Practice
Since 2013 I use a 10Micron GM1000 HPS for astrophotography. Since then I used the mount with a 8″ Vixen VC200L, a 4.5″ Newton and a 10″ Lacerta Newton. I take all my astronomical images from my balcony. The telescope and the GM 1000 HPS are mounted each time on a fixed pillar, which takes about 15 minutes. The setup and the actual pole adjustment of the GM 1000 HPS take another 20 minutes. During the entire night of observation no new adjustments to the mount are necessary. The annoying and time-consuming setup of an autoguider is no longer necessary. So far, all astro shots have been taken unguided, the photographic use without autoguider is an invaluable advantage, I can use every minute of the observation night time. Even a Meridian Flip is no problem, you can immediately start another exposure series.
Mount
The weight of the mounts is 19.5 kg. In addition, there is the screwable counterweight shaft with 1.5 kg and counterweights with 3 kg (small) and 6 kg (large). All parts of the high-quality processed mounting body are made of milled stainless steel and aluminium. The surface is glass bead blasted and black hard anodized. The construction is uncomplicated. First the base adapter flange is installed. This takes up the entire pole block of the GM 1000 HPS. The mount is fixed with four knurled screws ( M6 ) in oblong holes. Two opposing screws press on a pin located at the rear end, thus allowing the mount to be rotated to the west or east. The mount block is massively worked out, the latitude range can be adjusted very exactly and sensitively with the help of a large adjusting screw and a real worm wheel section in the mount block. A spirit level is also visibly integrated. The axes of the R.A. and Decl. unit are equipped with slipping clutches, the movement of which can be adjusted with two clamps each. At the upper end of the declination axis, there is a special dual dovetail adapter plate milled from one piece with two solid clamping pieces for holding telescopes. It adapts 3″ Losmandy and 44 mm (Celestron, Vixen) dovetails. The motor/encoder/gear units are completely encapsulated in metal and all motor and encoder cables are invisibly laid internally.
Mechanics
The GM 1000 HPS (High Precision and Speed) is conventionally driven by worm and worm wheel with the help of AC servo motors. The worm wheels are made of bronze, while the worm and the axle themselves are made of alloy steel. In addition to the usual motor encoders, the rectascension and declination axis is equipped with high-precision absolute encoders, which are calibrated with more than 10 million measuring points. The QCI control evaluates this information almost in real time and, if necessary, executes it and will make a correction immediately. With the combination of two electronic control loops per axis, the GM 1000 HPS combines the advantages of a conventional mounting (self-locking gear, high holding force during load changes) with excellent tracking accuracy even without autoguiding. Errors that occur between motor and axis encoders, such as inaccuracies in the mechanics, deflections, etc. are recorded and compensated. The mount also always detects its position with the greatest accuracy, even if the axes are released manually. The disadvantage of this mounting method is the worm error occurring in worm gears despite the most precise processing, which is reduced in the HPS mounting to up to +/-0.25″.
The GM 1000 HPS has a completely independent control system with a Linux-AMD-processor. The system is computer independent. It consists of the actual motor control and a hand box with a two-line display. The handbox is provided with a padded cover, which has a transparent window on the front side. The entire software is already installed, the device is immediately ready for use after a boot time of about 1 minute. Only a cable at the back of the right ascension motor connects the mount with the control box by means of a waterproof screwable plug. The QCI control offers a number of special functions for astrophotography, such as various electronic alignment algorithms, electronic balancing, storage of pointing models. (see technical data). In addition, the software can be updated via Internet updates.
A/D Gain: 0.37 e- / ADU unbinned
Read Noise: 9.3 e-rms
Cooling: Single stage thermoelectric (-35°C from ambient)
Filter Wheel: FW8-8300
Filters: Baader LRGBSllOlllHα (7 nm)
Connections
– R.A. and Decl. motors
– ST4-Autoguiderport
– RS-232-Port (control via planetarium software possible)
– Ethernet port
– GPS-Port
– hand box
– external contact for switching the mount on and off
– Additional auxiliary input (AUX)
– Power supply (24 V)
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