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VHF-band RFI in Geographically Remote Areas. 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. Outline.
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VHF-band RFI in Geographically Remote Areas Judd D. BowmanHubble Fellow, CaltechAlan E. E. RogersHaystack Observatory With support from: CSIRO/MRO and Curtin University Thanks to: The organizers and Murray Lewis and the NSF31 March 2010 RFI2010 Groningen
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
Experiment to Detect the Global Epoch of Reionization Signature (EDGES)
Exotic Telescopes Prepare to Probe Era of First Stars and Galaxies Science, Vol. 325. no. 5948, pp. 1617 – 1619, 25 September 2009
The approach for LOFAR, MWA, PAPER, SKA… “Science with the MWA” Greenhill, Bowman, et al. (2010, in prep) Figure by Matt McQuinn
The approach for EDGES [MHz] 10 50 100 500 50 0 -50 -100 Tb [mK] 21 cm global brightness temperature 100 10 z [redshift] Pritchard & Loeb 2008
EDGES Bowman & Rogers (in prep)
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
Total power in band vs. time Sum antenna temperature 90-205 MHz Orbcomm band ~138 MHz
Anomalous propagation – DTV 7 and 9 EDGES Memo#058, AEER, 2010
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
US TV and FM radio “pollution” West Forks, Maine D1 Array – Haystack Obs.
Rural New England, US D1 Array – Haystack Obs. West Forks, Maine EDGES Memo#044, AEER, 2009
Catlow Valley, Oregon, US EDGES Memo#052, AEER, JDB, 2009 60 dB 80 MHz 200 10 dB
Time-variable FM RFI FM band
Meteor scatter rates vs. elevation angle horizon zenith EDGES Memo#054, AEER, 2009
Summary • 3 month deployment in MRO • Deepest broadband spectrum ever acquired: 5 mK rms (-220 dBW/m2/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
Summary • 3 month deployment in MRO • Deepest broadband spectrum ever acquired: 5 mK rms (-220 dBW/m2/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