Annual Report 2013 TABLE of CONTENTS

Total Page:16

File Type:pdf, Size:1020Kb

Annual Report 2013 TABLE of CONTENTS Annual Report 2013 TABLE OF CONTENTS Trustee's Letter....................................3 Director's Letter..................................4 Public Program Highlights..................5 Science Highlights..............................6 Peer-Reviewed Publications...............13 Conference Proceedings & Abstracts...18 Statement of Financial Position..........22 Photo Credits...................................25 Trustee’s Letter Lowell Putnam Trustee y remarks for 2013 are brief as MI only became Sole Trustee at the end of October. I would like to express my respect and admiration for the work of my father, Bill Putnam. As Sole Trustee for 26 years, his leadership and direction have raised the level of the observatory in so many ways. There is much challenge and opportunity ahead of us, but we have a strong base to grow on thanks to his efforts. We have a great staff, stronger participation by our Advisory Board and a growing group of supporters in the private sector. I am looking forward to 2014! ■ 3 Director's Letter Jeff Hall Director or a starting point for this letter in Bill Putnam retired after 26 years; a recently with the addition of a wildly FLowell Observatory’s 2013 Annual message from his son, and my new boss, popular suite of summer camps for Report, I took a quick look at what I accompanies this letter. pre-K and elementary school students. wrote last year. Here’s a short extract: One other thing we did was to The central tool of our profession is the “At the start of the DCT’s construction, convene a new Visiting Committee, telescope, and we have a real beauty of just three months after groundbreaking comprised of seven distinguished a new telescope. Our staff is incredibly at Happy Jack, we convened the Visiting astronomers and scientists, to pay us dedicated to the institution. We have a Committee that our Trustee Bill Putnam a visit for two days in September of skilled and committed Advisory Board refers to in his letter accompanying 2013 and provide an outside eye on our that is playing an increasingly prominent mine…the document the committee operations. As we head into 2014, we and diverse role in supporting our produced proved a thoughtful and are acting on their recommendations, mission. With these essentials in place, prescient guide that helped the addressing areas where they provided this institution has a bright future and Discovery Channel Telescope become a helpful and constructive criticism and it’s an honor to be part of it. ■ reality.” doing our best to leverage those areas By prescient, I was referring to the where they offered compliments, in Visiting Committee’s comment that particular the success of the DCT. I building the DCT would change every intend that in five years or so, when aspect of Lowell Observatory. It did, we convene the next such Committee, and you are holding the report of an they will also be able to look back institution in the midst of that profound through the current lens more clearly change. and compliment us on surmounting the Our new telescope is rapidly current challenges. coming on line, with almost 90 science On December 31, 2013, my family nights delivered in 2013 and 180 and I went down to the corner of Beaver planned for 2014. Our staff is growing, and Leroux in Flagstaff to watch the approaching 100 employees as of this annual pine cone drop. I remember writing, and further hires are needed. watching the last moments of the old Our suite of institutional partnerships year tick away and feeling happy and is growing, with Northern Arizona confident that we will surmount those University having joined Boston challenges, because the fundamentals University, the University of Maryland, are good. As you will see in the science and the University of Toledo in access highlights herein, our research is to DCT. Our operating budget is world-class. Our outreach programs increasing. And in late 2013 our Trustee are outstanding and growing, most 4 2013 Public Program Highlights n 2013, Lowell welcomed 75,410 Iguests through the doors of the Steele Visitor Center for public and private programs. Regularly scheduled daytime activities included grounds tours, hands-on presentations, science demonstrations, and solar viewing. Nighttime programming included telescope viewing, SlipherVision (our 3D portable digital planetarium) presentations, and stargazing. The Starry Skies Shop stayed open during public and private functions, as did the exhibit hall. Samantha Christensen, Education Coordinator, directed efforts to build on the success of the first summer day camps developed in 2012. For 2013, camp leaders included Lowell educators, student interns from Mesa Community College, and local Newly appointed Outreach Manager Samantha Christensen helped teach Tykes teachers from the Flagstaff Unified Camp participants about balance using mobiles. This was just one of the many School District. Professional (Lowell hands-on STEM (Science, Technology, Engineering, and Math) activities in which scientists) and amateur astronomers campers participated. also participated. In addition to these summer camps, the observatory added and circulated by SITES). Tykes Camps to the suite of STEM- In anticipation of closing the themed, activity-rich programming. Clark Telescope for much-needed These hands-on opportunities renovation, staff supplemented targeted youth ages three to five who, normal fundraising efforts to accompanied by a parent, learned financially support this effort with a fundamental scientific concepts during crowdsourcing project that generated two-hour programs. donations via the internet. Total Following removal of the fundraising efforts resulted in nearly outdated permanent exhibit in 2012, $300,000 raised for the renovation, we continued to use the main exhibit and the project is set to take place in hall to house several traveling exhibits, 2014-2015. including A New Perspective of Mars: In November, Kevin Schindler The Red Planet in 3D (created by the stepped down from his position as European Space Agency and DLR, the Outreach Manager to take on the new German Aerospace Center), Suited role of Communications Manager. for Space (created by the Smithsonian Samantha Christensen assumed the Institution Traveling Exhibition position of Outreach Manager. ■ Service (SITES) and the Smithsonian’s National Air and Space Museum), and The Evolving Universe (developed by the Smithsonian Astrophysical Observatory (SAO), the Smithsonian's National Museum of Natural History, 5 2013 Science Highlights Kevin Covey Last, but not least, I also had FLITECAM but also wrapped up some Over the past year, I have the pleasure and good fortune to remaining tests for HIPO. From my continued my research into the collaborate with Sarah Smith, a master's personal perspective the highlights were properties and environments of the student in Applied Physics at Northern two demonstration extrasolar planet youngest stars. Arizona University, who successfully transit observations and a series of My primary project is the INfrared defended her thesis in April. For tests aimed at understanding how to Survey of Young Nebulous Clusters her thesis, Sarah worked with me to get the best photometric precision we (IN-SYNC), a Sloan Digital Sky Survey calibrate near-infrared emission lines can manage with our instruments on ancillary science program that I am as accretion indicators for young T SOFIA. leading, along with key collaborators Tauri stars, deriving new results for We know from our previous work from ETH-Zurich (Michiel Cottaar several lines which had never been with the PSST planet search system & Michael Meyer), the University of calibrated for such heavily accreting and Kepler that precise photometry Florida (Jonathan Tan & Nicola Da stars. Sarah's analysis also suggests that doesn't come easily, and SOFIA has its Rio) and Yale University (Jonathan the relationships used to correct stellar share of troubles too. We have found Foster). With high-quality near-infrared spectra for the influence of dust may not that the star position on our CCD, spectroscopic data for thousands of apply to the youngest stars, a conclusion small focus changes, the outside air young stars in the Perseus and Orion that could have important implications density, ozone overburden (except at star-forming regions, the IN-SYNC for previous measurements of young blue and very red wavelengths), and team has provided the most accurate stars and star-forming regions. ■ the size of the area of sky around the measurements to date of the internal object we're observing are all important motions within each of these star Ted Dunham factors. Fortunately we can control forming regions, providing a critical test most of these and make measurements for theoretical models of the formation This year all the development, for the others that we can use to back and evolution of young clusters. These engineering, and test work we've put out their effects later. Although we data also reveal that stars in a single into HIPO and SOFIA since 1997 has are still working hard on all this, we've cluster with identical temperatures can finally borne fruit. In the last eight already reached a fractional noise level nonetheless vary in size by up to 25%, months, the HIPO team was finally of several hundredths of a percent with likely a signature of the different ages able to work in some science flights time resolution of a half minute or so, or magnetic properties of the stars in with SOFIA! Peter Collins, Georgi good enough to start doing useful work question. Much of this work, the final Mandushev, and I flew HIPO with that can't be done from the ground. component of Michiel Cottar's Ph.D. FLITECAM twice in September of Although SOFIA is working thesis, will be published this summer 2013, the last flight being the night really well and there are four SOFIA in two papers focusing on the young the Government shut down, and six instruments that have flown many cluster IC 348, with subsequent papers times in February 2014.
Recommended publications
  • Qatar Exoplanet Survey: Qatar-6B--A Grazing Transiting Hot Jupiter
    DRAFT VERSION JULY 2, 2018 Typeset using LATEX preprint2 style in AASTeX61 QATAR EXOPLANET SURVEY: QATAR-6B – A GRAZING TRANSITING HOT JUPITER KHALID ALSUBAI,1 ZLATAN I. TSVETANOV,1 DAVID W. LATHAM,2 ALLYSON BIERYLA,2 GILBERT A. ESQUERDO,2 DIMITRIS MISLIS,1 STYLIANOS PYRZAS,1 EMMA FOXELL,3, 4 JAMES MCCORMAC,3, 4 CHRISTOPH BARANEC,5 NICOLAS P. E. VILCHEZ,1 RICHARD WEST,3, 4 ALI ESAMDIN,6 ZHENWEI DANG,6 HANI M. DALEE,1 AMANI A. AL-RAJIHI,7 AND ABEER KH.AL-HARBI8 1Qatar Environment and Energy Research Institute (QEERI), HBKU, Qatar Foundation, PO Box 5825, Doha, Qatar 2Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 3Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK 4Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK 5Institute for Astronomy, University of Hawai‘i at Manoa,¯ Hilo, HI 96720-2700, USA 6Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang 830011, China 7Qatar Secondary Independent High School, Doha, Qatar 8Al-Kawthar Secondary Independent High School, Doha, Qatar (Received Oct 6, 2017; Revised Dec 4, 2017; Accepted Dec 5, 2017) Submitted to AJ ABSTRACT We report the discovery of Qatar-6b, a new transiting planet identified by the Qatar Exoplanet Survey (QES). The planet orbits a relatively bright (V=11.44), early-K main-sequence star at an orbital period of P ∼ 3:506 days. An SED fit to available multi-band photometry, ranging from the near-UV to the mid-IR, yields a distance of d = 101 ± 6 pc to the system.
    [Show full text]
  • 'Hot Jupiter' Detected by the Qatar Exoplanet Survey 18 December 2017, by Tomasz Nowakowski
    New grazing transiting 'hot Jupiter' detected by the Qatar Exoplanet Survey 18 December 2017, by Tomasz Nowakowski Now, a team of astronomers, led by Khalid Alsubai of the Qatar Environment and Energy Research Institute (QEERI) in Doha, Qatar, reports the finding of a new addition to the short list of planets in a grazing transit configuration. They discovered Qatar-6b as part of the QES survey, which utilizes the New Mexico Skies Observatory located at Mayhill, New Mexico. "In this paper, we present the discovery of Qatar-6b, a newly found hot Jupiter on a grazing transit," the researchers wrote in the paper. According to the study, Qatar-6b has a radius about 6 percent larger than Jupiter and a mass of approximately 0.67 Jupiter masses, which indicates a density of 0.68 g/cm3. The exoplanet orbits its The discovery light curve for Qatar-6b phase folded with parent star every 3.5 days at a distance of about the BLS estimated period, as it appears in the QES 0.04 AU from the host. Due to the proximity of this archive. Credit: Alsubai et al., 2017. planet to the star, astronomers estimate that it has an equilibrium temperature of 1,006 K. The parameters suggest that Qatar-6b belongs to (Phys.org)—An international group of astronomers group of planets known as "hot Jupiters." These has found a new grazing transiting "hot Jupiter" exoworlds are similar in characteristics to the solar alien world as part of the Qatar Exoplanet Survey system's biggest planet, with orbital periods of less (QES).
    [Show full text]
  • AST413 Gezegen Sistemleri Ve Oluşumu Ders 4 : Geçiş Yöntemi – I Yöntemin Temelleri Geçiş Yöntemi HD 209458 B
    AST413 Gezegen Sistemleri ve Oluşumu Ders 4 : Geçiş Yöntemi – I Yöntemin Temelleri Geçiş Yöntemi HD 209458 b Charbonneau vd. 2000 2000 yılında David Charbonneau dikine hız yöntemiyle keşfedilmiş HD 209458 b’nin bir geçişini gözledi. Bu ilk gezegen geçiş gözlemidir. Charbonneau, cismin yörünge parametrelerini dikine hızdan bildiği için teleskobunu yapıyorsa geçişini gözlemek üzere ne zaman cisme doğrultması gerektiğini biliyordu. Ancak, gezegenin gözlemicyle arasından geçiş yapmak gibi bir zorunluluğu da yoktur. Venüs Geçişi Venüs örneğinde gördüğümüz gibi gezegen yıldızın önünden geçerken, yıldızın ışığı gezegenin (varsa) atmosferinin içinden geçerek bize ulaşır. Bu da -ideal durumda- gezegenin atmosferini çalışmamıza olanak sağlayabilir. Sıcak Jüpiterler Gerçekten Var! 51 Peg b keşfinden sonra sıcak Jüpiterlerin (yıldızına 1/20 AB'den daha yakın dev gaz gezegenler) yıldızlarına bu kadar yakın oluşup oluşamayacakları, sistemin başka bir yerinden göç etmiş olabilme olasılıkları hatta var olup olmadıkları uzun süre tartışıldı. Ancak bu cisimlerin yarıçaplarının (R p) büyük olması ve yıldızlarına yakınlıkları (a), daha büyük geçiş ışık değişim genliği ve daha kısa geçiş dönemi nedeniyle onların geçiş yöntemiyle keşfedillme olasılıklarını da arttırdığından, bu yöntemle diğer gezegenlere göre daha kolay keşfedilmelerini de sağladı. Dikine hız tekniğiyle keşfedilen HD 209458b, geçiş de gösteriyordu ve dikine hız ölçümleriyle, geçiş gözlemleri birlikte değerlendirildiğinde bu sıcak Jüpiter türü gezegenin gerçekten var olduğu kanıtlanmış oldu! Charbonneau vd. 2000 Mazeh vd. 2000 Geçiş Olasılığı Öncelikle gezegenin yörüngesinin çembersel (e = 0) olduğunu varsayalım. Bu durumda gezegenin gözlemcinin bakış yönü doğrultusunda yıldızla arasından (sıyırarak da olsa) geçmesi için yörüngenin yarı-büyük eksen uzunluğu a’nın cos i çarpanı kadar kısaltılmış kesitinin (a cos i) yıldızın yarıçapı ile gezegen yarıçapı toplamından (R* + Rg) küçük olması gerekir (a cos i ≤ R* + Rg).
    [Show full text]
  • KELT-23Ab: a Hot Jupiter Transiting a Near-Solar Twin Close to the TESS and JWST Continuous Viewing Zones
    The Astronomical Journal, 158:78 (14pp), 2019 August https://doi.org/10.3847/1538-3881/ab24c7 © 2019. The American Astronomical Society. All rights reserved. KELT-23Ab: A Hot Jupiter Transiting a Near-solar Twin Close to the TESS and JWST Continuous Viewing Zones Daniel Johns1 , Phillip A. Reed1 , Joseph E. Rodriguez2 , Joshua Pepper3 , Keivan G. Stassun4,5 , Kaloyan Penev6 , B. Scott Gaudi7 , Jonathan Labadie-Bartz8,9 , Benjamin J. Fulton10 , Samuel N. Quinn2 , Jason D. Eastman2 , David R. Ciardi10, Lea Hirsch11 , Daniel J. Stevens12,13 , Catherine P. Stevens14, Thomas E. Oberst14, David H. Cohen15, Eric L. N. Jensen15 , Paul Benni16, Steven Villanueva, Jr.7 , Gabriel Murawski17, Allyson Bieryla2 , David W. Latham2 , Siegfried Vanaverbeke18, Franky Dubois18, Steve Rau18, Ludwig Logie18, Ryan F. Rauenzahn1, Robert A. Wittenmyer19 , Roberto Zambelli20, Daniel Bayliss21,22 , Thomas G. Beatty13,23 , Karen A. Collins2 , Knicole D. Colón24 , Ivan A. Curtis25, Phil Evans26, Joao Gregorio27, David James28 , D. L. Depoy29,30, Marshall C. Johnson7 , Michael D. Joner31, David H. Kasper32, Somayeh Khakpash3 , John F. Kielkopf33, Rudolf B. Kuhn34,35, Michael B. Lund4,10 , Mark Manner36 , Jennifer L. Marshall29,30 , Kim K. McLeod37 , Matthew T. Penny7 , Howard Relles2, Robert J. Siverd4 , Denise C. Stephens31, Chris Stockdale38 , Thiam-Guan Tan39 , Mark Trueblood40, Pat Trueblood40, and Xinyu Yao3 1 Department of Physical Sciences, Kutztown University, Kutztown, PA 19530, USA 2 Center for Astrophysics | Harvard & Smithsonian, 60 Garden Steet, Cambridge,
    [Show full text]
  • Joint Institute for VLBI in Europe Biennial Report 2011-2012
    Joint Institute For VLBI in Europe 11-12 Biennial report 2011-2012 The Joint Institute for VLBI in Europe (JIVE) was established as a scientific foundation in December 1993. JIVE’s mandate is to support the operations of the European VLBI Network (EVN) in the widest sense. JIVE’s operations are supported via multi‐national funds from the following organisations: Netherlands Institute for Radio Astronomy (ASTRON), the Netherlands, National Center for Scientific Research (CNRS), France National Geographical Institute (IGN), Spain, Italian National Institute of Astrophysics (INAF), Italy, Max Planck Institute for Radio Astronomy (MPIfR), Germany, National Astronomical Observatories of China (NAOC), China, National Research Foundation (NRF), South Africa Netherlands Organisation for Scientific Research (NWO), the Netherlands, Onsala Space Observatory (OSO), Sweden, Science & Technology Facilities Council (STFC), UK Joint Institute for VLBI in Europe | Biennial report 2011‐2012 Contents 1. INSTITUTE ....................................................................................................................................................... 1 1.1. preparing for the next funding cycle ..................................................................................................... 1 1.2. enhancing the VLBI capabilities ............................................................................................................. 2 1.3. JIVE events ............................................................................................................................................
    [Show full text]
  • Keith Horne: Refereed Publications Papers Submitted: 425. “A
    Keith Horne: Refereed Publications Papers Submitted: 427. “The Lick AGN Monitoring Project 2016: Velocity-Resolved Hβ Lags in Luminous Seyfert Galaxies.” V.U, A.J.Barth, H.A.Vogler, H.Guo, T.Treu, et al. (202?). ApJ, submitted (01 Oct 2021). 426. “Multi-wavelength Optical and NIR Variability Analysis of the Blazar PKS 0027-426.” E.Guise, S.F.H¨onig, T.Almeyda, K.Horne M.Kishimoto, et al. (202?). (arXiv:2108.13386) 425. “A second planet transiting LTT 1445A and a determination of the masses of both worlds.” J.G.Winters, et al. (202?) ApJ, submitted (30 Jul 2021). (arXiv:2107.14737) 424. “A Different-Twin Pair of Sub-Neptunes orbiting TOI-1064 Discovered by TESS, Characterised by CHEOPS and HARPS” T.G.Wilson et al. (202?). ApJ, submitted (12 Jul 2021). 423. “The LHS 1678 System: Two Earth-Sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc” M.L.Silverstein, et al. (202?). AJ, submitted (24 Jun 2021). 422. “A temperate Earth-sized planet with strongly tidally-heated interior transiting the M8 dwarf LP 791-18.” M.Peterson, B.Benneke, et al. (202?). submitted (09 May 2021). 421. “The Sloan Digital Sky Survey Reverberation Mapping Project: UV-Optical Accretion Disk Measurements with Hubble Space Telescope.” Y.Homayouni, M.R.Sturm, J.R.Trump, K.Horne, C.J.Grier, Y.Shen, et al. (202?). ApJ submitted (06 May 2021). (arXiv:2105.02884) Papers in Press: 420. “Bayesian Analysis of Quasar Lightcurves with a Running Optimal Average: New Time Delay measurements of COSMOGRAIL Gravitationally Lensed Quasars.” F.R.Donnan, K.Horne, J.V.Hernandez Santisteban (202?) MNRAS, in press (28 Sep 2021).
    [Show full text]
  • Studying Exoplanets from Bridgewater State University Maria Patrone
    Bridgewater State University Virtual Commons - Bridgewater State University Honors Program Theses and Projects Undergraduate Honors Program 5-2-2018 Finding Alien Worlds: Studying Exoplanets from Bridgewater State University Maria Patrone Follow this and additional works at: http://vc.bridgew.edu/honors_proj Part of the Physics Commons Recommended Citation Patrone, Maria. (2018). Finding Alien Worlds: Studying Exoplanets from Bridgewater State University. In BSU Honors Program Theses and Projects. Item 275. Available at: http://vc.bridgew.edu/honors_proj/275 Copyright © 2018 Maria Patrone This item is available as part of Virtual Commons, the open-access institutional repository of Bridgewater State University, Bridgewater, Massachusetts. Finding Alien Worlds: Studying Exoplanets from Bridgewater State University Maria Patrone Submitted in Partial Completion of the Requirements for Commonwealth Honors in Physics Bridgewater State University May 2, 2018 Dr. Martina Arndt, Thesis Advisor Dr. Thomas Kling, Committee Member Dr. Jeffrey Williams, Committee Member Bridgewater State University Finding Alien Worlds: Studying Exoplanets from Bridgewater State University by Maria Patrone in the Department of Physics May 7, 2018 \Keep Looking Up" Neil Degrasse Tyson Bridgewater State University Abstract Department of Physics by Maria Patrone The search for exoplanets, or planets orbiting other stars in our galaxy, has only been a field of study since the early 1990's and is currently a popular area of research among astrophysicists. With the launch of the Kepler Space telescope in 2009, there are over three thousand confirmed exoplanets, and over four thousand Kepler Objects of Interest (KOI's), which are possible exoplanet candidates. With so much data obtained from Kepler, NASA relies on ground based observatories to follow up and confirm KOI's as exoplanets or false positives.
    [Show full text]
  • AST413 Gezegen Sistemleri Ve Oluşumu Ders 4A : Geçiş Yöntemi - I Geçiş Yöntemi HD 209458 B
    AST413 Gezegen Sistemleri ve Oluşumu Ders 4a : Geçiş Yöntemi - I Geçiş Yöntemi HD 209458 b Charbonneau vd. 2000 2000 yılında David Charbonneau dikine hız yöntemiyle keşfedilmiş HD 209458 b’nin bir geçişini gözledi. Bu ilk gezegen geçiş gözlemidir. Charbonneau, cismin yörünge parametrelerini dikine hızdan bildiği için teleskobunu yapıyorsa geçişini gözlemek üzere ne zaman cisme doğrultması gerektiğini biliyordu. Ancak, gezegenin gözlemicyle arasından geçiş yapmak gibi bir zorunluluğu da yoktur. Venüs Geçişi Venüs örneğinde gördüğümüz gibi gezegen yıldızın önünden geçerken, yıldızın ışığı gezegenin (varsa) atmosferinin içinden geçerek bize ulaşır. Bu da -ideal durumda- gezegenin atmosferini çalışmamıza olanak sağlayabilir. Sıcak Jüpiterler Gerçekten Var! 51 Peg b keşfinden sonra sıcak Jüpiterlerin (yıldızına 1/20 AB'den daha yakın dev gaz gezegenler) yıldızlarına bu kadar yakın oluşup oluşamayacakları, sistemin başka bir yerinden göç etmiş olabilme olasılıkları hatta var olup olmadıkları uzun süre tartışıldı. Ancak bu cisimlerin yarıçaplarının (R p) büyük olması ve yıldızlarına yakınlıkları (a), daha büyük geçiş ışık değişim genliği ve daha kısa geçiş dönemi nedeniyle onların geçiş yöntemiyle keşfedillme olasılıklarını da arttırdığından, bu yöntemle diğer gezegenlere göre daha kolay keşfedilmelerini de sağladı. Dikine hız tekniğiyle keşfedilen HD 209458b, geçiş de gösteriyordu ve dikine hız ölçümleriyle, geçiş gözlemleri birlikte değerlendirildiğinde bu sıcak Jüpiter türü gezegenin gerçekten var olduğu kanıtlanmış oldu! Charbonneau vd. 2000
    [Show full text]
  • Dr. Alex Harrison Parker Postdoctoral Fellow in Planetary Astronomy
    Dr. Alex Harrison Parker Postdoctoral Fellow in Planetary Astronomy Department of Astronomy University of California at Berkeley Phone: 360-599-5346 B-20 Hearst Field Annex #3411 [email protected] Berkeley, CA 94720-3411 www.astro.uvic.ca/~alexhp/ Higher Education Institution Field Degree Years University of Victoria Astronomy PhD 2007|2011. University of Washington Physics & Astronomy BSc 2005|2007. Whatcom Community College Physics AAS 2002|2005. PhD Details \Ultra-Wide Trans-Neptunian Binaries: Tracers of the Outer Solar System's History" | Advised by Dr. JJ Kavelaars, National Research Council of Canada | Thesis archived online at http://hdl.handle.net/1828/3400 | Enrolled September 2007 | Defended July 2011 | Awarded November 2011 Professional Appointments University of California at Berkeley - Postdoctoral Fellow 2013 | Present. University of California at Berkeley Department of Astronomy Ongoing support for New Horizons post-Pluto/Kuiper Belt mission development. Kuiper Belt Binaries team lead for CFHT-OSSOS Large Program. See \Ongoing Research" document. New Horizons Outer Solar System Science Fellow 2011 | 2013. Harvard-Smithsonian Center for Astrophysics, Cambridge MA USA. Survey specialist; searching for candidate Kuiper Belt Objects for NASA's New Horizons spacecraft to visit after its 2015 Pluto encounter. Perform advanced survey image analysis, trajectory analysis, target orbit and physical characterization. Manage central astrometry database and target submission to the Minor Planet Center. Science case development for remote-sensing observations of Kuiper Belt Objects at medium range (0.1-0.5 AU). National Science Foundation | Graduate Research Fellow 2008 | 2011. University of Victoria, Victoria BC Canada. PhD research in binary Kuiper Belt Object orbits, dynamics, and origin.
    [Show full text]
  • Finding New Earths Using Machine Learning & Committee Machine
    International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 07 Issue: 05 | May 2020 www.irjet.net p-ISSN: 2395-0072 Finding New Earths Using Machine Learning & Committee Machine Piyush Gawade1, Akshay Mayekar2, Ashish Bhosale3 , Dr. Sanjay Jadhav4 1Student, Computer Engineering, SIGCE, Navi Mumbai, Maharashtra, India 2Student, Computer Engineering, SIGCE, Navi Mumbai, Maharashtra, India 3Student, Computer Engineering, SIGCE, Navi Mumbai, Maharashtra, India 4Dean - Training and Placement , Professor, Computer Engineering, Smt. Indira Gandhi College of Engineering, Navi Mumbai, Maharashtra, India ---------------------------------------------------------------------***--------------------------------------------------------------------- Abstract - Planet identification has typically been a Machine learning techniques have been applied by citizen tasked performed exclusively by teams of astronomers astronomers to classify objects of interest. One of the more and astrophysicists using methods and tools accessible notable examples of this is the work done by Shallue and only to those with years of academic education and Vanderberg in their 2011 study (1). Shallue and Vanderberg training. NASA’s Exoplanet Exploration program has were two machine learning engineers at Google who trained introduced modern satellites capable of capturing a vast a neural network model to scour archived data to identify array of data regarding celestial objects of interest to planets using transit events which had gone unnoticed by assist with researching these objects. The availability of other researchers (1). The “Autovetter Project” created a satellite data has opened up the task of planet Navie Bayes Model to classify objects of interest based on identification to individuals capable of writing and transit data as well (1). In effect exoplanet classification has interpreting machine learning models. In this study, now been crowd sourced.
    [Show full text]
  • KELT-25 B and KELT-26 B: a Hot Jupiter and a Substellar Companion Transiting Young a Stars Observed by TESS
    Swarthmore College Works Physics & Astronomy Faculty Works Physics & Astronomy 9-1-2020 KELT-25 B And KELT-26 B: A Hot Jupiter And A Substellar Companion Transiting Young A Stars Observed By TESS R. R. Martínez R. R. Martínez Follow this and additional works at: https://works.swarthmore.edu/fac-physics B. S. Gaudi Part of the Astrophysics and Astronomy Commons J.Let E. us Rodriguez know how access to these works benefits ouy G. Zhou Recommended Citation See next page for additional authors R. R. Martínez, R. R. Martínez, B. S. Gaudi, J. E. Rodriguez, G. Zhou, J. Labadie-Bartz, S. N. Quinn, K. Penev, T.-G. Tan, D. W. Latham, L. A. Paredes, J. F. Kielkopf, B. Addison, D. J. Wright, J. Teske, S. B. Howell, D. Ciardi, C. Ziegler, K. G. Stassun, M. C. Johnson, J. D. Eastman, R. J. Siverd, T. G. Beatty, L. Bouma, T. Bedding, J. Pepper, J. Winn, M. B. Lund, S. Villanueva Jr., D. J. Stevens, Eric L.N. Jensen, C. Kilby, J. D. Crane, A. Tokovinin, M. E. Everett, C. G. Tinney, M. Fausnaugh, David H. Cohen, D. Bayliss, A. Bieryla, P. A. Cargile, K. A. Collins, D. M. Conti, K. D. Colón, I. A. Curtis, D. L. Depoy, P. Evans, D. L. Feliz, J. Gregorio, J. Rothenberg, D. J. James, M. D. Joner, R. B. Kuhn, M. Manner, S. Khakpash, J. L. Marshall, K. K. McLeod, M. T. Penny, P. A. Reed, H. M. Relles, D. C. Stephens, C. Stockdale, M. Trueblood, P. Trueblood, X. Yao, R. Zambelli, R. Vanderspek, S.
    [Show full text]
  • Allyson Bieryla 241 Crescent St, Apt
    Allyson Bieryla 241 Crescent St, Apt. 3603 Waltham , MA 02453 Phone: 303.709.2891 E-Mail: [email protected] Education Harvard University Extension School Master of Liberal Arts, Software Engineering. In progress. Harvard University Extension School Graduate-level Certificate in Data Science. June 2019. University of Colorado at Boulder B.A. in Astrophysics, Physics and Fine Arts; minor in Geology. May 2005. Professional Experience • Astronomy Lab and Telescope Manager - Harvard University, 1. Sept. 2008 - Present Cambridge, MA. • Astronomer – Smithsonian Astrophysical Observatory, Cambridge, Feb. 2009 - Present MA. • Geometry Technician – Tricon Geophysics, Denver, CO. Oct. 2007 – Aug. 2008 • Research Assistant – Southwest Research Institute, Boulder, CO. May 2005 – Oct. 2007 Management/Teaching Experience • Manage laboratory inventory and maintain instruments and telescope • Train graduate students and new users on equipment and lab materials • Work closely with faculty on course lab development • Run (and co-founded) the Harvard Observing Project (HOP) which gives students opportunities to learn about observational astronomy • Advise undergraduate students on research projects • Lead observing sessions and course laboratory sessions • Staff advisor the undergraduate astronomy club, Student Astronomers at Harvard- Radcliffe (STAHR) • Organize and analyze large amounts of data from space and ground based telescopes Research Experience • Exoplanet detection and characterization including velocity determination, orbit fitting and
    [Show full text]