| Order Line & Tech Support 888-427-8766 | |||||||||||||||
|
|
|
Saturn’s Opposition on March 21, 2010 Great viewing through June |
astrodon - NIR Tricolor - 50mm dia. NIRL Luminance
Goals
* Produce tri-color images entirely in the NIR
* Color combine weights for NIR1, 2, 3 are ~ 1:1:1.2.
* Examine objects highly obscured by dust in the plane of the Milky Way, such as the IC342/ Maffei group, that are difficult
to image at VIS wavelengths.
* Explore faint, extended red emission (ERE) nebula.
* Uncover stars and other details in nebula that are obscured by bright VIS emissions from H-a, SII, OIII or other elements.
* Mix NIR with RGB of globular clusters to enhance the appearance of cooler stars.
* Minimize terrestrial light pollution from sodium and mercury street lamps and oxygen skyglow for imagers living in suburban
or city locations
* Use the NIR luminance (no visible light) to explore galaxy structure in comparison to VIS luminance data.
Features
* 1.25" mounted, 50 mm diameter
* 3+/-0.05 mm thickness
* Parfocal with other Astrodon LRGB and Narrowband filters*
* NIR Luminance (>700 nm)
* NIR123 (700-800, 800-900, >850 nm)
* Set of 4 (NIRL123)
* NIR Luminance sold separately
* ~1:1:1 for KAF3200ME and similar detectors
|