|Dr. Matthew Kenworthy is an associate professor at Leiden Observatory in the Netherlands. His research is on the direct imaging of extrasolar planets around nearby stars using the world's largest telescopes. More recently, he has become interested in searching for the transit of giant ring systems around exoplanets.|
|Dr. Hans Moritz Günther received his undergraduate degree in Physics from the University of Hamburg, Germany, with a thesis on accretion signatures in T Tauri stars. He expanded that research for his PhD at the same institution. He also started to work on Roman river warships at that time. In 2010, Dr. Günther came to the U.S. as a Post-Doc, and is now a staff researcher at MIT. He is an active contributor to the development of astronomical software, and maintains the ray-tracing code for the Chandra X-ray observatory.|
|Melanie Crowson is the education director for the Pisgah Astronomical Research Institute. A recent graduate from American Public University in spring 2020 with a Masters of Science degree in astronomy and space studies, with honors. She's the former Vice Chair of the Board for SEDS USA, and Darrell Cain award recipient of 2017, as well as AAVSO Ambassador. An active participant in research projects on variable stars, with a passion for astronomy starting from childhood and fostered through years of homeschooling. Melanie's interest in stars was solidified when she built a telescope with her dad.|
|Dr. Sarah Antier is an astrophysicist at Laboratoire Astroparticule et Cosmologie (Paris, France). She is member of the Virgo collaboration and PI of the GRANDMA collaboration.|
|Dennis Conti is currently Chair of AAVSO’s Exoplanet Section. He is author of “A Practical Guide to Exoplanet Observing” (see www.astrodennis.com), has spoken at various amateur astronomy clubs on the subject, published articles in Astronomy and Discover magazines, and conducted workshops and online courses on exoplanet observing. In addition, Dennis is currently a member of the TESS exoplanet follow-up team; as the liaison between the AAVSO and TESS, he qualified a number of citizen astronomers to be official TESS ground-based observers.|
|Dr. Luisa Rebull is a research astronomer at the NASA/IPAC Infrared Science Archive (IRSA) at Caltech. Ever since she was very little, she has always wanted to be an astronomer. She earned her undergraduate degree in physics from the College of William and Mary in Virginia, and her graduate degrees in astronomy and astrophysics from the University of Chicago. She has been on the science staff at IPAC since 2002. Her research focuses on the formation of young, low-mass stars (stars ~1 to 50 million years old) all over our Galaxy, and in understanding how stellar rotation changes over the first billion years of a star’s life.|
|Dr. Margarita Karovska (Center for Astrophysics | Harvard & Smithsonian) is an astrophysicist who has worked on variable stars for many years (starting with her PhD Thesis on Betelgeuse). She has studied LPVs (and their companions) using ground- and space-based multi-mission observations at wavelengths ranging from X-ray & UV-optical to radio. Key to the success of these studies include the AAVSO long-term observations and monitoring of LPVs, and the supporting observing campaigns on specific objects, including several symbiotic systems containing LPVs with hot accreting companions.|
|Dr. Barbara Harris is a retired physician who has been interested in astronomy since high school. She got my first CCD camera in 1999 and decided she wanted to put her CCD camera to work by doing science, so she learned CCD photometry. She added DSLR photometry in 2015 as a method to measure bright stars.|
|Dr. Steve B. Howell is a senior research scientist at the NASA Ames Research Center in Mountain View, California. He was formerly the Head of Space Science and Astrobiology for the NASA Ames Research Center, and the project scientist for NASA's premier exoplanet finding missions: Kepler and K2. Steve received his PhD in Astrophysics from the University of Amsterdam, and has worked in many aspects of astronomy, including pioneering the use of charge-coupled devices in astronomy; building new technology instruments for ground and space-based telescopes; and university research, education, and public outreach programs. Howell wrote over 800 scientific publications and numerous popular and technical articles. He also authored and edited nine books on astronomy and astronomical instrumentation, and wrote two science fiction books related to exoplanets.|
|Professor Echevarría is a well known astronomer in the field of cataclysmic variables. He has written around fifty peer reviewed articles in his field and has also collaborated on around twenty-odd publications in other fields, like interstellar matter, planetary nebulae, cellar formation regions, open clusters, blazars, and neutron star pulsar binaries. He has worked closely with the AAVSO for several decades, in particular to try to detect dwarf novae during the early stages of outburst.|
|Dr. David Whelan is an astronomer, and a professor in the Physics Department at Austin College in Sherman, Texas. Along with two of his students, Megan Frank and Jessica Junginger, he pursued the classification of Algol C in the Fall of 2020, using the Adams Observatory at Austin College.|
Lauren Herrington is an amateur astronomer with a passion for teaching. As a young teenager, she fell in love with spectroscopy after reading A Grand and Bold Thing. Too young to have access to any of the standard equipment, Lauren believed that recording spectra of her very own was a distant, expensive, and exclusive dream—until she discovered that she could do it with her backyard dobsonian! Lauren has been working to perfect her drift scanning method ever since, all while posting educational materials on her website to help other wannabe-spectrographers record their own spectra on a budget. Lauren is an AAVSO Ambassador, and works for the AAVSO as webinar coordinator.
AAVSO's Short Period Pulsator (SPP) Observing Section is comprised of AAVSO observers who are passionate about observing stars that pulsate with periods from minutes to a few weeks.
Why should we observe these stars? For many reasons, including the period-luminosity relation of certain classes of pulsating stars allows them to be used as distance indicators. As we refine our understanding of this relation, it necessitates slight adjustments in the entire cosmic distance ladder.Two, we can see stellar evolution in the making: some stars show changes that could be evidence of the star evolving off the main sequence. Many changes that occur in the pulsational period of these objects are active research areas.
The SPP section aims to provide AAVSO observers with a wide variety of targets that will provide a range of challenges, and result in data that is useful to researchers when submitted to AAVSO's databases. For more information on the SPP section, please visit https://www.aavso.org/aavso-short-period-pulsator-section.
Dr. Adam Burgasser is a professor of physics at the University of California, San Diego, and director of the Cool Star Lab. He is an observational astrophysicist who studies the lowest-mass stars, brown dwarfs, and extrasolar planets. Adam is a specialist in stellar spectroscopy, low-mass binary systems, and stellar magnetic emission. In addition to his astronomical research, he conducts physics education research on metacognitive skill development, participates in art-science collaboratories, and works to address barriers to equity and inclusion in the practice of science.
|Dr. Boris Gänsicke grew up in Berlin during the cold war (the first question he usually gets asked is “on which side?”), where he also earned a degree in Physics. During his PhD work in Göttingen, he developed an enduring passion for cataclysmic variables, and began working with variable star observers. He later moved to the UK, eventually settling in the Midlands, where he helped set up the Astronomy group at the University of Warwick. His research remains focused on “white dwarfs with and without things going around them,” which these days include stars, brown dwarfs, other white dwarfs, and planets.|
|Bob Buchheim has been an amateur astronomer since childhood (his first telescope was a 2.5 inch Sears refractor). In the late ‘80’s he was introduced to CCD photometry, which dramatically changed his emphasis from visual deep-sky observing to photometry of asteroids and variable stars (and a recent addition: spectroscopy). He has been an AAVSO member for about a decade, and is currently on the AAVSO Board. He has submitted photometric measurements of pulsating and eclipsing variable stars, EB timing measurements, spectra of variable stars, and has participated in a few special campaigns (e.g. the M-31 “Hubble variable" campaign and the recent “b Per eclipse" campaign). He was part of the team that prepared the first draft of the DSLR observing manual, and is the author of two books describing research and education projects for small telescopes.|
|François Cochard is a French amateur astronomer and co-founder and manager of Shelyak Instruments. He was deeply involved in in the design and the manufacturing of instruments that are today considered standards: Lhires III, LISA, eShel, Alpy 600, and UVEX. As the organizer of the Spectro Star Party every year at the Observatoire de Haute Provence (OHP), he assisted a lot of observers in their first steps in spectroscopy. He is also the author of the book Successfully Starting in Astronomical Spectroscopy: A Practical Guide.|
|Trevor Dorn-Wallenstein is a sixth year graduate student at the University of Washington. His Ph.D. thesis focuses on utilizing new methods to constrain the structure and evolution of massive stars. In particular, he uses machine learning models to classify massive stars, then leverages these classifications to develop diagnostics to infer the impact of binary interactions on the evolution of stars as a function of their host environment. Recently, he has been using data from the TESS mission to probe the interiors of aging massive stars. Outside of his work, Trevor is a member of Seattle's best and only all-astronomer rock band, Night Lunch.|
|Dr. Burçin Mutlu-Pakdil is an observational astrophysicist at the University of Chicago. She is a lead member of several large-scale imaging surveys and uses observations of small and faint (dwarf) galaxies to study the smallest dark matter halos and how they get populated with stars. Her work has been recognized by several prestigious awards. She was honored as a 2018 Ted Fellow and 2020 TED Senior Fellow, featured in National Geographic as a “woman of impact,” named an AAAS IF/THEN Ambassador, and featured in a Science Friday film documentary, “Breakthrough: Portraits Of Women In Science.”|
|Richard Berry is an author, editor, telescope maker, observer, and astro-imager. He's built a variety of his own observatories and observed from many built by others. He is currently working on an observatory for his new home.|
|Dr. Dan Milisavljevic of the Supernova Early Warning System (SNEWS) Team is an Assistant Professor in the Department of Physics and Astronomy at Purdue University. He completed his undergraduate degree in liberal arts at McMaster University; masters degree in philosophy at the London School of Economics, under a Commonwealth Fellowship; and PhD in physics and astronomy at Dartmouth College. He's held research positions at Harvard University and the Smithsonian Astrophysical Observatory. Milisavljevic's research interests include multi-messenger signals of astrophysical transients discovered via time-domain surveys; autonomous AI-directed coordination of global observing facilities; the explosion mechanisms, progenitor stars, and compact object remnants of supernovae; massive star mass loss; and the formation and destruction of dust and molecules.|
|Tom Calderwood is head of the AAVSO Photoelectric Photometry Observing Section. He observes from Central Oregon, and is the author of "The Great Dimming of Betelgeuse" in the March 2021 issue of Sky and Telescope. A graduate of MIT in mathematics, he is a retired software engineer who worked on parallel processing computers, communication networks, video games, and the data system for the Chandra X-ray Observatory.|
Stay tuned for more!