نتایج جستجو برای: lsb matching

تعداد نتایج: 103032  

2014
G. Raj Kumar M. Maruthi Prasada Reddy T. Lalith Kumar

Steganography is the art or practice of concealing a message, image, or file within another message, image, or file. In steganography, there is a technique in which the least significant bit is modified to hide the secret message, known as the least significant bit (LSB) steganography. Least significant bit matching images are still not well detected, especially, at low embedding rate. In this ...

2005
Stark C. Draper Prakash Ishwar David Molnar Vinod M. Prabhakaran Kannan Ramchandran Daniel Schonberg David A. Wagner

We consider here the class of probability mass-function (PMF) based detectors of least significant bit (LSB) embedded steganography. That is, in this paper we investigate the use of frequency counts of pixel intensities as a statistic for tests detecting the presence of hidden messages. We focus on LSB replacement (though we briefly consider LSB matching) embedding as it is a simple technique w...

Journal: :IEEE Access 2022

This paper presents a novel image hiding method with improved block matching way and high embedding capacity that allows the important (IM) to be several times larger than cover image. Multi-layered least-significant-bit (LSB) planes of (CI) are obtained for constructing candidate block-matching set (CBMS) by using features fusion which consists texture wavelet transform gray leve...

Journal: :Fundam. Inform. 2008
Yu-Chen Hu Chih-Chiang Tsou Bing-Hwang Su

A novel LSB-based image-hiding scheme that embeds secret data into the grayscale cover image is proposed in this paper. Several LSB-based image hiding schemes such as simple LSB substitution technique, optimal LSB substitution technique, greedy LSB substitution technique, modulus LSB substitution technique had been proposed. To provide good image quality of the stego-image while requiring a low...

1998
Jeroen P.E. Gerritsen

We present N -body simulations of Low Surface Brightness (LSB) galaxies and their Interstellar Medium to investigate the cause for their low star formation rates (SFR). Due to their massive halos, stellar disks of LSB galaxies are very stable and thin. Lack of dust makes the projected edge-on surface brightness of LSB galaxies comparable to the projected edge-on surface brightness of dust-rich ...

2009
Andrew D. Ker Ivans Lubenko

WAM steganalysis is a feature-based classifier for detecting LSB matching steganography, presented in 2006 by Goljan et al. and demonstrated to be sensitive even to small payloads. This paper makes three contributions to the development of the WAM method. First, we benchmark some variants of WAM in a number of sets of cover images, and we are able to quantify the significance of differences in ...

Journal: :iranian journal of applied animal science 2013
m.m. mia m.a.m.y. khandoker s.s. husain m.o. faruque d.r. notter

the objective of this study was to evaluate genetic and phenotypic parameters for some reproductive traits of black bengal does. genetic parameters were estimated by residual maximum likelihood procedure, fitting an animal model ignoring maternal genetic or permanent environmental effects. the least-squares means of litter size at birth (lsb), litter size at weaning (lsw), litter weight at birt...

Journal: :International Journal of Computer Applications 2014

2014
Anum Javeed Zargar

Watermarking belongs to hide particular information, so that you can easily detect any tamper detection .It is used for confidenality, authentication and copy right protection. In this paper watermarking is done with the help of least significant bit technique (LSB).As LSB technique is used as it has less effect on image. This new algorithm is using LSB of original image and idoing ‘&&’ operati...

1999
M. Beijersbergen

We present results of broad band BVRI observations of a sample of galaxies with a low surface brightness (LSB) disk and a bulge. These galaxies are well described as exponential disks and exponential bulges with no preferred value for either scale length or central surface brightness. The median B band disk scale length is 12.6 kpc (H0 = 75 km s−1 Mpc−1) which is much larger than scale lengths ...

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