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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.

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Presentation on theme: "Judd D. Bowman Hubble Fellow, Caltech Alan E. E. Rogers Haystack Observatory With support from: CSIRO/MRO and Curtin University Thanks to: The organizers."— Presentation transcript:

1 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

2 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

3 Experiment to Detect the Global Epoch of Reionization Signature (EDGES)

4 Exotic Telescopes Prepare to Probe Era of First Stars and Galaxies Science, Vol. 325. no. 5948, pp. 1617 – 1619, 25 September 2009

5 The approach for LOFAR, MWA, PAPER, SKA… “Science with the MWA” Greenhill, Bowman, et al. (2010, in prep) Figure by Matt McQuinn

6 The approach for EDGES Pritchard & Loeb 2008 10010 z [redshift] 50 0 -50 -100 T b [mK] 21 cm global brightness temperature 5001005010  [MHz]

7 EDGES

8 Bowman & Rogers (in prep)

9

10 Deep VHF-band integrations at the MRO

11 Murchison Radio-astronomy Observatory

12 Radio Frequency Interference (RFI)

13 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

14 Orbcomm LEO satellite constellation (136-138 MHz)

15 Total power in band vs. time Sum antenna temperature 90-205 MHz Orbcomm band ~138 MHz

16

17 Anomalous propagation – DTV 7 and 9 EDGES Memo#058, AEER, 2010

18 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

19 Example excision rates

20 Shallow surveys in remote areas of the US

21 US TV and FM radio “pollution” D1 Array – Haystack Obs. West Forks, Maine

22 Rural New England, US D1 Array – Haystack Obs. West Forks, Maine EDGES Memo#044, AEER, 2009

23 US TV and FM radio “pollution”

24

25 Catlow Valley, Oregon, US 60 dB 10 dB 80 MHz 200 EDGES Memo#052, AEER, JDB, 2009

26 Meteor scattering

27 Time-variable FM RFI FM band

28 Meteor scatter rates vs. elevation angle EDGES Memo#054, AEER, 2009 horizon zenith

29 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

30 Aircraft at MRO

31 FM at MRO

32 RFI observed in Oregon, US

33 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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