... This oral history is being conducted with Richard Nygren in Houston, Texas, for the NASA Johnson Space Center Oral History Project. ... Because of the limited progress and Soyuz launch capability, we had very little science that we felt we could get accomplished, but we wanted to get as much as possible. ... You were working in the Payloads Office before we actually had Space Station up and going, as it took us a while to get there. ... Nygren: There you go, oral history, yes, that could be, could...
. Comment on J0319+4130 . Our image does represent the main source structure. However, due to the limited u-v coverage, it does not have as high fidelity as other known images, such as the one at 5 GHz by Romney et al. (1995). VLBApls home page . Last modified: 16 Oct 2000
... The radio structure is found to comprise very dim, nearly circular lobes with an extraordinarily bright and compact hot spot located at the western extremity of the western lobe. ... Further, the extraordinary brightness ratio between the western hot spot and the unusually dim and circular lobes argues for some unusual differences between this object and more `normal' examples of radio-loud AGN. ... Fig. ... The lobes Fig. 3 shows Pictor A at 20 cm with a resolution of 10 . ... A similar fea- Fig. ...
. Mac: the Mac binary works with MacOS X 10.6 - 10.10, though on 10.9 or later you should disable app nap: select Get Info on TUI; if you see a checkbutton labelled "Disable App Nap" then check it. The Mac version is not signed, so MacOS may complain when you try to launch it. If that happens simply right-click on the application and select "Open...". Unix: runs from source, so is compatible with all flavors of unix. See the installation instructions for the required version of Python and other libraries.