Imperial College London
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Dr Jonathan R. Pritchard

Faculty of Natural Sciences, Department of Physics

Reader in Astrophysics
 
 
 
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Contact

 

+44 (0)20 7594 7557j.pritchard Website CV

 
 
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Location

 

1018CBlackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Burns:2017:1538-4357/aa77f4,
author = {Burns, JO and Bradley, R and Tauscher, K and Furlanetto, S and Mirocha, J and Monsalve, R and Rapetti, D and Purcell, W and Newell, D and Draper, D and MacDowall, R and Bowman, J and Nhan, B and Wollack, EJ and Fialkov, A and Jones, D and Kasper, JC and Loeb, A and Datta, A and Pritchard, J and Switzer, E and Bicay, M},
doi = {1538-4357/aa77f4},
journal = {ASTROPHYSICAL JOURNAL},
title = {A Space-based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21cm Global Spectrum},
url = {http://dx.doi.org/10.3847/1538-4357/aa77f4},
volume = {844},
year = {2017}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - The redshifted 21 cm monopole is expected to be a powerful probe of the epoch of the first stars and galaxies ($10\lt z\lt 35$). The global 21 cm signal is sensitive to the thermal and ionization state of hydrogen gas and thus provides a tracer of sources of energetic photons—primarily hot stars and accreting black holes—which ionize and heat the high redshift intergalactic medium (IGM). This paper presents a strategy for observations of the global spectrum with a realizable instrument placed in a low-altitude lunar orbit, performing night-time 40–120 MHz spectral observations, while on the farside to avoid terrestrial radio frequency interference, ionospheric corruption, and solar radio emissions. The frequency structure, uniformity over large scales, and unpolarized state of the redshifted 21 cm spectrum are distinct from the spectrally featureless, spatially varying, and polarized emission from the bright foregrounds. This allows a clean separation between the primordial signal and foregrounds. For signal extraction, we model the foreground, instrument, and 21 cm spectrum with eigenmodes calculated via Singular Value Decomposition analyses. Using a Markov Chain Monte Carlo algorithm to explore the parameter space defined by the coefficients associated with these modes, we illustrate how the spectrum can be measured and how astrophysical parameters (e.g., IGM properties, first star characteristics) can be constrained in the presence of foregrounds using the Dark Ages Radio Explorer (DARE).
AU  - Burns,JO
AU  - Bradley,R
AU  - Tauscher,K
AU  - Furlanetto,S
AU  - Mirocha,J
AU  - Monsalve,R
AU  - Rapetti,D
AU  - Purcell,W
AU  - Newell,D
AU  - Draper,D
AU  - MacDowall,R
AU  - Bowman,J
AU  - Nhan,B
AU  - Wollack,EJ
AU  - Fialkov,A
AU  - Jones,D
AU  - Kasper,JC
AU  - Loeb,A
AU  - Datta,A
AU  - Pritchard,J
AU  - Switzer,E
AU  - Bicay,M
DO  - 1538-4357/aa77f4
PY  - 2017///
SN  - 0004-637X
TI  - A Space-based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21cm Global Spectrum
T2  - ASTROPHYSICAL JOURNAL
UR  - http://dx.doi.org/10.3847/1538-4357/aa77f4
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000405906300009&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/51788
VL  - 844
ER  -
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