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Atomic Emission Spectroscopy: Instrumentation01:22

Atomic Emission Spectroscopy: Instrumentation

The instrumentation of atomic emission spectrometry (AES) involves various components, including atomization devices that convert samples into gas-phase atoms and ions. There are two main types of atomization devices: continuous and discrete atomizers.  Continuous atomizers, like plasmas and flames, introduce samples in a constant stream, while discrete atomizers inject individual samples using syringes or autosamplers. The most common discrete atomizer is the electrothermal atomizer.
Atomic Absorption Spectroscopy: Instrumentation01:22

Atomic Absorption Spectroscopy: Instrumentation

An atomic absorption spectrophotometer (AAS) comprises several components: a radiation source, an atomizer, a monochromator, and a detector. The radiation source can be a hollow-cathode lamp (HCL) or an electrodeless-discharge lamp (EDL), both of which provide a narrow emission line of the required wavelength. However, some instruments use continuum sources and high-resolution monochromators to achieve a narrow range of radiation.
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Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation01:26

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation

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Attenuated Total Reflectance (ATR) Infrared Spectroscopy: Overview01:13

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Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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Invited article: millimeter-wave bolometer array receiver for the Atacama pathfinder experiment Sunyaev-Zel'dovich

D Schwan1, P A R Ade, K Basu

  • 1Department of Physics, University of California, Berkeley, California 94720, USA. schwan@berkeley.edu

The Review of Scientific Instruments
|October 7, 2011
PubMed
Summary

The Atacama Pathfinder Experiment-Sunyaev-Zel'dovich (APEX-SZ) instrument uses advanced superconducting detectors to map galaxy clusters. This millimeter-wave receiver significantly advanced Sunyaev-Zel'dovich effect observations with improved sensitivity and field-of-view.

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Area of Science:

  • Astronomy and Astrophysics
  • Cosmology
  • Instrumental Science

Background:

  • The Sunyaev-Zel ovich (SZ) effect provides a powerful probe of galaxy clusters, the largest structures in the universe.
  • Previous SZ instruments faced limitations in sensitivity and field-of-view, hindering comprehensive cluster mapping.
  • The Atacama Pathfinder Experiment (APEX) telescope provides a stable, high-altitude platform for millimeter-wave observations.

Purpose of the Study:

  • To describe the design and performance of the Atacama Pathfinder Experiment-Sunyaev-Zel ovich (APEX-SZ) instrument.
  • To highlight the technological advancements incorporated into the APEX-SZ receiver.
  • To present the results of APEX-SZ observations in mapping galaxy clusters.

Main Methods:

  • Utilized a focal plane of 280 superconducting Transition-Edge Sensor (TES) bolometers cooled to 280 mK.
  • Employed a frequency-domain multiplexed readout system for efficient data acquisition.
  • Integrated a three-stage helium sorption refrigerator and a pulse-tube cooler for cryogenics.

Main Results:

  • Achieved 1' angular resolution and a 22' field-of-view at 150 GHz, ideal for cluster mapping.
  • Demonstrated TES bolometer sensitivity of 890 μK(CMB)√s, with upgraded detectors reaching 530 μK(CMB)√s.
  • Successfully mapped 48 galaxy clusters since its commissioning in April 2007.

Conclusions:

  • The APEX-SZ instrument represents a significant technological leap in Sunyaev-Zel ovich observations.
  • Its advanced design and performance enable more sensitive and efficient mapping of galaxy clusters.
  • APEX-SZ has proven instrumental in advancing our understanding of large-scale structure formation.