Search Results - "KRUK, Jeffrey W"

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    The Impact of Interpixel Capacitance in CMOS Detectors on PSF Shapes and Implications for WFIRST by Kannawadi, Arun, Shapiro, Charles A., Mandelbaum, Rachel, Hirata, Christopher M., Kruk, Jeffrey W., Rhodes, Jason D.

    “…Unlike optical CCDs, near-infrared detectors, which are based on CMOS hybrid readout technology, typically suffer from electrical crosstalk between the pixels…”
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    Journal Article
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    Radiation-induced Backgrounds in Astronomical Instruments: Considerations for Geosynchronous Orbit and Implications for the Design of the WFIRST Wide-field Instrument by Kruk, Jeffrey W., Xapsos, Michael A., Armani, Nerses, Stauffer, Craig, Hirata, Christopher M.

    “…Geosynchronous orbits are appealing for solar or astrophysical observatories because they permit continuous data downlink at high rates. The radiation…”
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    Journal Article
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    The Hopkins Ultraviolet Telescope: The Final Archive by Dixon, William V., Blair, William P., Kruk, Jeffrey W., Romelfanger, Mary L.

    “…ABSTRACT The Hopkins Ultraviolet Telescope (HUT) was a 0.9 m telescope and moderate-resolution (Δλ = 3 Å) far-ultraviolet (820-1850 Å) spectrograph that flew…”
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    Breakthrough capability for UVOIR space astronomy: Reaching the darkest sky by Greenhouse, Matthew A., Benson, Scott W., Englander, Jacob, Falck, Robert D., Fixsen, Dale J., Gardner, Jonathan P., Kruk, Jeffrey W., Oleson, Steven R., Thronson, Harley A.

    Published in Advances in space research (15-02-2015)
    “…We describe how availability of new solar electric propulsion (SEP) technology can substantially increase the science capability of space astronomy missions…”
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    Interstellar Deuterium, Nitrogen, and Oxygen Abundances toward GD 246, WD 2331–475, HZ 21, and Lanning 23: Results from the FUSE Mission by Oliveira, Cristina M, Hébrard, Guillaume, Howk, J. Christopher, Kruk, Jeffrey W, Chayer, Pierre, Moos, H. Warren

    Published in The Astrophysical journal (10-04-2003)
    “…The interstellar abundances of D I, N I, and O I in the local ISM are studied using high-resolution spectra of four hot white dwarfs. The spectra of GD 246, WD…”
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    High-resolution FUV spectroscopy of the terrestrial day airglow with the Far Ultraviolet Spectroscopic Explorer by Feldman, Paul D., Sahnow, David J., Kruk, Jeffrey W., Murphy, Edward M., Moos, H. Warren

    Published in Journal of Geophysical Research (01-05-2001)
    “…During orbital verification the Far Ultraviolet Spectroscopic Explorer obtained spectra of the terrestrial day airglow between 905 and 1184 Å from an altitude…”
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    Variations in D/H and D/O from New Far Ultraviolet Spectroscopic Explorer Observations by Oliveira, Cristina M, Moos, H. Warren, Chayer, Pierre, Kruk, Jeffrey W

    Published in The Astrophysical journal (01-05-2006)
    “…We use data obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) to determine the interstellar abundances of D I, N I, O I, Fe II, and H sub(2)…”
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    Evidence for Deuterium Astration in the Planetary Nebula Sh 2-216? by Oliveira, Cristina M, Chayer, Pierre, Moos, H. Warren, Kruk, Jeffrey W, Rauch, Thomas

    Published in The Astrophysical journal (20-05-2007)
    “…We present FUSE observations of the line of sight to WD 0439+466 (LSV +4621), the central star of the old planetary nebula Sh 2-216. The FUSE data show…”
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    The Impact of Interpixel Capacitance in CMOS Detectors on PSF Shapes and Implications for WFIRST by Kannawadi, Arun, Shapiro, Charles A., Mandelbaum, Rachel, Hirata, Christopher M., Kruk, Jeffrey W., Rhodes, Jason D.

    “…Unlike optical CCDs, near-infrared detectors, which are based on CMOS hybrid readout technology, typically suffer from electrical crosstalk between the pixels…”
    Get full text
    Journal Article
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    Radiation-induced Backgrounds in Astronomical Instruments: Considerations for Geosynchronous Orbit and Implications for the Design of the WFIRST Wide-field Instrument by Kruk, Jeffrey W., Xapsos, Michael A., Armani, Nerses, Stauffer, Craig, Hirata, Christopher M.

    “…Geosynchronous orbits are appealing for solar or astrophysical observatories because they permit continuous data downlink at high rates. The radiation…”
    Get full text
    Journal Article
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