 �m), u (0.3591 �m), u (0.3798 �m), IA427 (0.4271 �m), B (0.446 �m), B (0.4556 �m), IA464 (0.4636 �m) g (0.4723 �m), g (0.47469 �m), g+ (0.478 �m), IA484 (0.4842 �m), IA505 (0.5063 �m), IA527 (0.5272 �m), V (0.5484 �m) IA574 (0.5743 �m), F606W (0.5956 �m), r (0.6213 �m) ,IA624 (0.6226 �m), r+ (0.6295 �m), IA679 (0.6788 �m) IA709 (0.7082 �m), NB711 (0.7126 �m), IA738 (0.7371 �m), i (0.7523 �m), i+ (0.7641 �m), i (0.7684 �m), IA767 (0.769 �m), I (0.8057 �m), NB816 (0.8154 �m) IA827 (0.8275 �m) F814W (0.8353 �m), z (0.8855 �m), z+ (0.9037 �m), z++ (0.9037 �m); near-IR: Y (1.02 �m) J1 (1.047 �m), J2 (1.195 �m), J (1.2 �m), F125W (1.25 �m), J (1.25 �m), J3 (1.279 �m), F140W (1.4 �m), F160W (1.545 �m) H1 (1.56 �m), H (1.6028 �m), H (1.631 �m), H (1.64 �m), H2 (1.708 �m), Ks (2.146 �m), K (2.15 �m), Ks (2.2 �m); mid-IR: IRAC1 (3.6 �m), IRAC2 (4.5 �m), IRAC3 (5.8 �m), IRAC4 (8 �m) MIPS24 (24 �m); far IR: MIPS70 (70 �m), PACS100 (100 �m), MIPS160 (160 �m), PACS160 (160 �m), SPIRE250 (250 �m), SPIRE350 (350 �m), SPIRE500 (500 �m); radio: 20 cm, 90 cm" Extragalactic: COSMOS region about 1 to 40 arcsec various space and ground NASA MUSYC: Multiwavelength Survey by Yale-Chile Herschel The Multiwavelength Survey by Yale-Chile (MUSYC) surveyed an extragalactic region with several telescopes, and the multi-wavelength data are available here. Note that the Spitzer observations of this field are part of SIMPLE, above. Optical: U (0.3505 �m), U38 (0.3655 �m), IA427 (0.4271 �m), IA445 (0.4456 �m), B (0.4605 �m), IA464 (0.4636 �m), IA484 (0.4842 �m), OIII (0.499 �m), IA505 (0.5063 �m), IA527 (0.5272 �m), V (0.5383 �m), BVR (0.55 �m), IA550 (0.5512 �m), IA574 (0.5743 �m), IA598 (0.6 �m), IA624 (0.6226 �m), IA651 (0.6502 �m), R (0.652 �m), IA679 (0.6788 �m), IA709 (0.7082 �m), IA738 (0.7371 �m), IA767 (0.769 �m), IA797 (0.7981 �m), IA827 (0.8275 �m), IA856 (0.8566 �m), I (0.8642 �m), z (0.9035 �m); near-IR: J (1.2461 �m), H (1.6534 �m), K (2.1323 �m) Extragalactic: survey region about 1 arcsec various space and ground BLAST: Balloon-borne Large Aperture Submillimeter Telescope BLAST The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) observed several regions during several balloon flights. Far-IR: 250 �m, 350 �m, 500 �m Compilation: survey region about 30 arcsec @ 250 �m 2005-2006 balloon-borne NASA/CSA and participating institutions IRTS: Infrared Telescope in Space IRTS The Infrared Telescope in Space (IRTS) surveyed ~10% of the sky over 20 days. Far-IR: 7.7 �m, 155 �m, 158 �m, 250 �m, 400 �m, 700 �m Compilation: survey region about 8 to 30 arcmin 1995 space ISAS (Japan) GPIPS Galactic Plane Infrared Polarization Survey GPIPS HERON used the Mimir instrument on the 1.8m Perkins telescope Near-IR: H (1.6 �m) Galactic: first Galactic quadrant midplane 18
