Architecture design study and technology road map for the Planet Formation Imager (PFI)

Author:

Monnier John D.1,Ireland Michael J.2,Kraus Stefan3,Baron Fabien4,Creech-Eakman Michelle5,Dong Ruobing6,Isella Andrea7,Merand Antoine8,Michael Ernest9,Minardi Stefano10,Mozurkewich David11,Petrov Romain12,Rinehart Stephen13,ten Brummelaar Theo4,Vasisht Gautam14,Wishnow Ed6,Young John15,Zhu Zhaohuan16

Affiliation:

1. Univ. of Michigan (United States)

2. Australian National Univ. (Australia)

3. Univ. of Exeter (United Kingdom)

4. Georgia State Univ. (United States)

5. New Mexico Institute of Mining and Technology (United States)

6. Univ. of California, Berkeley (United States)

7. Rice Univ. (United States)

8. European Southern Observatory (Chile)

9. Univ. of Chile (Chile)

10. Univ. of Jena (Germany)

11. Seabrook Engineering (United States)

12. Univ. of Nice (France)

13. NASA Goddard Space Flight Ctr. (United States)

14. Jet Propulsion Lab. (United States)

15. Univ. of Cambridge (United Kingdom)

16. Princeton Univ. (United States)

Publisher

SPIE

Reference14 articles.

1. Planet formation imager (PFI): introduction and technical considerations;Monnier,July 2014

2. The science case for the Planet Formation Imager (PFI);Kraus,July 2014

3. A dispersed heterodyne design for the planet formation imager;Ireland,July 2014

4. TRANSITIONAL AND PRE-TRANSITIONAL DISKS: GAP OPENING BY MULTIPLE PLANETS?

5. Orbital stability zones about asteroids

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