SCUBA-2: The 10000 pixel bolometer camera on the James Clerk Maxwell Telescope
arXiv:1301.3650 · doi:10.1093/mnras/sts612
Abstract
SCUBA-2 is an innovative 10000 pixel bolometer camera operating at submillimetre wavelengths on the James Clerk Maxwell Telescope (JCMT). The camera has the capability to carry out wide-field surveys to unprecedented depths, addressing key questions relating to the origins of galaxies, stars and planets. With two imaging arrays working simultaneously in the atmospheric windows at 450 and 850 microns, the vast increase in pixel count means that SCUBA-2 maps the sky 100-150 times faster than the previous SCUBA instrument. In this paper we present an overview of the instrument, discuss the physical characteristics of the superconducting detector arrays, outline the observing modes and data acquisition, and present the early performance figures on the telescope. We also showcase the capabilities of the instrument via some early examples of the science SCUBA-2 has already undertaken. In February 2012, SCUBA-2 began a series of unique legacy surveys for the JCMT community. These surveys will take 2.5 years and the results are already providing complementary data to the shorter wavelength, shallower, larger-area surveys from Herschel. The SCUBA-2 surveys will also provide a wealth of information for further study with new facilities such as ALMA, and future telescopes such as CCAT and SPICA.
23 pages, 20 figures, 3 tables. Accepted by MNRAS
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- Extremely-bright submillimeter galaxies beyond the Lupus-I star-forming region
- IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
- Sequential Star Formation in the filamentary structures of Planck Galactic cold clump G181.84+0.31
- Astronomical imaging Fourier spectroscopy at far-infrared wavelengths
- The Sub-mm Variability of IRC+10216 and Ceti
- Deep Submillimetre and Radio Observations in the SSA22 Field. II. Sub-millimetre source catalogue and number counts
- The spatial correlation between CN line and dust continuum emitting regions in high-mass star-forming cloud
- Evolution of magnetized hub-filament systems: Comparing the observed properties of W3(OH), W3 Main, and S 106
- Discovery of two embedded massive YSOs and an outflow in IRAS 18144-1723
- Multiple component decomposition from millimeter single-channel data
- Twisted magnetic field in star formation processes of L1521 F revealed by submillimeter dual band polarimetry using James Clerk Maxwell Telescope
- Submillimeter continuum variability in Planck Galactic cold clumps
- A possible far-ultraviolet flux-dependent core mass function in NGC 6357
- The JCMT Gould Belt Survey Complete Core Catalogue: Core mass function variations between nearby molecular clouds
- Demonstration of wideband metal mesh filters for submillimeter astrophysics using flexible printed circuits
- The HASHTAG project: The First Submillimeter Images of the Andromeda Galaxy from the Ground
- The distances of 61 PGCCs in the Second Galactic Quadrant
- Submillimeter galaxy overdensities around physically associated quasar pairs
- The JCMT Transient Survey: Four Year Summary of Monitoring the Submillimeter Variability of Protostars
- Deuterium fractionation of the starless core L 1498
- The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields
- The JCMT Nearby Galaxies Legacy Survey: SCUBA-2 observations of nearby galaxies
- Tracing obscured galaxy build-up at high redshift using deep radio surveys
- Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
- Magnetic Fields Studies in the Next Decade: EAO Submillimetre Futures White Paper Series, 2019
- The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10
- Commissioning of Namakanui on the JCMT
- Demonstration of ultra-low noise equivalent power using a longitudinal proximity effect transition-edge sensor
- Optical Response of Lumped-Element Kinetic-Inductance Detector Arrays
- Optical and Near-IR Microwave Kinetic Inductance Detectors (MKIDs) in the 2020s
- Optimisation-based alignment of wideband integrated superconducting spectrometers for sub-mm astronomy
- Performance-centric roadmap for building a superconducting quantum computer
- Broadband anti-reflection coating for sub-terahertz optics using dielectric multilayers
- Performance of the polarization leakage correction in the PILOT data
- Correlating Visual Characteristics and Cryogenic Performance of Superconducting Detectors
- The General Single-Dish Data Format: A Retrospective
- The JCMT BISTRO Survey: The magnetised evolution of star-forming cores in the Ophiuchus Molecular Cloud interpreted using Histograms of Relative Orientation
- Direct Imaging for the Debris Disk around Eridani with the Cool-Planet Imaging Coronagraph
- Studies of Evolved Stars in the Next Decade: EAO Submillimetre Futures White Paper Series, 2019
- First direct search for light dark matter interactions in a transition-edge sensor
- Cloud G074.11+00.11: a stellar cluster in formation
- The impact of the presence of water ice on the analysis of debris disk observations
- The Galaxy Evolution Probe
- The role of radiative torques in the molecular cloud core L43
- An S-shaped filament formed due to Cloud-Cloud Collision in molecular cloud G178.28-00.61
- Low-dimensional platforms for single photon detection
- Time-domain deep learning filtering of structured atmospheric noise for ground-based millimeter astronomy
- Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective
- The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
- Far-infrared observations of dust in Ly emitters at z=2-6
- Implementing Remote Observing at the JCMT