PPT-Double Trouble: ASKAP Early Science using Radio Galaxies

Lawrence Rudnick University of Minnesota Deepwidebandpolarization 30 m Jy800sq deg 7001800 More science using subsamples This is single project from large survey Feasible with JVLA only NVSS level investment. The Double Trouble Historic District occupies over 200 acres and includes the village and surrounding bogs The natural environment of cedar forest and rapidly flowing stream provided both raw materials and water power for an extensi ve lumber indust ASKAP is a next-generation radio telescope incorporating novel receiver technologies and leading-edge ICT systems. It will be made up of  antennas, each  metres in diameter, working together a Anatomy of Extragalactic . R. adio Sources. Miley. Symposium May, 2013, Chris Carilli NRAO. ‘Radio Galaxies as beacons to early, massive galaxy formation’. Anatomy at low redshift. High luminosity (FRII, L. Lisa Harvey-. Smith & Aidan . Hotan. . | ASKAP Project . Scientists. August 5. th. 2013. ASTRONONY & SPACE SCIENCE. ASKAP funding, fabrication, integration, commissioning is phased.. Science can also be phased.. CSIRO Astronomy and Space Science. David Brodrick. EPICS [Spring] Collaboration Meeting. 22nd October 2014. Australia Telescope Compact Array (Narrabri, NSW). We measure the spatial coherence function. Paul . Nulsen. (. CfA. ), Christine Jones (. CfA. ), . William Forman (. CfA. ), Eugene . Churazov. (MPA),. Laurence David (. CfA. ), Brian McNamara (Waterloo),. Steven Murray (. CfA. ) . AGN Outbursts in Giant . S. urveys . of . Local Galaxies. Michael . Brown. ARC Future Fellow. Monash. University. Where are we now?. NVSS / FIRST / SUMMS. 0.5 . mJy. RMS per beam. 15”-1’ beam. ~30 . uJy. RMS per beam in 12 hours . David Roberts, Jake Cohen, & Jing Lu. Brandeis University. Lakshmi . Saripalli. & Ravi . Subrahmanyan. Raman Research Institute. 1. Radio Galaxies. X-Shaped Radio Galaxies. Cheung’s Sample. Paul . Nulsen. (. CfA. ), Christine Jones (. CfA. ), . William Forman (. CfA. ), Eugene . Churazov. (MPA),. Laurence David (. CfA. ), Brian McNamara (Waterloo),. Steven Murray (. CfA. ) . AGN Outbursts in Giant . Bryan Gaensler. , Tom Landecker, Russ Taylor. and the POSSUM team. askap.org. /possum. New Discovery Space with ASKAP-12. Radio polarimetry: a highly sensitive probe of density, magnetic field and turbulence at all redshifts. Craig Sarazin. University of Virginia. M86. (. Randall et al. 2008). . Abell. 2052. (Blanton et . al. . 2011). Optical light dominated by bulge. Last star formation typically billions of years ago. Jeremy . Harwood. YERAC 2011. Background Image courtesy of NASA/CXC/CfA/R.Kraft et al.; MPIfR/ESO/APEX/A. Weiss et al.; ESO/WFI. What are radio galaxies?. Type of active galaxy. Fanaroff and Riley class I. Extragalactic radio . s. ources and their importance for astronomy. Leiden 10-13 June 2013. Ron Ekers. CSIRO, . Australia. George Miley. The largest, the furthest, the most powerful, and to some of us the most fascinating objects known in the Universe are to be found among the radio sources associated with some elliptical galaxies and QSO’s. In recent years it has become apparent that they are also objects of considerable beauty.. of . Local Galaxies. Michael . Brown. ARC Future Fellow. Monash. University. Where are we now?. NVSS / FIRST / SUMMS. 0.5 . mJy. RMS per beam. 15”-1’ beam. ~30 . uJy. RMS per beam in 12 hours .