Wanderer Astro White Dwarf Flat Panel
- Provides Uniform Illumination for Flat Frames
- Corrects Vignetting and Dust Motes
- Available in 5 Sizes for Telescopes up to 400mm
- Essential Tool for Astrophotography Calibration
Load a flat and find whether the dust is on the sensor, the camera window or a filter.
Analyze a flatThe Wanderer Astro White Dwarf is a lightweight handheld flat panel for astrophotography calibration, available in five sizes (150mm, 200mm, 250mm, 350mm and 400mm) to fit a wide range of telescope tubes and dew shields. Flat frames taken with it correct uneven field illumination and remove dust shadows from your final images.
Every astrophotography setup has a unique optical signature, including vignetting from reducers and dust particles on the sensor or filters. The Wanderer Astro White Dwarf Flat Panel is engineered to erase these flaws by producing a perfectly even field of light, allowing your camera to capture a "map" of your optical train's imperfections. This calibration frame, or flat, is the foundation of a clean, professional-grade astro-image.
Unlike inconsistent methods like sky flats or t-shirts, the White Dwarf panel delivers repeatable results any time, day or night. With five sizes available from 150mm to 400mm, you can select a panel slightly larger than the outer diameter of your telescope's tube or dew shield, so it covers the whole opening.
Choose a panel whose illuminated diameter is slightly larger than the outer diameter of your telescope's tube or dew shield, not its optical aperture. For example, Wanderer Astro's sizing guide puts a SharpStar 107PHQ, whose dew shield is 138mm across, on the 150mm size. Wanderer Astro also keeps an online flat panel size tool listing many telescopes.
While sky flats are a viable option, they are highly inconsistent. The sky's brightness changes rapidly, making it difficult to achieve the correct exposure, and weather can make them impossible to acquire. The Wanderer Astro White Dwarf Flat Panel provides a stable, repeatable light source you can use anytime, ensuring perfect flat frames for every imaging session.
The primary purpose of this flat panel is to create calibration frames that remove two main types of artifacts:
Yes. You should shoot your flat frames with the same gain and ISO as your light frames, but the exposure time will be different. The goal is to achieve a histogram peak that is roughly in the middle (around 50% of the maximum value) without clipping any data. The panel is very bright (less than 1 s for a 3 nm Ha filter at f/7), so broadband flats usually need much shorter exposures; set the brightness with the two voltage levels and the dimming knob.
Size the panel by the outer diameter of the tube or dew shield, not the 203mm aperture. The tube of an 8-inch SCT is wider than its 203mm aperture, so the 200mm panel is too small; measure your tube or dew shield and check it against the 250mm panel.
Yes, absolutely. Those dust spots are shadows on your sensor. By taking flat frames of a uniform light source with the Wanderer Astro White Dwarf Flat Panel, your processing software can identify those exact spots and mathematically remove them from your images of the Orion Nebula (M42), leaving a clean, artifact-free final result.
| Available Sizes | 150mm, 200mm, 250mm, 350mm, 400mm |
| Illuminated diameter | 150 mm / 200 mm / 250 mm / 350 mm / 400 mm |
| Power | 5.5 x 2.1 mm DC input |
| Brightness control | Manual knob, two voltage levels plus stepless dimming (about 10 stops) |
| Weight | 224 g (150mm), 341 g (200mm), 485 g (250mm), 800 g (350mm), 1050 g (400mm) |