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