With BRESSER, you can enjoy a smooth introduction to the vast world of astronomy. Our detailed information ("Telescope Guide") provides valuable tips for beginners—but even experienced astronomers can use the information we provide (e.g., tables for the geographical latitude of all major world cities) as a reference.
Here is the table of contents of the comprehensive BRESSER Telescope Guide:
The Sky Guide provides comprehensive information on constellations, planetary positions, and astronomical events – perfect for planning your observations and delving deeper into astronomy.
Visit the guide directly here to make the most of your observations!
Product information "Vixen Carrying Handle for Telescopes"
Practical carry handle for telescopes
Designed for VC, VMC and refractor telescopes
Note: Please check the correct length of the mounting screw before assembly
FEATURES
Designed for VC, VMC and refractor telescopes SD81, SD103s, SD115s, A80M, A105MII Not suitable for A70Lf, A80Mf, VSD 100 and R103Sf
The optics of the VMC260L surpass the traditional Schmidt-Cassegrain and this tube is only 650 mm in length, despite its long focal length of 3000 mm . With its large aperture of 260 mm , the telescope collects light for serious professional observations and photography of the planets, as well as countless deep-sky objects. The dielectrically coated mirrors of the VMV260L guarantee high sharpness and maximum brightness. Thanks to the open tube, this instrument cools down faster than conventional closed Cassegrain systems, and (having no front corrector plate) is not as prone to dewing issues either.An optional 0.62x focal reducer is available for expansion to reduce the focal ratio to 1: 7.1. This results in a shortening of the exposure times and the increasing the field of view, thus increasing the ability to photograph larger objects in the sky. Included accessories feature a finder, dovetail rail and a handle that assists considerably when mounting and de-mounting the scope and can also be used as a camera holder for star field recordings.CHARACTERISTICSAperture: 260 mm precision spherical mirror, multi-coatedLight gathering power: 1380xAdapter and connections: 60 mm on the focuser; 42 mm for T-mount and 31.7 mm with folding mirror; 50.8mm optionPhotography: primary focus and eyepiece projectionWHAT'S INCLUDEDVMC260L reflectorDovetail rail (3 inch for AXD)AXD SaddleplateCarrying handleFinderscope 7x50Flip mirror
The optics of the VMC260L are significantly better than the traditional Schmidt-Cassegrain telescope. Despite its high 3000 mm focal length, it is just 650 mm long.
Featuring a large 260 mm aperture, the telescope collects large amounts of light for serious professional observations and photography of the planets and countless deep-sky objects.
Thanks to the dielectric mirrors, the VMV260L guarantees razor-sharp images and maximum brightness.
The open lens barrels cool the telescope quicker than conventional closed Cassegrain systems.
The telescope can be used with an optional 0.62x focal reducer to reduce the aperture ratio to 1:7.1. This shortens the exposure times and allows you to photograph large objects. The telescope comes with a standard dovetail bar and a carry handle that doubles up as a camera holder for night sky photography. The Finder Scope and the Vixen Flip Mirror is not included in this version !
FEATURES
Very short cool-down time thanks to open lens barrel
Optimised system for photography
Very transportable – only 650 mm long
Lightweight design – only 12.1 kg
Large 260 mm aperture
Built-in correction lens in front of the secondary mirror
Backfocus without Reducer: 149,4 mmBackfocus with Reducer: 63,5 mmTotal weight: 12.1 kg
WHAT’S INCLUDED
VMC 260 telescope/lens barrel
Carry handle
VIXEN standard dovetail barFinder Bracket ShoeEA60 mm to 50.8 mm SX
Astrophotographers generally use two different focal lengths: Short focal lengths for overview photos and extensive deep-sky objects, and long focal lengths for objects which are further away. Our aspherical mirror optics offer the perfect solution for these scenarios. The VISAC primary mirror (Vixen Sixth-Order Aspheric Cassegrain) is specially designed for astrophotography and provides a fully flat and true-colour image over the entire image frame. Thanks to the three-element field corrector in front of the convex secondary mirror, there is no spherical aberration, coma or field curvature. Although the device is designed for astrophotography, it is also suitable for visual observations.
FEATURES
Photographically optimized thanks to field flattener lens
Revolutionary coating technology
High light-gathering power
Photographically optimised optical system
Built-in field flattener lens
200 mm aperture and 1800 mm focal length
Optional reducer availableBackfocus without Reducer: 142,9 mmBackfocus with Reducer: 63,5 mmWeight: 6.9 kg
DELIVERY CONTENT
VC200 reflector telescope
Carry handle
7x50 finder scope (illuminated)
Flip mirror
Dovetail adapter
The Vixen SD103SII Telescope OTA is a new 103 mm apochromatic refractor with high-performance Super-ED glass (= SD). The advantage of this SD refractor is its short length and low weight. The FPL53 glass reproduces an extremely clear and sharp image by an exceptionally high degree of elimination of residual chromatic aberrations. The SD glass is designed to bring all beams of violet, red, blue, yellow and green very precisely together on the same plane. The special lens material reduces chromatic aberration across all colours.The new Vixen SD103SII no longer uses spacer plates, which leads to a significantly better image quality, especially with bright stars. In photographic images, no spikes can be seen on the stars, which were otherwise produced by the spacer plates. In addition, you will be thrilled when you look at the moon or the brighter planets and observe the moon craters pin sharp as well as with extremely high contrast. Also look at the ring planet Saturn or the cloud bands on Jupiter. But of course, brighter deep sky objects such as the Orion Nebula or the Andromeda Galaxy can also be observed in impressive detail.In combination with the new optional SD Reducer HD Kit or SD Flattener HD, these refractors allow illumination with a 44 mm image circle for full format SLR cameras. The older ED81SII, ED103S, ED115S refractors were originally developed for visual observers and photographers using APS-C cameras. However, the new SD series is also optimised for use with full-frame cameras through the use of new inner baffle rings. The large 60 mm eyepiece extension also allows heavy cameras to be attached without tilting. Furthermore, the included folding mirror allows comfortable observation even in unfavourable observation situations and additionally offers a T2 thread for connecting a DSLR camera. This allows you to observe in straight line or at a 90° angle. The carrying handle attached to the tube clamps ensures a secure grip when transporting the telescope. FEATURESObjective lens: D=103 mm, multi-coated 2-lens SD apochromat without spacer plates No more spikes on the stars Focal length: 795 mm (f7.7) Resolution and limiting magnitude: 1.13 arcseconds; 11.8 Light gathering power: approx. 217x more than the human eye Dimensions and weight: 115 mm dia x 810 mm; 5.5 kg Viewfinder telescope: 7x50 illuminated Adapters and connections: 60 mm thread, 50.8 mm and 31.7 mm socket, thread for T-ring Connection: 50.8 mm and 31.7 mm socket with flip mirror / folding mirror Photography: primary focus and eyepiece projection SCOPE OF DELIVERY Refractor SD103SII Telescope (OTA) Tube clamp with dovetail Dew cap Flip mirror / folding mirror Carrying handle Dovetail rail 7x50 viewfinder
SXD2WL SD115SII Complete Telescope Set with GoTo Mount, Tripod and EyepiecesThis high-quality apochromatic refractor telescope-set impresses with its 115-mm-SD optics. The telescope is made in Japan and scores with its excellent workmanship, sharpness, and contrast performance. The advantage of this
SD refractor lies in its light
weight and very color-true and high-contrast imaging. You will be amazed when you use it
to observe the moon surface with its craters or Saturn with its
ring system. On Jupiter, on a good night, you can also see the two bright cloud bands and many smaller details as well as the great red spot on the planet. On moonless nights, you can observe the Andromeda Nebula, Orion Nebula, Eagle Nebula, Lagoon Nebula and many other interesting objects. Even weaker celestial objects become visible with this large aperture of 115 mm under a good sky.This telescope set "Made in Japan" leaves nothing to be desired. The FPL53 glass used in the telescope reproduces an extremely clear and sharp image
due to exceptionally high elimination of residual color errors. The
SD glass is designed to bring all rays – violet, red,
blue, yellow, and green – very precisely to the same level. The
special lens material thus reduces chromatic aberration across all colors. In the new Vixen SD115SII, no spacer plates are used anymore, which leads to a significantly better image quality especially with bright stars. Consequently, no spikes are seen on the stars in photographic images, which would otherwise be caused by the spacer plates.In combination with the optional SD Reducer HD Kit or SD Flattener HD (not included), this refractor telescope enables illumination with a 44-mm image circle for full-frame SLR cameras. The older ED81SII, ED103S, ED115S refractors were originally developed for
visual observers and photographers with APS-C cameras.
However, the new SD series is also optimized for use with full-frame cameras due to the use of new internal diaphragms. The large 60-mm eyepiece holder also allows the attachment of heavy cameras without tilting. Furthermore, the supplied flip mirror
allows comfortable observing even in unfavorable viewing conditions and
also provides a T2 thread for attaching a DSLR camera. So
you can observe at an 90° angle or directly. The carry handle attached to the tube clamps provides safe handling during transport of the telescope. The sturdy metal tripod allows vibration-free mounting of the telescope and mount even in windy conditions. The SXD2WL mount is simply operated via a Wifi module with a smartphone or tablet . For user-friendly control of the mount, the free app STAR BOOK Wireless is available. This allows you to use practical celestial navigation functions like the automatic GoTo swiveling to specific celestial objects simply via your smartphone or tablet. Since the power consumption of the traditional LCD screen (STAR BOOK TEN) is eliminated, the power consumption of the mount is reduced by up to 20%. This enables astronomical observations and astrophotography over longer periods.
When you tap the desired celestial object from a list, it is automatically swiveled into the telescope's field of view and tracking begins. An existing STAR BOOK TEN control can also be used on this mount without any problems. Equipped with the same precision stepper motors as the top model, the AXD mount, the SXD2WL sets a new standard for performance and precision in the Vixen mount family.
The axis cross of the mount is with a photographic carrying capacity of 15 kg just 9.2 kg light and thus excellent for mobile observations . Moreover, the motors located in the lower part of the mount also act as counterweights. This reduces the need for additional counterweights.
The SXD2 Mount in Detail
Precision stepper motors and Micro-Step-Motion-Control system
The heart of the SXD2 are the precision stepper motors, which offer better performance and response than previous models. The Micro-Step-Motion-Control system boasts powerful yet very quiet drive properties, which are present both in fine movements and in fast swivels.
Built-in bearings
The bearings of the RA and DEC axes and the worm shafts have been significantly improved to reduce the load on the motors. As a result, the motors move much quieter than in previous models.
High-precision worm gears
High-precision processing technologies eliminate errors in the worm gears. The edges of both worms and worm wheels are particularly smooth, enabling very precise tracking.
Declination axis as counterweight
The massive motor units are built into the lower part of the declination axis, so the center of gravity of the SXD2 is below the intersection of the RA and DEC axes. This means you need fewer additional counterweights.
Latitude adjustment
The latitude can be adjusted between 0 and 70 degrees (divided into 3 zones and adjustable +/- 15 degrees per zone, for high, medium, and low latitudes); latitude scale in 2-degree steps; fine adjustment with a tangent screw head, approx. 0.8 degrees per rotation.
Built-in PFL-II polar finder with illumination
The built-in 5x20-mm polar finder with a 10° field of view features a 3-star alignment system.
This eliminates the tedious setting of date and time. The illuminated reticle with variable brightness and automatic shutoff is adjustable in 8 levels and is red illuminated. The adjustment accuracy is 3 arc minutes.The Wireless Module in Detail
The Vixen WiFi Adapter for EQ mounts enables you to control your Vixen mount via a smartphone or tablet. This allows you to navigate the skies wirelessly using the STAR BOOK Wireless app (free), instantly transforming your mobile device into a controller for the equatorial mount. The response delay of the mount, a major drawback of wireless connections, has been reduced to a level comparable with wired solutions.
Reduced power consumption compared to conventional controls with LCD monitors
The power consumption of the mount is reduced by up to 20%, thus allowing for longer observation periods than with conventional wired controls such as the STAR BOOK TEN.
Operation similar to the STAR BOOK TEN controller
The STAR BOOK Wireless App is structured similarly to the STAR BOOK TEN controller you might already be familiar with. Depending on the star chart settings, it includes up to 259,000 celestial objects. Simply tap on a celestial object in the object list to start the GoTo. The mount then automatically moves to this target and positions it within the telescope’s field of view. All the popular features of the STAR BOOK TEN are retained.
Convenient operation
While looking through the telescope, you control the mount by swiping on the app’s star map. With no buttons required, you simply glide your finger over the star map, allowing for easy operation of the mount.
Comprehensive astronomical data included
This includes data on easily observable celestial bodies such as Messier objects, NGC objects, IC objects, as well as the sun, moon, planets, comets, and dwarf planets.
High-precision alignment
Aligning with one or two stars already provides a fairly accurate positioning of the mount. Aligning with three or more stars allows for high-precision alignment of the mount for high magnifications. The objects are then precisely centered in your telescope’s field of view. The alignment information is stored and can be retained even when the device is turned off. By leaving the telescope in its current state after observing, without moving it, you can start the next observation with the automatic setup using the same settings.
Individual setting options
Like the STAR BOOK TEN controller, the app offers various individual settings such as backlash compensation, red night mode, autoguider, as well as variable GoTo speed and LED brightness. You can also set the timing of the objective tube reversal (Meridian Flip) as desired. Even if the object moves south during tracking, you can prevent the telescope tube from reversing.Important Information
Not usable on old SX mounts with the old blue Star Book
Technical Information on the Wifi Module
CPU with a 32-bit CISC processor at 120 MHz
The unit connects to the mount with a D-SUB 9PIN connector, as with the STAR BOOK TEN.
It features a 6-pin 6-wire modular plug for external autoguider operation.
Supported operating systems include Android 6 or later, iOS 9.0 or later, WLAN standard: IEEE 802.11b/g/n
FEATURESSD115SII TelescopeLens: D=115 mm, fully multi-coated2-lens SD apochromat without spacerNo spikes on starsFocal length: 890 mm (f7.7)Resolution and limit magnitude: 1.01 arc seconds; 12.1Light gathering capacity: approximately 270x that of the human eyeDimensions and weight: 125 mm dia x 930 mm; 4.4 kg without accessoriesFinder scope: 7x50, illuminatedAdapters and connections: 60 mm thread, 50.8-mm and 31.7-mm sleeve, T-ring threadConnection: 50.8-mm and 31.7-mm sleeve with flip mirrorPhotography: Primary focus and eyepiece projection
SXD2WL Mount
RA gear: 180 teeth
DEC gear: 180 teeth
Axle material and diameter: Carbon steel / Dec. 35 mm, RA 40 mm thickness
Polar finder scope: 6x20 mm, PFL-II polar finder
Altitude fine adjustment: 0° to 70°, (fine adjustment +/- 15°, height)
Counterweight bar: 20 mm diameter
Azimuth adjustment: worm gear fine adjustment
Power supply: DC12 V; 0.4~1.7 A
Maximum load: 15 kg, photographic, without counterweight
Counterweights: 1x 1.9 kg and 1x 3.7 kg
Mounting: 45 mm spigot
Dimensions: 36 cm (H) x 12 cm (W) x 36 cm (L)
Weight: 8.8 kg (19.4 lb), without counterweight
32-bit CISC processor 120 MHz
Operating system: Android 6 or higher, iOS 9.0 or higher
Connection: D-SUB 9PIN plug
Autoguider input ST4
Power consumption SXD2WL+Wireless unit: DC12V / 0.3–2.0 A (load 10 kg), 0.4–2.2 A (load 15 kg)
SCOPE OF DELIVERYSXD2WL MountWireless UnitCounterweights: 1.9 kg and 3.7 kgPolar finder scope, illuminatedMounting toolsCar lighter cableSD115SII Refractor TelescopeFlip mirror2 eyepieces (SLV 20, SLV 5)Tube clampsDovetail plate7x50 finder, illuminatedSXG Aluminium tripod
A new 81 mm apochromatic refractor with high-performance Super ED glass (= SD). The advantage of these SD refractors is their short length and low weight.The FPL53 glass reproduces an extremely clear and sharp image due to an exceptionally high elimination of residual colour errors. The SD glass is designed to bring all rays of violet, red, blue, yellow and green together very precisely on the same plane. Thus, the special lens material reduces chromatic aberration across all colours.The new Vixen SD81SII no longer uses spacer plates, which leads to significantly better image quality, especially with bright stars. This means that there are no more spikes on the stars in photographic images, which were otherwise produced by the spacer plates. You will be thrilled when you look at the moon or the brighter planets and observe the moon craters pin sharp and with an extremely high contrast. Observe the ring planet Saturn or the cloud bands on Jupiter.But of course, brighter deep sky objects such as the Orion Nebula or the Andromeda Galaxy can also be observed impressively.In combination with the new optional SD Reducer HD Kit or SD Flattener HD, this refractor allows illumination with a 44 mm image circle for full-frame SLR cameras.The older ED81SII, ED103S, ED115S refractors were originally designed for the visual observer or the photographer using APS-C cameras. However, the new SD series has been optimised for use with full-frame cameras by inserting new inner baffle rings.The large 60 mm focuser allows heavy cameras to be attached without tilting. The supplied flip mirror allows comfortable observation, even in unfavourable observation situations, and also offers a T2 thread for connecting a DSLR camera.Thus, observing in degree view or at a 90° angle is possible. The carrying handle attached to the tube clamps ensures a secure hold when transporting the telescope.FEATURESObjective Lens: D=81 mm, multi-coated 2-Lens SD Apochromat without spacer plates No more spikes on the stars Focal Length: 625 mm (f7.7) Resolution and visual limit: 1.43 arcseconds; 11.3 Mag Light gathering capacity: 134x unaided eyesDimensions and weight: 90 mm dia x 585 mm, 3.6 kg Finderscope: XY Red Dot Finder II Adapter and connections: Adapter thread 60 mm and 31.7 mm for T2-ringConnection 50.8 mm and 31.7 mm socket with flip-mirror diagonal mirrorPhotography: primary focus and eyepiece projection SCOPE OF DELIVERY Refractor telescope SD81SII Tube rings Flip mirror system Carrying handle Dovetail rail Red dot viewfinder
Smartphone holder with spring clamp for holding standard smartphones with a maximum housing width of 100mm. Original spare part for Bresser Messier telescopes. Colour white.
Take photos with your smartphone through your spotting scope, microscope or telescope. It’s a child's play with the BRESSER Universal Smartphone Adapter. Simply attach the adapter to the eyepiece holder of your optical device and then use all together as a telephoto lens for your smartphone camera. Now you can shoot distant objects as if they were up close or take photos through a microscope.FEATURESuniversal adapter to assemble the smartphone to a spotting scope or telescopefor eyepieces up to 68 mm diameterfor smartphones with a width of 50-88mmSCOPE OF DELIVERYSmartphone adapterManual
The Vixen rigid Accessory Tray for HAL130 and Porta II Tripods offers practical storage space for eyepieces and various accessories.It also improves the overall stability of the tripod.The tray can be used on the HAL130 and SXG HAL 130 for GP and SX, as well as on the Porta II tripod.PROPERTIESFor eyepieces and various accessoriesIncreases the stability of the tripodsCan be used on HAL130, SXG HAL 130 and Porta tripodsWHAT'S INCLUDEDTray for tripodsScrew set
FEATURES
Carry case for Porta II and Mini Porta mounts
Length of the case can be easily adjusted via strapsFastening straps prevent the bag from slippingSeparate accessory bag for securing to the outside of the carry caseWith carry straps for carrying in hand or on shoulderZip fastener for quick and easy storagePadded compartment for the mount
DELIVERY CONTENT
Mount bag
Accessory bag
Vixen has developed a new generation of SX mounts for demanding observers and astrophotographers. The SXD2WL mount is simply operated via a Wifi module with a smartphone or tablet.
By controlling the mount with your smartphone using the free STAR BOOK Wireless app, you can easily use sky navigation functions such as automatic GoTo panning of celestial objects via your smartphone or tablet.
By eliminating the power consumption of the conventional LCD (STAR BOOK TEN), the power consumption on the mount is reduced by up to 20%, thus enabling longer astronomical observation and astrophotography. When the desired celestial object is selected from a list, it is automatically panned into the telescope's field of view and tracking begins. An existing STAR BOOK TEN controller can also be used on this mount without any problems.
Equipped with the same precision stepper motors as the top model, the AXD mount, the SXD2WL brings a new standard of performance and precision to the Vixen mount family. With a photographic load capacity of 15 kg, the axis cross of the mount weighs just 9.2 kg making it ideal for mobile observations. In addition, the motors mounted in the lower part of the mount also serve as a counterweight, so the mount requires fewer weights for balancing. The SXD2 mount in detail Precision stepper motors and micro-step motion control system At the heart of the SXD2 are the precision stepper motors, which offer better performance and response than previous models. The micro-step motion control system offers powerful and yet very smooth drive characteristics, which are given both in fine movements and in fast pans.
Built-in bearings
The bearings of the RA and DEC axes and the worm shafts have been significantly improved to reduce the load on the motors. As a result, the motors move much more smoothly than in previous models. High-precision worm gears
High-precision processing technologies eliminate worm gear errors. The edges of the two worms and worm wheels are particularly smooth, enabling very precise tracking.
Declination axis as counterweight
The solid motor units are installed in the lower part of the declination axis so that the center of gravity of the SXD2 is below the intersection point of the RA and DEC axes. This means you need fewer additional counterweights. Latitude setting
The latitude is adjustable between 0 and 70 degrees (divided into 3 zones and adjustable +/- 15 degrees per zone, for high, medium and low latitudes); latitude scale in 2-degree increments; fine adjustment with a tangent screw head, approx. 0.8 degrees per turn. Built-in PFL-II polar finder with illumination The built-in 5x20mm polar finder with 10° field of view has a 3-star alignment system.
This eliminates the inconvenience of setting the date and original time.
The illuminated reticle with variable brightness and automatic switch-off is adjustable in 8 levels and illuminated in red. The adjustment accuracy is 3 arc minutes. The wireless module in detail The Vixen Wifi adapter for EQ mounts allows you to control your Vixen mount via a smartphone or tablet.
With the smartphone app STAR BOOK Wireless (free of charge) you can navigate the sky without any cables.
The app turns your smartphone or tablet into a control unit for the equatorial mount in no time at all.
The response delay of the mount, which is considered the biggest disadvantage of wireless connections, has been reduced to a level comparable to wired connections. Reduced power consumption compared to conventional controllers with LCD monitor The power consumption of the mount is reduced by up to 20%, allowing longer observations than with conventional
wired controllers such as the STAR BOOK TEN. Operation similar to the STAR BOOK TEN controller. The STAR BOOK Wireless app has a similar structure to the STAR BOOK TEN controller.
Depending on the star map setting, it contains up to 259,000 celestial objects.
Tap on a celestial object in the object list and start the GoTo.
The mount will now automatically move to this target and bring it into the telescope's field of view.
All the popular features of the STAR BOOK TEN are retained Convenient operation When looking through the telescope operate the mount by swiping on the app's star chart. As there are no buttons, simply slide your finger over the star chart to operate the mount conveniently. Extensive astronomical data included In addition to data on easily observable celestial bodies such as Messier objects, NGC objects and IC objects, this also includes the sun, moon, planets, comets and dwarf planets. High-precision alignment By aligning the mount to one or two stars, you can already achieve fairly precise positioning.
By aligning the mount to three or more stars, you can achieve high-precision alignment of the mount for high magnifications.
The objects are then approached precisely and centrally in your telescope's field of view.
The alignment information is saved and can be retained even when the device is switched off.
By leaving the telescope in its current state after completing an observation without moving it, you can start the automatic installation with the same settings for the next observation. Individual setting options As with the STAR BOOK TEN control unit, the app offers various individual settings, such as gear backlash compensation, night mode in red,
autoguider and variable GoTo speed and LED brightness.
You can also set the timing of the reversal of the objective tube (meridian flip) as desired.
Even if the object moves to the south during tracking, you can prevent the telescope tube from reversing. Important note: Cannot be used on old SX mounts with the old blue Star Book! Technical information about the Wifi module: CPU with 32-bit CISC processor 120 MHz
The unit is connected to the mount via a D-SUB 9PIN connector as with the STAR BOOK TEN.
It has a 6-pin 6-wire modular plug for external autoguider operation.
Supported operating systems are Android 6 or higher, iOS 9.0 or higher, WLAN standard: IEEE 802.11b/g/n. FEATURESRA sprocket: 180 teeth DEC sprocket: 180 teeth Shaft material and diameter: Carbon steel / Decl. 35 mm, RA 40 mm thickness Polar finder scope: 6x20 mm, PFL-II polar finder Fine height adjustment: 0° to 70°, (fine adjustment +/- 15°, height) Backsight rod: 20 mm diameter Azimuth adjustment: worm fine adjustment Power supply: DC12 V; 0.4~1.7 A Maximum load: 15 kg, photographic, without counterweight Counterweight: 1x 1.9 kg and 1x 3.7 kg Tripod connection: 45 mm spigot Dimensions: 36 cm (H) x 12 cm (W) x 36 cm (L)
Weight: 8.8 kg (19.4 lb), without counterweight 32-bit CISC processor 120 MHz Operating system: Android 6 or higher, iOS 9.0 or higher Connection: D-SUB 9PIN connector Autoguider input ST4 Power consumption SXD2WL+Wireless unit: DC12V / 0.3-2.0 A (load 10 kg), 0.4-2.2 A (load 15 kg) SCOPE OF DELIVERYSXD2WL EQ mount Wireless unit 2 counterweights: 1.9 kg and 3.7 kg Mounting tools Pole finder PFL-II Cigarette lighter cable
Dovetail adapter with quick-release fastener for attaching various accessoriesEasy assembly and disassembly thanks to the quick-release fastenerThe adapter is compatible with thin mounting plates such as the ARCA-SWISS standard. The quick-release fastener of the mounting plate is clipped in from the side, making it easier to attach and remove small telescopes or camera accessories.Suitable for a wide range of different accessoriesThe M8 2-point attachment (35 mm spacing) makes it compatible not only with Vixen products, but also with many products from other manufacturers. The 1/4” standard camera thread in the centre allows for attachment to camera tripods and other equipment such as the SXP mount series.The long locking knob enables attachment to equatorial SXP mounts.Compatible equatorial mounts: SXP2 mount, SXP mountFEATURES Low-profile mounting plate (ARCA-SWISS standard) Screw: 1/4 inch screw hole Screw holes: 2x M8 hole (35 mm spacing) Can be used on: SXP, SXP2 equatorial mounts, VSD90SS Material: Aluminum alloy Dimensions: 87 x 55 x 15 mm Weight: 67 gSCOPE OF DELIVERY Dovetail adapter with quick-release fastener
Functional cookies are absolutely necessary for the functionality of the web shop. These cookies assign a unique random ID to your browser so that your unhindered shopping experience can be guaranteed over several page views.
Google Pay payments
Amazon Pay
Machine identifier:
Security token to identify the machine.
Stripe orig props:
Stripe referrer information.
Stripe orig props:
Stripe referrer information.
Private machine identifier cookie:
Security token to identify the private machine.
Private machine identifier cookie:
Security token to identify the private machine.
Private machine identifier cookie:
Security token to identify the private machine.
Site auth:
Stripe authentication cookie.
Site auth:
Stripe authentication cookie.
Site auth:
Stripe authentication cookie.
Stripe csrf:
CSRF token.
Stripe csrf:
CSRF token.
Stripe csrf:
CSRF token.
stripe-payments.stripe_pm.name:
stripe-payments.stripe_pm.description
stripe-payments.stripe_pm.name:
stripe-payments.stripe_pm.description
Osteraktion
PayPal payments
Cookie settings:
The cookie is used to store the cookie settings of the site user over several browser sessions.
Information on origin:
The cookie stores the referrer and the first page visited by the user for further use.
Payment provider (Stripe) session
Timezone:
The cookie is used to provide the system with the user's current time zone.
CAPTCHA integration
Payment provider (Stripe) session
Stripe:
The cookie is used by the payment provider to increase security when processing payments on the website.
Cache handling:
The cookie is used to differentiate the cache for different scenarios and page users.
Session:
The session cookie stores your shopping data over several page views and is therefore essential for your personal shopping experience.
Payment provider (Stripe) fraud prevention
Payment provider (Stripe) fraud prevention
CSRF token:
The CSRF token cookie contributes to your security. It strengthens the security of forms against unwanted hacker attacks.
Google Tag Manager debug mode:
Allows to run the Google Tag Manager in debug mode.
Activated cookies:
Saves which cookies have already been accepted by the user for the first time.
Allows Google to collect personal data for online advertising and marketing.
AWIN Tracking:
Affiliate marketing module which requires the use of cookies to confirm affiliate transactions.
Meta Pixel:
Cookie from Meta that is used for website analytics, ad targeting and ad measurement.
Microsoft Ads:
Cookie from Microsoft Ads that is used for website analytics, ad targeting and ad measurement.
Pinterest Ads:
Cookie from Pinterest Ads that is used for website analytics, ad targeting and ad measurement.
TikTok Ads:
Cookie from TikTok Ads that is used for website analytics, ad targeting and ad measurement.
YouTube video
Location maps:
We use OpenStreetMap as tile provider to show you visually the location of our stores and merchants.
Recently viewed products:
The cookie stores the most recently viewed products in order to suggest them on further product pages.
Wishlist
Customers also viewed:
The cookie stores the most recently viewed products in order to suggest them to other customers on product pages.
Cookies used for statistics and shop performance metrics.
Google Analytics
Conversion and usertracking via Google Tag Manager
Google Tag Manager:
Cookie from Google to control the advanced script and event handling.
Google Analytics:
Cookie from Google for website analysis. Generates statistical data about how the visitor uses the website.
Tracking cookies help the shop operator to collect and evaluate information about the behaviour of users on their website.
Matomo Tracking:
Tracking statistics for the optimization of user workflows. No personal data is stored.
Matomo:
The cookie is used to track website activity. The information collected is used for site analysis and to generate statistics.
Google Analytics:
Google Analytics is used for traffic analysis of the website. Thereby statistics about website activities can be created and read out.
Marketing cookies are used to display advertisements on the website in a targeted and individualized manner across multiple page views and browser sessions.
Google Advertising
Google Ads:
Advertising Targeting
Shopware Analytics is an analytics service for tracking shopping behavior on this webshop, provided by shopware AG (Ebbinghoff 10, 48624 Schöppingen, Germany) in joint responsibility (see also the data protection information). The legal basis for data processing is Art. 6 para. 1 s. 1 lit. a GDPR. If data is stored locally, please refer to our privacy policy for further details on data processing.
The recipient of the data is shopware AG and IT service providers. Technologies used include local storage. The collected data includes customer group, pages visited, click paths, date and time of visit, information about the end device used (resolution, resolution density, operating system), referrer URL, information about the browser used, locale, search queries, time zone. The purpose of data collection is for marketing, analysis, and statistical purposes.
Data processing takes place within the European Union. If you have any questions about data protection, you can contact the data protection officer at legal@shopware.com. Further information can be found at https://www.shopware.com/en/privacy/website.
Stored data:
Shopware Analytics adds the following information to your browser's local storage until consent is revoked: _swa_anonymousId (a unique identifier of the visitor), _swa_userTraits (user traits of the visitor).
To watch videos, you need to accept third-party cookies:
Facebook
Vimeo
Cookies
We use cookies to personalise and improve content and services, deliver relevant advertising and provide a secure experience. You can review your cookie controls at any time. Learn more about the use and control of cookies in our privacy policy.Imprint