Astronomical Data Collection and Processing of LLPVs in GGCs at the BGSU Observatory - PowerPoint PPT Presentation

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Astronomical Data Collection and Processing of LLPVs in GGCs at the BGSU Observatory

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Title: Astronomical Data Collection and Processing of LLPVs in GGCs at the BGSU Observatory


1
Astronomical Data Collection and Processing of
LLPVs in GGCs at the BGSU Observatory
  • J Leon Wilde

TAA Seminar, UT, February 2nd, 2007
2
Intro
  • Before observing
  • BGSUs telescope
  • CCD Imaging
  • Typical observing night
  • Image processing
  • My Thesis Work

3
Before observing
  • What to look at
  • Where to look from
  • What instruments?
  • 0.5 m Reflecting telescope
  • CCD imager

4
The telescope
Incoming starlight
Secondary Mirror
Primary Mirror
Focus on optics
5
The CCD Imager
  • Charge Coupled Device
  • Si diodes
  • KAF-1000E
  • Specs .pdf for
  • KAF-1001E

6
Why use CCDs?
  • High QE
  • High Linearity
  • Large dynamic range
  • Uniform response
  • Low Noise
  • Digital

7
Our CCDs QE
Blue KAF-1001E Black KAF-1401E
8
CCD Basic Design
  • Our CCD
  • 24x24 micron pixels
  • 1024x1024 array

9
Gate Structure/Function
  • Voltage push
  • Sends data to onboard amplifier and A/D converter
  • Our CCD
  • Two phase push
  • Charge transfer efficiency 0.99997

10
CCD illumination
  • Frontside
  • Photons pass through phasing gates
  • QE lower than Bs
  • Backside
  • Etched back
  • High QE
  • Hard to make, thus...
  • More expensive
  • Our CCD
  • Frontside

11
CCD Drawbacks
  • Noise!
  • Dark current
  • A/D conversion
  • CCD flaws
  • Worked out during processing
  • Expensive!
  • Delicate manufacturing process
  • Better science means higher standards

12
Dark Current
  • Thermal activity on CCD chip

13
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14
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15
CCD Linearity
SBIG ST8 Linearity Test
Pixel value (ADUs)
Integration time (seconds)
16
CCD Coatings
  • CCDs naturally insensitive to blue
  • Coatings used
  • Coronene Lumogen phosphors
  • Lumogen better of the two
  • Lumogen commercially used in highlighters
  • Our CCD
  • Blue Plus Transparent Gate

17
Blooming
  • Our CCD
  • No anti-blooming gates
  • Were careful! ?

18
Typical Night
  • Arrive an hour before sunset
  • Get equipment ready
  • Take bias frames / flat field frames
  • Observe!
  • Take more bias / flat fields
  • Send images to Dr. Laydens computer
  • Shut equipment down
  • Go home!

19
Image Processing
  • Correct the images
  • Optics arent perfect (dust donuts, vignetting)
  • CCDs arent perfect
  • Electronics arent perfect
  • Observers arent perfect
  • The problem exists between the chair and the
    computer.
  • Garbage in, garbage out.
  • Get science from the data
  • Convert relative values into real values
  • Programs
  • IDL and IRAF

20
Processing
  • Zero (Bias) frame
  • Remove floor value
  • Subtract combined image from data
  • Dark frame
  • Remove dark current
  • Subtract combined image from data
  • Flat field
  • Remove non-uniformities arising from
  • CCD flaws
  • Optics flaws
  • Divide combined image from data

21
Processing
  • Photometry
  • RR Lyrae Program, getting star magnitudes versus
    time
  • Pretty pictures
  • Combine images from different color filters

22
Pretty pictures
Ring Galaxy AM 0644-741 from Hubble
23
My Thesis WorkWhy Study LPVs?
  • Variability provides distance calibrations
  • LPVs are understudied
  • For SIM (Space Interferometry Mission)

24
Background
  • What are they?

25
Why look in GGCs?
  • Stars are of the same age
  • Stars are at the same distance
  • Stars are similar in composition

26
Detection
  • Acquire data over long enough time
  • Process images
  • Image subtraction
  • DAOPHOT, ISIS

27
GettingtheData
28
NGC 6539
  • 5 years of data
  • Fe/H -0.66

29
New GGCs
  • New to us!
  • Selected from Harris Catalogue
  • min Dec
  • max V_hb
  • Small
  • Core concentration
  • E(B-V) - Foreground reddening
  • Span of Fe/H

30
PROMPT Images!
31
PROMPT
  • Back to Harris Catalogue
  • Tracked down known LPVs
  • Corrected coordinates

32
PROMPT
  • NGC 288

33
PROMPT
  • NGC 1261

34
PROMPT
  • NGC 1851

35
Next steps
  • Our data
  • Finish processing / Photometery
  • Learn DAOPHOT
  • Perform DAOPHOT on recent data / NGC 6539
  • PROMPT data
  • Determine best collection method

36
References
  • People
  • Dr Andy Layden for his time, Dr John Laird for
    his books
  • Mike Smitka
  • Brian Pohl Dr. Bruce Carney, UNC Chapel Hill
  • Book
  • Steve B. Howell, 2000, Handbook of CCD Astronomy,
    Cambridge University Press
  • Websites
  • http//physics.bgsu.edu/layden/observatory.htm
  • http//zebu.uoregon.edu/ccd.html
  • http//www.ccd.com/ccdu.html
  • http//www.astro.virginia.edu/class/oconnell/astr5
    11/lec11-f03.html
  • http//www.wildealien.com/ccd/
  • PowerPoint file available online
  • http//physics.bgsu.edu/jlwilde/taatalk-feb07.ppt
  • Contacting me
  • jlwilde_at_bgsu.edu

37
Thanks for your attention!
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