2 code implementations • 11 Jan 2015 • N. P. M. Kuin, W. Landsman, A. A. Breeveld, M. J. Page, C. James, H. Lamoureux, M. Mehdipour, M. Still, V. Yershov, P. J. Brown, M. Carter, K. O. Mason, T. Kennedy, F. Marshall, P. W. A. Roming, M. Siegel, S. Oates, P. J. Smith, M. De Pasquale
The error in the effective area is from 9% in the UV grism clocked mode to 15% in the visible grism clocked mode .
Instrumentation and Methods for Astrophysics
1 code implementation • 2 Nov 2011 • A. P. Milone, G. Piotto, L. R. Bedin, A. Aparicio, J. Anderson, A. Sarajedini, A. F. Marino, A. Moretti, M. B. Davies, B. Chaboyer, A. Dotter, M. Hempel, A. Marin-Franch, S. Majewski, N. E. Q. Paust, I. N. Reid, A. Rosenberg, M. Siegel
We studied the radial distribution of binary stars, and the distribution of stellar mass ratios.
Solar and Stellar Astrophysics
