Zone 65, Master Map Normal View
|
|
- Marilyn Haynes
- 5 years ago
- Views:
Transcription
1 Zone Master, Normal View, 10 deg FOV, Master Map Normal View ear Paw Galaxy ψ9 ψ ' ' ' ' ' Lynx ψ4 08h 12m 08h 00m 07h 48m 07h 36m uriga 07h 24m 07h 12m 07h 00m ψ5 06h 48m
2 , Map 1 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. h2395 Hussey h 36m STF 1096 STF Lyn 07h 30m 07h 24m 19 Lyn Stein Lyn STF 1050 Espin h 18m STF 1033 Espin h 12m Espin 900 Espin 2622 STF h 06m STF 1001 Espin 1079 NGC h 00m h2350 h2348 uriga STF h 54m Espin 2620 OS 158 rej ' ' ' ' ' '
3 , Map 1 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. Espin 2620 STF 960 STF 968 OS 158 rej h2348 uriga h2350 STF 1001 STF 1009 Espin 1079 NGC 2320 Espin 900 Espin 2622 Espin 1081 STF 1033 STF Lyn Espin Lyn Stein 2187 STF Lyn Hussey 622 STF h 54m 07h 00m 07h 06m 07h 12m 07h 18m 07h 24m 07h 30m 07h 36m h ' ' ' ' ' '
4 , Map 2 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc STF 1092 STF 1096 Kuiper 30 ur 758 STF Lyn 2046 Espin Lyn STF 1032 Hussey 619 STF 1040 STF 1044 Espin 2624 STF 1071 Espin 2623 Espin 1241 Espin 900 Espin 2622 NGC uriga Kustner 91 STF 977 STF 979 ψ9 Lynx ' ' ' ' ' ' 07h 36m 07h 30m 07h 24m 07h 18m 07h 12m 07h 06m 07h 00m h 54m
5 , Map 2 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. uriga Kustner 91 STF STF 979 ψ9 Lynx Espin 900 Espin 2622 STF 1032 NGC STF 1040 STF Lyn Espin 2623 Hussey 619 Espin 1241 Espin 2624 STF 1071 Espin 1242 STF Lyn STF 1092 Kuiper 30 ur STF ' ' ' ' ' ' h 54m 07h 00m 07h 06m 07h 12m 07h 18m 07h 24m 07h 30m 07h 36m
6 , Map 3 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. STF 1172 STF 1165 NGC 2500 NGC G. 146 NGC 2446 h2395 Hussey 622 STF 1096 STF Lyn Stein Lyn ' ' ' ' ' ' 08h 06m Hipparcos h 00m 07h 54m 07h 48m Espin h 42m 07h 36m 22 Lyn 07h 30m 07h 24m
7 19 Lyn Stein 2187 STF Lyn STF 1091 Hussey 622 STF 1096, Map 3 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. h2395 NGC 2446 NGC G. 146 STF 1172 STF 1165 NGC 2500 Espin Lyn Espin 1082 Hipparcos h 24m 07h 30m 07h 36m 07h 42m 07h 48m 07h 54m 08h 00m 08h 06m ' ' ' ' ' '
8 , Map 4 Normal Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. h2428 Espin G. 146 Hipparcos 1136 Hussey 713 Pulkovo 8 STF 1161 Lynx Espin 588 Espin 1082 Espin 2627 STF Kuiper 30 ur 758 STF Lyn STF Lyn Espin ' ' ' ' ' ' 08h 06m 08h 00m 07h 54m 07h 48m 07h 42m 07h 36m 07h 30m 07h 24m
9 , Map 4 Mirror Image Sky charts generated by TheSky Software; used by permission of Software isque Inc. 20 Lyn Espin 2623 Espin 2624 Espin 1242 STF 1071 STF 1091 Kuiper 30 ur Lyn STF 1092 STF Espin 1082 Espin 2627 Espin 588. G. 146 Hipparcos 1136 Hussey 713 h2428 Pulkovo 8 STF 1161 Lynx ' ' ' ' ' ' 07h 24m 07h 30m 07h 36m 07h 42m 07h 48m 07h 54m 08h 00m 08h 06m
10 Index 32 Double Stars, 4 Galaxies Flamsteed 20 Lyn Lyn G E Espin Espin Espin Espin Espin Espin Espin Espin Espin Espin Espin H h Hussey Hussey K Kuiper N NGC NGC NGC NGC S STF STF STF STF STF STF STF STF STF STF STF
11 , Map 1 Double Stars Easy STF 1009 DS 5746; SO Rating: 2 E Position: Magnitude Separation P Year Spectra Colors Vs C C = 1991? 1830: 159. Over 100 measurements. This star is a member of the Hyades group. C 1879: measurements. C8 at 206x. Diameter: = 8.10 inches; = 6.30 inches. Separation: = 2.32 miles. Distance (LY): 347 Total luminosity (Suns):
12 20 Lyn Rating: 2 E STF 1065DS 6004; HD 57067; SO Position: Magnitude Separation P Year Spectra Colors II W F0 1826: measurements. The stars have common proper motion. The primary is a spectroscopic binary. C8 at 83x. STF 1050 DS 5968; HD 56385; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors V W V C = 1908? 1829: measurements. Hipparcos/Tycho data show different distances for these stars; they may be optical. However, the stars exhibit common proper motion. C 1880: measurements. C8 at 83x
13 Diameter: = 9.00 inches; = 6.40 inhes. Separation: = 8.13 miles; C = 83.2 miles. Distance (LY): 270 Total luminosity (Suns): 5.1 STF 1001 DS 5706; HD 52145; SO Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 7.42 F8 IV Y = R C = 1965? 1831: measurements. The stars share common proper motion. C 1867: measurements. C8 at 206x. Webb saw the primary as D. Diameter: = 8.40 inches. Separation: = 4.87 miles; C = 5.25 miles. Distance (LY): 351 Total luminosity (Suns): 14 Espin 1081 DS 5899 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.64 W No C W - 4 -
14 oth 1 measurement. C11 at 115x. was not detected. Moderate Espin 1079 DS 5697; HD 52098; SO Rating: 5 M Position: Magnitude Separation P Year Spectra Colors W W? 1 measurement. C11 at 115x. Diameter: = 7.13 inches. Separation: = 7.25 miles. Distance (LY): 750 Total luminosity (Suns):
15 Difficult STF 1033 DS 5896; HD 55199; SO Rating: 5 D Position: Magnitude Separation P Year Spectra Colors 7.83 F0 Y C W 1829: measurements. C 1783: measurements. Similar proper motions. C8 at 206x. Diameter: = 10.3 inches. Separation: = 2.38 miles; C = 125 miles. Distance (LY): 1,020 Total luminosity (Suns):
16 Deep Sky Objects Difficult NGC 2320 Other Names: H II 861, UGC 3659 Rating: 5 D Position: Type : Gal Class: E Magnitude : 11.9 Surface brightness: 11.9 Dimensions: 1.4' x 0.8' P: 140 This galaxy produced supernova 2000 (type Ia). C8 at 104x. Very faint spot seen with the help of a light pollution filter. 9m star lies just 1 minne. Model (where the Sun is a baseball): Its diameter would be 34 million miles. Distance (LY): 260,000,000 Luminosity (suns): 92,000,000,000 Radial velocity (km/sec): +5,
17 , Map 2 Double Stars Easy Espin 900 DS 5732; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.64 F W W 1910: measurements. The stars share proper motion. C11 at 115x. Espin 2622 HD 54368; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 8.05 G5 Y ! 1902: measurements. May be optical because Hipparcos gives different distances (760 and 3,260 light years). The stars also have different proper motions. C8 at 104x. Moderate field
18 1068 DS 5845; HD 54614; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.02 F5 W po 1905: measurements. C11 at 115x. Diameter: = 13.8 inches. Separation: = 1.51 miles. Distance (LY): 285 Total luminosity (Suns): 1.90 STF 1040 DS 5926; HD 55702; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors W = do 1830: measurements. C8 at 104x. Faint but moderate field
19 Diameter: = 7.75 inches. Separation: = 3,485 feet. Distance (LY): 59 Total luminosity (Suns): 0.1 Espin 2624 HD 57046; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 8.05 K2 po ? 1991 F8 V bw 1895: measurements. Quadrant reversal? May be optical because Hipparcos gives different distances (175 and 680 light years). The stars also have different proper motions. C8 at 104x. It is framed by a 9m equilateral triangle. STF 1044 DS 5932; HD 55725; SO Rating: 4 E Position: Magnitude Separation P Year Spectra Colors V? ? 1828: measurements. C8 at 83x
20 Diameter: = 8.40 inches. Separation: = 7.70 miles. Distance (LY): 392 Total luminosity (Suns): 16 Espin 1241 DS 5976 Rating: 4 E Position: Magnitude Separation P Year Spectra Colors Y = 1980 W 1913: 3. 4 measurements. C11 at 115x. Distance (LY): 30 Total luminosity (Suns): Hussey 619 DS 5975; HD Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.35 F0 W No C = 1991? 1902: measurements. C 1902: measurements. C8 at 104x. Moderately rich field
21 STF 1071 DS 6018; HD 57378; SO Rating: 5 E Position: Magnitude Separation P Year Spectra Colors 9.06 G0 Y ! 1991 W 1829: measurements. Hipparcos/Tycho data show different distances for these stars; they may be optical. The stars have different proper motions. C8 at 104x. Very faint. Diameter: = 18.0 inches. Separation: = 7.87 miles. Distance (LY): 256 Total luminosity (Suns): 1.4 Moderate Espin 2623 Sinachopoulos 28 (a); DS 5965; HD 56416; SO Rating: 4 M Position: Magnitude Separation P Year Spectra Colors W bw a ? a : measurements. a 1 measurement
22 C11 at 339x. C at 115x is nice. ut I needed 339x to get a glimpse of. Diameter: = 7.60 inches. Separation: = 6.19 miles; a = 6.19 miles. Distance (LY): 418 Total luminosity (Suns): 5.95 Espin 1242 DS 6061 Rating: 5 M Position: Magnitude Separation P Year Spectra Colors W = ? 1913: measurements. C11 at 115x. Very uneven! Distance (LY): 1,210 Total luminosity (Suns): 15.6 Difficult 2046 DS 6107; SO Rating: 3 D Position: Magnitude Separation P Year Spectra Colors 7.94 G5 W W 1909: measurements
23 C11 at 634x. Diameter: = 19.3 inches. Separation: = 1.59 miles. Distance (LY): 730 Total luminosity (Suns): 35 STF 1032 DS 5879; HD 55078; SO Rating: 4 D Position: Magnitude Separation P Year Spectra Colors V bw ? C = 1908 L 1831: measurements. C 1880: measurements. Diameter: = 9.00 inches. Separation: = 2.14 miles; C = 105 miles. Distance (LY): 510 Total luminosity (Suns): 23 Kuiper 30 C = ur 758; DS 6095; HD 58661; SO Rating: 4 D Position: Magnitude Separation P Year Spectra Colors p Mn W ? C ?
24 1942: measurements. C 1883: measurements. There is an excess of manganese in the spectrum of the primary. It is also a longperiod spectroscopic binary. C8 at 206x. Diameter: = 4.24 inches. Separation: = 3,696 feet; C = 10.6 miles. Distance (LY): 410 Total luminosity (Suns): 72 Deep Sky Objects Moderate NGC 2344 Other Names: UGC 3734 Rating: 4 M Position: Type : Gal Class: S(rs)c: Magnitude : 12.0 Surface brightness: 13.2 Dimensions: 2.2' x 2.0' C8 at 83x. It displayed a stellar nucleus with a very soft halo. 6.8m star lies just on the edge of the field about 12 min NE. Moderate field. Distance: 43,000,000 light years Radial velocity (km/sec): +974 Luminosity: 2,300,000,000 Suns
25 , Map 3 Double Stars Easy Hussey 622 DS 6198; HD Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.08 G5 Y O 1902: measurements. C11 at 115x! It looks better at 339x, though. Diameter: = 20.7 inches. Separation: = 4,594 feet. Distance (LY): 193 Total luminosity (Suns): 0.89 STF 1096 HD 59308; SO Rating: 4 E Position: Magnitude Separation P Year Spectra Colors W W
26 1901: measurements. Hipparcos/Tycho data show different distances for these stars; they may be optical. Tycho 2 suggests a single star entry. C8 at 104x. This star is the NE end of a line of 8m stars. Diameter: = 6.27 inches. Separation: = 32.6 miles. Distance (LY): 720 Total luminosity (Suns): 32 h2395 HD ; SO Rating: 4 E Position: Magnitude Separation P Year Spectra Colors 9.58 K0 yo W 1908: measurements. C11 at 115x. Diameter: = 26.6 inches. Separation: = 43.8 miles. Distance (LY): 1,550 Total luminosity (Suns):
27 Moderate. G. 146 Rating: 3 M DS 6481 Position: Magnitude Separation P Year Spectra Colors 9.66 G0 W W 1900: measurements. C8 at 280x. It was split at 104x, but 270 made it cleaner. Diameter: = 18.6 inches. Separation: = 3,115 feet. Distance (LY): 120 Total luminosity (Suns): Deep Sky Objects Difficult NGC 2446 Other Names: UGC 4027 Rating: 4 D Position: Type : Gal Class: Sb Magnitude : 12.9 Surface brightness: 13.4 Dimensions: 2.1' x 1.0' P:
28 C8 at 104x. With a light pollution filter, I was able to pick up a somewhat indistinct glow from where the charts say this galaxy is supposed to be. However, I could not make out any significant detail. Radial velocity (km/sec): +5,668 NGC 2475 Other Names: UGC 4114 Rating: 5 D Position: Type : Gal Class: E1 Magnitude : 13.1 Surface brightness: 12.5 Dimensions: 48" C11 at 193x. Very small and faint with a much brighter center. Radial velocity (km/sec): +5,
29 , Map 4 Double Stars Easy STF 1092 DS 6118; HD 58967; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors W W 1831: measurements. C11 at 115x! Diameter: = 9.00 inches. Separation: = 7.49 miles. STF 1091 HD ; SO Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.54 G0 V Y G5 Y 1829: measurements. Hipparcos/Tycho data show different distances for these stars; they may be optical. The stars have different proper motions
30 C8 at 104x. It is overpowerd by a very bright field that resembles a miniature Cassiopeia! Diameter: = 3.45 inches; = 21.7 inches. Separation: = 10.8 miles. Distance (LY): 233 Total luminosity (Suns): 1.2 Espin 1082 DS 6312 Rating: 3 E Position: Magnitude Separation P Year Spectra Colors 9.63 G0 Y = 318 = 1991 W 1911: measurements. C11 at 115x. Diameter: = 18.5 inches. Separation: = 3.60 miles. Distance (LY): 412 Total luminosity (Suns): Lyn Rating: 5 E Engelmann 31; HD 58855; SO Position: Magnitude Separation P Year Spectra Colors 5.35 F5 V yw W
31 C8 at 104x. nice area of 8m-9m stars (5 of them) lies 18 min N. Diameter: = 4.35 inches. Separation: = 17.1 miles. Distance (LY): 65 Total luminosity (Suns): 2.32 Espin 588 DS 6356 Rating: 4 M Position: Magnitude Separation P Year Spectra Colors 9.50 W W 1908: measurements. C11 at 339x. Espin 2627 DS 6316; HD 62068; SO Rating: 5 M Position: Magnitude Separation P Year Spectra Colors 7.50 K0 Y ? 1913: measurements. C8 at 206x. There is a 9m star 8 min W
32 Diameter: = 23.5 inches. Separation: = 6.59 miles. Distance (LY): 395 Total luminosity (Suns): Difficult 2048 DS 6199; SO Rating: 5 D Position: Magnitude Separation P Year Spectra Colors 9.57 F2 W W 1909: 2. 8 measurements. C11 at 634x
33 Mini-Catalog Double Stars Double Position Rating Map Comp Mag Sep P STF E 1 C C = 20 Lyn E Espin E Espin E E STF E 2 STF E 1 Espin E 2 STF E 4 STF E 4 Hussey E 3 Espin E 4 STF E 1 Espin E 1 STF E 2 Hussey E 2 Espin E 2 STF E 3 h E 3 STF E 2 22 Lyn E 4 C C C C = = 8.9 = ? = = !
34 Double Position Rating Map Comp Mag Sep P. G M Espin M 2 a a Espin M Espin M Espin M = Espin M 4 STF D 2 Kuiper D 2 STF D D 4 C C C Deep Sky Objects Object Position Rating Map Type and Class Mag Surf r Population NGC M 2 Gal (S(rs)c:) NGC D 3 Gal (Sb) NGC D 1 Gal (E) NGC D 3 Gal (E1)
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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 informationTransformation from Tri-colour DSLR observations to Johnson system
Transformation from Tri-colour DSLR observations to Johnson system A case story by anthrophosophical astronomer Søren Toft Photometry. The use of colour cameras for photometry is an alternative to the
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 informationLUCI1/2 AO commissioning: status and prospects
LUCI1/2 AO commissioning: status and prospects AO-image NGC 6543 Credit: Dave Thompson Jochen Heidt, Landessternwarte Heidelberg, Germany The (expanded) team Arcetri: S. Esposito G. Agapito E. Pinna A.
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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 informationGENERAL MACHINING PRACTICE FOR CMI ELECTROMAGNETIC IRON
GENERAL MACHINING PRACTICE FOR CMI ELECTROMAGNETIC IRON Electromagnetic Iron can be readily machined when proper tool angles are used. Tools should be ground to more acute cutting edge angles than are
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 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 informationDSLR FOCUS MODES. Single/ One shot Area Continuous/ AI Servo Manual
DSLR FOCUS MODES Single/ One shot Area Continuous/ AI Servo Manual Single Area Focus Mode The Single Area AF, also known as AF-S for Nikon or One shot AF for Canon. A pretty straightforward way to acquire
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 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 informationAtik Infinity; StarlightXpress Ultrastar; and Mallincam StarVision.
ICX825 Based Astro-Video Camera Comparison by Jim Thompson, P.Eng Test Report Oct. 7 th, 2016 Objectives: The choices of camera available for use in video astronomy has grown rapidly over the past couple
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 informationDigitally Removing Uneven Field Illumination
Digitally Removing Uneven Field Illumination A problem that is encountered with many telescopes, and nearly all camera lenses used for longexposure deepsky astrophotography is uneven field illumination.
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 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 informationVBS - The Optical Rendezvous and Docking Sensor for PRISMA
Downloaded from orbit.dtu.dk on: Jul 04, 2018 VBS - The Optical Rendezvous and Docking Sensor for PRISMA Jørgensen, John Leif; Benn, Mathias Published in: Publication date: 2010 Document Version Publisher's
More informationAstronomical Cameras
Astronomical Cameras I. The Pinhole Camera Pinhole Camera (or Camera Obscura) Whenever light passes through a small hole or aperture it creates an image opposite the hole This is an effect wherever apertures
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 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 informationGuide to Processing Spectra Using the BASS Software
British Astronomical Association Supporting amateur astronomers since 1890 Guide to Processing Spectra Using the BASS Software Andrew Wilson 04 June 2017 Applicable to BASS Project Version 1.9.7 by John
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 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 informationThe Color Wheel. The color wheel shows relationships between the colors.
Color Wheel The Color Wheel The color wheel shows relationships between the colors. Artists often use the color wheel to help understand how colors relate to one another. The Color Wheel Let s learn about
More informationBuilding a simple spectroscope
Quick and simple laser communicator. Make your own 3D pictures in minutes. Making permanent rainbows. Building the impossible kaleidoscope. Building a simple spectroscope. Make a solar hotdog cooker. Going
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 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 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 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 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 informationMini-spectrometer from a DVD and folded paper
Mini-spectrometer from a DVD and folded paper Writing up experiences with an open-source transmission grating spectrometer from DVD, paper and camera. A very effective gadget to get hands-on training in
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 informationfocus: Elegance Lightly Expressed Light Bars
Lightly Expressed Light Bars focus: Elegance Imagine being able to direct bright, pure light exactly where you want it and at exactly the right intensity without concern for heat, ultraviolet fading, or
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 informationBenchmark Test : Grade 6 Math. Class/Grade. Benchmark: MA.6.G.4.3. Benchmark: MA.6.G.4.2
Name lassrade ate enchmark: M... enchmark: M... Look at the figure below. The lengths of four of the five sides of the figure are shown. What is the area of this triangle? cm cm cm cm f the perimeter of
More informationA Method of Measuring High Delta m Doubles
Page 159 James A. Daley Ludwig Schupmann Observarory New Ipswich,NH rigel@net1plus.com Abstract: This paper describes a method of precisely measuring theta and rho for pairs in which the difference in
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 informationThe Imaging Chain in Optical Astronomy
The Imaging Chain in Optical Astronomy Review and Overview Imaging Chain includes these elements: 1. energy source 2. object 3. collector 4. detector (or sensor) 5. processor 6. display 7. analysis 8.
More informationThe Imaging Chain in Optical Astronomy
The Imaging Chain in Optical Astronomy 1 Review and Overview Imaging Chain includes these elements: 1. energy source 2. object 3. collector 4. detector (or sensor) 5. processor 6. display 7. analysis 8.
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 informationChapter 7. Optical Measurement and Interferometry
Chapter 7 Optical Measurement and Interferometry 1 Introduction Optical measurement provides a simple, easy, accurate and reliable means for carrying out inspection and measurements in the industry the
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 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 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 informationName Partner(s) Date Grade Category Max Points Points Received Tricolor Imaging 1. Introduction Background and Theory FILTER
29:50 Astronomy Lab #8 Stars, Galaxies, and the Universe Name Partner(s) Date Grade Category Max Points Points Received On Time 5 Printed Copy 5 Lab Work 90 Total 100 Tricolor Imaging 1. Introduction This
More informationUnit 1: Whole Numbers
Unit 1: Whole Numbers 1.1.1 Place Value and Names for Whole Numbers Learning Objective(s) 1 Find the place value of a digit in a whole number. 2 Write a whole number in words and in standard form. 3 Write
More informationCopyright (c) 2004 Cloudy Nights Telescope Reviews.
Untitled Document Copyright (c) 2004 Cloudy Nights Telescope Reviews www.cloudynights.com All rights reserved. No part of this article may be reproduced or transmitted in any form by an means without the
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 informationLecture 41: Interstellar Travel and Colonization
Lecture 41 Interstellar Travel and Colonization Astronomy 141 Winter 2012 This lecture is about the challenges of interstellar travel and colonization. Interstellar travel is extremely challenging due
More informationAdobe Illustrator. Mountain Sunset
Adobe Illustrator Mountain Sunset Adobe Illustrator Mountain Sunset Introduction Today we re going to be doing a very simple yet very appealing mountain sunset tutorial. You can see the finished product
More informationWhat does the universe look like in color?
EXPLORATION 3: ASTRO-PHOTOGRAPHER! What does the universe look like in color? The challenge Y ou have been asked by an astronomy magazine to write a short article about some part of the universe that interests
More informationIntroduction. Laser Diodes. Chapter 12 Laser Communications
Chapter 1 Laser Communications A key technology to enabling small spacecraft missions is a lightweight means of communication. Laser based communications provides many benefits that make it attractive
More informationDiffraction lens in imaging spectrometer
Diffraction lens in imaging spectrometer Blank V.A., Skidanov R.V. Image Processing Systems Institute, Russian Academy of Sciences, Samara State Aerospace University Abstract. А possibility of using a
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 information824BP Series. 8 Bit Programmable 2-Pole Pair Filters. Band Pass
824BP Series Band Pass 8 Bit Programmable 2-Pole Pair Filters Description: The 824BP Series is a 2-pole-pair digitally programmable precision band-pass active filter that provides high performance in a
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 informationMeasuring Double Stars with a Canon DSLR Camera
Page 188 Zsolt Giczi Halászi, Hungary aic7902 (at) gmail.com Abstract: 76 target pairs were measured from August 17, 2017 to January 6, 2018 using an 8-inch Schmidt-Cassegrain telescope and a Canon EOS
More informationWFC3 TV2 Testing: UVIS Filtered Throughput
WFC3 TV2 Testing: UVIS Filtered Throughput Thomas M. Brown Oct 25, 2007 ABSTRACT During the most recent WFC3 thermal vacuum (TV) testing campaign, several tests were executed to measure the UVIS channel
More informationLecture 8. Lecture 8. r 1
Lecture 8 Achromat Design Design starts with desired Next choose your glass materials, i.e. Find P D P D, then get f D P D K K Choose radii (still some freedom left in choice of radii for minimization
More informationLASER. Analog Laser Displacement Transducer. LAS Series. Key-Features:
LASER Analog Laser Displacement Transducer LAS Series Key-Features: Content: Measurement Principle & Installation...2 Overview of the Series...3 Technical Data.4 Technical Drawing...7 Linearity & Resolution...8
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 informationPassive optical link budget for LEO space surveillance
Passive optical link budget for LEO space surveillance Paul Wagner, Thomas Hasenohr, Daniel Hampf, Fabian Sproll, Leif Humbert, Jens Rodmann, Wolfgang Riede German Aerospace Center, Institute of Technical
More informationLM833 Dual Audio Operational Amplifier
LM833 Dual Audio Operational Amplifier General Description The LM833 is a dual general purpose operational amplifier designed with particular emphasis on performance in audio systems. This dual amplifier
More informationUSER S MANUAL. 580 TV Line OSD Bullet Camera With 2 External Illuminators
USER S MANUAL 580 TV Line OSD Bullet Camera With 2 External Illuminators Please read this manual thoroughly before operation and keep it handy for further reference. WARNING & CAUTION CAUTION RISK OF ELECTRIC
More informationCaldwell 109. Patrick Caldwell-Moore. 109 Oggetti
Patrick -Moore 109 Oggetti Pagina 1 1 C 1 NGC 188 OCL 309 OPNCL CEP 00 47.5 +85 14 8,1 99,9 14.0 m II 2 r Cl,vL,R,150-200 st 10...18 13 C 2 NGC 40 PK 120+9.1 PLNNB CEP 00 13.0 +72 31 10,7 7,3 60 s 40 s
More information