The Image Index is a system based on likes received on images, that incentivizes the most active and liked members of the community. Learn more.
The Contribution Index (beta) is system to reward informative, constructive, and valuable commentary on AstroBin. Learn more.
Imaging telescopes or lenses: Explore Scientific PN-208/812 Carbon Fiber OTA
Imaging cameras: ZWO ASI 1600MM Cool
Mounts: SkyWatcher AZ-EQ5
Guiding telescopes or lenses: ZWO Off Axis Guider
Guiding cameras: Starlight Xpress Lodestar Autoguider X2
Filters: ZWO H-alpha 7nm · Green · Blue · OIII · Red
Accessory: Explore Scientific HR Coma Corrector
Dates:Aug. 26, 2018 , Aug. 29, 2018 , Sept. 4, 2018 , Sept. 5, 2018 , Sept. 16, 2018 , Sept. 19, 2018 , Sept. 29, 2018 , Sept. 30, 2018 , Oct. 1, 2018 , Oct. 2, 2018 , Oct. 4, 2018 , Oct. 8, 2018 , Oct. 14, 2018 , Oct. 18, 2018 , Oct. 19, 2018 , Oct. 22, 2018
Frames:
Blue: 93x60" (gain: 139.00)
Green: 80x60" (gain: 139.00)
ZWO H-alpha 7nm: 267x400" (gain: 139.00)
OIII: 275x400" (gain: 139.00)
Red: 64x60" (gain: 139.00)
Integration: 64.2 hours
Avg. Moon age: 16.86 days
Avg. Moon phase: 57.58%
Bortle Dark-Sky Scale: 8.00
Astrometry.net job: 2327856
RA center: 1h 56' 31"
DEC center: +65° 28' 26"
Pixel scale: 0.457 arcsec/pixel
Orientation: 89.531 degrees
Field radius: 0.313 degrees
Resolution: 4000x2900
Locations: Home Roof (Bortle 7-8 / Est. Sky Quality: 18.53), Springfield, PA, United States
Data source: Backyard
IPHASX J015624.9+652830 (also known as Ferrero 6) is the final image in my ‘trio of faint targets’ this fall. IPHASX J015624.9+652830 is a ridiculously faint planetary nebula in Cassiopeia spectroscopically confirmed by Laurence Sabin as part of the IPHAS survey in 2011 and independently discovered by amateur astronomer Laurent Ferrero in 2013 using plates of the Digitized Sky Survey. To date, I’ve only been able to find four other versions of this target (all of which were shot with CCDs): Jim Shuder’s version using a C9.25 EdgeHD, Frank Slotosch’s version using an 8” Newtonian, Sascha Schueller’s version using a 16” f/4 Newtonian and 0.73x reducer and Mark Hanson’s utterly epic version in November of 2017 using a 24” Planewave. If there’s another version you happen to be aware of that I haven’t found, let me know so I can add it to this list.
Edits:
Just wanted to add Pat Rodgers' image to this list.
Also wanted to add Jerry Macon's image to the list.
Adding Peter Goodhew's epic version to the list.
Adding Andreas' (equinoxx) image to the list.
Adding Szeri László's image from June 8, 2019, which I randomly found today (11/17/2019).
While the OIII signal in PuWe1 is undoubtedly weaker than either the Ha or OIII signal in IPHASX J015624.9+652830 (Fe 6), the Ha signal in PuWe1 seems to be a good deal stronger, making this (probably) the faintest target I’ve ever done. I doubt more integration time would help me pull out anything more on this. A 30-hour stack looked like a single sub of other planetary nebulae I’ve worked on.
Description: Crop
Description: Uncropped bicolor draft (no RGB stars).
You have no new notifications. |
This page or operation is not available at the moment, because AstroBin is in READ ONLY mode. For more information, please check out our Twitter feed: https://twitter.com/AstroBin_com
This feature is only offered at higher membership levels.
Would you be interested in upgrading? AstroBin is a very small business and your support would mean a lot!
If this user has been harassing you, and you shadow-ban them, all their activities on your content will be invisible to everyone except themselves.
They will not know that they have been shadow-banned, and the goal is that eventually they will get bored while having caused no harm, since nobody saw what they posted.
You will remove your shadow-ban on this user, and their comments, messages, etc, will appear again on your content.
Such limitation improves the website as a whole by discouraging people from creating fake accounts to like their own content. Thank you for understanding!
Currently, your Image Index is .
To learn more about the Image Index, please visit the FAQ page. Thanks!
Comments