We explore the cosmological implications of 7 deep survey fields observed at the Berkeley-IllinoisMaryland Association (BIMA) Array with 30 GHz receivers. These observations probe the Cosmic Microwave Background anisotropy on scales corresponding to l ∼ 5500, and an earlier analysis of these data detected no galaxy clusters. We use numerical cluster simulations and mock observations to characte...

We present a complete survey of CO (1 → 0) emission in the Local Group dwarf irregular IC 10. The survey, conducted with the BIMA interferometer, covers the stellar disk and a large fraction of the extended H I envelope with the sensitivity and resolution necessary to detect individual giant molecular clouds (GMCs) at the distance of IC 10 (950 kpc). We find 16 clouds with a total CO luminosity...

Arterial grafts are frequently used in modern coronary artery bypass grafting (CABG) and the benefit of the 2 internal mammary arteries (IMA) has already been established. However, the choice of the third arterial conduit, in addition to the IMA, is controversial. We have retrospectively analized perioperative and the follow-up results of patients who underwent CABG with triple arterial bypass ...

This study aims to analyze the influence of career development and work discipline on performance SMKN teachers in Bima city with motivation as an intermediary variable. The method used this is quantitative. number research resondents was 68 people who were selected proportionally sampling a total population 217 at city. Data collection using questionnaires. analysis techniques SmartPLS 3. resu...

BACKGROUND Bilateral internal mammary artery (BIMA) grafting in coronary artery surgery provides better long term outcomes than single internal mammary artery and saphenous vein grafting but the optimum configuration of BIMAs has not been established. This study analyzed perioperative and late outcomes of patients who underwent BIMA grafting with a composite Y configuration. METHODS Patients ...

The precision imaging to be attained by the ALMA will be achieved through accurate calibration. The types of calibration are summarized in Table 3.1. Calibration strategies will be developed and implemented on the NRAO 12m telescope, and the OVRO and BIMA arrays. The principal goals to be achieved by the end of the ALMA Design and Development (D&D) Phase are to demonstrate radiometric phase cor...

Measurements have been made of the temperature distribution in the antenna backing structures on the 6 m diameter antennas of the BIMA Array at Hat Creek. 32 thermistors were distributed around the backing structure and on one panel and were monitored under varying conditions. Significant gradients were found between the front and rear of the backing structure, across the structure, and radiall...

The variation of the overlap of the astronomical and water-vapor radiometer beams with height in the atmosphere is investigated for the current BIMA setup, and is compared with similar calculations for OVRO and a proposed system for ALMA. The findings are that at BIMA, the 3-mm and 1.3-cm beams essentially do not overlap above a height of 1 km. The linear separation of the beams is 35 m at a ze...

OBJECTIVE The aim was to evaluate the early outcome of off-pump coronary artery bypass grafting (OPCABG) with a bilateral internal mammary artery (BIMA) Y configuration graft to achieve total arterial myocardial revascularization. MATERIALS AND METHODS From October 2002 to December 2008, 208 patients (196 male and 12 female patients) underwent OPCABG by only using a BIMA Y configuration graft...

We present results from an observing campaign of the molecular content of the coma of comet C/1999 S4 (LINEAR) carried out jointly with the millimeter arrays of the Berkeley-Illinois-Maryland Association (BIMA) and the Owens Valley Radio Observatory (OVRO). Using the BIMA array in autocorrelation (‘‘single-dish’’) mode, we detected weak HCN J 1⁄4 1 0 emission from comet C/1999 S4 (LINEAR) at 14...