The James Webb Space Telescope Mission

Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized space telescope with an aperture of at least $4m$. With the support of their governments in the US, Europe, and Canada, 20,000 people realized that vision as the $6.5m$ James Webb Space Telescope. A generation of astronomers will celebrate their accomplishments for the life of the mission, potentially as long as 20 years, and beyond. This report and the scientific discoveries that follow are extended thank-you notes to the 20,000 team members. The telescope is working perfectly, with much better image quality than expected. In this and accompanying papers, we give a brief history, describe the observatory, outline its objectives and current observing program, and discuss the inventions and people who made it possible. We cite detailed reports on the design and the measured performance on orbit.Comment: Accepted by PASP for the special issue on The James Webb Space Telescope Overview, 29 pages, 4 figure

Upper Gastrointestinal (GI) pH in Young, Healthy Men and Women

The pH in the upper gastrointestinal tract of young, healthy men and women was measured in the fasting state and after administration of a standard solid and liquid meal. Calibrated Heidelberg capsules were used to record the pH continuously over the study period of approximately 6 hr. In the fasted state, the median gastric pH was 1.7 and the median duodenal pH was 6.1. When the meal was administered the gastric pH climbed briefly to a median peak value of 6.7, then declined gradually back to the fasted state value over a period of less than 2 hr. In contrast to the pH behavior in the stomach, feeding a meal caused a reduction in the median duodenal pH to 5.4. In addition, there was considerable fluctuation in the postprandial duodenal pH on an intrasubject basis. The pH in the duodenum did not return to fasted state values within the 4-hr postprandial observation period. There was no tendency for the duodenal pH to be related to the gastric pH in either the fed or fasted phases of the study. Furthermore, pH in the upper GI tract of young, healthy subjects appears to be independent of gender. The differences in upper GI pH between the fasted and the fed state are discussed in terms of dosage form performance and absorption for orally administered drugs.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/41548/1/11095_2004_Article_305803.pd

Upper Gastrointestinal pH in Seventy-Nine Healthy, Elderly, North American Men and Women

Gastric and duodenal pH levels were measured in 79 healthy, elderly men and women (mean ± SD = 71 ± 5 years) under both fasted and fed conditions using the Heidelberg capsule technique. The pH was recorded for 1 hr in the fasted state, a standard liquid and solid meal of 1000 cal was given over 30 min, then the pH was measured for 4 hr postprandially. Results are given as medians and interquartile ranges: fasted gastric pH, 1.3 (1.1–1.6); gastric pH during the meal, 4.9 (3.9–5.5); fasted duodenal pH, 6.5 (6.2–6.7); and duodenal pH during the meal, 6.5 (6.4–6.7). Although fasted gastric pH, fasted duodenal pH, and duodenal pH during the meal differ statistically from those observed in young subjects, the differences are not expected to be clinically significant in terms of drug absorption for the majority of elderly subjects. Following a meal, gastric pH decreased from a peak pH of 6.2 (5.8–6.7) to pH 2.0 within 4 hr in most subjects. This rate of return was considerably slower than in young, healthy subjects. Nine subjects (11%) had a median fasted gastric pH >5.0, and in five of these subjects the median pH remained >5.0 postprandially. In this group, drugs and dosage forms which require an acidic environment for dissolution or release may be poorly assimilated.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/41426/1/11095_2004_Article_304755.pd

The James Webb Space Telescope Mission

Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized space telescope with an aperture of at least 4 m. With the support of their governments in the US, Europe, and Canada, 20,000 people realized that vision as the 6.5 m James Webb Space Telescope. A generation of astronomers will celebrate their accomplishments for the life of the mission, potentially as long as 20 yr, and beyond. This report and the scientific discoveries that follow are extended thank-you notes to the 20,000 team members. The telescope is working perfectly, with much better image quality than expected. In this and accompanying papers, we give a brief history, describe the observatory, outline its objectives and current observing program, and discuss the inventions and people who made it possible. We cite detailed reports on the design and the measured performance on orbit