... should not be much worse then 0.7'' FWHM and the variation of the seeing for each galaxy data set should not exceed 0.15 ... Maoz, D. et al. 1995, ApJ, 440, 91 . Rees, M. 1990, Science, 247, 817 . Renzini, A. et al. 1995, Nature, 378, 39 . ...
... Dolensky, M., Micol, A., & Pirenne, B., ``Browsing the HST archive with Java enriched Database Access'', this volume Dolensky, M., Micol, A., & Pirenne, B., Rosa, M., ``Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at STECF ...
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... table shows strongly related groups (about 15 groups appear on the diagonal ... having papers co-authored with M. Perryman (Hipparcos project scientist) and L ... Dousset, B., Rommens, M., & Sibue, D. 1995, Symposium International, Omega-3 ...
... absorption and emission, NICMOS covers the entire 0.8 m to 2.5 m wavelength range ... spectrophotometric standards covering the entire 0.8 m - 2.5 m wavelength range ... at 2.2 m - 2.5 m could be orders of magnitude larger than at 1.0 m and therefore ...
... Kessler,M.F. et al. 1996, A&A 15 The Infrared Space Observatory (ISO) mission . ... 1996, A&A 15 The Infrared Space Observatory (ISO) mission . Lahuis, F. 1997, ``ISO SWS Data Analysis", this volume . ...
... Hellerstein. J. M., Naughton, J. F., & Pfeffer, A. 1995, Proc. Int. Conf. on VLDBs, 562 . ... Pirenne, B., & Ochsenbein, F. 1991, ST-ECF Newsletter, 15, 17 . ...