Spitzer Chandra

NASA’s Great Observatories “an astronomical Mount Rushmore”

Compton Hubble !"#$%&$'()*&+&,#$-+$(.'/01$

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Past

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2008 FGS COS NICMOS STIS ACS WFC3

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And at other wavelengths… Chandra X-ray Observatory

Chandra and its complement XMM-Newton @"0$6'4'/

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Direct detection of IR from two “hot Jupiters” during eclipses, two wavelengths give temperature estimates

Across the spectrum - now

FarIR MidIR nearIR opt UV farUV X-ray gamma

GALEX INTEGRAL

COROT GLAST Spitzer

WMAP XMM-Newton

Hubble Swift

Akari Chandra c54<(.0/)*'4$G*0')0()$?-)($

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ROSAT GALEX Kitt Peak Spitzer VLA J$+07$N+-80*(0$)&$0B.4&*0$

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•! Z>Ju($vccP207)&+$ •! GJOZvR$JE'*-R$>7-m$ •! F*'/Mf9J$ •! J4,&()$&+$)"0$.'%]$Z>Ju($?0*(/"04$ •! J+%$&A$/&5*(0$r$2J>J:Z>J$j!>@$ •! M+$)"0$6*&5+%$'+%$,0'+)$)&$()'#$)"0*0]$ JOcJR$Gc@R$O>c@R$ZO@R$M!OL$ GALEX (Galaxy Evolution Explorer)

Ultraviolet imaging and spectroscopic survey of the sky – the first to be so deep and wide.

GALEX+SDSS and bimodal galaxy properties Akari ( JAXA’s TSFKA Astro-F)

Swift – catching gamma-ray bursts on the fly! X-ray UV/Optical

SN 2007uy

SN 2008D

X-ray supernova flash in NGC2770 SOFIA – Stratospheric Observatory for Infrared Astronomy - NASA/DLR

International Gamma-Ray Laboratory (INTEGRAL) It really is international:

ESA mission Russian launch NASA communication

Al-26 mass: 2.8 solar masses

Massive SN rate: 1.9/ century ESA Herschel Space Telescope 3.5m Far-IR optimized Ariane 5 launch (w/Planck) 2009 L2 halo orbit 3 instruments 3 years’ cryogens 60-670 µm range Gamma-Ray Large Area Space Telescope (GLAST) Fermi GLAST burst monitors at MSFC right before shipping to Phoenix for integration

(Richard Dubois) Across the spectrum - soon

FarIR MidIR nearIR opt UV farUV X-ray gamma

GALEX INTEGRAL JWST

GLAST Kepler

XMM-Newton Herschel Planck

Hubble Swift

WSO/Spektr-UV

Chandra SIM/TPF?