Simon Dawes Artemis 285. Kit Assembly The Completed Camera.

Slides:



Advertisements
Similar presentations
Steve Cannistra, Dark Halo Removal
Advertisements

Institute for Gravitational Research
Institute for Gravitational Research
Beginners Guide To Levels, Curves and Layer Masks.
Wide Field Imaging Not really a novice RV lifestyle forced change in 2009 Light weight and portable equipment Ideal for wide field imaging with camera.
By Kevin Saunders.  tml tml.
“The depth of field picture was correctly depicted of the type of picture. In the depth of field photo, the entire photo is in focus and the subject is.
With “like” denominators: 1)add/subtract across the top. 2)Leave the bottom alone. Ex: =
By Aaron Proia and Matthew Copenhaver.  For this presentation, we will be walking you through two processes that are commonly used in Photoshop.  These.
Image Processing Tutorial
Chapter 3 Image Enhancement in the Spatial Domain.
INTRODUCTION TO ADOBE ILLUSTRATOR VECTOR MONSTERS Created by CHRIS SPOONER.
Salk Institute Mobile Lab Gel Electrophoresis Teacher Instructions BioRad Set Up 8 groups Grossmont Kit.
Variety and Contrast. What is va r ie t y? The use of juxtaposition to make you look at a certain part or make the entire piece more interesting. Variety.
Multimedia Data Introduction to Image Processing Dr Mike Spann Electronic, Electrical and Computer.
Image Processing Developing Pictures In the Dark Room.
Weather By: Mallory Hart.
Signal vs Noise: Image Calibration First… some terminology:  Light Frame: The individual pictures you take of your target.  Dark Frame: An image taken.
CCD testing Enver Alagoz 12 April CCD testing goals CCD testing is to learn how to – do dark noise characterization – do gain measurements – determine.
Teacher: Kenji Tachibana Digital Photography I. Exposure Compensation Shoot. | | | | | | | | | | | | |
How To Silkscreen A T-Shirt! Mr. Hobbs Art. You Must Follow These Steps to Print your T-Shirt: 1. Find a partner to work with. 2. Place your T-shirt down.
Welcome to Part Two Now you will be adding photos that you downloaded earlier.
There are 3 switches downstairs, each corresponding to one of the light bulbs upstairs. How can you figure out which light switch goes to which light.
Photon Transfer Method 1. Using two identical flat field exposures it is possible to measure the read noise of a CCD with the Photon Transfer method. Two.
STEP 1: Determining the exact image width STEP 1: Determining the exact image width Position of X-ray Filter Position of X-ray Filter STEP 5: Crop Extra.
Color Correct and Remove Keystoning A minimalist approach to photographing your art By Paul Marley.
MATH 31 LESSONS PreCalculus 2. Powers. A. Power Laws Terminology: b x.
High Dynamic Range (HDR) Photography. Camera vs Eye Eye sees a wider range of color luminance than digital cameras HDR’s images compensate for this by.
Lecture Exposure/histograms. Exposure - Four Factors A camera is just a box with a hole in it. The correct exposure is determined by four factors: 1.
Faking Infrared Using Adobe CAMERA RAW. Open your RAW file in ACR, then head straight to the the HSL/Grayscale tab. Check the box for Convert to Grayscale,
CCD Detectors CCD=“charge coupled device” Readout method:
Remote Astronomy and Colour Imaging During these sessions you will learn how to make images from your own remote telescope observation just like this one.
Multimedia Data Introduction to Image Processing Dr Sandra I. Woolley Electronic, Electrical.
What’s in a sum? Simon Dawes CMHAS. Should you stack frames using Mean, Median or Sum?
 The image that the digital camera sensor captures is based on the light reflected or emitted from a subject and how much the sensor is exposed to that.
Nikon Spinning Disk Imaging & Training Support. Find your cells with DIC in Live Preview 1.The green DIA Lamp, used for DIC, should be on. 2. Condenser.
Digital Imaging. Digital image - definition Image = “a two-dimensional function, f(x,y), where x and y are spatial coordinates, and the amplitude of f.
Basic Black and White Photography Lynnwood High School Ms. Schou.
Chapter 4 Working with Frames. Align and distribute objects on a page Stack and layer objects Work with graphics frames Work with text frames Chapter.
Measuring Sky Brightness with a Digital Camera Paris 2004.
Scratch Art.
Machine Vision Introduction to Using Cognex DVT Intellect.
© 2011 Delmar, Cengage Learning Chapter 4 Working with Frames.
NICMOS Calibration Challenges in the Ultra Deep Field Rodger Thompson Steward Observatory University of Arizona.
1 Layer up to keep warm… A short tutorial on the usage of layers.
Physics 114: Lecture 8 Measuring Noise in Real Data Dale E. Gary NJIT Physics Department.
14 January Observational Astronomy SPECTROSCOPIC data reduction Piskunov & Valenti 2002, A&A 385, 1095.
The content of the picture itself is framed within a beautiful old archway and looks out onto the great wall of china. This adds to the attractiveness.
1 Printing & Imaging Technology Working with Layers Copyright © Texas Education Agency, All rights reserved. Images and other multimedia content.
CCD Image Processing: Issues & Solutions. CCDs: noise sources dark current –signal from unexposed CCD read noise –uncertainty in counting electrons in.
Astroschool: Image Calibration February 20 th,
{ Digital Image Processing By Professor Stelmark.
CCD Calibrations Eliminating noise and other sources of error.
Announcements After a short lecture we will adjourn to the Farm. Tonight is a Dark Sky make-up night. Class will meet Thursday night. If clear: meet at.
Relative Spectral Response and Flat Fields with Internal Calibration Lamps Luisa M. Lara IAA-CSIC Granada (SPAIN)
Charge Transfer Efficiency of Charge Coupled Device
CCD Image Processing …okay, I’ve got a bunch of .fits files, now what?
Photoshop Styles & Filters
Computer Animation Texture Mapping.
1.02 Investigate image editing.
Photometric Analysis of Asteroids
Announcements HR Diagram lab will be extended for one week. I’ll talk about it today. Homework: Chapter 9 # 1, 2 & 3 Next week is a Dark Sky Night. If.
Karen Meech Institute for Astronomy TOPS 2003
Technical Intro to Digital Astrophotography Part 1
Image calibration Geoff Smith, September 2018.
Technique 6: General gray-level transformations
Technique 6: General gray-level transformations
Deep Sky Imaging with SharpCap
1.02 Investigate image editing.
Improving Your Astrophotos
Presentation transcript:

Simon Dawes Artemis 285

Kit

Assembly

The Completed Camera

Problem 1 Thermal readout noise Solution: 1.New Peltier 2.More thermal paste on peltier (although Dark subtraction was quite effective)

Problem 2 Dust donuts! Solution: Flat fielding Light box (although they can sometimes be removed with clever processing)

Problem 3 & 4 Gradient from top left to bottom right Solution: Turn off Amp during exposure (Latest software always selects this for long exposures) Weird patterns! – Dew on CCD Solution: Seal the cold frame, desiccant was trying to dry the whole Earth! CCD was dripping wet

Problem 5 (will they ever stop) Another weird pattern! - Frost Solution: Thermal paste sealing CCD window, to warm the window slightly

Flat field light box

Raw 15s Frame, note top-bottom gradient and dust donuts

Stacked, dark subtracted, cube route scaled, de-convolved

Notice dust donuts (poor flat field) and sky gradient going from top left to bottom right

Median rank operator removes small scale structure, leaving the sky gradient, donuts and Globular

19,000 is added to every pixel in original image

One Image is subtracted from the other, removing gradient and donuts

Background is smoothed to remove some noise

Any pixel value less than 21,000 ADU is set to 17,000ADU

Black and white levels are adjusted