Getting Started in CCD Imaging

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Getting Started in CCD Imaging

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The Vixen GP-DX is probably the best low cost mount on the used market ... for the Synta EQ6 ( /-35) and Vixen Atlux ( /-10) 9. Aschen 10.19.03. Hardware: The ... – PowerPoint PPT presentation

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Title: Getting Started in CCD Imaging


1
Getting Started in CCD Imaging
  • An Overview by Alan Chen
  • Member of
  • CFAS Central Florida Astronomical Society
  • Chiefland Astronomy Club

2
Agenda
  • 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

3
Hardware 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?

4
Hardware 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

5
Hardware 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)

6
Hardware The Scope
  • Examples of fork and GEM mounts

7
Hardware 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)

8
Hardware The Scope
  • Examples of Periodic error in arc-seconds
  • PE for the Synta EQ6 (/-35) and Vixen Atlux
    (/-10)

9
Hardware The Scope
  • Examples of Periodic error
  • Losmandy G11 (/-12) and Takahashi NJP (/-5)

10
Hardware The Scope
  • Examples of Periodic error
  • Losmandy Titan - right plot (measured with the
    MX7C camera at approximately /-3.5)

11
Hardware 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

12
Hardware 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

13
Hardware 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

14
Hardware 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

15
Hardware 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)

16
Hardware 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

17
Hardware 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)

18
Hardware 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

19
Hardware 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

20
Hardware 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

21
Hardware 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

22
Hardware The Camera
  • Starlight Express
  • SXV-H9C - The camera Im currently using
  • On loan from Adirondack Video and Astronomy for
    me to try out

23
Hardware 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

24
Hardware 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

25
Hardware 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

26
Hardware 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

27
Hardware 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

28
Hardware 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

29
Hardware 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

30
Software 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

31
Basic Imaging Steps Taking the Image
  • Imaging process
  • Setup scope, camera, laptop and align
  • No hot plugging - turn everything on after full
    setup

32
Basic 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)

33
Basic 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

34
Basic 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

35
Basic Imaging Steps Processing
  • Color processing - LRGB combined result
  • This should approximate the final result

36
Basic 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

37
Some Images M16 - The Eagle Nebula
38
Some Images M27 - The Dumbell Nebula
39
Some Images M22
40
Some Images M22
41
Some Images NGC5907
42
Some Images NGC6992 - The Veil
43
Some Images Mars
44
Thanks 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)
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