Introducing Esther Hanko

Esther Hanko (@EstherHanko) is the local outreach coordinator of the Anton Pannekoek Institute for Astronomy of the UvA in Amsterdam, NL. She’s had an unconventional career path. After earning a master’s degree in Linguistics, she decided that an academic career was not for her and started working as a Linux system engineer in 2006. She worked for big companies like KLM (the Royal Dutch Airlines) but in 2015, she decided it was time for a change and started working for the API.

At the API, she organizes visits to the observatory. She also maintains much of the API website contents and the institute’s social media (@uva_api). One of her main goals is developing new audiences and finding ways to reach them. Another part of her job is maintenance of the observatory telescopes, working closely with a master student, in order to keep the students’ observing projects running smoothly.

She has been an amateur astronomer since 2012, after seeing an image of Io casting its shadow on Jupiter and realizing that she was now a grown up and could actually just buy herself a telescope. She also dabbles in no-telescope astrophotography, and shares her work online. She loves to write about her astronomy adventures and blogs about it in Dutch on her website oetie.nl. In her spare time, she is one of the moderators on the Dutch astronomy forum astroforum.nl, where one of her tasks is to help pick and write about the “Object of the Month”, a shared observing challenge.

She is passionate about creating awareness about light pollution, promoting the art of astronomical sketching, and teaching anyone who will listen to her that the skies are closer than you think.

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Introducing John Noonan

John Noonan (@J_Noons) is a graduate student at the University of Arizona’s Lunar and Planetary Laboratory in Tucson, Arizona. For the last three and a half years he has worked on the European Space Agency Rosetta mission during its rendezvous and escort of the comet 67P/Churyumov-Gerasimenko. More specifically, John works on the spacecraft’s ultraviolet spectrograph, Alice. Comets are typically thought of as some of the least altered objects from the beginning of the solar system, and their study helps bring planetary scientists as close as possible to this mysterious time. The ultraviolet realm of the electromagnetic spectrum is particularly useful for studying atomic and small molecular abundances, which is ideal for figuring out the formation location and thermal history of a comet.

John lived the vast majority of his life in the mountains of Colorado before moving to Boulder, Colorado to study Integrative Physiology at the University of Colorado, Boulder. Quickly after attending his first microbiology class he changed his major to astrophysics and graduated in 2016 summa cum laude. After graduation John continued to work on the Rosetta mission as well as a flight controller for NASA’s CYGNSS mission at the Southwest Research Institute. John moved to Tucson in August 2017 to begin his Ph.D. at the Lunar and Planetary Laboratory. You can find John riding his bike the vast majority of the time, which he finds to be the best stress therapy around.

Introducing James Davenport

James Davenport (@jradavenport) is a NSF Astronomy & Astrophysics postdoctoral fellow at Western Washington University, and a research fellow at the University of Washington’s new DIRAC Institute. His research is focused on stars, magnetic activity, flares, and starspots. He primarily uses data from the NASA Kepler and K2 missions, and is currently working on projects involving upcoming data releases from Gaia and ZTF.
For the past 5 years, Davenport has run a demographics survey of the annual AAS meetings that studies the gender dynamics of conference talks and Q/A periods. This work has found that men ask nearly twice as many talks as women in conference settings. However, the study is currently looking at ways to help level the playing field for all conference attendees. See this link for more details. (http://jradavenport.github.io/gender_study/)
Davenport currently maintains a monthly newsletter highlighting the latest in academic SETI research (http://seti.news), and is the author of the data, science, and visualization blog If We Assume (http://www.ifweassume.com). He earned his PhD from the University of Washington in 2015.

Introducing Rachael Ainsworth

Rachael Ainsworth (@rachaelevelyn) is a Research Associate at the Jodrell Bank Centre for Astrophysics (JBCA) at the University of Manchester. Her expertise lies in the interpretation of radio emission from protostellar systems in nearby star forming regions, particularly at very long (metre) wavelengths. Her primary research interests include astrophysical jets/outflows, star formation and evolution. She works on the Horizon 2020 RadioNET “Radio Interferometry Next Generation Software” (RINGS) project to develop software for calibrating dispersive delay corrections in long baseline radio interferometry for long wavelength telescopes such as the Low Frequency Array (LOFAR).

She is Open Science Champion for the Interferometry Centre of Excellence at JBCA, where she promotes, advocates and organises events relating to open science in astronomy. She is also a Mozilla Open Leader running the open project Resources for Open Science in Astronomy (ROSA), which aims to compile and tailor open science best practices from around the web into a toolkit for astronomers to work openly from proposal to publication. This project seeks input from the entire astronomy community, so feel to bookmark https://github.com/rainsworth/ROSA and become a contributor to the project in the coming weeks.

Rachael also organises the Manchester chapter of XX+Data (@xxplusdatamcr) – a community for women who work with and love data. The goal of the community is to bring together women with diverse expertise and experience to support one another, share experiences and talk data.

Introducing Ben Montnet

Ben Montet (@benmontet) is a NASA Sagan Fellow at the University of Chicago. He works to find and characterize planets with Kepler and K2, and soon, the upcoming TESS mission. He also uses Kepler data to better understand stellar activity through observations of long-term brightness variations of stars. (Ask him about KIC 8462852, or “Boyajian’s Star.”)
Ben is originally from the Chicagoland area, receiving his BS from the University of Illinois before heading to sunny California for his PhD at Caltech. When he’s not in the office, he enjoys traveling, watching the Cubs, and exploring his old and new hometown of Chicago.