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MarkWard 27 Sep 2017 Logbook 17 01 2018 Lots of investigation into vessel leaks, investigations done/tests Gas system control testing Few features ...
Star Matching Algorithm Original Image (simulated) Adjusted Image moved in x direction by 10 pixels: Star Matching Algorithm then matches stars to one another by using ...
Accelerator Journal Club The accelerator journal club meets once every two weeks in (room to be determined), where the accelerator group meetings are held the alternating ...
Star Simulation Stot distributed using Pareto distribution Star evaluated in a box, so runs quicker Gaussian noise added to background in addition to Poisson ...
import numpy as np import random as r import matplotlib.pyplot as plt from astropy.io import fits import math as m import scipy as sc #from scipy.stats import ...
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Fixed error in the star simulation were getting pixel values way bigger than 65,000. This was because of the Stot distribution used. Last week, I used the scipy ...
Star Field Simulation Stot distribution changed to a skewed Gaussian so there are more dim stars than bright stars Shape function fixed to be more realistic. Adds ...
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Background 301x301 401x401 Star finder Star finder on simulated data Analysis of Observation 1 Observation 1 image is saturated. Other profile taken of same star ...
from astropy.io import fits from scipy.optimize import curve fit import glob from photutils import CircularAperture BLACK 0 def OpenImageHist(filename): ...
15.11.17 HPTPC Sensitivities: Since the last group meeting I've run spectral function fake data fits for ND280 in Pmu cosTheta and Pp cos Theta. HPTPC Pmu Tmu ...
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Background Analysis Alpha persei image median plotted of 65x65 box centered around each pixel . . . . . . . . . . . . . . 101x101 201x201 . . . . . . . . . . ...
My links: My activities PP.JAI.NewClicBpm CTF3 prototype second generation edit
Observation 1 We took two images of the double cluster: NGC869, NGC884, with two different cameras, with different fields of view. Star Simulation Main aim this ...
Log of Observation 1: Academic Present: Prof S BoogertStudents Present: Rebekah Chafer, Luna BorellaWeather Conditions: Mostly clear, some cloudTime: 17:00 22 ...
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My Links ATasteOfTWiki view a short introductory presentation on TWiki for beginners WelcomeGuest starting points on TWiki TWikiUsersGuide complete ...
My Links ATasteOfTWiki view a short introductory presentation on TWiki for beginners WelcomeGuest starting points on TWiki TWikiUsersGuide complete ...
My Links ATasteOfTWiki view a short introductory presentation on TWiki for beginners WelcomeGuest starting points on TWiki TWikiUsersGuide complete ...
My Links ATasteOfTWiki view a short introductory presentation on TWiki for beginners WelcomeGuest starting points on TWiki TWikiUsersGuide complete ...
My Links ATasteOfTWiki view a short introductory presentation on TWiki for beginners WelcomeGuest starting points on TWiki TWikiUsersGuide complete ...
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My Links ATasteOfTWiki view a short introductory presentation on TWiki for beginners WelcomeGuest starting points on TWiki TWikiUsersGuide complete ...
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Star Field Simulation Attempted two things this week: Variations in brightness of star Statistical Fluctuations Stot was uniformly distributed over a chosen maximum ...
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Star Field Simulation: First a random position function was made for a variable canvas size and number of stars. At this point, the stars are just points. Next, a ...
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Added error bars to the Histogram Error bars are small We plotted the new hypothesis mean mean0 mu t , however since our data was all over the place we used the ...
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Topic revision: r5 - 15 Nov 2006 - TWikiContributor

 
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