Zobrazeno 1 - 10
of 972
pro vyhledávání: '"Flanagan, C."'
We report the results of a sensitive search for water maser emission in the Local Group Galaxy NGC 6822 with the Karl G. Jansky Very Large Array. The observations provide tentative single-epoch detections of four candidates, associated with two infra
Externí odkaz:
http://arxiv.org/abs/2205.00545
Publikováno v:
Journal of Intelligent Systems, Vol 2, Iss 1-4, Pp 187-224 (1992)
Externí odkaz:
https://doaj.org/article/4cf03bbbadd947c4b1af94d7a87d259a
Autor:
Bosak, J., Messersmith, L., Bryer, C., Drainoni, M., Goodman, D., Adams, M., Barry, T., Flanagan, C., Flanagan, V., Wolff, K., Declercq, E.
Publikováno v:
In Journal of Substance Use and Addiction Treatment February 2024 157
Autor:
PATRICK FLANAGAN, C. M.1
Publikováno v:
Catholic Theological Society of America Proceedings. 2023, Vol. 77, p225-229. 5p.
Autor:
Gwinn, C. R., Johnson, M. D., Reynolds, J. E., Jauncey, D. L., Tzioumis, A. K., Dougherty, S., Carlson, B., Del Rizzo, D., Hirabayashi, H., Kobayashi, H., Murata, Y., Edwards, P. G., Quick, J. F. H., Flanagan, C. S., McCulloch, P. M.
Publikováno v:
Astrophysical Journal (2012) 758, 6
We compare the noise in interferometric measurements of the Vela pulsar from ground- and space-based antennas with theoretical predictions. The noise depends on both the flux density and the interferometric phase of the source. Because the Vela pulsa
Externí odkaz:
http://arxiv.org/abs/1208.0039
Autor:
Gwinn, C. R., Johnson, M. D., Reynolds, J. E., Jauncey, D. L., Tzioumis, A. K., Hirabayashi, H., Kobayashi, H., Murata, Y., Edwards, P. G., Dougherty, S., Carlson, B., del Rizzo, D., Quick, J. F. H., Flanagan, C. S., McCulloch, P. M.
Publikováno v:
Astrophysical Journal (2012), 758, 7
We present measurements of the linear diameter of the emission region of the Vela pulsar at observing wavelength lambda=18 cm. We infer the diameter as a function of pulse phase from the distribution of visibility on the Mopra-Tidbinbilla baseline. A
Externí odkaz:
http://arxiv.org/abs/1208.0040
Autor:
Seward, F. D., Alpar, M. A., Flanagan, C., Kiziloglu, U., Markwardt, C., McCulloch, P., Ogelman, H.
The ROSAT HRI was used to monitor X-ray emission from the Vela Pulsar. Six observations span 2-1/2 years and 3 glitches. The summed data yield a determination of the pulse shape, and X-ray emission from the pulsar is found to be 12 % pulsed with one
Externí odkaz:
http://arxiv.org/abs/astro-ph/0004015
Autor:
Gwinn, C. R., Britton, M. C., Reynolds, J. E., Jauncey, D. L., King, E. A., McCulloch, P. M., Lovell, J. E. J., Flanagan, C. S., Preston, R. A.
We present measurements of the size of the Vela pulsar in 3 gates across the pulse, from observations of the distribution of intensity. We calculate the effects on this distribution of noise in the observing system, and measure and remove it using ob
Externí odkaz:
http://arxiv.org/abs/astro-ph/9908254
Autor:
Gwinn, C. R., Ojeda, M. J., Britton, M. C., Reynolds, J. E., Jauncey, D. L., King, E. A., McCulloch, P. M., Lovell, J. E. J., Flanagan, C. S., Smits, D. P., Preston, R. A., Jones, D. L.
We use interstellar scattering of the Vela pulsar to determine the size of its emission region. From interferometric phase variations on short baselines, we find that radio-wave scattering broadens the source by 3.4+/-0.3 milliarcseconds along the ma
Externí odkaz:
http://arxiv.org/abs/astro-ph/9608088
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