Canadian Hydrogen Intensity Mapping Experiment (CHIME) pathfinder

A pathfinder version of CHIME (the Canadian Hydrogen Intensity Mapping Experiment) is currently being commissioned at the Dominion Radio Astrophysical Observatory (DRAO) in Penticton, BC. The instrument is a hybrid cylindrical interferometer designed to measure the large scale neutral hydrogen power spectrum across the redshift range 0.8 to 2.5. The power spectrum will be used to measure the baryon acoustic oscillation (BAO) scale across this poorly probed redshift range where dark energy becomes a significant contributor to the evolution of the Universe. The instrument revives the cylinder design in radio astronomy with a wide field survey as a primary goal. Modern low-noise amplifiers and digital processing remove the necessity for the analog beam forming that characterized previous designs. The Pathfinder consists of two cylinders 37m long by 20m wide oriented north-south for a total collecting area of 1,500 square meters. The cylinders are stationary with no moving parts, and form a transit instrument with an instantaneous field of view of ~100 degrees by 1-2 degrees. Each CHIME Pathfinder cylinder has a feedline with 64 dual polarization feeds placed every ~30 cm which Nyquist sample the north-south sky over much of the frequency band. The signals from each dual-polarization feed are independently amplified, filtered to 400-800 MHz, and directly sampled at 800 MSps using 8 bits. The correlator is an FX design, where the Fourier transform channelization is performed in FPGAs, which are interfaced to a set of GPUs that compute the correlation matrix. The CHIME Pathfinder is a 1/10th scale prototype version of CHIME and is designed to detect the BAO feature and constrain the distance-redshift relation. The lessons learned from its implementation will be used to inform and improve the final CHIME design.

[1]  Kevin Bandura,et al.  A Radio-Frequency-over-Fiber link for large-array radio astronomy applications , 2013, 1308.5481.

[2]  A. Stebbins,et al.  ALL-SKY INTERFEROMETRY WITH SPHERICAL HARMONIC TRANSIT TELESCOPES , 2013, 1302.0327.

[3]  Adam D. Myers,et al.  Baryon Acoustic Oscillations in the Lyforest of BOSS quasars , 2012 .

[4]  Abraham Loeb,et al.  Possibility of precise measurement of the cosmological power spectrum with a dedicated survey of 21 cm emission after reionization. , 2008, Physical review letters.

[5]  Daniel Thomas,et al.  The clustering of galaxies in the sdss-iii baryon oscillation spectroscopic survey: Baryon acoustic oscillations in the data release 9 spectroscopic galaxy sample , 2012, 1312.4877.

[6]  X. Siemens,et al.  UvA-DARE ( Digital Academic Repository ) Fast Radio Burst Discovered in the Arecibo Pulsar ALFA Survey , 2014 .

[7]  Scott Croom,et al.  The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations , 2011, 1108.2635.

[8]  Meiling Deng,et al.  The cloverleaf antenna: A compact wide-bandwidth dual-polarization feed for CHIME , 2014, 2014 16th International Symposium on Antenna Technology and Applied Electromagnetics (ANTEM).

[9]  C. A. Oxborrow,et al.  Planck 2013 results. XVI. Cosmological parameters , 2013, 1303.5076.

[10]  Adam G. Riess,et al.  Observational probes of cosmic acceleration , 2012, 1201.2434.

[11]  Graeme Smecher,et al.  Calibrating CHIME: a new radio interferometer to probe dark energy , 2014, Astronomical Telescopes and Instrumentation.

[12]  M. Mclaughlin,et al.  A Bright Millisecond Radio Burst of Extragalactic Origin , 2007, Science.

[13]  E. R. Switzer,et al.  Determination of z ∼ 0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping autocorrelation , 2013, 1304.3712.

[14]  R. Nichol,et al.  Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies , 2005, astro-ph/0501171.

[15]  S. Burke-Spolaor,et al.  A Population of Fast Radio Bursts at Cosmological Distances , 2013, Science.

[16]  Edward J. Wollack,et al.  NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS , 2012, 1212.5226.

[17]  R. Ellis,et al.  The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications , 2005, astro-ph/0501174.

[18]  Martin Leung A wideband feed for a cylindrical radio telescope , 2008 .

[19]  Kevin Bandura,et al.  An intensity map of hydrogen 21-cm emission at redshift z ≈ 0.8 , 2010, Nature.

[20]  Ue-Li Pen,et al.  Coaxing cosmic 21 cm fluctuations from the polarized sky using m -mode analysis , 2014, 1401.2095.

[21]  E. R. Switzer,et al.  MEASUREMENT OF 21 cm BRIGHTNESS FLUCTUATIONS AT z ∼ 0.8 IN CROSS-CORRELATION , 2012, 1208.0331.

[22]  Adam D. Myers,et al.  Measurement of baryon acoustic oscillations in the Lyman-α forest fluctuations in BOSS data release 9 , 2013, 1301.3459.

[23]  J. N. Hewitt,et al.  Detectability of Late-Time Radio Afterglows from Compact Binary Coalescence , 2014 .