fitting
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B_Hose Fitting_Socket
winner的样本,即永华的资料
Winner®
软管接头 Hose Fitting
套筒 Socket
winner的样本,即永华的资料
01100
国产一层编织软管套筒
FERRULE FOR CHINA 1-WIRE HOSE
B-01
winner的样本,即永华的资料
01200
国产二层编织软管套筒
FERRULE FOR CHINA 2-WIRE HOSE
B-02
winner的样本,即永华的资料
01300
国产三层编织软管套筒
FERRULE FOR CHINA 3-WIRE HOSE
B-03
winner的样本,即永华的资料
00100
SAE100R1A/DIN20022 1ST软管套筒
FERRULE FOR SAE100R1A/DIN20022 1ST HOSE
B-04
winner的样本,即永华的资料
00200
SAE 100 R2AT/EN 853 2SN软管套筒
FERRULE FOR SAE 100 R2AT/EN 853 2SN HOSE
B-05
winner的样本,即永华的资料
00110
SAE100R1AT/EN 853 1SN软管套筒
FERRULE FOR SAE100R1AT/EN 853 1SN HOSE
B-06
winner的样本,即
Fitting Parameterized Three-dimensional Models to Images
Model-based recognition and motion tracking depends upon the ability to solve for projection and model parameters that will best fit a 3-D model to matching 2-D image features. This paper extends current methods of parameter solving to handle objects with
FittingParameterizedThree-DimensionalModelstoImages
DavidG.Lowe
ComputerScienceDepartment
UniversityofBritishColumbia
Vancouver,B.C.,CanadaV6T1Z4
Email:lowe@cs.ubc.ca
Abstract
Model-basedrecognitionandmotiontrackingdependsupontheabilitytosolveforprojectionandmodelparametersthatwil
Fitting the spectrum of the X-ray background the effects of high metallicity absorption
Recent work by Risaliti et al.(1999) suggests that more than half of all Seyfert 2 galaxies in the local universe are Compton-thick (N_H > 10^24 cm^-2). This has implications for AGN synthesis models for the X-ray background (XRB), the flexibility of which
Mon.Not.R.Astron.Soc.000,000–000(0000)Printed1February2008
A(MNLTEXstyle lev1.4)
FittingthespectrumoftheX-raybackground:thee ects
ofhighmetallicityabsorption
R.J.WilmanandA.C.Fabian
InstituteofAstronomy,MadingleyRoad,CambridgeCB30HA
1February2008
arXiv:astro-ph/9907204v1 15 Jul