... Home Education Classes AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb 2016 . ... Classes . AAA Fall Astronomy Class: Astronomy Basics тАУ October-November 2015 . AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb 2016 . AAA Spring Astronomy Class: The Physics of Astronomy тАУ February - March 2016 . ... This MonthтАЩs Sky тАУ April 2016 . ... Dec. ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ...

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• Observing-Events ? Amateur Astronomers Association of New York
• Observing Out-Of-Town ? Amateur Astronomers Association of New York
• Articles ? Amateur Astronomers Association of New York

... An OBJECT column gives the name of the object observed (usually a star name). ... In critical cases, it is common practice to measure sky on two or more positions around a target object, and these positions must be identified. ... A general treatment of this problem requires a column called OBJECT, bearing the usual name of the object (as in the star tables); a column labelled STARSKY, to distinguish between star+sky, star alone, or sky alone; and additional columns to identify the sky position. ...

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• Emission-line galaxies
• Cosmology Tutorial - Part 2
• HyperLEDA documentation: compilation of cz measurements (a110)

... HST Overview . ... Proposal ID = 11704 Principle Investigator = Brian Chaboyer - Dartmouth College Title = "The Ages of Globular Clusters and the Population II Distance Scale" Time = June 3, 2012 , 13:30:54 - 14:28:47 Targets = HIP-56291-FIX, HIP-56291-REF1, HIP-56291-REF2, HIP-56291-REF3, HIP-56291-REF4, HIP-56291-REF5, HIP-56291-REF6 Instrument = FGS . ... One of the most accurate ways to measure the age of globular clusters is to determine the absolute brightness of sub-giant stars in the...

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• Future Calibrations, Calibration by Observers, and Calibration Outsourcing
• Observing Faint Targets Near Bright Objects

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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• Astronomy HyperText Book: Planetary Motion
• Cosmological Issues for Theorists

... The following charts/text are intended as tools for monitoring the Type Ia supernovae ( SNe ) event visually or photographically (utilizing telescope equipped CCD equipment).The files include: A replication of The Type Ia SNe , V- magnitude (with data point checks from other cited references)and color index (B-V) templete (to indicate a general color-related trend of the type Ia ... I believe this might help alleviate some of the problems involving the making of acceptable amateur light curves...

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• Contributions by amateurs: SN1995V.
• Contributions by amateurs: SN1996X.
• APOD: May 30, 1999 - Tycho Brahe Measures the Sky

HI spectral-line observations of galaxies (Karen O'Neil) . Measuring the width, flux, etc. of the HI profile of two galaxies, using some combination of : dwarf emission line, HVC emission line, spiral emission line, and spiral absorption line. This project was designed to demonstrate the fundamentals of spectral line observing and position switching. ... The types of galaxies observed in this project are being kept open and will be determined when the project LST is known. ...

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• pdev_birdies_25jun07
• Spectral-Line Observing
• INTRODUCTION to Spectral Line Observing at AO

... 12c. Venus transit (1) . 12d. Venus transit (2) . 12e. Venus transit (3) . ... 1 The 2004 Venus transit . ... Kepler's third law allows one to evaluate the dimensions of the solar system in relative units, e.g. in " astronomical units " (AUs), where 1 AU is the mean Sun-Earth distance. ... Edmond Halley suggested using the transit of Venus across the Sun's disk, when it appears as a dark round spot --or to quote one observer of the 2004 transit, "like a blueberry in front of an orange." ...

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• The Scale of the Solar System
• les Satellites orient?s vers le bas pour observer la Terre
• Trigonometry--what it is good for?

... Tonight's Sky . ... Search By Name Enter coordinates Use current location . ... Observing . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... How do astronomers use Cepheid variables to measure distances? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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• Observing Basics: Distances in Space | Astronomy.com
• Great targets await lunar observers | Astronomy.com
• т??Eye of Sauronт?? provides new way of measuring distances to galaxies |

Next: Radial velocity of the Up: Optical spectrum of IRAS04296 Previous: Observations and spectra reduction . ... However, molecular emission features are only very rarely observed in the optical spectra of PPNe. ... On the other hand, it is well known that cometary nuclei spectra show prominent Swan band emission. In both spectra of IRAS04296 we have discovered strong emission in the (0;0) and (0;1) bands of the Swan system of the molecule. ... Now consider the case of IRAS04296. ...

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• instruct
• RATAN-600 CONTINUUM OBSERVER: refraction
• SCORPIO: IFP Gallery

. -!> download . Left: Consequtive explosion of 20 supernovae during 30 Myr. Right: Single hypernova (GRB) explosion with the total energy equivalent to 20 supernovae. The simulation was performed using a 2D Eulerian hydro code. The animation was done using IDL. -!>

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• Subsystems of the Galactic halo, figures

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• Description
• XMM-Newton Radiation Monitor Details

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Facilities . ATNF facilities . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• The observed distribution
• ATNF Colloquium
• Reducing 3-mm ATCA observations

... Posts tagged ?distance measure? ... From arxiv/math.st:0708.0169v1 . Data-Driven Goodness-of-Fit Tests by L. Mikhail . ... ArXiv] Data-Driven Goodness-of-Fit Tests, Aug. ... Tags: consistency , distance measure , distribution , goodness-of-fit test , inverse problem , Neyman type , regularity condition , score . Category: arXiv , Fitting , Uncertainty | 1 Comment . ... Entries RSS . Comments RSS . ... vlk on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

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• Direct Monitoring of Rotational Modulation
• Doug Burke's PDL page
• Period Criteria

Astronomy Discussion Forums . Forums: . ... TIME DILATION . ... Time dilation is what we take to be the disagreement in the total time of an event as measured by a moving frame and stationary frame. ... Imagine a car 100km from a stationary observer and which is positioned such that it would travel 200km on a straight line in a direction away from the stationary observer. ... Therefore the total time of motion of the car as measured by the stationary observer is T= t- 100km/C + (100km+200km/C). ...

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• New Theory Of Relativity [Nwobu's Effect] - an Astronomy Net
• Erie County Mobile Observers Group (pa), AstroGuide Listing
• FURTHER EXPLANATION [NWOBU'S EFFECT] - an Astronomy Net Observation_reports

home publications > mercury . ... Astronomy Beat . ... Hitching a Ride on a Comet . Mercury, November/December 1996 Table of Contents . ... Late in the evening of Jan. 30, 1996 in Japan's Kyushu region, Yuji Hyakutake left his home in Kagoshima and drove to an observing site far from city lights. ... We bought our daughter a telescope to see the comet," she said, "and we can't see anything!" ... This helps us as we select the Guest Observer, and it helps readers to understand what you studied. ...

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• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
• ASP: The New and Improved Hubble Space Telescope
• ASP: Walter Baade: Master Observer

... A theory suggests that a certain sub-class of gamma-ray bursts all have the same absolute magnitude. ... The author claims that this absolute magnitude is so different from that in the previous sample that this must belong to a new sub-class of gamma-ray bursts. ... To do this, there needs to be some feature in their spectra which correlates with their absolute magnitude. ... Consider a telescope which is continually monitoring a star, looking for transits due to planets orbiting this star. ...

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• Untitled1
• The SMS Survey
• Lesson 1: DC Circuits

... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Observing conditions . ... Service Mode Philosophy . ... The following definitions of the observing conditions are common between Phase 1 preparation and Phase 2 preparation, as well as between Service Mode and Visitor Mode observations. ... There are additional Service Mode Policies and Service Mode Guidelines regarding the observing conditions. ... Seeing (Phase 1) and Image quality (Phase2) constraints . ... Moon . ...

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• ESO - Thesis Topic: Cepheid stars, Ho and Dark Energy: precision stellar
• ESO - cosmology2002
• ESO - Science in Garching

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology
• UGC 2172, NGC 3239
• Ratan-600 schedule archive

spaceweb@oulu.fi - last update: 20 September 1998, 2020 UT (RR) . Traveling Convection Vortex (TCV) is a name given to a specific type of daytime magnetic impulsive events observed by high-latitude ground-based magnetometer arrays. Since the most likely source for TCVs is the solar wind , they are considered to be important processes in transfering energy from the solar wind into the magnetosphere . ... For example, one AMPTE Lithium release in the solar wind caused a TCV event . ...

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• Trigonometry--what it is good for?
• The Sun
• Parallax

ARCSAT ID NUMBER: AS08 DESCRIPTIVE TITLE: Stellar Environments of the Nearest Red Dwarfs PI: Michele Silverstein (GSU) OBSERVER(S): Michele Silverstein (GSU), Todd Henry (GSU) and Tiffany Pewett (GSU) UNCERTIFIED/UNTRAINED OBSERVERS: COLLABORATORS: Wei-Chun Jao (GSU) and Jen Winters (GSU) CONTACT INFORMATION: (PI/OBSERVER email/phone) silverstein@astro.gsu.edu (404-413-6024), thenry@astro.gsu.edu (404-413-6054) TIME REQUESTED: 7 nights 1. MAY 04-10 (note = first week of Q2, if possible) 2. ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS04.html
• ARC 3.5m | Closure Conditions
• Information for On-Site Observers