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TileSaw(Qep_60010)

Course: P 08605, Fall 2009
School: RIT
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Speed Dual 10" Tile Saw Rips tile 18" square, 12" diagonally # 60010 PRODUCT INFORMATION Capacitor start 2HP motor for extra power Automatic thermal overload protection Permanently attached rail assembly to saw frame for improved, precise cutting Rustproof, removable plastic water tray for easy cleaning Three diagonal support bars for maximum support of water tray Limited one year warranty Specifications: Item No.: #60010 Motor: 120V-60Hz Horsepower: Powerful 2HP RPM: 1750/2450 (dual speed) AMP: 15 Blade 6"-10" Range: Arbor: 5/8" Depth of Cut: 3 3/4" Length of Cut: 18" square 12"diagonally Weight: 99 lbs. Cutting Table: 161/4"L x 101/2"W Includes Standard Accessories: Stand with rear wheels (brakes) 10" standard continuous rim wet diamond blade Water pump Miter Block R...

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c043_s03_sov_data_totals_sv_sr_sos.txt

Berkeley - C - 043

+-+-+-+-+-+-+-+-+-+| name | sos_total | sv_total | sr_total | diff_sv_sr | diff_sr_sos | diff_sv_sos | election | county |+-+-+--+-+-+-+-+-+-+| ABSVOTE | 0 | 0 | 0 | 0 | 0 | 0 | s

hand0.pdf

NJIT - CIS - 786

Alex Gerbessiotis CIS 786-107:Parallel Computation Sep 1, 2004 Course InformationFall 2004 Page 1A course on aspects of parallel computing involving clusters and networks of PC workstations. Parallel algorithms are introduced in the context of si

hand0.ps

NJIT - CIS - 786

%!PS-Adobe-2.0 %Creator: dvips(k) 5.86 Copyright 1999 Radical Eye Software %Title: hand0.dvi %Pages: 1 %PageOrder: Ascend %BoundingBox: 0 0 612 792 %DocumentFonts: CMCSC10 CMR12 CMTT12 CMSY8 %EndComments %DVIPSWebPage: (www.radicaleye.com) %DVIPSComm

f726_midterm_s03.pdf

Ohio State - FIN - 726

Finance 726 MidtermProfessor Helwege Spring 2003You have the entire class period to finish this quiz. You may use a calculator, scrap paper, and a writing tool to complete the test. You may hand in the scrap paper (with your name on it) if you th

Drug Model Solns.pdf

Colorado State - M - 331

M34331Drug Model Project1. (a) Solve the two initial value problems for x t and y t and plot them on the same graph in the following three cases: k 1 k 2 , k 1 k 2 , and k 1 k 2 . In each case, describe what the plot tells you about the drug l

Drug model.pdf

Colorado State - M - 331

Absorption of Medications When you take a pill to obtain medication, the pill first goes into your stomach and the medication passes into your GI tract. From there the medication is absorbed into your bloodstream and circulated through your body befo

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Colorado State - M - 331

>restart :First, load the library that contains the LP software>with Optimization :y = Dark crudeNow we'll do the crude oil production problem: x = Light crude Minimize the cost function Subject to : C=25$x C 17$.21$x C .55$ R 3 y .50$x

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Colorado State - M - 331

M 331Linear Programming ProblemsThese problems will be due Monday Oct 16. You should have all the computing done by Friday Oct 13 but the Monday due date will give you the weekend to think over what you want to say in problem 4. I am especially i

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Colorado State - M - 331

Solutions to LP Problems >M331with Optimization ;ImportMPS, Interactive, LPSolve, LSSolve, Maximize, Minimize, NLPSolve, QPSolveProblem 1 MinimizeCost = 30(x11+x12+x13+x14) + 50(x21+x22+x23+x24) + 80(x31+x32+x33+x34) x11+x12+x13+x14 <= 50 x2

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Colorado State - M - 331

M 331Exam on Nonlinear Optimization.1. A beer company wants to make their cans so that the upper half is a cylinder and the lower half is a rectangular box having a square base. The circular base of the upper cylinder is perfectly inscribed in th

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Colorado State - M - 331

Assignment M331Scaling Problems 1. The equations X t k1X t , X0 A Y0 0 Y t k2Y t k1X t ,model the movement of a drug from the digestive system to the bloodstream. The model involves three parameters, k 1 , k 2 and A. Scale the problem to reduce

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Colorado State - M - 331

ScalingThe purpose of developing mathematical models for physical systems is to use them to predict or understand the behavior of the physical system by examining the behavior of the solution to the mathematical model as the inputs to the model are

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Colorado State - M - 331

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ch5[1].pdf

Colorado State - M - 331

"331boo 2005/8/ page 88C H A P T E R5Empirical Modeling with Data FittingIn this chapter the model building is empirical in nature, i.e., the functional form of the relationship between the dependent and independent variables is found by direc

ch6[1].pdf

Colorado State - M - 331

C H A P T E R6Modeling with Discrete Dynamical Systems6.1 INTRODUCTION One of the most exciting areas of modeling concerns predicting temporal evolution. The main question that is posed in this setting is how do variables of interest change over

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Colorado State - M - 331

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SylF09.doc

ASU - MAT - 343

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bat.txt

Berkeley - ASTRO - 00146970

-19.000000 -3.6399999 558.97861 169.77610 -3.6399999 -1.7200000 2876.7947 536.13983 -1.7200000 0.19999999 4746.4555 550.14303 0.20000011 2.1200001 5133.2623

both.txt

Berkeley - ASTRO - 00146970

-19.000000 -3.6399999 558.97861 169.77610 -3.6399999 -1.7200000 2876.7947 536.13983 -1.7200000 0.19999999 4746.4555 550.14303 0.20000011 2.1200001 5133.2623

gcn.txt

Berkeley - ASTRO - 00146970

# Time [days] Mag Magerr Band Uplim Ref 0.00427 15 -0.2 I no GCN3655 0.01720 -0.2 R no GCN3657 0.01736 -0.2 R no GCN3662 0.0

gcnR.txt

Berkeley - ASTRO - 00146970

1486.08 -0.2 0 no GCN3657 1499.9 -0.2 0 no GCN3662 3371.33 18.6 0.2 R no

gcnR_flux.txt

Berkeley - ASTRO - 00146970

1486.08 7.200302e+03 0.000000e+00 no GCN3657 1499.9 7.200302e+03 0.000000e+00 no GCN3662 3371.33 2.174456e-04 4.005497e-05 R no

gcnR_flux_ul.txt

Berkeley - ASTRO - 00146970

-19 1 1

index.txt

Berkeley - ASTRO - 00146970

15.360001 21.120001 5.5570212 0.94341827 728.65890 21.120001 23.040001 8.4765915 0.0000000 480.10577 23.040001 120.96000 10.555121 -0.92309061 2433.7325

index2.txt

Berkeley - ASTRO - 00146970

15.3600 21.1200 2.36748 0.983370 23.0400 120.960 -1.34270 0.187139 120.960 213.416 -6.42014 1.01643 213.416 440.889 -2.41914 0.160156 440.889 23194.7 -1.2977

modl.txt

Berkeley - ASTRO - 00146970

chi^2/nu= 235.05327 / 180The fit is rejectable at 99.635965 % Confidence -3.64000 -1.72000 3609.8236 -1.72000 0.200001 4009.1988 0.200001 2.12000 4406.1966 2.12000 4.0400

ned.txt

Berkeley - ASTRO - 00146970

<html><head><title>Your NED Search Results</title></head><body background="/pics/NEDbgHelp.gif" bgcolor="#FFFFFF"><center>NASA/IPAC&nbsp;<font size=6 color="#CC

xrt.txt

Berkeley - ASTRO - 00146970

193.91 194.416 19.3653 6.4551194.416 194.928 19.1384 6.37945194.928 196.038 18.2948 4.28912196.038 197.305 16.0278 3.75764197.305 197.72 23.6117 7.87056197.72 198.337 15.8814 5.29381198.337 199.009 16.6933 5.43247199.009 199.538 19.8646 6.5478

2mass_radec.txt

Berkeley - ASTRO - 00146970

#ra dec hmag dhmag253.434774 -28.630537 13.948 0.050253.434527 -28.629358 11.313 0.029253.436668 -28.625603 14.008 0.021253.410792 -28.626026 16.606 0.141253.407508 -28.627878 16.193 0.101253.409090 -28.627268 14.739 0.047253.416261 -28.626024

arf_pc.txt

Berkeley - ASTRO - 00146970

;instrument XRT;exposure 43935.123;xunit kev;bintype counts 0.0000000 0.0049999999 13.699265 1.00000 0.0049999999 0.0099999998 13.748119 1.00000 0.0099999998 0.015000000 13.796972 1.0

arf_wt.txt

Berkeley - ASTRO - 00146970

;instrument XRT;exposure 205.02987;xunit kev;bintype counts 0.0000000 0.0049999999 14.544516 1.00000 0.0049999999 0.0099999998 14.596416 1.00000 0.0099999998 0.015000000 14.648316 1.0

dss_radec.txt

Berkeley - ASTRO - 00146970

#ra dec rmag drmag253.719301-28.63056718.1380.154253.533132-28.63073817.7910.112253.446271-28.63072617.6680.100253.159740-28.63031717.6240.096253.157735-28.63031517.7370.106253.689486-28.63053417.3120.076253.600854-28.630578

hardVmag.txt

Berkeley - ASTRO - 00146970

chi^2/nu= 76.473382 / 322.000The fit is rejectable at 2.5688205e-47 % Confidence#index t1 t2 fade_index delta_mag_pk hindex dhindex rate1 drate1 rate2 drate2 logr dlogr 0 0.1939 0.2051 -2.97 0.0 -2.95 5.95 6.47E+0

hardness.txt

Berkeley - ASTRO - 00146970

# t1 t2 hardness error 0.19391000 0.19603800 0.45432251 0.14750030 0.19603800 0.19772000 0.20438850 0.18719565 0.19772000 0.19953800 0.12611560 0.18855479 0.19953800 0.20173200

pc_evlist.txt

Berkeley - ASTRO - 00146970

output00146970000_999/sw00146970000xpcw4po_cl.evtoutput00146970001_999/sw00146970001xpcw4po_cl.evtoutput00146970003_999/sw00146970003xpcw3po_cl.evtoutput00146970003_999/sw00146970003xpcw4po_cl.evtoutput00146970004_999/sw00146970004xpcw4po_cl.evt

radvt.txt

Berkeley - ASTRO - 00146970

# t1 t2 dt rad_min rad_max cts err scl bg bg_rat wt 0.193910 0.194416 0.000506 0. 16. 9.00 3.00 0.918476 0.000000 0.348314 1 0.194416 0.194928 0.000512 0. 16. 9.00

radvt.txt_haar_mod.txt

Berkeley - ASTRO - 00146970

tmin 128.60045tmin 1031.2218 2064.0582 33128.471 0.21688333 0.023000630 8tmax 46869.069

radvt0.txt

Berkeley - ASTRO - 00146970

# t1 t2 dt rad_min rad_max cts err scl bg bg_rat wt 0.193910 0.194416 0.000506 0. 16. 9.00 3.00 0.918476 0.000000 0.348314 1 0.194416 0.194928 0.000512 0. 16. 9.00

spec_pc.txt

Berkeley - ASTRO - 00146970

# tmin tmax 0.324104 3385.42 [ksec];instrument XRT;exposure 41436.321;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.000000 0

spec_pc_bg.txt

Berkeley - ASTRO - 00146970

spec_wt.txt

Berkeley - ASTRO - 00146970

# tmin tmax 0.193910 4.75645 [ksec];instrument XRT;exposure 196.86733;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.000000 0

spec_wt_bg.txt

Berkeley - ASTRO - 00146970

wavdetect.txt

Berkeley - ASTRO - 00146970

Wavdetect Sources with S/N>3: # ra dec err ["] signif counts steady? -log10(Prob_steady) 0253.435698-28.3811270.16580.91127.3 0-531.6 1253.633184-28.5347640.44018.155.5 0-31.6 2253.670469-28.4859820.67611.327.7 0-23.2

wt_evlist.txt

Berkeley - ASTRO - 00146970

output00146970000_999/sw00146970000xwtw2po_cl.evtoutput00146970001_999/sw00146970001xwtw2po_cl.evtoutput00146970003_999/sw00146970003xwtw2po_cl.evtoutput00146970004_999/sw00146970004xwtw2po_cl.evtoutput00146970005_999/sw00146970005xwtw2po_cl.evt

bat_hdr.txt

Berkeley - ASTRO - 00146970

SIMPLE = T / file does conform to FITS standardBITPIX = 8 / number of bits per data pixelNAXIS = 0 / number of data axesEXTEND = T / FITS dataset may contain extensio

ep_fl_dat.txt

Berkeley - ASTRO - 00146970

# Ep dEp lprob lEiso dlEiso60.668 0.050 -1.19e-04 -9.850 0.09660.721 0.057 -4.32e-04 -9.850 0.09660.782 0.065 -8.18e-04 -9.850 0.09660.852 0.075 -1.29e-03 -9.850 0.09560.931 0.085 -1.88e-03 -9.750 0.14861.023 0.098 -2.61e-03 -9.800 0.11261.128

ep_flu.txt

Berkeley - ASTRO - 00146970

# Ep lEiso1.403 -8.8822.018 -8.94215.301 -9.04127.019 -8.97329.323 -9.06832.436 -9.26933.533 -9.16934.393 -9.06435.572 -9.15635.602 -9.15236.137 -9.04837.065 -9.15037.408 -9.16538.025 -9.04738.433 -9.05438.601 -9.03139.332 -9.40639.

ep_nfl_dat.txt

Berkeley - ASTRO - 00146970

# Ep dEp lprob lNiso dlNiso60.668 0.050 -1.19e-04 7.678 0.27360.721 0.057 -4.36e-04 7.678 0.27160.782 0.065 -8.18e-04 7.678 0.27160.852 0.075 -1.29e-03 7.678 0.27160.931 0.085 -1.88e-03 7.678 0.27161.023 0.098 -2.61e-03 7.678 0.27161.128 0.112

ep_nflu.txt

Berkeley - ASTRO - 00146970

# Ep lNiso1.404 9.2202.025 9.10915.388 8.71827.028 8.39829.305 8.02132.425 7.60433.510 8.40634.353 7.93935.540 7.61335.571 7.62536.117 7.93437.065 7.74837.415 8.19438.037 7.95938.447 7.75738.616 7.44139.352 7.89939.468 8.16039.750

swb_fit2.txt

Berkeley - ASTRO - 00146970

Spectra Extracted from tstart=-11.695 tstop=104.405(Trigger Time, GPS=805955367.280000, Redshift, z=0.0)Power-Law Model FitNorm@15keV 3.3212e-02 (2.6378e-02 4.0886e-02)alpha -1.8424 (-2.0413 -1.6498)Energy Fluence (15-350 keV) 5.6701e-06 (5.10

swb_slew_times.txt

Berkeley - ASTRO - 00146970

-300.28000 140.99460 151.17210 165.60360

swb_timeinfo_1s.txt

Berkeley - ASTRO - 00146970

#file=swb15-350lc.txt dt=1.0 tstart=-6.535 tstop=40.765#t90 dt90 t50 dt50 rt90 drt90 rt50 drt50 rt45 drt45 tav dtav tmax dtmax trise dtrise tfall dtfall cts cts_err pk_rate dpk_rate band 39.000 2.921 21.000 3.344 27.000 3

swb_trig1.txt

Berkeley - ASTRO - 00146970

# S/N T1 T2 T90 T50# Estimated T100 Interval: -11.695 104.405 T90= 101.480 19.3 -4.385 21.415 21.500 10.750 7.1 22.275 48.075 23.650 10.750 5.2 96.235 104.405

spec_pc.txt

Berkeley - ASTRO - 00146970

# tmin tmax 10.0000 3385.4225 [ksec];instrument XRT;exposure 40192.500;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.00000

arf_pc.txt

Berkeley - ASTRO - 00146970

;instrument XRT;exposure 42634.623;xunit kev;bintype counts 0.0000000 0.0049999999 13.915290 1.00000 0.0049999999 0.0099999998 13.964909 1.00000 0.0099999998 0.015000000 14.014527 1.0

spec_pc_bg.txt

Berkeley - ASTRO - 00146970

cs486lab4.pdf

Loyola Maryland - CS - 486

CS486 Lab 4: 3D shape modeling Due: Friday, March 29rd Objectives: To write our own glutDrawShape routines. The Lab: This lab will use the programs from Lab 3 for viewing an object at the origin. Part I. Extrusion Write a function that takes a polyl

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Colorado - MCDB - 2150

MCDB 215005: Problem Set 10 1MCD Biology 2150 - Problem Set 10:Here is the pedigree for a family with an inherited predisposition to a form of cancer. The filled symbols indicate cases of cancer. The stippled symbols are tumor biopsies from the i

215005PS11.doc

Colorado - MCDB - 2150

MCDB 215005: Problem Set 11 1MCD Biology 2150 - Problem Set 11:Due: April 28, 11:55 PMHere is data from a three point cross as practice before the final. Female flies that are phenotypically wild-type are heterozygous for each of three differe

215005PS3.doc

Colorado - MCDB - 2150

MCDB 215005 PS 3 pg. 1MCD Biology 2150 S05 - Problem Set 3: Due: February 3, 2002, 11:55 PM Questions 1 to 4 are a group. Read them all before solving: Question 1. You have isolated 8 his- yeast strains (numbered 1 through 8 in the grid below). Th

2150S05PS4.doc

Colorado - MCDB - 2150

MCDB 215005 PS 4 pg. 1MCD Biology 2150 - Problem Set 4: Due: February 17, 2005, 11:55 PM Question 1: A woman's mother has X-linked color blindness and this trait is recessive. The woman's father is not color blind. Her husband is not color-blind.