CHIANTI

CHIANTI is an ongoing collaboration involving the George Mason University, the University of Michigan (USA), the University of Cambridge (UK) and NASA Goddard Space Flight Center (USA). This collaboration is made possible only with the support of funding agencies in the United States and Europe, and the help of individual scientists outside the CHIANTI consortium.

• The consolidated grants to the atomic astrophysics group (AAG) at DAMTP, University of Cambridge (ST/P000665/1 and ST/T000481/1).
• The NASA Heliophysics Data Environment Enhancements program.

• NASA - Ultraviolet, Visible and Gravitational Astrophysics grant (USA)
• NASA - Applied Information Systems Research Program grant (USA)
• NASA - Living With a Star grant (USA)
• NASA - Solar and Heliospheric Physics CHIANTI grant (USA)
• Chandra Emission Line Project (USA)
• NATO grant
• Agenzia Spaziale Italiana (ASI, Italy)
• Ministero dell'Istruzione dell'Universita' e della Ricerca (MIUR, Italy)
• Particle Physics and Astronomy Research Council (PPARC, UK)
• STFC, UK

We are grateful to the individual scientists who made available to us the electronic files of their calculations. These include:

N. Badnell, M. O’Mullane (University of Strathclyde, UK)

M. Bautista (Western Michigan University, USA)

A.K. Bhatia (GSFC, USA)

J. Dubau (Univ. Paris)

M.F. Gu (Stanford, USA)

T. Kato (TU)

G. Liang (Chinese Academy of Sciences)

J. Pelan, C.A. Ramsbottom, K. Bell, C. Ballance (QUB, UK)

U.I. Safronova (IS/RAS)

D.H. Sampson (PSU)

P.J. Storey (UCL, UK)

S.S. Tayal (Clark Atlanta University, USA)

K.G. Widing (NRL, USA)

W.L. Wiese, W.C. Martin, A. Musgrove and T. Shirai (NIST)

M.C. Witthoeft (CUA/GSFC, USA)

O. Zatsarinny (Drake University, USA)

H.L. Zhang and A.K. Pradhan (OSU, USA)