Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)
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SH2-101 the Tulip Nebula in Cygnus, Mark Wetzel
SH2-101 the Tulip Nebula in Cygnus
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SH2-101 the Tulip Nebula in Cygnus

Revision title: SH2-101 the Tulip Nebula in Cygnus (Reprocessed)

Getting plate-solving status, please wait...
SH2-101 the Tulip Nebula in Cygnus, Mark Wetzel
SH2-101 the Tulip Nebula in Cygnus
Powered byPixInsight

SH2-101 the Tulip Nebula in Cygnus

Revision title: SH2-101 the Tulip Nebula in Cygnus (Reprocessed)

Equipment

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Acquisition details

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Description

Monmouth, OR
September 3 and 4, 2021

Modified image with limited data

The summer of 2021 has been a bad one for me.  Clouds, smoke and travel caused me to miss several new moon cycles.  Also, making my Losmandy G11 mount and ZWO ASI 2600 camera upgrades function optimally remain a work in progress.  Since the Oregon Star Party was cancelled, a fellow astrophotographer held a “mini OSP” at his house.  This gave me the opportunity to start my first deep sky project with the ASI 2600 camera.  The ASI 2600 has a Sony APS-C sensor and a large thermoelectric cooler.  The 16-bit sensor has high sensitivity, low noise, wide dynamic range and good quantum efficiency.  The Tulip nebula was a good target to test camera performance.  In order to reach and maintain the desired cooling temperature, the camera uses a Sunon high-speed fan.  Several threads on Cloudy Nights discussed a fan vibration issue.  I suspected that my new camera suffered from vibration problems as stars were highly elongated while guiding was decent.  I attempted to reduce the fan vibration coupling to the sensor by adding several vibration dampening measures: silicone fan mounts, a silicon mason jar seal for isolating the back plate from the camera housing, and silicon O-rings on the screw heads holding the back plate to the camera housing.  Another issue with the ASI 2600 is a serious flaw in the ASCOM driver.  ZWO decided to limit the gain to a maximum of 100.  This requires longer exposures for autofocus and plate solving processes.  Since Sequence Generator Pro no longer supports native camera drivers, I was forced to use the ASCOM driver.  Even though other ZWO camera ASCOM drivers do not have this limit, ZWO refuses change the driver to allow astrophotographers to use the entire range of the camera.  The other problem with the ASCOM driver is that Sequence Generator Pro cannot set the offset: I fixed it to 68 in the ASCOM driver settings dialog.  Also, as part of the system upgrade, I purchased a Flypower 60Ah LiFePO4 battery and a battery box on Amazon for imaging in the field.

On September 3, I started a new project with narrowband imaging of the SH2-101, the Tulip nebula, in the constellation Cygnus.  The Tulip nebula is large emission nebula which was ideal for the new camera’s field of view.  SH2-101 is a moderately bright emission nebula, dominated by Hydrogen.  The Oxygen and Sulfur signals were rather faint, but present.  The seeing was good and there was no smoke for a change.  The stars were sharp, but slightly elongated (eccentricity between 0.4 and 0.55 per PixInsight analysis).  I did attempt to use PEMPro to create a Periodic Error Correction curve, but it failed to complete the calibration process with the Pattern.fit file not found error.  PEC correction is on the To Do list for October.  I collected a limited amount of data over 1 ½ nights of imaging.  I switched to planetary imaging for two hours to collect data on Jupiter as it was bright and near the meridian, and the Great Red Spot was visible.  The lure of Jupiter was too much to resist.The ASI 2600 did perform very well at -10oC and the vibration problem seemed to be resolved.  The sensor thermoelectric cooling requires a significant amount of power.  I selected -10oC as the temperature so that the camera could reach setpoint and use less than 75% power (over 1 Amp).  The subframes from the ASI 2600 had good quality without any amp glow or distortions around bright stars, a big improvement over the ASI 1600.  Autoguiding performance was decent with an RMS error ranging between 0.5 and 0.7 arcsec (the image scale was 0.471 arcsec).  I anticipate an improvement in mount performance when a good PEC curve is created in PEMPro and loaded into the mount.  The battery test was successful, and the battery maintained its output over the 8 hours of imaging time.  The battery is unregulated with an output voltage that started at 13.4 VDC and dropped to 31.1 V.  I use a 12 Volt regulator in my power distribution system, so the higher voltage is no problem.

I calibrated the limited data in PixInsight with a new dark library, flats and dark flats.  I used all subframes since they were of high quality and had low noise.  The Hydrogen-a, Oxygen-III and Sulfur-II 7nm narrowband filter data were combined by assigning H-a to the red, S-II to the green, and O-III to the blue channel.  The HSO combination makes the tulip stand out.  I used Starnet in PixInsight for the first time to remove the stars so that the nebula could be processed separately from the star field.  The nebula was cleaned up and sharpened.  The star colors were adjusted and then the stars image was combined with the starless image to produce the final result.  In October, I will image the Tulip nebula for one more night to get more O-III, S-II and some RGB data for star color.

The Tulip nebula is in the plane of the Milky Way in a region rich in gas and dust in Cygnus the Swan.  It is about 8,000 light-years distant, and it is 70 light-years across (NASA).

Imaging details:

Celestron 9.25" Edge HD SCT
Celestron 0.7x Focal Reducer (FL = 1645mm, f/7)
Celestron off-axis guider with a ZWO ASI 174MM mini guide camera
Losmandy G11 mount with Gemini 2
ZWO ASI 2600MM Pro cooled monochrome camera (-10C)
ZWO 36mm Hydrogen-a, Oxygen-III and Sulfur-II filters

Software:     Sequence Generator Pro, ASTAP plate solving, PHD2 guiding, 
                  Losmandy Gemini ASCOM mount control and web client interface,
                  SharpCap Pro for polar alignment with the Polemaster camera,
                  PixInsight 1.8.8-9 and Photoshop CC 2021

Hydrogen-alpha 10 min x 21 subframes (210 min), Gain 100, Offset 68, 1x1 binning
Oxygen-III   10 min x 16 subframes (160 min), Gain 100, Offset 68, 1x1 binning
Sulfur-II 10 min x 15 subframes (150 min), Gain 100, Offset 68, 1x1 binning

Comments

Revisions

  • SH2-101 the Tulip Nebula in Cygnus, Mark Wetzel
    Original
  • Final
    SH2-101 the Tulip Nebula in Cygnus, Mark Wetzel
    C

C

Title: SH2-101 the Tulip Nebula in Cygnus (Reprocessed)

Description: Monmouth, OR
September 3 and 4, 2021, Reprocessed January 14, 2022

With additional data, I reprocessed the Tulip Nebula narrowband filter images using the Hubble pallet (Sulfur-II to Red, Hydrogen-a to Green and Oxygen-III to Blue channels, SHO). Several new tools and techniques were tested in PixInsight, so the resulting false color image is a work in progress. In the first processing version, I had created a HSO color image that made the tulip glow in red-yellow hues. This time, I wanted to create more of a rainbow effect and utilize starless images in the processing workflow. While the image is no longer scientifically relevant, it does show more details in the nebula than the previous version.

Key steps in the image processing workflow:
1) I used the Ha, Oiii and Sii calibrated and integrated images generated in the previous HSO image processing version. Each channel image had been cropped and then denoised with the Mure Denoise script.
2) Russ Croman’s StarXTerminator was used to create starless and stars images for each channel in the linear state. The one issue with StarXTerminator using the Version 7 AI weighting is that very faint ghosts of stars remain in the combined starless image, resulting in subtle mottling where stars are not present in the image combined with the stars image.
3) The stars narrowband images were combined into one RGB image and the Photometric Color Calibration was used to create some semblance of acceptable star colors. Short of taking RGB data, there is probably a better way to handle the stars images to obtain more realistic colors.
4) The stars RGB image was stretched and processed to get a desired number of stars with adequate brightness and morphology. The CurvesTransformation tool was used to tweak the star brightness and how many stars were visible and to make the background black for subsequent combination with the processed starless image.
5) The Ha, Oiii and Sii channels were linearized with LinearFit to the brightest channel without saturating any one channel. To determine which image was the brightest (or dimmest), the Statistics tool was used, and the Mean and Median values defined the ranking. Each channel when combined would then have similar or enhanced brightness. Starless images provide great capability and flexibility for image processing.
6) The narrowband starless images were combined with the ChannelCombine tool using the Hubble Pallet assignment (SHO) to create an RGB color image. This made Sii and Oiii contributions strong and there was no green cast to be removed.
7) The Luminance was extracted from the RGB image.
8) The Luminance image was stretched, denoised (background) and sharpened. I downloaded and tried the Generalized Hyperbolic Stretch script to stretch the image in several passes. The tool provides excellent curve shaping parameters. The downside is that there is no real time preview when moving sliders, so I had to use the histogram after the first stretch. This script allows you to shape the curve to prevent clipping stars while being more aggressive with the midtone and shadow regions. I used this script for all image stretching, including the RGB starless and stars images. Sharpening was done with the Histogram Equalization process tool with three kernel sizes and bit depths to sharpen details for different scales. Denoising was done with the TVGDenoise process tool using a low contrast mask and a support mask.
9) The starless RGB image was stretched, denoised with the MultiscaleLinearTransform tool, and then it was blurred with the Convolution tool.
10) The Luminance image was then combined with the starless RGB image using the LRGB Combine process tool.
11) I started using a new set of PixelMath expressions to create and then blur color masks that seem to produce better masks than the Color Mask script. The LRGB starless image was adjusted with several color masks (Yellow, Green, Blue, Cyan and Magenta) and the Curves and Histogram Transformation tools. The color mask PixelMath process icons can be downloaded from the lumatico YouTube channel at
(https://drive.google.com/drive/folders/138L6Z2vbTzNAutbfe5cuhL9Pl0-iltRp). Process Icon Merge was used to integrate these icons into my PixelMath_Comos workspace. First, a color mask is created using the stretched starless image. Next, the MaskBlur is applied to the new mask. Finally, the mask is applied to the starless image and the CurvesTransformation is used to adjust brightness, hue and saturation. Although the mask has been blurred, Curves have to be somewhat subtle to prevent the creation of color artifacts.
12) The starless image was saved as 16-bit TIF and then opened in Photoshop 2022 to selectively sharpen (sharpen tool), dodge and saturate (sponge tool) different regions of the image.
13) The starless and stars images were combined in PixInsight using the PixelMath combine function with the op_screen() option [ combine(stars,starless,op_screen()) ]. Note that there are far fewer stars, and they are somewhat dimmed so that they do not overwhelm the nebula. There are some minor color artifacts on the edges of the stars that may have been created with the Ha, Oiii and Sii stars images, their combination or color calibration.

Imaging details:

Celestron 9.25" Edge HD SCT
Celestron 0.7x Focal Reducer (FL = 1645mm, f/7)
Celestron off-axis guider with a ZWO ASI 174MM mini guide camera
Losmandy G11 mount with Gemini 2
ZWO ASI 2600MM Pro cooled monochrome camera (-10oC)
ZWO 36mm Hydrogen-, Oxygen-III and Sulfur-II filters

Software: Sequence Generator Pro, ASTAP plate solving, PHD2 guiding,
Losmandy Gemini ASCOM mount control and web client interface,
SharpCap Pro for polar alignment with the Polemaster camera.
Software for image processing on a Macbook Pro:
PixInsight 1.8.8-12, StarXTerminator for PixInsight, and Photoshop 2022

Hydrogen-a 10 min x 21 subframes (210 min), Gain 100, Offset 68, 1x1 binning
Oxygen-III 10 min x 16 subframes (160 min), Gain 100, Offset 68, 1x1 binning
Sulfur-II 10 min x 15 subframes (150 min), Gain 100, Offset 68, 1x1 binning

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SH2-101 the Tulip Nebula in Cygnus, Mark Wetzel