View allAll Photos Tagged Subframing
***************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada
(285 km by road north of Toronto)
between 00.32 and 00.52 EDT
* Altitude of centre of frame at time of exposures: 44°, increasing to 47°
* Temperature 9° C.
* Total exposure time: 10 minutes
* 1253 mm focal length telescope
___________________________________________
Description:
The constellation Auriga is festooned with open star clusters, three of which (M36, M37 and M38) are listed in Charles Messier's catalogue of non-stellar objects, commonly known as the Messier List.
In the centre of this image is the bright and large cluster M38, which was discovered in 1654, lies about 3,480 light years from our solar system, and is estimated to be about 250 million years old. It is quite bright, at magnitude 7.4, and is a very pretty sight in even a small telescope.
Below M38, near the bottom edge of the frame and just a little right of centre, is the smaller cluster NGC 1907, which is further away (4,500 light years), fainter (magnitude 8.2) and older (~500 million years) than M82.
For a version of this photo WITH LABELS, click on your screen to the RIGHT of the photo, or click here:
www.flickr.com/photos/97587627@N06/52472161224
___________________________________________
Technical information:
Nikon D810A camera body on Explore Scientific 152 mm (6") apochromatic refracting telescope, mounted on Astrophysics 1100GTO equatorial mount
Ten stacked subframes; each frame:
ISO 6400; 1 minute exposure at f/8
(with LENR - long exposure noise reduction)
Subframes stacked in RegiStar;
Processed in Photoshop CS6 (brightness, colour balance & saturation, sharpening)
***************************************************************************
******************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada
(285 km by road north of Toronto)
between 00.51 and 01.26 EDT
* Altitude of the nebula at time of exposures: 35°, increasing to 41°
* Temperature 13° C.
* Total exposure time: 15 minutes
* 1200 mm focal length telescope
___________________________________________
Description:
This is a combination emission / reflection gas cloud, about 5 light years in diameter and lying 1,500 light years distant from our solar system.
The bright star that is embedded in the nebula is a "runaway star", the 6.0-magnitude irregular variable star AE Aurigae, which is known as the "Flaming Star". For more about this star, click here:
en.wikipedia.org/wiki/AE_Aurigae
___________________________________________
Nikon D810a camera body on Explore Scientific 152 mm (6") apochromatic refracting telescope, mounted on Astrophysics 1100GTO equatorial mount with a Kirk Enterprises ball head
Fourteen stacked subframes; each frame:
ISO 8000; 1 minute exposure at f/8
(with LENR - long exposure noise reduction)
Subframes stacked in RegiStar;
Processed in Photoshop CS6 (brightness, contrast, levels, colour balance, sharpening, partial blurring of graininess in image)
******************************************************************************
1994 SAAB 900 S convertible.
Registered in August 1996.
Last MoT test expired in August 2020 (SORN).
It failed a test on 22nd April 2021 -
Offside front headlamp aim too low (4.1.2 (a)) - Major
Nearside front side repeater not working (4.4.1 (a) (ii)) - Major
Nearside front service brake excessively binding (1.2.1 (f)) - Major
Offside front subframe mounting prescribed area excessively corroded significantly reducing structural strength near lower arm. (5.3.6 (a) (i)) - Major
Nearside rear suspension component mounting prescribed area excessively corroded significantly reducing structural strength close to rear suspension mount. (5.3.6 (a) (i)) - Major
A shock find on streetview. While prepping for a spotting trip, I thought I'd have a look in a random newbuild estate, just because the streetview had been done pretty recently. To my surprise, this pre-facelift Ulysse was sitting, so I went to go and see it the next day.
Long term ownership and off the road since last year, after failing it's MOT on the dreaded Front Subframe. I'd say it's the end of the road for this rare MPV, but kudos to the owners for keeping it about.
P797 FJA
I like how the nebulosity emerged with both emission and hints of reflective nebulae. But I’ll need to figure out how to manage “bloated” stars.
TMB 80mm f/6.3 refractor, TV 0.8x field flattener/reducer, ASI533MC Pro, 20 60-second subframes with a dual narrow band filter and 20 90-second subframes without filter. Calibrated with darks, flats, etc. Post-processed with DSS and PS.
January 24, 2025; Backyard, Tallahassee, Florida. Bortle 7 sky. Waves of cirrus moved in during imaging making what would otherwise be good seeing variable. Guiding total error was about 2 arcsec. I’ve been using the ST-4 port to connect the guider. I’ll try using the ASCOM driver next time. I also used NINA’s sequencer and it worked fine. I had a few glitches due to “operator error” which should resolve with experience. NINA is an impressive program but has a bit of a learning curve. That’s what makes this hobby so much fun, all the learning curves. It’s hard to get complacent because there are always new challenges.
This image is mainly in Hydrogen Alpha, mixed with some green subframes to create a colour image and bring out detail in this faint nebula. It is the sharpest I have managed with my largest telescope following a much needed collimation session. It consists mainly of seventeen five-minute subframes in H Alpha taken through my 12inch SCT, lightly cropped to allow the image to be centred.
Peter
NGC 1999 is the reflection nebula at centre right and it is just south of the Orion nebula which is off the right hand edge
of the frame.
This is an integration of 18 hours total exposure shot in multiple 180s and 240s subframes on a QHY168C camera. The scope was a WO Zenithstar 103. Image capture was managed with SGP and PHD2, post-processing was done in PixInsight.
Observed from Prachinburi, Thailand
Shot with an STC duo-narrowband filter on a QHY168C OSC camera, this is an integration of 240 x 5 minute subframes. The scope was a WO Zenithstar 103 mounted on a Skywatcher EQ6R Pro. Image capture was managed via SGP and PHD2, all post-processing was carried out in PixInsight.
Observed from Prachinburi, Thailand
This emission nebula, found in Cygnus slightly SE of η Cygni, was first recorded by Stewart Sharpless in 1959 in the Sh-2 catalog. It is primarily hydrogen and is excited by the hot, young star HD 227018, the relatively small, blue star (O6) located just above the much brighter star on the right hand side of the nebula. There is a loop of Oiii (blue) surrounding it.
Cygnus X-1, associated with HD 226868, aka SAO 69181 is just slightly out of the frame here. Unfortunately, the field of view of the scope-camera combination is slightly too small to fit the star in while presenting Sh2-101 in an aesthetically pleasing way. In this image, North is approximately to the left.
I used a C-11 Edge with f/7 focal reducer for a focal length of 1960 mm. The mount was a Losmandy G11 and the camera an ASI 1600mm equipped with a seven position filter wheel. The Field of View (FOV) is 31’ x 23’ and resolution is 0.39 arc seconds/px. Guiding was done with an ASI 120 mm through an AT65 refractor, via PhD2.
This image was captured from my light-polluted Albuquerque back yard in Sii, Hα and Oiii. 36 x 300 second subframes were captured with Hα and Oiii. I was only able to capture 13 x 300 seconds subframes with Sii.
Processing was done in PixInsight; the image is presented in a modified version of the Hubble Palette, (S, Hα, Oiii). A deconvolved version of the Hα stack was used as a Luminance layer.
****************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada
(285 km by road north of Toronto)
between 23.30 and 23.50 EDT
* Total exposure time: 10 minutes
* 660 mm focal length telescope
* Field of view: ~2.8° wide x 1.7° high
* Altitude of galaxy at time of exposures: 22.5°, declining to 20.4°
___________________________________________
Description:
This was my first attempt at photographing this magnitude 8.8 galaxy, which is famous in the history of astronomy, as you will see from reading the description below:
From Wikipedia:
"NGC 6822 (also known as Barnard's Galaxy, IC 4895, or Caldwell 57) is a barred irregular galaxy approximately 1.6 million light-years away in the constellation Sagittarius. Part of the Local Group of galaxies, it was discovered by E. E. Barnard in 1884, with a six-inch refractor telescope. It is the closest non-satellite galaxy to the Milky Way, but lies just outside its virial radius. It is similar in structure and composition to the Small Magellanic Cloud. It is about 7,000 light-years in diameter.
Edwin Hubble, in the paper N.G.C. 6822, A Remote Stellar System, identified 15 variable stars (11 of which were Cepheids) of this galaxy. ... Hubble's detection of eleven Cepheid variable stars was a milestone in astronomy. Utilizing the Cepheid Period-Luminosity relationship, Hubble determined a distance of 214 kiloparsecs or 698,000 light-years. This was the first system beyond the Magellanic Clouds to have its distance determined. (Hubble continued this process with the Andromeda Galaxy and the Triangulum Galaxy). This distance to the galaxy was way beyond Harlow Shapley's value of 300,000 light-years for the size of the universe. In the paper, Hubble concluded the "Great Debate" of 1920 between Heber Curtis and Shapley over the scale of the universe and the nature of the "spiral nebula". It soon became evident that all spiral nebulae were in fact spiral galaxies far outside our own Milky Way."
__________________________________________
Technical information:
Nikon D810a camera body on Tele Vue 127is (127 mm - 5" - diameter) apochromatic refracting telescope, mounted on a Sky-Watcher EQ6-R PRO SynScan mount
Ten stacked subframes - each frame:
660 mm focal length
ISO 3200; 1 minute exposure at f/5.2, unguided, with long exposure noise reduction
Stacked in RegiStar 1.0.10
Processed in Photoshop CS6 (brightness, contrast, colour balance)
****************************************************************************
Rationalisation at NCS HQ yielded the Modular MQB platform (Modular, Quick-change, Basic) with a common body mated to a wide range of powertrain subframes.
Here we have an MQB body mated to a Sondo-Reata-Nautics Hovercraft platform kit.
(Apologies for the polygons - Blender doesn't like doing those corner pipes in rubber for some reason)
As seen from an elevation of 4,000 feet at the top of Mary's Peak in Oregon. My Seestar S50 ran from 9:50PM till 4:30AM collecting 1,020 ten-second subframes. The night was moonless, clear and cold.
******************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada, between 23.07 and 23.36 EDT
(285 km by road north of Toronto)
* Temperature 7° C.
* Total exposure time: 14 minutes
* 540 mm focal length telescope
___________________________________________
Description:
This supernova remnant is a delicate and beautiful sight in long exposure photos. It can also be glimpsed in good amateur telescopes in a dark sky as gossamer silver strands crossing the field of view.
Read more about the Veil Nebula here:
en.wikipedia.org/wiki/Veil_Nebula
... and here:
www.astronomy-mall.com/Adventures.In.Deep.Space/Dissectin...
For a version of this photo WITH LABELS, click on your screen to the RIGHT of the photo, or click here:
www.flickr.com/photos/97587627@N06/29424927240
___________________________________________
Technical information:
Nikon D810a camera body on Teleview 101is apochromatic refracting telescope, mounted on Astrophysics 1100GTO equatorial mount with a Kirk Enterprises ball head
Fourteen stacked frames; each frame:
540 mm focal length
ISO 6400; 1 minute exposure at f/5.4; unguided
(with LENR - long exposure noise reduction)
Subframes registered in RegiStar;
Stacked and processed in Photoshop CS6 (levels, brightness, contrast, colour balance)
******************************************************************************
563 ten-second subframes.
I imaged the Flaming Star Nebula using two different smartscopes with dramatically different results. There were also differences in post-processing that influence the differences. The two smartscopes' cost was nearly identical. No one scope is better than the other, but each has a distinct look. See below for comparison.
Rationalisation at NCS HQ yielded the Modular MQB platform (Modular, Quick-change, Basic) with a common body mated to a wide range of powertrain subframes.
Here we have an MQB body mated to Boston Dynamics 4x4 'Iron Horse' Walking platform.
5 x 240s subframes- Testing out what Rho Ophiuchi looks like at 135mm.
Earth & Sky - Mount John University Observatory
******************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada
(285 km by road north of Toronto)
* Temperature 11° C.
* Total exposure time: 8 minutes.
___________________________________________
Description:
The familiar "W" shape of the bright stars in the constellation Cassiopeia rides high in the northern hemisphere autumn and winter sky, with our home galaxy, the Milky Way, running through it and down into the constellation Perseus.
Many large and bright nebulae (hydrogen gas clouds) appear in this area of the sky, along with numerous gravitationally bound open clusters of stars.
Above centre are the bright red hydrogen gas clouds known as the "Heart" and "Soul' Nebulae. For a close-up view of the Heart Nebula made with a 540 mm focal length telescope on the same evening, click here:
www.flickr.com/photos/97587627@N06/31079231531
For a version of this photo WITH labels, click on the right side of your screen, or click here:
www.flickr.com/photos/97587627@N06/30406597543
___________________________________________
Technical information:
Sigma 50 mm f/1.4 DG HSM ART lens on Nikon D810a camera body, mounted on Astrophysics 1100GTO equatorial mount with a Kirk Enterprises ball head
Eight stacked frames; each frame:
50 mm focal length
ISO 2500; 1 minute exposure at f/4; unguided
(with LENR - long exposure noise reduction)
Subframes registered in RegiStar;
Stacked and processed in Photoshop CS6 (brightness, contrast, levels, colour balance, colour desaturation)
******************************************************************************
This is the Rho Ophiuchi Cloud Complex, which lies near the summer Milky Way on the border between the constellations of Scorpius and Ophiuchus. This area is loaded with gas and dust, and is home to many deep sky objects. It is also one of the more colorful nebulae in the sky.
Image Info
Imaged from the KPO field in Saint Cloud, Florida.
Camera : ZWO ASI1600MM Pro, Gain set to 200
Lens: Canon 100-400 f/5.6L lens, set to 135mm
Mount: iOptron SmartEQ Pro
Red: 12 subframes of 300s = 60 min integration
Green: 8 subframes of 300s = 40 min integration
Blue: 10 subframes of 300s = 50 min integration
Luminance: 11 subframes of 300s = 55 min integration
Hydrogen Alpha: 2 subframes of 300s = 10 min integration
Total integration time: 215 min = 3.6 hours.
Captured via ASIAir Pro automation
Optical tracking via ASIAir automation, currently using ST4 mount control via the ASI120MM-S guide camera
Separate channels stacked and HaLRGB integrated in Astro Pixel Processor, and processing for light pollution sky fog removal
Image cropped, stretched, and noise processed in Nebulosity.
Final processing in Aperture
Another of my favourite winter objects. This is a stack of twenty-two eight minute subframes in H Alpha from tonight, 7 January 2016.
Peter
Equipment used: Atik460EX camera, HA filter, 0.75 reducer, 130mm triplet APO refractor and EQ8 mount
Skywatcher 72ED apo with field flattener,SX Trius 694/filterwheel/OAG (Lodestar) riding on CEM60.
Six 10 minute subframes captured through Ha and OIII filters,stacked in Deepskystacker and colour combined (Ha,OIII,OIII) in Maxim DL4. Processed in Astroart 8 and PS CS2.
Taken 31/10/21
***************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada, between 22.58 and 23.09 EDT
(285 km by road north of Toronto)
* Temperature 17° C.
* Total exposure time: 6 minutes.
___________________________________________
Description:
The centre of our home galaxy, the Milky Way, lies in the constellation Sagittarius, which in the northern hemisphere summer lies low in the south at midnight.
In this view appear many favourite targets of amateur astronomers with modest telescopes, including the large glowing Lagoon Nebula at the lower right.
For a version of this photo WITH LABELS, click on your screen to the RIGHT of the photo, or click here:
www.flickr.com/photos/97587627@N06/28589630170
___________________________________________
Technical information:
Nikkor AF-S 70 - 200 mm f/2.8 G ED VRII lens on Nikon D810a camera body, mounted on Astrophysics 1100GTO equatorial mount with a Kirk Enterprises ball head
Six stacked frames; each frame:
135 mm focal length
ISO 4000; 1 minute exposure at f/4.5; unguided
(with LENR - long exposure noise reduction)
Subframes registered in RegiStar;
Stacked and processed in Photoshop CS6 (brightness, contrast, levels, colour balance, colour desaturation)
***************************************************************************
This nebula is rich in ionized hidrogen and some interesting dark bands. Telescope GSO RC 30cms, camera STF8300/AO-8, 16min subframes, 5 hours total in Ha-L-RGB composite from my backyard homemade observatory at La Colonia, Illapel, Chile. Take care and have a good day!
Esta nebulosa de emisión ubicada en Puppis es rica en hidrogeno alfa y bandas oscuras. Imagen de 5 horas en Ha-L-RGB, telescopio GSO RC 30cms, camara STF8300/AO8, desde mi observatorio hecho en casa en La Colonia, Illapel, Chile; saludos y cuídense, que tengan un buen día...
Watch out! Fire truck in a hurry to help!
I present to you my version of the fire truck of the 60s. Its distinguishing feature is a nice design, detail, a fairly simple but intricate design and rich functionality.
The machine is equipped with everything necessary, there is a water monitor, hoses, ladder, tool holders, boxes. There are two taps for water supply.
In detail even the bottom, deploying the machine you will notice the imitation of the subframe and the drive system.
Inside you can place a minifigure.
The fire engine blends well with the modular building 10197 and fits in the garage.
Assembled from 322 existing parts.
1997 Jaguar XK8 4 Litre auto.
Previously registered J20 AKS, JR 7237, J853 GGP, VOT 92 and P804 UAV.
Last MoT test expired in November 2015 (SORN).
It failed a test that month -
Nearside rear subframe mounting prescribed area is excessively corroded outer sill area (2.4.a.3)
Offside rear subframe mounting prescribed area is excessively corroded outer sill area (2.4.a.3)
Nearside brake pipe excessively corroded front to rear (3.6.b.2c)
A few shockers in this one for me - the colour for a start - this colour became "fashionable" not that long ago? Certainly not something I would expect to see on a scrapped car anyway. Looking up the history of SL12 NRO, it amazes me to see that it failed an MOT in March 2021 for corrosion to the subframe - it did get repaired and still has a current MOT, with only 58k recorded - but as you can see, it was scrapped. I can happily report that my old Corsa is still on the go, now with 144k on the clock and no serious issues in it's MOT history - how could two cars starting out from the same point have such different histories?
******************************************************************************
Photographed at Algonquin Provincial Park, Ontario, Canada, between 00.12 and 00.45 EDT
(285 km by road north of Toronto)
* Altitude of the nebula at time of exposures: 55°, decreasing to 50°
* Temperature 5° C.
* Total exposure time: 15 minutes
* 2483 mm focal length telescope
___________________________________________
Situated in the heart of our Milky Way galaxy as it passes directly overhead during the summer in the northern hemisphere, the Crescent Nebula is a half ring of ionized hydrogen gas, which glows with a characteristic red-pink colour. The nebula has an angular size of 20' x 10', which makes it about 1/3 the apparent size (in area) of the Moon as seen from Earth.
From Wikipedia:
The Crescent Nebula is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by Friedrich Wilhelm Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.
It is a rather faint object located about 2 degrees SW of [the bright star] Sadr. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".
Click here to see a wider angle view of this region, which shows adjacent larger diffuse hydrogen gas clouds in the constellation Cygnus:
www.flickr.com/photos/97587627@N06/29549773051
Click here to see the equipment used to photograph this galaxy:
www.flickr.com/photos/97587627@N06/29939255555
___________________________________________
Nikon D810a camera body at prime focus of Meade 30 cm (12") LX-850 Schmidt-Cassegrain telescope, mounted on Astrophysics 1100GTO equatorial mount
Fifteen stacked frames; each frame:
2483 mm focal length; ISO 10,000; 60 seconds exposure at f/8, unguided
(with LENR - long exposure noise reduction)
Subframes stacked in RegiStar;
Processed in Photoshop CS6 (brightness, contrast, levels, sharpening)
******************************************************************************
I took an image of the Heart Nebula back in the autumn of 2013. While working on that image I was struck by the beauty of IC 1795, the appendage protruding from the "point" of the heart. At that time I acquired a few Ha subframes of IC 1795, but didn't get enough for an image. It's been on my unfinished business list since then.
This year while I was tuning the 16" I thought I'd use some of the time I was testing tracking accuracy to try to check IC 1795 off my todo list. This is the result.
The Heart Nebula itself is IC 1805/SH2 190. The gorgeous center of this nebula is a complex structure that I interpret as being a typical dust pillar, but seen from above rather than the side. If this is the case, then Melotte 15, the star cluster powering this entire complex, must be in front of the central pillar complex. Perhaps the Heart Nebula isn't so heart-shaped at all. It's a more typical hollow cavity, with an incredibly dense pillar on its far inner wall.
There is a considerable amount of oxygen and sulfur in this nebula. This indicates that it is older and much more evolved than most starbirth regions where these elements are much more rare. This is supported by the relative sparseness of Melotte 15. Perhaps many of its original members have been gravitationally ejected from the system and have entered the general population of the galaxy.
Sometimes when I take an image, I ultimately end up rather unimpressed by the result. Not too many people see those results. This one, though... I'm really pleased with this one. This goes into my picture book, and maybe even on my wall :)
This is 28x900Ha, 12x900OIII, and 13x900SII for a total of 13,25 hours of imaging on the Twin City Amateur Astronomers - TCAA.16" AG Optical Systems imaging Harmer-Wynne.
1,042 ten-second subframes. This overlaps with a previous image I made below and adds to the upper left.
Seestar S50 | Mosaic mode | Polar Alignment
Full write-up here: theastroenthusiast.com/orion-widefield/
Cradled in cosmic dust and glowing hydrogen, stellar nurseries in Orion the Hunter lie at the edge of a giant molecular cloud some 1,500 light-years away. Spanning nearly 25 degrees, this breath-taking vista stretches across the well-known constellation from head to toe (left to right). The Great Orion Nebula, the closest large star forming region, is right of center. To its left are the Horsehead Nebula, M78, and Orion’s belt stars.
Equipment:
Nikon D800
50mm f1.4 lens
GEM 28
NINA
Nikonhacker
Acquisition:
ISO 800, F2.8
Taken from a bortle 1 zone in Northwest CT
155 x 240s subframes (10 hours) – Taken on 12/26/2022, 12/27/2022
Processing:
Pre-processing and stacking
- All subframes were calibrated and normalized through WBPP
- The subframes were debayered and split into monochrome channels
- The subframes were registered with distortion correction
- the subframes were registered based on a PSF snr estimate
- The subframes were normalized using local normalization
- Each channel was integrated separately using the ESD clipping algorithm
Preparation of all frames:
- Stacking artifacts were cropped
- the RGB channels were combined to create an RGB image
- the RGB image was plate solved
- DBE was applied iteratively
- the RGB image was photometrically color calibrated
Linear noise reduction
- A low-contrast mask was applied
- Two iterations of TGV noise reduction were applied, one targeting high-frequency noise and one targeting low-frequency noise
- A medium-contrast mask was applied
- MMT targeting all 8 scales was applied to remove large-scale noise
Stretching
- The stars were seperated from the nebula using Starnet 2
- the RGB image was stretched using Arcsinh stretch
Non-linear adjustments:
- LRGB combination
- HDR, LHE, and curves to increase local contrast
- MLT was applied targeting 5 layers of luminance
- The background level was set to .09
- the stars were stretched using Arcinh stretch
- The image was relinearized and the stars were added back
Website: theastroenthusiast.com/
Instagram: www.instagram.com/the_astronomy_enthusiast/
Running through a film in a short timeframe means going to places you can be certain of a few shots. Old Fergie's cottage (Glenside) in Fin Glen meets that description nicely. It's sad that he never fulfilled his dream to renovate this ruin, but the place has loads of character.
I didn't take notes as I was taking these shots, but I think this was taken with the Auto-Takumar 55/1.8.
Straighten and crop a little in PP. Darkened LHS of window frame slightly.
1991 Ford Sierra Sapphire 1.8 GLX.
Supplied by Evans Halshaw (Ford).
Last MoT test expired in January 2007.
It failed a test in October 2007 -
Offside Front coil spring cracked (2.4.C.1a)
Nearside Rear Subframe mounting prescribed area is excessively corroded (2.4.A.3)
Year of first registration: 1992.
The GTM Rossa is a Mini based 2+2 kit car by GTM Cars.[1] The car was based on two front mini subframes, with the steering being locked on the rear subframe. The Mark 1 car was produced from 1987 to 1990, and the Mark 2 car was produced beginning in 1990.
Bron: Wikipedia.org