Digitizing Olin Eggen's Legacy
Quick link: want to get involved? Visit the Eggen Data Project Google group !
Introduction
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Photo credit: Olin Eggen Photo Archive, AURA-O |
Olin Jeuck Eggen (July 9, 1919 – October 2, 1998) received his Ph.D. in astrophysics from the University of Wisconsin (Madison) in 1948, working with Joel Stebbins and Albert Whitford on the light curves of Algol. His seminal paper in 1962 with Lynden-Bell and Sandage ("Evidence from the Motions of Old Stars that the Galaxy Collapsed") is his most cited paper (both Lynden-Bell and Sandage later were awarded the Bruce medal by the ASP, partly based on this paper). Eggen also introduced the concept of moving (or kinematic) groups of stars. Eggen moved to the Southern Hemisphere in 1966, assuming Directorship of Mt. Stromlo Observatory and pursuing the development of the AAT large reflector. He moved to Cerro Tololo Inter-American Observatory (CTIO) in 1977 where he stayed until he passed away 20 years later.
Olin Eggen was a vice-president of the RAS and a life member of the ASP. He was awarded the American Astronomical Society Henry Norris Russell Lectureship in 1985 and the Pawsey Memorial Lectureship of the Australian Institute of Physics. The Australian National University established a scholarship program in his honor, and the library at CTIO now bears his name.
He was an extremely prolific researcher, publishing some 400 papers during his 50-year career, with articles being written up until his death in 1998 from a heart attack. He was well known as a careful researcher, never observing unless it was perfectly clear, and always substantiating any claim he made in a paper. Eggen was also well known as a proponent of small-telescope science.
However, Eggen published only a small part of the enormous amount of data he collected over his lifetime. The AAVSO is most interested in this untapped resource. All of his observations were handwritten onto index cards that he kept in his office. Often, when a visitor would ask a question about a star, he would look up the coordinates, go to his card file, and retrieve observations that he had made of that target.
In early 2007, we made contact with CTIO to find out what had happened to that card catalog, mainly because we were interested in some observations that Eggen had made on a variable star but had never published. CTIO had taken the cards out of Eggen's office upon his passing, and had placed them in storage at La Serena. Since they were not serving any useful purpose in storage, CTIO Director Alistair Walker gave the AAVSO the entire collection of 78,000 cards on long-term loan.
The AAS helped with a Small Research Grant in 2007 to pay for the equipment to scan the cards. John Menke has given a grant for the publishing of the scans.
Over the past three summers, we have had summer assistants scan these cards, and are happy to report today that each and every card has been scanned! This web page contains links to all of the scanned images in PDF format.
Card Contents
The cards are all handwritten, and were a combination of detailed archives of photometry of individual stars, as well as miscellaneous cards containing scribbled notes. No two cards are in identical format, though some aspects are reasonably consistent.
Below is a "typical" card, for the star HD107814, also known as TT Crv. Its 1950 coordinates are listed as 12:20:43.96 -11:32:05.4 in Simbad, with B=8.122 and V=6.501. This is a semiregular variable, spectral type M3III, referenced by Eggen in PASP 88, 426, 1976. It's listed in VSX as having a magnitude range of 6.47 to 6.57 in V. Many periods from 15.4 to 182.8 days have been discovered in this star. However, if you look at the AAVSO International Database, only a handful of visual estimates are available for this star, and it's too bright for ASAS. Accompanying the image of Eggen's card for this star is his published table of photometry from the 1976 paper mentioned above.
As you can see, the basic information regarding the coordinates is given in 1966 coordinates (basically, coordinates of date, useful for old-style telescopes), along with magnitudes, colors, and dates.
"VE" stands for "Eggen V," which is actually "Johnson V." Nicholas Suntzeff explained to me that "Olin once got into an argument with a referee over the magnitude system he was using. The referee did not believe Olin's calibration and niggled him over this. So Olin, instead of carefully reasoning with the referee, just decided to call his magnitude VE and be done with it."
You Can Help!
There are two remaining phases of this project. First, to make the cards even partially usable, we need to catalog the contents. Perhaps there is an RA order. Perhaps the order is by year of observation. Perhaps there is no order! However, each PDF file has 20 or so cards, and identifying the star names in each scan will enable a researcher to go to a specific PDF file for information on a star that they are studying. If people will pick a "box" or "bundle", and give us a listing of the contents of a box/bundle/PDF, we can create a master index.
For the final phase, we want to take as many cards as possible and digitize the data. This will be more difficult, as you need to interpret the handwriting and what each figure means. However, if we can get volunteers to adopt bundles and give us back all of the information contained in that bundle, we'll be finished with the project!
Arne Henden
September 1, 2009
Index of Eggen Cards
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