Australia s Optical Data Centre
|
|
|
- Janel Poole
- 5 years ago
- Views:
Transcription
1 Australia s Optical Data Centre A Data Central and SkyMapper Collaboration Milky Way over the Pinnacles in Australia - Michael Goh
2 Explore Tools for data retrieval and automatic cross-matching make for intuitive and easy data exploration. Collaborate View and explore the data on our system collaboratively, manage your team and your data Science Rich & complex system to bring together data products from multiple surveys to facilitate new science with legacy and current surveys Australia s Optical Data Centre 2
3 NASA Ames/STScI/G. Bacon
4 Welcome back. Sign in to access your personalised data portal, collaborate with other researchers and manage your data Sign in with Data Central Sign in with SkyMapper Sign in with TAO Sign in with MWA Sign in with CASDA No account? Create one. Click Sign in above to accept our Terms of Service & Privacy Policy Milky Way over the Pinnacles in Australia - Michael Goh
5 Search Filter by 8 2 Data Central / NAVIGATION Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs Wiki ACTIVE JOBS 3 2 complete, 1 failed TOTAL DOWNLOADS 151 Last: 130 LATEST: 1D Spec LATEST: Light Curve STATISTICS 29 2 complete, 1 failed 1DSPEC DOWNLOAD 4,551 Last: 4,238 OzDES GAMA RA Dec OzDES DEVILS My Surveys 487 REDSHIFTS MEASURED 23,781 REDSHIFTS MEASURED LATEST: RGB My Articles VISTA-K VST-r GALEX-NUV OzDES GAMA RA Dec Title Date Using the AAT Archive 08/06/19 Integrating the 07/06/19 Data Release 1 07/06/19 manage My Notebooks Title Type Date My New Project Python 28/06/19 z > 3 galaxies R 10/05/19 HBeta line emi Python 21/04/19 manage LATEST: SED AAT Schedule manage Date Survey Observer 04/06/18 OzDES CLidman 12/07/18 DEVILS LDavies Cloud 13/07/18 Commissioning more Title Date Latest DR from OzDES 28/06/19 Support About OzDES GAMA RA Dec OzDES GAMA RA Dec Fast and slow rotato 10/05/19 HBeta line emission 21/04/19 manage
6 Search 8 2 OzDES Data Central / Single Object Viewer/ GAMA NAVIGATION J RA Dec SDSS_ObjID OzDES GAMA SAMI AAT Archive Tools Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs 1D Spec Light Curve SED Catalogues DATA RELEASE GROUP TABLE DR1 InputCat InputCatA OzDES_ID RA DEC z flag types OzDES_ StrongLens Wiki Cloud query Support About
7 Search 8 2 SAMI Data Central / Single Object Viewer/ GAMA NAVIGATION J RA Dec SDSS_ObjID OzDES GAMA SAMI AAT Archive Tools Surveys Cubes Spectra Data Access Cutout SOV Search Schema Archives Tools Notebooks Maps DATA RELEASE DR2 TYPE Velocity Map: Ionized Gas DATA RELEASE TYPE DATA RELEASE DR2 3kpc Aperture Spectrum: Blue DR2 TYPE Flux Cube: Blue Catalogues DATA RELEASE GROUP TABLE DR2 sami StellarKinemat.. CATID PA_STELKIN E_PA_STELKIN SIGMA_RE E_SIGMA_RE sigma_3kpc_ro e_sigma 3kpc Docs Wiki query Cloud Line-of-sight velocity map of ionized gas fit with a single Gaussian component Support About
8 Search 8 2 OzDES Data Central / Single Object Viewer/ GAMA NAVIGATION J RA Dec SDSS_ObjID OzDES GAMA SAMI AAT Archive Tools Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Greyscale Image Cutout BAND SCALING VSTKIDS-r log CONTOUR LEVELS MWA-GLEAM 4,8,12 UNITS hms, dms SOURCE POSITIONS GAMA DR2 RGB Image Cutout R VISTA-K VST-r UNITS SOURCE POSITIONS hms, dms GAMA DR2 G B GALEX-NUV Docs advanced advanced Wiki Cloud Support About
9 Search 8 2 Data Central / SQL / New NAVIGATION New History Builder Tools Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs Schema Browser Wiki DEVILS GAIA GALAH GAMA Hector Huntsman MWA OzDES RAVE SAMI SkyMapper TAIPAN WAVES Settings Cloud Support About
10 Search 8 2 Result Data Central / SQL / Result NAVIGATION Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs Wiki Cloud Support About
11 Search Filter by 8 2 Data Central / NAVIGATION Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs Wiki ACTIVE JOBS 3 2 complete, 1 failed TOTAL DOWNLOADS 151 Last: 130 LATEST: 1D Spec LATEST: Light Curve STATISTICS 29 2 complete, 1 failed 1DSPEC DOWNLOAD 4,551 Last: 4,238 OzDES GAMA RA Dec OzDES DEVILS My Surveys 487 REDSHIFTS MEASURED 23,781 REDSHIFTS MEASURED LATEST: RGB My Articles VISTA-K VST-r GALEX-NUV OzDES GAMA RA Dec Using the AAT Archive 08/06/19 Integrating the 07/06/19 Data Release 1 07/06/19 manage My Notebooks Title Type Date My New Project Python 28/06/19 z > 3 galaxies R 10/05/19 HBeta line emi Python 21/04/19 manage LATEST: SED AAT Schedule Title manage Date Date Survey Observer 04/06/18 OzDES CLidman 12/07/18 DEVILS LDavies Cloud 13/07/18 Commissioning more Title Date Latest DR from OzDES 28/06/19 Support About OzDES GAMA RA Dec OzDES GAMA RA Dec Fast and slow rotato 10/05/19 HBeta line emission 21/04/19 manage
12 Search 8 2 My New Project Data Central / Notebooks/ My New Project NAVIGATION Last edited: June Surveys Code Settings E K C + Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs Wiki Cloud Support About
13 Search 8 2 My Files Data Central / Cloud NAVIGATION Last edited: June Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks mysurvey_dr2 35GB Publish Publish DEVILS DR2 back to Data Central. Need Help? Check out the Getting Started Guide Docs Wiki Cloud Support About
14 Search 8 2 Paper ment Data Central / Papers NAVIGATION Last edited: June GAMA OzDES DEVILS Hector WAVES TAIPAN Settings Surveys Data Access Cutout SOV Search Schema Archives Tools Notebooks Docs Mark as CW LM KS LM KS Showing 6 of 21 Latest All GAMA Papers GROUP Group Finding Probing dark matter and galaxy evolution with proper motions of galaxies Measurement of the primordial helium abundance from the intergalactic medium Investigating the X-ray enhancements of highly radio-loud quasars at z > 4 Understanding mechanical feedback from HERGs and LERGs The spin alignment of galaxies with the largescale tidal field in hydrodynamic simulations Showing 1 of 8 groups Action REVIEW REFEREE COMMENTS PROVIDE COMMENTS REVIEW CO-AUTHORS REVIEW COMMENTS REVIEW COMMENTS 6 per page Title Status Authors Probing dark matter and galaxy evolution with proper motions of galaxies IN PROGRESS KS LM + 4 more My Papers Recent Probing dark matter and 06/06/2019 Measurement of the primord 12/07/2019 Investigating the X-ray 12/07/2019 Understanding mechanical 12/07/2019 The spin alignment of galaxi 12/07/2019 Showing 5 of 12 Status SUBMITTED PUBLISHED IN PROGRESS PUBLISHED PUBLISHED View all TOTAL PROPOSED 74 Since Dec 2018 ACTIVE 15 5 in EnvironmentMeasures PUBLISHED 29 MNRAS, APJ SUBMITTED 14 MNRAS, APJ UNASSIGNED 16 5 in EnvironmentMeasures Wiki Cloud Measurement of the primordial helium abundance from the intergalactic medium Investigating the X-ray enhancements of highly radio-loud quasars at z > 4 UNASSIGNED AWAITING APPROVAL LD RM + 4 more Understanding mechanical feedback from HERGs and LERGs SUBMITTED The spin alignment of galaxies with the large-scale tidal field in hydrodynamic simulations KS PUBLISHED CW + 24 more Support About Showing 6 of 74 6 per page
15 Explore Collaborate Science Datasets Tens of millions of galaxies Billions of stars All-sky coverage in multiple bands Thousands of cubes Millions of spectra SAMI OzDES GAIA GALAH RAVE GAMA S7 AAPS WIGGLEZ Huntsman 6dFGS TAIPAN 2dFGRS FunnelWeb SkyMapper DEVILS Many small (lost) datasets! WAVES Hector? your data here? your survey here Australia s Optical Data Centre 15
16 Archives UKSCHMIDT.. SKYMAPPER & ANU 2.3M.. AAT.. HUNTSMAN..
17 Explore Collaborate Science ESO Integrated access to ESO archive Data visualisation tools compatible with ESO data products ESO Archive LSST SKA Data Centre VIEW IN Seamless interoperability Australia s Optical Data Centre 17
18 DATA PROVIDED BY: Australia s Optical Data Centre Catalog and Classify Millions of Galaxies Lorem ipsum dolor sit amet, consectetur adipiscing elit, sed do eiusmod tempor incididunt ut labore et dolore magna aliqua. Ut enim ad minim veniam, quis nostrud exercitation ullamco laboris nisi ut aliquip ex ea commodo consequat. Australia s Optical Data Centre 18
19 DATA PROVIDED BY: Australia s Optical Data Centre CITIZEN SCIENCE OUTREACH EDUCATIONAL PROGRAMS TOOLS LATEST New Galaxies, new Galaxy Zoo! 06/06/2019 Discovered galaxy cluster named after two citizen scientists 12/07/2019 New Tool: What is redshift? 12/07/2019 Video: The SAMI instrument and Survey 12/07/2019 Read more Australia s Optical Data Centre 19
20 Data Centres Milky Way over the Pinnacles in Australia - Michael Goh
PROJECT TITLE. B.Tech. BRANCH NAME NAME 2 (ROLL NUMBER)
PROJECT TITLE A thesis submitted in partial fulfillment of the requirements for the award of the degree of B.Tech. in BRANCH NAME By NAME 1 (ROLL NUMBER) NAME 2 (ROLL NUMBER) DEPARTMENT OF DEPARTMENT NAME
Dorset Coastal Explorer Planning
Dorset Coastal Explorer Planning Please read this information carefully. If you wish to proceed after reading this information you must signify your agreement to the following conditions of access by selecting
CLEAR SPACE AND MINIMUM SIZE. A clear space area free of competing visual elements should be maintained.
BRAND TOOL KIT LOGO The preferred logoversion to use is on white background. Negative version is reversed (white) on a dark blue background. Also a black and white version is available for 1-colour print
Text Analysis. Week 5
Week 5 Text Analysis Reference and Slide Source: ChengXiang Zhai and Sean Massung. 2016. Text Data Management and Analysis: a Practical Introduction to Information Retrieval and Text Mining. Association
Brand guidelines 2014
Brand guidelines 2014 // master logo // master logo & alternative colour breakdowns Blue C: 100 M: 95 Y: 5 K: 0 R: 43 G: 57 B: 144 #2b3990 // master logo - alternate colourful version // master logo -
Introduction to the Sloan Survey
Introduction to the Sloan Survey Title Rita Sinha IUCAA SDSS The SDSS uses a dedicated, 2.5-meter telescope on Apache Point, NM, equipped with two powerful special-purpose instruments. The 120-megapixel
MEDIA KIT D E S T I N A T I O N S M A G A Z I N E D E S T I N A T I O N S M A G A Z I N E. C O M
MEDIA KIT 201 8 D E S T I N A T I O N S M A G A Z I N E 2 0 1 8 D E S T I N A T I O N S M A G A Z I N E. C O M O U R B R A N D A platform for those consumed by wanderlust. D E S T I N A T I O N S M A G
Recurrent Neural Networks. COMP-550 Oct 5, 2017
Recurrent Neural Networks COMP-550 Oct 5, 2017 Outline Introduction to neural networks and deep learning Feedforward neural networks Recurrent neural networks 2 Classification Review y = f( x) output label
USER MANUAL. ICIM S.p.A. Certifi cation Mark
USER MANUAL ICIM S.p.A. Certifi cation Mark Index Informative note 4 The Certifi cation Mark 6 Certifi ed Management System 8 Certifi ed Management System: Examples 20 Certifi ed Product 28 Certifi ed
{SOP_Title} Standard Operating Procedure. Owner: {SOP_Author} {SOP_Description} {SOP_ID} {Date}
Standard Operating Procedure {SOP_Title} {SOP_Description} {SOP_ID} {Date} {Company_Name} Phone: {Company_Phone} {Company_Website} Owner: {SOP_Author} Table of Contents 1. Purpose 3 2. Terminology 4 3.
Week 7 Sentiment Analysis, Topic Detection
Week 7 Sentiment Analysis, Topic Detection Reference and Slide Source: ChengXiang Zhai and Sean Massung. 2016. Text Data Management and Analysis: a Practical Introduction to Information Retrieval and Text
How to give. an IYPT talk
How to give Today you will learn: 1. What is IYPT and where is it from 2. How US was involved before 3. How to craft physics arguments 4. How to use presentation tricks 5. How to criticize flaws an IYPT
Neural Networks for NLP. COMP-599 Nov 30, 2016
Neural Networks for NLP COMP-599 Nov 30, 2016 Outline Neural networks and deep learning: introduction Feedforward neural networks word2vec Complex neural network architectures Convolutional neural networks
The Dark Energy Survey Public Data Release 1
The Dark Energy Survey Public Data Release 1 Matias Carrasco Kind (NCSA/UIUC) and the DR1 Release Team https://des.ncsa.illinois.edu/ Near-Field Cosmology with DES DR1 and Beyond Workshop, June 27-29th,
KING AND GODFREE SALAMI FEST MARCH TEN LYGON STREET CARLTON
Pidapipo KING AND GODFREE SALAMI FEST MARCH TEN LYGON STREET CARLTON ON HOVER: RED OVERLAY, WHITE TEXT BANNER HYPERLINKED TO EVENT IN NEWS PAGE FIXED FOOTER. ON HOVER: RED ON CLICK: MENU SLIDES FROM LEFT.
Reduced data products in the ESO Phase 3 archive (Status: 02 August 2017)
Reduced data products in the ESO Phase 3 archive (Status: 02 August 2017) The ESO Phase 3 archive provides access to reduced and calibrated data products. All these data are stored in standard formats
The Cosmic Evolution of Neutral Atomic Hydrogen Gas Philip Lah
The Cosmic Evolution of Neutral Atomic Hydrogen Gas Philip Lah University of Sydney Colloquium 27 November 2014 Collaborators: Frank Briggs (ANU) Jayaram Chengalur (NCRA) Matthew Colless (ANU) Roberto
Real Astronomy from Virtual Observatories
THE US NATIONAL VIRTUAL OBSERVATORY Real Astronomy from Virtual Observatories Robert Hanisch Space Telescope Science Institute US National Virtual Observatory About this presentation What is a Virtual
Rick Ebert & Joseph Mazzarella For the NED Team. Big Data Task Force NASA, Ames Research Center 2016 September 28-30
NED Mission: Provide a comprehensive, reliable and easy-to-use synthesis of multi-wavelength data from NASA missions, published catalogs, and the refereed literature, to enhance and enable astrophysical
Celebrating PHILANTHROPY. Brian Hew
Celebrating PHILANTHROPY Brian Hew Publisher / Editor-in-Chief Beaver Shriver Beaver@GiveSarasota.com Editor Viia Beaumanis VBeaumanis@gmail.com Welcome to GIVE Sarasota! em ipsum dolor sit amet, consectetuer
The Cosmic Evolution of Neutral Atomic Hydrogen Gas. Philip Lah. Macquarie University Colloquium 27th March 2015
The Cosmic Evolution of Neutral Atomic Hydrogen Gas Philip Lah Macquarie University Colloquium 27th March 2015 Collaborators: Frank Briggs (ANU) Jayaram Chengalur (NCRA) Matthew Colless (ANU) Roberto De
HI in Galaxies at Redshifts 0.1 to 1.0: Current and Future Observations Using Optical Redshifts for HI Coadding. Philip Lah
HI in Galaxies at Redshifts 0.1 to 1.0: Current and Future Observations Using Optical Redshifts for HI Coadding Philip Lah Deep Surveys of the Radio Universe with SKA Pathfinders Collaborators: Frank Briggs
Sediment Management for Coastal Restoration in Louisiana -Role of Mississippi and Atchafalaya Rivers
Sediment Management for Coastal Restoration in Louisiana -Role of Mississippi and Atchafalaya Rivers Syed M. Khalil Louisiana Applied Coastal Engineering & Science (LACES) Division 9 th INTECOL International
Exemplo de Apresentação
Exemplo de Apresentação Subtítulo: sthlm v2.0.2 baseado em hsrm & mtheme -Autor- MarkOlson.SE Data: 2017/04/24 Universidade de Brasília File: apresentacao_unb Overview 1. General Information 2. Colors
Science and Status of the Maunakea Spectroscopic Explorer
Science and Status of the Maunakea Spectroscopic Explorer Science and status of the Alan McConnachie MSE Project Scientist CFHT Users Meeting, May 3 2016 Maunakea Spectroscopic Explorer Alan McConnachie
Public ESO
Public Surveys @ ESO Magda Arnaboldi, Head - Archive Science Group marnabol@eso.org EST (M. Hilker, G. Hussain, M. Petr-Gotzens, M. Rejkuba) ASG (N. Delmotte, S. Geier, A. Micol, J. Retzlaff) Outline Why
STELLAR DYNAMICS IN THE NUCLEI OF M31 AND M32: EVIDENCE FOR MASSIVE BLACK HOLES A LAN D RESSLER
STELLAR DYNAMICS IN THE NUCLEI OF M31 AND M32: EVIDENCE FOR MASSIVE BLACK HOLES A LAN D RESSLER ABSTRACT 이웃하는두은하인 M32, M32 의중심에거대블랙홀이있는것같다!! Ca II M31, M32, maximum entropy technique 3 2 M31, M32 M/L masses
Introduction to SDSS -instruments, survey strategy, etc
Introduction to SDSS -instruments, survey strategy, etc (materials from http://www.sdss.org/) Shan Huang 17 February 2010 Survey type Status Imaging and Spectroscopy Basic Facts SDSS-II completed, SDSS-III
Linear Algebra. Dave Bayer
Linear Algebra Dave Bayer c 2007 by Dave Bayer All rights reserved Projective Press New York, NY USA http://projectivepress.com/linearalgebra Dave Bayer Department of Mathematics Barnard College Columbia
ESASky, ESA s new open-science portal for ESA space astronomy missions
ESASky, ESA s new open-science portal for ESA space astronomy missions Bruno Merín ESAC Science Data Centre European Space Agency bruno.merin@esa.int Visit to NAOC, Beijing, 19/05/2017 ESA UNCLASSIFIED
Lecture Outlines. Chapter 25. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 25 Astronomy Today 7th Edition Chaisson/McMillan Chapter 25 Galaxies and Dark Matter Units of Chapter 25 25.1 Dark Matter in the Universe 25.2 Galaxy Collisions 25.3 Galaxy Formation
Cosmology with the ESA Euclid Mission
Cosmology with the ESA Euclid Mission Andrea Cimatti Università di Bologna Dipartimento di Astronomia On behalf of the Euclid Italy Team ESA Cosmic Vision 2015-2025 M-class Mission Candidate Selected in
ALFALFA: The Arecibo Legacy Fast ALFA Survey: Martha Haynes (Cornell)
ALFALFA: The Arecibo Legacy Fast ALFA Survey: Martha Haynes (Cornell) 1. Determination of the faint end of the HI Mass Function and the abundance of low mass gas rich halos 2. Environmental variation in
Measuring star formation in galaxies and its evolution. Andrew Hopkins Australian Astronomical Observatory
Measuring star formation in galaxies and its evolution Andrew Hopkins Australian Astronomical Observatory Evolution of Star Formation Evolution of Star Formation Evolution of Star Formation Evolution of
Flagging Bad Data in Imaging
Flagging Bad Data Flagging Bad Data in Imaging Observations are never perfect, due to observing conditions e.g., bad seeing, moonlight, the solar wind, clouds, airplanes, cosmic rays, telescope malfunctions
Data challenges of the Virtual Observatory in Time Domain Astronomy
Data challenges of the Virtual Observatory in Time Domain Astronomy Ada Nebot Gomez-Moran Astronomical Data Analysis Software & Systems Nov. 11-15 2018 Time Domain Astronomy The study of variability of
Data Release 5. Sky coverage of imaging data in the DR5
Data Release 5 The Sloan Digital Sky Survey has released its fifth Data Release (DR5). The spatial coverage of DR5 is about 20% larger than that of DR4. The photometric data in DR5 are based on five band
RLW paper titles:
RLW paper titles: http://www.wordle.net Astronomical Surveys and Data Archives Richard L. White Space Telescope Science Institute HiPACC Summer School, July 2012 Overview Surveys & catalogs: Fundamental
Pleo Mobile Strategy
Pleo Mobile Strategy Lorem ipsum dolor sit amet, consectetur adipiscing elit, sed do eiusmod tempor incididunt ut labore et dolore magna aliqua. Nunc lobortis mattis aliquam faucibus purus in massa. Convallis
Big-Data as a Challenge for Astrophysics
Big-Data as a Challenge for Astrophysics ESA / Euclid Consortium Hubble deep field, NASA/STScI HESS collaboration, F. Acero and H. Gast ESA/ATG medialab; ESO/S. Brunier Volker Beckmann Institut National
Galaxy formation and evolution. Astro 850
Galaxy formation and evolution Astro 850 Introduction What are galaxies? Systems containing many galaxies, e.g. 10 11 stars in the Milky Way. But galaxies have different properties. Properties of individual
Time Domain Surveys: Proper Motion
Time Domain Surveys: Proper Motion Time Domain Surveys: Parallax Another use of data from time domain surveys is the measurement of proper motion and parallax Parallax is the change in a star s position
Astroinformatics: massive data research in Astronomy Kirk Borne Dept of Computational & Data Sciences George Mason University
Astroinformatics: massive data research in Astronomy Kirk Borne Dept of Computational & Data Sciences George Mason University kborne@gmu.edu, http://classweb.gmu.edu/kborne/ Ever since humans first gazed
Continuous Performance Testing Shopware Developer Conference. Kore Nordmann 08. June 2013
Continuous Performance Testing Shopware Developer Conference Kore Nordmann (@koredn) 08. June 2013 About Me Kore Nordmann @koredn Co-founder of Helping people to create high quality web applications. http://qafoo.com
Age-redshift relation. The time since the big bang depends on the cosmological parameters.
Age-redshift relation The time since the big bang depends on the cosmological parameters. Lyman Break Galaxies High redshift galaxies are red or absent in blue filters because of attenuation from the neutral
Brand Guidelines Preparation for winter << name here >> North East Lincolnshire Leeds
Brand Guidelines Contents Introduction.... 3 The logo................................. 4 Exclusion zone... 5 Do s & don ts.... 6 Cold weather plan levels.... 7 Creating sub brand logos... 9 The Winter
The GALEX Observations of Planetary Nebulae. Ananta C. Pradhan 1, M. Parthasarathy 2, Jayant Murthy 3 and D. K. Ojha 4
The GALEX Observations of Planetary Nebulae. Ananta C. Pradhan 1, M. Parthasarathy 2, Jayant Murthy 3 and D. K. Ojha 4 1 National Institute of Technology, Odisha 769008, India 2 Inter-University Centre
GOODS/VIMOS Spectroscopy: Data Release Version 2.0.1
ESO Phase 3 Data Release Description Data Collection GOODS_VIMOS_SPEC Release Number 1 Data Provider C. Cesarsky Date 10.03.2010 Migrated to Phase 3 infrastructure 08.12.2014 GOODS/VIMOS Spectroscopy:
ALFALFA status Jan Martha Haynes Cornell University UAT13 Jan 2013
ALFALFA status Jan 2013 Martha Haynes Cornell University UAT13 Jan 2013 ALFALFA observing status Jan 2013 It s done! ALFALFA catalog & results ALFALFA 40%: α40 catalog published! Included in data products:
Studying galaxies with the Sloan Digital Sky Survey
Studying galaxies with the Sloan Digital Sky Survey Laboratory exercise, Physics of Galaxies, Spring 2017 (Uppsala Universitet) by Beatriz Villarroel *** The Sloan Digital Sky Survey (SDSS) is the largest
Investigation of Radio Structures of High-z QSOs by VLBI Observation
Investigation of Radio Structures of High-z QSOs by VLBI Observation Challenges of 512 Frey et al.: High resolution radio imaging parsec-scale jet component speeds (Fig. 4). More radio luminous sources
The Hale Solar Sector Boundary - Revisited
Solar Physics DOI: 10.1007/ˆˆˆˆˆ-ˆˆˆ-ˆˆˆ-ˆˆˆˆ-ˆ The Hale Solar Sector Boundary - Revisited L. Svalgaard P.H. Scherrer The Authors (2010) ˆˆˆˆ Abstract Lorem ipsum dolor sit amet, consectetuer adipiscing
The First Galaxies. Erik Zackrisson. Department of Astronomy Stockholm University
The First Galaxies Erik Zackrisson Department of Astronomy Stockholm University Outline The first galaxies what, when, why? What s so special about them? Why are they important for cosmology? How can we
D4.2. First release of on-line science-oriented tutorials
EuroVO-AIDA Euro-VO Astronomical Infrastructure for Data Access D4.2 First release of on-line science-oriented tutorials Final version Grant agreement no: 212104 Combination of Collaborative Projects &
Hubble Legacy Archive and Hubble Source Catalog
Hubble Legacy Archive and Hubble Source Catalog Rick White & Brad Whitmore Current teams: HLA: Michael Dulude, Mark Kyprianou, Steve Lubow, Brian McLean, Lee Quick, Lou Strolger, Rick White HSC: Tamás
Downtown: Location of Choice for Living 13. Message from the President 2. Downtown: Location of Choice for Business 7
Alliance for Downtown New York 2008 Message from the President 2 Downtown: Location of Choice for Business 7 Downtown: Location of Choice for Living 13 Downtown: Location of Choice for Recreation 17 Downtown:
GOODS/FORS2 Final Data Release: Version 3.0
ESO Phase 3 Data Release Description Data Collection GOODS_FORS2 Release Number 1 Data Provider C. Cesarsky Date 30.10.2007 update 11.07.2014 GOODS/FORS2 Final Data Release: Version 3.0 As part of the
Studies of diffuse UV radiation
Bull. Astr. Soc. India (2007) 35, 295 300 Studies of diffuse UV radiation N. V. Sujatha and Jayant Murthy Indian Institute of Astrophysics, Bangalore 560 034, India Abstract. The upcoming TAUVEX mission
VISTA HEMISPHERE SURVEY DATA RELEASE 1
Release date (will be set by ESO) VISTA HEMISPHERE SURVEY DATA RELEASE 1 PROPOSAL ESO No.: 179.A-2010 PRINCIPAL INVESTIGATOR: Richard McMahon Authors: R. McMahon, M. Banerji, N. Lodieu for the VHS Collaboration
The Secrets of Galaxies. Student s Guide Advanced Level CESAR s Science Case
The Secrets of Galaxies Student s Guide Advanced Level Introduction Galaxies are fundamental building blocks of the Universe. Some are simple, while others are very complex in structure; some have enormous
Unusual orbits in the Andromeda galaxy Post-16
Unusual orbits in the Andromeda galaxy Post-16 Topics covered: spectra, Doppler effect, Newton s law of gravitation, galaxy rotation curves, arc lengths, cosmological units, dark matter Teacher s Notes
Dr Carolyn Devereux - Daphne Jackson Fellow Dr Jim Geach Prof. Martin Hardcastle. Centre for Astrophysics Research University of Hertfordshire, UK
Millennium simulation of the cosmic web MEASUREMENTS OF THE LINEAR BIAS OF RADIO GALAXIES USING CMB LENSING FROM PLANCK Dr Carolyn Devereux - Daphne Jackson Fellow Dr Jim Geach Prof. Martin Hardcastle
ALFALFA status Jan 2012
ALFALFA status Jan 2012 UAT11 Martha Haynes Cornell University UAT12 Jan 2012 ALFALFA observing status Jan 2012 We hope to complete the drift scan survey in Fall 2012! ALFALFA catalog & results ALFALFA
NASA/IPAC EXTRAGALACTIC DATABASE
GRITS 2009 NASA/IPAC EXTRAGALACTIC DATABASE 20 years, 163 million objects, 3.3 billion rows, and beyond The Team Rick Ebert presenting What is? Mission A brief history 20 years, 3 dbms, multiple uif The
(Astro)Physics 343 Lecture # 13: cosmic microwave background (and cosmic reionization!)
(Astro)Physics 343 Lecture # 13: cosmic microwave background (and cosmic reionization!) Welcome back! (four pictures on class website; add your own to http://s304.photobucket.com/albums/nn172/rugbt/) Results:
Probing the history of star formation in the Local Group using the galactic fossil record
Probing the history of star formation in the Local Group using the galactic fossil record Brian O Shea (Michigan State University) Collaborators: Tim Beers, Carolyn Peruta, Monica Derris (MSU), Jason Tumlinson
Large Synoptic Survey Telescope
Large Synoptic Survey Telescope Željko Ivezić University of Washington Santa Barbara, March 14, 2006 1 Outline 1. LSST baseline design Monolithic 8.4 m aperture, 10 deg 2 FOV, 3.2 Gpix camera 2. LSST science
JINA Observations, Now and in the Near Future
JINA Observations, Now and in the Near Future Timothy C. Beers Department of Physics & Astronomy Michigan State University & JINA: Joint Institute for Nuclear Astrophysics Examples SDSS-I, II, and III
Blazars behind the Magellanic Clouds
Blazars behind the Magellanic Clouds Natalia Żywucka-Hejzner In collaboration with Michał Ostrowski, Arti Goyal, Łukasz Stawarz, Marek Jamrozy, Szymon Kozłowski, and Andrzej Udalski Astronomical Observatory
PDF hosted at the Radboud Repository of the Radboud University Nijmegen
PDF hosted at the Radboud Repository of the Radboud University Nijmegen The following full text is a publisher's version. For additional information about this publication click this link. http://hdl.handle.net/2066/84153
Yuji Shirasaki. National Astronomical Observatory of Japan. 2010/10/13 Shanghai, China
Yuji Shirasaki National Astronomical Observatory of Japan 1 Virtual Observatory Infrastructure for efficient research environment International standard for data publication & access Sharing data worldwide,
From the VLT to ALMA and to the E-ELT
From the VLT to ALMA and to the E-ELT Mission Develop and operate world-class observing facilities for astronomical research Organize collaborations in astronomy Intergovernmental treaty-level organization
Galaxy and Mass Assembly (GAMA): Evolution of the mass-size relation
Galaxy and Mass Assembly (GAMA): Evolution of the mass-size relation Jon Loveday University of Sussex!!&% "@""%,- 7-) #-7 % A 89 : % 4 #-@" ;
NEW CONSTRAINTS ON THE BLACK HOLE SPIN IN RADIO LOUD QUASARS
NEW CONSTRAINTS ON THE BLACK HOLE SPIN IN RADIO LOUD QUASARS Andreas Schulze (NAOJ, EACOA Fellow)) Chris Done, Youjun Lu, Fupeng Zhang, Yoshiyuki Inoue East Asian Young Astronomers Meeting, EAYAM 2017
LSST, Euclid, and WFIRST
LSST, Euclid, and WFIRST Steven M. Kahn Kavli Institute for Particle Astrophysics and Cosmology SLAC National Accelerator Laboratory Stanford University SMK Perspective I believe I bring three potentially
Rajib Ganguly (University of Michigan-Flint)
Rajib Ganguly (University of Michigan-Flint) A major theme in most recent simulations of galaxy evolution is AGN feedback, quantified by the kinetic luminosity, or power. In this ongoing work, we wish
Our Galaxy. Milky Way Galaxy = Sun + ~100 billion other stars + gas and dust. Held together by gravity! The Milky Way with the Naked Eye
Our Galaxy Milky Way Galaxy = Sun + ~100 billion other stars + gas and dust Held together by gravity! The Milky Way with the Naked Eye We get a special view of our own galaxy because we are part of it!
Characterizing the Gigahertz radio sky
THE US NATIONAL VIRTUAL OBSERVATORY Mining multi-wavelength data in large area surveys with VO tools Yogesh Wadadekar STScI This work is partly supported by a NVO Research Initiative award. Collaborator:
Let s Get Visual. Michelle Samplin-Salgado Andrea Goetschius Liesl Lu
Let s Get Visual Michelle Samplin-Salgado Andrea Goetschius Liesl Lu CBA@JSI Today s Presenters MICHELLE ANDI LIESL WHERE ARE WE GOING? Basic principles of design How effective design can improve the promotion
Putting Weirdness to Work: Quantum Information Science QIS. Quantum Computer
Putting Weirdness to Work: Quantum Information Science QIS Quantum Computer John Preskill, Caltech Biedenharn Lecture 6 September 2005 ??? 2005 2100 ??? 2005 Q Information is encoded in the state of a
Quasars in the SDSS. Rich Kron NGC June 2006 START CI-Team: Variable Quasars Research Workshop Yerkes Observatory
Quasars in the SDSS Rich Kron 28 June 2006 START CI-Team: Variable Quasars Research Workshop Yerkes Observatory NGC 1068 About 10% of all of the spectra in the SDSS database are of quasars (as opposed
VOSA. A VO Spectral Energy Distribution Analyzer. Carlos Rodrigo Blanco 1,2 Amelia Bayo Arán 3 Enrique Solano 1,2 David Barrado y Navascués 1
VOSA A VO Spectral Energy Distribution Analyzer Carlos Rodrigo Blanco 1,2 Amelia Bayo Arán 3 Enrique Solano 1,2 David Barrado y Navascués 1 1 CAB,INTA-CSIC 2 Spanish Virtual Observatory 3 European Southern
Scientific Data Flood. Large Science Project. Pipeline
The Scientific Data Flood Scientific Data Flood Large Science Project Pipeline 1 1 The Dark Energy Survey Study Dark Energy using four complementary* techniques: I. Cluster Counts II. Weak Lensing III.
Cosmology on the Beach: Experiment to Cosmology
Image sky Select targets Design plug-plates Plug fibers Observe! Extract spectra Subtract sky spec. Cosmology on the Beach: Experiment to Cosmology Fit redshift Make 3-D map Test physics! David Schlegel!1
Searching for Needles in the Sloan Digital Haystack
Searching for Needles in the Sloan Digital Haystack Robert Lupton Željko Ivezić Jim Gunn Jill Knapp Michael Strauss University of Chicago, Fermilab, Institute for Advanced Study, Japanese Participation
The Sloan Digital Sky Survey
The Sloan Digital Sky Survey Robert Lupton Xiaohui Fan Jim Gunn Željko Ivezić Jill Knapp Michael Strauss University of Chicago, Fermilab, Institute for Advanced Study, Japanese Participation Group, Johns
CHAPTER 28 STARS AND GALAXIES
CHAPTER 28 STARS AND GALAXIES 28.1 A CLOSER LOOK AT LIGHT Light is a form of electromagnetic radiation, which is energy that travels in waves. Waves of energy travel at 300,000 km/sec (speed of light Ex:
Quasars and Active Galactic Nuclei (AGN)
Quasars and Active Galactic Nuclei (AGN) Astronomy Summer School in Mongolia National University of Mongolia, Ulaanbaatar July 21-26, 2008 Kaz Sekiguchi Hubble Classification M94-Sa M81-Sb M101-Sc M87-E0
Mario Santos (on behalf of the Cosmology SWG) Stockholm, August 24, 2015
Mario Santos (on behalf of the Cosmology SWG) Stockholm, August 24, 2015 Why is the expansion of the Universe accelerating? Dark energy? Modified gravity? What is the nature of the primordial Universe?
Dark Matter. ASTR 333/433 Spring Today Stars & Gas. essentials about stuff we can see. First Homework on-line Due Feb. 4
Dark Matter ASTR 333/433 Spring 2016 Today Stars & Gas essentials about stuff we can see First Homework on-line Due Feb. 4 Galaxies are made of stars - D. Silva (1990) private communication Stars Majority
SDSS Data Management and Photometric Quality Assessment
SDSS Data Management and Photometric Quality Assessment Željko Ivezić Princeton University / University of Washington (and SDSS Collaboration) Thinkshop Robotic Astronomy, Potsdam, July 12-15, 2004 1 Outline
Quasar Absorption Lines
Tracing the Cosmic Web with Diffuse Gas DARK MATTER GAS STARS NEUTRAL HYDROGEN Quasar Absorption Lines use quasars as bright beacons for probing intervening gaseous material can study both galaxies and
The Iguaçu Lectures. Nonlinear Structure Formation: The growth of galaxies and larger scale structures
April 2006 The Iguaçu Lectures Nonlinear Structure Formation: The growth of galaxies and larger scale structures Simon White Max Planck Institute for Astrophysics z = 0 Dark Matter ROT EVOL Cluster structure
Formation of z~6 Quasars from Hierarchical Galaxy Mergers
Formation of z~6 Quasars from Hierarchical Galaxy Mergers Yuexing Li et al Presentation by: William Gray Definitions and Jargon QUASAR stands for QUASI-stellAR radio source Extremely bright and active
Life In The Forests Of The Far East Or, Travels In Northern Borneo Volume 1 By Spenser St. John READ ONLINE
Life In The Forests Of The Far East Or, Travels In Northern Borneo Volume 1 By Spenser St. John READ ONLINE If searching for a book by Spenser St. John Life in the forests of the Far East or, Travels in
Chandra: the Next Decade
Chandra The Next Decade Cyg A Tycho Crab 2016: Excellent Senior Review Results! Belinda Wilkes Director Chandra X-ray Center Cen A Chandra:17 years and counting! Detailed engineering review showed no show-stoppers
GMRT observations of radio halo clusters
GMRT observations of radio halo clusters Viral Parekh Raman Research Institute Bangalore Collaborators K.S. Dwarakanath (RRI), Ruta Kale (NCRA), and Huib Intema (Leiden Observatory) SPARCS Meeting, November,
CONFIRMATION OF A SUPERNOVA IN THE GALAXY NGC6946
CONFIRMATION OF A SUPERNOVA IN THE GALAXY NGC6946 G. Iafrate and M. Ramella INAF - Astronomical Observatory of Trieste 1 Introduction Suddenly a star runs out its nuclear fuel. Its life as a normal star
A unique. Living Heritage
A unique Living Heritage Innovative Materials Rich Colour Palette PANTONE 2695 PANTONE 549 PANTONE 4515 PANTONE 532 PANTONE 201 PANTONE 159 PANTONE 623 PANTONE 577 PANTONE Warm Grey 1 Illustration Style
The Universe in the Cloud. Darren Croton Centre for Astrophysics and Supercomputing Swinburne University
PART III The Universe in the Cloud Darren Croton Centre for Astrophysics and Supercomputing Swinburne University dcroton@astro.swin.edu.au Let s recap... The skeleton The flesh Schmidt law star formation