Zobrazeno 1 - 10
of 51
pro vyhledávání: '"B. J. Geldzahler"'
Autor:
Patrick Charlot, L. D. Zhang, David A. Boboltz, B. J. Geldzahler, G. E. Lanyi, Alan L. Fey, Edward B. Fomalont, O. J. Sovers, Christopher S. Jacobs, C. J. Naudet, Chopo Ma, David Gordon, Jonathan D. Romney
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2010, 139 (5), pp.1713-1770. ⟨10.1088/0004-6256/139/5/1713⟩
The Astrophysical Journal, American Astronomical Society, 2010, 139 (5), pp.1713-1770. ⟨10.1088/0004-6256/139/5/1713⟩
We have measured the sub-milli-arcsecond structure of 274 extragalactic sources at 24 and 43 GHz in order to assess their astrometric suitability for use in a high frequency celestial reference frame (CRF). Ten sessions of observations with the Very
Publikováno v:
The Astrophysical Journal. 592:486-497
Rossi X-Ray Timing Explorer (RXTE) observations of Sco X-1 during 1997-1999 have been analyzed for spectral characteristics. All the X-ray branches of Sco X-1 were observed during these epochs. On the basis of our observations, we present a simple mo
Publikováno v:
Quantum Information and Computation XII.
Establishing a quantum communication network would provide advantages in areas such as security and information processing. Such a network would require the implementation of quantum teleportation between remote parties. However, for photonic "qudits
Publikováno v:
The Astrophysical Journal. 553:L27-L30
The evolution of the radio emission from Sco X-1 is determined from a 56-hour continuous VLBI observation and from shorter observations over a four-year period. The radio source consists of a variable core near the binary, and two variable compact ra
Publikováno v:
The Astrophysical Journal. 512:L121-L124
The results of eight VLBA observations at 5 GHz, spanning 3 yr, have yielded a measured trigonometric parallax for Sco X-1 of 000036±000004; hence, its distance is 2.8±0.3 kpc. This is the most precise parallax measured to date. Although our measur
Publikováno v:
The Astrophysical Journal. 484:L55-L58
From three VLBA observations at 5 GHz, taken over 13 months, we have measured the trigonometric parallax of Sco X-1 as 000023 ± 000028; hence, its distance is greater than 1300 pc. This supports the hypothesis that Sco X-1 radiates at or near the Ed
Publikováno v:
The Astrophysical Journal. 481:489-499
We present the results of the flux density variability observations of Sco X-1 obtained during six VLA observing sessions between 1981 and 1990. The light curves indicate three timescales of flux density variation: slow, intermediate, and rapid. The
Autor:
B. J. Geldzahler
Publikováno v:
SPIE Proceedings.
With the successful completion of a field demonstration of uplink arraying at 8 GHz (X-band) using real-time atmospheric compensation enabled by phase transfer rather than time transfer techniques- completion in mid-Aug 2010, NASA is interested in de
Autor:
B. J. Geldzahler
Publikováno v:
SPIE Proceedings.
For several years, NASA has been pursuing demonstrations and development of coherent uplink arraying techniques for the next generation space communications and planetary radar systems. In addition radio science experiments would benefit with a 1000
Autor:
A. L. Fey, B. J. Geldzahler, David Gordon, P. Charlot, C. Ma, O. J. Sovers, David A. Boboltz, Jonathan D. Romney, L. D. Zhang, C. J. Naudet, G. E. Lanyi, Christopher S. Jacobs, Ed Fomalont
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2010, 139, pp.1695-1712. ⟨10.1088/0004-6256/139/5/1695⟩
The Astronomical Journal, American Astronomical Society, 2010, 139, pp.1695-1712. ⟨10.1088/0004-6256/139/5/1695⟩
International audience; We present astrometric results for compact extragalactic objects observed with the Very Long Baseline Array at radio frequencies of 24 and 43 GHz. Data were obtained from ten 24 hr observing sessions made over a five-year peri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68decfdefd838603be080e0ea08e16a6
https://hal.archives-ouvertes.fr/hal-00466226
https://hal.archives-ouvertes.fr/hal-00466226