Photographing the Night Sky DSLR Astrophotography
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Noise and ISO CS 178, Spring 2014
Noise and ISO CS 178, Spring 2014 Marc Levoy Computer Science Department Stanford University Outline ✦ examples of camera sensor noise • don’t confuse it with JPEG compression artifacts ✦ probability, mean, variance, signal-to-noise ratio (SNR) ✦ laundry list of noise sources • photon shot noise, dark current, hot pixels, fixed pattern noise, read noise ✦ SNR (again), dynamic range (DR), bits per pixel ✦ ISO ✦ denoising • by aligning and averaging multiple shots • by image processing will be covered in a later lecture 2 © Marc Levoy Nokia N95 cell phone at dusk • 8×8 blocks are JPEG compression • unwanted sinusoidal patterns within each block are JPEG’s attempt to compress noisy pixels 3 © Marc Levoy Canon 5D II at dusk • ISO 6400 • f/4.0 • 1/13 sec • RAW w/o denoising 4 © Marc Levoy Canon 5D II at dusk • ISO 6400 • f/4.0 • 1/13 sec • RAW w/o denoising 5 © Marc Levoy Canon 5D II at dusk • ISO 6400 • f/4.0 • 1/13 sec 6 © Marc Levoy Photon shot noise ✦ the number of photons arriving during an exposure varies from exposure to exposure and from pixel to pixel, even if the scene is completely uniform ✦ this number is governed by the Poisson distribution 7 © Marc Levoy Poisson distribution ✦ expresses the probability that a certain number of events will occur during an interval of time ✦ applicable to events that occur • with a known average rate, and • independently of the time since the last event ✦ if on average λ events occur in an interval of time, the probability p that k events occur instead is λ ke−λ p(k;λ) = probability k! density function 8 © Marc Levoy Mean and variance ✦ the mean of a probability density function p(x) is µ = ∫ x p(x)dx ✦ the variance of a probability density function p(x) is σ 2 = ∫ (x − µ)2 p(x)dx ✦ the mean and variance of the Poisson distribution are µ = λ σ 2 = λ ✦ the standard deviation is σ = λ Deviation grows slower than the average. -
About Raspberry Pi HQ Camera Lenses Created by Dylan Herrada
All About Raspberry Pi HQ Camera Lenses Created by Dylan Herrada Last updated on 2020-10-19 07:56:39 PM EDT Overview In this guide, I'll explain the 3 main lens options for a Raspberry Pi HQ Camera. I do have a few years of experience as a video engineer and I also have a decent amount of experience using cameras with relatively small sensors (mainly mirrorless cinema cameras like the BMPCC) so I am very aware of a lot of the advantages and challenges associated. That being said, I am by no means an expert, so apologies in advance if I get anything wrong. Parts Discussed Raspberry Pi High Quality HQ Camera $50.00 IN STOCK Add To Cart © Adafruit Industries https://learn.adafruit.com/raspberry-pi-hq-camera-lenses Page 3 of 13 16mm 10MP Telephoto Lens for Raspberry Pi HQ Camera OUT OF STOCK Out Of Stock 6mm 3MP Wide Angle Lens for Raspberry Pi HQ Camera OUT OF STOCK Out Of Stock Raspberry Pi 3 - Model B+ - 1.4GHz Cortex-A53 with 1GB RAM $35.00 IN STOCK Add To Cart Raspberry Pi Zero WH (Zero W with Headers) $14.00 IN STOCK Add To Cart © Adafruit Industries https://learn.adafruit.com/raspberry-pi-hq-camera-lenses Page 4 of 13 © Adafruit Industries https://learn.adafruit.com/raspberry-pi-hq-camera-lenses Page 5 of 13 Crop Factor What is crop factor? According to Wikipedia (https://adafru.it/MF0): In digital photography, the crop factor, format factor, or focal length multiplier of an image sensor format is the ratio of the dimensions of a camera's imaging area compared to a reference format; most often, this term is applied to digital cameras, relative to 35 mm film format as a reference. -
Making Your Own Astronomical Camera by Susan Kern and Don Mccarthy
www.astrosociety.org/uitc No. 50 - Spring 2000 © 2000, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. Making Your Own Astronomical Camera by Susan Kern and Don McCarthy An Education in Optics Dissect & Modify the Camera Loading the Film Turning the Camera Skyward Tracking the Sky Astronomy Camp for All Ages For More Information People are fascinated by the night sky. By patiently watching, one can observe many astronomical and atmospheric phenomena, yet the permanent recording of such phenomena usually belongs to serious amateur astronomers using moderately expensive, 35-mm cameras and to scientists using modern telescopic equipment. At the University of Arizona's Astronomy Camps, we dissect, modify, and reload disposed "One- Time Use" cameras to allow students to study engineering principles and to photograph the night sky. Elementary school students from Silverwood School in Washington state work with their modified One-Time Use cameras during Astronomy Camp. Photo courtesy of the authors. Today's disposable cameras are a marvel of technology, wonderfully suited to a variety of educational activities. Discarded plastic cameras are free from camera stores. Students from junior high through graduate school can benefit from analyzing the cameras' optics, mechanisms, electronics, light sources, manufacturing techniques, and economics. Some of these educational features were recently described by Gene Byrd and Mark Graham in their article in the Physics Teacher, "Camera and Telescope Free-for-All!" (1999, vol. 37, p. 547). Here we elaborate on the cameras' optical properties and show how to modify and reload one for astrophotography. An Education in Optics The "One-Time Use" cameras contain at least six interesting optical components. -
Name: NAAP – the Rotating Sky 1/11
Name: The Rotating Sky – Student Guide I. Background Information Work through the explanatory material on The Observer, Two Systems – Celestial, Horizon, the Paths of Stars, and Bands in the Sky. All of the concepts that are covered in these pages are used in the Rotating Sky Explorer and will be explored more fully there. II. Introduction to the Rotating Sky Simulator • Open the Rotating Sky Explorer The Rotating Sky Explorer consists of a flat map of the Earth, Celestial Sphere, and a Horizon Diagram that are linked together. The explanations below will help you fully explore the capabilities of the simulator. • You may click and drag either the celestial sphere or the horizon diagram to change your perspective. • A flat map of the earth is found in the lower left which allows one to control the location of the observer on the Earth. You may either drag the map cursor to specify a location, type in values for the latitude and longitude directly, or use the arrow keys to make adjustments in 5° increments. You should practice dragging the observer to a few locations (North Pole, intersection of the Prime Meridian and the Tropic of Capricorn, etc.). • Note how the Earth Map, Celestial Sphere, and Horizon Diagram are linked together. Grab the map cursor and slowly drag it back and forth vertically changing the observer’s latitude. Note how the observer’s location is reflected on the Earth at the center of the Celestial Sphere (this may occur on the back side of the earth out of view). • Continue changing the observer’s latitude and note how this is reflected on the horizon diagram. -
Low-Cost Computational Astrophotography
Low-cost Computational Astrophotography Joseph Yen Peter Bryan Electrical Engineering Electrical Engineering Stanford University Stanford University [email protected] [email protected] Abstract 2. Related Work When taking photographs of the night sky, long ex- Currently, most astrophotographers compensate for posure times help photographers observe many stars, the rotation of the earth by physically moving the cam- but the rotation of the earth results in long star streak era along with the earth. However, some attempts arcs about the celestial pole. An algorithm for re- have been made to remove this requirement. To accu- moving these star streaks and substituting accurately rately localize stars in streaked images, one researcher placed point-like stars is designed and implemented. has re-mapped the star streak to polar coordinates, so Images containing star streaks are transformed into that all stars will have the same point-spread function. ones with un-streaked starry skies while retaining This technique was designed for locating specific stars color and brightness information. The procedure is for the purpose of identifying specific stars, but will shown to work consistently on a 35-image dataset. be applicable for our purposes when removing star streaks [4]. Other factors besides streaking can cause quality degradation in star images, and attempts have 1. Introduction been made to correct this. These have used such tech- niques as Richardson-Lucy deblurring [2] and maxi- Astrophotography is a widespread pastime in which mally sparse optimization [1]. DSLR cameras are used to take images of objects in space. Certain factors make this a very expen- sive hobby. -
The Definitive Guide to Shooting Hypnotic Star Trails
The Definitive Guide to Shooting Hypnotic Star Trails www.photopills.com Mark Gee proves everyone can take contagious images 1 Feel free to share this eBook © PhotoPills December 2016 Never Stop Learning A Guide to the Best Meteor Showers in 2016: When, Where and How to Shoot Them How To Shoot Truly Contagious Milky Way Pictures Understanding Golden Hour, Blue Hour and Twilights 7 Tips to Make the Next Supermoon Shine in Your Photos MORE TUTORIALS AT PHOTOPILLS.COM/ACADEMY Understanding How To Plan the Azimuth and Milky Way Using Elevation The Augmented Reality How to find How To Plan The moonrises and Next Full Moon moonsets PhotoPills Awards Get your photos featured and win $6,600 in cash prizes Learn more+ Join PhotoPillers from around the world for a 7 fun-filled days of learning and adventure in the island of light! Learn More Index introduction 1 Quick answers to key Star Trails questions 2 The 21 Star Trails images you must shoot before you die 3 The principles behind your idea generation (or diverge before you converge) 4 The 6 key Star Trails tips you should know before start brainstorming 5 The foreground makes the difference, go to an award-winning location 6 How to plan your Star Trails photo ideas for success 7 The best equipment for Star Trails photography (beginner, advanced and pro) 8 How to shoot single long exposure Star Trails 9 How to shoot multiple long exposure Star Trails (image stacking) 10 The best star stacking software for Mac and PC (and how to use it step-by-step) 11 How to create a Star Trails vortex (or -
AG-AF100 28Mm Wide Lens
Contents 1. What change when you use the different imager size camera? 1. What happens? 2. Focal Length 2. Iris (F Stop) 3. Flange Back Adjustment 2. Why Bokeh occurs? 1. F Stop 2. Circle of confusion diameter limit 3. Airy Disc 4. Bokeh by Diffraction 5. 1/3” lens Response (Example) 6. What does In/Out of Focus mean? 7. Depth of Field 8. How to use Bokeh to shoot impressive pictures. 9. Note for AF100 shooting 3. Crop Factor 1. How to use Crop Factor 2. Foal Length and Depth of Field by Imager Size 3. What is the benefit of large sensor? 4. Appendix 1. Size of Imagers 2. Color Separation Filter 3. Sensitivity Comparison 4. ASA Sensitivity 5. Depth of Field Comparison by Imager Size 6. F Stop to get the same Depth of Field 7. Back Focus and Flange Back (Flange Focal Distance) 8. Distance Error by Flange Back Error 9. View Angle Formula 10. Conceptual Schema – Relationship between Iris and Resolution 11. What’s the difference between Video Camera Lens and Still Camera Lens 12. Depth of Field Formula 1.What changes when you use the different imager size camera? 1. Focal Length changes 58mm + + It becomes 35mm Full Frame Standard Lens (CANON, NIKON, LEICA etc.) AG-AF100 28mm Wide Lens 2. Iris (F Stop) changes *distance to object:2m Depth of Field changes *Iris:F4 2m 0m F4 F2 X X <35mm Still Camera> 0.26m 0.2m 0.4m 0.26m 0.2m F4 <4/3 inch> X 0.9m X F2 0.6m 0.4m 0.26m 0.2m Depth of Field 3. -
DSLR Astrophotography They Say… Start with a Joke
DSLR Astrophotography They say… start with a joke. DLSR Wide-field Astrophotography The Advantages It’s Relatively Inexpensive All you need is a DLSR camera …and a tripod You Don’t Need This! Nikon v.s. Canon Most DSLR astrophotographers use Canon cameras. Canon releases the details of the camera’s software. This allows the development of third party software, designed specifically for astrophotography. Nikon does not create a truly raw image A simple median blurring filter is always applied... removing many stars, as they are seen as noise. This prohibits precise image calibration. Some Nikons allow the “Mode 3” work around. Using Nikon’s Mode 3 Simply start the bulb time exposure and terminate it by turning off the camera. The camera sees this as a low-power warning and immediately saves the image without running the median blurring filter Testing For Mode 3 Availability Take a one-minute dark exposure in Mode 1. This is a raw image with “no noise reduction” selected. Take a one-minute Mode 3 dark exposure. If Mode 3 is available, that exposure will have noticeably more hot pixels and noise. For Starters… Keep It Simple Set the focus to infinity... before it’s dark Mount the camera on a sturdy tripod Use a wide angle lens (18mm is nice) Set the lens to its lowest f-stop Use the RAW image format, at the highest ISO setting Shoot 20-30 second exposures Take about five dark exposures (more on this later) …and you can get an image like this! Nikon D40X 18mm @ f/4 ISO 1600 Mode 1 4 30-Sec exposures 4 30-Sec darks After taking several Milky Way shots it may be time to get more adventurous. -
A Guide to Smartphone Astrophotography National Aeronautics and Space Administration
National Aeronautics and Space Administration A Guide to Smartphone Astrophotography National Aeronautics and Space Administration A Guide to Smartphone Astrophotography A Guide to Smartphone Astrophotography Dr. Sten Odenwald NASA Space Science Education Consortium Goddard Space Flight Center Greenbelt, Maryland Cover designs and editing by Abbey Interrante Cover illustrations Front: Aurora (Elizabeth Macdonald), moon (Spencer Collins), star trails (Donald Noor), Orion nebula (Christian Harris), solar eclipse (Christopher Jones), Milky Way (Shun-Chia Yang), satellite streaks (Stanislav Kaniansky),sunspot (Michael Seeboerger-Weichselbaum),sun dogs (Billy Heather). Back: Milky Way (Gabriel Clark) Two front cover designs are provided with this book. To conserve toner, begin document printing with the second cover. This product is supported by NASA under cooperative agreement number NNH15ZDA004C. [1] Table of Contents Introduction.................................................................................................................................................... 5 How to use this book ..................................................................................................................................... 9 1.0 Light Pollution ....................................................................................................................................... 12 2.0 Cameras ................................................................................................................................................ -
Astrophotography a Beginner’S Guide
Astrophotography A Beginner’s Guide By James Seaman Copyright © James Seaman 2018 Contents Astrophotography ................................................................................................................................... 5 Equipment ........................................................................................................................................... 6 DSLR Cameras ..................................................................................................................................... 7 Sensors ............................................................................................................................................ 7 Focal Length .................................................................................................................................... 8 Exposure .......................................................................................................................................... 9 Aperture ........................................................................................................................................ 10 ISO ................................................................................................................................................. 11 White Balance ............................................................................................................................... 12 File Formats .................................................................................................................................. -
Does Size Matter.Sanitized-20151026-GGCS
Does Size Matter? What’s New in Small Cameras and Should I Switch? Doug Kaye dougkaye.com [email protected] • Portfolio at DougKaye.com • Co-Host of All About the Gear • Cuba & Street Photography Workshops • Frequent guest on This Week in Photo • Active on Social Media • Portfolio at DougKaye.com • Co-Host of All About the Gear • Cuba & Street Photography Workshops • Frequent guest on This Week in Photo • Active on Social Media The Acronyms • DSLR: Digital Single-Lens Reflex • MILC: Mirrorless Interchangeable-Lens Camera • APS-C: ~1.5x Crop-Factor Sensor Size • MFT: Micro Four-Thirds • LCD: Liquid Crystal Display (rear) • OVF: Optical Viewfinder • EVF: Electronic Viewfinder MILCs • Mirrorless • Interchangeable Lens • Autofocus • Electronic Viewfinder Who’s Who • The Old Guard • Nikon & Canon • The Upstarts • Sony & Fujifilm (Full-Frame and APS-C) • Olympus & Panasonic/Lumix (MFT) • Leica? Samsung? iPhone? DSLR vs. Mirrorless MILC History MILC History • 2004: Epson RD-1 (1st Mirrorless) • 2006: Leica M8 (1st Digital Leica) • 2008: Panasonic G1 (1st MFT) • 2009: Leica M9 (1st Full Frame) • 2010: Sony NEX-5 (1st M-APS-C, Hybrid AF) • 2012: Fuji X-Pro1 (Hybrid VF, X-Trans) • 2013: Olympus OM-D E-M1 • 2014: Sony a7S (High ISO), a7R (36MP) • 2015: Sony a7 II, a7R II, a7S II (Full-Frame IBIS) MILC Advantages • Smaller & Lighter • Simpler & Less Expensive • EVF vs. OVF • Always in LiveView Mode (WYSIWYG) • Accurate Autofocus • Quieter & Less Vibration • Simpler Wide-Angle Lens Designs • Compatible w/Other Lens Mounts MILC Disadvantages • EVF vs. OVF? • Continuous Autofocus Speed/Accuracy • Lack of Accessories • Legacy Wide-Angle Lens Issues Sensor Size • Full 35mm Frame (FF): 1x • APS-C: 1.5x • MFT: 2x Pixel Size • Larger Pixels Capture More Light • Higher ISO, Lower Noise • Broader Dynamic Range • 16MP APS-C = 36MP Full Frame • 16MP MFT = 64MP Full Frame Field of View (FoV) • Smaller sensors just crop the image. -
A Practical Guide to Panoramic Multispectral Imaging
A PRACTICAL GUIDE TO PANORAMIC MULTISPECTRAL IMAGING By Antonino Cosentino 66 PANORAMIC MULTISPECTRAL IMAGING Panoramic Multispectral Imaging is a fast and mobile methodology to perform high resolution imaging (up to about 25 pixel/mm) with budget equipment and it is targeted to institutions or private professionals that cannot invest in costly dedicated equipment and/or need a mobile and lightweight setup. This method is based on panoramic photography that uses a panoramic head to precisely rotate a camera and shoot a sequence of images around the entrance pupil of the lens, eliminating parallax error. The proposed system is made of consumer level panoramic photography tools and can accommodate any imaging device, such as a modified digital camera, an InGaAs camera for infrared reflectography and a thermal camera for examination of historical architecture. Introduction as thermal cameras for diagnostics of historical architecture. This article focuses on paintings, This paper describes a fast and mobile methodo‐ but the method remains valid for the documenta‐ logy to perform high resolution multispectral tion of any 2D object such as prints and drawings. imaging with budget equipment. This method Panoramic photography consists of taking a can be appreciated by institutions or private series of photo of a scene with a precise rotating professionals that cannot invest in more costly head and then using special software to align dedicated equipment and/or need a mobile and seamlessly stitch those images into one (lightweight) and fast setup. There are already panorama. excellent medium and large format infrared (IR) modified digital cameras on the market, as well as scanners for high resolution Infrared Reflec‐ Multispectral Imaging with a Digital Camera tography, but both are expensive.