Kimberly Kowal Arcand | |
---|---|
Born | Warwick, Rhode Island, U.S. | December 20, 1975
Alma mater | University of Rhode Island Brown University Harvard University University of Otago |
Spouse | John L. Arcand |
Children | 2 |
Scientific career | |
Fields | Data visualization Science communication |
Institutions | Smithsonian Astrophysical Observatory |
Thesis | Putting the stars within reach: NASA 3D data-based models in 3D print and virtual reality applications, and their potential effects on improving spatial reasoning skills and STEM interest in underrepresented groups of young female learners (2020) |
Doctoral advisor | Lisa F. Smith |
Website | www |
Kimberly Kowal Arcand (born December 20, 1975) is a data visualizer and science communicator for NASA's Chandra X-ray Observatory. [1] She is also the visualization coordinator for the Aesthetics and Astronomy image response project at the Center for Astrophysics | Harvard & Smithsonian [2] located in Cambridge, Massachusetts.
As a child, Arcand wanted to be an astronaut. [3] She studied molecular biology at the University of Rhode Island and also became a developer for the University of Rhode Island Center for Vector-Borne Disease Public Health project. [4] She was awarded a fellowship with the Rhode Island Public Health Partnership to work on Lyme disease. [5] Arcand studied briefly at the Harvard University Department between 2000 and 2002. [6] In 2013 Arcand earned a Master's degree in Public Humanities from Brown University, focusing on image and meaning research. [7] In 2020, Arcand completed her doctorate at the University of Otago in visualization science, under the supervision of Lisa Smith. [8] [9] She worked in the University of Rhode Island Department of Computer Science as an instructor between 1997 and 1999. [10] She joined the Smithsonian Astrophysical Observatory and Chandra X-ray Observatory in 1998. [6]
In 2009 Arcand launched From Earth to the Universe with UNESCO. [5] [12] She is the visualization coordinator of the Aesthetics and Astronomy image response project at the Center for Astrophysics | Harvard & Smithsonian. [13] The project launched in 2010 and looks at variations in the presentation of color and scale in astronomical images. The team also studies how people respond to images, and the misconceptions that non-experts have when they view them. [13] The project began when Randall, Jeffrey, and Lisa F. Smith realized that the art would provide astrophysicists a more effective way in conveying the results to a much larger audience. [14] The group explored the public perception of astronomical pictures using a survey linked to the NASA Astronomical Picture of the Day site. [15]
She worked closely with UNESCO to celebrate the International Year of Light, [16] an open-source exhibition that showcased science based on light. [17] The celebration was supported by SPIE. [16] Using NASA data, Arcand developed a way to 3D print a supernova remnant. [18] [19]
In 2016 the White House selected Arcand as a changemaker at the United State of Women Summit. [20] where she wrote about the event for HuffPost. [21] In 2017 Vinita Marwaha Madill's profiled her on Rocket Women. [22] Arcand also serves on the boards of Rhode Island Museum of Science and Art (RIMOSA). [23] and Rhode Island's Tech Collective. [24] In 2019, Arcand collaborated with the Smithsonian Institution to launch the "Journey through an Exploded Star” 3-D Interactive Experience website. [25]
Arcand has won several awards for her work from NASA and the Smithsonian Institution.
Arcand has written several popular science books. Her book Colouring the Universe was selected by Cosmos as one of the Top Illustrated Science Books of 2016. [30] She collaborates with Megan Watzke and Travis Rector, Ph.D. [31] Her book Light: The Visible Spectrum and Beyond was selected by Forbes as one of the Top 10 Gifts of 2016. [32]
The Chandra X-ray Observatory (CXO), previously known as the Advanced X-ray Astrophysics Facility (AXAF), is a Flagship-class space telescope launched aboard the Space ShuttleColumbia during STS-93 by NASA on July 23, 1999. Chandra is sensitive to X-ray sources 100 times fainter than any previous X-ray telescope, enabled by the high angular resolution of its mirrors. Since the Earth's atmosphere absorbs the vast majority of X-rays, they are not detectable from Earth-based telescopes; therefore space-based telescopes are required to make these observations. Chandra is an Earth satellite in a 64-hour orbit, and its mission is ongoing as of 2024.
The Harvard College Observatory (HCO) is an institution managing a complex of buildings and multiple instruments used for astronomical research by the Harvard University Department of Astronomy. It is located in Cambridge, Massachusetts, United States, and was founded in 1839. With the Smithsonian Astrophysical Observatory, it forms part of the Center for Astrophysics | Harvard & Smithsonian.
NASA's series of Great Observatories satellites are four large, powerful space-based astronomical telescopes launched between 1990 and 2003. They were built with different technology to examine specific wavelength/energy regions of the electromagnetic spectrum: gamma rays, X-rays, visible and ultraviolet light, and infrared light.
The Smithsonian Astrophysical Observatory (SAO) is a research institute of the Smithsonian Institution, concentrating on astrophysical studies including galactic and extragalactic astronomy, cosmology, solar, earth and planetary sciences, theory and instrumentation, using observations at wavelengths from the highest energy gamma rays to the radio, along with gravitational waves. Established in Washington, D.C., in 1890, the SAO moved its headquarters in 1955 to Cambridge, Massachusetts, where its research is a collaboration with the Harvard College Observatory (HCO) and the Harvard University Department of Astronomy. In 1973, the Smithsonian and Harvard formalized the collaboration as the Center for Astrophysics | Harvard & Smithsonian (CfA) under a single Director.
The Center for Astrophysics | Harvard & Smithsonian (CfA), previously known as the Harvard–Smithsonian Center for Astrophysics, is an astrophysics research institute jointly operated by the Harvard College Observatory and Smithsonian Astrophysical Observatory. Founded in 1973 and headquartered in Cambridge, Massachusetts, United States, the CfA leads a broad program of research in astronomy, astrophysics, Earth and space sciences, as well as science education. The CfA either leads or participates in the development and operations of more than fifteen ground- and space-based astronomical research observatories across the electromagnetic spectrum, including the forthcoming Giant Magellan Telescope (GMT) and the Chandra X-ray Observatory, one of NASA's Great Observatories.
Cassiopeia A (Cas A) is a supernova remnant (SNR) in the constellation Cassiopeia and the brightest extrasolar radio source in the sky at frequencies above 1 GHz. The supernova occurred approximately 11,000 light-years (3.4 kpc) away within the Milky Way; given the width of the Orion Arm, it lies in the next-nearest arm outwards, the Perseus Arm, about 30 degrees from the Galactic anticenter. The expanding cloud of material left over from the supernova now appears approximately 10 light-years (3 pc) across from Earth's perspective. It has been seen in wavelengths of visible light with amateur telescopes down to 234 mm (9.25 in) with filters.
The Perseus cluster is a cluster of galaxies in the constellation Perseus. It has a recession speed of 5,366 km/s and a diameter of 863′. It is one of the most massive objects in the known universe, containing thousands of galaxies immersed in a vast cloud of multimillion-degree gas.
Bryan Malcolm Gaensler is an Australian astronomer based at the University of California, Santa Cruz. He studies magnetars, supernova remnants, and magnetic fields. In 2014, he was appointed as Director of the Dunlap Institute for Astronomy & Astrophysics at the University of Toronto, after James R. Graham's departure. He was the co-chair of the Canadian 2020 Long Range Plan Committee with Pauline Barmby. In 2023, he was appointed as Dean of Physical and Biological Sciences at UC Santa Cruz.
Amy J. Barger is an American astronomer and Henrietta Leavitt Professor of Astronomy at the University of Wisconsin–Madison. She is considered a pioneer in combining data from multiple telescopes to monitor multiple wavelengths and in discovering distant galaxies and supermassive black holes, which are outside of the visible spectrum. Barger is an active member of the International Astronomical Union.
The known history of supernova observation goes back to 1006 AD. All earlier proposals for supernova observations are speculations with many alternatives.
Lisa Jennifer Kewley is an Australian Astrophysicist and current Director of the Center for Astrophysics | Harvard & Smithsonian. Previously, Kewley was Director of the ARC Centre of Excellence for All Sky Astrophysics in 3-D and ARC Laureate Fellow at the Australian National University College of Physical and Mathematical Sciences, where she was also a Professor. Specialising in galaxy evolution, she won the Annie Jump Cannon Award in Astronomy in 2005 for her studies of oxygen in galaxies, and the Newton Lacy Pierce Prize in Astronomy in 2008. In 2014 she was elected a fellow of the Australian Academy of Science. In 2020 she received the James Craig Watson Medal. In 2021 she was elected as an international member of the National Academy of Sciences. In 2022 she became the first female director of the Center for Astrophysics | Harvard & Smithsonian.
Somak Raychaudhury is an Indian astrophysicist. He is the Vice-Chancellor at Ashoka University and was the Director of the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune. He is on leave from Presidency University, Kolkata, India, where he is a Professor of Physics, and is also affiliated to the University of Birmingham, United Kingdom. He is known for his work on stellar mass black holes and supermassive black holes. His significant contributions include those in the fields of gravitational lensing, galaxy dynamics and large-scale motions in the Universe, including the Great Attractor.
SN 1979C was a supernova about 50 million light-years away in Messier 100, a spiral galaxy in the constellation Coma Berenices. The Type II supernova was discovered April 19, 1979 by Gus Johnson, a school teacher and amateur astronomer. This type of supernova is known as a core collapse and is the result of the internal collapse and violent explosion of a large star. A star must have at least 9 times the mass of the Sun in order to undergo this type of collapse. The star that resulted in this supernova was estimated to be in the range of 20 solar masses.
PSR J0108−1431 is a solitary pulsar located at a distance of about 130 parsecs (424 light-years) in the constellation Cetus. This pulsar was discovered in 1994 during the Parkes Southern Pulsar Survey. It is considered a very old pulsar with an estimated age of 166 million years and a rotation period of 0.8 seconds. The rotational energy being generated by the spin-down of this pulsar is 5.8 × 1023 W and the surface magnetic field is 2.5 × 107 T. As of 2008, it is the second faintest known pulsar.
Belinda Jane Wilkes is a Senior Astrophysicist at the Smithsonian Astrophysical Observatory (SAO) in Cambridge, Massachusetts, US, and former director of the Chandra X-ray Center.
Wanda Díaz-Merced is a Puerto Rican astronomer known for using sonification to turn large data sets into audible sound. Currently at the European Gravitational Observatory Cascina, Italy, Wanda is the Director of the Arecibo Observatory. While losing her eyesight, Wanda brought attention to increasing equality of access to astronomy and using audible sound to study astrophysical data.. Wanda is a part of the 7 most trailblazing women in science by the BBC.
Blakesley Burkhart is an astrophysicist. She is the winner of the 2017 Robert J. Trumpler Award awarded by the Astronomical Society of the Pacific, which recognizes a Ph.D. thesis that is "particularly significant to astronomy." She also is the winner of the 2019 Annie Jump Cannon Award in Astronomy and the 2022 winner of The American Physical Society's Maria Goeppert-Mayer Award. The awards both cited her work on magnetohydrodynamic turbulence, and for developing innovative techniques for comparing observable astronomical phenomena with theoretical models.
Alexey Vikhlinin is a Russian-American astrophysicist notable for achievements in the astrophysics of high energy phenomenon, namely galaxy cluster cosmology and the design of space-based X-ray observatories. He is currently a senior astrophysicist at the Smithsonian Astrophysical Observatory, part of the Center for Astrophysics | Harvard & Smithsonian in Cambridge, Massachusetts. He was recently the Science and Technology Definition Team (STDT) Community Co-chair for the Lynx X-ray Observatory, a NASA-funded Large Mission Concept Study under consideration by the 2020 Decadal Survey on Astronomy and Astrophysics.
Fabio Pacucci is an Italian theoretical astrophysicist and science educator, currently at Harvard University and at the Smithsonian Astrophysical Observatory. He is widely known for his contributions to the study of black holes, in particular the first population of black holes formed in the Universe and high redshift quasars. He discovered the only two candidate direct collapse black holes known so far, and he was in the team that discovered the farthest lensed quasar known. Pacucci is also a science educator, engaged in public talks on astronomy and science in general. Since 2018 he is a collaborator of TED in developing educational videos about science. The four videos released so far were watched by millions of people worldwide and translated into 25 languages.
Grant Tremblay is an American astrophysicist notable for research on supermassive black holes, science communication, and public advocacy for large space telescopes. He is currently an Astrophysicist at the Harvard-Smithsonian Center for Astrophysics, and was formerly a NASA Einstein Fellow at Yale University, a Fellow at the European Southern Observatory (ESO), and an Astronomer at ESO's Very Large Telescope (VLT).
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