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Depth-Aware Blending of Smoothed Images for Bokeh Effect Generation
1 Depth-aware Blending of Smoothed Images for Bokeh Effect Generation Saikat Duttaa,∗∗ aIndian Institute of Technology Madras, Chennai, PIN-600036, India ABSTRACT Bokeh effect is used in photography to capture images where the closer objects look sharp and every- thing else stays out-of-focus. Bokeh photos are generally captured using Single Lens Reflex cameras using shallow depth-of-field. Most of the modern smartphones can take bokeh images by leveraging dual rear cameras or a good auto-focus hardware. However, for smartphones with single-rear camera without a good auto-focus hardware, we have to rely on software to generate bokeh images. This kind of system is also useful to generate bokeh effect in already captured images. In this paper, an end-to-end deep learning framework is proposed to generate high-quality bokeh effect from images. The original image and different versions of smoothed images are blended to generate Bokeh effect with the help of a monocular depth estimation network. The proposed approach is compared against a saliency detection based baseline and a number of approaches proposed in AIM 2019 Challenge on Bokeh Effect Synthesis. Extensive experiments are shown in order to understand different parts of the proposed algorithm. The network is lightweight and can process an HD image in 0.03 seconds. This approach ranked second in AIM 2019 Bokeh effect challenge-Perceptual Track. 1. Introduction tant problem in Computer Vision and has gained attention re- cently. Most of the existing approaches(Shen et al., 2016; Wad- Depth-of-field effect or Bokeh effect is often used in photog- hwa et al., 2018; Xu et al., 2018) work on human portraits by raphy to generate aesthetic pictures. -
Adaptive Optics in Laser Processing Patrick S
Salter and Booth Light: Science & Applications (2019) 8:110 Official journal of the CIOMP 2047-7538 https://doi.org/10.1038/s41377-019-0215-1 www.nature.com/lsa REVIEW ARTICLE Open Access Adaptive optics in laser processing Patrick S. Salter 1 and Martin J. Booth1 Abstract Adaptive optics are becoming a valuable tool for laser processing, providing enhanced functionality and flexibility for a range of systems. Using a single adaptive element, it is possible to correct for aberrations introduced when focusing inside the workpiece, tailor the focal intensity distribution for the particular fabrication task and/or provide parallelisation to reduce processing times. This is particularly promising for applications using ultrafast lasers for three- dimensional fabrication. We review recent developments in adaptive laser processing, including methods and applications, before discussing prospects for the future. Introduction enhance ultrafast DLW. An adaptive optical element Over the past two decades, direct laser writing (DLW) enables control over the fabrication laser beam and allows with ultrafast lasers has developed into a mature, diverse it to be dynamically updated during processing. Adaptive – and industrially relevant field1 5. The ultrashort nature of elements can modulate the phase, amplitude and/or the laser pulses means that energy can be delivered to the polarisation of the fabrication beam, providing many focus in a period shorter than the characteristic timescale possibilities for advanced control of the laser fabrication for thermal diffusion, leading to highly accurate material process. In this review, we briefly outline the application modification1. Thus, by focusing ultrashort pulses onto areas of AO for laser processing before considering the 1234567890():,; 1234567890():,; 1234567890():,; 1234567890():,; the surface of the workpiece, precise cuts and holes can be methods of AO, including the range of adaptive elements manufactured with a minimal heat-affected zone. -
C5 Spotting Scope XLT 52291
C5 Spotting Scope - #52291 Instruction Manual A spotting scope is nothing more than a telescope that is designed to look around the Earth. Unlike astronomical telescopes, which produce inverted or reverted images, spotting scopes produce correctly oriented images. Celestron offers several different models, each of which uses the highest quality optics to produce the best possible images. All models have rugged, durable housings to give you a lifetime of pleasure with a minimal amount of maintenance. Your Celestron spotting scope is designed to give you hours of fun and rewarding observations. There are, however, a few things to consider before using your spotting scope that will ensure your safety and protect your equipment. • Never look directly at the Sun with the naked eye or with your spotting scope. Permanent and irreversible eye damage may result. • Never use your spotting scope to project an image of the Sun onto any surface. Internal heat build-up can damage your spotting scope and/or any accessories attached to it. • Never use an eyepiece solar filter or a Herschel wedge. Internal heat build- up inside your spotting scope can cause these devices to crack or break, allowing unfiltered sunlight to pass through to the eye. • Never leave your spotting scope unsupervised, either when children are present or adults who may not be familiar with the correct operating procedures of your spotting scope. • Never point your spotting scope at the Sun unless you have the proper solar filter. We recommend Celestron solar filters only. Don't take chances -- use Celestron filters for safety and performance! When using your spotting scope with the proper solar filter, ALWAYS cover the finderscope. -
A Curriculum Guide
FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE This page is an excerpt from Focus on Photography: A Curriculum Guide Written by Cynthia Way for the International Center of Photography © 2006 International Center of Photography All rights reserved. Published by the International Center of Photography, New York. Printed in the United States of America. Please credit the International Center of Photography on all reproductions. This project has been made possible with generous support from Andrew and Marina Lewin, the GE Fund, and public funds from the New York City Department of Cultural Affairs Cultural Challenge Program. FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE PART IV Resources FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE This section is an excerpt from Focus on Photography: A Curriculum Guide Written by Cynthia Way for the International Center of Photography © 2006 International Center of Photography All rights reserved. Published by the International Center of Photography, New York. Printed in the United States of America. Please credit the International Center of Photography on all reproductions. This project has been made possible with generous support from Andrew and Marina Lewin, the GE Fund, and public funds from the New York City Department of Cultural Affairs Cultural Challenge Program. FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE Focus Lesson Plans Fand Actvities INDEX TO FOCUS LINKS Focus Links Lesson Plans Focus Link 1 LESSON 1: Introductory Polaroid Exercises Focus Link 2 LESSON 2: Camera as a Tool Focus Link 3 LESSON 3: Photographic Field -
A Theoretical and Practical Introduction to Optics a Theoretical and Practical Introduction to Optics
White Paper A Theoretical and Practical Introduction to Optics A Theoretical and Practical Introduction to Optics Be honest: do you really know how to calculate the focal length of a lens? If so, you are an exception to the rule and can stop reading here !! For the rest of you, here is a second chance. Back to square one "Piece of broken glass starts forest fire"– a common headline during the summer. But how could this have happened? Due to the enormous distance between the Earth and the Sun, the Sun only appears as a tiny point emitting parallel rays of light (figure 1a) Should these parallel rays pass through a lens (or a piece of glass, which has similar characteristics) the rays would meet behind the lens at what is called the focal point. But what happens if our point of light is so near to the lens that we can not assume to have parallel rays of light? They cross each other behind the focal point (figure 1b). If we take a look at the image of our point of light at the focal points position we will see a unclear blurred spot. And so the question arises- "what is focusing?". Focusing is to increase the distance between the focal plane and the lens until the focal plane and the junction of the rays overlap each other (figure 1c). Thus, for single points of light the situation is quite simple. But what happens to the image of screws, PCBs or plates of steel? From points of light to images A point of light does not necessarily originate directly from the sun, candles or lamps, it can also result from a reflection. -
Mission to the Solar Gravity Lens Focus: Natural Highground for Imaging Earth-Like Exoplanets L
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8203.pdf MISSION TO THE SOLAR GRAVITY LENS FOCUS: NATURAL HIGHGROUND FOR IMAGING EARTH-LIKE EXOPLANETS L. Alkalai1, N. Arora1, M. Shao1, S. Turyshev1, L. Friedman8 ,P. C. Brandt3, R. McNutt3, G. Hallinan2, R. Mewaldt2, J. Bock2, M. Brown2, J. McGuire1, A. Biswas1, P. Liewer1, N. Murphy1, M. Desai4, D. McComas5, M. Opher6, E. Stone2, G. Zank7, 1Jet Propulsion Laboratory, Pasadena, CA 91109, USA, 2California Institute of Technology, Pasadena, CA 91125, USA, 3The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA,4Southwest Research Institute, San Antonio, TX 78238, USA, 5Princeton Plasma Physics Laboratory, Princeton, NJ 08543, USA, 6Boston University, Boston, MA 02215, USA, 7University of Alabama in Huntsville, Huntsville, AL 35899, USA, 8Emritus, The Planetary Society. Figure 1: A SGL Probe Mission is a first step in the goal to search and study potential habitable exoplanets. This figure was developed as a product of two Keck Institute for Space Studies (KISS) workshops on the topic of the “Science and Enabling Technologies for the Exploration of the Interstellar Medium” led by E. Stone, L. Alkalai and L. Friedman. Introduction: Recent data from Voyager 1, Kepler and New Horizons spacecraft have resulted in breath-taking discoveries that have excited the public and invigorated the space science community. Voyager 1, the first spacecraft to arrive at the Heliopause, discovered that Fig. 2. Imaging of an exo-Earth with solar gravitational Lens. The exo-Earth occupies (1km×1km) area at the image plane. Using a 1m the interstellar medium is far more complicated and telescope as a 1 pixel detector provides a (1000×1000) pixel image! turbulent than expected; the Kepler telescope According to Einstein’s general relativity, gravity discovered that exoplanets are not only ubiquitous but induces refractive properties of space-time causing a also diverse in our galaxy and that Earth-like exoplanets massive object to act as a lens by bending light. -
Camera Settings Guide
Camera Settings Guide • " " and " " are trademarks or registered trademarks of Sony Corporation. • All other company and product names mentioned herein are used for identification purposes only and may be the trademarks or registered trademarks of their respective owners. TM and ® symbols are not included in this booklet. • Screen displays and effects used to illustrate some functions are simulated. Conventional autofocus has until now dealt with space alone. Sony goes one step further — a big step, with an innovative image sensor that picks up both space and time to capture moving subjects with new clarity. Sony spells the beginning of a new autofocus era. 4D FOCUS allows you to take crisper photos than ever. Plain old autofocus is a thing of the past. The future of photography is in motion. What is 4D FOCUS? Space: 3D Time: 4D 4D FOCUS Area Depth Time Wide Fast Steadfast The wide AF area, covering nearly the Fast Hybrid AF, combining phase- An advanced AF algorithm accurately entire frame, allows focusing on a detection AF and contrast-detection AF, predicts subject’s next move. Precise AF subject positioned even off the center instantly detects distance to the subject tracking allows focus to be maintained of the frame. to focus accurately. even on fast-moving subjects. Meeting your focusing demands Basic AF performance of Wide Fast Steadfast Focusing over wide area Instant focusing! Once it's focused, it never lets go The 6000 employs a focal plane phase- Advanced Fast Hybrid AF combines phase- With Focus Mode set to AF-C, the camera detection AF sensor with 179 AF points spread detection AF and contrast-detection AF to achieve displays one or more small green frames to cover nearly the entire frame. -
Longitudinal Chromatic Aberration
Longitudinal Chromatic Aberration Red focus Blue focus LCA Transverse Chromatic Aberration Decentered pupil Transverse Chromatic Aberration Chromatic Difference of Refraction Atchison and Smith, JOSA A, 2005 Why is LCA not really a problem? Chromatic Aberration Halos (LCA) Fringes (TCA) www.starizona.com digitaldailydose.wordpress.com Red-Green Duochrome test • If the letters on the red side stand out more, add minus power; if the letters on the green side stand out more, add plus power. • Neutrality is reached when the letters on both backgrounds appear equally distinct. Colligon-Bradley P. J Ophthalmic Nurs Technol. 1992 11(5):220-2. Transverse Chromatic Aberration Lab #7 April 15th Look at a red and blue target through a 1 mm pinhole. Move the pinhole from one edge of the pupil to the other. What happens to the red and blue images? Chromatic Difference of Magnification Chief ray Aperture stop Off axis source Abbe Number • Also known as – Refractive efficiency – nu-value –V-value –constringence Refractive efficiencies for common materials water 55.6 alcohol 60.6 ophthalmic crown glass 58.6 polycarbonate 30.0 dense flint glass 36.6 Highlite glass 31.0 BK7 64.9 Example • Given the following indices of refraction for BK7 glass (nD = 1.519; nF = 1.522; nC = 1.514) what is the refractive efficiency? • What is the chromatic aberration of a 20D thin lens made of BK7 glass? Problem • Design a 10.00 D achromatic doublet using ophthalmic crown glass and dense flint glass Carl Friedrich Gauss 1777-1855 Heinrich Seidel 1842-1906 Approximations to -
Computer Vision: Projection
Image formation and cameras Photography CSE P 576 Larry Zitnick ([email protected]) Many slides courtesy of Steve Seitz Image formation Pinhole camera Object Film Object Barrier Film Add a barrier to block off most of the rays • This reduces blurring Let’s design a camera • The opening known as the aperture • Idea 1: put a piece of film in front of an object • How does this transform the image? • Do we get a reasonable image? 1 Camera Obscura Shrinking the aperture The first camera • Known to Aristotle • How does the aperture size affect the image? Why not make the aperture as small as possible? • Less light gets through • Diffraction effects... Shrinking the aperture Adding a lens Object Lens Film ―circle of confusion‖ A lens focuses light onto the film • There is a specific distance at which objects are ―in focus‖ – other points project to a ―circle of confusion‖ in the image • Changing the shape of the lens changes this distance 2 Lenses Thin lenses Object Lens Film Lens Aperture Film Focal Focal point point Optical center (Center of projection) Focal length A lens focuses parallel rays onto a single focal point Not quite right… Thin lens equation: • focal point at a distance f beyond the plane of the lens – f is a function of the shape and index of refraction of the lens • Aperture of diameter D restricts the range of rays • Any object point satisfying this equation is in focus – aperture may be on either side of the lens • What is the shape of the focus region? • Lenses are typically spherical (easier to produce) • How can we change the focus region? • Thin lens applet: http://www.phy.ntnu.edu.tw/java/Lens/lens_e.html (by Fu-Kwun Hwang ) Thin lens assumption Depth of field Aperture Film The thin lens assumption assumes the lens has no thickness, but this isn’t true… Object Lens Film f / 5.6 Focal point f / 32 Changing the aperture size affects depth of field By adding more elements to the lens, the distance at which a scene is in focus can be made roughly planar. -
L E N S E S & a C C E S S O R I
P. 4 P. 5 P. 6 P. 7 Scott Grant / Hai Tre / Jeff Carter / Gathot Subroto / Canada Vietnam UK Indonesia P. 8 P. 9 P.10 Matt Hart / Bert Stephani / Max De Martino / UK Belgium Italy P.11 P.12 P.13 P.14 Omar Z Robles / Simone Sbarglia / Pål Laukli / LS Trung / U.S.A. Italy Norway Vietnam P.15 P.16 P.17 Yonghui Wang / Supalerk Fabian De Backer / China Narubetkrausee / Belgium Thailand P.18 P.19 P.20 Taeyoung An / Joe Ng / Chalit Padoongcheep / Korea Canada Thailand P.21 P.21 Torwong Salwala / Giulia Torra / Thailand Italy Cover_P.2-3 Jonas Dyhr Rask / Denmark Specifications are subject to change without notice. LENSES & ACCESSORIES For more information, please visit our website: http://www.http://fujifilm-x.com/en/accessories/ c 2016 FUJIFILM Corporation P2-3/P36 The vision of the X Series, the choice for X Series owners A collection of creativity-oriented lenses, which complement the X-Trans CMOS sensor perfectly and eliminate the low-pass filter for ultimate sharpness. X Mount Lenses _ P.4-21 Accessories _ P.23-29 Technology _ P.30-33 Specifications _ P.34-35 2 3 P4-5/P36 XF14mmF2.8 R XF16mmF1.4 R WR X-T2 : F11 1/4 sec. ISO200 Scott Grant / Canada High resolving power across the frame from the centre to the edges. This ultra-wide-angle lens, which has a diagonal angle of view greater than 90°, produces extraordinary images. Distortion has been kept to a measured value of zero, with sharpness right across the frame, even when the subject is near the edges. -
TECHSPEC® Fixed Focal Length Lenses
Edmund Optics® BROCHURE FIXED FOCAL LENGTH LENSES ® COPYRIGHT 2017 EDMUND OPTICS, INC. ALL RIGHTS RESERVED 7/17 RIGHTS RESERVED ALL 2017 EDMUND OPTICS, INC. ® COPYRIGHT INNOVATION STARTS HERE . Global Design & Support | Rapid Prototyping Volume Manufacturing & Pricing Contact us for a Stock or Custom Quote Today! USA: +1-856-547-3488 | EUROPE: +44 (0) 1904 788600 ASIA: +65 6273 6644 | JAPAN: +81-3-3944-6210 www.edmundoptics.com/fixed-focal UC SERIES FIXED FOCAL LENGTH LENSES • Ultra-Compact (UC) Form Factor • 4K Resolution Designed for Small Pixels (≤2.2µm) • Optimized for 1/2•5" Sensors and Supports up to 1/1•8" Our ultra-compact, TECHSPEC® UC Series Fixed Focal Length Lenses are designed to optimize performance, cost, and size without sacrificing quality or feel. Designed for pixels that are ≤2.2μm, these lenses provide high levels of resolution (>200 lp/mm) across the sensor and are compatible with all standard C-Mount cameras. TECHSPEC® UC Series Fixed Focal Length Lenses feature focus and iris adjustments, as well as re- cessed set screws, and are manufactured for use at typical machine vision working distances. While they are optimized for 1/2.5" sensors, many focal lengths will work on sensors up to 1/1.8". The TECHSPEC® UC Series lenses are an outstanding option for use on all smaller format camera sensors, along with both short and long working dis- tance applications, making them ideal for inspection, factory automation, biomedical devices, and a broad range of other applications. Dimensions Units: mm Focal Length A B C D Filter Thread Focus Adjustment Iris Locking Screw Iris Adjustment Focus Locking Screw C-Mount 4mm 40 40.6 30 2.8 M62.0 x 0.75 with required filter adapter #33-308 6mm 36 40.9 30 3.2 M34.0 x 0.5 Max. -
Tele Vue-60 Operating Guide
Qwik-Point Installation Instructions: TV60OG 1003 PRICE $5.00 Printed in U.S.A. 1) Remove the 2 but- ton head screws from the dew shield with a 1/8” Allen key. OPERATING GUIDE (You won’t be needing the screws anymore.) 2) Attach the Qwik- Tele Vue-60 Point adapter block using the socket-head cap screws and wrench supplied with the Qwik- Point (model QBT-1006). 3) Follow instructions packaged with Qwik-Point for alignment and use. Since the Qwik-Point installs on the dew shield (sometimes called Sun Shade), it can be rotated to any conve- nient angle. It stores in the Tele Vue-60 carrybag with out need to remove it. Optional equipment shown. 360mm f/6.0 APO REFRACTOR ® Tele Vue 32 Elkay Dr., Chester, New York 10918 (845) 469 - 4551 www.televue.com Visionary 16 OPERATING GUIDE 11. SPECIFICATIONS: Congratulations on purchasing the Tele Vue-60 APO telescope. We worked hard Type 2-element APO refractor to ensure that the Tele Vue-60 embodies all the performance and features of the fi nest Clear Aperture 2.4 inches (60mm) astronomical-quality telescopes along with the compact size, ease-of-use, and versatility Aperture Gain 73, compared to a 7mm eye pupil of a top spotting scope. Please take the time to read this operating guide to familiarize Focal Length 14.2 inches (360mm) yourself with the various parts, operating suggestions and care instructions that will enable Focal Ratio f/6 you to obtain maximum enjoyment from your new Tele Vue-60. Resolution 1.9 arc-sec.