View allAll Photos Tagged 67X
NS 67X with a newer KCS Tier IV GEVO on the point is slowing coming up to MP 278 while snow gusts across the rails in front of it. After a mild last weekend a big late winter storm has moved through mid week dumping snow through the day. Clay Center, OH 2/26/2020
Broadstone based VT26 ready to operate 25th Bogey duty as the 07.50 67X to Waterloo road. 27th February 2009. #dublinbus #vt26
RGB : 40x2min x3 ; Ha 110x5min ; Oiii 101x5min
Ritchey chrétien 250/2000 GSO avec réducteur 0.67x
Camera mono Starlight HSX694
Eq 6 R Pro
NS 67X had the Penn Central leading a few days ago. Really starting to look prototypical Penn Central with all the paint loss.
Sweet evening light shines on empty oil train 67X as it heads west under the NYC signal bridge at MP 195 on the NS Chicago Line.
A ahot with perfect symmetry. Broadstone's VT40 is seen at UCD Belfield having completed a 66X, with VT41 seen beside it having completed a 67X. Both routes start from Maynooth although route 67X has a longer routing through Celbridge, while route 66X has a more direct route through Lexlip.
A rare SD70M is on the point of westbound 67X as it ducks under the now removed 257 intermediates on the Pittsburgh Line's west slope.
Celestron Schmidt Cassegrain 5"
Canon 60D Modificada y Refrigerada
Reductor Focal Celestron 0.67x
Guiado: QHY5-II Mono + Guidescope 50mm
Raspberry Pi3+ + Astroberry
Celestron AVX
Lights: 40x180s
Darks | Flats | Bias: 20
Iso: 2000
F: 10
PHD2 + Kstars Ekos
Pixinsight 1.8
Guillermo Cervantes Mosqueda
Observatorio Astronómico Altaïr
Poncitlán Jalisco México
The Pelican Nebula (also known as IC 5070 and IC 5067) is an H II region associated with the North America Nebula in the constellation Cygnus. The gaseous contortions of this emission nebula bear a resemblance to a pelican, giving rise to its name. The Pelican Nebula is located nearby first magnitude star Deneb, and is divided from its more prominent neighbour, the North America Nebula, by a molecular cloud filled with dark dust.
The Pelican is much studied because it has a particularly active mix of star formation and evolving gas clouds. The light from young energetic stars is slowly transforming cold gas to hot and causing an ionization front gradually to advance outward. Particularly dense filaments of cold gas are seen to still remain, and among these are found two jets emitted from the Herbig–Haro object 555. Millions of years from now this nebula might no longer be known as the Pelican, as the balance and placement of stars and gas will leave something that appears completely different.
Acquired on June 2018
H-alpha - 210 x 120 sec
OIII - 105 x 120 sec
SII - 104 x 120 sec
Total integration time -13:58 hours
Imaging telescope and camera:
TS Optics Ritchey-Chrétien 203/1080-1624 mm with 0.67x AP reducer.
ASI1600MM-Cool
Processed with: Pixinsight and Photoshop CC
Location:
Home Backyard, Geleen, Limburg, Netherlands (Bortle 6/7)
Camera: Moravian G2 8300
Filters: 31mm unmounted Tecnosky
Optic: RC GSO 8" - Astro Physics telecompressor 0.67X
Mount: Takahashi EM200 Temma 2M
Autoguider: Magzero QHY 5L II, OAG 9mm TS, Phd guiding
Frames: H-Alpha 7nm: 17X600 sec Bin1 - RGB: 8X600sec each Bin2
Processing: Pixinsight, Photoshop
Part of the Rho Ophiuchus Molecular Cloud Complex
Taken with ASKAR PHQ80 and 0.67X reducer and ASI2600MC camera. 52 x 5 minutes exposures in total.
Technical card
Imaging telescope or lens: GSO RC8 Carbon Fiber
Imaging camera: ZWO ASI1600MM-Cool
Mount: Skywatcher AZ EQ-6 GT
Guiding telescope or lens: Celestron OAG Deluxe
Guiding camera: QHYCCD QHY5III174
Focal reducer: Astro-Physics CCDT67 - 0.67x Reducer
Software: Main Sequence Software Seqence Generator Pro, Pleiades Astrophoto PixInsight
Filters: Baader Planetarium OIII 1.25" 8.5nm, Baader Planetarium Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm
Accessory: ZWO EFW
Resolution: 4158x3197
Dates: July 6, 2017, July 30, 2017, Sept. 23, 2017
Frames:
Baader Planetarium Ha 1.25" 7nm: 14x180" (gain: 200.00) -20C bin 1x1
Baader Planetarium Ha 1.25" 7nm: 14x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium OIII 1.25" 8.5nm: 20x120" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 19x120" (gain: 200.00) -20C bin 1x1
Integration: 3.2 hours
Avg. Moon age: 7.15 days
Avg. Moon phase: 47.68%
Astrometry.net job: 1755318
RA center: 323.882 degrees
DEC center: 57.485 degrees
Pixel scale: 0.735 arcsec/pixel
Orientation: 272.399 degrees
Field radius: 0.535 degrees
Locations: Berga Resort, Berga, Barcelona, Spain
Nebulosa Trífida (Messier 20) en LRGB + H-Alpha
GSO Ritchey Chrétien 8 " + 0.75x + ASI294MM
TS Optics Ritchey Chrétien + 0.67x + ASI1600MM
L=48x240"
RGB=15x240" per canal
H-Alpha=10x400"
Total 7 hores d'exposició integrades
Nit del 5 de Juliol del 2022
Messier 82 (also known as NGC 3034, Cigar Galaxy or M82) is a starburst galaxy approximately 12 million light-years away in the constellation Ursa Major. A member of the M81 Group, it is about five times more luminous than the whole Milky Way and has a center one hundred times more luminous than our galaxy's center. The starburst activity is thought to have been triggered by interaction with neighboring galaxy M81. As the closest starburst galaxy to Earth, M82 is the prototypical example of this galaxy type.
Acquisition: April 2019
Light pollution - 125 x 120 sec
UV/IR Cut - 352 x 60 sec
H-alpha - 186 x 180 sec
Red - 99 x 120 sec
Green - 98 x 120 sec
Blue - 98 x 120 sec
Total integration time: 29:10 hours
Imaging telescope and camera:
TS Optics Ritchey-Chrétien 203/1080-1624 mm with 0.67x AP reducer.
ASI1600MM-Cool
Processed with: Pixinsight and Photoshop CC
Location:
Home Backyard, Geleen, Limburg, Netherlands (Bortle 6/7)
Taken with RC8 plus 0.67x reducer using ASI2600MC camera Image consists of 10 x 5 minutes exposures.
NGC 5907 (also known as Knife Edge Galaxy or Splinter Galaxy) is a spiral galaxy located approximately 50 million light years from Earth. It has an anomalously low metallicity and few detectable giant stars, being apparently composed almost entirely of dwarf stars. It is a member of the NGC 5866 Group.
NGC 5907 has long been considered a prototypical example of a warped spiral in relative isolation. In 2006, an international team of astronomers announced the presence of an extended tidal stream surrounding the galaxy that challenges this picture and suggests the gravitational perturbations induced by the stream progenitor may be the cause for the warp.
The galaxy was discovered in 1788 by William Herschel.
Acquired on March 2020
IR cut-off - 194 x 90 sec
Light pollution - 10 x 180 sec
Red - 31 x 180 sec
Green - 32 x 180 sec
Blue - 30 x 180 sec
Total integration time: 10:00 hours
Imaging telescope and camera:
TS Optics Ritchey-Chrétien 203/1080-1624 mm with 0.67x AP reducer.
ASI1600MM-Cool
Processed with: Pixinsight and Photoshop CC
Location:
Home Backyard, Geleen, Limburg, Netherlands (Bortle 6/7)
Technical card
Imaging telescope or lens: GSO RC8 Carbon Fiber
Imaging camera: ZWO ASI1600MM-Cool
Mount: Skywatcher AZ EQ-6 GT
Guiding telescope or lens: Celestron OAG Deluxe
Guiding camera: QHYCCD QHY5III174
Focal reducer: Astro-Physics CCDT67 - 0.67x Reducer
Software: Main Sequence Software Seqence Generator Pro, Pleiades Astrophoto PixInsight
Filters: Baader Planetarium OIII 1.25" 8.5nm, Baader Planetarium Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm, ZWO green, ZWO blue
Accessories: ZWO EFW, Baader Planetarium Steeltrack 2"
Resolution: 4352x3140
Dates: Sept. 20, 2017
Frames:
Baader Planetarium Ha 1.25" 7nm: 60x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium OIII 1.25" 8.5nm: 13x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 13x300" (gain: 200.00) -20C bin 1x1
ZWO green: 20x60" (gain: 200.00) -20C bin 1x1
ZWO red: 10x60" (gain: 200.00) -20C bin 1x1
Integration: 7.7 hours
Avg. Moon age: 29.31 days
Avg. Moon phase: 0.06%
Astrometry.net job: 1751696
RA center: 344.191 degrees
DEC center: 62.615 degrees
Pixel scale: 0.688 arcsec/pixel
Orientation: 84.523 degrees
Field radius: 0.512 degrees
Locations: Berga Resort, Berga, Barcelona, Spain
Astrodon Ha 5nm: 12x900"
Astrodon OIII 3nm: 10x900"
Astrodon SII 5nm: 8x900"
Integration: 7.5 hours
Imaging telescopes or lenses: TS APO80
Imaging cameras: QSI 660wsg-8
Mounts: Orion HDX110 EQ-G
Focal reducers: Astro-Physics CCDT67 - 0.67x Reducer
Locality: Bisbee, Cochise, Arizona
Size: 109x 67x 48
Part of the Gem and Mineral Hall Collection of the Natural History Museum of Los Angeles
NHMLA-56502
M27 Cropped version 20/06/2014 17 x 600 secs subs Bias, Flats and Cosmetic Correction was used with a master dark. First time using the Astro Physics CCDT67 0.67x Reducer as you can tell it still needs fine tuning to get the right spacing.
Camera: QHY8L CCD cooled to -20C
Guiding: Maxim DL ,9x50 Finder Scope,QHY5 Mono with IR filter ( Finder Guider )
Optics: Altair Astro 8" RC Astrograph fitted with a Astro Physics CCDT67 0.67x Reducer.
Filter: Astronomik CLS Filter
Mount: Skywatcher AZ EQ6-GT EQ & Alt-Az Mount connected to the Sky X and Eqmod via HitecAstro EQDIR adapter
Image Acquisition: Maxim DL 6 Pro
Stacking and Calibrating: Pixinsight 1.8
拍攝難易度：★★★★
處理難易度：★★★★
IC 342 又稱 隱藏的星系
位於鹿豹座的一個螺旋星系
它的位置很接近銀河赤道
因此受到塵埃遮蔽而隱藏著
較少被觀測紀錄而被忽略
去年拍的...學藝不精
晴時捕魚；雨時補網
如今總算能夠把圖完成
器材參數：
GSO RC8 / 1600mm - F/8
AP CCDT67 0.67x RD
MoonLite CSL 2.5" RC Focusers
QHY695A@-15度
Guiding with OAG QHY5II-L-M
iOptron CEM60
300s x 27 - Luminance
300s x 10 - Red
300s x 10 - Green
300s x 10 - Blue
總曝光時間 285 分
Sequence Generator Pro
Process by PixInsight & Photoshop
2018/11/04於大雪山50K
Testing my new 1958 Takumar 55mm f2. This lens has 10 blades which gives a beautifull bokeh. I use a Viltrox 0,67x mft to EF with a EF to m42 adapter. The Viltrox makes the 55mm f/2 a 75mm f/1 lens on the digital Olympus PEN-F.
NGC 2403 (also known as Caldwell 7) is an intermediate spiral galaxy in the constellation Camelopardalis. It is an outlying member of the M81 Group, and is approximately 8 million light-years distant. It bears a similarity to M33, being about 50,000 light years in diameter and containing numerous star-forming H II regions. The northern spiral arm connects it to the star forming region NGC 2404. NGC 2403 can be observed using 10×50 binoculars. NGC 2404 is 2000 light-years in diameter, making it one of the largest known H II regions, even larger than Tarantula Nebula in Large Magellanic Cloud. This H II region represents striking similarity with NGC 604 in M33, both in size and location in galaxy.
Acquired on September 2018
Luminance - 320 x 45 sec
Light pollution - 82 x 180 sec
H-alpha - 54 x 180 sec
Red - 60 x 90 sec
Green - 55 x 90 sec
Blue - 65 x 90 sec
Total integration time: 15:18 hours
Imaging telescope and camera:
TS Optics Ritchey-Chrétien 203/1080-1624 mm with 0.67x AP reducer.
ASI1600MM-Cool
Processed with: Pixinsight and Photoshop CC
Location:
Home Backyard, Geleen, Limburg, Netherlands (Bortle 6/7)
The Veil nebula consists of different parts, each with their own designation. The best known ones are NGC6960, or the Eastern Veil Nebula, and NGC6992/NGC6995, or the Western Veil Nebula.
"The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus.It constitutes the visible portions of the Cygnus Loop, a supernova remnant, many portions of which have acquired their own individual names and catalogue identifiers. The source supernova was a star 20 times more massive than the Sun, and it exploded between 10,000 and 20,000 years ago. The remnants have since expanded to cover an area of the sky roughly 3 degrees in diameter (about 6 times the diameter, and 36 times the area, of the full Moon)."
- Wikipedia
Shooting Location :
* 51° N 3° E
* Bortle class 5 backyard
Object Information
* Type : Supernove Remnant
* Visual Size : Approximately 3°
* Magnitude : 7.0
* Frame Center (J2000.0): RA 20h 51m 07s / DEC +30° 40' 07"
* Approximate distance : 2.400 lightyears
Hardware
* Mount : iOptron CEM25P
* Imaging Scope : Canon EF 70-200mm f/2.8 L IS II USM
* Focal Length Setting : 128mm
* Aperture Setting : f/2.8
* Imaging Camera : ZWO ASI 183MM
* Filter Wheel : ZWO EFW 7*36mm + Baader Ha 7nm, Baader OIII 8.5nm + Baader SII 8.5nm + Baader LRGB
* Guide Scope : --- No Guiding ---
* Guide Camera : --- No Guiding ---
Exposures
* Gain : 111
* Sensor Temperature : -20°C
* Light Frames :
- Baader Hydrogen-Alpha : 71x 120sec
- Baader Oxygen-III : 67x 120sec
* Dark Frames : 50x
* Total Integration Time : 4h36m
* Capture Dates : 2020-09-14 & 2020-09-21
Capture Software
* ZWO ASIair Pro
Color Mapping :
* Red : Hydrogen-Alpha
* Green : Oxygen-III
* Blue : Oxygen-III
Processing Software
* AstroPixelProcessor
* PixInsight
* Adobe Photoshop
13/07/2014 Second light with my Starlight Xpress Trius SX-694 Mono 20 X 600 secs subs ( 3 Hrs 20 mins ) in H-alpha 7nm bias,flats no darks. Used Pixelmath for blending two images together one that was sharpened with the unsharp mask tool and another that was not. Had a few problems lately with maxlm dl this time I used Sequence Generator Pro and it worked a treat.
Camera: Xpress Trius SX-694 Mono Cooled to -20C
Guiding: PHD ,9x50 Finder Scope, Lodestar X2 ( Finder Guider )
Optics: Altair Astro 8" RC Astrograph fitted with a Astro Physics CCDT67 0.67x Reducer.
Filter: Baader H-alpha 7nm,Astronomik CLS Filter
Mount: Skywatcher AZ EQ6-GT EQ & Alt-Az Mount connected to the Sky X and Eqmod via HitecAstro EQDIR adapter
Image Acquisition: Sequence Generator Pro
Stacking and Calibrating: Pixinsight
Processing: Pixinsight 1.8
The Great Nebula in Orion, an immense, nearby starbirth region, is probably the most famous of all astronomical nebulas. Here, glowing gas surrounds hot young stars at the edge of an immense interstellar molecular cloud only 1500 light-years away. In the deep image in assigned colors, wisps and sheets of dust and gas are particularly evident. The Great Nebula in Orion can be found with the unaided eye near the easily identifiable belt of three stars in the popular constellation Orion. In addition to housing a bright open cluster of stars known as the Trapezium, the Orion Nebula contains many stellar nurseries. These nurseries contain much hydrogen gas, hot young stars, proplyds, and stellar jets spewing material at high speeds. Also known as M42, the Orion Nebula spans about 40 light years and is located in the same spiral arm of our Galaxy as the Sun.
سديم الجبار – M42
سديم الجبار، منطقة ضخمة قريبة لولادة النجوم وهو من أشهر السدم الفلكية. هنا، يحيط الغاز المتوهج بالنجوم الفتية الساخنة على حافة سحابة جزيئية هائلة بين النجوم على بعد 1500 سنة ضوئية فقط. في الصورة العميقة بالألوان المخصصة، تظهر الخصلات وألواح الغبار والغاز بشكل خاص. يمكن رؤية السديم العظيم في الجبار بالعين المجردة بالقرب من الحزام الذي يسهل التعرف عليه المكون من ثلاثة نجوم في كوكبة الجبار الشهيرة. بالإضافة إلى احتوائه على مجموعة من النجوم المفتوحة الساطعة المعروفة باسم Trapezium، يحتوي سديم الجبار على العديد من الحضانات النجمية. تحتوي هذه المشاتل على الكثير من غاز الهيدروجين، والنجوم الشابة الساخنة، والدوافع، والنفاثات النجمية التي تقذف المواد بسرعات عالية. يُعرف أيضًا باسم M42 ويمتد على حوالي 40 سنة ضوئية ويقع في نفس الذراع الحلزونية لمجرتنا مثل الشمس.
Tech card:
Imaging telescopes: Explore Scientific 127mm ED TRIPLET APO · Teleskop Service TS 10" RC.
Imaging camera: ZWO ASI294MM-Pro.
Mount: iOptron CEM60.
Guiding camera: ZWO ASI290MM mini.
Focal reducers: Teleskop Service CCD47 0.67x reducer for RC telescopes · Explore Scientific 0.7 Reducer/Flattener.
Accessory: ZWO OAG · ZWO EAF Electronic Auto Focuser · ZWO ASIAIR Pro · ZWO 8x 1.25" Filter Wheel (EFW).
Frames:
Astrodon Gen2 E-Series Tru-Balance Lum: 17x120" (34') (gain: 120.00) -10C bin 2x2.
Astrodon Gen2 E-Series Tru-Balance Lum: 21x30" (10' 30") (gain: 120.00) -10C bin 2x2.
Astrodon Gen2 E-Series Tru-Balance Red: 35x60" (35') (gain: 120.00) -10C bin 2x2.
Astrodon Gen2 E-Series Tru-Balance Red: 20x30" (10') (gain: 120.00) -20C bin 1x1.
Astrodon Gen2 E-Series Tru-Balance Green: 27x60" (27') (gain: 120.00) -10C bin 2x2.
Astrodon Gen2 E-Series Tru-Balance Green: 21x30" (10' 30") (gain: 120.00) -20C bin 1x1.
Astrodon Gen2 E-Series Tru-Balance Blue: 29x60" (29') (gain: 120.00) -10C bin 2x2.
Astrodon Gen2 E-Series Tru-Balance Blue: 28x30" (14') (gain: 120.00) -20C bin 1x1.
Chroma 3nm Ha: 40x120" (1h 20') (gain: 120.00) -20C bin 1x1.
Chroma 3nm OIII: 41x120" (1h 22') (gain: 120.00) -20C bin 1x1.
Chroma 3nm SII: 41x120" (1h 22') (gain: 120.00) -20C bin 1x1.
Integration: 6h 54'
Darks: 30.
Flats: 30.
Flat darks: 30.
Avg. Moon age: 4.86 days.
Avg. Moon phase: 31.17%
Bortle Dark-Sky Scale: 4.00.
RA center: 05h35m05s.3.
DEC center: -05°23′27″
Pixel scale: 0.705 arcsec/pixel.
Orientation: 91.747 degrees.
Field radius: 0.977 degrees.
Imaging dates: Jan. 14, 2021, Nov. 12, 2021.
Imaging location: Abu Dhabi desert, UAE.
Our eleventh highlight for 2021 is the C-Spine start. The C-Spine launched routes C1, C2, C3, C4, route 52, night routes C5, C6, express routes X25, X26, X27, X28, X30, X31, X32, peak-hour route P29, and local routes L51, L52, L53, L54, L58 and L59. This caused the removal of the existing routes 25, 25a, 25b, 25d, 25x, 66, 66a, 66b, 66n, 66x, 67, 67n, 67x and 239.
Seen in the photo is Dublin Bus Alexander-Dennis / Enviro400ER PA273 seen on Aston Quay, Dublin City operating the brand new C3 service to Maynooth. This route has replaced route 66.
12/2/2021