- 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
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- 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
- ID:
- ivo://nasa.heasarc/skyview/sdss
- Title:
- Sloan Digital Sky Survey g-band
- Short Name:
- SDSS
- Date:
- 18 Apr 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- The Sloan Digital Sky Survey is the deepest large scale survey of the sky currently available. SkyView dynamically queries the SDSS archive (current release DR16) to retrieve data and resample it into the user requested frame. All releases after DR9 are spectra only, so all imaging data originates from DR9. Further information about SDSS and many additional services are available at the <a href="https://www.sdss.org">SDSS website</a>. Provenance: Sloan Digital Sky Survey Team. This is a service of NASA HEASARC.
- ID:
- ivo://nasa.heasarc/skyview/sdssdr7
- Title:
- Sloan Digital Sky Survey g-band DR7
- Short Name:
- SDSSDR7
- Date:
- 04 Apr 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- The Sloan Digital Sky Survey is the deepest large scale survey of the sky currently available. SkyView dynamically queries the SDSS archive to retrieve information and resample it into the user requested frame. Further information on the SDSS and many additional services are available at the <a href="https://www.sdss.org/">SDSS website</a>. Provenance: Sloan Digital Sky Survey Team. This is a service of NASA HEASARC.
- 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
236. 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.
237. 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.
238. 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.
239. 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.
- ID:
- ivo://nasa.heasarc/skyview/goods-isaac-h
- Title:
- Southern GOODS Field: VLT ISAAC Observations, H band
- Short Name:
- GOODS ISAAC H
- Date:
- 18 Apr 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- As part of the Great Observatories Origins Deep Survey (GOODS), near-infrared imaging observations of the Chandra Deep Field South (CDF-S) were carried out in J, H, Ks bands, using the ISAAC instrument mounted at the Antu Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile. <p> These data were obtained as part of the ESO Large Programme 168.A-0485 (PI: C. Cesarsky). Data covering four ISAAC fields in J and Ks bands were also drawn from the ESO programmes 64.O-0643, 66.A-0572 and 68.A-0544 (PI: E.Giallongo), which were part of the previous data releases. <p> This data release covers 172.4, 159.6, and 173.1 arcmin2 of the GOODS/CDF-S region in J, H and Ks respectively. More than 50% of the images reach a 5-sigma depth for point sources of at least 25.2 mag (J), 24.7 mag (H and Ks) in the AB system ("median depth"). <p> This final GOODS/ISAAC data release accumulates observational data which have been acquired in 12814 science integrations between October 1999 and January 2007 totaling 1.3 Msec integration time. [Above adapted from reference website.] <p> <i> SkyView</i> uses the mosaic files provided in this delivery. The Version 1.5 mosaic is used for the KS band. Provenance: Data downloaded from VLT archive. This is a service of NASA HEASARC.