Skip to main content Accessibility help

We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.

Close cookie message
×
Home
  • Home
EnglishFrançais
Symposium - International Astronomical Union Symposium - International Astronomical Union

Article contents

The Conversion from the B1950 FK4-Based Position to the J2000 Position of Celestial Objects

Published online by Cambridge University Press:  04 August 2017

S. Aoki ,
M. Sôma ,
K. Nakajima ,
Y. Niimi ,
M. Fujishita  and
Y. Takahashi
S. Aoki
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
M. Sôma
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
K. Nakajima
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
Y. Niimi
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
M. Fujishita
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
Y. Takahashi
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
Save pdf (1 mb)

Extract

We present here the fundamental idea of the conversion method between old and new reference frameworks. Some practical applications are made for the optical observations for Tokyo PZT. The method can be also applied to the conversion of radio sources where we have met a great difficulty in performing the conversion because of no citation of observation epochs in general. We discuss their necessity in order to establish a concrete compilation of the position of the radio sources.

Type
I. Reduction Technique
Information
Symposium - International Astronomical Union , Volume 109: Astrometric Techniques , 1986 , pp. 123 - 131
Copyright
Copyright © Reidel 1986 

References

Aoki, S., Guinot, B., Kaplan, G.H., Kinoshita, H., McCarthy, D.D. and Seidelmann, P.K.: 1982, Astron. Astrophys. 105, 359.Google Scholar
Aoki, S. and Kinoshita, H.: 1983, Celest. Mech. 29, 335.CrossRefGoogle Scholar
Aoki, S., Sôma, M., Kinoshita, H. and Inoue, K.: 1983, Astron. Astrophys. 128, 263.Google Scholar
Clark, T.A., Hutton, L.K., Marandino, G.E., Counselman, C.C., Robertson, D.S., Shapiro, I.I., Wittels, J.J., Hinteregger, H.F., Knight, C.A., Rogers, A.E.E., Whitney, A.R., Niell, A.E., Rönnäng, B.O. and Rydbeck, O.E.H.: 1976, Astron. J. 81, 599.CrossRefGoogle Scholar
de Vegt, C. and Gehlich, U.K.: 1981, Astron. Astrophys. 101, 191.Google Scholar
de Vegt, C. and Gehlich, U.K.: 1982, Astron. Astrophys. 113, 213.Google Scholar
Elsmore, B.: 1979, in Modern Astrometry, eds. Prochaska, F.V. and Tucker, R.H., Univ. Obs. Vienna, p.93.Google Scholar
Fanselow, J.L., Sovers, O.J., Thomas, J.B., Bletzacker, F.R., Kearns, T.J., Cohen, E.J., Purcell, G.H., Rogstad, D.H., Skjerve, L.J. and Young, L.E.: 1981, in Reference Coordinate System for Earth Dynamics, eds. Gaposhkin, E.M. and Kołaszek, B.K., Reidel, Dordrecht, p.351 (JPL 1980-1).CrossRefGoogle Scholar
Fanselow, J.L., Sovers, O.J., Thomas, J.B., and Purcell, G.H. Jr.: 1983, in Very Long Baseline Interferometry Techniques, p.183.Google Scholar
Fricke, W.: 1977, Veröff. Astronomischen Rechen-Instituts, Nr.25.Google Scholar
Fricke, W.: 1981, in Reference Coordinate System for Earth Dynamics, eds. Gaposhkin, E.M. and Kołaszek, B.K., Reidel, Dordrecht, p.331.CrossRefGoogle Scholar
Fricke, W.: 1982, Astron. Astrophys. 107, L13.Google Scholar
Fricke, W. and Kopff, A.: 1963, Veröff. Astronomischen Rechen Instituts, Nr.10.Google Scholar
Harrington, R.S. Douglass, G.G., Kallarakal, V.V., Smith, C.A. and Guetter, H.H.: 1983, Astron. J. 88, 1376.CrossRefGoogle Scholar
Hazard, C., Sutton, J., Argue, A.N., Kenworthy, C.M., Morrison, L.V. and Murray, C.A.: 1971, Nature Phys. Sci. 233, 89.CrossRefGoogle Scholar
IAU, 1954, Trans. 8, 90.Google Scholar
IAU, 1977, Trans. 16B, 52.Google Scholar
IAU, 1980, Trans. 17B, 41.Google Scholar
IAU, 1983, Trans. 18B, 48.Google Scholar
Lieske, J.H., Lederle, T., Fricke, W. and Morando, B.: 1977, Astron. Astrophys. 58, 1.Google Scholar
Ma, C., Clark, T.A., and Shaffer, D.B.: 1982, Bull. AAS 13, 899.Google Scholar
Robertson, D.S. and Carter, W.E.: 1982, Proc. Symp. No.5: Geodetic Applications of Radio Interferometry, NOAA Technical Rep. NOS95 NGS24, 63.Google Scholar
Seidelmann, P.K.: 1982, Celest. Mech. 27, 79.CrossRefGoogle Scholar
Wade, C.M. and Johnston, K.J.: 1977, Astron. J. 82, 791.CrossRefGoogle Scholar
Witzel, A. and Johnston, K.J.: 1982, Abhandlungen aus der Hamburger Sternwarte, 10, 151.Google Scholar

Full text views

Full text views reflects PDF downloads, PDFs sent to Google Drive, Dropbox and Kindle and HTML full text views.

Total number of HTML views: 0
Total number of PDF views: 32 *
View data table for this chart

* Views captured on Cambridge Core between 04th August 2017 - 24th January 2021. This data will be updated every 24 hours.

Access
Hostname: page-component-76cb886bbf-7fh6l Total loading time: 0.861 Render date: 2021-01-24T10:43:10.658Z Query parameters: { "hasAccess": "1", "openAccess": "0", "isLogged": "0", "lang": "en" } Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": false, "newCiteModal": false }

Send article to Kindle

To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

The Conversion from the B1950 FK4-Based Position to the J2000 Position of Celestial Objects
Available formats
×

Send article to Dropbox

To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

The Conversion from the B1950 FK4-Based Position to the J2000 Position of Celestial Objects
Available formats
×

Send article to Google Drive

To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

The Conversion from the B1950 FK4-Based Position to the J2000 Position of Celestial Objects
Available formats
×
×

Reply to: Submit a response

Your details

Conflicting interests

Do you have any conflicting interests? *