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The Canadian Hydrogen Intensity Mapping Experiment Matt Dobbs

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Page 1: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

The Canadian Hydrogen Intensity Mapping Experiment

Matt Dobbs

Page 2: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 4

(slide adapted from NASA publicity figure)

today

Page 3: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 5

(slide adapted from NASA publicity figure)

today

TODAY

Page 4: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 9

At z=1-3 for 21cm line, need 100m telescope to resolve BAO clearly.

Unresolved galaxies, resolved BAO.

BAO Scale

Blanton et al. (2003)

Galaxy Surveys vs. Intensity Mapping Galaxy Surveys !  ~1% (2 Gpc3/h3) of the

universe has been mapped with optical light from galaxies.

!  Galaxy surveys are expensive

!  Rely on (non-linear) galaxies as tracers for BAO

Page 5: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 10

21 cm Hydrogen Line

(Parkes Telescope)

Frequency gives redshift: ν = 1420MHz / (1+z)

Oort et al. 1958

HI map of the Milky Way Rate 3 x 10-15/s

Page 6: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 11

3-D Intensity Mapping

Page 7: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 12

Simulation Video: Nick Gnedin & Dave McGinnis (Fermilab),

Cosmic Sound Start: z=0.01 End: z=0.62

Page 8: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 15

Mapping the

Observable Universe

WiggleZ

13.7Gy

CMB Big Bang

Reionization

SDSS

1100

z ∞ 50 9 5 3 2 1

7Gy CHIME

300ky

0

500My

Age of Universe

CHIME will: •  survey BAO •  measure the growth of space •  from 0.8<z<2.5 •  over a volume of ~400 co-moving Gpc3

Slide from K. Vanderlinde

SPT

Page 9: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 18

Illinois 1937: Grote Reber, 9m First parabolic dish radio telescope Sky survey

Illinois 400’ (120x180m) 1959 !  610 MHz !  BW ~ 5 MHz

Green Bank Telescope, 100m

Page 10: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 24

Cylinder Antenna

Page 11: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 25

Cylinder Telescope

Page 12: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 26

CHIME

Page 13: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

The Canadian Hydrogen Intensity Mapping Experiment

UBC !  Mandana Amiri !  Greg Davis !  Meiling Deng !  Mark Halpern !  Gary Hinshaw !  Kris Sigurdson !  Mike Sitwell

U Toronto / CITA !  Dick Bond !  Ue-li Pen !  Richard Shaw !  Keith Vanderlinde !  Ivan Padilla

HIA, DRAO !  Tom Landecker

McGill U !  Kevin Bandura !  Jean-Francois Cliche !  Matt Dobbs !  Adam Gilbert !  David Hanna !  Juan Mena Parra

View poster!

Page 14: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

The Canadian Hydrogen Intensity Mapping Experiment

•  a transit telescope •  no moving parts •  one scan strategy •  24/7 observations •  no TAC (time allocation committee)

Page 15: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 32

Full CHIME Specs Full CHIME Layout

Structure 5 cylinders, 100m x 20m each

Bandwidth 400-800 MHz Digitize 8bits at 800 MSPS

Number Feeds/cylinder 256 dual pol feeds per cylinder (2560 digitizers total)

~31cm spacing

Frequency Channels 512 frequency channels, 781 kHz wide (1.28 µs) (for cosmology, you can channelize further!)

Data Rate 2NFEEDS x 3.2 Gbit/s = 8 TeraBit/s (assumes 4bit truncation)

Observing Frequency 400 MHz to 800 MHz

Wavelength 75 cm 37 cm

21cm Redshift z=2.5 (11 Gyr ago) z=0.8 (7 Gyr ago)

Beam Size 0.52o 0.26o

E-W FoV 2.5o 1.3o

N-S FoV -45o to +135o (max possible) 0o to +90o (more likely)

Time/pixel/day 10min, 14min, 24hrs equator, 45deg, ncp

5min, 7min, 24hrs equator, 45deg, ncp

Receiver Noise Temperature Flux Conversion Daily Sensitivity Final Survey

50k ~2K / Jy

~50 µJy / pixel ~1.5 µJy/pixel

(Approximate – for planning purposes only)

Page 16: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 33

CHIME

Page 17: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 34

Page 18: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 35

Page 19: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 36

Page 20: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 37

Page 21: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 38

Page 22: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 39

Two FMC Mezzanines (analog signals come in the front)

FPGA

Two Gbit Ethernet

Digital signals come in the back

ARM processor DDR RAM Ethernet

9U VME Front-panel

Custom Backplane Power, clock, timestamp Board inter-connect

Page 23: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 40

Page 24: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 41

1 TB/s = 86 PB/day

Page 25: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 43

1280 x 10 Gbe

Page 26: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 45

CHIME&Development&

40m 40m

Prototype, two 8m Dishes •  4 channels •  running since March 2011 Pathfinder, two 20m x 40m Cylinders •  256 channels •  under construction Full CHIME, five 20m x 100m Cylinders •  2560 channels •  FUNDED by CFI. Operating in 2016.

Page 27: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 46

DRAO – CHIME Site

Jan 2013: Construction of CHIME Pathfinder

Page 28: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 47

DRAO – CHIME Site

Pathfinder construction, April 14, 2013

Page 29: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 48

Beyond Cosmology !  Chime will map the polarization and intensity of 40% of the

sky with great sensitivity in a poorly explored frequency band.

!  Pulsar monitoring "  Nightly all-sky monitoring for Pulsar Timing Arrays "  Monitor “space weather”, to correct observations at higher frequency.

!  Pulsar search "  Detect new pulsars, then monitor them daily.

!  Radio transient phenomena "  New ground. "  Surprisingly bright and distant radio events have been reported

recently. CHIME is an ideal all-sky monitor. !  Galactic Magnetic Fields

Page 30: The Canadian Hydrogen Intensity Mapping Experimentastro.physics.mcgill.ca/WorkshopTrottier/CHIME.pdfIvan Padilla HIA, DRAO ! Tom Landecker McGill U ! Kevin Bandura ! Jean-Francois

[email protected], CHIME Overview 2013-04 54

Summary !  Intensity mapping—new tool

to map the expansion history of the universe. "  z=1-3 key for Dark Energy

!  FFT Telescope will come of Age with CHIME – seeing the whole overhead sky at once.

!  CHIME will map the largest volume of the universe to date.

!  CHIME will measure the expansion of space in a large chunk of the observable universe, to z~2.5.

!  Hydrogen mapping can (in theory) probe anything to z~>50.

CMB Big Bang

Reionization

1100

z ∞ 50

9 5 3 2 1

WiggleZ

SDSS

SPT

CHIME