View allAll Photos Tagged gso
Imaging telescope or lens:GSO 8" f/5 Newton
Imaging camera:ZWO ASI 183 MM PRO
Mount:SkyWatcher NEQ6 Pro Goto
Guiding telescope or lens:GSO 8" f/5 Newton
Guiding camera:Astrolumina Alccd5L-IIc
Focal reducer:Pal Gyulai GPU Aplanatic Koma Korrector 4-element
Software:Main Sequence Software Seqence Generator Pro, Adobe PhotoShop CS5, FitsWork 4, DeepSky Stacker Deep Sky Stacker 3.3.4, PHD2 Guiding
Filters:Baader Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm, Baader Planetarium O3 1.25" 8.5nm
Accessory:TSOptics TS Off Axis Guider - 9mm
Dates:Sept. 11, 2018, Sept. 19, 2018, Sept. 20, 2018
Frames:
Baader Ha 1.25" 7nm: 32x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium O3 1.25" 8.5nm: 32x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 35x600" (gain: 200.00) -20C bin 1x1
Integration: 16.5 hours
Darks: 35
Flats: 27
Scope: GSO RC6 with WO 0.8x flattener
Camera: ASI1600MM pro
Guider Camera: ASI290MM
Guider: Orion thin Off-axis guider
Mount: Orion Sirius EQMOD driven
Software: APT, DSS64, PS
Integration:
~4HRS Ha in 6min exposures,
~4HRS Oiii in 6min exposures,
~2HRS RGB
Zenit Observatory
Luogo: Manciano (Grosseto)
Telescopio: RC GSO Truss 10"
Riduttore di Focale: Riccardi 0,75X - M63
Focale: 1500 mm
Montatura: 10Micron Gm1000HPS
CCD: Moravian G2 8300
Filtri: LRGB Astrodon Gen2 36mm
Pose:
L 80 X 350" bin 2
R 26 X 350" bin 2
G 30 X 350" bin 2
B 29 X 350" bin 2
Temperatura sensore -20°
Integrazione LRGB: 16 ore
YY17 GSO is an AD E20D/AD Enviro200 new to Borders Buses in March 2017 as their 11714. It joined the sister fleet Glasgow Citybus and is seen here in George Square in Glasgow showing off its new livery.
Equipment:
GSO RC8 + CCDT67 Reducer
1100mm f5,5
Moravian CCD G2-8300FW10
Astrodon LRGB Filter
Losmandy G11 LFE Photo
Guiding:
Starlight Lodestar an Celestron OAG + PHD
Date: Dezember 2014
Zenit Observatory
Luogo: Manciano (Grosseto)
Telescopio: RC GSO Truss 10"
Riduttore di Focale: Riccardi 0,75X - M63
Focale: 1500 mm
Montatura: 10Micron Gm1000HPS
CCD: Moravian G2 8300
Filtri: LRGB Astrodon Gen2 36mm
Pose:
L 52 X 900" bin 1
R 7 X 350" bin 2
G 7 X 350" bin 2
B 7 X 350" bin 2
Temperatura sensore -20°
Integrazione LRGB: 14,8 ore
YY17 GSO is an AD E20D/AD Enviro200 new to Borders Buses in March 2017 as their 11714.
It joined the sister fleet Glasgow Citybus and is seen here on North Hanover Street in bewteen journeys on service 15 (Milngavie-George Square).
26x60s. GSO 8"-Newton, HEQ5, Canon EOS 1000Da. The nebula stood 15° above the horizon in the south. So I could'nt take longer exposures because of the light pollution and the difficult seeing conditions.
GSO 200/1000, HEQ5, QHY5-IIc, 2,25x-Barlow. Usually I don't take any photos of the moon surface, but I've seen amazing pictures of Plato today, so I had to try it on my own.
Imagem capturada durante o décimo segundo ENCONTRO BRASILEIRO DE ASTROFOTOGRAFIA na zona rural de Padre Bernardo - GO - Brasil.
Câmera Canon 5D - Mark II - modificada para astrofotografia.
Telescópio GSO RC 8" com Coma Corrector Komakorr F4
61 frames de 300s em ISO 1600
Exposição total de 5 horas - darks, flats e bias aplicados.
Stagecoach 37181 (YY64 GSO) in Chesterfield, 23rd March 2022. YY64 GSO is an Alexander Dennis E20D chassis fitted with an Alexander Dennis Enviro 200 B37F body delivered new to Stagecoach in October 2014.
astro.carballada.com/libration-and-near-side-of-the-moon/
As is mention on the wikipedia:
Since the Moon’s orbit is both somewhat elliptical and inclined to its equatorial plane, libration allows up to 59% of the Moon’s surface to be viewed from Earth (though only half at any moment from any point).
The central crater at the picture is Pitiscus, it's about 82 km of diameter.
Anyway, it’s an another exercise performing more tests on the new remote planetary config.
This picture was taken using a QHYCCD QHY5III174 with a Baader Q Barlow on a camera DIY switch.
It was taken at 3800mm f/19 with a GSO 8″ f/12 Classical Cassegrain Reflector using an Astronomik ProPlanet 642 BP IR-pass filter.
With this config I am covering a field of 10.2 x 6.37 arcmin at 0.319 arcsec/pixel.
It was a video of 10k frames at 80fps using only the best 1% of them.
This DIY switch allows me to change between two cameras, currently this QHYCCD and other ASI183MM-C for bigger field of view.
Telescopio GSO 200mm F4
ZWO 585 MC Pro + Corrector de Coma
Filtros:
UV/IR Cut Astronomik L2
Montura Skywatcher NEq6
Lights: (RGB) 415 de 1' Gain 101 0°C
100 Darks
ZWO 662 mc + SvBony Guider F4
ASIAir Plus
ZWO EAF
Potrero de los Funes, San Luis, Argentina
Polución Lumínica: Bortle 5
Equipment:
GSO RC8 + CCDT67 Reducer
1100mm f5,5
Moravian CCD G2-8300FW10
Astrodon LRGB Filter
Losmandy G11 LFE Photo
Guiding:
Starlight Lodestar an Celestron OAG + PHD
Date: April 2013
M51 2014-05-25 Crop_2
120min. (12x600sec. ISO800), 40 Flats, 40 Flatdarks, 40 Biasframes
GSO 200/1000 Newton (selfmade tuning)
Skywatcher NEQ6 Synscan (VTSB mod)
Canon EOS 60D (mod)
GPU Coma Corrector
Autoguiding per Lacerta Off Axis Guider, Alccd5L-IIc, PHD2 Guiding
Dithering per BackyardEOS
After some videos of Mars I realized the clouds would possibly totally disappear. So I decided to record for 1 hour (stupid short summer nights - just 1 dark hour...). I chose an object with a high magnitude. Sadly the interesting things were occupied behind trees or the balcony over me.
Canon EOS 1000Da, GSO 200/1000, HEQ5. 30x120s ISO 1600.
Il Quintetto di Stephan è un gruppo di 5 galassie nella costellazione di Pegaso, con magnitudine apparente tra 12.6 e 13.9; venne scoperto nel 1877 dall'astronomo francese Édouard Stephan all'osservatorio di Marsiglia.
Dall'immagine è evidente l'interazione tra le 5 galassie: in realtà dall'analisi dei redshifts è emerso che la galassia azzurra sulla destra - catalogata come NGC 7320 - si troverebbe ad una distanza di 32 milioni di anni luce, mentre le altre quattro galassie si troverebbero ad una distanza compresa tra i 280 e 340 milioni di anni luce.
NGC 7320 apparirebbe quindi all'interno del Quintetto solo per un effetto di prospettiva.
Su tutta l'immagine è visibile una debole nebulosità biancastra di poco più luminosa del fondo cielo: si tratta della IFN (Integrated Flux Nebula), appartenente alla nostra Galassia.
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Stephan's Quintet is a group of five galaxies in the constellation Pegasus, with apparent magnitudes between 12.6 and 13.9; it was discovered in 1877 by the French astronomer Édouard Stephan at the Marseille Observatory (France). The Stephan Quintet galaxies are not really connected to each other: according to redshift values measured, the blue galaxy on the right - named NGC 7320 - could be 32 million light-years away from us, while the other four are at distances between 280 and 340 million light-years. NGC 7320 would therefore appear inside the Quintet only as a matter of perspective.
On all the image it is visible a faint nebulosity, slightly brighter that the sky background: it is the IFN (Integrated Flux Nebula), belonging to our galaxy.
Technical data
GSO RC12 Truss - Aperture 304mm, focal lenght 2432mm, f/8
Mount 10Micron GM2000 HPSII
Camera ZWO ASI 2600 MM Pro with filter wheel 7 positions
Filters Astrodon Gen2 E-Serie Tru-Balance 50mm unmounted LRGB
Guiding system ZWO OAG-L with guide camera ASI 174MM
Exposure details:
L 54x300", R 18x300", G 18x300", B 18x300" all in bin3 -15C
Total integration time: 9h
Acquisition: Voyager, PHD2
Processing: Pixinsight 1.8, Photoshop CS5, StarXTerminator, NoiseXTerminator, BlurXTerminator
SQM-L: 21.1
Location: Promiod (Aosta Valley, Italy), own remote observatory
Date 10/11 September 2023
I tried GSO RC10f8 again after addition of TS Extension for The Baffle Tube. Stray lights disappeared. I could have finished refinement of the OTA twelve years after purchase. I hope to image nebulae and comets with this one.
TS Optics Extension for the Baffle Tube of 10" RC Telescopes:
www.teleskop-express.de/shop/product_info.php/language/en...
Here is a view of the OTA with TS extension:
www.flickr.com/photos/hiroc/52504139488
Here is a frame of the object taken with the OTA with no extension:
www.flickr.com/photos/hiroc/52490891703
equipment: Guan Sheng Optical Ritchey–Chrétien telescope RC 10" f8 with aigrette pattern mask on the vanes, TS 2.5" field flattener and Canon EOS R-SP4II, modified by Seo-san on Vixen AXD Equatorial Mount, auto guided at a star with Fujinon 1:2.8/75mm C-Mount Lens, Pentax x2 Extender, ZWO ASI 120MM-mini, GPUSB, and PHD2 Guiding
exposure: 15 times x 120 seconds, 18 x 30 sec, 20 x 8 sec, 20 x 4 sec, and 20 x 2 seconds at ISO 1,600 and f/8.0
site: in my backyard at the bottom of almost the center of the world worst light pollution dome over Tokyo
Recorded at a height of 13° over the horizon. So I had to take short exposures to reduce atmospheric influences. 87% moon.
GSO 200/1000 Newton, HEQ5, Canon EOS 1000Da. 70x60s.
M51 2014-05-25 Crop_1
120min. (12x600sec. ISO800), 40 Flats, 40 Flatdarks, 40 Biasframes
GSO 200/1000 Newton (selfmade tuning)
Skywatcher NEQ6 Synscan (VTSB mod)
Canon EOS 60D (mod)
GPU Coma Corrector
Autoguiding per Lacerta Off Axis Guider, Alccd5L-IIc, PHD2 Guiding
Dithering per BackyardEOS
Camera: SBIG ST-10XME sensor -20°C with Sbig CFW10 and SXV-AO-LF
Optics: GSO 10" f/8 RC carbon fiber
Filters: Baader 31,8mm
Exposure time (seconds):
L: 21×300 bin 1×1
R: 6×300 bin 1×1
G: 6×300 bin 1×1
B: 6×300 bin 1×1
Guiding camera: Starlight Xpress Lodestar
Place: Pesaro Italy
Date: 17_18/07/2015
Imaging telescope or lens:GSO 8" f/5 Newton
Imaging camera:ZWO ASI 183 MM PRO
Mount:SkyWatcher NEQ6 Pro Goto
Guiding telescope or lens:GSO 8" f/5 Newton
Guiding camera:Astrolumina Alccd5L-IIc
Focal reducer:Pal Gyulai GPU Aplanatic Koma Korrector 4-element
Software:Adobe PhotoShop CS5, FitsWork 4, CCDCiel, DeepSky Stacker Deep Sky Stacker 3.3.4, PHD2 Guiding
Filters:Baader Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm, Baader Planetarium O3 1.25" 8.5nm
Accessory:TSOptics TS Off Axis Guider - 9mm
Dates:July 18, 2018, July 19, 2018, July 24, 2018
Frames:
Baader Ha 1.25" 7nm: 23x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium O3 1.25" 8.5nm: 25x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 25x600" (gain: 200.00) -20C bin 1x1
Integration: 12.2 hours
Darks: 29
Flats: 29
Object description (wikipedia.org):
The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth. The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star (HD 206267) that is just to the west of IC 1396A. (In the Figure above, the massive star is just to the left of the edge of the image.) The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.
The Elephant's Trunk nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.
The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk nebula. This pressure has triggered the current generation of protostars.
NGC 4565 è una galassia a spirale visibile nella costellazione della Chioma di Berenice.
E' chiamata anche "Galassia Ago" per via della sua forma caratteristica: si mostra infatti di profilo e questo mette in risalto il rigonfiamento in prossimità della zona centrale e la banda scura di polveri che la attraversa.
La sua distanza è stimata tra i 40 e i 60 milioni di anni luce e la sua estensione reale è di 162000 anni luce: è quindi più grande della nostra Via Lattea (che ha una estensione di 100000 anni luce) ma si pensa che la VIa Lattea vista "dall'esterno" si mostri proprio come NGC 4565.
Guardando attentamente l'immagine, si può notare che i due bordi estremi della galassia sono leggermente incurvati in due direzioni opposte: si pensa che questo sia l'effetto dell'interazione con la galassia IC 3571 che è quel piccolo batuffolo blu appena a sinistra di NGC 4565.
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NGC 4565 is a spiral galaxy visible in the Coma Berenices constellation.
Due to its edge-on view and the presence of a very evident dust lane near the core region, it is also known with the nickname “Needle Galaxy”.
Its estimated distance is in the range 40/60 million light years and the real dimension is around 162000 light years.
Looking at carefully the disc, it could be noted some warp on the opposite edges: this could be the effect of the interaction with the small satellite galaxy IC 3571 visible on the left side of NGC 4565.
Technical data
GSO RC12 Truss - Aperture 304mm, focal lenght 2432mm, f/8
Mount 10Micron GM2000 HPSII
Camera ZWO ASI 2600 MM Pro with filter wheel 7 positions
Filters Astrodon Gen2 E-Serie Tru-Balance 50mm unmounted LRGB
Guiding system ZWO OAG-L with guide camera ASI 174MM
Exposure details:
L 45x300", RGB 15x300" for each channel, all in bin3 -15C gain 100
Total integration time: 7h30'
Acquisition: Voyager, PHD2
Processing: Pixinsight 1.8, Photoshop CS5, StarXTerminator, NoiseXTerminator, BlurXTerminator
SQM-L: 21.20
Location: Promiod (Aosta Valley, Italy), own remote observatory
Date 15/18 February, 12 April 2024
Scope: GSO RC6 with WO 0.8x flattener
Camera: ASI1600MM pro
Guider Camera: ASI290MM
Guider: Orion thin Off-axis guider
Mount: Orion Sirius EQMOD driven
Software: APT, DSS 5.1.3, PS
Integration:
4HRS Ha in 6min exposures,
~2HRS ea L, R, G, B
Ha is combined with the R channel
Jupiter , QHYCCD QHY5III462 , GSO(Kasai) GS-150CC + Tele Vue 2.5x PowerMate , Sky-Watcher AZ-GTi
ガニメデとイオをDe-Rotation前の画像にして合成してみました。
スッキリした感じになりますね。
Messier 81
GSO 10" RC telescope and AP 0.67 reducer
QSI 583wsg CCD camera,
Astrodon LRGB and hydrogen-alpha filters,
Paramount ME equatorial mount
Starlight Xpress Lodestar guider
Lum: 29 x 10m
Red: 20 x 10
Green: 21 x 10m
Blue: 38 x 10m
H-alpha: 25 x 10m
22 hours total exposure
Processed in Maxim DL, Photoshop CC and PixInsight.
Images taken from Boxted, Essex, UK.
Supernova 2022hrs was discovered by amateur astronomer Koichi Itagaki on April 16, 2022. It can been seen as the very bright star in the small spiral galaxy NGC4647 next to the larger eliptical galaxy M60. I find it fascinating that the star exploded about 63 million years ago, and we will get to see it's light on earth only for the next few weeks. The explosion is so bright and powerful that it outshines the core of the galaxy it is within.
Equipment Details:
•6 Inch GSO Ritchey-Chretien (RC) F9 1370mm Focal length
•Skywatcher NEQ6 Mount
•ZWO ASI1600mm Cmos Camera cooled to -10'c
•ZWO EFW7 Filter Wheel
•Baader 36mm unmounted L, R, G, B
•Orion ST80 80mm Guide Scope
•ZWO ASI120mm mini Guide Camera
•ZWO ASIAIR Pro for full automation
Exposure Details: (HOO Combination
•Lum 30X180 seconds - Bin 1x1
•Red 10X180 seconds - Bin 1x1
•Green 10X180 seconds - Bin 1x1
•Blue 10X180 seconds - Bin 1x1
Total Integration Time: 3 hours
The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common name comes from a drawing that somewhat resembled a crab with arms produced by William Parsons, 3rd Earl of Rosse, in 1842 or 1843 using a 36-inch (91 cm) telescope. The nebula was discovered by English astronomer John Bevis in 1731. It corresponds with a bright supernova observed in 1054 C.E. by Native American, Japanese, and Arabic stargazers; this supernova was also recorded by Chinese astronomers as a guest star. The nebula was the first astronomical object identified that corresponds with a historically-observed supernova explosion.
At an apparent magnitude of 8.4, comparable to that of Saturn's moon Titan, it is not visible to the naked eye but can be made out using binoculars under favourable conditions. The nebula lies in the Perseus Arm of the Milky Way galaxy, at a distance of about 2.0 kiloparsecs (6,500 ly) from Earth. It has a diameter of 3.4 parsecs (11 ly), corresponding to an apparent diameter of some 7 arcminutes, and is expanding at a rate of about 1,500 kilometres per second (930 mi/s), or 0.5% of the speed of light.
The Crab Pulsar, a neutron star 28–30 kilometres (17–19 mi) across with a spin rate of 30.2 times per second, lies at the center of the Crab Nebula. The star emits pulses of radiation from gamma rays to radio waves. At X-ray and gamma ray energies above 30 keV, the Crab Nebula is generally the brightest persistent gamma-ray source in the sky, with measured flux extending to above 10 TeV. The nebula's radiation allows detailed study of celestial bodies that occult it. In the 1950s and 1960s, the Sun's corona was mapped from observations of the Crab Nebula's radio waves passing through it, and in 2003, the thickness of the atmosphere of Saturn's moon Titan was measured as it blocked out X-rays from the nebula. [text from wikipedia]
Long: 07 41 40 E Lat: 45 28 18 N
Camera: ASI 6200 MMPro
Telescope: GSO 10” Truss
Mount: Astro Physics 1100GTO
Filters: Antlia Halpha 3nm Antlia OIII 3 nm, Astrodon Gen2 LRGB
Ha: 24x720sec, OIII 26x720sec
RGB: 13x420 sec each
Pixinsight, Photoshop
Scope: GSO RC6 with WO 0.8x flattener
Camera: ASI1600MM pro
Guider Camera: ASI290MM
Guider: Orion thin Off-axis guider
Mount: Orion Sirius EQMOD driven
Software: APT, DSS64, PS
Integration:
~4HRS Ha in 6min exposures,
~4HRS Oiii in 6min exposures
EQUIPMENT
GSO Newtonian 150/610 mm HPS Newtonian
ZWO Optical ASI533MC Pro (CMOS)
Equatorial Losmandy GM8
Optolong Light pollution L-Pro Filter 2.00" 90%
Coma corrector Explore Scientific 2.00"
Lights41 x 300 sec
Darks4 x 300 sec
Flats50 x 0.4 sec
Dark Flats50 x 0.4 sec
Total lights integration time 3:25 hours
NGC7331
GSO RC8"
N-EQ6 belt mod
QHY 183M cooled CCD -20° (di Alessandro Pensato)
Baader L_170x420 bin 1x1
Baader R_15x300 bin 2x2
Baader G_ 11x300 bin 2x2
Baader B_12x300 bin 2x2
Total esposition 23 hours
Softwar:
Acquisition: APT - Astro Photography Tool
Processing: Pixinsight 1.8.7
M86 (top center) and other galaxies of the Virgo Cluster of galaxies
Optic: RC GSO 8" - Astro Physics telecompressor 0.67X
Mount: Ioptron CEM60 HP
Autoguider: ZWO ASI290MM mini, Phd guiding
Camera: QSI 583wsg Filters: 31mm unmounted Astrodon gen. 2
Frames: L 16X600sec Bin1 - RGB 5X600sec each Bin2 -30°
Processing: Pixinsight, Photoshop
APT automation
Mars will reach opposition on Oct. 13, 2020, when the Red Planet will be only 39 million miles (62.7 million km) from Earth, the closest pairing until 2035.
As a result, Mars looks much brighter and bigger than usual.
Classic Cassegrain 8" at 3800mm.
4x video files at 200fps
best 200 of 30.000x4
Imaging telescopes or lenses: GSO 8" f12 Classical Cassegrain
Imaging cameras: QHYCCD QHY5III174
Mounts: Mesu 200 Mk2
Focal reducers: Baader Q-Barlow
Software: FireCapture · Emil Kraaikamp Autostackert! 3 · Pleiades Astrophoto PixInsight
Filters: Astronomik Proplanet 642 - 842 nm & Baader r + g + b
Accessory: ZWO EFW · MoonLite CSL 2.5" Focuser with High Res Stepper Motor
Waxing Gibbous Moon
Taken on the 9th March 2014
64% illuminated
9 days old
403,261.07 km away
Best viewed at (1600 x 1513) or (2048 x 1936)
The original is enormous and is 102MB in size.
46 Panel Mosaic
Telescope: AA GSO RC 8"
Camera: ZWO ASI120MM
AVI: 3300 Frames per panel
Stacking: 30% in AVISTACK 2
Final Assembly: Microsoft ICE
Camera: SBIG ST-10XME sensor -20°C with Sbig CFW10 and SXV-AO-LF
Optics: GSO 10" f/8 RC carbon fiber
Filters: Baader 31,8mm
Exposure time (seconds):
L: 30×900 bin 1×1
R: 1×900 bin 1×1
G: 1×900 bin 1×1
B: 1×900 bin 1×1
Guiding camera: Starlight Xpress Lodestar
Place: Pesaro Italy
Date: 27_28/03/2017
Menzione d'onore nel concorso fotografico Astronomy in Movie 2018 - Telescope Service Italia
Leo-Triplett
Equipment:
GSO RC8 + CCDT67 Reducer
1100mm f5,5
Moravian CCD G2-8300FW10
Astrodon LRGB Filter
Losmandy G11 LFE Photo
Guiding:
Starlight Lodestar an Celestron OAG + PHD
Date:
7. April 2013
Equipment:
GSO RC8
1800mm f8
Moravian CCD G2-8300FW10
Astrodon LRGB Filter
Losmandy G11 LFE Photo
Guiding:
Starlight Lodestar an Celestron OAG + PHD
Date: März 2012
West Coast Motors Alexander Dennis Enviro200 11714 (YY17 GSO) is seen here in Glasgow city centre about to commence a journey to Milngavie on service 15.
It was new to the Borders Buses fleet and both fleets are under Craig of Campbeltown ownership.
Moon , Sony Alpha 7m3 , GSO(Kasai) GS-150CC + ED屈折用0.8xレデューサーII + Astronomik ProPlanet 642 BP IR , Sky-Watcher EQ6-R
やっとIRパスフィルターが見つかりました。
別のフィルターのケースに入れていたため分からなくなっていました、、、整理整頓、大切ですね。
この日のお月様は十三夜。
ひと月前の満月を私は見ていないのですが、こういうのを「片月見」と言うそうです。
これって曇ったり雨だったりするとどうなるんやろ、、、