Blink
Frames one after another — the classic view.Infrared time domain · synthetic demo
Find what
moves.
Blink through the infrared sky over time. Most stars stay put; the dot that jumps is worth investigating.
Infrared image sequences◆Six detectors◆Inspect what changes◆Export with provenance
The instrument
Four ways to look at the same sky.
Difference
Subtract frames so only changes survive.Stack
Median of the sequence — the still sky.Trail
Maximum of each frame — the moving path.Method
How blinking works.
- 01
Define a field
Choose right ascension, declination, field of view and detector, or start from a documented challenge target.
- 02
Play the sequence
Inspect the same patch of sky across different dates with blink, difference, stack and trail views.
- 03
Inspect what moves
Measure, compare, export and keep the provenance; a candidate remains a lead, not a discovery.
Preset fields
Start where the movers are.
Epsilon Indi B ↗
331.0441° · −56.7828°
Nearby brown dwarf binary; a documented Blink test target.
Barnard's Star ↗
269.4521° · +4.6934°
High proper-motion nearby star used to test the mover workflow.
WISE 0855 ↗
133.8189° · −7.2470°
Cold brown-dwarf target from the documented challenge list.
RW Aurigae ↗
76.9565° · +30.4014°
Variable young star in a star-forming region.
R Draconis ↗
248.1676° · +66.7550°
Mira variable in a wide challenge field.
Research workflow
A dot that jumps frame to frame is a candidate.
Use Find Movers to link bright dots across a sequence. The page reports motion, significance and each supporting detection, while keeping synthetic and observed inputs clearly labelled.
Run the workspace