Copyright DSS Consortium. These data are from the DSS2 survey.
http://gsss.stsci.edu/Acknowledgements/DataCopyrights.htm
http://www.worldwidetelescope.org/thumbnails/DSS.png
PanSTARRS / STScI / C. Brasseur
https://panstarrs.stsci.edu/
http://data1.wwtassets.org/packages/2020/06_ps1_3pi/thumb.png
Gaia Data Processing and Analysis Consortium (DPAC); A. Moitinho / A. F. Silva / M. Barros / C. Barata, University of Lisbon, Portugal; H. Savietto, Fork Research, Portugal
https://sci.esa.int/web/gaia/-/60196-gaia-s-sky-in-colour-equirectangular-projection
http://data1.wwtassets.org/packages/2020/09_gaia_dr2/thumb.jpg
Image Courtesy Douglas Finkbeiner. 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. The Wisconsin H-Alpha Mapper (WHAM) survey provides a stable zero-point over 3/4 of the sky on a one degree scale.
http://www.astro.princeton.edu/~dfink/halpha/processing.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=halpha
NASA/JPL-Caltech/UCLA
http://wise.ssl.berkeley.edu/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wise
This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
http://www.ipac.caltech.edu/2mass/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=2mass
Data provided by two NASA satellites, the Infrared Astronomy Satellite (IRAS) and the Cosmic Background Explorer (COBE). Processing by David J. Schlegel, Douglas P. Finkbeiner and Marc Davis, Princeton University and University of California, Berkeley.
http://astro.berkeley.edu/~marc/dust/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=dust
Planck is a European Space Agency mission, with significant participation from NASA. NASAs Planck Project Office is based at JPL. JPL contributed mission-enabling technology for both of Plancks science instruments. European, Canadian and U.S. Planck scientists work together to analyze the Planck data.
http://www.nasa.gov/mission_pages/planck/index.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=planck
National Radio Astronomy Observatory. The NVSS project includes J. J. Condon, W. D. Cotton, E. W. Greisen, Q. F. Yin, R. A. Perley (NRAO), and J. J. Broderick (VPI). TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope.
http://www.cv.nrao.edu/nvss/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=vlss
Space Telescope Science Institute. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope. The Galaxy Explorer instrument allows observations to be made in ultraviolet bands Far UV 1350-1780A and Near UV 1770-2730A. This is the GR2/3 release.
http://galex.stsci.edu/GR2/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexboth
This is a composite of three RASS3 surveys from the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope. Red is soft band (RASS3sb), Green is broad band (RASS3bb), Blue is hard band (RASS3hb)
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosatcolor
Gamma-ray intensity map (photons cm^-2 s-1 sr^-1, >1 GeV) =>1000 MeV
Credit: NASA and FERMI-LAT Team.
https://www.nasa.gov/content/fermi-gamma-ray-space-telescope
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=fermi_lat_8_year
VLSS Cohen, A. S.; Lane, W. M.; Cotton, W. D.; Kassim, N. E.; Lazio, T. J. W.; Perley, R. A.; Condon, J. J.; Erickson, W. C.; Served From NASA Skyview
http://lwa.nrl.navy.mil/VLSS/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=VLA
The FIRST project team: R.J. Becker, D.H. Helfand, R.L. White M.D. Gregg. S.A. Laurent-Muehleisen. 1994, University of California.
http://sundog.stsci.edu/top.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=vlafirst
National Radio Astronomy Observatory. The NVSS project includes J. J. Condon, W. D. Cotton, E. W. Greisen, Q. F. Yin, R. A. Perley (NRAO), and J. J. Broderick (VPI). TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope.
http://www.cv.nrao.edu/nvss/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=vlss
The SUMSS project team and 1997-2000 School of Physics, University of Sydney. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (SUMSS, Min=0.001, Max=10).
http://www.physics.usyd.edu.au/ioa/Main/SUMSS
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=most4sumss
WENSS Team. The WENSS project is a collaboration between the Netherlands Foundation for Research in Astronomy (NFRA/ASTRON) and the Leiden Observatory. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (WENSS, Min=0.001, Max=10), who got it from the WENSS FTP site 1999-03-18. The original data was found using the Westerbork Synthesis Radio Telescope, which is operated by NFRA/ASTRON with support from the Netherlands Foundation for Scientific Research (NWO).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#Westerbork%20Northern%20Sky%20Survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wsrt
Max Planck Institute for Radio Astronomy, generated by Patricia Reich and Wolfgang Reich using with the Bonn Stockert 25m telescope. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (1420MHz, Min=3000, Max=35000).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#Bonn%201420%20MHz%20Survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=1420mhz
Max Planck Institute for Radio Astronomy, generated by Glyn Haslam using data taken at Jodrell Bank, Effelsberg and Parkes telescopes. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (408MHz, Min=10, Max=200).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#HI%20All-Sky%20Continuum%20Survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=1420mhz
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_ilc_200uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_23ghz_k_200uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_23ghz_k_nonlin
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_polmap_k_50uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_33ghz_ka_200uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_33ghz_ka_nonlin
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_polmap_ka_35uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_41ghz_q_200uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_41ghz_q_nonlin
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_polmap_q_35uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_61ghz_v_200uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_61ghz_v_nonlin
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_polmap_v_35uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_94ghz_w_200uk
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_94ghz_w_nonlin
Courtesy WMAP Science Team
http://lambda.gsfc.nasa.gov/product/map/current/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap5yr_polmap_w_35uk
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
Courtesy WMAP Science Team
http://map.gsfc.nasa.gov/m_mm/tm_1.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wmap
http://wwtfiles.blob.core.windows.net/plnk/planck4channel_thumb.jpg
Planck is a European Space Agency mission, with significant participation from NASA. NASAs Planck Project Office is based at JPL. JPL contributed mission-enabling technology for both of Plancks science instruments. European, Canadian and U.S. Planck scientists work together to analyze the Planck data.
http://www.nasa.gov/mission_pages/planck/index.html
http://wwtfiles.blob.core.windows.net/plnk/planckthermaldust_thumb.jpg
http://wwtfiles.blob.core.windows.net/plnk/planckspinningdust_thumb.jpg
http://wwtfiles.blob.core.windows.net/plnk/planckco_thumb.jpg
http://wwtfiles.blob.core.windows.net/plnk/planckfreefree_thumb.jpg
http://wwtfiles.blob.core.windows.net/plnk/plancksynchrotron_thumb.jpg
http://wwtfiles.blob.core.windows.net/plnk/planckmassmap_thumb.jpg
Planck is a European Space Agency mission, with significant participation from NASA. NASAs Planck Project Office is based at JPL. JPL contributed mission-enabling technology for both of Plancks science instruments. European, Canadian and U.S. Planck scientists work together to analyze the Planck data.
http://www.nasa.gov/mission_pages/planck/index.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=planck
This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
http://www.ipac.caltech.edu/2mass/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=2mass
NASA/JPL-Caltech/UCLA
http://wise.ssl.berkeley.edu/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=wise
Data provided by two NASA satellites, the Infrared Astronomy Satellite (IRAS) and the Cosmic Background Explorer (COBE). Processing by David J. Schlegel, Douglas P. Finkbeiner and Marc Davis, Princeton University and University of California, Berkeley.
http://astro.berkeley.edu/~marc/dust/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=dust
Original IRAS data: NASA/JPL IPAC, IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut d'Astrophysique Spatiale. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (Red is IRIS100, Green IRIS60, Blue IRIS12).
http://www.cita.utoronto.ca/~mamd/IRIS/IrisOverview.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=iriscolor
Image Jina Suh from 2MASS catalog Copyright Microsoft 2007; This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
http://www.ipac.caltech.edu/2mass/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=2mass
Original IRAS data: NASA/JPL IPAC, IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut d'Astrophysique Spatiale. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (IRIS12, Min=0.5, Max=1000).
http://www.cita.utoronto.ca/~mamd/IRIS/IrisOverview.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=iris12
Original IRAS data: NASA/JPL IPAC, IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut d'Astrophysique Spatiale. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (IRIS25, Min=1, Max=2000).
http://www.cita.utoronto.ca/~mamd/IRIS/IrisOverview.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=iris25
Original IRAS data: NASA/JPL IPAC, IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut d'Astrophysique Spatiale. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (IRIS60, Min=1, Max=2000).
http://www.cita.utoronto.ca/~mamd/IRIS/IrisOverview.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=iris60
Original IRAS data: NASA/JPL IPAC, IRIS Reprocessing: Canadian Institute for Theoretical Astrophysics/Institut d'Astrophysique Spatiale. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (IRIS100, Min=4, Max=4000).
http://www.cita.utoronto.ca/~mamd/IRIS/IrisOverview.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=iris100
Data provided by two NASA satellites, the Infrared Astronomy Satellite (IRAS) and the Cosmic Background Explorer (COBE). Processing by David J. Schlegel, Douglas P. Finkbeiner and Marc Davis, Princeton University and University of California, Berkeley. TOASTing of images done by NASA's SkyView Virtual Telescope (SFD100m, Min=5, Max=5000).
http://adsabs.harvard.edu/abs/1998ApJ...500..525S
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=sfddust
COBE Team. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (COBE, Min=10, Max=5000).
http://lambda.gsfc.nasa.gov/product/cobe/dirbe_overview.cfm
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=cobe
COBE Team. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (COBEAAM, Min=10, Max=5000).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#Cosmic%20Background%20Explorer%20DIRBE%20Annual%20Average%20Map
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=cobe
COBE Team. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (COBEZSMA, Min=10, Max=5000).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#Cosmic%20Background%20Explorer%20DIRBE%20Zodi-Subtracted%20Mission%20Average
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=cobe
Copyright DSS Consortium. These data are from the DSS2 survey.
http://gsss.stsci.edu/Acknowledgements/DataCopyrights.htm
http://www.worldwidetelescope.org/thumbnails/DSS.png
PanSTARRS / STScI / C. Brasseur
https://panstarrs.stsci.edu/
http://data1.wwtassets.org/packages/2020/06_ps1_3pi/thumb.png
Gaia Data Processing and Analysis Consortium (DPAC); A. Moitinho / A. F. Silva / M. Barros / C. Barata, University of Lisbon, Portugal; H. Savietto, Fork Research, Portugal
https://sci.esa.int/web/gaia/-/60196-gaia-s-sky-in-colour-equirectangular-projection
http://data1.wwtassets.org/packages/2020/09_gaia_dr2/thumb.jpg
Ernie Wright, Laurence Schuler, Ian Jones; NASA/Goddard Space
Flight Center Scientific Visualization Studio; Gaia team/ESA
This set of star maps was created by plotting the position,
brightness, and color of 1.7 billion stars from the Hipparcos-2, Tycho-2,
and Gaia Data Release 2 star catalogs, with help from the Yale Bright Star
Catalog, UCAC3, and the XHIP Hipparcos cross-reference.
http://data1.wwtassets.org/packages/2020/10_dsm2020/thumb.jpg
Image Courtesy Douglas Finkbeiner. 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. The Wisconsin H-Alpha Mapper (WHAM) survey provides a stable zero-point over 3/4 of the sky on a one degree scale.
http://www.astro.princeton.edu/~dfink/halpha/processing.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=halpha
Copyright SDSS
http://www.sdss.org/collaboration/credits.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=sloan
NASA/Goddard Space Flight Center Scientific Visualization Studio
http://svs.gsfc.nasa.gov/vis/a000000/a003400/a003442/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=tychobrahe
Monet D.G., Levine S.E., Casian B., et al. Astron. J., 125, 984 (2003). Rendering by Jina Suh (Microsoft).
http://cdsarc.u-strasbg.fr/viz-bin/Cat?I/284
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=usnob
This is the Near UV band (1770-2730A) of the GALEX GR4 data release archived at MAST/STScI.
TOAST-formatted mosaics were obtained using facilities of NASA's SkyView Virtual Telescope.
http://galex.stsci.edu/GR4/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexnear
This is the Far UV band(1350-1780A) of the GALEX GR4 data release archived at MAST/STScI.
TOAST-formatted mosaics were obtained using facilities of NASA's SkyView Virtual Telescope.
http://galex.stsci.edu/GR4/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexfar
Space Telescope Science Institute. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope. The Galaxy Explorer instrument allows observations to be made in ultraviolet bands Far UV 1350-1780A and Near UV 1770-2730A. This is the GR2/3 release.
http://galex.stsci.edu/GR2/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexboth
Space Telescope Science Institute. The GALEX, Galaxy Explorer, instrument allows imaging and spectroscopic observations to be made in two ultraviolet bands, Far UV 1350-1780A and Near UV 1770-2730A. This is the GR2/3 release, not the most recent GR4 release. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope.
http://galex.stsci.edu/GR2/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexboth
Space Telescope Science Institute. The GALEX, Galaxy Explorer, instrument allows imaging and spectroscopic observations to be made in two ultraviolet bands, Far UV 1350-1780A and Near UV 1770-2730A. This is the GR2/3 release, not the most recent GR4 release. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope.
http://galex.stsci.edu/GR2/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexnear
Space Telescope Science Institute. The GALEX, Galaxy Explorer, instrument allows imaging and spectroscopic observations to be made in two ultraviolet bands, Far UV 1350-1780A and Near UV 1770-2730A. This is the GR2/3 release, not the most recent GR4 release. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope.
http://galex.stsci.edu/GR2/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=galexfar
Data from Center for Extreme UV Astronomy, University of California at Berkeley. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope. Red is 555 Angstroms (euve555), Green 405 Angstroms, Red 83 Angstroms.
http://archive.stsci.edu/euve/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=euve_jbis_map
Center for Extreme UV Astronomy, University of California at Berkeley. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (euve83, Min=1, Max=150).
http://archive.stsci.edu/euve/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=euvebw_jbis_map
Center for Extreme UV Astronomy, University of California at Berkeley. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (euve171, Min=4, Max=200).
http://archive.stsci.edu/euve/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=euvebw_jbis_map
Center for Extreme UV Astronomy, University of California at Berkeley. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (euve405, Min=0.7, Max=70).
http://archive.stsci.edu/euve/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=euvebw_jbis_map
Center for Extreme UV Astronomy, University of California at Berkeley. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (euve555, Min=5, Max=500).
http://archive.stsci.edu/euve/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=euvebw_jbis_map
This is a composite of three RASS3 surveys from the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope. Red is soft band (RASS3sb), Green is broad band (RASS3bb), Blue is hard band (RASS3hb)
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosatcolor
We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (RASS3sb, Min=0.2, Max=50).
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosat
We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (RASS3hb, Min=0.2, Max=50).
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosat
We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (RASS3bb, Min=0.2, Max=50).
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosat
We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (RASSSB, Min=0.0002, Max=10).
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosathard
We have made use of the ROSAT Data Archive of the Max-Planck-Institut fur extraterrestrische Physik (MPE) at Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (RASSHB, Min=0.0002, Max=10).
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosathard
Observational data from NASA Goddard Space Flight Center, mosaicking and TOASTing of images done by NASA's SkyView Virtual Telescope (PSPC2int, Min=0.00002, Max=0.01).
http://skyview.gsfc.nasa.gov/help/pspc_generation.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=rosatpspc2int
NASA BAT Team. TOASTing of images done by NASA's SkyView Virtual Telescope (BATSig, Min=1, Max=10).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#Swift%20BAT%20All-Sky%20Survey:%20Significance%2014-195%20keV
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=batsig
NASA BAT Team. TOASTing of images done by NASA's SkyView Virtual Telescope (BATFlux, Min=1e-5, Max=1e-3).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#Swift%20BAT%20All-Sky%20Survey:%20Flux%2014-195%20keV
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=batflux
Original data: 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; Federation de Recherche Astroparticule et Cosmologie Universite de Paris, France. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (GRANAT_SIGMA_sig, Min=0.5, Max=50).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#GRANAT/SIGMA
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=granatsigmasig
Original data: 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; Federation de Recherche Astroparticule et Cosmologie Universite de Paris, France. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (GRANAT_SIGMA_flux, Min=1e-5, Max=0.01).
http://skyview.gsfc.nasa.gov/cgi-bin/survey.pl#GRANAT/SIGMA%20Flux
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=granatsigmaflux
Gamma-ray intensity map (photons cm^-2 s-1 sr^-1, >1 GeV) =>1000 MeV
Credit: NASA and FERMI-LAT Team.
https://www.nasa.gov/content/fermi-gamma-ray-space-telescope
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=fermi_lat_8_year
NASA and the FERMI-LAT Team. Survey announced 26 AUgust 2008.
http://www.nasa.gov/mission_pages/GLAST/main/index.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=fermilogo
NASA and the FERMI-LAT Team.
http://www.nasa.gov/mission_pages/GLAST/main/index.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=FermiYearTwo
NASA and the FERMI-LAT Team.
http://www.nasa.gov/mission_pages/GLAST/main/index.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=FermiYearThree
CompTel Instrument Team. Maps generated by Andrew Strong, Max-Planck Institute for Extraterrestrial Physics, Garching, Germany. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (comptel, Min=0.00005, Max=0.1).
http://wwwgro.unh.edu/comptel/comptel_main.html
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=comptel
EGRET Instrument team, NASA Goddard Space Flight Center. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (EGRETsoft, Min=0.0001, Max=0.002).
http://cossc.gsfc.nasa.gov/docs/cgro/egret/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=egretmap
EGRET Instrument team, NASA Goddard Space Flight Center. TOAST-formatted data was obtained from NASA's SkyView Virtual Telescope (EGREThard, Min=0.00002, Max=0.005).
http://cossc.gsfc.nasa.gov/docs/cgro/egret/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=egretmap
Andrew Saydjari, etc.
http://data1.wwtassets.org/packages/2022/09_decaps2/thumb.jpg
Andrew Saydjari, etc.
https://faun.rc.fas.harvard.edu/wwt/decaps2/rgb-riY/tiles/thumb.jpg
NASA/JPL-Caltech/Univ. of Wisconsin. The GLIMPSE 360 survey was performed using the Spitzer Space Telescope.
http://www.astro.wisc.edu/sirtf/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=glimpsetn
NASA/JPL-Caltech/Univ. of Wisconsin. The GLIMPSE survey was performed using the Spitzer Space Telescope.
http://www.astro.wisc.edu/sirtf/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=glimpsetn
NASA/JPL-Caltech/Univ. of Wisconsin. The GLIMPSE survey was performed using the Spitzer Space Telescope.
http://www.astro.wisc.edu/sirtf/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=glimpsemipsgaltn
George Djorgovski, IPAC/CalTech. This single continuous digital sky image is a cut through the core of the Virgo Cluster of galaxies, derived from the Palomar-Quest digital sky survey. This image contains nearly a million faint galaxies, about half a million stars in our Milky Way and about a thousand distant quasars.
http://bigpicture.caltech.edu/
http://www.worldwidetelescope.org/wwtweb/thumbnail.aspx?name=dss
Public Domain