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New Great Observatories

About NGO SAG

New Great Observatories

The goals of the New Great Observatories Science Analysis Group (NGO SAG) are to analyze and answer the following questions:

To what degree can the Key Science Questions from Astro2020 be advanced by contemporaneous flight of current, imminent, and future IR/O/UV, X-ray, and FIR Great Observatories? In particular, what discoveries in the Astro2020 Priority Areas might be uniquely made possible by coordinated use of X-ray through FIR space observatories using powerful and varied instruments? What gaps require contemporaneous flight of several or even all of these observatories, and to what degree is asynchronous panchromatic coverage sufficient? How might gaps be closed by the notional future multi-scale multiwavelength mission portfolio, including future explorers and probes?

In the scenario that any or all of these missions not be launched, or should their missions see minimal overlap, what are the corresponding scientific impacts with regards to loss of discovery space or inability of the community to address the priority areas of Astro2020?ity.

NASA's Great Observatories — HST, Spitzer, and Chandra — have produced a matched trio of images of the central region of our Milky Way galaxy. Each image shows the telescope's different wavelength view of the galactic center region, illustrating the unique science each observatory conducts.
NASA / JPL-Caltech / ESA / CXC / STScI

Cross-PAG Science Analysis Group

NGO SAG, PhysPAG, COPAG, and ExoPAG Chairs

NameInstitution
Grant TremblayHarvard CFA
Meredith MacGregorJohns Hopkins University
John O’MearaUniversity of Hawaii, Keck Observatory
Jessie ChristansenCalTech
Amanda Hendrix

How to Participate

We invite participation from the community, particularly from early-career researchers and those from under represented backgrounds in astronomy. Please contact us for more information about our activities and mission, and how you can get involved.

Contact Us about How to Participate
Webb and Hubble�s Views of Spiral Galaxy NGC 628

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.