Astrophotography acquisition and processing in Nebulosity


Nebulosity is an application for astrophotography - image acquisition and processing. It's not free, but it's very easy to use, and supports various cameras (Atik, QHY, SBIG, SX, FLI, QSI, Meade, Moravian... DSLR). For processing it offers at least full set of "basic" features (stacking with optional rotation or scaling, darks/flats/bias support, hot pixel maps, curves, levels, colour balance etc.). For acquisition it offers very handy and clean user interface.

Nebulosity UI - image acquisition

The main window looks like this:
Nebulosity main window
Most of the window is occupied by the image (last image from camera or current open image). On the right you will find controls for image acquisition and display.

"Display" box shows a histogram of the image. When using Nebulosity you have to look on it often... By default the Auto is checked and on the viewed image histogram will be cut to the signal level. This may surprise new users. Image at short exposure may look "bright", while the histogram is barely filled. If you disable the auto the histogram won't be cut for the preview (and you will see "real" brightness of the object on the image). Without histogram clipping the M57 frame from the first screenshot looks like so:

Nebulosity image preview without histogram clip

So the frame is underexposed. For 16-bit cameras the signal is saved as a value between 0 (black, no signal) and 65535 (white). When setting exposure time it's good to get as high histogram fill as possible (brightest objects close to the max value).

Below "Display" you will find "Capture Control" that handles camera settings - type, gain, offset, exposure time. Advanced button will allow modifying additional settings (like binning). Things like cooling may be set from the top menu ("Edit" -> "Preferences").

On the bottom of the column you will find few more buttons: You can also set Name label which will be used as a frame prefix (good thing is to mark object, filter used). When you capture all required frames (light, darks, flats etc.) you can proceed with processing those images in Nebulosity.

Processing raw frames

For processing the camera settings are of no meaning, but still - look at the histogram (and auto-clip checkbox). All the processing functions are in Batch and Image top menus.

Batch menu in Nebulosity 2
Batch menu in Nebulosity 2
In Batch we will find options such like frame stacking, bad (hot) pixel removal or dark/bias/flat execution on "light" frames (your images). Most important are: When you want to stack frames in Align and Combine Images then you have few options on how to do it:
Stacking options in Nebulosity
Save stack will make a stacked frame out of selected frames, while Save each file will copy and save all frames under new names - used when we want to align frames against each other and not stack them. Below that there are alignment options. None is used for darks, flats, bias frames (no custom alignment). Translation is the common method for stacking by selecting a star. If we have frames from different runs we can use Translation + Rotation or Translation + Rotation + Scale to align them correctly. Just choose the options and then select the frames. For all the Translations stacking you will have to choose one or two stars to align on:
Star selection when stacking

For stacking we need frames that have been "processed by" dark/flat/bias frames (if needed). To do that we have to stack and execute those frames before stacking the object frames. Stack dark/flat/bias frames with "None" alignment and then open "Pre-proces Color or BW Images". A window will show up asking to choose some of those special frames. When you select them you will be able to select raw frames on which they will be executed:
If the camera has some (or a lot) hot pixels then dark substraction may not be as good as needed. In Nebulosity you may create a Bad Pixel Map (using the dark frame or light frame if you don't have a dark), just look into Bad Pixels submenu. You make the map with "Make Bad Pixel Map" and then you can extract bad pixels from the dark frame and from raw images (to be processed with the processed dark frame).
Bad Pixels in Nebulosity

Processing stacked images

When you have the final stack of the astrophotograph you can process it with tools available in Image menu:
Nebulosity image processing options
The most basic processing may limit to editing level (clipping the histogram) and, or using one of pre-defined curves:
Editing levels may be used to limit the background strength and to make object brighter
Curves may increase contrast or brightness of some features on the image

Adaptive Median Noise Reduction may be used to limit the grainy noise. Deinterlace will be handy for removing interlacing given by interlaced CCD sensors (DSI II, QHY6, 6 Pro, Brightstar Lyuba 429 and others).

Creating RGB and LRGB images

To make a colour image out of monochrome R,G,B (or other) channels you need to process images for every channel. Then align them against each other ("save each file" in stacking window). After that from Image you can choose LRGB colour Synthesis. In the window you will be able to choose frames for RGB and optionally L channels.

Generated colour image may require colour balancing. Quickest and automatic path is to use Adjust Color Background and then Auto Color Balance.

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