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Only one ResourceType (SIAP) found.
93 resources. Showing 1 to 19.
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SIA Service for Subaru/XMM-Newton Deep Survey 01(sia-sxds)
SIAP
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the Subaru/XMM-Newton Deep Survey (SXDS) SIA Service(sxds_sia)
The Subaru/XMM-Newton Deep Survey (SXDS) is a major new multi-wavelength survey of a ~1.3 square degree region of sky.
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the Subaru/XMM-Newton Deep Survey (SXDS) SIA Service(SubaruSXDS)
The Subaru/XMM-Newton Deep Survey (SXDS) is a major new multi-wavelength survey of a ~1.3 square degree region of sky.
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NCSA Astronomy Digital Image Library Simple Image Access(ADIL)
This allows searching for ADIL images via the SIA protocol.
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The IRAS Galaxy Atlas(IGA)
The IRAS Galaxy Atlas (IGA) is a high resolution image atlas of the Galactic plane at 60 and 100 microns, it has been produced using the IRAS satellite data. The HIRES program was developed by the Infrared Processing and Analysis Center (IPAC) to produce high resolution (~ 1 arcmin) images from IRAS data using the Maximum Correlation Method (H.H. Aumann, J.W. Fowler and M. Melnyk, 1990, Astronomical Journal, 99, 1674).
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Spitzer First Look Survey (FLS) -- Ancillary VLA Data(FLS_VLA)
The Spitzer First Look Survey has obtained VLA radio data. Available to the public is a catalog of radio sources along with a mosaic of 35 VLA pointings taken during 2001 and 2002, representing 240 hours in B-array at 1.4 GHz.
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2MASS 6X Lockman Hole Ancillary Data Atlas(LH)
These Lockman Hole (LH) data represent a preliminary analysis of the deep 2MASS observations of this region, and are not a product endorsed by the 2MASS project. These data are described in The Astronomical Journal, Volume 125, Issue 5, pp. 2521-2530 "A Deep 2MASS survey of the Lockman Hole" by Beichman et al.
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The Mid-Infrared Galaxy Atlas(MIGA)
The Mid-Infrared Galaxy Atlas (MIGA) is a high resolution image atlas of the Galactic plane at 12 microns and 25 microns, it has been produced using the HIRES processed infrared data from the IRAS satellite. It is a counterpart to the far-infrared IRAS Galaxy Atlas (IGA) and the Extended IRAS Galaxy Atlas (EIGA).
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2MASS Large Galaxy Atlas(LGA)
The high sensitivity and angular resolution of the 2MASS Large Galaxy Atlas (LGA) images allows closer inspection of diverse stellar populations, large-scale structures such as spirals, bulges, warps and bars, star formation regions and evolution of galaxies. This image atlas represents the first uniform, all-sky, view of galaxies as seen in the near-infrared wavelength window that is most sensitive to the dominant mass component of galaxies.
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The Midcourse Space Experiment Data Atlas(MSX)
The Midcourse Space Experiment (MSX), a Ballistic Missile Defense Organization satellite, was launched in April 1996. The first ten months of the mission were devoted to mid-infrared observations with a solid hydrogen-cooled telescope. This instrument had five line-scanned focal plane arrays that spanned the spectral region from 4.2 to 26 microns.
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The Infrared Telescope in Space Data Atlas(IRTS)
The Infrared Telescope in Space (IRTS) is a cryogenically cooled, small infrared telescope that flew from March - April in 1995. It surveyed approximately 10% of the sky with a relatively wide beam during its 20 day mission. Four focal-plane instruments , the Near-Infrared Spectrometer (NIRS), the Mid-Infrared Spectrometer (MIRS), the Far-Infrared Line Mapper (FILM), and the Far-Infrared Photometer (FIRP) made simultaneous observations of the sky at wavelengths ranging from 1 to 1000 um.
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SFD IR and Dust Map Surveys ( SFD IR )
The full sky 100 micron map is a reprocessed composite of the COBE/DIRBE and IRAS/ISSA maps, with the zodiacal foreground and confirmed point sources removed. Artifacts from the IRAS scan pattern were removed. The result of these manipulations is a map with DIRBE-quality calibration and IR AS resolution. A map proportional to dust column density is also calculated using this information and data from 240 microns.
surveys SIAP
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Digitized Sky Survey: Version 1 ( DSS1 )
his survey comprises the compressed digitization of the Southern Sky Survey and the Palomar Sky Survey E plates as distributed on CD ROM by the Space Telescope Science Institute. Coverage of the entire sky is included. This survey consists of the digititized Southern Sky Survey conducted at the UK Southern Schmidt Survey Group by the Royal Observatory, Edinburgh (prior to 1988) and the Anglo-Australian Observatory (since 1988) Additional plates covering regions with bright objects are also included. The plates were digitized at the Space Telescope Science Institute and compressed using algorithms developed by R.White. These data are distributed on a set of 101 CD-ROMs. i
surveys SIAP
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ROSAT PSPC Pointed Observations Mosaic ( ROSAT/PSPC )
The ROSAT PSPC surveys were generated by SkyView as mosaics from publically available PSPC observations. Approximately 15% of the sky is covered by one or more PSPC observation. These are scattered over the sky but concentrate on targets of interest. Note that a query to the SIA service will return a link regardless of whether there are any observations at the given region. A total of 9 maps were created with a count, exposure and intensity map for each of three different cutoff radii. Since the spatial resolution of the PSPC was a strong function of offset from the center of the field of view, use of the smaller cutoffs is recommended when looking for evidence of spatial extent. However, the small cutoff maps have much smaller total sky coverage.
surveys SIAP
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The NASA/IPAC Extragalactic Database Image Data Atlas(NED(images))
NED is built around a master list of extragalactic objects for which cross-identifications of names have been established, accurate positions and redshifts entered to the extent possible, and some basic data collected. Bibliographic references relevant to individual objects have been compiled, and abstracts of extragalactic interest are kept on line. Detailed and referenced photometry, position, and redshift data, have been taken from large compilations and from the literature. NED also includes images for over 773,000 extragalactic objects from 2MASS, from the literature, and from the Digitized Sky Survey. NED's data and references are being continually updated, with revised versions being put on-line every 2-3 months.
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The IRAS Sky Survey Atlas(ISSA)
The IRAS Sky Survey Atlas (ISSA) is a survey of 98% of the sky in four bands with effective wavelengths of 12, 25, 60 and 100 microns, which was done during a ten month period from January to November, 1983. The ISSA covers the sky with 430 fields. Each field is a 12.5 deg. by 12.5 deg. region centered every 10 deg. along declination bands which are spaced 10 deg. apart.
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2MASS All-Sky Quicklook Image Service(2MASS QL)
This service provides access to and information about the 2MASS All-Sky Quicklook Images. The Quicklook Images delivered by this service are restored from lossy-compressed files in FITS format with full WCS information contained in the image headers. These images are suitable for position measurements, finding charts and visual inspection of the near-infrared sky.
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The MAST Image Scrapbook(MAST-Scrapbook)
The MAST Spectral/Image Scrapbook is designed to allow users to take a quick look at sample data in the MAST archive of a particular astronomical object of interest. It is set up here as an interoperability project between IRSA and MAST.
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SIAP Service Hubble Space Telescope preview images(HST/SIAP/PREVIEW)
SIAP service for HST preview images. Supported instruments: WFPC2 ACS NICMOS FOC.
SIAP
Found 93 resources. Showing 1 to 19.
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Sponsored by the National Science Foundation under Cooperative Agreement AST0122449 with
The Johns Hopkins University. Developed in collaboration with the International Virtual Observatory Alliance.