Title: Getting Started in CCD Imaging
1Getting Started in CCD Imaging
- An Overview by Alan Chen
- Member of
- CFAS Central Florida Astronomical Society
- Chiefland Astronomy Club
2Agenda
- Hardware
- The scope
- Optics
- Mount
- About Periodic Error
- The camera
- Choices
- MX7C - my first camera
- SXV-H9C - my second camera - a loaner
- Software choices for imaging/processing
- Basic imaging steps
- Some Images
3Hardware The Scope
- The choice of telescope is as important as the
choice of camera - Important factors The optics
- Choose a scope with the best optics you can
afford - Investigate on-line the pros and cons (i.e. Yahoo
Groups) - How color free is the scope (i.e. achro vs. APO)
- How flat is the field - this is important if the
cameras chip is large (i.e. gt10mm or you intend
to use film) - RC and refractors are best, but expensive
- Fast Newts and focal reduced SCTs have more
curvature - Amount tolerable depends on cameras chip size to
be used - Dedicated field flatteners will help, but adds
glass and cost - How large and heavy is the scope - easy to setup?
4Hardware The Scope
- Important factors The mount
- The mount should be rated to handle at least 1.3x
the maximum amount of weight you intend to carry - Allows a degree of stability margin
- Total includes the scope, guide scope, scope
brackets, dovetails, camera(s), and accessories
(camera adapters, dew heaters, etc.) as part of
the total weight - Most popular scopes are packaged with mounts
- Meade LX and Celestron Nexstar series - the most
popular first choice for starting out - Fork mounts do not allow significant weight to be
added (only about 10 to 12lbs. with careful
balancing required) - Periodic error is higher, but can be guided out
if smooth
5Hardware The Scope
- Important factors The mount
- GEMS (German Equatorial Mount)
- The mount of choice for higher end imaging,
although at generally higher costs - Celestron has the new CGE series - not much data
out yet, but promises to be a step up from the
fork mounts at a competitive price to forks - Aftermarket GEMs provide an alternative
- Paramount ME (10000), Astro-Physics (4000 to
8000), Takahashi (3000 up), and Losmandy (2000
to 6000) are good examples of higher end mounts - The Vixen GP-DX is probably the best low cost
mount on the used market - Advantages are higher total weight capacity
(except for the Vixen GP-DX) and improved
Periodic Error (PE)
6Hardware The Scope
- Examples of fork and GEM mounts
7Hardware The Scope
- Periodic error or PE - what is this and why is it
important - PE is a measure of the fundamental error present
in the worm/gear assembly during tracking - Caused by machining errors, out of roundness in
either worm or main gear, particles/dirt, bearing
tolerances, etc. - Errors are typically reported in /- arc-seconds
- Typical mass produced mounts have errors that are
on the order of /-20 arc-sec or higher - High-end GEMs are typically specd at better than
/-5 arc-sec - PE is easily measurable with ccd camera and
tracking software (deviation from ideal tracking)
8Hardware The Scope
- Examples of Periodic error in arc-seconds
- PE for the Synta EQ6 (/-35) and Vixen Atlux
(/-10)
9Hardware The Scope
- Examples of Periodic error
- Losmandy G11 (/-12) and Takahashi NJP (/-5)
10Hardware The Scope
- Examples of Periodic error
- Losmandy Titan - right plot (measured with the
MX7C camera at approximately /-3.5)
11Hardware The Scope
- Periodic error
- Mounts with the smoother PE plots from point to
point and the smallest total errors will guide
better - Smoother lines means that there are no large
error jumps to guide out (no fast transients) - Smaller total error means fewer and smaller
corrections during guiding - This does not discount mass produced scopes for
imaging - For mounts with higher errors, use of shorter
focal length scopes or SCTs with focal reducers
will provide excellent guiding results and very
nice images - Most of my images with the LX200 were taken at
f/4
12Hardware The Scope
- In summary
- Choose a scope/mount combination that has good
optics and comes with a sturdy mount - An alternative is to buy the optical tube by
itself and an aftermarket mount if this fits your
budget - PE is an important factor if the scope is to be
used for imaging - High end mounts have low PE to allow higher
resolution imaging (i.e. at f/10 with a 12
scope) - Mass market scopes can do very well at imaging,
but may require focal reducers (SCTs) or shorter
focal length refractors to account for increased
PE
13Hardware The Camera
- Choosing the camera
- There are many options to begin imaging with
- Digital camera - easiest way to start
- Research the web for choices
- Nice results achieved with Olympus, Nikon and
others - SLRs coming into popularity (like the Canon D60)
but expensive - Webcam - excellent for planets (check QCUIAG
website) - True CCD version (not CMOS based)
- Philips Toucam Pro, Vesta Pro, Older
Logitech/Connectix - Video camera - i.e. StellaCam-EX
- Deepsky capable with integrating software
- True CCD camera for astro-imaging
- Utilizes the most sensitive chips for deepsky
imaging
14Hardware The Camera
- What makes a deepsky capable CCD camera?
- The chips employed are the most sensitive
available - Sensitivities range from about 50 to 90
efficient - For example 50 efficiency occurs when an
electron is generated for every 2 photons hitting
that pixel - There are other techniques to improve
sensitivity, including the use larger pixels,
incorporating micro-lenses on top of the pixel
(Kodak and Sony both use this technique) and back
illumination, where the photons hit the back of a
very thin chip to avoid being blocked by the
front side circuitry (Site chips) - The cameras employ active cooling of the chip
- Peltier coolers (like those in portable coolers)
are used - Cools the ccd chip to approximately 30C below
ambient - Primary purpose is to reduce the thermal noise of
the chip
15Hardware The Camera
- What makes a deepsky capable CCD camera?
- The newer cameras are all 16bit for the highest
quality images (65k shades of gray) - Resolutions are lower but catching up to digital
SLR (most common are 0.4 to 1.6 megapixels) - Unlike typical cameras, there are no built-in
lenses or other user adjustments to the hardware - Requires software to extract the image from the
camera - Requires software to control the camera
including - Exposure time
- Taking a sequence of exposures
- Guiding or tracking (with a guide camera)
- Cooling (if software controlled like the SBIG
line)
16Hardware The Camera
- True CCD camera
- Several major CCD camera vendors
- Apogee - high end cameras (i.e. more expensive)
- Utilizes SITE chips - very sensitive as a result
of back illumination - FLI - high end cameras (i.e. more expensive)
- Also utilizes back illuminated chips, but has
more inexpensive offerings as well from Kodak - SAC - very inexpensive to start with
- SAC8 the best choice, but requires parallel and
USB ports - Older models use vid cam technology for summed
exposures - Lacks strong software support, but still
relatively new
17Hardware The Camera
- True CCD camera
- Several major CCD camera vendors
- SBIG - probably the largest and most recognizable
- Wide range of cameras based on Kodak chips
- Excellent standalone autoguiders (STV, ST4)
- Starlight Express - excellent values for ccd
cameras - Wide range of cameras based on Sony chips
- Kits for Cookbook or Audine cameras are available
for those who are handy - All are good choices and span prices ranges for
all levels of imager (approximately 1000 to
10,000)
18Hardware The Camera
- Starlight Express - my choice!
- MX7C - why was this a good first choice for me?
- An excellent first camera
- Good chip size for starters and more advanced
imagers - Relatively simple to operate, especially for
color images - Affordable by CCD standards
- 750x582 resolution tops in its price range
- Small and compact - only 2 dia
- Light weight
- Balance kit not necessary for the LX200
- Approximately the weight of a good 2 eyepiece -
only 200 grams - Primary SBIG equivalent considered at the time
ST-7E
19Hardware The Camera
- Starlight Express
- MX7C - why was this a good choice for me (cont.)?
- One shot camera - color matrix filters - CMY
- Synthesizes RGB from the filtered signals
- Much less overall imaging time involved for color
- Color filter wheel not required
- Probably not as accurate a color balance as RGB
imaging - Color synthesis routines much improved recently
in Astroart - Self-guiding capability with Star2000 interface
- Uses the same chip for imaging and guiding (every
other interlaced row) - Sensitivity reduced by 50 as a result
- Full frame usable to locate a suitable guidestar
(convenient)! - Simple software interface to self-guide
20Hardware The Camera
- Starlight Express
- MX7C - why was this a good first choice for me
(cont.)? - USB output
- 6.47mmx4.83mm chip
- 752x580 resolution
- Small size (50mmx100mm)
- Light weight - 200 g
- MX716 - mono version
21Hardware The Camera
- Starlight Express
- Todays alternate choices I would consider
- MX716 - a sensitive and low cost mono camera -
the best value on the market today (1395) - SXV-H9 - first megapixel camera (2795)
- Extremely low noise/dark current
- Dark frame not used by many SXV imagers
- SXV-H9C - good sensitivity, especially for color
(2795) - Uses an RGBG (Bayer Matrix) - not CMYG
- Color resolution will be much improved
- Extremely low noise/dark current - dark frames
not required - Primary SBIG equivalent to consider ST2000XM
- Slightly larger chip and slightly higher cost
(3495) - Includes built-in guide chip - very convenient
22Hardware The Camera
- Starlight Express
- SXV-H9C - The camera Im currently using
- On loan from Adirondack Video and Astronomy for
me to try out
23Hardware The Camera
- Comparing the 2 one-shot cameras
- MX7C
- USB 1.1 output
- 6.47mmx4.83mm chip
- CMYG filter matrix - G used for luminance
- 752x580 resolution
- 8.6umx8.3um pixels
- Small camera size (50mmx100mm)
- Light weight - 200 g
- MX716 - mono version
- SXV-H9C (mega-pixel)
- USB 2.0 output
- 9.00mmx6.70mm chip
- RGBG filter matrix - G used for luminance
- 1392x1040 resolution
- 6.45umx6.45um pixels
- Small camera size (63mmx100mm)
- Light weight - 400g
- SXV-H9 mono version
24Hardware The Camera
- The SXV-H9C has improved color resolution
- Compare M27 (single 4 or 5 min. frame) - MX7C
(top), SXV-H9C (bottom) - only RGB, no Luminance
25Hardware The Camera
- The SXV-H9C has improved color resolution
- Close-up of the red frames
- New extraction technique in the works to improve
color resolution further
26Hardware The Camera
- The SXV-H9C uses an improved interface
- Simple hookup (shown w/optional guide camera)
- Only 2 connections - 1 to computer and 1 to AC
power
27Hardware The Camera
- Use a rigid coupling of camera to scope if
possible to minimize flexing - Left to right
- Camera
- T-thread spacers
- T-thread to SCT adapter
- Focal reducer
- SCT to 2 adapter
28Hardware The Camera
- Alternate method of coupling camera to scope not
as rigid using set screw arrangement - Left to right
- Camera
- Camera to 1.25 adapter
- 1.25 visual back
- Focal reducer
- SCT to 2 adapter
29Hardware Matching Scope and Camera
- General guidelines
- Sampling definitions
- Good seeing (i.e. lt2 arc-sec) can tolerate higher
sampling rates - Sampling rate (arc-sec/pixel) 206 x (pixel
size)/(focal length) - Pixel size is dependent on the camera
- FL can be varied by focal reducers and barlow
lenses - Rule of thumb scope and camera should provide a
typical sampling rate of between 1 and 3
arc-sec/pixel - 12LX200 _at_ f/3.3 1.7 arc-sec/pixel (good
match!) - Ratesgt2 is under-sampling and rateslt2 is
over-sampling - High resolution imagers use 1/3 to 1/4 the seeing
value to maximize resolution (i.e. down to 0.5
arc-sec/pixel!) - My advice - dont worry about sampling
- Excellent results can be achieved from 0.3 to gt7
arc-sec/pixel
30Software Choices
- Software comes in several flavors
- Bundled with camera
- Generally not as full functioned, but enough to
get started - All in one handles both image capture and
processing (2 main ones listed) - Astroart by MSB (179) - excellent value
- Maxim CCD/DL (365) - higher end package
- Processing only
- Maxim DL (285)
- Post processing (tweaks)
- Photoshop
- Corel Photo
31Basic Imaging Steps Taking the Image
- Imaging process
- Setup scope, camera, laptop and align
- No hot plugging - turn everything on after full
setup
32Basic Imaging Steps Taking the Image
- Choose and locate first object
- For LX200, slew to it using HPP (nice ccd
feature) - For other setups, manually locate or goto
- Focus on a nearby star when convenient
- Will get focus close before slewing to object
- Take a quick 10 sec shot
- Focus on a brighter star
- Setup guider (if applicable)
33Basic Imaging Steps Taking the Image
- Set the exposure time (240s in this case)
- Note the guide window and active tracking at the
top right - Image started with 240 seconds set - bar at
bottom left indicates exposure progress - The image will pop up on screen when completed
34Basic Imaging Steps Processing
- Use the processing software to complete the image
- Typical processing includes
- Stacking and aligning images if more than one
image is taken - Multiple images taken for increased total
exposure - Improves signal to noise
- Shorter images prevents saturation from light
pollution - Sharpening to improve object definition
- Median filtering to remove hot pixels (bright
dots) - Contrast and stretching to bring out fainter
details
35Basic Imaging Steps Processing
- Color processing - LRGB combined result
- This should approximate the final result
36Basic Imaging Steps Processing
- Color processing
- Use color balance and saturation commands to
further enhance the image - Flipped image for orientation
- Can tweak further in Photoshop and Corel
Photopaint
37Some Images M16 - The Eagle Nebula
38Some Images M27 - The Dumbell Nebula
39Some Images M22
40Some Images M22
41Some Images NGC5907
42Some Images NGC6992 - The Veil
43Some Images Mars
44Thanks for watching!Check out
http//www.heavenlyview.comfor more info on ccd
imaging and the latest images (in full size - the
ones used here were resized and cropped to fit
causing some resolution loss)