jase
26-05-2009, 05:05 PM
Hi All,
It’s been a while between images, though still actively imaging, output has been slow. I’d like to present an image in which I’ve been working on for a while. I previously imaged this target before but at a much longer focal length. I’m pleased to revisit the area with a shorter focal length instrument to portray the majestic nature of the scene. Anyway, here it is; Mandel-Wilson 9 (MW9) – Integrated Flux Nebula (IFN) in Apus. (http://cosmicphotos.com/gallery/image.php?fld_image_id=179&fld_album_id=9)
Warning: large resolution images may take some time to load.
About the target;
Mandel-Wilson 9 (MW9) is the result of the ongoing search for unexplored nebulae surrounding the very high and low galactic latitudes. Known as Integrated Flux Nebula (IFN), it’s illuminated not by a single star, but by the energy from the integrated flux of all the stars in the Milky Way. These nebulae clouds, an important component of the Interstellar Medium, are composed of dust particles, hydrogen, carbon monoxide and other elements. Nestled amongst this vast, yet faint nebulosity is the spiral galaxy IC4633. Reference
(http://www.galaxyimages.com/UNP1.html)
About the image;
The image is a six panel LRGB mosaic covering a 6.2 degree square field of view. I used a synthetic luminance to boost the relatively short luminance filtered data S/N. As seen, it’s not been the easiest data to work with given a couple of the nights were heavily compounded by smoke from control burns that occurred sometime back (22/04). While I acquired the data when the target was high, the smoke haze resulted in diffused stellar profiles and halos in which I was partly able to address through selective processing. In some instances however, I needed to re-acquired data as the masters were ghastly and complex to match between frames. I estimate I threw out around 3 hours of data due to this. Interestingly, the blue filtered data was extremely weak across the frames. Other than the O, B and A spec. type stars and the subtle blue reflection nebulosity, the area is mostly void of any blue hues in the IFN. This was rather troublesome resulting in the need to use pixel math to reach a desirable channel balance. Apologies - no accurate G2V here; really “whacked out” in my opinion which I’m not overly pleased about. However, I’m willing to accept this as colour fidelity is compromised when trying to match colours between mosaic panels. A single frame image is trivial in comparison. Perhaps the most frustrating part of producing this image was panel rotation. I set the PA to 251 degrees for the correct framing as per the mosaic plan in TheSky, yet two frames didn’t overlap which resulted in a star void triangle almost center of the image. Arrggg! Back to the scope to acquire more data. I attribute this to two items; bad planning i.e. image overlap was rather tight at 5% as I was attempting to maximise the FOV. A higher overlap percentage is a sacrifice, but probably best to be cautious. In addition, I failed to adhere to golden rule of aligning northern parts of the frames if the target is south of the celestial equator to ensure sufficient overlap. The opposite is true for northern targets. Will pay more attention to TheSky mosaic plan in future. I’ve found adherence to this rule is not a problem for targets close to the celestial equator or imaging at longer focal lengths as noticeable rotation is usually to a minimum for both situations. Rotation appears quicker closer to pole. With the pain/negative comments out the way, I have to say that this was an enjoyable challenge in which I suspect will fuel similar projects.
No surprises on the processing side so will keep it short calibration (dark/bias/flats), hot/dead pixel removal, subs registered and combined in CCDStack. With the lum masters created, they were loaded into Registar to precisely align the panels for the mosaic. The lum master panels were then loaded into MaximDL for a mild DDP stretch to aid in keeping the same brightness/contrast across the frames. Not perfect, but reduces the workload. I don’t heavily DDP stretch the frames, just a subtle boost to manage the bit space. These were then loaded into PS as individual layers. Each panel was further stretch using level/curves along with the application of the brightness and contrast tool to match the illumination. At this point, any gradients present where manually removed in PS. There were a few, but didn’t pose too much of an issue. The panels were stitched together using layer masks to provide a smooth transition between them before being flattened. Didn't do a very good job of this in specific areas. The individual RGB combined panels went under similar treatment, but were registered directly with the stitched luminance instead of each other. The Integrated Flux Nebula is quite faint, marginally higher than the background ADU count. This required some additional stretching and masking to bring it out. I went for a natural colour saturation of the dusty IFN features. While it was very tempting to boost the saturation to extract a darker and richer tone, I found the result compounded the tonal differences of the nebulosity. It began to take on a mono-tone and featureless appearance. The presented image has been reduced by 50% in size and is a crop of a larger image - web friendly.
Anyway, sit back and have a swim around the scene. Not much in the way of background galaxies (a couple of PGCs and ICs) or other extended objects in this region, just a bucket load of stars, dust and errmm more dust. I particularly like the star (SAO 257486) nestled amongst the IFN producing blue reflection nebulosity. No idea if this is catalogued as I didn’t see it on any star charts during planning. Rather cool. Happy for someone to enlighten me with details.
Thanks for taking the time to read the blurp and/or check out the image. Hope you enjoyed it!
Cheers
It’s been a while between images, though still actively imaging, output has been slow. I’d like to present an image in which I’ve been working on for a while. I previously imaged this target before but at a much longer focal length. I’m pleased to revisit the area with a shorter focal length instrument to portray the majestic nature of the scene. Anyway, here it is; Mandel-Wilson 9 (MW9) – Integrated Flux Nebula (IFN) in Apus. (http://cosmicphotos.com/gallery/image.php?fld_image_id=179&fld_album_id=9)
Warning: large resolution images may take some time to load.
About the target;
Mandel-Wilson 9 (MW9) is the result of the ongoing search for unexplored nebulae surrounding the very high and low galactic latitudes. Known as Integrated Flux Nebula (IFN), it’s illuminated not by a single star, but by the energy from the integrated flux of all the stars in the Milky Way. These nebulae clouds, an important component of the Interstellar Medium, are composed of dust particles, hydrogen, carbon monoxide and other elements. Nestled amongst this vast, yet faint nebulosity is the spiral galaxy IC4633. Reference
(http://www.galaxyimages.com/UNP1.html)
About the image;
The image is a six panel LRGB mosaic covering a 6.2 degree square field of view. I used a synthetic luminance to boost the relatively short luminance filtered data S/N. As seen, it’s not been the easiest data to work with given a couple of the nights were heavily compounded by smoke from control burns that occurred sometime back (22/04). While I acquired the data when the target was high, the smoke haze resulted in diffused stellar profiles and halos in which I was partly able to address through selective processing. In some instances however, I needed to re-acquired data as the masters were ghastly and complex to match between frames. I estimate I threw out around 3 hours of data due to this. Interestingly, the blue filtered data was extremely weak across the frames. Other than the O, B and A spec. type stars and the subtle blue reflection nebulosity, the area is mostly void of any blue hues in the IFN. This was rather troublesome resulting in the need to use pixel math to reach a desirable channel balance. Apologies - no accurate G2V here; really “whacked out” in my opinion which I’m not overly pleased about. However, I’m willing to accept this as colour fidelity is compromised when trying to match colours between mosaic panels. A single frame image is trivial in comparison. Perhaps the most frustrating part of producing this image was panel rotation. I set the PA to 251 degrees for the correct framing as per the mosaic plan in TheSky, yet two frames didn’t overlap which resulted in a star void triangle almost center of the image. Arrggg! Back to the scope to acquire more data. I attribute this to two items; bad planning i.e. image overlap was rather tight at 5% as I was attempting to maximise the FOV. A higher overlap percentage is a sacrifice, but probably best to be cautious. In addition, I failed to adhere to golden rule of aligning northern parts of the frames if the target is south of the celestial equator to ensure sufficient overlap. The opposite is true for northern targets. Will pay more attention to TheSky mosaic plan in future. I’ve found adherence to this rule is not a problem for targets close to the celestial equator or imaging at longer focal lengths as noticeable rotation is usually to a minimum for both situations. Rotation appears quicker closer to pole. With the pain/negative comments out the way, I have to say that this was an enjoyable challenge in which I suspect will fuel similar projects.
No surprises on the processing side so will keep it short calibration (dark/bias/flats), hot/dead pixel removal, subs registered and combined in CCDStack. With the lum masters created, they were loaded into Registar to precisely align the panels for the mosaic. The lum master panels were then loaded into MaximDL for a mild DDP stretch to aid in keeping the same brightness/contrast across the frames. Not perfect, but reduces the workload. I don’t heavily DDP stretch the frames, just a subtle boost to manage the bit space. These were then loaded into PS as individual layers. Each panel was further stretch using level/curves along with the application of the brightness and contrast tool to match the illumination. At this point, any gradients present where manually removed in PS. There were a few, but didn’t pose too much of an issue. The panels were stitched together using layer masks to provide a smooth transition between them before being flattened. Didn't do a very good job of this in specific areas. The individual RGB combined panels went under similar treatment, but were registered directly with the stitched luminance instead of each other. The Integrated Flux Nebula is quite faint, marginally higher than the background ADU count. This required some additional stretching and masking to bring it out. I went for a natural colour saturation of the dusty IFN features. While it was very tempting to boost the saturation to extract a darker and richer tone, I found the result compounded the tonal differences of the nebulosity. It began to take on a mono-tone and featureless appearance. The presented image has been reduced by 50% in size and is a crop of a larger image - web friendly.
Anyway, sit back and have a swim around the scene. Not much in the way of background galaxies (a couple of PGCs and ICs) or other extended objects in this region, just a bucket load of stars, dust and errmm more dust. I particularly like the star (SAO 257486) nestled amongst the IFN producing blue reflection nebulosity. No idea if this is catalogued as I didn’t see it on any star charts during planning. Rather cool. Happy for someone to enlighten me with details.
Thanks for taking the time to read the blurp and/or check out the image. Hope you enjoyed it!
Cheers