Zone 217, Master Map Normal View
|
|
- Simon Perry
- 5 years ago
- Views:
Transcription
1 Zone Master, Normal View, 10 deg FOV, Master Map Normal View β Zubeneschamali ε δ ξ ' ' ' ' ' ' γ η ο Libra 16h 00m 15h 52m 15h 44m 15h 36m 15h 28m 15h 20m 15h 12m 15h 04m 14h 56m
2 , Map 1 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. h4779 h4758 STF 1925 STF 1914 Holden 23 ur 119 Hough 391 os 2781 δ NGC ' ' ' ' ' Sh 202 Zubeneschamaliβ eta Lib 15h 30m 15h 25m 15h 20m 15h 15m 15h 10m 15h 05m 15h 00m
3 , Map 1 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. NGC 5812 δ Hough 391 os 2781 ur 119 Holden 23 STF 1914 STF 1925 h ' ' ' ' ' β Zubeneschamali eta Lib Sh h 00m 15h 05m 15h 10m 15h 15m 15h 20m 15h 25m 15h 30m
4 , Map 2 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. ε STF 1939 NGC ' ' ' ' ' ur h 30m 15h 25m 15h 20m 15h 15m 15h 10m 15h 05m 15h 00m
5 , Map 2 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. 18 Lib ε STF ' ' ' ' ' NGC 5878 ur h 00m 15h 05m 15h 10m 15h 15m 15h 20m 15h 25m 15h 30m
6 , Map 3 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF 3100 STF 3097 STF STF 3094 STF ' ' ' ' ' Hipparcos h 00m 15h 55m 15h 50m 15h 45m 15h 40m 15h 35m 15h 30m
7 , Map 3 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF 3094 STF STF 3096 STF 3097 STF ' ' ' ' ' Hipparcos h 30m 15h 35m 15h 40m 15h 45m 15h 50m 15h 55m 16h 00m
8 , Map 4 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF 1966 Torino Obs 60 ur ' ' ' ' ' Hussey 478 Gamma Lib Howe 37 γ 16h 00m 15h 55m 15h 50m STF 3095 Glasenapp 11 15h 45m 15h 40m 15h 35m 15h 30m
9 , Map 4 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. Torino Obs 60 ur 33 STF ' ' ' ' ' γ Gamma Lib Howe 37 Hussey 478 STF 3095 Glasenapp 11 15h 30m 15h 35m 15h 40m 15h 45m 15h 50m 15h 55m 16h 00m
10 23 Double Stars, 2 Galaxies os ur ur G Gamma Lib H h h Hipparcos Holden Hough Howe Hussey N NGC NGC S Sh STF STF STF STF STF STF STF STF STF T Torino Obs
11 , Map 1 Double Stars Easy Holden 23 DS 9519; HD Rating: 3 E Position: Magnitude Separation P Year Spectra Colors G0 W W C W 1881: measurements. C 1 measurement. C11 at 193x. STF 1925 DS 9564; HD ; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 7.85 G5 Y O C ? D ? E ? 1831: measurements. C, D and E, all 1 measurement
12 C8 at 83x. Diameter: = inches. Separation: = 1.16 miles; C = 12.8 miles; D = 24.2 miles; E = 42.0 miles. Distance (LY): 124 Total luminosity (Suns): Sh 202 HD ; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 6.89 K2 V Y = 1993 K2 V Y C ? C : measurements. The stars share a large common proper motion. The primary is a spectroscopic binary of very high eccentricity, period of days. C 1 measurement. C is optical m star at 20 min shares proper motion of. C8 at 104x. Diameter: = 2.10 inches; = 26.1 inches. Separation: = 5.32 miles; C = 16.9 miles. Distance (LY): 65 Total luminosity (Suns):
13 STF 1914 HD ; SO Rating: 4 E Position: Magnitude Separation P Year Spectra Colors W G0 p 1827: measurements. The stars share common proper motion. C8 at 83x. Diameter: = 6.24; = 18.7 inches. Separation: = 29.6 miles. Distance (LY): 610 Total luminosity (Suns): 14 h4758 DS 9581 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.62 F8 W W 1892: measurements. May be optical because Hipparcos gives different distances (135 and 49 light years). C11 at 98x
14 os 2781 HD ; SO Rating: 5 E Position: Magnitude Separation P Year Spectra Colors 7.49 M ro! = 1996? 1893: measurements. C8 at 104x. Diameter: = 52.6 inches. Separation: = 373 miles. Distance (LY): 5,400 Total luminosity (Suns): 1,258 h4779 HD Rating: 5 E Position: Magnitude Separation P Year Spectra Colors 8.59 K2 Y = 1991? 1892: measurements. C11 at 98x. Diameter: = 27.8 inches. Separation: = 31.3 miles. Distance (LY): 920 Total luminosity (Suns):
15 Moderate ur 119 DS 9497; HD Rating: 3 M Position: Magnitude Separation P Year Spectra Colors 7.56 G0 W ! 1999 W C !! ? 1875: measurements. C 1906: measurements. C11 at 339x. Diameter: = 16.4 inches. Separation: = 2,640 feet; C = 16.4 miles. Distance (LY): 148 Total luminosity (Suns): 2.48 Hough 391 DS 9497; HD ; SO Rating: 5 M Position: Magnitude Separation P Year Spectra Colors 7.72 G0 W ! 1997 W C ! ? 1891: measurements. C 1891: measurements. C8 at 280x. half-field sized 7m triangle lies about 1 deg S. Moderate field
16 Diameter: = 16.6 inches. Separation: = 1,690 feet; C = 5.37 miles. Distance (LY): 114 Total luminosity (Suns): Deep Sky Objects Moderate NGC 5812 Other Names: H I 71; PGC stronomical League Program: Herschel II Club Rating: 4 M Position: Type: Gal Class: E0 Magnitude: 11.2 Surface brightness: 12.6 Dimensions: 2.4' P: 130 C8 at 104x. Very quickly brightens to the center, but not quite a stellar nucleus. Moderate field. Distance (LY): 88,000,000 Total luminosity (Suns): 16,600,000,000 Radial velocity (km/sec): +2,
17 , Map 2 Double Stars Easy STF 1939 DS 9640; HD ; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 7.80 G0 Y O 1830: measurements. C8 at 65x. Diameter: = 16.7 inches. Separation: = 4.87 miles. Distance (LY): 329 Total luminosity (Suns): 8-8 -
18 Deep Sky Objects Easy NGC 5878 Other Names: PGC 54364, H III 736 stronomical League Program: Herschel II Club Rating: 3 E Position: Type: Gal Class: S(s)b Magnitude: 11.5 Surface brightness: 12.9 Dimensions: 2' x 1.4' P: 90 This galaxy produced supernova 1988H (type II). C8 at 63x Very bright nucleus and significant halo (out to about 30"). Two bright stars share the field (one E, one N). Distance (LY): 90,000,000 Total luminosity (Suns): 16,000,000,000 Radial velocity (km/sec): +1,991 NGC 5878 Galaxy (S:(s)bc II or II-III) Observed with C8 on7/26/03 Magnification: 64x Louisburg Lake (SKC star party) - 9 -
19 , Map 3 Double Stars Easy STF 1962 DS 9728; HD ; SO Rating: 1 E Position: Magnitude Separation P Year Spectra Colors 6.45 F6 V W F6 IV W 1825: measurements. Star is a spectroscopic binary. The stars share common proper motion. C8 at 104x. Webb called it "a striking object." Scale model (in which the Sun is the size of a baseball): Diameter: = 4.20 inches; = 12.4 inches. Separation: = 1.50 miles. Distance (LY): 81 Total luminosity (Suns): 2.47 STF 1962 Observed with C8 on 5/20/95; s7, t8 Magnification: 104x
20 , Map 4 Double Stars Easy Howe 37 DS 9743 Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 8.87 F8/G0 V W = yw 1876: measurements. C11 at 98x. Diameter: = 3.45 inches. Separation: = 2.08 miles. Distance (LY): 248 Total luminosity (Suns): 2.24 STF 1966 HD ; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.27 F8 W F8 W 1831: measurements. The stars share common proper motion. Quadrant reversal?
21 C8 at 104x. Diameter: = 16.1 inches; = 16.2 inches. Separation: = 6.95 miles. Distance (LY): 193 Total luminosity (Suns): 1.1 Hussey 478 DS 9773; HD Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.74 F0 V W = No C W 1902: measurements. C 1904: measurements. C8 at 104x. Diameter: = 5.70 inches. Separation: = 792 feet; C = 2.48 miles. Distance (LY): 25 Total luminosity (Suns): Torino Obs 60 HD Rating: 5 E Position: Magnitude Separation P Year Spectra Colors G5 W = 1991 W
22 1906: measurements. C8 at 104x. Moderate ur 33 Doolittle; DS 9680 Rating: 5 M Position: Magnitude Separation P Year Spectra Colors 7.71 F8 V W ? C ? D ? E ! ? 1875: measurements. C 1898: measurements. CD 1897: : measurements. E 1898: measurements. C8 at 516x. Diameter: = 3.60 inches. Separation: = 1.35 miles; C = 109 miles; CD = 2.74 miles; E = 9.32 miles. Distance (LY): 280 Total luminosity (Suns):
23 Gamma Lib Rating: 5 M 38 Lib; Goecking 1; Goldschmidt 1; DS 9704; HD ; SO Position: Magnitude Separation P Year Spectra Colors 3.91 K0 III yg ? 1878: measurements. The primary is an infra-red source. C8 at 83x. Star is very faint. Note the 11m star 178. Diameter: = 46.2 inches. Separation: = 9.91 miles. Distance (LY): 152 Total luminosity (Suns): 50.1 Hipparcos 2205 SO Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.68 F2 W W? 1895: measurements. C11 at 98x. Diameter: = 12.8 inches. Separation: = 45.5 miles. Distance (LY): 2,700 Total luminosity (Suns):
24 Moderate STF 3094 DS 9732 Rating: 3 M Position: Magnitude Separation P Year Spectra Colors 8.93 G0 W W 1831: measurements. C11 at 339x. STF 1962, about 12 min S, is stunning! Diameter: = 17.9 inches. Separation: = 2.34 miles. Distance (LY): 600 Total luminosity (Suns): 13.6 STF 3096 DS 9785; HD Rating: 3 M Position: Magnitude Separation P Year Spectra Colors 9.93 G5 W W 1831: measurements. C8 at 516x. Diameter: = 21.6 inches. Separation: = 1.00 mile. Distance (LY): 165 Total luminosity (Suns):
25 STF 3097 DS 9805 Rating: 4 M Position: Magnitude Separation P Year Spectra Colors 9.72 G0 W W 1831: measurements. Hipparcos/Tycho data show different distances for these stars; they may be optical. C8 at 516x. Diameter: = 18.6 inches. Separation: = 1,267 feet. Distance (LY): 39 Total luminosity (Suns): 0.03 STF 3100 DS 9837 Rating: 4 M Position: Magnitude Separation P Year Spectra Colors W = O? 1831: measurements. C11 at 98x
26 Difficult 19 DS 9759 Rating: 3 D Position: Magnitude Separation P Year Spectra Colors G0 W W 1899: measurements. C11 at 634x. Diameter: = 19. inches. Separation: = 1.00 mile. Distance (LY): 381 Total luminosity (Suns):
27 Mini-Catalog Double Stars Designation Position Rating Map Component Mag Separation P STF E Holden E 1 C STF E 1 STF E 2 Sh E 1 Howe E 4 STF E 4 STF E 1 h E 1 Hipparcos E 3 Hussey E 4 os E 1 h E 1 Torino Obs E 4 ur M 1 STF M 3 STF M 3 STF M 3 STF M 3 C D E C C C C = = !! = = = 18 = 357 = 277 -! 71 +!!
28 Designation Position Rating Map Component Mag Separation P Hough M 1 C ! 96 -! ! ur M 4 Gamma Lib M D 3 C D E ! Deep Space Objects Specifications Object Position Rating Map Type Mag Surface r NGC E 2 Gal (S(s)b) NGC M 1 Gal (E1) Pop
Zone 7, Master Map Normal View
, Master Map Normal View Zone Master, Normal View, 10 deg FOV Draco P Muller 352 ur 353 H I 41 STF 2572 rej P Muller 209 STF 2326 40, 41 Dra NGC 6412 7-1 Ursa Minor NGC 6324 Hussey 65 STF 2299 Kustner
More informationZone 21, Master Map Normal View
, Master Map Normal View Zone Master, Normal View, 10 deg FOV NGC 4589 STF 1654 h2613 STF 1588 h2590 LDS 1744 STF 1590 OS 242 76 STF 1626 NGC 4236 h3336 STF 1614 NGC 4125 NGC 4291 STF 1602 STF 1599 STF
More informationZone 151, Master Map Normal View
Zone Master, Normal View, 10 deg FOV, Master Map Normal View κ Vulpecula Pegasus Delphinus +16 00' +18 00' +20 00' +22 00' +24 00' 22h 00m 21h 52m 21h 44m 21h 36m 21h 28m 21h 20m 21h 12m 21h 04m 20h 56m
More informationZone 65, Master Map Normal View
Zone Master, Normal View, 10 deg FOV, Master Map Normal View ear Paw Galaxy ψ9 ψ6 +46 00' +48 00' +50 00' +52 00' +54 00' Lynx ψ4 08h 12m 08h 00m 07h 48m 07h 36m uriga 07h 24m 07h 12m 07h 00m ψ5 06h 48m
More informationZone 147, Master Map Normal View
Zone Master, Normal View, 10 deg FOV, Master Map Normal View δ +16 00' +18 00' +20 00' +22 00' +24 00' 18h 00m 17h 52m 17h 44m 17h 36m Octans 17h 28m 17h 20m α1 α2 Rasalgethi 17h 12m 17h 04m 16h 56m ,
More informationZone 141, Master Map Normal View
Zone Master, Normal View, 10 deg FOV, Master Map Normal View Leo Minor Copeland's Septet δ Zosma +16 00' +18 00' +20 00' +22 00' +24 00' θ Chertan Denebolaβ 12h 00m 11h 52m 11h 44m 11h 36m 11h 28m 11h
More informationZone 98, Master Map Normal View
Zone Master, Normal View, 10 deg FOV Zone 98, Master Map Normal View η The Wall M13 σ Great Cluster in Hercules Hercules Globular Cluster Corona orealis φ τ λ χ Hercules κ oo +36 00' +38 00' +40 00' +42
More informationZone 122, Master Map Normal View
Zone Master, Normal View, 10 deg FOV Zone 122, Master Map Normal View κ ε ζ ν1 ν2 ξ υ σ ρ ι ε +26 00' +28 00' +30 00' +32 00' +34 00' Hercules Serpens Cauda 17h 00m 16h 48m 16h 36m 16h 24m 16h 12m 16h
More informationZone 78, Master Map Normal View
Zone Master, Normal View, 10 deg FOV Zone 78, Master Map Normal View ω2 ω1 ψ +46 00' +48 00' +50 00' +52 00' +54 00' α Deneb δ North merican Nebula ξ Pelican Nebula 21h 12m 21h 00m 20h 48m 20h 36m 20h
More informationZone 134, Master Map Normal View
Zone Master, Normal View, 10 deg FOV, Master Map Normal View χ ι Orion τ σ2 σ1 α ldebaran ε θ1 θ2 υ κ1 κ2 δ3 δ1 δ2 γ ω2 Struve's Lost Nebula Hind's Variable Nebula Taurus ω1 +16 00' +18 00' +20 00' +22
More informationZone 124, Master Map Normal View
Zone Master, Normal View, 10 deg FOV Zone 124, Master Map Normal View λ Vulpecula γ M57 Sulafat Hercules β Sheliak Ring Nebula in Lyra ν1 ν2 Lyra ο ν ξ +26 00' +28 00' +30 00' +32 00' +34 00' 19h 00m 18h
More informationZone 87, Master Map Normal View
Zone Master, Normal View, 10 deg FOV Zone 87, Master Map Normal View β Menkalinan θ uriga ν υ τ σ ρ λ µ η ε ζ ω Pe +36 00' +38 00' +40 00' +42 00' +44 00' M38 M36 φ Flaming Star 06h 00m 05h 48m 05h 36m
More informationTIRCAM2 (TIFR Near Infrared Imaging Camera - 3.6m Devasthal Optical Telescope (DOT)
TIRCAM2 (TIFR Near Infrared Imaging Camera - II) @ 3.6m Devasthal Optical Telescope (DOT) (ver 4.0 June 2017) TIRCAM2 (TIFR Near Infrared Imaging Camera - II) is a closed cycle cooled imager that has been
More information12.5" f/8 Newtonian. 12.5" f/8 Newtonian. 12.5" f/8 Newtonian. 12.5" f/8 Newtonian. 12.5" f/8 Newtonian. 12.5" f/8 Newtonian
Object Arp Number Date Time Seeing Trans. Location Equipment Description NGC 5457 (M101) 26 05/14/88 0:09 Good Good TSP-Ft. Davis, TX NGC 221 (M32) 168 11/29/86 18:35 Good Good Atoka, OK NGC 4472 (M49)
More informationSmall Wonders: Quick Peeks - Sculptor Tom Trusock 1/09. Small Wonders: Quick Peeks Sculptor
Small Wonders: Quick Peeks - Sculptor Tom Trusock 1/09 This small, faint constellation is located low in the southern sky for mid latitude northern observers. Contrary to most of the constellations I've
More informationChasing Faint Objects
Chasing Faint Objects Image Processing Tips and Tricks Linz CEDIC 2015 Fabian Neyer 7. March 2015 www.starpointing.com Small Objects Large Objects RAW Data: Robert Pölzl usually around 1 usually > 1 Fabian
More informationUsing Gaia for studying Milky Way star clusters
Using Gaia for studying Milky Way star clusters Eugene Vasiliev Institute of Astronomy, Cambridge Synopsis Overview of the Gaia mission and DR: scientific instruments, catalogue contents, measurement uncertainties,
More informationGetting started with Digital Astrophotography - Part I Rodger King - May 2016
Getting started with Digital Astrophotography - Part I Rodger King - May 2016 Flame Nebula orsehead Nebula. Question Astronomy Which type of Telescope is better - A Lens or Mirror? 500-900 More compact
More informationSOAR Integral Field Spectrograph (SIFS): Call for Science Verification Proposals
Published on SOAR (http://www.ctio.noao.edu/soar) Home > SOAR Integral Field Spectrograph (SIFS): Call for Science Verification Proposals SOAR Integral Field Spectrograph (SIFS): Call for Science Verification
More informationPhotometry using CCDs
Photometry using CCDs Signal-to-Noise Ratio (SNR) Instrumental & Standard Magnitudes Point Spread Function (PSF) Aperture Photometry & PSF Fitting Examples Some Old-Fashioned Photometers ! Arrangement
More informationDouble Star Measurements Using a Webcam: Annual Report of 2010
Page 233 Double Star Measurements Using a Webcam: Annual Report of 2010 J. S. Schlimmer Seeheim-Jugenheim, Hessen, Germany Email: js@epsilon-lyrae.de Abstract: I report on the measurements of 144 double
More informationBinocular and Scope Performance 57. Diffraction Effects
Binocular and Scope Performance 57 Diffraction Effects The resolving power of a perfect optical system is determined by diffraction that results from the wave nature of light. An infinitely distant point
More informationGPI INSTRUMENT PAGES
GPI INSTRUMENT PAGES This document presents a snapshot of the GPI Instrument web pages as of the date of the call for letters of intent. Please consult the GPI web pages themselves for up to the minute
More informationYou, too, can make useful and beautiful astronomical images at Mees: Lesson 1
You, too, can make useful and beautiful astronomical images at Mees: Lesson 1 Useful references: The Mees telescope startup/shutdown guide: http://www.pas.rochester.edu/~dmw/ast142/projects/chklist.pdf
More informationVEGAS: VST survey of Elliptical GAlaxies in the Southern hemisphere
INAF-GTO program VEGAS: VST survey of Elliptical GAlaxies in the Southern hemisphere P.I. Massimo Capaccioli University of Naples Federico II in collaboration with A. Grado, E. Iodice, N.R. Napolitano,
More informationBinocular Observer s Challenge:
Binocular Observer s Challenge: If you came to the Table Mountain Star Party (TMSP) with your binoculars or have access to binoculars while at the TMSP this program is for you. This program will give you
More informationDouble Star Marathon Observing List by: Glenn Chaple, 2016 R.A. (2000) Dec.
Double Star Marathon Observing List by: Glenn Chaple, 2016 Num Object Con SAO # R.A. (2000) Dec. PSA Mags. Sep ( ) PA ( ) Notes Time Eyepiece/Comments h m deg min 7 gamma And AND 037734 02 03.9 +42 20
More informationTotal Comet Magnitudes from CCD- and DSLR-Photometry
European Comet Conference Ondrejov 2015 Total Comet Magnitudes from CCD- and DSLR-Photometry Thomas Lehmann, Weimar (Germany) Overview 1. Introduction 2. Observation 3. Image Reduction 4. Comet Extraction
More informationSupplementary 110 Deep-Sky Objects
Appendix Supplementary 110 Deep-Sky Objects A variety of objects, some challenging, by the Deep Sky Group Saguaro Astronomy Club Version 1.0, dated Friday, 2 May 1991 This list is used by members of the
More informationIntroduction to Radio Astronomy
Introduction to Radio Astronomy The Visible Sky, Sagittarius Region 2 The Radio Sky 3 4 Optical and Radio can be done from the ground! 5 Outline The Discovery of Radio Waves Maxwell, Hertz and Marconi
More informationDouble Star Measures Using the Video Drift Method - XI
Page 566 Richard L. Nugent International Occultation Timing Association RNugent@wt.net Ernest W. Iverson International Occultation Timing Association ewiverson@consolidated.net Abstract: Position angles
More informationEnd-of-Chapter Exercises
End-of-Chapter Exercises Exercises 1 12 are conceptual questions designed to see whether you understand the main concepts in the chapter. 1. Red laser light shines on a double slit, creating a pattern
More informationPlanetary Nebulae. Planetary Nebulae 1
Planetary Nebulae A planetary nebula is a kind of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from old red giant stars late in their lives. The term "planetary nebula"
More informationBlack Holes in Giant Elliptical Galaxies
Gemini Observatory/AURA artwork by Lynette Cook Black Holes in Giant Elliptical Galaxies Chung-Pei Ma (UC Berkeley) Nicholas McConnell (UCB) Shelley Wright (UToronto) James Graham (UCB) Karl Gebhardt (UTexas)
More informationIntroducing Celestron s EdgeHD Optical System
Introducing Celestron s EdgeHD Optical System See the Universe in HD EdgeHD is an Aplanatic Schmidt telescope designed to produce aberration free images across a wide visual and photographic field of view.
More informationOptics and Telescopes
Optics and Telescopes Properties of Light Law of Reflection - reflection Angle of Incidence = Angle of Law of Refraction - Light beam is bent towards the normal when passing into a medium of higher Index
More informationPresented by Jerry Hubbell Lake of the Woods Observatory (MPC I24) President, Rappahannock Astronomy Club
Presented by Jerry Hubbell Lake of the Woods Observatory (MPC I24) President, Rappahannock Astronomy Club ENGINEERING A FIBER-FED FED SPECTROMETER FOR ASTRONOMICAL USE Objectives Discuss the engineering
More informationChapter 16 Light Waves and Color
Chapter 16 Light Waves and Color Lecture PowerPoint Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. What causes color? What causes reflection? What causes color?
More informationPhotometric Calibration for Wide- Area Space Surveillance Sensors
Photometric Calibration for Wide- Area Space Surveillance Sensors J.S. Stuart, E. C. Pearce, R. L. Lambour 2007 US-Russian Space Surveillance Workshop 30-31 October 2007 The work was sponsored by the Department
More information57 R.A. 20h 32' Decl Deep Sky Surfing
57 R.A. 20h 32' Decl. 30.0 57 38 56 58 82 83 84 57 Deep Sky Surfing 57 Chart 57 Basel 6 CYG 7.7 OC 14.0m 20h 06.8m 38 21.0' 40 13''-pB,pL,arrowhead shape, 22* at 100X Berk 86 CYG 7.9 OC 8.0m 20h 20.4m
More informationImage Enhancement (from Chapter 13) (V6)
Image Enhancement (from Chapter 13) (V6) Astronomical images often span a wide range of brightness, while important features contained in them span a very narrow range of brightness. Alternatively, interesting
More informationData Sheet. HMMC-5200 DC 20 GHz HBT Series Shunt Amplifier. Features. Description
HMMC-52 DC 2 GHz HBT Series Shunt Amplifier Data Sheet Description The HMMC-52 is a DC to 2 GHz, 9.5 db gain, feedback amplifier designed to be used as a cascadable gain block for a variety of applications.
More informationChapter 34. Images. Copyright 2014 John Wiley & Sons, Inc. All rights reserved.
Chapter 34 Images Copyright 34-1 Images and Plane Mirrors Learning Objectives 34.01 Distinguish virtual images from real images. 34.02 Explain the common roadway mirage. 34.03 Sketch a ray diagram for
More informationARRAY CONTROLLER REQUIREMENTS
ARRAY CONTROLLER REQUIREMENTS TABLE OF CONTENTS 1 INTRODUCTION...3 1.1 QUANTUM EFFICIENCY (QE)...3 1.2 READ NOISE...3 1.3 DARK CURRENT...3 1.4 BIAS STABILITY...3 1.5 RESIDUAL IMAGE AND PERSISTENCE...4
More informationExoplanet transit, eclipse, and phase curve observations with JWST NIRCam. Tom Greene & John Stansberry JWST NIRCam transit meeting March 12, 2014
Exoplanet transit, eclipse, and phase curve observations with JWST NIRCam Tom Greene & John Stansberry JWST NIRCam transit meeting March 12, 2014 1 Scope of Talk NIRCam overview Suggested transit modes
More informationIntroduction. Imaging and Processing Overview -Equipment and Software
Introduction Modern observing and imaging techniques, with automated goto mounts and CCD (charge-coupled device) cameras, http://en.wikipedia.org/wiki/charge-coupled_device allow detailed observation and
More informationPhotometry. Variable Star Photometry
Variable Star Photometry Photometry One of the most basic of astronomical analysis is photometry, or the monitoring of the light output of an astronomical object. Many stars, be they in binaries, interacting,
More informationProposal for a research project to be carried. out in Physics 400 (Senior Research) and. IDIS 493 (Honors Thesis).
Proposal for a research project to be carried out in Physics 400 (Senior Research) and IDIS 493 (Honors Thesis). Variable Star CCD Photometry and Analysis Amber L. Stuver Submitted in fulfillment of requirements
More informationPhase-2 Preparation Tool
Gran Telescopio Canarias Phase-2 Preparation Tool Valid from period 2012A Updated: 6 March 2012 1 Contents 1. The GTC Phase-2 System... 3 1.1. Introduction... 3 1.2. Logging in... 3 2. Defining an observing
More informationIntroduction to Trigonometry. Algebra 2
Introduction to Trigonometry Algebra 2 Angle Rotation Angle formed by the starting and ending positions of a ray that rotates about its endpoint Use θ to represent the angle measure Greek letter theta
More informationPHYS 202 OUTLINE FOR PART III LIGHT & OPTICS
PHYS 202 OUTLINE FOR PART III LIGHT & OPTICS Electromagnetic Waves A. Electromagnetic waves S-23,24 1. speed of waves = 1/( o o ) ½ = 3 x 10 8 m/s = c 2. waves and frequency: the spectrum (a) radio red
More informationAutoguiding the Remote Telescope
1 of 8 1/17/2009 8:28 PM Autoguiding the Remote Telescope When the ST-10XE is installed in the C14, you can use the built-in autoguiding chip to autoguide long exposures. For most exposures with the ST-10XE,
More informationDBSP Observing Manual
DBSP Observing Manual I. Arcavi, P. Bilgi, N.Blagorodnova, K.Burdge, A.Y.Q.Ho June 18, 2018 Contents 1 Observing Guides 2 2 Before arrival 2 2.1 Submit observing setup..................................
More informationDefocusing and Deblurring by Using with Fourier Transfer
Defocusing and Deblurring by Using with Fourier Transfer AKIRA YANAGAWA and TATSUYA KATO 1. Introduction Image data may be obtained through an image system, such as a video camera or a digital still camera.
More informationIntroduction to Astronomy Images and the DS9 Image Viewer
Introduction to Astronomy Images and the DS9 Image Viewer George J. Bendo School of Physics and Astronomy The University of Manchester Version: 11 March 218 Contents Introduction to Astronomy Images 3
More informationTelescope Observer s Challenge:
Telescope Observer s Challenge: If you came to the Table Mountain Star Party (TMSP) with your telescope or have access to a telescope while at the TMSP this program is for you. This program will give you
More informationMicroscope & Measuring
Name: ate: 1. microscope is supplied with 10 and 15 eyepieces, and with 10 and 44 objectives. What is the maximum magnification that can be obtained from this microscope?. 59. 150. 440. 660 3. student
More informationVisualizing the Chances of Winning a Lottery
Visualizing the Chances of Winning a Lottery By W. Conway Link Department of Mathematics Louisiana State University in Shreveport One University Place Shreveport, LA 71115 PH: 318.797.5300 Email: clink@pilot.lsus.edu
More informationYou identified, analyzed, and graphed quadratic functions. (Lesson 1 5) Analyze and graph equations of parabolas. Write equations of parabolas.
You identified, analyzed, and graphed quadratic functions. (Lesson 1 5) Analyze and graph equations of parabolas. Write equations of parabolas. conic section degenerate conic locus parabola focus directrix
More informationMaking Dark Shadows with Linear Programming
Making Dark Shadows with Linear Programming Robert J. Vanderbei 28 Nov 1 Faculty of Engineering Dept. of Management Sciences University of Waterloo http://www.princeton.edu/~rvdb Are We Alone? Indirect
More informationApplications: Signal Isolation. The is a Current-to-Current Opto-Isolator designed for high temperature applications to 200ºC.
52458 Dual Current-to-Current Opto-Isolator, High (200 C) Mii Features: Hermetically Sealed Package Optically Coupled Input/Output Isolation Tested to 1000 VDC 200 C Operation Applications: Signal Isolation
More informationSONG Stellar Observations Network Group. The prototype
SONG Stellar Observations Network Group The prototype F. Grundahl1, J. Christensen Dalsgaard1, U. G. Jørgensen2, H. Kjeldsen1,S. Frandsen1 and P. Kjærgaard2 1) Danish AsteroSeismology Centre, University
More informationOlivier Thizy François Cochard
Alpy guiding User Guide Olivier Thizy (olivier.thizy@shelyak.com) François Cochard (francois.cochard@shelyak.com) DC0017B : feb. 2014 Alpy guiding module User Guide Olivier Thizy (olivier.thizy@shelyak.com)
More informationChapters 1 & 2. Definitions and applications Conceptual basis of photogrammetric processing
Chapters 1 & 2 Chapter 1: Photogrammetry Definitions and applications Conceptual basis of photogrammetric processing Transition from two-dimensional imagery to three-dimensional information Automation
More informationAPPENDIX D: ANALYZING ASTRONOMICAL IMAGES WITH MAXIM DL
APPENDIX D: ANALYZING ASTRONOMICAL IMAGES WITH MAXIM DL Written by T.Jaeger INTRODUCTION Early astronomers relied on handmade sketches to record their observations (see Galileo s sketches of Jupiter s
More informationA CATALOG OF 120 NGC OPEN STAR CLUSTERS
Journal of The Korean Astronomical Society doi:10.5303/jkas.2011.44.1.1 44: 1 11, 2011 February ISSN:1225-4614 c 2011 The Korean Astronomical Society. All Rights Reserved. http://jkas.kas.org A CATALOG
More informationAngles 1. Angles 2. Which equation can be used to find the value of x? What is the m AGH? a. 180º. a. 2 x = x b. 30º. b. 2 x + x + 15 = 180
Angles 1 In the accompanying diagram, parallel lines AB and CD are intersected by transversal EF at points G and H, respectively, m AGH = x + 15, and m GHD = 2x. Which equation can be used to find the
More informationStellar Photometry: I. Measuring. Ast 401/Phy 580 Fall 2014
What s Left (Today): Introduction to Photometry Nov 10 Photometry I/Spectra I Nov 12 Spectra II Nov 17 Guest lecture on IR by Trilling Nov 19 Radio lecture by Hunter Nov 24 Canceled Nov 26 Thanksgiving
More informationPhotovoltaic Series. Planar Diffused Silicon Photodiodes FEATURES APPLICATIONS
Photovoltaic Series Planar Diffused Silicon Photodiodes The Photovoltaic Detector series is utilized for applications requiring high sensitivity and moderate response speeds, with an additional sensitivity
More informationAchieving milli-arcsecond residual astrometric error for the JMAPS mission
Achieving milli-arcsecond residual astrometric error for the JMAPS mission Gregory S. Hennessy a,benjaminf.lane b, Dan Veilette a, and Christopher Dieck a a US Naval Observatory, 3450 Mass Ave. NW, Washington
More informationPhysics Learning Guide Name:
Physics Learning Guide Name: Instructions: Using a pencil, complete the following notes as you work through the related lessons. Show ALL work as is explained in the lessons. You are required to have this
More informationOptics & Light. See What I m Talking About. Grade 8 - Science OPTICS - GRADE 8 SCIENCE 1
Optics & Light See What I m Talking About Grade 8 - Science OPTICS - GRADE 8 SCIENCE 1 Overview In this cluster, students broaden their understanding of how light is produced, transmitted, and detected.
More informationPhotometry. La Palma trip 2014 Lecture 2 Prof. S.C. Trager
Photometry La Palma trip 2014 Lecture 2 Prof. S.C. Trager Photometry is the measurement of magnitude from images technically, it s the measurement of light, but astronomers use the above definition these
More informationPocket Pumped Image Analysis Ivan Kotov Brookhaven National Laboratory
Pocket Pumped Image Analysis Ivan Kotov Brookhaven National Laboratory Instrumentation Division Seminar November 13, 2013 1 CCD Readout Architecture Terms Charge motion Image area (exposed to light) Parallel
More informationModel ST-9XE CCD Imaging Camera SBIG ASTRONOMICAL INSTRUMENTS
Model ST-9XE CCD Imaging Camera.. SBIG ASTRONOMICAL INSTRUMENTS 1... Model ST-9XE Dual CCD Self-Guiding Camera The ST-9XE is identical to the ST-7/8/10/2000 cameras with the exception of the imaging CCD.
More informationSection 3. Imaging With A Thin Lens
3-1 Section 3 Imaging With A Thin Lens Object at Infinity An object at infinity produces a set of collimated set of rays entering the optical system. Consider the rays from a finite object located on the
More informationCheckerboard-Mask Coronagraphs for High-Contrast Imaging
Checkerboard-Mask Coronagraphs for High-Contrast Imaging Robert J. Vanderbei Operations Research and Financial Engineering, Princeton University rvdb@princeton.edu N. Jeremy Kasdin Mechanical and Aerospace
More information1 Laboratory 7: Fourier Optics
1051-455-20073 Physical Optics 1 Laboratory 7: Fourier Optics 1.1 Theory: References: Introduction to Optics Pedrottis Chapters 11 and 21 Optics E. Hecht Chapters 10 and 11 The Fourier transform is an
More informationPinhole Camera. Nuts and Bolts
Nuts and Bolts What Students Will Do Build a specialized, Sun-measuring pinhole camera. Safely observe the Sun with the pinhole camera and record image size measurements. Calculate the diameter of the
More informationUnit 1.5 Waves. The number waves per second. 1 Hz is 1waves per second. If there are 40 waves in 10 seconds then the frequency is 4 Hz.
Unit 1.5 Waves Basic information Transverse: The oscillations of the particles are at right angles (90 ) to the direction of travel (propagation) of the wave. Examples: All electromagnetic waves (Light,
More informationJust How Good Are Flats? John Menke May 2005
Just How Good Are Flats? John Menke May 2005 Abstract Using flats as a means of correcting various errors in CCD images is well known. What is not so well known is how well they work. This paper describes
More informationD I S T R I B U T I O N. Reference : GAIA-EST-RD Date : 21th May 2013 Issue 3 - revision 1 page ii. organisation
D I S T R I B U T I O N Reference : GAIA-EST-RD-00553 page ii name organisation page iii C H A N G E L O G date issue revision pages reason for change 1-7-2005 1 0 First Issue 16-11-2006 2 0 5, 16, 20,
More informationGeometric optics & aberrations
Geometric optics & aberrations Department of Astrophysical Sciences University AST 542 http://www.northerneye.co.uk/ Outline Introduction: Optics in astronomy Basics of geometric optics Paraxial approximation
More informationChapter 23 Electromagnetic Waves Lecture 14
Chapter 23 Electromagnetic Waves Lecture 14 23.1 The Discovery of Electromagnetic Waves 23.2 Properties of Electromagnetic Waves 23.3 Electromagnetic Waves Carry Energy and Momentum 23.4 Types of Electromagnetic
More informationOPTOLONG L Pro pollution filter testing
OPTOLONG L Pro pollution filter testing The Chinese filter manufacturer OPTOLONG based in Kunming city in the southern province of Yunnan contacted me to test their light pollution premium filter, the
More informationHigh Dynamic Range Processing Ken Crawford
High Dynamic Range Processing Ken Crawford Deep sky astronomical Images are produced by capturing and building up very faint signals over an extended period of time. Although faint, some objects produce
More informationQHY5III290MM Review. 1 - Read noise tests. 2 - Anti Amp-glow tests. 3 - Sky surveilance tests. 4 - Test behind the scope
QHY5III290MM Review This is a review after 6 months of use, overall i'm very pleased. This camera allows number of things that would be impossible to acheive with anything else, and i hope improvements
More informationScience Detectors for E-ELT Instruments. Mark Casali
Science Detectors for E-ELT Instruments Mark Casali 1 The Telescope Nasmyth telescope with a segmented primary mirror. Novel 5 mirror design to include adaptive optics in the telescope. Classical 3mirror
More informationElectromagnetism and Light
Electromagnetism and Light Monday Properties of waves (sound and light) interference, diffraction [Hewitt 12] Tuesday Light waves, diffraction, refraction, Snell's Law. [Hewitt 13, 14] Wednesday Lenses,
More informationColor and the Human Eye
Color Images Source: wikipedia Biophysical basis: Color and the Human Eye - The human eye contains 3 kinds photoreceptive cells (cone) cells that respond to different wavelengths: L : longer wavelengths
More informationDynamic Range. Can I look at bright and faint things at the same time?
Detector Basics The purpose of any detector is to record the light collected by the telescope. All detectors transform the incident radiation into a some other form to create a permanent record, such as
More informationSAC's. 110 Best of the NGC. 110 Best of the NGC
SAC's 110 Best of the NGC 110 Best of the NGC Pagina 1 F,vS,R,vsmbM,L*cont f 13 NGC 40 PK 120+9.1 PLNNB CEP 00 13.0 +72 31 10,7 7,3 60 s 40 s 3b(3) # 37 NGC 185 UGC 396 GALXY CAS 00 39.0 +48 20 9,2 14,3
More informationSimulations of the STIS CCD Clear Imaging Mode PSF
1997 HST Calibration Workshop Space Telescope Science Institute, 1997 S. Casertano, et al., eds. Simulations of the STIS CCD Clear Imaging Mode PSF R.H. Cornett Hughes STX, Code 681, NASA/GSFC, Greenbelt
More informationAlgebra 1 Final Exam 4 B. 1, 2.5, 1 2, 0.75, 4 4, x 30. Name Period Score / 51pts.
Algebra 1 Final Exam Name Period Score / 51pts Multiple Choice: 1 pt each 1 List the numbers from least to greatest: 075, 4, 25, 1 2, 1 A 1 2, 075, 25, 1, 4 B 1, 25, 1 2, 075, 4 C 25, 1, 1 2, 075, 4 D
More informationDouble Star Measurements Using a Webcam and CCD Camera, Annual Report of 2016
Page 22 Double Star Measurements Using a Webcam and CCD Camera, Annual Report of 2016 Joerg S. Schlimmer 64342 Seeheim-Jugenheim, Germany js@epsilon-lyrae.de Abstract: This report shows the results on
More informationRF Noise Simulation for Submicron MOSFET s Based on Hydrodynamic Model
RF Noise Simulation for Submicron MOSFET s Based on Hydrodynamic Model Jung-Suk Goo, Chang-Hoon Choi, Eiji Morifuji, Hisayo Sasaki Momose, Zhiping Yu, Hiroshi Iwai, Thomas H. Lee, and Robert W. Dutton,
More informationOn the variation of the energy scale 3
22-Nov-15 On the variation of the energy scale 3 Page 1 On the variation of the energy scale 3 Parameters for galaxy rotation curves by Jo. Ke. Sun 22nd Nov 215 22-Nov-15 On the variation of the energy
More informationThrough Hole Lamp Product Data Sheet LTL-4231N-002 Spec No.: DS Effective Date: 03/25/2000 LITE-ON DCC RELEASE
Through Hole Lamp Product Data Sheet LTL-4231N-002 Spec No.: DS20-2000-100 Effective Date: 03/25/2000 Revision: - LITE-ON DCC RELEASE BNS-OD-FC001/A4 LITE-ON Technology Corp. / Optoelectronics No.90,Chien
More information25 cm. 60 cm. 50 cm. 40 cm.
Geometrical Optics 7. The image formed by a plane mirror is: (a) Real. (b) Virtual. (c) Erect and of equal size. (d) Laterally inverted. (e) B, c, and d. (f) A, b and c. 8. A real image is that: (a) Which
More informationPhysics 1C. Lecture 25B
Physics 1C Lecture 25B "More than 50 years ago, Austrian researcher Ivo Kohler gave people goggles thats severely distorted their vision: The lenses turned the world upside down. After several weeks, subjects
More information