Zone 252, Master Map Normal View

Zone 258, Master Map Normal View

Zone Master, Normal View, 10 deg FOV Zone 258, Master Map Normal View Hydra Vela κ ε δ γ Pyxis α ζ β η ρ ξ ο M93-38 00' -36 00' -34 00' -32 00' -30 00' -28 00' -26 00' -24 00' ζ Puppis 09h 28m 09h 20m

Zone 257, Master Map Normal View

Zone Master, Normal View, 10 deg FOV, Master Map Normal View ρ ξ ο Puppis τ η ludra π ω Canis Major δ Wezen σ ε ο1 dhara κ Colum -38 00' -36 00' -34 00' -32 00' -30 00' -28 00' -26 00' -24 00' ζ 08h 32m

Zone 102, Master Map Normal View

Zone Master, Normal View, 10 deg FOV Zone 102, Master Map Normal View α Deneb δ North merican Nebula ξ ν λ Pelican Nebula Cygnus γ M29 Sadr Crescent Nebula +36 00' +38 00' +40 00' +42 00' +44 00' η 21h

Zone 136, Master Map Normal View

Zone Master, Normal View, 10 deg FOV Zone 136, Master Map Normal View ε Mebsuta ζ ω Mekbuda γ lhena ν µ Orion η Propus M35 Gemini χ2 Taurus χ1 +16 00' +18 00' +20 00' +22 00' +24 00' ν ξ 07h 04m 06h 56m

Binocular Targets: Omega Centauri is also a good object to view in binoculars.

Eridanus Optics CC April 2006 Targets in Centaurus The following three targets are selected from the Constellation 'Centaurus' to present a naked eye challenge, as well as telescopic challenges. Binoculars

Eridanus Optics CC. August Deep sky targets in Aquarius. Introduction

Eridanus Optics CC August 2008 Deep sky targets in Aquarius. Introduction Aquarius is one of the zodiacal constellations. The Sun passes through Aquarius from late February to mid March. In August (six

Mathematics Review Exercises. (answers at end)

Brock University Physics 1P21/1P91 Mathematics Review Exercises (answers at end) Work each exercise without using a calculator. 1. Express each number in scientific notation. (a) 437.1 (b) 563, 000 (c)

T m / A. Table C2 Submicroscopic Masses [2] Symbol Meaning Best Value Approximate Value

APPENDIX C USEFUL INFORMATION 1247 C USEFUL INFORMATION This appendix is broken into several tables. Table C1, Important Constants Table C2, Submicroscopic Masses Table C3, Solar System Data Table C4,

Rømer Science Mission Plan

Institute of Physics and Astronomy, University of Aarhus Rømer Science Mission Plan Danish Small Satellite Programme Document No.(issue): MONS/IFA/MAN/PLN/0001(1) Date: 2001-05-29 Prepared by: Jørgen Christensen-Dalsgaard,

Entities for Symbols and Greek Letters

Entities for Symbols and Greek Letters The following table gives the character entity reference, decimal character reference, and hexadecimal character reference for symbols and Greek letters, as well

. α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω. Friday April 1 ± ǁ

. α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω Friday April 1 ± ǁ 1 Chapter 5. Photons: Covariant Theory 5.1. The classical fields 5.2. Covariant

How to Understand Stars Chapter 17 How do stars differ? Is the Sun typical? Location in space. Gaia. How parallax relates to distance

How to Understand Stars Chapter 7 How do stars differ? Is the Sun typical? Image of Orion illustrates: The huge number of stars Colors Interstellar gas Location in space Two dimensions are easy measure

Lecture 16 The Measuring the Stars 3/26/2018

Lecture 16 The Measuring the Stars 3/26/2018 Test 2 Results D C B A Questions that I thought were unfair: 13, 18, 25, 76, 77, 80 Curved from 85 to 79 Measuring stars How far away are they? How bright are

Spring Messier List Observing Club

Spring Messier List Observing Club Raleigh Astronomy Club Version 1.1 24 November 2012 Introduction Welcome to the Spring Messier List Observing Club. The objects on this list represent many of the most

Fall Messier List Observing Club

Fall Messier List Observing Club Raleigh Astronomy Club Version 1.1 24 November 2012 Introduction Welcome to the Fall Messier List Observing Club. The objects on this list represent many of the most prominent

Gaia News:Counting down to launch A. Vallenari. INAF, Padova Astronomical Observatory on behalf of DPACE

Gaia News:Counting down to launch A. Vallenari INAF, Padova Astronomical Observatory on behalf of DPACE Outline Gaia Spacecraft status The Gaia sky Gaia open and globular clusters From data to science:

Future prospects for finding Milky Way satellites. Amit and Carl 31 March 2010

Future prospects for finding Milky Way satellites Amit and Carl 31 March 2010 Where have all the satellites gone? The missing satellite problem! DM simulations (like Via Lactea) predict that there should

! # #%& () %+(%,#. / # 0 1(,& 23(4. 5( (67# :;!

! # #%& () %+(%,#. / # 0 1(,& 23(4. 5( (67#8.4 9299 2:;! #& (? # %&% (!) +%,! %./012.345!6+10! -0.8-1.0 7.23 1809!: 7! )+1(,!: 7! log N/O -1.2-1.4-1.6-1.8-2.0 7.6 7.8 8.0 8.2 8.4 8. 12+log

obtuse triangle close N with the nearest star 1.8' NW.

Abell 262 - Observing Notes I observed the cluster on eight occasions and identified a total of 47 cluster members down to photographic magnitude 15.7, the majority of which are so-called anonymous galaxies

3% 5% 1% 2% d t = 1,, T d i j J i,d,t J i,d,t+ = J i,d,t j j a i,d,t j i t d γ i > 0 i j t d U i,j,d,t = μ i,j,d + β i,j,d,t γ i + ε i,j,d,t ε i,j,d,t t ε i,,d,t μ β μ μ i,j,d d t d, t j μ i,j,d i j d

Halo Tidal Star Streams with DECAM. Brian Yanny Fermilab. DECam Community Workshop NOAO Tucson Aug

Halo Tidal Star Streams with DECAM Brian Yanny Fermilab DECam Community Workshop NOAO Tucson Aug 19 2011 M31 (Andromeda) Our Local Group neighbors: Spiral galaxies similar to The Milky Way 150 kpc M33

II. Morphology and Structure of Dwarf Galaxies

II. Morphology and Structure of Dwarf Galaxies Ferguson & Binggeli 1994, A&ARev 6, 67 1 1. Properties low mass : 10 6 10 10 M slow rotators : 10 100 km s -1 low luminosity : 10 6 10 10 L low surface brightness

Fluctuations of cosmic parameters in the local universe

Fluctuations of cosmic parameters in the local universe Alexander Wiegand Dominik Schwarz Fakultät für Physik Universität Bielefeld 6. Kosmologietag, Bielefeld 2011 A. Wiegand (Universität Bielefeld) Fluctuations

Summer Messier List Observing Club

Summer Messier List Observing Club Raleigh Astronomy Club Version 1.1 24 November 2012 Introduction Welcome to the Summer Messier List Observing Club. The objects on this list represent many of the most

M3 Globular Cluster Chart 6 Canes Venatici RA 13h 42.2m Dec m. Size 18 Mag 6.3 Difficulty Medium. Equipment Requires binoculars

M3 Globular Cluster Chart 6 Canes Venatici RA 13h 42.2m Dec +28 23m Size 18 Mag 6.3 Difficulty Medium Requires binoculars Locate Arcturus the brightest star in Bootes Locate Cor Caroli the brightest star

1 Integration of Rational Functions Using Partial Fractions

MTH Fall 008 Essex County College Division of Mathematics Handout Version 4 September 8, 008 Integration of Rational Functions Using Partial Fractions In the past it was far more usual to simplify or combine

Astro 1050 Fri. Apr. 14, 2017

Astro 1050 Fri. Apr. 14, 2017 Today: Ch. 19: Our Galaxy, the Milky Way Reading in Bennett: Ch 12 this week, Ch. 13 for next week 1 2 Chapter 12 The Milky Way Galaxy Band of light running around sky in

The Great Debate: The Size of the Universe (1920)

The Great Debate: The Size of the Universe (1920) Heber Curtis Our Galaxy is rather small, with Sun near the center. 30,000 LY diameter. Universe composed of many separate galaxies Spiral nebulae = island

What s Up! For November 2017

What s Up! For November 2017 The November Night Sky N As at 10 p.m. mid-month Mercury An evening sky object this month, but poorly placed, low in southwest after sunset. Best in last few days of November,

Preliminary Rejection of Global 21-cm Models with EDGES High-Band (ongoing work)

Preliminary Rejection of Global 21-cm Models with EDGES High-Band (ongoing work) Raul Monsalve CASA, University of Colorado Boulder SESE, Arizona State University November 23, 216 2 Description Here I

Celeste: Variational inference for a generative model of astronomical images

Celeste: Variational inference for a generative model of astronomical images Jerey Regier Statistics Department UC Berkeley July 9, 2015 Joint work with Jon McAulie (UCB Statistics), Andrew Miller, Ryan

Set 5: Expansion of the Universe

Set 5: Expansion of the Universe Cosmology Study of the origin, contents and evolution of the universe as a whole Expansion rate and history Space-time geometry Energy density composition Origin of structure

Demographics of radio galaxies nearby and at z~0.55. Are radio galaxies signposts to black-hole mergers?

Elaine M. Sadler Black holes in massive galaxies Demographics of radio galaxies nearby and at z~0.55 Are radio galaxies signposts to black-hole mergers? Work done with Russell Cannon, Scott Croom, Helen

The Galactic Exoplanet Survey Telescope (GEST)

The Galactic Exoplanet Survey Telescope (GEST) D. Bennett (Notre Dame), J. Bally (Colorado), I. Bond (Auckland), E. Cheng (GSFC), K. Cook (LLNL), D. Deming, (GSFC) P. Garnavich (Notre Dame), K. Griest

Exploring the Structure of the Milky Way with WFIRST

Exploring the Structure of the Milky Way with WFIRST Heidi Jo Newberg Rensselaer Polytechnic Institute Simulation: Stefan Gottlöber/AIP Image Credit: Heidi Newberg Milky Way Structure we want it all: The

for Astrometry in the 21st Century William van Altena

The Opportunities and Challenges for Astrometry in the 21st Century William van Altena Yale University, New Haven, CT USA (With slides from Elliott Horch, Dana Casetti-Dinescu and Daniel Harbeck) ADeLA

IRS Spectroscopy of z~2 Galaxies

IRS Spectroscopy of z~2 Galaxies Houck et al., ApJ, 2005 Weedman et al., ApJ, 2005 Lutz et al., ApJ, 2005 Astronomy 671 Jason Marshall Opening the IR Wavelength Regime for Discovery One of the primary

and in each case give the range of values of x for which the expansion is valid.

α β γ δ ε ζ η θ ι κ λ µ ν ξ ο π ρ σ τ υ ϕ χ ψ ω Mathematics is indeed dangerous in that it absorbs students to such a degree that it dulls their senses to everything else P Kraft Further Maths A (MFPD)

Hubble Science Briefing: 25 Years of Seeing Stars with the Hubble Space Telescope. March 5, 2015 Dr. Rachel Osten Dr. Alex Fullerton Dr.

Hubble Science Briefing: 25 Years of Seeing Stars with the Hubble Space Telescope March 5, 2015 Dr. Rachel Osten Dr. Alex Fullerton Dr. Jay Anderson Hubble s Insight into the Lives of Stars Comes From:

Messier Bennett & Caldwell Objects for the VicSouth Desert Spring Starparty 36 27' 16" S ' 07" E

Messier Bennett & Caldwell Objects for the VicSouth Desert Spring Starparty 36 27' 16" S 141 40' 07" E Selection criteria: objects south of +45 that are listed in the Messier and/or Bennett and/or Caldwell

National Aeronautics and Space Administration. Glos. Glossary. of Astronomy. Terms. Related to Galaxies

National Aeronautics and Space Administration Glos of Astronomy Glossary Terms Related to Galaxies Asterism: A pattern formed by stars not recognized as one of the official 88 constellations. Examples

Deep fields around bright stars ( Galaxies around Stars )

Deep fields around bright stars ( Galaxies around Stars ) Scientific context: the morphological evolution of faint field galaxies Near-IR observations ground-based observations with AO: PUEO/CFHT deep

Days 3 & 4 Notes: Related Rates

AP Calculus Unit 4 Applications of the Derivative Part 1 Days 3 & 4 Notes: Related Rates Implicitly differentiate the following formulas with respect to time. State what each rate in the differential equation

Milky Way star clusters

Using Γα ια for studying Milky Way star clusters Eugene Vasiliev Institute of Astronomy, Cambridge MODEST-, 26 June Overview of Gaia mission Scanning the entire sky every couple of weeks Astrometry for

TELESCOPE OBSERVING. EQUIPMENT: Observatory telescopes, observing forms, and a pencil. Be sure to dress warmly - the observing deck is not heated!

ASTR 1030 Astronomy Lab 161 Telescope Observing TELESCOPE OBSERVING SYNOPSIS: You will view and sketch a number of different astronomical objects through the SBO telescopes. The requirements for credit

Imaging with SPIRIT Exposure Guide

Imaging with SPIRIT Exposure Guide SPIRIT optical telescopes utilise extremely sensitive cameras to record the light from distant astronomical objects. Even so, exposures of several seconds up to a few

Dark Energy. Cluster counts, weak lensing & Supernovae Ia all in one survey. Survey (DES)

Dark Energy Cluster counts, weak lensing & Supernovae Ia all in one survey Survey (DES) What is it? The DES Collaboration will build and use a wide field optical imager (DECam) to perform a wide area,

Single-Photon Techniques for the Detection of Periodic Optical Signals

Single-Photon Techniques for the Detection of Periodic Optical Signals Presentation at Vienna Fast Photometer Mini-Workshop Vienna University, Institut für Astrophysik Nov. 21, 2014 Walter Leeb 1 Publications

PHY2083 ASTRONOMY. Dr. Rubina Kotak Office F016. Dr. Chris Watson Office S036

PHY2083 ASTRONOMY Dr. Rubina Kotak r.kotak@qub.ac.uk Office F016 Dr. Chris Watson c.a.watson@qub.ac.uk Office S036 PHY2083 ASTRONOMY Weeks 1-6: Monday 10:00 DBB 0G.005 Wednesday 9:00 PFC 02/018 Friday

80 2 Observational Cosmology L and the mean energy

80 2 Observational Cosmology fluctuations, short-wavelength modes have amplitudes that are suppressed because these modes oscillated as acoustic waves during the radiation epoch whereas the amplitude of

Winter Messier List Observing Club

Winter Messier List Observing Club Raleigh Astronomy Club Version 1.1 24 November 2012 Introduction Welcome to the Winter Messier List Observing Club. The objects on this list represent many of the most

. α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω. Wednesday March 30 ± ǁ

. α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω Wednesday March 30 ± ǁ 1 Chapter 5. Photons: Covariant Theory 5.1. The classical fields 5.2. Covariant

Galactic, stellar (and planetary) archaeology with Gaia: The galactic white dwarf population

Galactic, stellar (and planetary) archaeology with Gaia: The galactic white dwarf population Boris Gänsicke & Roberto Raddi Richard Ashley Jay Farihi Nicola Gentile Fusillo Mark Hollands Paula Izquierdo

ASTRONOMY QUALIFYING EXAM Fall 2018

ASTRONOMY QUALIFYING EXAM Fall 2018 L = 3.9 10 33 erg s 1 M = 2 10 33 g M bol = 4.74 R = 7 10 10 cm 1 AU = 1.5 10 13 cm 1 pc = 3.26 Ly. = 3.1 10 18 cm a = 7.56 10 15 erg cm 3 K 4 c = 3 10 10 cm s 1 σ =

The Gravitational Microlensing Planet Search Technique from Space

The Gravitational Microlensing Planet Search Technique from Space David Bennett & Sun Hong Rhie (University of Notre Dame) Abstract: Gravitational microlensing is the only known extra-solar planet search

Physics Lab #9: Measuring the Hubble Constant

Physics 10263 Lab #9: Measuring the Hubble Constant Introduction In the 1920 s, Edwin Hubble discovered a relationship that is now known as Hubble s Law. It states that the recession velocity of a galaxy

5 Dark matter and dark energy, the Universe revealed

5 Dark matter and dark energy, the Universe revealed Our place Courtesy: NASA How much matter? Add up all we can see ~ 1 atom per 10 m -3 Ω = 1? ~ 1 atom m -3 Dark matter MACHOS WIMPS The quintuplet cluster,

The Gaia Mission. Coryn Bailer-Jones Max Planck Institute for Astronomy Heidelberg, Germany. ISYA 2016, Tehran

The Gaia Mission Coryn Bailer-Jones Max Planck Institute for Astronomy Heidelberg, Germany ISYA 2016, Tehran What Gaia should ultimately achieve high accuracy positions, parallaxes, proper motions e.g.

Extra Gal 9: Photometry & Dynamics

Extra Gal 9: Photometry & Dynamics Two books, among many others, that can be used by the studenys for extensive references and details are: Binney and Merrifield: Galactic Astronomy Binney and Tremaine

Y1 Double Maths Assignment λ (lambda) Exam Paper to do Core 1 Solomon C on the VLE. Drill

α β γ δ ε ζ η θ ι κ λ µ ν ξ ο π ρ σ τ υ ϕ χ ψ ω Nature is an infinite sphere of which the centre is everywhere and the circumference nowhere Blaise Pascal Y Double Maths Assignment λ (lambda) Tracking

By September the nights are getting a little bit shorter and the centre of our Milky Way Galaxy is heading for the western horizon.

By September the nights are getting a little bit shorter and the centre of our Milky Way Galaxy is heading for the western horizon. So make the best use of the central region of our galaxy while you can.

Name: AST 114 Date: THE DEEP SKY

Name: AST 114 Date: THE DEEP SKY The purpose of this lab is to familiarize the student with the use of the planisphere, sky atlas, and coordinate systems for the night sky and introduce the student to

Advanced Telescope Observations (Evening Observation)

Chapter 14 Advanced Telescope Observations (Evening Observation) Carefully align your telescope before you begin to reduce drift in your observations. Although the Telrad finder charts are helpful, they

IO March The Newsletter of the Eugene Astronomical Society EAS. Next Meeting: Thursday, March 16. PO Box 7264 Springfield, OR 97475

IO March 2017 The Newsletter of the Eugene Astronomical Society PO Box 7264 Springfield, OR 97475 Next Meeting: Thursday, March 16 Optics workshop At this month's EAS meeting, John Walley will discuss

Page # Astronomical Distances. Lecture 2. Astronomical Distances. Cosmic Distance Ladder. Distance Methods. Size of Earth

Size of Astronomical istances ecture 2 Astronomical istances istance to the Moon (1 sec) istance to the Sun (8 min) istance to other stars (years) istance to centre of our Galaxy ( 30,000 yr to centre)

PHYS-333: Problem set #1 Solutions

PHYS-333: Problem set #1 Solutions VERSION of February 10, 2018. 1. Energy flux and magnitude: a. Suppose two objects have energy fluxes of f and f + f, where f f. Derive an approximate expression for

Galaxies. Galaxy Diversity. Galaxies, AGN and Quasars. Physics 113 Goderya

Galaxies, AGN and Quasars Physics 113 Goderya Chapter(s): 16 and 17 Learning Outcomes: Galaxies Star systems like our Milky Way Contain a few thousand to tens of billions of stars. Large variety of shapes

CSSS/STAT/SOC 321 Case-Based Social Statistics I. Levels of Measurement

CSSS/STAT/SOC 321 Case-Based Social Statistics I Levels of Measurement Christopher Adolph Department of Political Science and Center for Statistics and the Social Sciences University of Washington, Seattle

The magnitude system. ASTR320 Wednesday January 30, 2019

The magnitude system ASTR320 Wednesday January 30, 2019 What we measure: apparent brightness How bright a star appears to be in the sky depends on: How bright it actually is Luminosity and its distance

Light: Transverse WAVE

Light Longitudinal WAVES Light: Transverse WAVE Light: Particle or wave Photon The Wave Nature of Light 1. Unlike other branches of science, astronomers cannot touch or do field work on their samples.

JEWELS of the COSMIC DEEP Messier's first guide to the night sky

JEWELS of the COSMIC DEEP Messier's first guide to the night sky Shane L. Larson USU Physics & Cache Valley Stargazers s.larson@usu.edu Cache Valley Stargazers 12 March 2010 M78 IN ORION 1 Storyline What

Structure and Evolution of Stars Lecture 13: Homology Solutions (#1)

Structure and Evolution o Stars Lecture 13: Homology Solutions (#1) Equations o Stellar Structure with mass as the independent variable Review o Observed relations between L, T and M Homology sel-similar

SERCH FOR LARGE-SCALE

SERCH FOR LARGE-SCALE Université Libre de Bruxelles (ULB) Brussels SNOWPAC 23-28 March, 2010 Matter tracer model: generic model of CRs under the assumptions: nearly straight propagation typical deflections

Einführung in die Astronomie II

Einführung in die Astronomie II Teil 12 Peter Hauschildt yeti@hs.uni-hamburg.de Hamburger Sternwarte Gojenbergsweg 112 21029 Hamburg 13. September 2017 1 / 77 Overview part 12 The Galaxy Historical Overview

Lincoln Hills Astronomy Group Exploring the Night Sky. October 28, 2009

Exploring the Night Sky October 28, 2009 1 Exploring the Night Sky Course Outline Session 1 OC lodge - Ron Presentation: Orientation to the Night Sky Viewing: Naked eye Session 2 OC Lodge John Presentation:

ASTRONOMY. MINNESOTA REGIONS 2011 by Michael Huberty

ASTRONOMY MINNESOTA REGIONS 2011 by Michael Huberty Team Number School Name Total Points You may tear this sheet off of the rest of the test to use as your answer sheet. Please make sure that you print

Building the cosmic distance scale: from Hipparcos to Gaia

The Fundamental Distance Scale: state of the art and the Gaia perspectives 3-6 May 2011 Building the cosmic distance scale: from Hipparcos to Gaia Catherine TURON and Xavier LURI 1 ESA / ESO-H. Heyer Fundamental

Astr As ome tr tr ome y I M. Shao

Astrometry I M. Shao Outline Relative astrometry vs Global Astrometry What s the science objective? What s possible, what are fundamental limits? Instrument Description Error/noise sources Photon noise

The motions of stars in the Galaxy

The motions of stars in the Galaxy The stars in the Galaxy define various components, that do not only differ in their spatial distribution but also in their kinematics. The dominant motion of stars (and

The History of Active Galaxies A.Barger, P. Capak, L. Cowie, RFM, A. Steffen, and Y. Yang

The History of Active Galaxies A.Barger, P. Capak, L. Cowie, RFM, A. Steffen, and Y. Yang Active Galaxies (AKA quasars, Seyfert galaxies etc) are radiating massive black holes with L~10 8-10 14 L sun The

Terrestrial Planet (and Life) Finder. AST 309 part 2: Extraterrestrial Life

Terrestrial Planet (and Life) Finder AST 309 part 2: Extraterrestrial Life The Drake Equation: N = N * f pl n hab f L f C f T L/T Stars? Planets? Habitable Origin Complex Intelligence, Lifetime planets?

X-ray observations of neutron stars and black holes in nearby galaxies

X-ray observations of neutron stars and black holes in nearby galaxies Andreas Zezas Harvard-Smithsonian Center for Astrophysics The lives of stars : fighting against gravity Defining parameter : Mass

Cosmic Optical Background: The View from Pioneer 10/11. Cosmic Optical Background the View from Pioneer 10/11

Cosmic Optical Background: The View from Pioneer 10/11 Cosmic Optical Background the View from Pioneer 10/11 Matsuoka et al. 2011, ApJ, 736, 119 Yoshiki Matsuoka (Nagoya University) Nobuyuki Ienaka, Kimiaki

HOMEWORK 4: H-R DIAGRAM

NAME(S) SECTION DAY/TIME ASTRONOMY25 (LLOYD) SPRING 2012 Purpose HOMEWORK 4: H-R DIAGRAM To plot the H-R diagram of a star cluster and estimate its age and distance. Background Magnitude is a measure of

DETECTION OF POLARIZATION EFFECTS IN GAIA DATA

Title : will be set by the publisher Editors : will be set by the publisher Publications Series, Vol.?, 2012 DETECTION OF POLARIZATION EFFECTS IN GAIA DATA F. Raison 1 Abstract. The Gaia satellite will

The Atlanta Astronomy Club. Charlie Elliot Chapter. Observing 101

The Atlanta Astronomy Club Charlie Elliot Chapter Observing 101 1 Observing 101 Dec 2010 Astro Events Target List Featured Object 2 Astro Events Tonight: Sunset at 5:29 PM Moon sets at 4:34 PM Mercury

Distinguishing Between Warm and Cold Dark Matter

Distinguishing Between Warm and Cold Dark Matter Center for Cosmology Aspen Workshop Neutrinos in Physics & Astrophysics 2/2/2007 Collaborators: James Bullock, Manoj Kaplinghat astro-ph/0701581.. Motivations

BAS - MONTHLY SKY GUIDE

BAS - MONTHLY SKY GUIDE September 2019 By September the nights are getting a little bit shorter and the centre of our Milky Way Galaxy is heading for the western horizon. So make the best use of the central

Where are oxygen synthesized in stars?

The oxygen abundance from X-rays : methods and prospects K. Matsushita Where are oxygen synthesized in stars? Hot intracluster medium (ICM) Warm-hot intergalactic medium? Hot interstellar medium in early-type

Scale Length of the Galactic Thin Disk

J. Astrophys. Astr. (2000) 21, 53-59 Scale Length of the Galactic Thin Disk D. Κ. Ojha, Tata Institute of Fundamental Research, Dr. Homi Bhabha Road, Mumbai 400 005, India Received 1999 September 14; accepted

Star clusters (and other neat stuff) in Ophiuchus

Star clusters (and other neat stuff) in Ophiuchus Michael L Allen mlfa.astro@gmail.com Palouse Divide Lodge Star Party 2016 Michael L Allen Ophiuchus PDLSP 16 1 / 19 Quick facts 11th-largest constellation

Astronomy: Division C Science Olympiad, Round 1 Tryout Test

Astronomy: Division C Science Olympiad, Round 1 Tryout Test Student Name : Student Number : DIRECTIONS 1. Write the answers that you want graded legibly on the answer sheet, along with your name and student

Lecture 2: Transfer Theory

Lecture 2: Transfer Theory Why do we study transfer theory? The light we detect arrives at us in two steps: - first, it is created by some radiative process (e.g., blackbody, synchrotron, etc etc ) -

Stars: Stars and their Properties

Stars: Stars and their Properties Astronomy 110 Class 10 WHEN I heard the learn d astronomer; When the proofs, the figures, were ranged in columns before me; When I was shown the charts and the diagrams,

Basic Properties of the Stars

Basic Properties of the Stars The Sun-centered model of the solar system laid out by Copernicus in De Revolutionibus (1543) made a very specific prediction: that the nearby stars should exhibit parallax

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

Solutions Mock Examination

Solutions Mock Examination Elena Rossi December 18, 2013 1. The peak frequency will be given by 4 3 γ2 ν 0. 2. The Einstein coeffients present the rates for the different processes populating and depopulating

Measuring the Milky Way

Printed: Mar/01/2013 Milky Way Lab Page MW- 13 NAME Name Group NAME Name Date Measuring the Milky Way References B Carroll and D. Ostlie, An Introduction to Modern Astrophysics (Addison-Wesley, 1996),

The Massive Star Content of M31. Phil Massey Lowell Observatory The 2nd MMT Science Symposium

The Massive Star Content of M31 Phil Massey Lowell Observatory The 2nd MMT Science Symposium The Team Maria Drout Knut Olsen Me Nelson Caldwell Kathryn Neugent Dave Silva Emily Levesque Georges Meynet

Further Maths A2 (M2FP2D1) Assignment ψ (psi) A Due w/b 19 th March 18

α β γ δ ε ζ η θ ι κ λ µ ν ξ ο π ρ σ τ υ ϕ χ ψ ω The mathematician s patterns, like the painter s or the poet s, must be beautiful: the ideas, like the colours or the words, must fit together in a harmonious