LOGIN TO YOUR ACCOUNT

Username
Password
Remember Me
Or use your Academic/Social account:

CREATE AN ACCOUNT

Or use your Academic/Social account:

Congratulations!

You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.

Important!

Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message

CREATE AN ACCOUNT

Name:
Username:
Password:
Verify Password:
E-mail:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:
fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Dodson, R.; Hirabayashi, H.; Murata, Y.; Edwards, P. G.; Wiik, K.; Murphy, D.; Kameno, S. (2004)
Languages: English
Types: Preprint
Subjects: Astrophysics
Given the scientific goals of VSOP-2, including the possibility of observations of the shadows of black holes, we have investigated the fidelity of the recovered images given a typical uv-coverage. We find that we can achieve a dynamic range of better than 1000:1.
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • 1 Falcke H., Melia F., Agol E. 2000, ApJ 528, L13 2 Hirabayashi, H., 2003, New Technologies in VLBI ed Minh, CS-306 3 Manmoto, Mineshige, Kusunose, 1997, ApJ, 554, 964 4 Phillips, R. et al 1996, AJ, 111, 918 5 Takahashi et al 2004, in prep.
    • 6 Zavala, R Taylor, G., 2003, NewAR, 47, 589
  • No related research data.
  • No similar publications.

Share - Bookmark

Cite this article

Collected from