Search Results - "PRAVDO, S"

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    Early optical emission from the γ-ray burst of 4 October 2002 by Fox, D. W, Yost, S, Kulkarni, S. R, Torii, K, Kato, T, Yamaoka, H, Sako, M, Harrison, F. A, Sari, R, Price, P. A, Berger, E, Soderberg, A. M, Djorgovski, S. G, Barth, A. J, Pravdo, S. H, Frail, D. A, Gal-Yam, A, Lipkin, Y, Mauch, T, Harrison, C, Buttery, H

    Published in Nature (London) (20-03-2003)
    “…Observations of the long-lived emission-or 'afterglow'-of long-duration γ-ray bursts place them at cosmological distances, but the origin of these energetic…”
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    Direct Detection of the Brown Dwarf GJ 802B with Adaptive Optics Masking Interferometry by Lloyd, James P, Martinache, Frantz, Ireland, Michael J, Monnier, John D, Pravdo, Steven H, Shaklan, Stuart B, Tuthill, Peter G

    Published in The Astrophysical journal (20-10-2006)
    “…We have used the Palomar 200" adaptive optics (AO) system to directly detect the astrometric brown dwarf GJ 802B reported by Pravdo et al. This observation is…”
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    Discovery of X-rays from the protostellar outflow object HH2 by Pravdo, Steven H, Feigelson, Eric D, Garmire, Gordon, Maeda, Yoshitomo, Tsuboi, Yohko, Bally, John

    Published in Nature (London) (18-10-2001)
    “…Herbig-Haro (HH) objects have been known for 50 years to be luminous condensations of gas in star-forming regions, but their underlying physical nature is…”
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    Astrometric Discovery of GJ 802b: In the Brown Dwarf Oasis? by Pravdo, Steven H, Shaklan, Stuart B, Lloyd, James

    Published in The Astrophysical journal (01-09-2005)
    “…The Stellar Planet Survey is an ongoing astrometric search for giant planets and brown dwarfs around a sample of 630 M dwarfs. We have discovered several…”
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    Astrometric Discovery of GJ 164B by Pravdo, Steven H, Shaklan, Stuart B, Henry, Todd, Benedict, G. Fritz

    Published in The Astrophysical journal (20-12-2004)
    “…We discovered a low-mass companion to the M dwarf GJ 164 with the CCD-based imaging system of the Stellar Planet Survey astrometric program. The existence of…”
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    Masses of Astrometrically Discovered and Imaged Binaries: G78-28ABand GJ 231.1BC by Pravdo, SH, Shaklan, S B, Wiktorowicz, S J, Kulkarni, S, Lloyd, J P, Martinache, F, Tuthill, P G, Ireland, MJ

    Published in The Astrophysical journal (20-09-2006)
    “…The Stellar Planet Survey (STEPS) is an ongoing astrometric search for giant planets and brown dwarfs around a sample of 630 M dwarfs. We have discovered…”
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    X-rays from the Power Sources of the Cepheus A Star-Forming Region by Pravdo, S. H, Tsuboi, Y, Uzawa, A, Ezoe, Y

    Published 02-09-2009
    “…Astrophys.J.704:1495-1505,2009 We report an observation of X-ray emission from the exciting region of Cepheus A with the Chandra/ACIS instrument. What had been…”
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    Modelling of a space-based Ronchi ruling experiment for high-precision astrometry by Shaklan, S., Pravdo, S., Gatewood, G., Ftaclas, C.

    Published in Astrophysics and space science (01-02-1994)
    “…An end-to-end modelling program for an astrometric telescope employing a Ronchi ruling has been developed. The program models the aberrated images formed…”
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    A reduced estimate of the number of kilometre-sized near-Earth asteroids by Rabinowitz, David, Helin, Eleanor, Lawrence, Kenneth, Pravdo, Steven

    Published in Nature (London) (13-01-2000)
    “…Near-Earth asteroids are small (diameters < 10 km), rocky bodies with orbits that approach that of the Earth (they come within 1.3 AU of the Sun). Most have a…”
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    Galactic distribution of X-ray burst sources by LEWIN, W. H. G, HOFFMAN, J. A, DOTY, J, CLARK, G. W, SWANK, J. H, BECKER, R. H, PRAVDO, S. H, SERLEMITSOS, P. J

    Published in Nature (London) (05-05-1977)
    “…Data on X-ray bursts recorded by the OSO-8 and SAS-3 satellites and criteria (rise time, duration, recurrence) for X-ray bursts are examined in a study of…”
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    Evidence for a 17-d periodicity from Cyg X-3 by HOLT, S. S, BOLDT, E. A, SERLEMITSOS, P. J, KALUZIENSKI, L. J, PRAVDO, S. H, PEACOCK, A, ELVIS, M, WATSON, M. G, POUNDS, K. A

    Published in Nature (London) (15-04-1976)
    “…Data are presented from the Ariel-V All-Sky Monitor which indicate a 17-day periodicity of the X-ray spectra from Cyg X-3 (3U2030+40). The data are consistent…”
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    The identification of H2311 + 77 with HD220140, a probable RS CVn star by Pravdo, S. H., White, N. E., Giommi, P.

    “…H2311 + 77, one of the bright soft X-ray sources in the sky originally detected with HEAO 1, has been identified in an Exosat imaging observation with a…”
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