eMERLIN+EVN status update
Eskil Varenius Operational Support Scientist Jodrell Bank Observatory
EVN TOG meeting 2018-03-19 Shanghai Astronomical Observatory
eMERLIN+EVN status update Eskil Varenius Operational Support - - PowerPoint PPT Presentation
eMERLIN+EVN status update Eskil Varenius Operational Support Scientist Jodrell Bank Observatory EVN TOG meeting 2018-03-19 Shanghai Astronomical Observatory Outline Why eMERLIN in EVN? What works already? What doesnt work
Eskil Varenius Operational Support Scientist Jodrell Bank Observatory
EVN TOG meeting 2018-03-19 Shanghai Astronomical Observatory
Baselines (i.e. science) ! VLA (<36 km) <-> eMERLIN (11 km to 217 km) <-> EVN (>100 km)
Baselines (i.e. science) ! VLA (<36 km) <-> eMERLIN (11 km to 217 km) <-> EVN (>100 km)
−4 −3 −2 −1 1 2 3 4 ∆ R.A. [arcseconds] −4 −3 −2 −1 1 2 3 4 ∆δ [arcseconds] 6 12 18 24 30 36 42 48 mJy / beam
Ultra-Luminous Infrared Galaxy Arp 220 0.5 mas @ 5 GHz Global VLBI (Varenius et al., submitted) Ultra-Luminous Infrared Galaxy Arp 220 0.5 arcsec @ 150 MHz
50-5 mas
Ef-Cm Ef-Da Ef-De Ef-Jb2 (DBBC) Ef-Kn Ef-Ta (Pi) (De wire mesh)
Note: Jb2 (and Jb1) can be improved