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AzTEC millimetre survey of the COSMOS field – I. Data reduction and source catalogue
Scott, K. S.,Austermann, J. E.,Perera, T. A.,Wilson, G. W.,Aretxaga, I.,Bock, J. J.,Hughes, D. H.,Kang, Y.,Kim, S.,Mauskopf, P. D.,Sanders, D. B.,Scoville, N.,Yun, M. S. Blackwell Publishing Ltd 2008 MONTHLY NOTICES- ROYAL ASTRONOMICAL SOCIETY Vol.385 No.4
<P>ABSTRACT</P><P>We present a 1.1 mm wavelength imaging survey covering 0.3 deg<SUP>2</SUP> in the COSMOS field. These data, obtained with the AzTEC continuum camera on the James Clerk Maxwell Telescope, were centred on a prominent large-scale structure overdensity which includes a rich X-ray cluster at <I>z</I>≈ 0.73. A total of 50 mm-galaxy candidates, with a significance ranging from 3.5 to 8.5σ, are extracted from the central 0.15 deg<SUP>2</SUP> area which has a uniform sensitivity of ∼1.3 mJy beam<SUP>−1</SUP>. 16 sources are detected with S/N ≥ 4.5, where the expected false-detection rate is zero, of which a surprisingly large number (9) have intrinsic (deboosted) fluxes ≥5 mJy at 1.1 mm. Assuming the emission is dominated by radiation from dust, heated by a massive population of young, optically obscured stars, then these bright AzTEC sources have far-infrared luminosities >6 × 10<SUP>12</SUP> L<SUB>⊙</SUB> and star formation rates >1100 M<SUB>⊙</SUB> yr<SUP>−1</SUP>. Two of these nine bright AzTEC sources are found towards the extreme peripheral region of the X-ray cluster, whilst the remainder are distributed across the larger scale overdensity. We describe the AzTEC data reduction pipeline, the source-extraction algorithm, and the characterization of the source catalogue, including the completeness, flux deboosting correction, false-detection rate and the source positional uncertainty, through an extensive set of Monte Carlo simulations. We conclude with a preliminary comparison, via a stacked analysis, of the overlapping MIPS 24-μm data and radio data with this AzTEC map of the COSMOS field.</P>
Design of a Track-Leg Hybrid Locomotive Mobile Robot
K. N. M. Perera,D. L. F. M. Liyanage,P. V. K. Asanka,D. N. Rajapaksha,Y. W. R. Amarasinghe,R. A. R. C. Gopura,S. A. Nanayakkara 제어로봇시스템학회 2020 제어로봇시스템학회 국제학술대회 논문집 Vol.2020 No.10
The use of robotic platforms for operations in harsh and high risk environments such as mining sites has become more popular with the advancements within the field of mobile robotics. In this paper, the designing of a hybrid locomotive mobile platform that utilizes both tracked locomotion and legged-like movements to achieve mobility is presented. The proposed track-leg mechanism and power transmission methodology are discussed in detail along with the overall design framework. The functionality validation and analysis of the legged locomotion was done in a simulation environment using MSC ADAMS with open-loop track-leg velocity control. The designed mobile robot demonstrated the ability to traverse a flat terrain and overcome a semi-cylindrical obstacle without tipping over in the simulations for the selected gait. The mobile robot also consists of 3 degrees of freedom (DOF) robotic arm which facilitates total human replacement by enabling the ability to perform any sample collecting, inspecting, pick and place tasks. The design of the robotic arm is also presented within this paper.
Austermann, J. E.,Aretxaga, I.,Hughes, D. H.,Kang, Y.,Kim, S.,Lowenthal, J. D.,Perera, T. A.,Sanders, D. B.,Scott, K. S.,Scoville, N.,Wilson, G. W.,Yun, M. S. Blackwell Publishing Ltd 2009 Monthly notices of the Royal Astronomical Society Vol.393 No.4
<P>ABSTRACT</P><P>We report an overdensity of bright submillimetre galaxies (SMGs) in the 0.15 deg<SUP>2</SUP> AzTEC/COSMOS survey and a spatial correlation between the SMGs and the optical-IR galaxy density at <I>z</I>≲ 1.1. This portion of the COSMOS field shows a ∼3σ overdensity of robust SMG detections when compared to a background, or ‘blank-field’, population model that is consistent with SMG surveys of fields with no extragalactic bias. The SMG overdensity is most significant in the number of very bright detections (14 sources with measured fluxes <I>S</I><SUB>1.1 mm</SUB> > 6 mJy), which is entirely incompatible with sample variance within our adopted blank-field number densities and infers an overdensity significance of ≫ 4σ. We find that the overdensity and spatial correlation to optical-IR galaxy density are most consistent with lensing of a background SMG population by foreground mass structures along the line of sight, rather than physical association of the SMGs with the <I>z</I>≲ 1.1 galaxies/clusters. The SMG positions are only weakly correlated with weak-lensing maps, suggesting that the dominant sources of correlation are individual galaxies and the more tenuous structures in the survey region, and not the massive and compact clusters. These results highlight the important roles cosmic variance and large-scale structure can play in the study of SMGs.</P>