... Distribution of simulated 8 µm luminosities. ... for four filters on the SIRTF IRAC instrument: 3.6 µm, 4.5 µm, 5.8 µm, and 8.0 µm. The table look-up method used to generate ...
2. http://www.adass.org/adass/proceedings/adass96/reprints/otts.pdf
... 3 D. Elbaz,3 P. Gallais,1,3 R. Gastaud,3 S. Guest,1,7 G. Helou,8 M. Kong,8 F. Lacomb e,9 J. Li,8 D. Landriu,3 L. Metcalfe,1 K ...
3. Design and Implementation of CIA, the ISOCAM Interactive Analysis System
... Delaney, 1,6 T. Deschamps, 3 F-X. Desert, 2 P. Didelon, 3 D. Elbaz, 3 P. Gallais, 1,3 R. Gastaud, 3 S. Guest, 1,7 G. Helou, 8 M. Kong, 8 F. Lacombe, 9 J. Li, 8 D. Landriu, 3 L. Metcalfe, 1 K. Okumura, 1 M. Perault, 2 A. M. T. Pollock, 1 D. Rouan, 9 J. Sam ...
4. Algorithms for CCD Stellar Photometry
... could be accomplished with a 8-m primary mirror that is diffraction limited at near ... photometry with a 1.5-micron diffraction-limited 8-m Next Generation Space Telescope ...
5. Data Structure and Software of the UCAC-S Project
... survey of the entire southern hemisphere for the 7 - 16 magnitude range, aiming at an accuracy of 20 mas for 8-14 m stars ...
6. Infrared Astronomy and NGST
... The primary mirror is a compact 8 m diameter segmented aperture. ... IR-optimized ground-based 8 m telescopes), and Space Infrared Telescope Facility ... than an optimally operated and equipped 8 m telescope with laser guide stars and ...