... Previous all-sky surveys at these wavelengths, notably those made with EGRET and other instruments on board of the Compton Gamma Ray Observatory (CGRO), could not determine source positions to better than 1 degree (slightly less for higher energies). ...
2. Arecibo Observatory Publications
... M.P., Matz, S.M., Schroeder, P.C., Patt, B.L., Arzoumanian, Z., Cordes, J.M. and Strickman, S., CGRO-OSSE Observations of Isolated Pulsars , in Proceedings of IAU Colloquium 160, "Pulsars: Problems and Progress", S. Johnston, M. Bailes, and M. Walker, eds ...
3. NAIC-NRAO Single Dish Summer School NAIC-NRAO Single Dish Summer School 2005
... These include the 21-cm line (LDS), diffuse IR emission (IRAS, DIRBE), H alpha line (WHAM + others), short-wavelength radio maps (WMAP), X-rays (ROSAT), cm-wave radio maps (various), gamma ray (CGRO). ...
4. Arecibo Observatory Publications
... McLaughlin, M.A., J.R. Mattox, J.M. Cordes, and D.J. Thompson, Variability of CGRO/EGRET Gamma Ray Sources , Astrophys. J., 473, 763, 1996. ...
5. http://www.naic.edu/~tghosh/a1724/402
... The past 15 years have seen a growth of space-based solar physics investigations (e.g. SMM, CGRO, Yokoh, WIND, Ulysses, SOHO, ACE, TRACE, RHESSI). ...