Prime Focus (10-08)
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Publications for Dr. Peter L. Capak 1 of 21 Publication Summary 369
Publications for Dr. Peter L. Capak Publication Summary 369 Publications 319 Refereed Publications Accepted or Submitted 50 Un-refereed Publications Top 1% of Cited Researchers in 2017-2019 >30,000 Citations >1,600 Citations on first author papers 99 papers with >100 citations, 6 as first author. H Index = 99 First Author publications 1) Capak et al., 2015, “Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission”, Nature, 522, 455 2) Capak et al., 2013, “Keck-I MOSFIRE Spectroscopy of the z ~ 12 Candidate Galaxy UDFj-39546284”, ApJL, 733, 14 3) Capak et al., 2011, “A massive protocluster of galaxies at a redshift of z~5.3” , Nature, 470, 233 4) Capak et al., 2010, “Spectroscopy and Imaging of three bright z>7 candidates in the COSMOS survey”, ApJ, 730, 68 5) Capak et al., 2008, "Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547", ApJL, 681, 53 6) Capak et. al., 2007, "The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey", ApJS, 172, 284 7) Capak et. al., 2007, "The First Release COSMOS Optical and Near-IR Data and Catalog", ApJS, 172, 99 8) Capak, 2004, “Probing global star and galaxy formation using deep multi-wavelength surveys”, Ph.D. Thesis 9) Capak et. al., 2004, "A Deep Wide-Field, Optical, and Near-Infrared Catalog of a Large Area around the Hubble Deep Field North", AJ, 127, 180 Other Publications (P. Capak was a leading author in bolded entries) 10) Faisst et al., 2020, “The ALPINE-ALMA [CII] survey: Multi-Wavelength Ancillary Data. -
Observing Galaxy Evolution in the Context of Large
Astro2020 Science White Paper Observing Galaxy Evolution in the Context of Large-Scale Structure Thematic Areas: Planetary Systems Star and Planet Formation Formation and Evolution of Compact Objects Cosmology and Fundamental Physics Stars and Stellar Evolution Resolved Stellar Populations and their Environments 7Galaxy Evolution Multi-Messenger Astronomy and Astrophysics Principal Author: Name: Mark Dickinson Institution: NOAO Email: [email protected] Phone: 520-318-8531 Co-authors: Yun Wang (Caltech/IPAC), James Bartlett (NASA JPL), Peter Behroozi (Arizona), Jarle Brinchmann (Leiden Observatory; Porto), Peter Capak (Caltech/IPAC), Ranga Chary (Caltech/IPAC), Andrea Cimatti (Bologna; INAF), Alison Coil (UC San Diego), Charlie Conroy (CfA), Emanuele Daddi (CEA, Saclay), Megan Donahue (Michigan State University), Peter Eisenhardt (NASA JPL), Henry C. Ferguson (STScI), Karl Glazebrook (Swinburne), Steve Furlanetto (UCLA), Anthony Gonzalez (Florida), George Helou (Caltech/IPAC), Philip F. Hopkins (Caltech), Jeyhan Kartaltepe (RIT), Janice Lee (Caltech/IPAC), Sangeeta Malhotra (NASA GSFC), Jennifer Marshall (Texas A&M), Jeffrey A. Newman (Pittsburgh), Alvaro Orsi (CEFCA), James Rhoads (NASA GSFC), Jason Rhodes (NASA JPL), Alice Shapley (UCLA), Risa H. Wechsler (Stanford/KIPAC; SLAC) Abstract: Galaxies form and evolve in the context of their local and large-scale environments. Their baryonic content that we observe with imaging and spectroscopy is intimately connected to the properties of their dark matter halos, and to their location in the “cosmic web” of large-scale structure. Very large spectroscopic surveys of the local universe (e.g., SDSS and GAMA) measure galaxy positions (location within large-scale structure), statistical clustering (a direct constraint on dark matter halo masses), and spectral features (measuring physical conditions of the gas and stars within the galax- ies, as well as internal velocities). -
HEIC0701: for IMMEDIATE RELEASE 19:30 (CET)/01:30 PM EST 7 January, 2007
HEIC0701: FOR IMMEDIATE RELEASE 19:30 (CET)/01:30 PM EST 7 January, 2007 http://www.spacetelescope.org/news/html/heic0701.html News release: First 3D map of the Universe’s Dark Matter scaffolding 7-January-2007 By analysing the COSMOS survey – the largest ever survey undertaken with Hubble – an international team of scientists has assembled one of the most important results in cosmology: a three-dimensional map that offers a first look at the web-like large-scale distribution of dark matter in the Universe. This historic achievement accurately confirms standard theories of structure formation. For astronomers, the challenge of mapping the Universe has been similar to mapping a city from night-time aerial snapshots showing only streetlights. These pick out a few interesting neighbourhoods, but most of the structure of the city remains obscured. Similarly, we see planets, stars and galaxies in the night sky; but these are constructed from ordinary matter, which accounts in total for only one sixth of the total mass in the Universe. The remainder is a mysterious component - dark matter - that neither emits nor reflects light. An international team of astronomers led by Richard Massey of the California Institute of Technology (Caltech), USA, has made a three-dimensional map that offers a first look at the web-like large-scale distribution of dark matter in the Universe in unprecedented detail. This new map is equivalent to seeing a city, its suburbs and surrounding country roads in daylight for the first time. Major arteries and intersections are revealed and the variety of different neighbourhoods becomes evident. -
CURRICULUM VITAE Andreas Faisst | Caltech - Infrared Processing and Analysis Center | [email protected]
December 5, 2019 CURRICULUM VITAE Andreas Faisst | Caltech - Infrared Processing and Analysis Center | [email protected] PERSONAL INFORMATION RESEARCH INTERESTS Name Andreas Faisst • Physics during the Epoch of Reionization Citizenship Switzerland • Early phases of galaxy formation and Contact Infrared Processing and Analysis Center evolution California Institute of Technology • Physical and structural properties of high- 314-6 Keith Spalding redshift galaXies 1200 E. California Blvd. • Quenching of star formation in massive Pasadena, CA 91125, USA galaxies E-mail [email protected] Social Media @astrofaisst (Twitter) Webpage http://www.astro.caltech.edu/~afaisst MAIN LEADS AND INVOLVEMENTS U.S. lead principal investigator of ALPINE (a 70-hour large ALMA program). Member of the IPAC Joint PiXel Processing and Tech Initiative. Science co-investigator and science operation center (SOC) scientist for ISCEA (a NASA small satellite mission). Part of the science and outreach team for CASTOR (a Canada- led space telescope). REFERENCES Dr. Peter Capak (Caltech/IPAC), [email protected]. More references are available upon request. CAREER AND EDUCATION Jan 2019 to present Assistant Research Scientist at Caltech/IPAC Oct 2016 to Dec 2018 Postdoctoral Researcher at Caltech/IPAC May 2015 to Oct 2016 SNSF Postdoctoral Fellow at Caltech (Visitor in Astronomy) April 2015 Dr. Sc. ETH Zurich in Physics ETH Zurich, Switzerland Thesis: “The Evolution of Star-forming and Quiescent Massive Galaxies through Cosmic Time” March 2011 M.Sc. in Physics ETH Zurich, Switzerland Thesis: “Star-forming Galaxies at Redshifts z~2 and z~4” September 2009 B.Sc. in Physics ETH Zurich, Switzerland GRANTS, HONORS, AND AWARDS April 2014 SNSF Early Postdoc Mobility Fellowship March 2012 ETH Medal for outstanding Master thesis March 2011 M.Sc. -
From Dark Matter to Galaxies with Convolutional Networks
From Dark Matter to Galaxies with Convolutional Networks Xinyue Zhang*, Yanfang Wang*, Wei Zhang*, Siyu He Yueqiu Sun*∗ Department of Physics, Carnegie Mellon University Center for Data Science, New York University Center for Computational Astrophysics, Flatiron Institute xz2139,yw1007,wz1218,[email protected] [email protected] Gabriella Contardo, Francisco Shirley Ho Villaescusa-Navarro Center for Computational Astrophysics, Flatiron Institute Center for Computational Astrophysics, Flatiron Institute Department of Astrophysical Sciences, Princeton gcontardo,[email protected] University Department of Physics, Carnegie Mellon University [email protected] ABSTRACT 1 INTRODUCTION Cosmological surveys aim at answering fundamental questions Cosmology focuses on studying the origin and evolution of our about our Universe, including the nature of dark matter or the rea- Universe, from the Big Bang to today and its future. One of the holy son of unexpected accelerated expansion of the Universe. In order grails of cosmology is to understand and define the physical rules to answer these questions, two important ingredients are needed: and parameters that led to our actual Universe. Astronomers survey 1) data from observations and 2) a theoretical model that allows fast large volumes of the Universe [10, 12, 17, 32] and employ a large comparison between observation and theory. Most of the cosmolog- ensemble of computer simulations to compare with the observed ical surveys observe galaxies, which are very difficult to model theo- data in order to extract the full information of our own Universe. retically due to the complicated physics involved in their formation The constant improvement of computational power has allowed and evolution; modeling realistic galaxies over cosmological vol- cosmologists to pursue elucidating the fundamental parameters umes requires running computationally expensive hydrodynamic and laws of the Universe by relying on simulations as their theory simulations that can cost millions of CPU hours. -
Jrasc-August'99 Text
Publications and Products of August/août 1999 Volume/volume 93 Number/numero 4 [678] The Royal Astronomical Society of Canada Observer’s Calendar — 2000 This calendar was created by members of the RASC. All photographs were taken by amateur astronomers using ordinary camera lenses and small telescopes and represent a wide spectrum of objects. An informative caption accompanies every photograph. This year all of the photos are in full colour. The Journal of the Royal Astronomical Society of Canada Le Journal de la Société royale d’astronomie du Canada It is designed with the observer in mind and contains comprehensive astronomical data such as daily Moon rise and set times, significant lunar and planetary conjunctions, eclipses, and meteor showers. The 1999 edition received two awards from the Ontario Printing and Imaging Association, Best Calendar and the Award of Excellence. (designed and produced by Rajiv Gupta). Price: $13.95 (members); $15.95 (non-members) (includes taxes, postage and handling) The Beginner’s Observing Guide This guide is for anyone with little or no experience in observing the night sky. Large, easy to read star maps are provided to acquaint the reader with the constellations and bright stars. Basic information on observing the moon, planets and eclipses through the year 2005 is provided. There is also a special section to help Scouts, Cubs, Guides and Brownies achieve their respective astronomy badges. Written by Leo Enright (160 pages of information in a soft-cover book with otabinding which allows the book to lie flat). Price: $15 (includes taxes, postage and handling) Looking Up: A History of the Royal Astronomical Society of Canada Published to commemorate the 125th anniversary of the first meeting of the Toronto Astronomical Club, “Looking Up — A History of the RASC” is an excellent overall history of Canada’s national astronomy organization. -
Key Information • This Exam Contains 6 Parts, 79 Questions, and 180 Points Total
Reach for the Stars *** Practice Test 2020-2021 Season Answer Key Information • This exam contains 6 parts, 79 questions, and 180 points total. • You may take this test apart. Put your team number on each page. There is not a separate answer page, so write all answers on this exam. • You are permitted the resources specified on the 2021 rules. • Don't worry about significant figures, use 3 or more in your answers. However, be sure your answer is in the correct units. • For calculation questions, any answers within 10% (inclusive) of the answer on the key will be accepted. • Ties will be broken by section score in reverse order (i.e. Section F score is the first tiebreaker, Section A the last). • Written by RiverWalker88. Feel free to PM me if you have any questions, feedback, etc. • Good Luck! Reach for the stars! Reach for the Stars B Team #: Constants and Conversions CONSTANTS Stefan-Boltzmann Constant = σ = 5:67 × 10−8 W=m2K4 Speed of light = c = 3 × 108m/s 30 Mass of the sun = M = 1:99 × 10 kg 5 Radius of the sun = R = 6:96 × 10 km Temperature of the sun = T = 5778K 26 Luminosity of the sun = L = 3:9 × 10 W Absolute Magnitude of the sun = MV = 4.83 UNIT CONVERSIONS 1 AU = 1:5 × 106km 1 ly = 9:46 × 1012km 1 pc = 3:09 × 1013km = 3.26 ly 1 year = 31557600 seconds USEFUL EQUATIONS 2900000 Wien's Law: λ = peak T • T = Temperature (K) • λpeak = Peak Wavelength in Blackbody Spectrum (nanometers) 1 Parallax: d = p • d = Distance (pc) • p = Parallax Angle (arcseconds) Page 2 of 13Page 13 Reach for the Stars B Team #: Part A: Astrophotographical References 9 questions, 18 points total For each of the following, identify the star or deep space object pictured in the image. -
Enhancing LSST Science with Euclid Synergy Arxiv:1904.10439V1 [Astro
Enhancing LSST Science with Euclid Synergy P. Capak, J-C. Cuillandre, F. Bernardeau, F. Castander, R. Bowler, C. Chang, C. Grillmair, P. Gris, T. Eifler, C. Hirata, I. Hook, B. Jain, K. Kuijken, M. Lochner, P. Oesch, S. Paltani, J. Rhodes, B. Robertson, D. Rubin, R. Scaramella, C. Scarlata, D. Scolnic, J. Silverman, S. Wachter, Y. Wang, The Tri-Agency Working Group November, 30, 2018 Abstract This white paper is the result of the Tri-Agency Working Group (TAG) appointed to develop synergies between missions and is intended to clarify what LSST observations are needed in order to maximally enhance the combined science output of LSST and Euclid. To facilitate LSST planning we provide a range of possible LSST surveys with clear metrics based on the improvement in the Dark Energy figure of merit (FOM). To provide a quantifiable metric we present five survey options using only between 0.3 and 3.8% of the LSST 10 year survey. We also provide information so that the LSST DDF cadence can possibly be matched to those of Euclid in common deep fields, SXDS, COSMOS, CDFS, and a proposed new LSST deep field (near the Akari Deep Field South). Co-coordination of observations from the Large Synoptic Survey Telescope (LSST) and Euclid will lead to a significant number of synergies. The combination of optical multi-band imaging from LSST with high resolution optical and near-infrared photom- etry and spectroscopy from Euclid will not only improve constraints on Dark Energy, but provide a wealth of science on the Milky Way, local group, local large scale struc- ture, and even on first galaxies during the epoch of reionization. -
Dr. Peter Capak
Dr. Peter Capak https://www.linkedin.com/in/peter-capak/ Summary Demonstrated leadership and extensive expertise in Research and Development, Machine Learning, Statistics, Project Management, and Systems Engineering. Has worked at the junction of hardware, software, and human factors in projects with budgets up to $4.5 billion. Has a strong track record of delivering software and hardware systems, requiring significant R&D, on deadline and budget. Over 15 years of experience recruiting, leading, and mentoring international cross-functional teams of scientists, hardware engineers and software engineers to develop cutting edge systems including products. Recognized for effectiveness in managing and negotiating international partnerships between industry, academia, and governments. Work History April 2020 – Present Architect of Perception Systems for Augmented and Virtual Reality, Facebook/Oculus June 2004 – Present Project Lead and Scientist, California Institute of Technology (Caltech) and NASA Jet Propulsion Laboratory (JPL), Pasadena, CA Skills & Expertise Systems Engineering: Has been part of the leadership for several international teams that designed and developed complex systems including hardware, software, and human factors. The projects tackled by these teams include scientific satellites, IT systems, technical user-interface (UI) systems, and focused technical projects with total budgets of up to $4.5 billion. One example is the ESA/NASA Euclid mission. Has extensive experience setting up requirements matrixes, accountability systems, and management structures for trans-national, multi-organizational projects that include government, industry, and academic partners. Research and Development (R&D) Management: Has successfully lead both focused small groups and large international cross-functional teams of independent researchers to develop leading edge scientific breakthroughs. -
October's Meeting
October 2008 October’s Meeting Calendar Inside this Issue Sep 4, 2008 – “ Past Saturn and The next meeting of S*T*A*R will be 7 More Years to Pluto: ” New on Thursday, October 2. Our program Horizons Mission, Michael October’s Meeting will be “An Idea That Would Not Die” Lewis, NASA Solar System 1 2008-2009 Calendar by Robert Zimmerman. All are Ambassador welcome. The meeting will begin Oct 2, 2008 – " An Idea That President’s Corner promptly at 8:00pm at the Monmouth Would Not Die" by Robert September Meeting Museum on the campus of Brookdale 2 Zimmerman Minutes Community College. Extreme Starburst Editor’s Corner Nov 6, 2008 – “TBD" 3 Dec 4, 2008 – “Low Energy Thanks to Gavin Warnes, Steve Fedor, Routes to the Moon and & Randy Walton for contributing to this Beyond” by Dr. Edward month’s Spectrogram. Belbruno, Innovative Orbital 4 Design, Inc., Princeton Reminder to pay membership dues S*T*A*R Membership University $25/individual, $35/family. Donations Celestial Events 5 are appreciated. Make payments to Paul Jan 8, 2009 - “Celestial Nadolny at the October meeting or mail Navigation” by Justin Dimmell, In the Eyepiece a check payable to S*T*A*R Island School, Eleuthera, Astronomy Society Inc to: 6 Bahamas S*T*A*R Astronomy Society Moon Phases P.O. Box 863 Feb 5, 2009 - "TBD" 7 Jupiter Moons Calendar Red Bank, NJ 07701 Mar 5, 2009 - “Solar Saturn Moons Calendar Telescopes" by Alan Traino of Astro Crossword Puzzle Lunt Solar Systems November Issue 8 Apr 2, 2009 – “ TBD ” Please send articles and contributions for the next Spectrogram by Friday, May 7, 2009 – “TBD” October 24 . -
MY SO October Showdown Rules
S P A C E - O C T O B E R 2 0 2 0 MY SO STEM SHOWDOWN C O N T E N T , R E C O M M E N D E D M A T E R I A L S & S C O R I N G STEM SHOWDOWN CONTENT The STEM Showdown will consist of a series of online multiple-choice questions. Middle school (Grade 6-9) participant questions will center around the properties and evolution of stars and galaxies as well as their observation using different portions of the electromagnetic spectrum (e.g., Radio, Infrared, Visible, Ultraviolet, X-Ray, Gamma Ray). While high school (Grades 9-12) participants will focus on Star and Galaxy Formation and Evolution. A Showdown participant will have 55- minutes to answer as many questions as possible. The middle school (Grades 6-9) content and skills covered by the Showdown this month is as follows: 1.Stellar and galactic evolution 2.Spectral classification of stars 3.Hubble classification of galaxies 4.Observation using multiple portions of the electromagnetic spectrum 5.The relationship between stellar temperature, radius, and luminosity 6.Magnitude and luminosity scales, distance modulus, inverse square law 7.Identification of the stars, constellations, and deep sky objects included in the list below as they appear on star charts, H-R diagrams, portable star labs, photos, or planetariums. Note: Constellations are underlined; Stars are boldface; Deep Sky Objects are italicized. a.Andromeda: M31 (Andromeda Galaxy) b.Aquila: Altair c.Auriga: Capella d.Bootes: Arcturus e.Cancer: DLA0817g f.Canis Major: Sirius g.Canis Minor: Procyon h.Centaurus: NGC5128 i.Coma Berenices: NGC4676, NGC4555 j.Corvus: NGC4038/NGC4039 k.Crux: Dragonfish Nebula l.Cygnus: Deneb m.Dorado: 30 Doradus, LMC n.Gemini: Castor, Pollux o.Lyra: Vega p.Ophiuchus: Zeta Ophiuchi, Rho Ophiuchi cloud complex q.Orion: Betelgeuse, Rigel & M42 (Orion Nebula) r.Perseus: Algol, NGC1333 Science Olympiad, Inc. -
Annual Report 2007 ESO
ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2007 ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2007 presented to the Council by the Director General Prof. Tim de Zeeuw ESO is the pre-eminent intergovernmental science and technology organisation in the field of ground-based astronomy. It is supported by 13 countries: Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. Further coun- tries have expressed interest in member- ship. Created in 1962, ESO provides state-of- the-art research facilities to European as- tronomers. In pursuit of this task, ESO’s activities cover a wide spectrum including the design and construction of world- class ground-based observational facili- ties for the member-state scientists, large telescope projects, design of inno- vative scientific instruments, developing new and advanced technologies, further- La Silla. ing European cooperation and carrying out European educational programmes. One of the most exciting features of the In 2007, about 1900 proposals were VLT is the possibility to use it as a giant made for the use of ESO telescopes and ESO operates the La Silla Paranal Ob- optical interferometer (VLT Interferometer more than 700 peer-reviewed papers servatory at several sites in the Atacama or VLTI). This is done by combining the based on data from ESO telescopes were Desert region of Chile. The first site is light from several of the telescopes, al- published. La Silla, a 2 400 m high mountain 600 km lowing astronomers to observe up to north of Santiago de Chile.