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January 26 th , 2011 The future of the VLBA Eduardo Ros. The 40m YEBES RT and the HSA. Note. Material for this talk provided by the Observatorio Astronómico Nacional (F. Colomer et al.). IGN YEBES 40m radio telescope.
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January 26th, 2011 The future of the VLBA Eduardo Ros The 40m YEBES RT and the HSA E. Ros - Yb and the HSA
Note Material for this talk provided by the ObservatorioAstronómicoNacional (F. Colomer et al.) E. Ros - Yb and the HSA
IGN YEBES 40m radio telescope • Owned and operated by the National Geographical Institute (IGN) – National Astronomical Observatory (OAN) • Currently member of the European VLBI Network (EVN) and International VLBI Service for Geodesy and Astrometry (IVS). Joining GMVA in 2011. • Receivers in 2-115 GHz bands (Q band under construction). • VLBI instrumentation (MK5B, DBBC, 1 Gbps fiber connection). • Frequency agile (change in few minutes) • More available at high frequencies. E. Ros - Yb and the HSA
Location Jodrell (Lovell) 72-m WSRT 14 × 25-m Effelsberg 100-m Nançay 100-m Robledo 70-m Yebes 40-m Sardinia 64-m E. Ros - Yb and the HSA
Optics: Nasmyth focus E. Ros - Yb and the HSA
Receivers and VLBI instrumentation E. Ros - Yb and the HSA
Sensitivity • EVN sensitivity calculator (256 Mbps, 150min integration, natural weighting; thermal noise sensitivity in mJy/beam). E. Ros - Yb and the HSA
Sensitivity * EVN sensitivity calculator (256 Mbps, 150min integration, natural weighting; thermal noise sensitivity in mJy/beam). E. Ros - Yb and the HSA
uv coverage VLBA+Ar+GB+Y27 only Adding Ys E. Ros - Yb and the HSA
Radio Supernovae – target for HSA observations (and globals) Marcaide et al. Young supernovae in near galaxies can be probed and monitored by VLBI SN1993J, SN1979C, SN1986J, targets in M82, and many others E. Ros - Yb and the HSA