Number of results to display per page
Search Results
- ID:
- ivo://mast.stsci/siap/hst.previews
- Title:
- Hubble Space Telescope Preview Images
- Short Name:
- HST Previews
- Date:
- 22 Jul 2020 22:27:41
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Quick-look preview images produced and processed by CADC. Data from the following HST instruments are included: WFPC, WFPC2, STIS, NICMOS, FOC, and ACS.
- ID:
- ivo://mast.stsci/siap/3cr
- Title:
- Hubble Space Telescope Snapshots of 3CR Radio Galaxies
- Short Name:
- HST.3cr
- Date:
- 23 Jul 2020 19:40:22
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The revised 3C catalogue (3CR, Bennett 1962) forms a flux-limited sample of the most radio-powerful sources in the northern hemisphere. Over the decade and a half of HST operation we have performed "snapshot" imaging from the near-IR to the near-UV of a large number of these sources. Most recently we have completed a NICMOS 1.6 micron survey of low-redshift (z less than 0.3) 3CR sources (Madrid et al. 2006, Floyd et al 2008). The fully-reduced data for all 101 sources included in those papers are presented here in numerical order.
- ID:
- ivo://mast.stsci/ssap/hst
- Title:
- Hubble Space Telescope Spectra
- Short Name:
- HST Spectra
- Date:
- 22 Jul 2020 21:49:04
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the following HST instruments are available: GHRS (processed by CADC), FOS (processed by ECF), and STIS (1st order). Separate SSAP services are registered for each instrument. VO-compatible FITS files were created by MAST staff.
- ID:
- ivo://mast.stsci/siap/udfuv
- Title:
- Hubble Space Telescope Ultraviolet Images of the UDF and HDF
- Short Name:
- HST.udfuv
- Date:
- 22 Jul 2020 22:22:46
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Wavelength coverage of the Hubble Ultra Deep Field (UDF) has been extended to ultraviolet wavelength observations. Observations include ACS-SBC images in the Far-UV {1500 Angstrom} and WFPC2 images in the Near-UV {F300W} during excution of the HST Treasury program 10403 ( PI Harry Teplitz -- California Institute of Technology). Included with this set of data are ACS/SBC observations of the Hubble Deep Field (HDF) North.
- ID:
- ivo://mast.stsci/hudf09
- Title:
- Hubble Ultra Deep Field 2009 (HUDF09)
- Short Name:
- HUDF09
- Date:
- 22 Jul 2020 22:33:31
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Hubble Ultra Deep Field 2009 (HUDF09) program observations were obtained as HST program 11563 (PI: Garth Illingworth) from August 2009 to February 2011 (Cycle 17). The program uses WFC3/IR as the prime instrument for 192 orbits to image the deep ACS fields that were obtained in the original HUDF (PI: Steven Beckwith) program and in the HUDF05 (PI: Massimo Stiavelli) program. The data are organized into sets of images by HUDF09 pointing and by passband (WFC3/IR F105W, F125W & F160W). Each image is approximately 3k x 3k pixels in size and a scale of 0.06 arcsec/pixel. All three pointings reside in the GOODS/Chandra South field and each pointing includes a drizzled science image and a weight image.
- ID:
- ivo://obs-lyon.fr/hfa/ssa
- Title:
- HyperLeda FITS Archive Simple Spectrum Data Access(HFA SSA)
- Short Name:
- HFA
- Date:
- 15 Apr 2008 20:18:49
- Publisher:
- CRAL-Observatoire de Lyon
- Description:
- A compilation of 1D reference spectra of stars and galaxies. Spectra from several archives and libraries have been collected, re-documented and re-formatted. The spectral resolution is between R=100 and 250000. Some spectra give the physical flux, either or not corrected for the Galactic extinction, and some others are normalized to the pseudo-continuum. Some are given in physical units, and some are momalized to some particular wavelengths (often 5500 A).
268. IAC80 Image Archive
- ID:
- ivo://iacvo/IAC80
- Title:
- IAC80 Image Archive
- Short Name:
- IAC80
- Date:
- 11 Aug 2023 00:47:36
- Publisher:
- Instituto de Astrofisica de Canarias
- Description:
- General optical CCD observations of the north sky with the IAC80 telescope at the Teide Observatory (Tenerife)
- ID:
- ivo://nasa.heasarc/icecubepsc
- Title:
- IceCube All-Sky Point-Source Neutrino Events Catalog (2008-2018)
- Short Name:
- ICECUBEPSC
- Date:
- 07 Mar 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- IceCube has performed several searches for point-like sources of neutrinos. The events contained in this release make up the sample used in IceCube's 10-year time-integrated neutrino point source search [1]. Events in the sample are track-like neutrino candidates detected by IceCube between April 2008 and July 2018. The data contained in this release of IceCube's point source sample shows 3.3 sigma evidence of a cumulative excess of events from a catalog of 110 potential sources, primarily driven by four sources (NGC 1068, TXS 0506+056, PKS 1424+240, and GB6 J1542+6129). NGC 1068 gives the largest excess and appears in spatial coincidence with the hottest spot in the full Northern sky search [1]. IceCube's 10-year neutrino point source event sample includes updated processing for events between April 2012 and May 2015, leading to differences in significances of some sources, including TXS 0506+056. For more information, please refer to [2]. This release contains data beginning in 2008 (IC40) until the spring of 2018 (IC86-VII). In order to standardize the release format of IceCube's point source candidate events, this release duplicates and supplants previously released data from 2012 and earlier. Events from this release cannot be combined with other IceCube public data releases. Please note that this dataset is dominated by background events from atmospheric muons and neutrinos detected by IceCube, with a subdominant astrophysical event contribution. Any spatial or temporal correlations should therefore be carefully evaluated on a statistical basis. See [1] and references therein for details regarding the statistical techniques used by IceCube. [1] Time-integrated Neutrino Source Searches with 10 years of IceCube Data, Phys. Rev. Lett. 124, 051103 (2020) [2] IceCube Data for Neutrino Point-Source Searches: Years 2008-2018, <a href="https://arxiv.org/abs/2101.09836">https://arxiv.org/abs/2101.09836</a> For additional questions about this table, please contact the authors: data [AT] icecube.wisc.edu. This database table was ingested by the HEASARC in July 2021 and is based upon files provided by the IceCube Collaboration and available from their <a href="http://doi.org/DOI:10.21234/sxvs-mt83">website</a>. This is a service provided by NASA HEASARC .
- ID:
- ivo://nasa.heasarc/skyview/iris
- Title:
- Improved Reprocessing of the IRAS Survey: 12
- Short Name:
- IRIS
- Date:
- 07 Mar 2025
- Publisher:
- NASA/GSFC HEASARC
- Description:
- The IRIS data is a reprocessing of the IRAS data set and has the same geometry as the IRAS Sky Survey Atlas (ISSA, labeled as IRAS nnn micron in <i>SkyView</i>) surveys. This new generation of IRAS images, called IRIS, benefits from a better zodiacal light subtraction, from a calibration and zero level compatible with DIRBE, and from a better destriping. At 100 micron the IRIS product is also a significant improvement from the Schlegel et al. (1998) maps. IRIS keeps the full ISSA resolution, it includes well calibrated point sources and the diffuse emission calibration at scales smaller than 1 degree was corrected for the variation of the IRAS detector responsivity with scale and brightness. The uncertainty on the IRIS calibration and zero level are dominated by the uncertainty on the DIRBE calibration and on the accuracy of the zodiacal light model. <p> More information about the IRIS dataset is available at <a href="https://www.cita.utoronto.ca/~mamd/IRIS"> the IRIS website</a> whence most of the preceding description came. Provenance: Original IRAS data: NASA/JPL IPAC, <br> IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut d'Astrophysique Spatiale<br> See the <a href="https://www.cita.utoronto.ca/~mamd/IRIS"> IRIS website</a>.. This is a service of NASA HEASARC.
![the Fornax VST Survey is licensed under the `Creative Commons Attribution 4.0 License <http://creativecommons.org/licenses/by/4.0/>`_ .. image:: /static/img/ccby.png :alt: [CC-BY]](/registry-search/?f%5Brights_facet%5D%5B%5D=the+Fornax+VST+Survey+is+licensed+under+the+%60Creative+Commons+Attribution+4.0+License+%3Chttp%3A%2F%2Fcreativecommons.org%2Flicenses%2Fby%2F4.0%2F%3E%60_%0A%0A..+image%3A%3A+%2Fstatic%2Fimg%2Fccby.png%0A+++%3Aalt%3A+%5BCC-BY%5D%0A%0A&f%5Btype_facet%5D%5B%5D=Archive&f%5BvalidationLevel_facet%5D%5B%5D=2){kind=link}