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Start Over Publisher NASA/IPAC Infrared Science Archive Resource Type Survey
1. A 24 and 70 Micron Survey of the Inner Galactic Disk with MIPS
ID:
ivo://irsa.ipac/Spitzer/Images/MIPSGAL
Title:
A 24 and 70 Micron Survey of the Inner Galactic Disk with MIPS
Short Name:
MIPSGAL
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
MIPSGAL is a survey of the inner 248 square degrees of the Galactic plane at 24 and 70 microns using the MIPS instrument aboard the Spitzer Space Telescope. The survey covers Galactic latitudes of -1° < b < +1° for Galactic longitudes of l < 62° and l > 298°. Version 3.0 of the MIPSGAL data includes mosaics only at 24um, but covering the entire survey region. |b| < 1° is covered for -68° < l < 69°, and |b| < 3° is covered for -8° < l < 9°.
2. AllWISE Atlas (L3a) Coadd Images
ID:
ivo://irsa.ipac/WISE/Images/AllWISE/L3a
Title:
AllWISE Atlas (L3a) Coadd Images
Short Name:
AllWISE L3a
Date:
16 Mar 2017 01:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The AllWISE program builds upon the work of the successful Wide-field Infrared Survey Explorer mission (WISE; Wright et al. 2010) by combining data from the WISE cryogenic and NEOWISE (Mainzer et al. 2011 ApJ, 731, 53) post-cryogenic survey phases to form the most comprehensive view of the full mid-infrared sky currently available. By combining the data from two complete sky coverage epochs using an advanced data processing system, AllWISE has generated new products that have enhanced photometric sensitivity and accuracy, and improved astrometric precision compared to the 2012 WISE All-Sky Data Release. Exploiting the 6 to 12 month baseline between the WISE sky coverage epochs enables AllWISE to measure source motions for the first time, and to compute improved flux variability statistics. The AllWISE Images Atlas is comprised of 18,240 4-band calibrated 1.56°x1.56° FITS images, depth-of-coverage and noise maps, and image metadata produced by coadding nearly 7.9 million Single-exposure images from all survey phases.
3. Auriga-California Molecular Cloud
ID:
ivo://irsa.ipac/Herschel/Images/ACMC
Title:
Auriga-California Molecular Cloud
Short Name:
ACMC
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Auriga-California molecular cloud is a large region of relatively modest star formation that is part of the Gould Belt. The Herschel Space Observatory program OT1_pharvey01_3 ("The Auriga-California Molecular Cloud: A Massive Nearby Cloud With Powerful Diagnostics For Early Stages of Star Formation", PI Paul Harvey) observed a 14.5 square degree area of the cloud in five far-infrared bands.
4. Bolocam Lockman Hole Map
ID:
ivo://irsa.ipac/Bolocam/Images/Bolocam_LH
Title:
Bolocam Lockman Hole Map
Short Name:
Bolocam_LH
Date:
23 May 2023 20:55:52
Publisher:
NASA/IPAC Infrared Science Archive
Description:
A deep 1.1 mm survey using Bolocam of the Lockman Hole, producing a map and galaxy candidate list. This survey encompasses 324 square arcmin to an rms noise level (filtered for point sources) of 1.4 mJy/beam. This project is described by Laurent et al., ApJ, 2005.
5. Bolocam Planck SZ Cluster
ID:
ivo://irsa.ipac/Bolocam/Images/Bolocam_Planck_SZ
Title:
Bolocam Planck SZ Cluster
Short Name:
Bolocam_PlanckSZ
Date:
23 May 2023 20:55:52
Publisher:
NASA/IPAC Infrared Science Archive
Description:
Caltech Submillimeter Observatory data corresponding to 46 galaxy clusters which have been observed by Bolocam at 2.1mm.
6. Cosmic Dawn
ID:
ivo://irsa.ipac/Spitzer/Images/CosmicDawn
Title:
Cosmic Dawn
Short Name:
CosmicDawn
Date:
07 Apr 2023
Publisher:
NASA/IPAC Infrared Science Archive
Description:
Cosmic Dawn is a new infrared survey covering the three Euclid deep fields and four other Euclid calibration fields using Spitzer's Infrared Array Camera (IRAC). These new observations are combined with all relevant IRAC archival data of these fields in order to produce the deepest possible mosaics of these regions. In total, these observations represent nearly 11% of the total Spitzer mission time. The resulting mosaics cover a total of approximately 71.5 deg^2 in the 3.6 and 4.5 micron bands, and approximately 21.8 deg^2 in the 5.8 and 8 micron bands. They reach at least 24 AB magnitude in the 3.6 micron band and up to ~5 mag deeper in the deepest regions. The astrometry is tied to the Gaia astrometric reference system, and the typical astrometric uncertainty for sources with 16 < [3.6] < 19 is 0.15". The photometric calibration is in excellent agreement with previous WISE measurements. Given that the Spitzer Space Telescope has now been decommissioned these mosaics are likely to be the definitive reduction of these IRAC data. This survey therefore represents an essential first step in assembling multi-wavelength data on the Euclid deep fields which are set to become some of the premier fields for extragalactic astronomy in the 2020s.
7. Cosmic Evolution Survey with HST
ID:
ivo://irsa.ipac/COSMOS/Images
Title:
Cosmic Evolution Survey with HST
Short Name:
COSMOS
Date:
16 Mar 2017 01:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The COSMOS Archive serves data taken for the Cosmic Evolution Survey with HST (COSMOS) project, using IRSA's general search service, Atlas. COSMOS is an HST Treasury Project to survey a 2 square degree equatorial field with the ACS camera.
8. Cygnus-X: A Spitzer Legacy Survey of the Cygnus-X Complex
ID:
ivo://irsa.ipac/Spitzer/Images/Cygnus-X
Title:
Cygnus-X: A Spitzer Legacy Survey of the Cygnus-X Complex
Short Name:
Cygnus-X
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Cygnus-X region is one of the brightest regions of the sky at all wavelengths and one of the richest known regions of star formation of the Galaxy. The goals of the Cygnus-X survey are to provide a detailed picture of the processes that govern the evolution of massive star forming complexes, to study star formation in the massive star forming complex environment, and to provide a rich sample of intermediate to high mass protostars spanning the full range of protostellar evolution. The project will also allow us to assess the role of feedback in a massive OB star/molecular cloud complex. The survey imaged a ~24 square degree region centered near 20:30:25, +40:00 (J2000). The IRAC images had a median coverage of 3x12s high dynamic range (HDR) frames, and the MIPS data were taken in fast scanning mode in the 24 and 70 μm bands.
9. Digitized Sky Survey
ID:
ivo://irsa.ipac/DSS/Images
Title:
Digitized Sky Survey
Short Name:
DSS
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Digitized Sky Survey (DSS) is a ground-based imaging survey of the entire sky in several colors. The survey, performed with Palomar and UK Schmidt telescopes, produced photographic plates that were later digitized at the Space Telescope Science Institute (STScI) to produce the Hubble Guide Stars Catalog (GSC). Each plate produced by the Survey covers 6.5 x 6.5 degrees of the sky, and the plates have been digitized using a modified PDS microdensitometer. The digital images have a pixel size of either 25 microns (1.7 arcsec per pixel) or 15 microns (1.0 arcsec per pixel), and are 14000 x 14000 or 23040 x 23040 pixels per side. The images are stored on 12-inch optical media and are difficult to access quickly.
10. Euclid ERO
ID:
ivo://irsa.ipac/Euclid/Images/ERO
Title:
Euclid ERO
Short Name:
Euclid_ERO
Date:
18 Jun 2024 16:17:50
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The ERO program is an initiative of the Euclid Science Team / ESA to collect 1 day of observations to showcase the Euclid mission and its capabilities before the start of the nominal survey. The ERO data products available at IRSA for the convenience of the US astronomy community are the same data products that are available through ESAC. The FITS files were processed with an ERO-specific pipeline, which is different from the standard Euclid pipeline that will be used for future data releases.