1. Alan Holmes Founder and President New products at SBIG

2. SBIG is Now Part Of Aplegen New Management intends to: –increase astronomical product research and development –adds new cameras with features suited to life sciences applications such as: Gel Imaging Fluorescence microscopy New CEO is Ron Bissinger, known for amateur exoplanet measurements

3. Past SBIG Cameras over the last 23 years ST-4 (my baby) ST-6 ST-5/ 237/ PixCel 237 ST-7/ 8/ 9/ 10/ 2000 line STL-11000/ 6303/ 1001 line STX-16803/ 6303 ST-402/ 1603/ 3200 SG-4

4. New Camera Models in Last Year ST-I ST-8300 and STF-8300 STX-6303

5. ST-I is a new Guider/Planet Camera

6. ST-I Features 640 x 480 pixel interline CCD 7.4 micron square pixels Exposures as short as 1 millisecond 16 bit A/D converter 10 electrons read noise powered off USB port Shutter for automatic dark frames Fits in 1.25 inch eyepiece tube

7. ST-I Comes with a Case and Software

8. A Guiding package is Available that is all Most Users Need

9. Planetary Imaging is also Possible (Not the best but it ’ s mine!)

10. ST-8300 is our most Popular Camera Features –8.3 million pixels –16 bit A/D –38 degree C cooling –5.4x5.4 micron pixels - good for refractors –EXCELLENT low dark current –Just went on sale at a great price - $1795 US

11. 5 (and 8) Position Filter Wheels are Available

12. The ST-8300 is capable of Great Images! Peter Clausen

14. New STF-8300 Provides Faster Readout 10 Megapixels / Second Full Frame Image Buffer Readout and Download Simultaneously Download Full Frame < 1 sec. User Rechargeable Desiccant Plug Internal Image Processing – Raw or Processed Even-illumination (Photometric) Shutter 32-bit and 64- bit drivers for all Windows O/S Equinox Image and Equinox Pro for Mac Base Price $2495 US

15. STX-16803 is our largest CCD Camera 4096x4096 pixels 9 micron pixels Excellent Cooling

16. Martin Pugh

17. STX Images -Johannes Schedler - Austria M97-Owl Nebula (too far north for Santiago!)

18. More STX Images from Johannes NGC 5033

19. New STX-6303 is Excellent for Narrow Band Imaging and Faint Objects Adriana Sherman, Guatemala

20. New Accessory Products at SBIG Differential Guiding ST-8300 Off Axis Guider

21. Differential Guiding Solves a Difficult Problem When guiding at long focal lengths with a guide scope, the scope-to-scope alignment drifts due to: –Gravity direction changes –Thermal effects –mirror flop –mechanical shifts Differential guiding eliminates all of these

22. SBIG’s New Technique: Differential Guiding * An artificial star is created near the imaging CCD focal plane Beam of light from artificial star exits telescope Beam is retro-reflected into guide scope Guide scope views both artificial star and background star Separation of artificial and real stars is maintained by guiding * Patented

23. Differential Guiding Diagram Main Scope Guide Scope LED Guide Camera Retro- Reflector Imaging Camera

24. Guiding is Adjusted to Maintain X and Y Offsets Constant Guide Star Artificial Star X Y

25. Retroreflector is Derived from Corner Cube and Dove Prism Corner Cube Dove Prism Beam is exactly retro-reflected, and displaced to outside the telescope aperture. Retro-reflected angle is insensitive to small mechanical misalignments.

26. Testing was Performed in my Backyard

27. A Celestron Edge 14 was used for the Test

28. Retroreflector Assembly and Guide Scope (Hutech 50 mm F/5)

29. ST-8300 and Artificial Star Generator

30. Conventionally Guided Image - 30 minutes

31. Differential Guided Image - 3 x 30 Minutes - no Shifts!

32. It Works Great! (ST-8300C Data Added)

33. New Off-Axis Guider for ST-8300

34. Guider Ray Trace Diagram Allows guiding in front of the filters Also provides focal reduction for 2X more area Imager CCD ST-I CCD

35. It uses an ST-I and Mounts to Filter Wheel Low Profile – Adds only 19mm backfocus to camera and filter wheel (total about 58mm) Built-in relay lenses and 0.7X reducer doubles the field of view of the ST-i Guide camera can be mounted at 90 degrees x 4

36. St-I Guider Image at F/3.5! Stars are excellent for guiding

37. Celestron Edge 14 Image using OAG With ST-8300 Alan Holmes

38. OAG Makes Guiding Narrow Band Images Easy Peter Clausen

39. -Astrophotography Hints- Stray Light and Flat Fields

40. An Example of the Problem - An Expensive Refractor with an ST-8300 Center to edge variation = 6% There is NO vignetting in either image! “Hot Spot” is caused by glints off internal cylindrical surfaces near CCD Camera Green Flat FieldIR (940 nm) Flat Field

41. Measuring Stray Light: My “CCD View” Pinhole Camera Chamber window of ST-3200 replaced with a tiny lens View of my office through a short 1.25 inch nosepiece

42. Looking into that High-End Refractor Actual Aperture! Bad Stuff! Problem is glints off of “black” anodized surfaces. Total Stray Light is 8% Green, 18% IR

43. $5 Million Peso (!) RC Scope Green - 13% Stray LightNear IR - 37% Stray Light Aperture Edge

44. Why is this important? - Astronomical Features have very Low Contrast against the Sky Background 9% contrast 1% contrast (Images are from a Dark Site) Tony Hallas

45. Stray Light is also a Serious Problem for Photometry VignettingStray LightSum Using a flat field to correct an image with stray light incorrectly increases brightness of stars near edge of field (Looks like vignetting but it ’ s not)

46. A Collection of “Black” Objects Imaged at Near Infrared Wavelengths (940 nm) White Business Card Black Felt (79% reflectivity Black Paper Flat Black Paint

47. Flat Black Paint can solve this Problem - User Flat Field Images STL-11K - Flat Field with Moonlite Focuser and ribbed draw tube Flat field after painting draw tube with flat black paint

48. How to detect the problem yourself Point your telescope at a flat field screen Put your eye at the point where you usually insert the camera Look into the tube

49. What can you do? Paint black anodized surfaces Flat Black –I prefer barbeque black - low temperature paints may use dyes that are transparent beyond 700 nm Add thin shim rings to work as knife edges baffles Do NOT use incandescent bulbs for flat fields –Use white LEDS instead –Better, but still not perfect Sky flats may help - matches spectrum better for LRGB imaging Use flat field for each color if doing RGB images Photometrists should map response by moving stars around in field to detect problem

50. It is Worth the Effort! Tony Hallas

51. Particularly with Huge Mosaics (Rogelio Bernal Andreo - 19 APODs!)