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GBT 21 cm intensity mapping collaboration. Academia Sinica (Tzu-Ching Chang, Victor Yu-wei Liao ) Beijing (Xuelei Chen, Yi-Chao Li ) Carnegie Mellon University ( Aravind Natarajan , Jeff Peterson, Tabitha Voytek ) - PowerPoint PPT Presentation
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GBT 21 cm intensity mapping collaboration
Academia Sinica (Tzu-Ching Chang, Victor Yu-wei Liao)Beijing (Xuelei Chen, Yi-Chao Li)Carnegie Mellon University (Aravind Natarajan, Jeff Peterson, Tabitha Voytek)CITA/UToronto (Nidhi Banavar, Liviu Calin, Adam Lewis, Kiyo Masui, Ue-Li Pen, Richard Shaw, Eric Switzer)McGill (Kevin Bandura)
ARAA review article May 2010 (Morales and Wyithe) comparing to z ~ 10:
Two months later:
IM: now and thenz ~1 ~10
Science goal BAO EoR
Signal (mK) 0.1 10
Thermal noise (K) 30 300
Foreground spatial fluctuation (K)
0.1 10
Angular scale ~10’+ (non-linear scale)
~10’- (bubble scale)
First proposed 2007 1970’s?
First detected 2010 >2012
Strategy single dish Interferometers
RFI
Liu and Tegmark 2011
The real data
Signal-only simulations
20 Mpc
ΩHI = 10-3
Relaxed quadratic estimation
Most general: Inverse covariance, down-weight foreground in both angle and frequency.
Imperfect spectral baseline – need non-parametric removal: SVD on cross maps
Liu & Tegmark MNRAS, Volume 419, Issue 4, pp. 3491-3504.Projecting (idempotent) LOS modes is “good enough” vs. optimal downweighting.
These suggest that our method is slightly sub-optimal (in theory), but ideal in practice because we use the covariance of the real data!
SVD eigenvalues
Modes falling off rapidly: few DOF to describe most of the foregrounds.
Mode number (sorted)
Eig
enva
lue
Real data, cleaned
(25 modes removed here.)
Cross-pairs: GBT power
( *
(
)
)*×
Map A
Weight B
Map B
Weight A
Cross-pairs: WiggleZ crosspower
( *
(
)
)*×
Map A
Selection function
Galaxy catalog
Weight A
Preliminary
Fisher-matrix predictions
Conclusions• End-to-end demonstration: calibration, ionosphere,
point sources, galaxy, spectral response, etc. No show stoppers. Lessons learned for EoR.
• Foreground subtraction under control: ready for z~1 21cm intensity mapping.
• Consistent autonomous 21cm maps and power spectra.
• Proposal for GBT 0.5<z<1 BAO survey using new ASIAA 9 pixel receiver array starting 2013.
• Retires major risk for CHIME!