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TrigMC software release coordination: PTD's logbook May 2018 Notes Use reverse chronological order. For each shift date show the NEW MRs, and any related relevant ...
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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 ...
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Non collision background for ATLAS detector The main task of the group is characterisation and migitation of non collision background in ATLAS analyses. Main sources ...
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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 ...
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Physics motivation of HE LHC Particle physics accelerators in the current days focus on achieving better precision on various physics parameters defined by proved ...
Work on Atlas non collision beam background using the LHC and HL LHC settings. NCB Work on the NCB HE LHC Work on HE LHC HelenaPikhartova1 01 Feb ...
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Error estimate Main squence fitting Using the magnitude distance equation, where the offset for the first 2 are 6.3 and the offset for the third is 6 we find a distance ...
Meetings 20171013 meeting 20171020 meeting 20171027 meeting 20171103 meeting 20171110 meeting 20171117 meeting 20171124 meeting ...
Finding the best radius of the aperture circle. Simulated a star with 2D Gaussian with a sigma of 2 pixels, with no background. Then, I gradually increased the radius ...
Error estimate Green Filter HR Diagram LunaBorella 13 Feb 2018
Error estimate Blue filter Green Filter: Removing Stars due to proximity #radius apart, not sigma. LunaBorella 08 Feb 2018
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Error estimate Using star fitting of a single star e.g Found Flux plotted hist Blue filter Green Filter Red filter: Star Matching Red UnmatchedGreen Matched Zoomed ...
My Topics Accelerator Journal Club a bi weekly meeting of the JAI group where we read and discuss relevant articles in the field in order to gain wider knowledge ...
My links: My activities Accelerator Journal Club My work edit
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MarkWard 27 Sep 2017 Logbook 24 01 2018 This will be my last wednesday meeting :( Sorry to be leaving you all :( I will be joining TRIUMF working on LXe optical ...
Professional stuff RIS Profile Academic diary HEP name entry scholar Public.StewartBoogertPhotos Photos Research related Dropbox ...
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Observation Took multiple photos of Pleiades in small field of view in different filters. Then moved to a wider field of view, no filter. Aiming to use this for HR ...
Pleiades is too wide to get in one shot with normal telescope. Would take approximately 25 tiles to get whole cluster. Therefore, the plan is to use the smaller telescope ...
Academic Present: Dr Laurie NevayStudents Present: Luna Borella, Rebekah ChaferWeather Conditions: ClearTime: 22:40 1:50Targets: Betelgeuse Pleiades Cluster in ...
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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Physics WebpagesRHUL WebpagesCampus Connect • Royal Holloway, University of London, Egham, Surrey TW20 0EX; Tel/Fax +44 (0)1784 434455/437520

Topic revision: r5 - 15 Nov 2006 - TWikiContributor

 
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