A history of the warfare of science with theology in christendom /

Includes bibliographical references and index.

The popes and science; the history of the papal relations to science during the Middle Ages and down to our own time,

Mode of access: Internet.

American medical biography: or, Memoirs of eminent physicians who have flourished in America. To which is prefixed a succinct history of medical science in the United States, from the first settlement of the country.

Mode of access: Internet.

Calendar, History, and General Summary of Regulations of the Dept. of Science and Art

Mode of access: Internet.

The Canadian Naturalist and Quarterly Journal of Science with the Proceedings of the Natural History Society of Montreal

Title Varies: 1856-57, the Canadian Naturalist and Geologist. , the Canadian Naturalist and Geologist and Proceedings of the Natural History Society of Montreal. Conducted by a Committee of the Natural History Society; More

The Canadian Record of Science, Including the Proceedings of the Natural History Society of Montreal, and Replacing the Canadian Naturalist

Preceded by the Canadian Naturalist and Geologist (Called Later the Canadian Naturalist and Quarterly Journal of Science) 1856-83

Dunedin and its neighbourhood; a short account of its history, biology, and geology; and of the commerce and industries of Otago. A handbook for the use of members of the Australasian association for the advancement of science.

Mode of access: Internet.

Cyclopædia of political science, political economy, and of the political history of the United States,

First published, 1881.

Studies in the science and history of music.

Mode of access: Internet.

American medical biography, or, Memoirs of eminent physicians who have flourished in America to which is prefixed a succinct history of medical science in the United States from the first settlement of the country.

Reprint of the 1828 ed.

The ancient life-history of the earth. A comprehensive outline of the principles and leading facts of palæontological science.

Mode of access: Internet.

Recovery of the star formation history of the LMC from the VISTA survey of the Magellanic system

The VISTA near infrared survey of the Magellanic System (VMC) will provide deep YJK(s) photometry reaching stars in the oldest turn-off point throughout the Magellanic Clouds (MCs). As part of the preparation for the survey, we aim to access the accuracy in the star formation history (SFH) that can be expected from VMC data, in particular for the Large Magellanic Cloud (LMC). To this aim, we first simulate VMC images containing not only the LMC stellar populations but also the foreground Milky Way (MW) stars and background galaxies. The simulations cover the whole range of density of LMC field stars. We then perform aperture photometry over these simulated images, access the expected levels of photometric errors and incompleteness, and apply the classical technique of SFH-recovery based on the reconstruction of colour-magnitude diagrams (CMD) via the minimisation of a chi-squared-like statistics. We verify that the foreground MW stars are accurately recovered by the minimisation algorithms, whereas the background galaxies can be largely eliminated from the CMD analysis due to their particular colours and morphologies. We then evaluate the expected errors in the recovered star formation rate as a function of stellar age, SFR(t), starting from models with a known age-metallicity relation (AMR). It turns out that, for a given sky area, the random errors for ages older than similar to 0.4 Gyr seem to be independent of the crowding. This can be explained by a counterbalancing effect between the loss of stars from a decrease in the completeness and the gain of stars from an increase in the stellar density. For a spatial resolution of similar to 0.1 deg(2), the random errors in SFR(t) will be below 20% for this wide range of ages. On the other hand, due to the lower stellar statistics for stars younger than similar to 0.4 Gyr, the outer LMC regions will require larger areas to achieve the same level of accuracy in the SFR( t). If we consider the AMR as unknown, the SFH-recovery algorithm is able to accurately recover the input AMR, at the price of an increase of random errors in the SFR(t) by a factor of about 2.5. Experiments of SFH-recovery performed for varying distance modulus and reddening indicate that these parameters can be determined with (relative) accuracies of Delta(m-M)(0) similar to 0.02 mag and Delta E(B-V) similar to 0.01 mag, for each individual field over the LMC. The propagation of these errors in the SFR(t) implies systematic errors below 30%. This level of accuracy in the SFR(t) can reveal significant imprints in the dynamical evolution of this unique and nearby stellar system, as well as possible signatures of the past interaction between the MCs and the MW.

Charles Darwin goes to school: the role of cartoons and narrative in setting science in an historical context

Science education is under revision. Recent changes in society require changes in education to respond to new demands. Scientific literacy can be considered a new goal of science education and the epistemological gap between natural sciences and literacy disciplines must be overcome. The history of science is a possible bridge to link these `two cultures` and to foster an interdisciplinary approach in the classroom. This paper acknowledges Darwin`s legacy and proposes the use of cartoons and narrative expositions to put this interesting chapter of science into its historical context. A five-lesson didactic sequence was developed to tell part of the story of Darwin`s expedition through South America for students from 10 to 12 years of age. Beyond geological and biological perspectives, the inclusion of historical, social and geographical facts demonstrated the beauty and complexity of the findings that Darwin employed to propose the theory of evolution.