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Judd D. Bowman Hubble Fellow, Caltech Alan E. E. Rogers Haystack Observatory With support from: CSIRO/MRO and Curtin University Thanks to: The organizers and Murray Lewis and the NSF 31 March 2010 RFI2010 Groningen VHF-band RFI in Geographically Remote Areas
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Outline Experiment to Detect the Global EoR Signature (EDGES) RFI at Murchison Radio-astronomy Observatory (MRO) Quick surveys in the US Rural New England Catlow Valley, Oregon A few words on meteor scattering
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Experiment to Detect the Global Epoch of Reionization Signature (EDGES)
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Exotic Telescopes Prepare to Probe Era of First Stars and Galaxies Science, Vol. 325. no. 5948, pp. 1617 – 1619, 25 September 2009
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The approach for LOFAR, MWA, PAPER, SKA… “Science with the MWA” Greenhill, Bowman, et al. (2010, in prep) Figure by Matt McQuinn
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The approach for EDGES Pritchard & Loeb 2008 10010 z [redshift] 50 0 -50 -100 T b [mK] 21 cm global brightness temperature 5001005010 [MHz]
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EDGES
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Bowman & Rogers (in prep)
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Deep VHF-band integrations at the MRO
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Murchison Radio-astronomy Observatory
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Radio Frequency Interference (RFI)
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Integrated spectrum at MRO by EDGES Murchison Radio-Astronomy Observatory (MRO) Aug 20 – Oct 20, 2009 1440 wall-clock hours on sky ~50 hours actual integration +15 dB +40 dB
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Orbcomm LEO satellite constellation (136-138 MHz)
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Total power in band vs. time Sum antenna temperature 90-205 MHz Orbcomm band ~138 MHz
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Anomalous propagation – DTV 7 and 9 EDGES Memo#058, AEER, 2010
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Integrated RFI (time excision only – by broadband power level in FM, Orbcomm, DTV bands: 30% removal) Note: shows every channel that ever had RFI over 3 months Conservatively excise any channel that had RFI: 11% removal
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Example excision rates
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Shallow surveys in remote areas of the US
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US TV and FM radio “pollution” D1 Array – Haystack Obs. West Forks, Maine
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Rural New England, US D1 Array – Haystack Obs. West Forks, Maine EDGES Memo#044, AEER, 2009
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US TV and FM radio “pollution”
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Catlow Valley, Oregon, US 60 dB 10 dB 80 MHz 200 EDGES Memo#052, AEER, JDB, 2009
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Meteor scattering
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Time-variable FM RFI FM band
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Meteor scatter rates vs. elevation angle EDGES Memo#054, AEER, 2009 horizon zenith
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Summary 3 month deployment in MRO – Deepest broadband spectrum ever acquired: 5 mK rms (-220 dBW/m 2 /Hz) – First redshifted 21 cm EoR science – Simple time and spectral flagging sufficient to remove RFI – FM band a good indicator of anomalous transmission events – Total power in band varies strongly with Orbcomm and aircraft Quiet sites in US – not as good as MRO – Meteor scatter a significant source of RFI, dependent on elevation angle of sky coverage
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Aircraft at MRO
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FM at MRO
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RFI observed in Oregon, US
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Summary 3 month deployment in MRO – Deepest broadband spectrum ever acquired: 5 mK rms (-220 dBW/m 2 /Hz) – First redshifted 21 cm EoR science – Simple time and spectral flagging sufficient to remove RFI – FM band a good indicator of anomalous transmission events – Total power in band varies strongly with Orbcomm and aircraft Quiet sites in US – not as good as MRO – Meteor scatter a significant source of RFI, dependent on elevation angle of sky coverage
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