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AMiBA: First-year results for Sunyaev-Zel'dovich effect

  • Jiun Huei Proty Wu
  • , Tzi Hong Chiueh
  • , Chi Wei Huang
  • , Yao Wei Liao
  • , Fu Cheng Wang
  • , Pablo Altimirano
  • , Cha Hao Chang
  • , Su Hao Chang
  • , Su Wei Chang
  • , Ming Tang Chen
  • , Guillaume Chereau
  • , Chih Chiang Han
  • , Paul T.P. Ho
  • , Yao De Huang
  • , Yuh Jing Hwang
  • , Homin Jiang
  • , Patrick Koch
  • , Derek Kubo
  • , Chao Te Li
  • , Kai Yang Lin
  • Guo Chin Liu, Pierre Martin-Cocher, Sandor Molnar, Hiroaki Nishioka, Philippe Raffin, Keiichi Umetsu, Michael Kesteven, Warwick Wilson, Mark Birkinshaw, Katy Lancaster

Research output: Contribution to journal › Article (Academic Journal) › peer-review

5 Citations (Scopus)

Abstract

We discuss the observation, analysis, and results of the first-year science operation of AMiBA, an interferometric experiment designed to study cosmology via the measurement of Cosmic Microwave Background (CMB). In 2007, we successfully observed 6 galaxy clusters (z < 0.33) through the Sunyaev-Zel'dovich effect. AMiBA is the first CMB interferometer operating at 86-102 GHz, currently with 7 close-packed antennas of 60 cm in diameter giving a synthesized resolution of around 6 arcminutes. An observing strategy with on-off-source modulation is used to remove the effects from electronic offset and ground pickup. Formalism of the analysis is given and preliminary science results are summarized. Tests for systematic effects are also addressed. We also discuss the expansion plan.

Original languageEnglish
Pages (from-to)1675-1686
Number of pages12
JournalModern Physics Letters A
Volume23
Issue number17-20
Publication statusPublished - 28 Jun 2008

Keywords

  • Cosmic microwave background
  • Cosmology
  • Galaxy cluster

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