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Mosaic Imaging and 3D Distance Vectors

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Mosaic Imaging and 3D Distance Vectors. NGC 4088 and NGC 4085 Interacting Galaxies. Chelsea Braun. Image: Digitized Sky Survey. North: up. East: Left – PowerPoint PPT presentation

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Title: Mosaic Imaging and 3D Distance Vectors


1
Mosaic Imaging and 3D Distance Vectors
North up East Left
  • NGC 4088 and NGC 4085 Interacting Galaxies
  • Chelsea Braun

Image Digitized Sky Survey
2
Outline
North up East Left
  • Introduction
  • Theory
  • Mosaic Image Plan
  • Creating the Images
  • Final Image
  • Distance Calculation
  • Discussion

Image Jeff Johnson, croppedhttp//jeffjastro.com
/dso/NGC4088_30Jan09.htm
3
Introduction
North up East Left
  • NGC 4088 is a weakly barred spiral galaxy with
    morphological type SAB(rs)bc
  • NGC 4085 is an Sc D galaxy
  • Found in the Ursa Major constellation
  • Part of the M109 group

Image Stellarium
Credit Simbad
4
Theory
  • The 3D distance vector
  • Calculating the distance between 2 galaxies
  • Not as simple as finding the distance in arc
    seconds on an image and then converting to
    parsecs
  • Requires knowing the distance to these objects

5
Geometry
6
Distance
  • 4 equations
  • Where the distance to the galaxies, d1 and d2,
  • can be determined using arcmins, is determined
    from the image with scale, S

7
Imaging
  • Spent a night collecting 1hr 30mins of data
  • 30 mins for 3 7x7 images
  • Difficulties?
  • Telescope moved a lot
  • Provided difficulties when combining the images

8
Mosaic Image Plan
North up East Left
  • Take three 7x7 images, 30 mins at 60sec
    exposures
  • North up and East right (for all images)
  • Have common stars in each image to line up the
    images

NGC 4088
MID
NGC 4085
Image Digitized Sky Survey
9
Mosaic Image Plan
North up East Left
15x7
Image Digitized Sky Survey
10
NGC 4088
North up East Left
  • 30 images at 60sec exposures, 7x7 image
  • Calibrated the images
  • Broke into 2 subgroups 1-9, 10-30

11
NGC 4088
North up East Left
12
NGC 4088
North up East Left
  • Final NGC 4088 image
  • Combine the final averaged images from the
    substacks into 1 stack
  • Register them
  • Combine

13
NGC 4088
North up East Left
Image 6.7x5.2
14
MID
  • 30 images at 60 second exposures, 7x7 images
  • The middle star image had the most difficulties
  • Most noise
  • First 5 frames removed (guide stars missing)
  • Broken down into 3 substacks
  • Substack 1 6-15
  • Substack 216-21
  • Substack 3 22-30

15
Substack 1
  • Most difficult to register
  • done for the 10 frames using TurboReg scaled
    rotation
  • Pick 2 points on 2 different images
  • Aligns those 2 points using translation and
    rotation
  • Rotation is a bad thing

16
Substack 1
North up East Left
Slide 6
Slide 15
17
Substack 1
  • Crop all the manually registered images and place
    in a stack
  • PROBLEM slight rotation in the TurboReg plugin
    caused a very noisy averaged image

18
Substack 1
North up East Left
19
Substack 1
North up East Left
20
Substack 2 3 Final Images
North up East Left
21
Mid Final Image
North up East Left
Image 6.5 x 5.5
22
NGC 4085
  • 30 images at 60 second exposures, 7x7
  • No substacks needed
  • Although 2 registrations were necessary to align
    the images

23
NGC 4085 Final Image
Image 6.7x5.8
North up East Left
24
Background Levels
  • Background levels were matched to create the
    mosaic
  • Measured the background levels of the 3 final
    images
  • Took the darkest background level and matched
    them into the other images
  • Subtracted the differences in background levels

25
North up East Left
26
Background Levels
Image Background Level Difference
NGC 4088 1060.86 0
MID 1109.77 48.91
NGC 4085 1170.32 109.46
  • Convert to 16 bit to use MosaicJ
  • Find the minimum and maximum pixel values for
    all three images and set the B C min and max to
    these values over all 3 images
  • Then convert to 16 bit

27
Final Image
North up East Left
Image 16.8 x 7.6
28
Distance Between Galaxies
  • Measured a distance of 894.79 pixels between
    galaxies

Variable Value Error
d1 distance to NGC 4088 12.22 Mpc Given
d2 distance to NGC 4085 12.55 Mpc Given
D 894.79 pixels 8 pixels
S, image scale 0.0136 arcmins/pixel 0.0003 arcmins/pixel
29
Distance Between Galaxies
  • Using the 4 equations
  • Darcmins 12.2' 0.4'
  • Drads 0.0035 0.0001
  • Dparsecs 0.043 0.001 Mpc
  • d1-d2 0.33 Mpc
  • D' 0.33 0.03 Mpc

30
Discussion
  • Fixing the MID image
  • Save a ROI line between stars for substack 1 and
    use the same length distance
  • Should eliminate rotation?

31
END
  • THANKS!!!!!!

32
References
  • Association of Universities for Research in
    Astronomy, Inc. 1994. The Digitized Sky
    Survey http//stdatu.stsci.edu/cgi-bin/dss_form
  • Chereau F, Gates M, Kerr N, Marcos D, Marinov B.
    et al. 2010. Stellarium
  • Goldman, D. (2008). NGC 4088 in UMa. Last
    accessed 15th Nov. lthttp//dg-imaging.astrodon.com
    /gallery/display.cfm?imgID135gt
  • This research has made use of the SIMBAD
    database, operated at CDS, Strasbourg, France. 
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