Passer au contenu
IMPORTANT: Our store is located in Canada. All orders that include products manufactured outside of Canada or USA will be subject to tariffs and duties, regardless of the order value. US customers are responsible for all applicable duties and tariffs, and those will be billed by the carrier, except for the Lacerta upgrade kit, for which we collect them at checkout.
IMPORTANT: Our store is located in Canada. All orders that include products manufactured outside of Canada or USA will be subject to tariffs and duties, regardless of the order value. US customers are responsible for all applicable duties and tariffs, and those will be billed by the carrier, except for the Lacerta upgrade kit, for which we collect them at checkout.

Langue

Pays

Shelyak LISA Spectroscope (VIS)

par Shelyak
UGC SHK-PF0021V
Prix d'origine $4,987.00 - Prix d'origine $4,987.00
Prix d'origine
$4,987.00
$4,987.00 - $4,987.00
Prix actuel $4,987.00
Égalisation de prix!
  • Designed for spectroscopy of faint deep-sky objects
  • Fast optical design optimized for modern telescopes
  • Interchangeable slits to balance resolution and brightness
  • Mirror slit design for accurate target acquisition and guiding
  • Lightweight 1.4 kg chassis
En rupture temporaire
Info disponibilité
Livraison GRATUITE aux USA
  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • LISA Spectroscope (VIS)

    The LISA Spectroscope is a lightweight 1.4 kg instrument designed for the scientific analysis of faint celestial objects from comets to quasars. It features a 4 mm long slit and an optical system with custom-made components, enabling you to capture detailed spectra of targets like novae, supernovae, and the redshift of distant galaxies.

    Engineered for Faint Object Spectroscopy

    The LISA's optical path is specifically engineered for low-light targets. Its fast focal ratio makes it an ideal match for telescopes operating natively at f/5, or for Schmidt-Cassegrain and Ritchey-Chrétien systems paired with a focal reducer. This design maximizes throughput for challenging subjects such as faint variable stars or confirming planetary nebulae.

    With a resolving power of approximately 1,000, the LISA separates spectral lines with enough detail for serious scientific work. Its spectral range covers the entire visible spectrum and extends into the near-ultraviolet and near-infrared, providing broad coverage for a wide variety of astronomical targets.

    Mirror Slit and Interchangeable Slits

    Acquiring and holding a faint object on a narrow slit is a primary challenge in spectroscopy. The LISA incorporates a mirror slit that allows you to see the entire starfield, making it simple to accurately position your target. For long exposures, a C-mount guide port allows you to connect an autoguiding camera to maintain perfect tracking.

    To adapt to different targets and conditions, the LISA includes a standard set of four interchangeable slits (15, 19, 23, and 35µm). This allows you to prioritize high resolution for brighter objects or greater light throughput for the faintest targets. Additional specialized slits, such as wide or photometric versions, are available separately to further expand the instrument's capabilities.

    Standardized Telescope and Camera Interfaces

    The LISA connects to your telescope via a standard 2" nosepiece, which is included. This nosepiece can be removed to expose a female M42x0.75 T-thread for more rigid connections. The imaging camera also connects via a T-thread, with a backfocus of 54.9 mm to accommodate filter wheels and other accessories.

    The dedicated guiding camera port uses a standard C-mount thread with a 17.5 mm backfocus. For users of ATIK cameras, the LISA also includes a 13 mm T-thread extension ring to ensure the sensor is placed at the correct distance from the optics.

  • What kind of objects is the LISA Spectroscope designed for?

    The LISA Spectroscope is optimized for faint deep-sky objects. Its primary targets include comets, novae, supernovae, faint variable stars, distant galaxies, and quasars. It is an ideal instrument for pro-am research and scientific characterization of these challenging targets.

    What kind of telescope do I need to use the LISA Spectroscope?

    The LISA performs best with telescopes that have a fast focal ratio, around f/5. It can be used directly on instruments with this native focal ratio. For telescopes with longer focal ratios, such as most Schmidt-Cassegrains or Ritchey-Chrétiens (f/8 to f/10), you will need to use a focal reducer to achieve optimal performance.

    How do I keep a star centered on the LISA Spectroscope's slit for long exposures?

    The LISA Spectroscope features two key systems for this. First, its mirror slit allows you to see the starfield around the slit for easy initial positioning. Second, it has a dedicated C-mount guide port, allowing you to attach an autoguiding camera that sends corrections to your mount, keeping the target perfectly centered automatically.

    Can I change the resolution of the LISA Spectroscope?

    Yes. The LISA comes with a set of four interchangeable slits of different widths. Using a narrower slit provides higher spectral resolution, which is ideal for separating close spectral lines on brighter targets. A wider slit allows more light to pass through, which is better for capturing a signal on very faint objects at the cost of lower resolution.

    How would I use the LISA Spectroscope to study a supernova like SN 2023ixf in the Pinwheel Galaxy (M101)?

    For a faint target like a supernova in a distant galaxy, you would likely select one of the wider slits (e.g., 23µm or 35µm) to maximize light throughput. You would use the mirror slit to locate the supernova within M101 and position it precisely. For the necessary long exposures, an autoguiding camera attached to the C-mount port would be essential to ensure the target does not drift off the slit.

    Can I use the LISA Spectroscope with my 8" f/10 SCT?

    Yes, but you will need two accessories for optimal results. First, you'll need a focal reducer (e.g., 0.63x or 0.5x) to shorten your SCT's focal ratio to be closer to f/5. Second, for a secure mechanical connection to the SCT's rear cell, you will need a specific adapter like the Shelyak BA0027 variable T-adapter instead of the standard 2" nosepiece.

  • Slit Length 4 mm
    Weight 1.4 kg (without camera)
    Resolving Power ~1,000 (with 23 µm slit)
    Spectral Range 400 - 700 nm (extends to near-UV/IR)
    Aperture f/5
    Included Slits 15, 19, 23, 35 µm
    Telescope Connection 2" Nosepiece or M42x0.75 T-thread (female)
    Imaging Camera Connection M42x0.75 T-thread (male)
    Imaging Camera Backfocus 54.9 mm
    Guiding Camera Connection C-mount
    Guiding Camera Backfocus 17.5 mm
    • LISA Spectroscope

      × 1

    • Interchangeable Slit Holder with 4 Slits (15, 19, 23, 35µm)

      × 1

    • 2" Telescope Nosepiece

      × 1

    • 13mm T-thread Extension Ring (for ATIK cameras)

      × 1

  • Shelyak 1-Year Warranty