Spelling suggestions: "subject:"very long baseline interferometry"" "subject:"nery long baseline interferometry""
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Signal processing and analysis of VLBI data using frequency-agile bandwidth synthesis /Searle, Anthony. January 2008 (has links)
Thesis (M.Sc.)--York University, 2008. Graduate Programme in Physics and Astronomy. / Typescript. Includes bibliographical references (leaves 108-110). Also available on the Internet. MODE OF ACCESS via web browser by entering the following URL: http://gateway.proquest.com/openurl?url_ver=Z39.88-2004&res_dat=xri:pqdiss&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&rft_dat=xri:pqdiss:MR38824
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High sensitivity VLBI study of the quasar 3C454.3 /Luca, Peter. January 2007 (has links)
Thesis (M.Sc.)--York University, 2007. Graduate Programme in Physics and Astronomy. / Typescript. Includes bibliographical references (leaves 105-109). Also available on the Internet. MODE OF ACCESS via web browser by entering the following URL: http://gateway.proquest.com/openurl?url_ver=Z39.88-2004&res_dat=xri:pqdiss&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&rft_dat=xri:pqdiss:MR38804
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Sensitive very long baseline interferometry studies of interacting/merging galaxiesMomjian, Emmanuel. January 2003 (has links) (PDF)
Thesis (Ph. D.)--University of Kentucky, 2003. / Title from document title page (viewed onJune 1, 2004). Document formatted into pages; contains ix, 106 leaves : ill. (some col.). Includes abstract and vita. Includes bibliographical references (p. 99-104).
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VLBI observations of the candidate guide stars and their reference sources for the spaceborne NASA/Stanford gyroscope relativity mission (Gravity Probe B)Ransom, Ryan R. January 1997 (has links)
Thesis (M. Sc.)--York University, 1997. Graduate Programme in Physics and Astronomy. / Typescript. Includes bibliographical references (leaves 137-141). Also available on the Internet. MODE OF ACCESS via web browser by entering the following URL: http://wwwlib.umi.com/cr/yorku/fullcit?pMQ27373.
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Sensitive very long baseline interferometry studies of interacting/merging galaxies /Momjian, Emmanuel. Unknown Date (has links) (PDF)
Thesis (Ph. D.)--University of Kentucky, College of Arts and Sciences, 2003. / Each library has both a paper copy and a CD-ROM version. Includes bibliographical references.
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Radioemision dy supernovas y astrometria de alta precision = radio emission from supernovae and high precision astrometry / memoria presentada por Miguel Angel Perez Torres.Perez-Torres, Miguel ©¹ngel. January 1999 (has links)
Thesis (Ph.D.) - Universidad de Valencia, 1999. / Introductory pages in Spanish. Thesis is in English. Includes subject index, pages 177 - 178.
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A VLBI polarisation study of 43 GHZ SiO masers towards VY CMA /Richter, Laura. January 2005 (has links)
Thesis (M. Sc. (Physics and Electronics))--Rhodes University, 2006. / A thesis submitted in partial fulfilment of the requirements for the degree of Masters in Science.
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Studies of radio galaxies and starburst galaxies using wide-field, high spatial resolution radio imagingLenc, Emil. January 2009 (has links)
Thesis (Ph.D) - Swinburne University of Technology, Faculty of Information & Communication Technologies, 2009. / A dissertation presented in fulfillment of the requirements for the degree of Doctor of Philosophy, [Faculty of Information and Communication Technologies], Swinburne University of Technology, 2009. Typescript. Bibliography p. 215-236.
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A VLBI polarisation study of 43 GHZ SiO masers towards VY CMARichter, Laura January 2006 (has links)
This thesis reports the calibration, imaging and analysis of one epoch of VLBI observations of the v (italics) = J (italics) = 1-0 transition of SiO towards VY CMa. Full polarisation information was recorded, allowing high resolution synthesis maps of each of the four Stokes parameters to be produced. A total of 81 maser components were extracted from the total intensity map, each approximately 1 mas in size. The emission spans approximately 100 x 80 mas in right ascension and declination and is concentrated to the east. The maser component positions were fitted to a ring of radius ~ 3.2R₊ (italics), or 7.2 x 1O¹⁴ cm for a stellar distance of 1.5 kpc. If the stellar position is assumed to be the centre of this ring then almost all of the maser components fall within the inner dust shell radius, which is at ~ 5R (italics)ϰ All of the maser components fall between 1.5R (italics)ϰ and 6R (italics)ϰ. A velocity gradient with position angle was observed in the sparsely filled western region of the maser ring. If interpreted as evidence of shell rotation, this gradient implies a rotational velocity of v (italics) rot (subscirpt) sin i (italics) = 18 km.s⁻¹. The fractional circular and linear polarisations of the maser spots were derived from the Stokes parameter maps. The mean fractional circular polarisation of the masers components was ~ 2 percent and the median fractional linear polarisation was ~ 6 percent, with many spots displaying over ~ 30 percent linear polarisation. The mean circular polarisation implies a magnetic field of ~ 4 G in the SiO maser region if the polarisation is due to Zeeman splitting. Two maser components display a rotation of linear polarisation position angle with velocity, possibly implying a connection between the magnetic field and the velocity field variations in the region of these components.
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A VLBI study of OH masers in a proto-planetary nebula OH 0.9+1.3. /McAlpine, Kim. January 1900 (has links)
Thesis (M.Sc. (Physics & Electronics)) - Rhodes University, 2008.
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