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408-238-9614, Tina Kurth

Greg Doppmann An Interest and/or experience with scientific instrumentation as well as experience observing and/or working at an astronomical observatory; must be capable of working effectively with visiting observers and coordinating multi-disciplinary instrument commissioning and maintenance teams. 408-238-0652, Michele Redel Sam plays a lead role in the Keck All-sky Precision Adaptive optics (KAPA) and the Keck Planet Imager and Characterizer (KPIC) projects. Sam was a major contributor to the development of the Keck Interferometer (KI) and served as the KI Operations Manager/Scientist of the during 2007-2012.

420 Waiakamilo Road, Suite 205Honolulu, HI 96817Main (808) 847-3246News (808) 847-1112. We operate the Lick Observatory, the UCO technical labs at UC Santa Cruz and UCLA, and we are a managing partner of the W. M. Keck Observatory in Hawaii. I worked as apost-doctoral researcher at the Max Plank Institut für Astronomie in Heidelberg (Germany) (2002 – 2004) on high spatial resolution observations of massive star forming regions. The two 10-meter telescopes of the W. M. Keck Observatory (WMKO) are located near the summit of Mauna Kea on the island of Hawaii, in the state of Hawaii. Building Maintenance Worker He worked with Prof. Brent Tully at the University of Hawai’i at Manoa on building the largest extragalactic distance database and mapping the largest superstructures in the Local Universe. Important Message from the Director about COVID-19. He has technical expertise in developing and maintaining the instrumentation of the observatory, in particular the laser guide star adaptive optics (LGSAO) used to remove image blur caused by atmospheric turbulence. and a Ph. And then here we are 25 years later. The nebulae are expanding at high velocities and the timing of the observations is vital since they are only bright enough to study for a few years, the blink of an eye in astronomical time scales. A full program description can be found here. Lewis was recruited in 1986 to lead the design and development of the software that controls Keck Observatory’s twin telescopes. 208-238-9619, Jesse Dolan

volunteer@ucolick.org, Adam Nichols Sam’s research interests include high spatial resolution studies of debris disks and disks surrounding young stellar objects, and high contrast imaging of exoplanets.The focus this year is to offer projects that are directly or indirectly related to the KAPA project.

Josh Walawender received B.A.s in Physics and Astrophysics from the University of California at Berkeley in 2000 and his Ph.D. from the University of Colorado at Boulder in 2006. Program Scientist, NASA, Robert McLaren, Interim Director For example, a Staff Astronomer who has interest and skills in software can focus more towards software development and working with WMKO’s Scientific Software group, while a Staff Astronomer with interest in hardware and instrumentation can focus on hands-on instrument work in conjunction with our instrument engineers and technicians. Keck Observatory gratefully acknowledges the Keck Visiting Scholars Program sponsors Roy and Frances Simperman and major contributors: the M. R. and Evelyn Hudson Foundation; the W. M. Keck Foundation; the Edge of Space Inc.; Tom Blackburn; John and Ann Broadbent; Bent and Candee Forbes; Carl and Marsha Hewitt; Doug Johnson and Valerie Gordon-Johnson; Andy and Worth Ludwick; Tom McIntyre; and Jeff Steele and Rebecca Miller Steele. Our well-supported workforce development … Josh has experience working on astronomical software such as data reduction pipelines, infrared instrumentation on large telescopes (e.g. Greg Doppmann received his BA and Ph.D. astronomy degrees from the University of Texas at Austin in 1994 and 2002. Our well-supported workforce development programs are perfect all students across disciplines as we offer positions in both STEM and non-STEM fields. Sr. Building Maintenance Worker Application Randy leads a team of scientists and operators that provide visiting astronomers with observing support for using the Keck telescopes. Elena did her PhD thesis at the Max Planck Institute for Astronomy (Heidelberg, Germany) between 2011 and 2015, in the field of Low-mass stars, Brown Dwarfs and Exoplanets.

The nebulae are expanding at high velocities and the timing of the observations is vital since they are only bright enough to study for a few years, the blink of an eye in astronomical time scales. Copyright 2020 Hawaii News Now. The W. M. Keck Observatory (WMKO) on the Big Island of Hawaii operates the world's two largest optical/infrared telescopes from the summit of Mauna Kea. The demonstrations on Mauna Kea aren't just personal for those hoping to stop construction, telescope workers say protests are preventing them from doing their job. As Director, Lewis is responsible for the operation and performance of W. M. Keck Observatory with its twin 10-meter optical/infrared telescopes, and for the development of new capabilities. His professional interests include leadership and motivation of high-tech teams, strategic planning, multiple-year plan design, and effective project planning and execution. Dr. Elena Manjavacas graduated in 2010 in Physics from the Universidad Complutense de Madrid (Spain).

Sherry has worked on the interactions between massive stars and their interstellar medium in extragalactic HII regions, understanding the stellar feedback mechanisms such as radiation pressure and stellar winds. Dr. Carlos Alvarez graduated in Solid State Physics from the Universidad del Pais Vasco (Spain) (1988 – 1994) and in Astrophysics from the Universidad de La Laguna (Spain) (1996 – 1998). Randy is member of the UCLA Galactic Center Group where he contributes TDA expertise and tools for three-dimensional visualization of data. EDUCATION OUTREACH: Shelly Pelfrey outreach@keck.hawaii.edu. Director, Caltech Optical Observatories, California Institute of Technology, Hashima Hasan, NASA Liaison Currently he is the instrument scientist for NIRES (Near-Infrared Echelette Spectrometer) mounted on Keck 2. Keck Observatory offers a robust rewards package which include a competitive salary; a broad benefits bundle including a 403(b) plan; a highly regarded tuition assistance program for dependent children (K-12 grade); and an unmatched focus of excellence. the FMOS, MOIRCS, and MOSFIRE instruments), small robotic telescopes, and citizen science projects. Institute for Scientist & Engineer Educators (ISEE). Read about us, our science and our mission, go to www.keckobservatory.org. in Physics from the Pontificia Universidad Catolica del Peru and M.S. W. M. Keck Foundation. Applicants living outside of the United States, who require a work visa sponsorship are not eligible for employment with our organization at this time under Proclamation 10014 signed by President Donald Trump. Candidates for this position are encouraged to think about how they might specialize. Staff Astronomers Percy Gomez received a B.S. Construction of the telescopes was made possible through private grants totaling more than $140 million provided by the W. M. Keck Foundation.

Would you like to join a high-performance team of like-minded scientists responsible for instrumentation and observing support at a renowned astronomical observatory, working with the biggest telescopes on the planet and residing in one of the world’s most uniquely beautiful and diverse locations?

While certain key job duties like night support are expected of all SAs, the numerous other job duties that exist allow each individual SA to grow and develop within their own area of emphasis. Gift Shop
Administrative Assistant Dr. Lyke’s research interests include classical novae. WMKO on the Big Island of Hawaii operates the world’s two largest optical/infrared telescopes from … LGSAO is a powerful technique that greatly improves image quality to realize the full potential of the world’s largest telescope. This research involves capturing the event at time the ejecta of these exploding stars enter the nubulous stage in order to better understand the astrophysical processes that power the nova phenomenon. Telescope Technician/Laser Technician The Staff Astronomers work primarily at the headquarters in Waimea, renowned as one of Hawaii’s most livable communities, and travel to the Maunakea summit for occasional work.

A description of the projects funded with our scholarships in 2018 can be found here. UC Observatories (UCO) is a multicampus astronomical research unit that serves eight UC campuses. Randy leads a team of scientists and operators that provide visiting astronomers with observing support for using the Keck telescopes. Josh’s research interests lie in the area of protostellar outflows and young stars.

I have an interest in a wide range of topics in Astrophysics, but in recent years I have become particularly interested in the study of Solar System objects.

408-238-4273, Elinor Gates Greg Doppmann received his BA and Ph.D. astronomy degrees from the University of Texas at Austin in 1994 and 2002. in Physics from the Pontificia Universidad Catolica del Peru and M.S. Randy Campbell is the Science Operations Lead Astronomer at the W. M. Keck Observatory , where is has been part of the staff for over 23 years. Before moving to W. M. Keck Observatory as a Support Astronomer in 2016 he was an Associate Scientist at  Gemini Observatory. Principal Telescope Technician/Mechanician Principle Telescope Technician In 2006, Greg moved to NOAO in Tucson where he began his research on planet formation by characterizing the dynamics and composition of inner disk regions (i.e., terrestrial planet-forming zones) surrounding protostars from high resolution L and M-band spectra and detailed fits to circumstellar model spectra. She started using the Keck Observatory atop Mauna Kea for research some 25 years ago. Submit a cover letter and resume telling us how your background and passion relate to the position.

Sam Ragland Sherry worked at Subaru Telescope as a NAOJ-Subaru Research Fellow from 2013 to 2016, and she joined W. M. Keck Observatory as a Staff Astronomer in 2017. in Astrophysics in 1997 and his Ph.D. in Astrophysics in 2003 from the University of Minnesota. Luca Rizzi received both his Laurea (undergraduate) and Ph.D. from the University of Padova, in Italy, in 1999 and 2003. She’s just the fourth woman ever to receive the award for Nobel Prize for Physics. Scientifically, Luca is interested in the field of resolved stellar population and in the use of simulated color-magnitude diagrams to retrieve the star formation and chemical enrichment histories of Local Group and Local Universe galaxies. As a graduate student, he was directly involved in infrared instrumentation, building two spectrographs and a dichroic speckle camera for the McDonald Observatory. Team members can allocated up to 20% of their time to active astronomical research. 408-238-9610, Gina Genovese Randy’s research is primarily in the study of classical novae, a type of cataclysmic variable star. Interior background photo © Vadim Kurland, licensed Creative Commons Attribution. Keck Observatory, where he is the instrument scientist for LRIS and KCWI.

Dr. Sherry Yeh received her Ph.D. in Astronomy and Astrophysics from the University of Toronto in Canada in 2013. Thursday-Sunday, 12-5 p.m. Public Programs Volunteer Coordinator

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