Zone 7, Master Map Normal View
|
|
- Joel O’Neal’
- 5 years ago
- Views:
Transcription
1 , 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 , 41 Dra NGC Ursa Minor NGC 6324 Hussey 65 STF 2299 Kustner 1 STF 2077 rej STF 2134 rej ε STF 2125 rej Epsilon UMi P Muller 351 η 856 STF 2002 rej NGC 6217 STF 1997 rej STF 2066 ζ STF 1980 Pi 1 UMi θ STF 2013 rej STF 2020 rej Hussey STF 1971 rej P Muller 194 P Muller ' ' ' ' ' ' ' ' ' ' ' STF 2179 NGC 6434 h3346 NGC 6340 STF h 20m 17h 00m 16h 40m 16h 20m 16h 00m 15h 40m
2 , Map 1 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. δ 24 UMi OS 340 Draco P Muller 218 Hussey 65 STF 2299 STF 2326 Ursa Minor 40, 41 Dra P Muller 352 STF 2125 rej ε Epsilon UMi P Muller ' ' ' ' ' ' ' 18h 00m 17h 36m 17h 12m 16h 48m 16h 24m
3 , Map 1 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF UMi OS 340 δ ur 353 STF 2002 rej P Muller 351 P Muller 352 Draco STF 2299 STF 2125 rej ε Epsilon UMi P Muller 218 Hussey 65 STF 2326 Ursa Minor 40, 41 Dra ' ' ' ' ' ' ' 16h 24m 16h 48m 17h 12m 17h 36m 18h 00m
4 , Map 2 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF 2302 STF , 41 Dra Draco P Muller 209 NGC 6412 NGC 6324 Ursa Minor ε STF 2125 rej Epsilon UMi P Muller 351 NGC 6217 Kustner 1 STF 2077 rej STF 2134 rej η ' ' ' ' ' ' ' ' ' H I 41 18h 00m 17h 40m 17h 20m 17h 00m 16h 40m
5 , Map 2 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. 856 P Muller 351 STF 2077 rej STF 2066 NGC 6217 ε Kustner 1 STF 2125 rej Epsilon UMi STF 2134 rej Draco NGC 6324 NGC 6412 Ursa Minor STF , 41 Dra P Muller ' ' ' ' ' ' ' ' ' H I 41 16h 40m 17h 00m 17h 20m 17h 40m 18h 00m
6 , Map 3 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. Kustner 1 P Muller 351 NGC 6217 STF 2066 η Hussey 916 ζ STF 1997 rej θ STF 2013 rej STF 2020 rej STF 1971 rej P Muller 349 P Muller 194 STF 1933 rej ' ' ' ' ' ' ' STF 2036 STF h 24m 16h 00m 15h 36m Gamma UMiγ Pherkad 15h 12m
7 , Map 3 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. Hussey 908 STF 1933 rej θ ζ STF 1997 rej STF 1971 rej P Muller 351 STF 2013 rej STF 2066 STF 2020 rej η Hussey 916 Draco P Muller 194 P Muller ' ' ' ' ' ' ' STF 1928 STF 2036 γ Pherkad Gamma UMi 15h 12m 15h 36m 16h 00m 16h 24m
8 , Map 4 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF 2125 rej STF 2002 rej 856 STF 1980 Pi 1 UMi STF 1933 rej Hussey 908 OSS 130 Cam STF 1880 rej ' ' ' ' ' ' ' ζ STF 1997 rej θ 16h 00m 15h 40m 15h 20m 15h 00m 14h 40m
9 , Map 4 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. OS 281 OSS 130 STF Camelopardalis 1851 STF 1880 rej STF 2002 rej 856 STF 1980 Pi 1 UMi STF 1933 rej Hussey 908 ε ' ' ' ' ' ' ' ζ STF 1997 rej θ 14h 40m 15h 00m 15h 20m 15h 40m 16h 00m
10 Index 19 double stars, 3 galaxies 4 40, 41 Dra E Epsilon UMi... 3 K Kustner N NGC NGC NGC P P Muller P Muller Pi 1 UMi S STF 1933 rej STF 1971 rej STF STF 1997 rej STF 2002 rej STF 2013 rej STF 2020 rej STF STF 2077 rej... 4 STF 2125 rej... 2 STF 2134 rej... 5 STF
11 , Map 1 Double Stars Easy STF 2125 rej Other name(s): DS 10220; SO 2757 Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 8.89 K0 Y = pr? 1899: measurements. May be optical because Hipparcos gives different distances (960 and 396 light years). C11 at 98x. STF 2299 Other name(s): SO 2933 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.46 F8 W ? 1991 W 1899: measurements. Quadrant reversal? C11 at 115x
12 Epsilon UMi Rating: 5 M Other name(s): Harvard 143; DS 10242; HD ; SO 2770 Position: Magnitude Separation P Year Spectra Colors 4.23 G5 III Y ? 1879: 7. 4 measurements. Star is an eclipsing binary like lgol, with a day period. C8 at 104x. Moderate field. Scale model (in which the Sun is the size of a baseball): Diameter: = 39.0 inches. Separation: = 41.7 miles; a = 6.09 feet. Distance (LY): 347 Total luminosity (Suns): Difficult - 3 -
13 , Map 2 Double Stars Easy STF 2066 Other name(s): DS Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.98 F8 W W 1832: measurements. C8 at 104x. Nice field, but a faint pair. Too bad it is not brighter. Scale model (in which the Sun is the size of a baseball): Diameter: = 16.7 inches. Separation: = 1.14 miles. Distance (LY): 141 Total luminosity (Suns): 0.29 STF 2077 rej Other name(s): SO 8524 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.27 F8 Y ro 1894: measurements
14 C8 at 104x. Very, very rich field to the W. Scale model (in which the Sun is the size of a baseball): Diameter: = 16.1 inches. Separation: = 8.45 miles. Distance (LY): 308 Total luminosity (Suns): 1.47 P Muller 351 Rating: 3 E Position: Magnitude Separation P Year Spectra Colors W W 1896: measurements. C11 at 193x. STF 2134 rej Other name(s): SO 8679 Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.42 F2 W W? 1895: measurements. This system may be optical as Hipparcos shows different distances (870 and 847 light years)
15 C11 at 115x. Nice field. 40, 41 Dra Rating: 1 E Other name(s): STF 2308; DS 11061; HD ; SO 8994 L League Program: Double Star Certificate Position: Magnitude Separation P Year Spectra Colors 5.74 F7 V W F7 V W C W 1832: 236. Over 100 measurements. C 1932: measurements. alega discovered to be a spectroscopic binary, resolved with speckle interferometry, at 322. has a period of 1,247.2 days and the highest known eccentricity to date with e = 0.975! is also a spectroscopic binary with a period of only days. C8 at 104x. Very nice set of "headlights!" Scale model (in which the Sun is the size of a baseball): Diameter: = 3.9 inches; = 12.5 inches. Separation: = 4.99 miles; C = 60.4 miles; a = 142 feet. Distance (LY): 173 Total luminosity (Suns): 21 For a sketch, see the next page
16 40 and 41 Dra Double Star; 5.7, ) C8 at 100x Jul. 6, 1995 Difficult Kustner 1 Other name(s): DS 10214; HD ; SO 8612 Rating: 5 D Position: Magnitude Separation P Year Spectra Colors 5.99 F4 IV yw ? C ? 1889: measurements
17 C 1914: measurements. Hipparcos shows the C star to be at a distance of 43 light years. C8 at 280x. Scale model (in which the Sun is the size of a baseball): Diameter: = 8.1 inches. Separation: = 2,482 feet; C = 21.0 miles. Distance (LY): 117 Total luminosity (Suns): 4.6 P Muller 209 Other name(s): SO 8923 Rating: 2 D Position: Magnitude Separation P Year Spectra Colors F5 W W 1971: measurements. C11 at 634x. It lies at the center of a "Y" asterism
18 Deep Sky Objects Moderate NGC 6324 Other Names: UGC 10725, H III 945 Rating: 4 M Position: Type : Gal Class: Sbc Magnitude : 12.8 Surface brightness: 11.9 Dimensions: 1' x 0.6' P: 78 C11 at 140x. Small (30" diameter) and round, with a very gradually brighter middle. n 11m star lies just to the S, and an 8.6m star to the N. Difficult NGC 6217 Other Names: UGC 10470; rp 185, H I 280 stronomical League Program: Herschel 400 Rating: 5 D Position: Type : Gal Class: (R)S(rs)bc Magnitude : 11.9 Surface brightness: 13.6 Dimensions: 2' x 1' This is a Seyfert galaxy and shows signs of starburst activity. C8 at 104x. Small and faint. It forms a line with two faint stars. Its axis runs N-S
19 NGC 6412 Other Names: rp 38, UGC 10897, H VI 41 Rating: 5 D Position: Type : Gal Class: S(s)c II Magnitude : 12.4 Surface brightness: 13.2 Dimensions: 2' x 1.5' C8 at 104x. Small and faint, Geoff Chester called it "a bear!" Several nearby stars almost wash it out, including 8.3m SO min S
20 , Map 3 Double Stars Easy STF 2013 rej Other name(s): SO 8383 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors K0 Y W 1894: measurements. This system may be optical as Hipparcos shows different distances (86 and 100 light years). The proper motions are also quite different. C11 at 115x. STF 2020 rej Other name(s): DS 7522 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.86 G5 yo : measurements. C8 at 104x
21 Scale model (in which the Sun is the size of a baseball): Diameter: = 21.5 inches. Separation: = 10.0 miles. Distance (LY): 242 Total luminosity (Suns): 0.8 Moderate STF 1971 rej Other name(s): SO 8288 Rating: 5 M Position: Magnitude Separation P Year Spectra Colors 9.64 K5 Y ? 1907: measurements. C11 at 115x. STF 1997 rej Other name(s): SO 8348 Rating: 5 M Position: Magnitude Separation P Year Spectra Colors 9.31 K0 Y ? 1896: measurements. C8 at 104x
22 Scale model (in which the Sun is the size of a baseball): Diameter: = 26.2 inches. Separation: = 4.01 miles. Distance (LY): 139 Total luminosity (Suns): 0.32 Double Stars, Map 4 Easy STF 1933 rej Other name(s): SO 8168 Rating: 5 E Position: Magnitude Separation P Year Spectra Colors 9.38 G0 yw = 1991 W? 1905: measurements. C11 at 115x. Scale model (in which the Sun is the size of a baseball): Diameter: = 18.3 inches. Separation: = 21.4 miles. Distance (LY): 540 Total luminosity (Suns):
23 Pi 1 UMi Other name(s): STF 1972; DS 9696; HD ; SO 2556 Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 6.57 G8 IV Y G5 V W C ? 1832: measurements. Stars and are a spectroscopic binaries. C 1911: measurements. C8 at 104x. This star is the S vertex of a nice 7m triangle with SO 2562 to the N and 2576 to the NE. Webb saw them as Y and bw. Scale model (in which the Sun is the size of a baseball): Diameter: = 11.1 inches; = 18.5 inches. Separation: = 3.57 miles; C = 17.3 miles. Distance (LY): 72 Total luminosity (Suns): 1.44 STF 1980 Other name(s): DS 9724; SO 2568 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.10 F R 1832: measurements. The stars have a small difference in proper motion. C8 at 104x
24 STF 2002 rej Other name(s): HD ; SO 2619 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 8.81 F5 W : measurements. Hipparcos/Tycho data show different distances for these stars; they may be optical. C8 at 104x. It sits inside a bright, large triangle made up of 7.3m SO 2606, 7.1m SO 2625, and 8.2m SO Scale model (in which the Sun is the size of a baseball): Diameter: = 13.7 inches. Separation: = 22.2 miles. Distance (LY): 333 Total luminosity (Suns): 3.66 Moderate 856 Other name(s): DS 9798; HD ; SO 2599 Rating: 4 M Position: Magnitude Separation P Year Spectra Colors 8.27 G5 yw No C ? 1904: measurements. C 1899: measurements
25 C8 at 104x. It is set amidst a flock of 9m stars. Scale model (in which the Sun is the size of a baseball): Diameter: = 19.7 inches. Separation: = 3.33 miles; C = 43.5 miles. Distance (LY): 419 Total luminosity (Suns):
26 Mini-Catalog Double Stars Star Specifications Designation Position Rating Map Component Mag Sep from P from 40, 41 Dra E 2 C Pi 1 UMi E 4 P Muller E 2 STF 2125 rej E 1 STF 2134 rej E 2 STF E 4 STF 2002 rej E 4 STF 2013 rej E 3 STF 2020 rej E 3 STF E 2 STF 2077 rej E 2 STF E 1 STF 1933 rej E M 4 STF 1971 rej M 3 STF 1997 rej M 3 Epsilon UMi M 1 P Muller D 2 Kustner D 2 Hussey TD 3 C C C C = = ? 277 =
27 Deep Sky Objects Zone Specifications Object Position Rating Submap Type Mag Surface r Population NGC M 2 Gal (Sbc) NGC D 2 Gal ((R)S(rs)b c) NGC D 2 Gal (S(s)c II)
Zone 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 217, Master Map Normal View
Zone Master, Normal View, 10 deg FOV, Master Map Normal View β Zubeneschamali ε δ ξ2-14 00' -12 00' -10 00' -08 00' -06 00' -04 00' γ η ο Libra 16h 00m 15h 52m 15h 44m 15h 36m 15h 28m 15h 20m 15h 12m 15h
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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 informationMeasurement of Double Stars Using Webcams 2011 and 2012
Page 176 Measurement of Double Stars Using Webcams 2011 and 2012 Allen S. Malsbury, P.E Parsippany, New Jersey, USA clearskyobserverwebmaster@gmail.com Abstract: A description is given of the equipment
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 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 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 informationSection 5.1 Angles and Radian Measure. Ever Feel Like You re Just Going in Circles?
Section 5.1 Angles and Radian Measure Ever Feel Like You re Just Going in Circles? You re riding on a Ferris wheel and wonder how fast you are traveling. Before you got on the ride, the operator told you
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 informationA Recipe For Dark Sky Photography
Fountain Hills Photography Club Information Series A Recipe For Dark Sky Photography March 14, 2018 Examples of Dark Sky pictures you can take without expensive gear (like telescope with a clock drive)
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 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 informationHercules - The Son of Zeus
IC 1152 IC 1153 IC 1156 VF,CS,OVAL,NND,AV,R=F IC 4593 Jun 03 2005 VB,VS,R,HISB,R=G Planetary Neb 2+2 IC 4615 Non-Existent MAC 1644+4005 VF,VS,R,NND,AV,R=F Galaxy NGC 6013 Galaxy SBb VF,CS,EL,OVAL,NND,AV,R=F
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 informationTelescopes and their configurations. Quick review at the GO level
Telescopes and their configurations Quick review at the GO level Refraction & Reflection Light travels slower in denser material Speed depends on wavelength Image Formation real Focal Length (f) : Distance
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 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 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 information-NGC NGC NGC NGC M109 -NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC 3941
Ursa Major - Generale Ursa Minor -NGC 2985 -M82 -M81 -NGC 2976 Bootes -NGC 5473 -NGC -M101 5474 -NGC 5308 -NGC 5322 -NGC 5204 -r5055 Canes Venatici -NGC 2880 -NGC 2654 -NGC 2742 -NGC 4605 -NGC 3359 -NGC
More informationWEBCAMS UNDER THE SPOTLIGHT
WEBCAMS UNDER THE SPOTLIGHT MEASURING THE KEY PERFORMANCE CHARACTERISTICS OF A WEBCAM BASED IMAGER Robin Leadbeater Q-2006 If a camera is going to be used for scientific measurements, it is important to
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 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 informationColor-Contrast Double Stars
SAO RA h:m:s Dec :m:s Sorted by RA / Sigma Cassiopeia 35947 23:59:00 +55d45m00s 5 7.1 3.1 326-0.07-0.05 0.02 Contrasting blue and green hues OSS254 Cassiopeia 00:01:12 +60d21m00s 7.6 8.7 58 2.93 0.00 2.93
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 informationThe Wave Nature of Light
The Wave Nature of Light Physics 102 Lecture 7 4 April 2002 Pick up Grating & Foil & Pin 4 Apr 2002 Physics 102 Lecture 7 1 Light acts like a wave! Last week we saw that light travels from place to place
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 information1. Measure angle in degrees and radians 2. Find coterminal angles 3. Determine the arc length of a circle
Pre- Calculus Mathematics 12 5.1 Trigonometric Functions Goal: 1. Measure angle in degrees and radians 2. Find coterminal angles 3. Determine the arc length of a circle Measuring Angles: Angles in Standard
More informationASTR130: Astro-Photography Lab. Orientation Session Spring 2009
ASTR130: Astro-Photography Lab Orientation Session Spring 2009 Rachael Beaton April 16, 2009 I. Objectives 1.Explain Lab Requirements 2.Explain Available Equipment and Check-Out Procedures 3.Learn and
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 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 informationAdaptive Coronagraphy Using a Digital Micromirror Array
Adaptive Coronagraphy Using a Digital Micromirror Array Oregon State University Department of Physics by Brad Hermens Advisor: Dr. William Hetherington June 6, 2014 Abstract Coronagraphs have been used
More informationTelescope Basics by Keith Beadman
Telescope Basics 2009 by Keith Beadman Table of Contents Introduction...1 The Basics...2 What a telescope is...2 Aperture size...3 Focal length...4 Focal ratio...5 Magnification...6 Introduction In the
More informationS.A.A. 100 Observing Club
S.A.A. 100 Observing Club Raleigh Astronomy Club Version 1.2 07-AUG-2005 Introduction Welcome to the S.A.A. 100 Observing Club! This list started on the USENET newsgroup sci.astro.amateur when someone
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 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 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 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 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 informationCircuit Analysis-II. Circuit Analysis-II Lecture # 2 Wednesday 28 th Mar, 18
Circuit Analysis-II Angular Measurement Angular Measurement of a Sine Wave ü As we already know that a sinusoidal voltage can be produced by an ac generator. ü As the windings on the rotor of the ac generator
More informationMATH Exam 2 Solutions November 16, 2015
MATH 1.54 Exam Solutions November 16, 15 1. Suppose f(x, y) is a differentiable function such that it and its derivatives take on the following values: (x, y) f(x, y) f x (x, y) f y (x, y) f xx (x, y)
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 informationStation # 1. Reflection off of a rough surface. The Law of reflection. Problem: How is light reflected off of a flat smooth surface?
In your notes Station # 1 LABEL ME When a light ray strikes an object and bounces off Ex. Mirror Reflection off of a smooth surface Reflection off of a rough surface The Law of Reflection states that the
More informationAlgebra II B Review 3
Algebra II B Review 3 Multiple Choice Identify the choice that best completes the statement or answers the question. Graph the equation. Describe the graph and its lines of symmetry. 1. a. c. b. graph
More informationTODAY S OUTCOMES: BEHAVIOR OF LIGHT - Review concepts behind visibility in mirrors and pinhole cameras
TODAY S OUTCOMES: BEHAVIOR OF LIGHT - Review concepts behind visibility in mirrors and pinhole cameras - Discover what mirror images are and how they are formed by reflections - Predict where mirror images
More informationAdaptive Optics Lectures
Adaptive Optics Lectures Andrei Tokovinin 3. SOAR Adaptive Module (SAM) SAM web pages: SOAR--> SAM http://www.ctio.noao.edu/new/telescopes/soar/instruments/sam/ Paper (2016, PASP, 128, 125003): http://www.ctio.noao.edu/~atokovin/papers/sam-pasp.pdf
More informationUV/Optical/IR Astronomy Part 2: Spectroscopy
UV/Optical/IR Astronomy Part 2: Spectroscopy Introduction We now turn to spectroscopy. Much of what you need to know about this is the same as for imaging I ll concentrate on the differences. Slicing the
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 informationOberwerk Ultra 15x70 Compared to other 70mm binoculars by Ed Zarenski Oct. 15, 2006
Oberwerk Ultra 15x70 Compared to other 70mm binoculars by Ed Zarenski Oct. 15, 2006 Are These All the Same? The buzz on the street is all about the new "premium" binocular. There are a number of importers/distributors
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 informationLocally Optimized Combination of Images (LOCI) Algorithm
Locally Optimized Combination of Images (LOCI) Algorithm Keck NIRC2 Implementation using Matlab Justin R. Crepp 1. INTRODUCTION Of the myriad post-processing techniques used to reduce highcontrast imaging
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 informationTitle: Oct 9 8:27 AM (1 of 30)
Applied Max and Min (Optimization) 1. If you have 100 feet of fencing and you want to enclose a rectangular area up against a long, straight wall, what is the largest area you can enclose? Title: Oct 9
More information12-6 Circular and Periodic Functions
26. CCSS SENSE-MAKING In the engine at the right, the distance d from the piston to the center of the circle, called the crankshaft, is a function of the speed of the piston rod. Point R on the piston
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 informationIP, 4K/UHD & HDR test & measurement challenges explained. Phillip Adams, Managing Director
IP, 4K/UHD & HDR test & measurement challenges explained Phillip Adams, Managing Director Challenges of SDR HDR transition What s to be covered o HDR a quick overview o Compliance & monitoring challenges
More informationEASTMAN TRI-X Reversal Film 7278
MPTVI Data Sheet XXXXXXXXXXX XX KODAK XX XX TInet XX XXXXXXXXXXX Technical Information Copyright, Eastman Kodak Company, 1994 1) Description EASTMAN TRI-X Reversal Film 7278 EASTMAN TRI-X Reversal Film
More informationML # 1: Similar Figures and Scale Drawings (Unit 7 Math 7 PLUS) SCALE FACTOR: SIMILAR FIGURES:
ML # 1: Similar Figures and Scale Drawings (Unit 7 Math 7 PLUS) SCALE FACTOR: SIMILAR FIGURES: Corresponding Sides and Angles Corresponding Sides and Angles: Sides or angles that lie in the same location
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 informationSYNGUIDER USER'S MANUAL
SYNGUIDER USER'S MANUAL GETTING STARTED PREPARING THE SYNGUIDER BASIC OPERATIONS OPERATION UNDER THE NIGHT SKY SPECIFICATIONS 1 3 4 9 15 060613V1 Thank you for choosing the SynGuider. The SynGuider can
More informationDigital Image Processing. Lecture # 3 Image Enhancement
Digital Image Processing Lecture # 3 Image Enhancement 1 Image Enhancement Image Enhancement 3 Image Enhancement 4 Image Enhancement Process an image so that the result is more suitable than the original
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 informationLow-Cost Single Mirror Telescope Product Requirements Document Team Z-Telescope
Low-Cost Single Mirror Telescope Product Requirements Document Team Z-Telescope Team Members: Yeyue Chen, Akil Bhagat, Josh Hess Customer: Jim Zavislan, Professor of Optics at the University of Rochester
More informationUnderstanding Resolution Diffraction and The Airy Disk, Dawes Limit & Rayleigh Criterion by Ed Zarenski
Understanding Resolution Diffraction and The Airy Disk, Dawes Limit & Rayleigh Criterion by Ed Zarenski ezazaz@juno.com These explanations of terms are based on my understanding and application of published
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 informationFluid Flow Analysis By A Modified, Sharp Focussing, White Light Lau Interferometer
Stickland, M.T. and Waddell, Peter and Mason, S. and McKay, S. and Mair, L. (00) Fluid flow analysis by a modified, white light, Lau interferometer. Experiments in Fluids. ISSN 073-4864, This version is
More informationASD and Speckle Interferometry. Dave Rowe, CTO, PlaneWave Instruments
ASD and Speckle Interferometry Dave Rowe, CTO, PlaneWave Instruments Part 1: Modeling the Astronomical Image Static Dynamic Stochastic Start with Object, add Diffraction and Telescope Aberrations add Atmospheric
More information33. Riemann Summation over Rectangular Regions
. iemann Summation over ectangular egions A rectangular region in the xy-plane can be defined using compound inequalities, where x and y are each bound by constants such that a x a and b y b. Let z = f(x,
More informationWide X-ray Field of View
NAOC Beijing June 25 th 2013 Wide X-ray Field of View Dick Willingale University of Leicester Scientific Motivation Soft X-ray surveys High angular resolution Large sky area Faint sources AGN, Clusters
More information1 Trigonometric Identities
MTH 120 Spring 2008 Essex County College Division of Mathematics Handout Version 6 1 January 29, 2008 1 Trigonometric Identities 1.1 Review of The Circular Functions At this point in your mathematical
More informationWavefront Sensing In Other Disciplines. 15 February 2003 Jerry Nelson, UCSC Wavefront Congress
Wavefront Sensing In Other Disciplines 15 February 2003 Jerry Nelson, UCSC Wavefront Congress QuickTime and a Photo - JPEG decompressor are needed to see this picture. 15feb03 Nelson wavefront sensing
More informationColorado School of Mines. Computer Vision. Professor William Hoff Dept of Electrical Engineering &Computer Science.
Professor William Hoff Dept of Electrical Engineering &Computer Science http://inside.mines.edu/~whoff/ 1 Sensors and Image Formation Imaging sensors and models of image formation Coordinate systems Digital
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 informationHyperbolas Graphs, Equations, and Key Characteristics of Hyperbolas Forms of Hyperbolas p. 583
C H A P T ER Hyperbolas Flashlights concentrate beams of light by bouncing the rays from a light source off a reflector. The cross-section of a reflector can be described as hyperbola with the light source
More informationMEGA MOUTH HEAVY DUTY 3 WHEEL SLICKLINE MEASUREMENT DEVICE WITH COMBINED DEPTH AND TENSION CERTIFIED FOR USE IN A ZONE 2 ENVIRONMENT
MEGA MOUTH HEAVY DUTY 3 WHEEL SLICKLINE MEASUREMENT DEVICE WITH COMBINED DEPTH AND TENSION CERTIFIED FOR USE IN A ZONE 2 ENVIRONMENT AMSLA416 ZONE 2 MEGA MOUTH SPECIFICATION AMSLA416 Rev A Sep 2008 Page
More informationSQIID Supplement. Supplement I: Channel-specific Characteristics. Filter Transmission. Return to SQIID User Manual
SQIID Supplement Return to SQIID User Manual Supplement I: Channel-specific Characteristics Filter Transmission Supplement I: Channel-specific Characteristics 1 of 10 10/22/02 3:26 PM Fig. 1 Warm transmission
More informationJoeri van Leeuwen The dynamic radio sky: Pulsars
Joeri van Leeuwen The dynamic radio sky: Pulsars Joeri van Leeuwen The dynamic radio sky: Pulsars Coenen, van Leeuwen et al. 2015 Joeri van Leeuwen The dynamic radio sky: Pulsars Joeri van Leeuwen The
More informationSPECTROCLICK KIT EXPLORE THE INTERACTION OF LIGHT AND MATTER THE SCIENCE OF SPECTROSCOPY. 101 W. Tomaras Ave. Bldg.
SPECTROCLICK KIT EXPLORE THE INTERACTION OF LIGHT AND MATTER THE SCIENCE OF SPECTROSCOPY 101 W. Tomaras Ave. Bldg. B Savoy, IL 61874 WARNING: NOT INTENDED FOR CHILDREN UNDER THE AGE OF 6 ADULT SUPERVISION
More informationPHOTOGRAPH OF SHADOW BANDS
PHOTOGRAPH OF SHADOW BANDS A. E. DOUGLASS Reprinted for private circulation from Tm: AsTROPHYSICAL JoURNAL, Vol. LXIII, No. 3, April 1926 t PlliNTED IN TBII: U.S.A. PHOTOGRAPH OF SHADOW BANDS BY A. E.
More informationOperating Manual Supplement for Model ST-4000XCM
Operating Manual Supplement for Model ST-4000XCM Santa Barbara Instrument Group 147A Castilian Drive Santa Barbara, CA 93117 USA Phone (805) 571-7244 Fax (805) 571-1147 Web: www.sbig.com E-mail: sbig@sbig.com
More information