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Start Over Capability Type Simple Image Access Protocol
81. GOODS Chandra ACIS: Full band (0\.5\-8 keV)
ID:
ivo://nasa.heasarc/skyview/goodsacisfb
Title:
GOODS Chandra ACIS: Full band (0\.5\-8 keV)
Short Name:
GOODSACISFB
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
This survey comprises the 2 Ms Chandra Deep Field North and 4 Ms Deep Field South ACIS observations. All observations are co-added into two fields in the north and south. Data are provided in three bands, the soft 0.5-2 keV band, the hard 2.0-8.0 keV and the full 0.5 to 8 keV band. Provenance: Taken from the Neil Brandt's PSU websites for the the <a href="https://personal.psu.edu/wnb3/hdf/hdf-chandra.html">north</a> and <a href="https://personal.psu.edu/wnb3/cdfs/cdfs-chandra.html">south</a>.. This is a service of NASA HEASARC.
82. GOODS Herschel 100 micron, DR1 data release
ID:
ivo://nasa.heasarc/skyview/goodsherschel1
Title:
GOODS Herschel 100 micron, DR1 data release
Short Name:
GOODSHerschel1
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
GOODS-Herschel is an open time key program of more than 360 hours of observation with the Hershel, SPIRE and PACS, from 100 um and 500. <p> North and South GOODS data is available for 100 and 160 microns (using PACS) but only the northern field is available at 250, 350 and 500 microns (using SPIRE). <p> Note that the scale and resolution of the underlying pixels is different in each band. Provenance: Downloaded from the <a href="https://hedam.lam.fr/GOODS-Herschel/">Herschel Database in Marseille</a>. Release DR1.. This is a service of NASA HEASARC.
83. GOODS Herschel 350 micron, DR1 data release
ID:
ivo://nasa.heasarc/skyview/goodsherschel4
Title:
GOODS Herschel 350 micron, DR1 data release
Short Name:
GOODSHerschel4
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
GOODS-Herschel is an open time key program of more than 360 hours of observation with the Hershel, SPIRE and PACS, from 100 um and 500. <p> North and South GOODS data is available for 100 and 160 microns (using PACS) but only the northern field is available at 250, 350 and 500 microns (using SPIRE). <p> Note that the scale and resolution of the underlying pixels is different in each band. Provenance: Downloaded from the <a href="https://hedam.lam.fr/GOODS-Herschel/">Herschel Database in Marseille</a>. Release DR1.. This is a service of NASA HEASARC.
84. GOODS Herschel 160 micron, DR1 data release
ID:
ivo://nasa.heasarc/skyview/goodsherschel2
Title:
GOODS Herschel 160 micron, DR1 data release
Short Name:
GOODSHerschel2
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
GOODS-Herschel is an open time key program of more than 360 hours of observation with the Hershel, SPIRE and PACS, from 100 um and 500. <p> North and South GOODS data is available for 100 and 160 microns (using PACS) but only the northern field is available at 250, 350 and 500 microns (using SPIRE). <p> Note that the scale and resolution of the underlying pixels is different in each band. Provenance: Downloaded from the <a href="https://hedam.lam.fr/GOODS-Herschel/">Herschel Database in Marseille</a>. Release DR1.. This is a service of NASA HEASARC.
85. GOODS Herschel 500 micron, DR1 data release
ID:
ivo://nasa.heasarc/skyview/goodsherschel5
Title:
GOODS Herschel 500 micron, DR1 data release
Short Name:
GOODSHerschel5
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
GOODS-Herschel is an open time key program of more than 360 hours of observation with the Hershel, SPIRE and PACS, from 100 um and 500. <p> North and South GOODS data is available for 100 and 160 microns (using PACS) but only the northern field is available at 250, 350 and 500 microns (using SPIRE). <p> Note that the scale and resolution of the underlying pixels is different in each band. Provenance: Downloaded from the <a href="https://hedam.lam.fr/GOODS-Herschel/">Herschel Database in Marseille</a>. Release DR1.. This is a service of NASA HEASARC.
86. GOODS Herschel 250 micron, DR1 data release
ID:
ivo://nasa.heasarc/skyview/goodsherschel3
Title:
GOODS Herschel 250 micron, DR1 data release
Short Name:
GOODSHerschel3
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
GOODS-Herschel is an open time key program of more than 360 hours of observation with the Hershel, SPIRE and PACS, from 100 um and 500. <p> North and South GOODS data is available for 100 and 160 microns (using PACS) but only the northern field is available at 250, 350 and 500 microns (using SPIRE). <p> Note that the scale and resolution of the underlying pixels is different in each band. Provenance: Downloaded from the <a href="https://hedam.lam.fr/GOODS-Herschel/">Herschel Database in Marseille</a>. Release DR1.. This is a service of NASA HEASARC.
87. GOODS HST ACS B Filter
ID:
ivo://nasa.heasarc/skyview/goods-acs-b
Title:
GOODS HST ACS B Filter
Short Name:
GOODS ACS B
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
This is a <i>SkyView</i> rendering of the HST ACS data as described in the <a href="https://archive.stsci.edu/pub/hlsp/goods/v2/h_goods_v2.0_rdm.html">release document</a>. This comprises four bands of observations of each both the north and south GOODS regions. <p> These data are stored in SkyView as a hierarchical image with 7 levels of pixels, each with a factor of 2 change in scale. Thus the coarsest sampling using pixels 64 times larger than the finest. As we go to coarser pixels, 4 adjacent pixels forming a square are averaged to create the pixel in the next level. The coarsest pixel scale that is at least the resolution requested is used. <p> The exposure times are given as: <table> <tr><th colspan=3> GOODS ACS exposure (s)</th></td></tr> <tr><th>Band</th><th>North></th><th>South</th> <tr><td>z850</td><td>24760</td><td>18232</td></tr> <tr><td>i775</td><td>8530</td><td>7028</td></tr> <tr><td>V606</td><td>5650</td><td>5450</td></tr> <tr><td>B435</td><tr>7200</td><td>7200</td></tr> </table> Provenance: Created by the GOODS team and distributed by MAST. This is a service of NASA HEASARC.
88. GOODS NICMOS Survey
ID:
ivo://nasa.heasarc/skyview/gns
Title:
GOODS NICMOS Survey
Short Name:
GNS
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The GOODS NICMOS Survey (GNS) is a 180 orbit Hubble Space Telescope survey consisting of 60 pointings with the NICMOS-3 near-infrared camera. Each pointing is centred on a massive galaxy (M<sub>*</sub> > 1011 M<sub>sun</sub>) in the redshift range 1.7 < z < 3, selected by their optical-to-infrared colours (Papovich+06,Yan+04,Daddi+07) from the GOODS (Great Observatories Origins Deep Survey) fields. <p> The positions of the 60 GNS pointings were optimised to contain as many massive galaxies as possible and are partly overlapping, covering a total area of about 45 arcmin2. The field of view of the NICMOS-3 camera is 51.2 × 51.2 arcsec with a resolution of about 0.1 arcsec/pixel. The PSF has a width of about 0.3 arcsec FWHM. The limiting magnitude in H band reached at 5σ is HAB = 26.8, about 2 magnitudes fainter than in available ground based data of the GOODS fields. [Taken from reference website.] Provenance: University of Nottingham, GNS group.. This is a service of NASA HEASARC.
89. GOODS North Observations with the VLA
ID:
ivo://nasa.heasarc/skyview/goodsnvla
Title:
GOODS North Observations with the VLA
Short Name:
GOODSNVLA
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
A combination of VLA measurements in all four configurations combined to generate a very deep image of the GOODS North region. A total of about 150 hours of VLA time was used. Data are sensitive to about 5 microJanskies in the central region. A total of 1230 discrete sources where found in the 40'x40' region. Provenance: VLA Observations taken by Morrison et al. as provided through their <a href="https://www.ifa.hawaii.edu/~morrison/GOODSN/">website</a>.. This is a service of NASA HEASARC.
90. GRANAT/SIGMA Significance
ID:
ivo://nasa.heasarc/skyview/granat
Title:
GRANAT/SIGMA Significance
Short Name:
GRANAT
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The Soviet orbital observatory GRANAT was launched in December 1989 and was operational till November 1998. One of the main instruments of the observatory was the French-Soviet hard X-ray coded mask telescope SIGMA (Paul et al.1 1991, Adv.Space Res., 11, 279). It was the first space telescope that used coded aperture technique for reconstruction of sky images in hard X-rays (35-1300 keV). The angular resolution of the telescope was approximately 12' and the accuracy of a source localization is approximately 2-3'.<p> SIGMA discovered numerous interesting hard X-ray sources including GRS 1758-258, which is located only 40' from bright soft X-ray source GX 5-1. It detected hard X-ray flux from X-ray burster A1742-294, which is very near to bright black hole binary 1E1740.7-2942. SIGMA set an upper limit on the hard X-ray flux of from the central supermassive black hole in our Galaxy.<p> During the period 1990-1998 SIGMA observed more that one quarter of the sky with sensitivity better than 100 mCrab. The Galactic Center region had the deepest exposure ( approximately 9 million sec), with the sensitivity to a source discovery (S/N &gt; ~ 5) or approximately 10 mCrab.<p> A list of all detected sources with references to publications on them is presented in the paper of Revnivtsev et al. 2004, Astr. Lett. v.6. In these survey images (40-100 keV) all performed observations are averaged together. Transient sources that were discovered by SIGMA may not visible in the averaged image. <p> This survey has some features that users should keep in mind. The SIGMA telescope is a complicated instrument and is strongly dominated by the accuracy of the background subtraction. The presence of a very bright source in the field of view of the telescope sometimes cannot be fully accounted for and as a result of it some 'ghost' sources can appear. Such features can be seen in the regions near very bright sources like Crab Nebula, Cyg X-1, Nova Per 1992, Nova Mus 1991, Nova Oph 1993, and in the Galactic Center region. In addition to its nominal field of view (~17x17 deg) located around the optical axis of the telescope, SIGMA had another window of relatively high transparency of its shield, approximately 20-30&amp;#176;; apart from the optical axis. Becuase of this a very bright sources like Cyg X-1 can cause non zero illumination of the SIGMA detector if they are located approximately 20-30&amp;#176;; from the optical axis. The ring-like features caused by this effect, can be seen around Cyg X-1, and Nova Per 1992. <p> The count rate of detected sources (or upper limits) can be roughly translated into mCrab using the fact that that Crab nebula gives the count rate approximately 2.8e<sup>-3</sup> cnts/s in the units, provided in 'flux' maps Provenance: High Energy Astrophysics Department, Space Research Institute, Moscow, Russia; CEA, Centre d'Etudes de Saclay Orme des Merisiers, France; Centre d'Etude Spatiale des Rayonnements, Toulouse, France; F&amp;eacute;d&amp;eacute;ration de Recherche Astroparticule et Cosmologie Universit&amp;eacute; de Paris, France. This is a service of NASA HEASARC.
91. Great Observatories All-sky LIRG Survey
ID:
ivo://irsa.ipac/GOALS/Images
Title:
Great Observatories All-sky LIRG Survey
Short Name:
GOALS
Date:
25 Mar 2017
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The GOALS sample consists of a total of 179 LIRGs (log (L_IR/L_sun) = 11.0-11.99) and 22 ultra-luminous infrared galaxies (ULIRGs: log (L_IR/L_sun) > 12.0) selected from the IRAS Revised Bright Galaxy Sample; these 201 objects comprise a statistically complete flux-limited sample of infrared-luminous galaxies in the local universe. The GOALS objects have been the subject of an intense multi-wavelength observing campaign, including space-based imaging and spectroscopy from Spitzer and Herschel.
92. Great Observatories Origins Deep Survey
ID:
ivo://irsa.ipac/Spitzer/Images/GOODS
Title:
Great Observatories Origins Deep Survey
Short Name:
GOODS
Date:
13 Jun 2023 01:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths.
93. Great Observatories Origins Deep Survey (GOODS)
ID:
ivo://mast.stsci/siap/goods.hst
Title:
Great Observatories Origins Deep Survey (GOODS)
Short Name:
HST.GOODS
Date:
23 Jul 2020 19:32:07
Publisher:
Space Telescope Science Institute Archive
Description:
GOODS aims to unite extremely deep observations from NASA's Great Observatories, the Spitzer Space Telescope, Hubble, and Chandra, ESA's XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS will survey a total of roughly 320 square arcminutes in two fields centered on the Hubble Deep Field North and the Chandra Deep Field South.
94. Great Observatories Origins Deep Survey (GOODS) Cutout Service
ID:
ivo://mast.stsci/siap-cutout/goods.hst
Title:
Great Observatories Origins Deep Survey (GOODS) Cutout Service
Short Name:
HST.GOODS.Cutout
Date:
05 Dec 2018 16:38:09
Publisher:
Space Telescope Science Institute Archive
Description:
GOODS aims to unite extremely deep observations from NASA's Great Observatories, the Spitzer Space Telescope, Hubble, and Chandra, ESA's XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the broadest range of wavelengths. GOODS will survey a total of roughly 320 square arcminutes in two fields centered on the Hubble Deep Field North and the Chandra Deep Field South.
95. GTC OSIRIS Simple Image Access Service
ID:
ivo://svo.cab/gtc_osiris
Title:
GTC OSIRIS Simple Image Access Service
Short Name:
GTC OSIRIS
Date:
29 May 2020 10:28:02
Publisher:
Spanish Virtual Observatory
Description:
GTC OSIRIS Simple Image Access Service
96. GTEE 0035 MHz Radio survey
ID:
ivo://nasa.heasarc/skyview/gtee
Title:
GTEE 0035 MHz Radio survey
Short Name:
GTEE
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
This survey is a mosaic of data taken at the low frequency T-array near Gauribidanur, India. The data was distributed in the NRAO Images from the Radio Sky CD ROM. <p> The original 287x101 tiles had only 1 pixel overlap. To allow higher order resampling, the data were retiled into two hemisphere files of 1726x600 pixels with an overlap of 10 pixels. <p> The southernmost tiles were only 287x100 pixels. We assumed that bottom row of these tiles (as compared with the others) was truncated. Provenance: . This is a service of NASA HEASARC.
97. Haloes and Environments of Nearby Galaxies
ID:
ivo://irsa.ipac/HERON
Title:
Haloes and Environments of Nearby Galaxies
Short Name:
HERON
Date:
01 May 2023 19:00:00
Publisher:
NASA/IPAC Infrared Science Archive
Description:
HERON used a dedicated 0.7-m telescope to image the haloes of 124 galaxies in the Local Volume to surface brightnesses of 28-30 mag/arcsec^2. The sample is primarily from the Two Micron All Sky Survey Large Galaxy Atlas and extended to include nearby dwarf galaxies and more distant giant ellipticals, and spans fully the galaxy color-magnitude diagram including the blue cloud and red sequence
98. H-alpha Full Sky Map
ID:
ivo://nasa.heasarc/skyview/halpha
Title:
H-alpha Full Sky Map
Short Name:
HAlpha
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
The full-sky H-alpha map (6' FWHM resolution) is a composite of the Virginia Tech Spectral line Survey (VTSS) in the north and the Southern H-Alpha Sky Survey Atlas (SHASSA) in the south. Stellar artifacts and bleed trails have been carefully removed from these maps. The Wisconsin H-Alpha Mapper (WHAM) survey provides a stable zero-point over 3/4 of the sky on a one degree scale. This composite map can be used to provide limits on thermal bremsstrahlung (free-free emission) from ionized gas known to contaminate microwave-background data. The map (in Rayleighs; 1R=10<sup>6</sup>/4pi photons/cm<sup>2</sup>/s/sr), an error map, and a bitmask are provided in 8640x4320 Cartesian projections as well as HEALPIX (Nside 256, 512, and 1024) projections on the <a href="https://faun.rc.fas.harvard.edu/dfink/skymaps/halpha/"> H-Alpha Full-Sky Map website</a>. Provenance: . This is a service of NASA HEASARC.
99. HDAP -- Heidelberg Digitized Astronomical Plates
ID:
ivo://org.gavo.dc/lswscans/res/positions/siap
Title:
HDAP -- Heidelberg Digitized Astronomical Plates
Short Name:
hdap_siap
Date:
31 Oct 2023 19:15:05
Publisher:
The GAVO DC team
Description:
Scans of plates kept at Landessternwarte Heidelberg-Königstuhl. They were obtained at location, at the German-Spanish Astronomical Center (Calar Alto Observatory), Spain, and at La Silla, Chile. The plates cover a time span between 1880 and 1999. Specifically, HDAP is essentially complete for the plates taken with the Bruce telescope, the Walz reflector, and Wolf's Doppelastrograph at both the original location in Heidelberg and its later home on Königstuhl.
100. HEAO 1A
ID:
ivo://nasa.heasarc/skyview/heao1a
Title:
HEAO 1A
Short Name:
HEAO1A
Date:
10 May 2024
Publisher:
NASA/GSFC HEASARC
Description:
These data were generated at the HEASARC in 1994. Certain gaps and streaks in the image have been fixed by interpolating over the the gap. Typically these gaps are no more than a pixel or two wide. A brief description of the satellite and the data analysis follows. The map used in <i> SkyView </i> is the map designated <tt> 322_15_tot_ecl_samp.img</tt> in the <a href=ftp://legacy.gsfc.nasa.gov/heao1/data/a2/maps/heasarc_med_hed> HEASARC FTP area</a>. Many other maps are available. These differ in epoch, resolution, energy band, coordinate system and projection, and sampling methods. Details are given in the README file in the archive. <p> See Allen, Jahoda, and Whitlock (1994) for full details about the available maps, their processing, and methods for converting the map intensities into familiar physical units. Provenance: NASA, HEASARC. This is a service of NASA HEASARC.

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