Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Richard L. Bybee"'
Autor:
S. Franka, J. B. Hutchings, Edward B. Jenkins, Chuck Bowers, D. Rose, Richard F. Green, Alan W. Delamere, M. Bottema, D. Hood, W. Meyer, Sara R. Heap, Morley M. Blouke, Charles L. Joseph, George F. Hartig, Fred L. Roesler, Lee Feinberg, Randy A. Kimble, Jeffrey L. Linsky, J. J. Loiacono, J. F. Grady, Albert Boggess, J. C. Hetlinger, David A. Dorn, H. Garner, Steven B. Kraemer, David Michika, Vic S. Argabright, C. Ludtke, B. E. Woodgate, Mark D. Brumfield, Theodore R. Gull, H. W. Moos, Anthony C. Danks, J. G. Timothy, C. VanHouten, Mary Elizabeth Kaiser, Donna Weistrop, R. Stocker, Robert A. Woodruff, D. J. Lindler, Stephen P. Maran, I. Becker, Richard L. Bybee, Joe H. Sullivan
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:1183-1204
The Space Telescope Imaging Spectrograph (STIS) instrument was installed on the Hubble Space Telescope (HST) during the second servicing mission, in 1997 February. Four bands cover the wavelength range of 115–1000 nm, with spectral resolving powers
Publikováno v:
Review of Scientific Instruments. 69:1898-1905
We conducted a study to estimate the impact that thermal variations and electronic drifts would have on the photometric stability of the multianode microchannel array (MAMA) detectors that are currently flying aboard the space telescope imaging spect
Autor:
Dennis Ebbets, Mark D. Brumfield, R. Breyer, Stefi A. Baum, Mary Elizabeth Kaiser, P. R. Christon, S. I. Becker, Chuck Bowers, Randy A. Kimble, Sara R. Heap, R. J. Hill, Richard F. Green, Alan W. Delamere, L. W. Brown, S. Downey, Melissa A. McGrath, J. F. Grady, Richard D. Robinson, J. J. Yagelowich, D. Rose, A. Grusczak, David A. Dorn, C. Standley, A. Boggess, Vic S. Argabright, J. C. Blades, Anthony C. Danks, C. Ludtke, Stephen P. Maran, P. A. Driggers, Theodore R. Gull, J. G. Timothy, W. B. Fowler, W. Meyer, Mark Clampin, V. L. Krueger, M. N. Isaacs, J. A. Valenti, Wayne B. Landsman, George F. Hartig, J. J. Loiacono, Ralph C. Bohlin, Richard L. Bybee, R. Stocker, Fred L. Roesler, H. W. Moos, D. Hood, R. L. Lettieri, Eliot M. Malumuth, V. Balzano, C. Biagetti, Steven B. Kraemer, Henry C. Ferguson, David Michika, Robert S. Hill, R. Nyquist, Paul Goudfrooij, J. C. Hetlinger, M. Bottema, T. Wolfe, T. L. Beck, R. W. Melcher, Robert A. Woodruff, D. J. Lindler, Morley M. Blouke, Jennifer L. Sandoval, Lee Feinberg, F. J. Rebar, Charles L. Joseph, Nicholas R. Collins, C. N. Van Houten, J. F. Sullivan, J. K. Feggans, J. S. Gallegos, Carolyn A. Krebs, R. Doxsey, D. Weistrop, Stephen J. Hulbert, P. Plait, Bruce E. Woodgate, R. Kutina, R. H. Cornett, Jeffrey L. Linsky, R. Reed, H. Garner, H. D. Vitagliano, J. B. Hutchings, Edward B. Jenkins
Publikováno v:
The Astrophysical Journal. 492:L83-L93
The Space Telescope Imaging Spectrograph (STIS) was successfully installed into the Hubble Space Telescope (HST) in 1997 February, during the second HST servicing mission, STS-82. STIS is a versatile spectrograph, covering the 115-1000 nm wavelength
Autor:
Max Styonavich, Bruce E. Woodgate, Charles N. Van Houten, James Abraham, Ronald L. Gilliland, Steven Franka, Chris A. Long, Vic S. Argabright, Don J. Lindler, Ralph C. Bohlin, H. Edward Culver, Mary Elizabeth Kaiser, Charles L. Joseph, J. Gethyn Timothy, Richard L. Bybee, Randy A. Kimble, Richard A. Shaw, Anthony C. Danks
Publikováno v:
SPIE Proceedings.
The Space Telescope Imaging Spectrograph (STIS) is a versatile HST instrument covering the 115 - 1000 nm wavelength range in a variety of spectroscopic and imaging modes. Coverage of the ultraviolet range (115 - 310 nm) is provided by two Multi- Anod
Autor:
Randy A. Kimble, Richard L. Bybee, Charles L. Joseph, Vic S. Argabright, Bruce E. Woodgate, George A. Lorman, Anthony C. Danks, Charles N. Van Houten, James Abraham, Peter Frank, Steven Franka
Publikováno v:
Space Telescopes and Instruments V.
Two multi-anode microchannel array (MAMA) detectors were fabricated at Ball Aerospace Technology Corporation for the Space Telescope Imaging Spectrograph (STIS) which was installed into the Hubble Space Telescope in February 1997. The photometric sta
Autor:
Mary Elizabeth Kaiser, Bruce E. Woodgate, Randy A. Kimble, Charles W. Bowers, Steven B. Kraemer, Vic S. Argabright, Phillip A. Driggers, Don J. Lindler, Ralph C. Bohlin, Charles N. Van Houten, Richard L. Bybee, Alan W. Delamere, David A. Dorn, Anthony C. Danks, Charles L. Joseph, J. Gethyn Timothy, Theodore R. Gull, Terrence L. Beck, Morley M. Blouke, Lawrence W. Brown, Mark D. Brumfield, Mark Clampin, David A. Content, Lee D. Feinberg, Walter B. Fowler, Paul Goudfrooij, Robert J. Hill, Richard Reed, Clive Standley, J. J. Yagelowich
Publikováno v:
Space Telescopes and Instruments V.
The space telescope imaging spectrograph (STIS) was designed as a versatile spectrograph capable of maintaining or exceeding the spectroscopic capabilities of both the Goddard High Resolution Spectrograph and the Faint Object Spectrograph (FOS) over
Autor:
David Michika, Charles W. Bowers, G. A. Bower, M. Bottema, J. F. Grady, Stephen P. Maran, Fred L. Roesler, Albert Boggess, D. Hood, W. Meyer, S. R. Heap, Harry W. Garner, Bruce E. Woodgate, Joseph F. Sullivan, Mary Elizabeth Kaiser, Lee Feinberg, Don J. Lindler, H. W. Moos, Charles L. Joseph, Richard L. Bybee, Alan W. Delamere, Randy A. Kimble, Richard F. Green, Donna Weistrop, Charles N. Van Houten, George Sonneborn, J. C. Hetlinger, Morley M. Blouke, David A. Dorn, J. Gethyn Timothy, Vic S. Argabright, Theodore R. Gull, J. B. Hutchings, Robert A. Woodruff, Mark D. Brumfield, Edward B. Jenkins, Anthony C. Danks, Ralph B. Stocker, Jonathan P. Gardner, J. J. Loiacono, Steven B. Kraemer, D. V. Rose, J. B. Linsky
Publikováno v:
SPIE Proceedings.
The STIS instrument was installed into HST in February 1997 during the Servicing Mission 2. It has almost completed checkout and is beginning its science program, and is working well. Several scientific demonstration observations were taken to illust
Publikováno v:
SPIE Proceedings.
The space telescope imaging spectrograph (STIS), a next-generation instrument for the Hubble Space Telescope, has fabricated several engineering model units (EMUs) of the multi-anode microchannel array (MAMA) detectors. Good tube yields have been rea
Publikováno v:
SPIE Proceedings.
The multianode microchannel array (MAMA) has been chosen as the detector for two instruments on the ESA/NASA Solar Heliospheric Observatory. The response of the MAMA to the two extreme types of solar spectra, disk and corona, have been modeled with a
Publikováno v:
IEEE Transactions on Nuclear Science. 28:689-697
The Multi-Anode Microchannel Arrays (MAMA's) are a family of photoelectric photon-counting array detectors being developed for use in instruments on both ground-based and space-borne telescopes. These detectors combine high sensitivity and photometri