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Start Over Resource Type Survey Capability Type Simple Image Access Protocol
61. Sloan Digital Sky Survey DR4 - Images
ID:
ivo://sdss.jhu/services/SIAPDR4-images
Title:
Sloan Digital Sky Survey DR4 - Images
Short Name:
SDSSDR4
Date:
14 Feb 2012 18:49:26
Publisher:
The Johns Hopkins Univer
Description:
The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
62. Sloan Digital Sky Survey DR5 - Images
ID:
ivo://sdss.jhu/services/SIAPDR5-images
Title:
Sloan Digital Sky Survey DR5 - Images
Short Name:
SDSSDR5
Date:
14 Sep 2011 17:51:46
Publisher:
The Johns Hopkins University
Description:
The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
63. Sloan Digital Sky Survey Images (Latest Release)
ID:
ivo://sdss.jhu/services/SIAP-images
Title:
Sloan Digital Sky Survey Images (Latest Release)
Short Name:
SDSS SIAP
Date:
05 Feb 2015 21:10:39
Publisher:
The Johns Hopkins University
Description:
The Sloan Digital Sky Survey is a project to survey a 10000 square degree area on the Northern sky over a 5 year period. A dedicated 2.5m telescope is specially designed to take wide field (3 degrees in diameter) images using a 5x6 mosaic of 2048x2048 CCD`s, in five wavelength bands, operating in drift scan mode. The total raw data will exceed 40 TB. A processed subset, of about 1 TB in size, will consist of 1 million spectra, positions and image parameters for over 100 million objects, plus a mini-image centered on each object in every color. The data will be made available to the public after the completion of the survey
64. SOFIA FLITECAM
ID:
ivo://irsa.ipac/SOFIA/Images/FLITECAM
Title:
SOFIA FLITECAM
Short Name:
SOFIA_FLITECAM
Date:
05 Sep 2024 03:39:50
Publisher:
NASA/IPAC Infrared Science Archive
Description:
FLITECAM was an infrared camera operating in the 1.0 - 5.5 um waveband. It consisted of a 1024x1024 InSb detector with 0.475"x0.475" pixels and used refractive optics to provide an 8' diameter field of view. The instrument had a set of filters for imaging, and grisms for moderate resolution spectroscopy. The filter suite consisted of standard Barr filters used for imaging at J, H, K, L and M in one filter wheel. A second filter wheel held a selection of narrow-band imaging filters including Pa-alpha, Pa-alpha continuum, 3.07 um H2O ice, 3.3 um PAH, L-narrow and M-narrow. Additionally there were order sorting filters for use with the grisms. A selection of three grisms was available to provide medium resolution (R ~ 1500) spectra over the entire wavelength range.
65. SOFIA FORCAST
ID:
ivo://irsa.ipac/SOFIA/Images/FORCAST
Title:
SOFIA FORCAST
Short Name:
SOFIA_FORCAST
Date:
05 Sep 2024 03:40:07
Publisher:
NASA/IPAC Infrared Science Archive
Description:
FORCAST was a dual-channel mid-infrared camera and spectrograph sensitive from 5 - 40 um. Spectroscopy was also possible using a suite of grisms, which provided coverage from 5 - 40 um with a low spectral resolution of R ~ 200.
66. SOFIA FPI+
ID:
ivo://irsa.ipac/SOFIA/Images/FPI
Title:
SOFIA FPI+
Short Name:
SOFIA_FPI
Date:
05 Sep 2024 03:39:30
Publisher:
NASA/IPAC Infrared Science Archive
Description:
FPI+ was the standard tracking camera for the SOFIA telescope with a 1024x1024 pixel science grade CCD sensor. As a science instrument it was intended to be used as a fast frame-rate imaging photometer in the 360 - 1100 nm wavelength range. The FPI+ CCD had a plate scale of 0.51 arcsec/pixel and a square field of view of 8.7x8.7 arcminutes. Its permanent installation on the SOFIA telescope allowed for its use while any other science instrument was installed on the main Science Instrument flange. Five Sloan Digital Sky Survey filters u', g', r', i', z' and a Schott RG1000 NIR cut on filter were available.
67. SOFIA HAWC+
ID:
ivo://irsa.ipac/SOFIA/Images/HAWC
Title:
SOFIA HAWC+
Short Name:
SOFIA_HAWC
Date:
06 Sep 2024 03:40:27
Publisher:
NASA/IPAC Infrared Science Archive
Description:
HAWC+ was a far-infrared camera and imaging polarimeter. It was designed to allow total and polarized flux imaging in five broad bands between wavelengths of 50 um and 240 um. Diffraction-limited imaging yielded spatial resolutions of ~5 - 20 arcseconds with fields of view ~2 - 10 arcminutes, respectively.
68. Spitzer Archival Far-Infrared Extragalactic Survey
ID:
ivo://irsa.ipac/Spitzer/Images/SAFIRES
Title:
Spitzer Archival Far-Infrared Extragalactic Survey
Short Name:
SAFIRES
Date:
27 Oct 2022 19:00:00
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.
69. Spitzer-Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey
ID:
ivo://irsa.ipac/Spitzer/Images/S-CANDELS
Title:
Spitzer-Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey
Short Name:
S-CANDELS
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Spitzer-Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (S-CANDELS) is a Spitzer Cycle 8 Exploration Program (PI G. Fazio) that obtained deep IRAC channel 1 and 2 imaging in five widely separated extragalactic fields: the UKIDSS Ultra-Deep Survey (UDS), the Extended Chandra Deep Field South (ECDFS), COSMOS, the HST Deep Field North (HDFN), and the Extended Groth Strip (EGS). S-CANDELS builds upon the existing coverage of these fields obtained as part of the Spitzer Extended Deep Survey (SEDS), a Cycle 6 Exploration Program, by increasing the integration time from 12 hours to a total of 50 hours within a smaller area of 0.16 deg2.
70. Spitzer Deep Wide-Field Survey
ID:
ivo://irsa.ipac/Spitzer/Images/SDWFS
Title:
Spitzer Deep Wide-Field Survey
Short Name:
SDWFS
Date:
27 Oct 2022 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Spitzer Deep Wide-Field Survey is a four-epoch survey of roughly 10 square degrees of the NOAO Deep, Wide-Field Survey field in Boötes. The first visit to the field occurred very early in the Spitzer mission, in 2004 January, as part of the IRAC Shallow Survey (Eisenhardt et al. 2004). Subsequent visits to the field as part of the SDWFS program reimaged the same area to the same depth.