On Software in Astronomy

Importance of the Hubble archive. The number of archival papers has exceeded the number of PI-led papers since 2006 (from White et al., 2009)

ResearchBlogging.org
I’ve been giving some thought to software development in astronomy, which is a difficult topic. All astronomers agree that good data processing, and hence good software, is crucial to doing rigorous science. To interpret observational data, to translate electrons on a detector to scientific knowledge, requires a solid understanding of the instrument, the observing conditions, and of the exact process with which the data were treated. Many large ground- and space-based observatories, like those run by ESO, Gemini and NASA, strive to provide the community with “science-ready” data. This means that the data are processed to remove all instrumental signatures, allowing astronomers to dive straight into the analysis.

The rationale is that providing science-ready data essentially makes them usable by a much wider community than those involved in the observing campaign, or those used to working with a given instrument. Indeed, a big driver behind the global Virtual Observatory initiative is the “democratisation of astronomy” by providing anyone in the world with ready-to-use astronomical data, irrespective of their location or affiliation to large organisations.

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Bloggers and publishers team up

The post I just wrote on laser guide stars and magnetometers reminded me that I meant to write something about the recently announced collaboration between ResearchBlogging and Public Library of Science (PLoS). PLoS publishes several peer-reviewed journals in the biomedical science and provides open access to all the articles published. In an attempt to move away from journal impact factors in assessing the importance of a paper, PLoS make available a number of article-level metrics, such as ratings, citations, downloads. The most recent addition to these metrics is  the integration of the ResearchBlogging portal, to provide links to blog posts that scientists have written about the article, as an added way of measuring an article’s impact. To see how it works, watch the video below.

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Astronomers lead the pack on Arxiv

The growing success of Arxiv, 1991-2009 (Ingoldsby, 2009)

The growing success of Arxiv, 1991-2009 (arxiv.org)

How much of the research record in physics can actually be found on Arxiv? How accurately does Arxiv reflect what is happening in physics today? On the whole, not so well, says the American Institute of Physics. Over at the Scholarly Kitchen, Philip Davis reports on a presentation given at a science editors’ conference by Tim Ingoldsby of the AIP that shows a highly inconsistent coverage of the literature on Arxiv between the different fields of physics research. [Read more...]

Tweeting Arxiv

tweprintsFellow astronomer, blogger and developer Rob (@orbitingfrog) has put together a great new site in recent months that makes the most of two of my favourite places on the web, arxiv and Twitter. Arxiv on Twitter, or Tweprints for short, tracks all tweets about publications listed on arxiv, the online preprint service where many scientists post their new papers in a variety of sciences, including astronomy. Authors often post their work to arxiv before they are officially published by the journals, so it’s an excellent way to disseminate new results to the community more quickly than the time it takes a journal to publish (months sometimes).

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