Astronomy image mosaic R.I.T Bo Mu. Project Goals Mosaic 2MASS images and Chandra X-ray images Visualize the overlay result Reposition and register display.

Slides:



Advertisements
Similar presentations
Supplementary slideshow Image capture and processing. A representative optic nerve cross section is presented to illustrate each step of the image capturing.
Advertisements

Applications of one-class classification
Mid-Infrared Variability and Mass Accretion Toward NGC2264 Protostars Susan Terebey CSULA Dept of Physics & Astronomy Ann Marie Cody, Luisa M. Rebull,
Welcome to IT-Training -We’re here to teach you PowerPoint-
Synchrotron Diffraction. Synchrotron Applications What? Diffraction data are collected on diffractometer beam lines at the world’s synchrotron sources.
Optical Astronomy Imaging Chain: Telescopes & CCDs.
Tecnológico de Monterrey Campus Estado de México Multimedia BS2001 MTI Fernando Carlos Rivero I. The interface.
ASSESSMENT OF DAYLIT GLARE PARAMETERS WITH IMAGING LUMINANCE MEASURING DEVICES (ILMD) AND IMAGE PROCESSING Porsch, Tobias; Schmidt, Franz.
Adobe Photoshop CS5 – Illustrated Unit B: Selecting Pixels
The Image Histogram.
Adobe Photoshop CS5 – Illustrated Unit B: Selecting Pixels.
Real-time Embedded Face Recognition for Smart Home Fei Zuo, Student Member, IEEE, Peter H. N. de With, Senior Member, IEEE.
Multi video camera calibration and synchronization.
1 Color Segmentation: Color Spaces and Illumination Mohan Sridharan University of Birmingham
Segmentation Divide the image into segments. Each segment:
Imaging Science FundamentalsChester F. Carlson Center for Imaging Science The LASP* at RIT’s Center for Imaging Science *Laboratory for Astronomy in Strange.
DIP Realized by IDL Author: Ying Li Course: computer for imaging science.
California Car License Plate Recognition System ZhengHui Hu Advisor: Dr. Kang.
The ICE Tool Feng Wen Qi Yuan Kin Wah Leung. Presentation Overview  Project goal  Interactive GUI  Introduce image enhancement techniques  Integration.
Real-Time Face Detection and Tracking Using Multiple Cameras RIT Computer Engineering Senior Design Project John RuppertJustin HnatowJared Holsopple This.
Can people meet from 2:40 to 3:30 on Tuesday, September 5?
Light Field. Modeling a desktop Image Based Rendering  Fast Realistic Rendering without 3D models.
1 Motivation Video Communication over Heterogeneous Networks –Diverse client devices –Various network connection bandwidths Limitations of Scalable Video.
Surgical Planning Laboratory -1- Brigham and Women’s Hospital Slicer Training 1: Loading and Viewing Data.
The Digital Image.
Digitized Sky Survey Update Brian McLean : Archive Sciences Branch / Operations and Engineering Division.
→ Herschel data for absolute beginners Herschel Science Centre (ESAC)
P olarized R adiation I maging and S pectroscopy M ission Probing cosmic structures and radiation with the ultimate polarimetric spectro-imaging of the.
M81 – Bode’s galaxy M82 – Cigar Galaxy. ASTR 2401 Goal Target selection Object information Data collection Image calibration Processing Mosaicing Perils.
Machine Vision for Robots
HW 2 Discussion Remember, everything is still an illusion.
Long-Wave Infrared and Visible Image Fusion for Situational Awareness Nathaniel Walker.
© 1999 Rochester Institute of Technology Introduction to Digital Imaging.
1 Sun Tracking Stablility Through Imaging Tyson Seto-Mook Institute for Astronomy.
15 October Observational Astronomy Direct imaging Photometry Kitchin pp ,
Calibration & Measurements. Calibrating the System Before we can make any measurements we need to calibrate our imaging system to create real world numbers.
The T-A-P survey: NGC1333 data Davis, Scholz, Lucas, Smith, Adamson (MNRAS, 387, 954)
03/05/03© 2003 University of Wisconsin Last Time Tone Reproduction If you don’t use perceptual info, some people call it contrast reduction.
UTILIZING HIGH ALTITUDE BALLOON PLATFORMS FOR SUPER RESOLUTION IMAGING JACK LIGHTHOLDER MENTOR: DR. TOM SHARP SPACE GRANT SYMPOSIUM APRIL 18 TH, 2015.
7 elements of remote sensing process 1.Energy Source (A) 2.Radiation & Atmosphere (B) 3.Interaction with Targets (C) 4.Recording of Energy by Sensor (D)
WFIRST 10  m Pixel Pitch Detector Considerations March 10, /10/
Class 4 : Basic properties of stars
The Table Lens: Merging Graphical and Symbolic Representations in an Interactive Focus+Context Visualization for Tabular Information Ramana Rao and Stuart.
Mosaic Creator Lance Finfrock CS 470. Introduction A Mosaic is hundreds or thousands of pictures comprised to make one picture.
MedIX – Summer 07 Lucia Dettori (room 745)
VisDB: Database Exploration Using Multidimensional Visualization Maithili Narasimha 4/24/2001.
Large Area Surveys - I Large area surveys can answer fundamental questions about the distribution of gas in galaxy clusters, how gas cycles in and out.
BOĞAZİÇİ UNIVERSITY DEPARTMENT OF MANAGEMENT INFORMATION SYSTEMS MATLAB AS A DATA MINING ENVIRONMENT.
Oct 021 Outline What is a widget? Buttons Combo boxes Text components Message boxes.
Machine Vision Introduction to Using Cognex DVT Intellect.
Chapter 3 Response Charts.
PROJECT#3(b) Astrocyte Analysis
M. Pilar Esquej, XMM-Newton European Space Astronomy Centre Page 1 Status of the XMM-Newton Slew Survey P. Esquej, R. Saxton, B. Altieri, A. Read, M. Freyberg,
Video Tracking G. Medioni, Q. Yu Edwin Lei Maria Pavlovskaia.
By: David Gelbendorf, Hila Ben-Moshe Supervisor : Alon Zvirin
Intelligent Robotics Today: Vision & Time & Space Complexity.
Rapture of the Deep Sky Mel Ulmer Dept of Physics & Astronomy Northwestern University This talk posted on
Digital Image Processing Image Enhancement in Spatial Domain
What you need: In order to use these programs you need a program that sends out OSC messages in TUIO format. There are a few options in programs that.
Zhaoxia Fu, Yan Han Measurement Volume 45, Issue 4, May 2012, Pages 650–655 Reporter: Jing-Siang, Chen.
Motion tracking TEAM D, Project 11: Laura Gui - Timisoara Calin Garboni - Timisoara Peter Horvath - Szeged Peter Kovacs - Debrecen.
SalsaJ (Such a Lovely Software for Astronomy) Practical Session.
Chapter 3: I Need a Tour Guide (Introduction to Visual Basic 2012)
Chapter 14 Spiral Galaxy.
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.
Resolution Resolution: 6 x 4.
Detecting Dark Clouds in the Galactic Plane with 2MASS data
Observational Astronomy
Boyce Astro: Online Catalogs BRIEF Boyce Astro:
(AO) Observations of the Galactic Center
Presentation transcript:

Astronomy image mosaic R.I.T Bo Mu

Project Goals Mosaic 2MASS images and Chandra X-ray images Visualize the overlay result Reposition and register display images relative to reference points

Background 2MASS 1. 2 Micron All Sky survey. 2. High resolution infrared Image. 3. Potential to detect members nearby(d<2kpc) cluster. 4. color is helpful to distinguish stars FOR MORE INFO... pegasus.phast.umass.edu/ A parsec is the distance at which a star has a parallax of 1 arcsec.

Background Chandra X-ray image 1. Represent powerful - Young,low-mass star are highly luminous and variable X-ray source 2. Overcome the ambiguities in crowed regions near the galactic plane. FOR MORE INFO...

Trade Off 2mass,CXO High resolution(~0.1”), Low sensitivity Optical Image Low resolution(5’’), High sensitivity Need to Combine with 2mass, CXO and XMM/Newton(optical) image

Example NGC2362

Challenge Easy? Coordination known. No! 1. Coordination has limited accuracy 2. Multi-resolution 3. Background differs significantly 4. Bad Pixel effect

Solution Refine coordination system by reference point Multi-resolution Algorithm (wavelet?) Back ground equalization Subtract the dark image.

Expectation Visualization Contrast adjust interactively Zoom Some filters to help investigate image.

Current Status Astronomy image file format –fits file –keyword (naxis,crpix,crval,crot,cdelta) in header Process: Structure array to save multi image data.

Current Status Algorithm –Read into multi astro images with fits format –Calculate max,min border –Adjust the order of images according to the coordinates(RA,DEC) –Data Structure

A B C A B C Data relation

Current Status Algorithm –Multi-resolution. Use shift function to solve it. More complex, try wavelet Algorithm. –Try Crosscorrealtion –Calculate the gray level(Average back ground or histogram. Value –1,0, ,>10000) –Geometric correction(option) –Redefine the data structure –Write into a new fits file

GUI Read multifiles into a structure by >>Dialog_Pickfile(,/multiple) >>Readfits Initialize interface Dynamic distribute display window according to the number of images Display images with mouse position and astronomy coordinates.

GUI

GUI GUI: menu, label, text,slider display window,dialog Slider to adjust image contrast Solve the trouble on displaying multiimages and capture mouse focus among subwindows. Working on zooming image

GUI Plan to design file select dialog

Thanks!