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Steward Regents' Professor Dave Arnett to Receive Honorary Degree from the University of Kentucky

Steward Regents' Professor Dave Arnett to Receive Honorary Degree from the University of Kentucky

The University of Kentucky Board will confer an honorary degree (Honorary Doctor of Science)  upon UA Astronomy/Steward Regents' Professor W. David Arnett. Dave is a native son of Kentucky, so it's probably an exceptional pleasure for him.  Congratulations, Dave!
We quote from the Kentucky press release: 
"Leaders in the areas of astrophysics; military and the law; food chemistry; and service to victims of sexual violence have been selected to receive honorary doctorates from the University of Kentucky at its Commencement ceremonies in May. An honorary degree pays tribute to those whose lives and work exemplify professional, intellectual, or artistic achievement and who have made significant contributions to society, the state and the University of Kentucky. Nominated by the University Joint Committee on Honorary Degrees and approved by the University Senate, the honorary degree recipients approved by the UK Board of Trustees today are: W. David Arnett, who will receive an Honorary Doctor of Science. One of the world's preeminent astrophysicists, Arnett grew up in Ballard County and began his college academic career as a physics major at UK. He went on to earn his doctorate at Yale University and later held academic positions at Rice University, the University of Texas, the University of Illinois and the University of Chicago. He currently is Regents' Professor at Steward Observatory at the University of Arizona where he continues to conduct research to bring further clarity to understanding the universe. Highly honored for his work in astrophysics — an area in which he has published more than 400 papers and a renowned scientific book — Arnett also has a physical law named for him. Arnett's Law describes how stars regulate energy transport as they explode..."

The Peter Wehinger Fellowship Fund

Steward Observatory Astronomer and Development Officer Peter Wehinger passed away on April 27, 2015. During his tenure at the UA (1995 to 2012), Peter helped advance major telescope projects and worked to support astronomy graduate students. Known for his work on comets and quasars, Peter previously held appointments in astronomy at the University of Michigan, Tel-Aviv University, the Royal Greenwich Observatory, the Max Planck Institute for Astronomy in Heidelberg, and Arizona State University. In 1967 Peter married Susan Wyckoff, herself an astronomer and longtime collaborator.

Peter was inspired to pursue a career in astronomy through his explorations of the sky, using his home-built telescopes, from his backyard in Goshen, New York. While in college he held summer appointments at the U.S. Naval Observatory, the Utrecht Observatory, and the Lowell Observatory. At the University of Michigan he oversaw the funding, design and construction in 1969 of a 1.3-m telescope located near Ann Arbor. Still in use and now named the McGraw-Hill Telescope, this facility has since been relocated to a mountain top site, Kitt Peak, Arizona, adjacent to the telescopes of the Kitt Peak National Observatory, where it is operated by the MDM Observatory Consortium.

While at Steward Observatory, Peter played major roles in establishing the Arizona Astronomy Board, creating the Mt. Lemmon Sky Center, obtaining initial funding for the LSST project, developing a collaboration with the Tokyo Atacama Observatory group, and assisting students in obtaining scholarship funds – to list a few of his accomplishments and contributions.

Peter greatly enjoyed teaching and working with students. He was particularly dedicated and successful in supporting the efforts of graduate students. Aligned with this strong interest of Peter’s and in his memory, a fund has been established to recognize graduate students in the Department of Astronomy with demonstrated records of exceptional or creative work. Sue Wyckoff has asked that those that would like to honor Peter's memory and legacy at Steward Observatory consider making a contribution to the University of Arizona Foundation in support of this fund. The contributed funds will be used to endow "Peter Wehinger Fellowships" in the Department of Astronomy, for the support of the educational and research activities of selected graduate students. Checks should be made payable to "University of Arizona Foundation", with a note on the memo/subject line of, For Wehinger Fund/Department of Astronomy and be sent to:

University of Arizona Foundation
1111 N. Cherry Avenue
P.O. Box 210109
Tucson, AZ 85721-0109

or online at https://uafoundation.org/netcommunity/donations/wehinger-fellowship-fund

Neither Rain Nor Sleet Nor Dark Of Night...

Neither Rain Nor Sleet Nor Dark Of Night...

While making tests of the JWST telescope instrument suite, the teams, including a contingent from UA (Stacey Alberts, Karl Misselt, and Lisa May Walker, among others over an extended period) were stranded at Goddard in a blizzard. HERE is an article from Atlantic. A NASA press release about the primary mirror completion is found HERE.

 

Finding the Progenitor of the Supernova in Cen A Using MagAO

Finding the Progenitor of the Supernova in Cen A Using MagAO

"A week ago (February 8), a bright supernova, SN 2016adj, appeared in the active galaxy NGC 5128 (Centaurus A). Classified as Type IIb, its progenitor is believed to be a very massive star in a binary system, undergoing a significant mass loss before explosion. However, direct identification of the progenitor remains challenging. Since SN 2016adj is only 4" from a bright foreground star, it is an ideal target for Arizona's Magellan Adaptive Optics system and its visible AO camera. Steward Observers Jared Males, Laird Close, and Katie Morzinski observed the supernova on February 13. Steward grad student Ya-Lin Wu compared the new MagAO image to archival HST and VLT data, and we were able to identify a possible progenitor star. Notably, this is the 5th Type IIb progenitor identified in pre-explosion images over the past 20 years. Yesterday we posted our results on the Astronomer's Telegram." You can find the link HERE and the blog from which these words were excerpted (with permission) HERE.

 
What SOFIA Observations Tell Us About Planetary Debris Disks

What SOFIA Observations Tell Us About Planetary Debris Disks

Steward Scientist Kate Su will be holding a press conference at the AAS meeting Jan 7. The title is "What SOFIA Observations Tell Us About Planetary Debris Disks." Here is the meeting abstract for her Friday AAS talk. We will have the press release when it's available.

Oral Talk: Nature of the Warm Excess in eps Eri: Asteroid belt or Dragged-in Grains
Kate Y. Su, George Rieke, Massimo Marengo, & Karl R. Stapelfeldt

Epsilon Eri and its debris disk provide a unique opportunity to probe the outer zones of a planetary system due to its young age (roughly 1 Gyr) and proximity (3.22 pc, the closest prominent debris disk by more than a factor of two). It is the Rosetta Stone for more distant exoplanetary debris systems and thus critical to understanding the mid-term evolution of our Solar System. From resolved images in the far-infrared and submillimeter along with spectra from 10-35 and 55-95 microns, the eps Eri disk was suggested to have a complex structure, with multiple zones in both warm (asteroid-like) and cold (KBO-like) components. Alternatively, the warm excess can also originate from small grains in the cold disk, which are transported inward by the combination of Poynting-Robertson and stellar wind drags. Here we present a SOFIA/FORCAST 35 micron image of the system, and provide additional constraints on the nature of the warm excess inferred from previous Spitzer and Herschel observations.

Invited AAS Talk on Event Horizon Telescope

Invited AAS Talk on Event Horizon Telescope

Professor Feryal Ozel gave a plenary talk at the American Astronomical Society Meeting on Jan 6, entitled "Black Hole Physics with the Event Horizon Telescope." The abstract of her talk follows:

The Event Horizon Telescope is an experiment that is being performed on a large and ever-increasing array of radio telescopes that span the Earth from Hawaii to Chile and from the South Pole to Arizona. When data will be taken with the full array, it will image the event horizons of the supermassive black hole at the center of our Galaxy, Sagittarius A*, and the black hole at the center of M87, with an unprecedented 10 microarcssecond resolution. This will allow us to take the first ever pictures of black holes at 1.3 and 0.85 mm wavelengths and look for the shadow that is a direct evidence for a black hole predicted by the theory of General Relativity. In addition, the Event Horizon Telescope will also enable us to study the process by which black holes accrete matter and grow in mass. I will discuss the theoretical developments in simulating the properties of the black hole accretion flows and their expected images using state-of-the-art algorithms and high performance computing. Interpreting the upcoming observations within this theoretical framework will open new horizons in black hole astrophysics.

You can read two accounts of her talk HERE and HERE.

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