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ToneLib Zoom Don't let your pedal distract you from music. Best way to manage your Zoom processor Tonelib Zoom is an easy-to-use application which allows you to see, change and save all the settings in your Zoom r guitar pedal through your computer.

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Skip to main content. Download Center. Zoom Client for Meetings The web browser client will download automatically when you start or join your first Zoom meeting, and is also available for manual download here. Home Privacy policy Contact us guitarpatches. Slow Dancing in a Burning Room.

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Data Science Front Matter Pages Alarape, Ahmed O. Ameen, Kayode S. Adewole Pages Back to top. The book presents several hot research topics which include artificial intelligence and data science, big data analytics, Internet of Things IoT , information security, cloud computing, networking and computational informatics.

He received his B. He published more than 80 papers in indexed journals and international conferences. His research interests are data mining, information retrieval and machine learning.

He received his Ph. His research interests are networking, management network, virtualization. Mohammed Al-Sarem received the M. Therefore, detailed lens modeling is necessary to obtain the true properties of the lensed galaxies. Design of large zoom for visible and infrared optical system in hemisphere space.

In the field of space optical, the application of advanced optical instruments for related target detection and identification has become an advanced technology in modern optics. In order to complete the task of search in wide field of view and detailed investigation in small field of view, it is inevitable to use the structure of the zoom system to achieve a better observation for important targets.

The innovation of this paper lies in using the zoom optical system in space detection, which achieve firstly military needs of searched target in the large field of view and recognized target in the small field of view. The visible system has a zoom range of mm, a detection band of 0.

The MTF of the visible zoom system is above 0. The design results show that the system has a good image quality. Electronic magnification and perceived contrast of video. Electronic magnification of an image results in a decrease in its perceived contrast. The decrease in perceived contrast could be due to a perceived blur or to limited sampling of the range of contrasts in the original image.

We measured the effect on perceived contrast of magnification in two contexts: either a small video was enlarged to fill a larger area, or a portion of a larger video was enlarged to fill the same area as the original. Subjects attenuated the source video contrast to match the perceived contrast of the magnified videos, with the effect increasing with magnification and decreasing with viewing distance. These effects are consistent with expectations based on both the contrast statistics of natural images and the contrast sensitivity of the human visual system.

We demonstrate that local regions within videos usually have lower physical contrast than the whole, and that this difference accounts for a minor part of the perceived differences. We detail how the effects of magnification on perceived contrast can be measured while avoiding confounding factors. We have designed and fabricated a miniature microscope from off-the-shelf components and webcam, with built-in fluorescence capability for biomedical applications.

This mini-microscope has adjustable magnifications from X, achieves a resolution as high as magnification of 8X. The mini-microscope was able to chronologically monitor cell migration and analyze beating of microfluidic liver and cardiac bioreactors in real time, respectively. The mini-microscope system is cheap, and its modularity allows convenient integration with a wide variety of pre-existing platforms including but not limited to, cell culture plates, microfluidic devices, and organs-on-a-chip systems.

What collaborative process can teachers offer in order to stimulate their students' reading of and writing on Shakespeare's plays? How can new technologies contribute to facilitating the classroom experience?

The e Zoom Book eZB template was designed for teachers to create and share multi-level digital books called "e Zoom Books" that…. Magnifying image intensifier. Coil assembly for zoom operation produces axial magnetic flux density that decreases in strength from photocathode to target.

This results in magnification factor greater than unity. To extend magnification range, field is reversed in direction between object and image planes.

Optical design of laser zoom projective lens with variable total track. In order to project the laser command information to the proper distance , so a laser zoom projective lens with variable total track optical system is designed in the carrier-based aircraft landing system. ZOOM Lite: next-generation sequencing data mapping and visualization software.

High-throughput next-generation sequencing technologies pose increasing demands on the efficiency, accuracy and usability of data analysis software.

In this article, we present ZOOM Lite, a software for efficient reads mapping and result visualization. With a kernel capable of mapping tens of millions of Illumina or AB SOLiD sequencing reads efficiently and accurately, and an intuitive graphical user interface, ZOOM Lite integrates reads mapping and result visualization into a easy to use pipeline on desktop PC. The software handles both single-end and paired-end reads, and can output both the unique mapping result or the top N mapping results for each read.

Additionally, the software takes a variety of input file formats and outputs to several commonly used result formats. Zebra Zoom : an automated program for high-throughput behavioral analysis and categorization. The zebrafish larva stands out as an emergent model organism for translational studies involving gene or drug screening thanks to its size, genetics, and permeability.

At the larval stage, locomotion occurs in short episodes punctuated by periods of rest. Although phenotyping behavior is a key component of large-scale screens, it has not yet been automated in this model system. We developed Zebra Zoom , a program to automatically track larvae and identify maneuvers for many animals performing discrete movements.

Our program detects each episodic movement and extracts large-scale statistics on motor patterns to produce a quantification of the locomotor repertoire. We used Zebra Zoom to identify motor defects induced by a glycinergic receptor antagonist. The analysis of the blind mutant atoh7 revealed small locomotor defects associated with the mutation. Using multiclass supervised machine learning, Zebra Zoom categorized all episodes of movement for each larva into one of three possible maneuvers: slow forward swim, routine turn, and escape.

For all maneuvers in the data set, Zebra Zoom agreed with four experimenters in We modeled the series of maneuvers performed by larvae as Markov chains and observed that larvae often repeated the same maneuvers within a group. When analyzing subsequent maneuvers performed by different larvae, we found that larva—larva interactions occurred as series of escapes. Overall, Zebra Zoom reached the level of precision found in manual analysis but accomplished tasks in a high-throughput format necessary for large screens.

Optimization design of periscope type 3X zoom lens design for a five megapixel cellphone camera. This paper presents a periscope type 3X zoom lenses design for a five megapixel cellphone camera. The zoom lenses can be embedded in mobile phone with a thickness of 6 mm.

The zoom lenses have three groups with six elements. Intuitive tactile zooming for graphics accessed by individuals who are blind and visually impaired. One possibility of providing access to visual graphics for those who are visually impaired is to present them tactually: unfortunately, details easily available to vision need to be magnified to be accessible through touch.

For this, we propose an "intuitive" zooming algorithm to solve potential problems with directly applying visual zooming techniques to haptic displays that sense the current location of a user on a virtual diagram with a position sensor and, then, provide the appropriate local information either through force or tactile feedback.

Our technique works by determining and then traversing the levels of an object tree hierarchy of a diagram. In this manner, the zoom steps adjust to the content to be viewed, avoid clipping and do not zoom when no object is present. The algorithm was tested using a small, "mouse-like" display with tactile feedback on pictures representing houses in a community and boats on a lake.

We asked the users to answer questions related to details in the pictures. Comparing our technique to linear and logarithmic step zooming , we found a significant increase in the correctness of the responses odds ratios of 2.

Optical zoom lens module using MEMS deformable mirrors for portable device. The thickness of the smart phones in today's market is usually below than 10 mm, and with the shrinking of the phone volume, the difficulty of its production of the camera lens has been increasing. Therefore, how to give the imaging device more functionality in the smaller space is one of the interesting research topics for today's mobile phone companies. In this paper, we proposed a thin optical zoom system which is combined of micro-electromechanical components and reflective optical architecture.

By the adopting of the MEMS deformable mirrors, we can change their radius of curvature to reach the optical zoom in and zoom out. And because we used the all-reflective architecture, so this system has eliminated the considerable chromatic aberrations in the absence of lenses. In our system, the thickness of the zoom system is about 11 mm. The smallest EFL effective focal length is 4.

The longest EFL of the module is 9. Ultrathin zoom lens system based on liquid lenses. In this paper, we propose an ultrathin zoom lens system based on liquid lenses. The proposed system consists of an annular folded lens and three electrowetting liquid lenses.

The annular folded lens has several concentric surfaces. The annular folded lens is used to get the main power and correct aberrations. The three liquid lenses are used to change the focal length and correct aberration. An analysis of the proposed system is presented along with the design, fabrication, and testing of a prototype.

All the elements in the proposed system are very thin, so the system is an ultrathin zoom lens system, which has potential application as lightweight, thin, high-quality imagers for aerospace, consumer, and military applications.

Tudorica, A. Measuring and calibrating relations between cluster observables is critical for resource-limited studies. The mass-richness relation of clusters offers an observationally inexpensive way of estimating masses. Its calibration is essential for cluster and cosmological studies, especially for high-redshift clusters. Weak gravitational lensing magnification is a promising and complementary method to shear studies, that can be applied at higher redshifts.

Aims: We aim to employ the weak lensing magnification method to calibrate the mass-richness relation up to a redshift of 1. Methods: Lyman-break galaxies LBGs selected using the u-band dropout technique and their colours were used as a background sample of sources. LBG positions were cross-correlated with the centres of the sample of SpARCS clusters to estimate the magnification signal, which was optimally-weighted using an externally-calibrated LBG luminosity function.

The signal was measured for cluster sub-samples, binned in both redshift and richness. Results: We measured the cross-correlation between the positions of galaxy cluster candidates and LBGs and detected a weak lensing magnification signal for all bins at a detection significance of 2.

Conclusions: Our measurements demonstrated the feasibility of using weak lensing magnification as a viable tool for determining the average halo masses for samples of high redshift galaxy clusters. The results also established the success of using galaxy over-densities to select massive clusters at z. Moon illusion and spiral aftereffect: illusions due to the loom- zoom system? The moon illusion and the spiral aftereffect are illusions in which apparent size and apparent distance vary inversely.

Because this relationship is exactly opposite to that predicted by the static size--distance invariance hypothesis, the illusions have been called "paradoxical.

When stimulated by its characteristic stimulus of symmetrical expansion or contraction, the loom- zoom system produces the perception of a rigid object moving in depth. If this system is stimulated by a rotating spiral, a negative motion-aftereffect is produced when rotation ceases. If fixation is then shifted to a fixed-sized disc, the aftereffect process alters perceived distance and the loom- zoom system alters perceived size such that the disc appears to expand and approach or to contract and recede, depending on the direction of rotation of the spiral.

If the loom- zoom system is stimulated by a moon-terrain configuration, the equidistance tendency produces a foreshortened perceived distance for the moon as an inverse function of elevation and acts in conjunction with the loom- zoom system to produce the increased perceived size of the moon. Mechanically assisted liquid lens zoom system for mobile phone cameras. Camera systems with small form factor are an integral part of today's mobile phones which recently feature auto focus functionality.

Ready to market solutions without moving parts have been developed by using the electrowetting technology. Besides virtually no deterioration, easy control electronics and simple and therefore cost-effective fabrication, this type of liquid lenses enables extremely fast settling times compared to mechanical approaches.

As a next evolutionary step mobile phone cameras will be equipped with zoom functionality. We present first order considerations for the optical design of a miniaturized zoom system based on liquid-lenses and compare it to its mechanical counterpart. We propose a design of a zoom lens with a zoom factor of 2. The lens possesses auto focus capability and is based on liquid lenses and one additional mechanical actuator. The combination of liquid lenses and a single mechanical actuator enables extremely short settling times of about 20ms for the auto focus and a simplified mechanical system design leading to lower production cost and longer life time.

The camera system has a mechanical outline of 24mm in length and 8mm in diameter. The number of these groups has increased recently as well as the complexity of their relative movements and functions.

In this paper, we give a short history of zooming and focusing techniques ; we discuss the inconvenience of traditional solutions. We then introduce the concept of bidimensional law. We propose a systematic classification of possible lens-types according to the 4 possible types of group. Effects of dental magnification lenses on indirect vision: a pilot study. The purpose of this pilot study was to evaluate the effect of magnification lenses on the indirect vision skills of dental hygiene students.

This pilot study examined the accuracy and efficiency of dental hygiene students' indirect vision skills while using traditional safety lenses and magnification lenses. The sample was comprised of 14 students in their final semester of a dental hygiene program.

A crossover study approach was utilized, with each participant randomly assigned to a specific order of eyewear. The study included evaluation of each participant taking part in 2 separate clinical sessions. During the first session, each participant completed a clinical exercise on a dental manikin marked with 15 dots throughout the oral cavity while wearing the randomly as signed eyewear, and then completed a similar exercise on a differently marked dental manikin while wearing the randomly assigned eyewear.

This procedure was repeated at a second clinical session, however, the dental manikin and eyewear pairings were reversed. Accuracy was measured on the number of correctly identified dots and efficiency was measured by the time it took to identify the dots.

Perceptions of the participants' use of magnification lenses and the participants' opinion of the use of magnification lenses in a dental hygiene curriculum were evaluated using a questionnaire. Comparing the mean of the efficiency scores, students are more efficient at identifying indirect vision points with the use of magnification lenses 3 minutes, 36 seconds than with traditional safety lenses 3 minutes, 56 seconds.

Overall, the students report ed an increased quality of dental hygiene treatment provided in the clinical setting and an improved clinical posture while treating patients with the use of magnification lenses.

Development and application of variable- magnification x-ray Bragg optics. A feasibility test of this optical system was carried out at the vertical-wiggler beamline BLB of the Photon Factory. X-ray absorption-contrast images of a leaf were observed at various magnification factors.

Solutions on a high-speed wide-angle zoom lens with aspheric surfaces. Recent development in CMOS and digital camera technology has accelerated the business and market share of digital cinematography. In terms of optical design, this technology has increased the need to carefully consider pixel pitch and characteristics of the imager.

When the field angle at the wide end, zoom ratio, and F-number are specified, choosing an appropriate zoom lens type is crucial. In addition, appropriate power distributions and lens configurations are required. At points near the wide end of a zoom lens, it is known that an aspheric surface is an effective means to correct off-axis aberrations.

On the other hand, optical designers have to focus on manufacturability of aspheric surfaces and perform required analysis with respect to the surface shape.

Centration errors aside, it is also important to know the sensitivity to aspheric shape errors and their effect on image quality. In this paper, wide angle cine zoom lens design examples are introduced and their main characteristics are described. Moreover, technical challenges are pointed out and solutions are proposed. Photographic zoom fisheye lens design for DSLR cameras. Photographic fisheye lenses with fixed focal length for cameras with different sensor formats have been well developed for decades.

However, photographic fisheye lenses with variable focal length are rare on the market due in part to the greater design difficulty. This paper presents a large aperture zoom fisheye lens for DSLR cameras that produces both circular and diagonal fisheye imaging for mm sensors and diagonal fisheye imaging for APS-C sensors. The history and optical characteristics of fisheye lenses are briefly reviewed.

Then, a 9. Image quality and tolerance performance analysis for this lens are also presented. Chromoendoscopy and magnification endoscopy in Barrett's esophagus. Chromoendoscopy and magnification endoscopy appear to be a valuable adjuncts for the detection and classification of BE. These techniques may also prove to be useful aids in surveillance protocols for identifying dysplastic epithelium or early cancer within a segment of BE.

Ideally, the use of these techniques would enable the endoscopist to rule in or out the presence of IM and of dysplastic or cancerous epithelium by obtaining only a minimal number of targeted biopsy specimens, or potentially performing no biopsies at all. This could transform upper endoscopy into a much more effective screening and surveillance tool for BE.

Several problems currently exist for the use of chromoendoscopy for BE. Results of studies reporting the accuracy of chromoendoscopy remain mixed,and are likely explained by the wide range of techniques and materials used in the investigations.

Staining adds several steps, and likely several minutes, to an upper endoscopy. Staining within the esophagus is often patchy and uneven. In addition, poor spraying technique exaggerates the irregular uptake by the mucosa. There is a high false-positive rate when staining gastric-type epithelium and denuded epithelium. Areas of dysplasia or cancer may take up stain in an irregular manner, or may not stain at all.

Chromoendoscopy is a relatively new technique in the management of BE and depends on the skill and experience of the endoscopist. Magnification , however, only allows the endoscopist to observe small areas of mucosa at a time, increasing the overall complexity and length of the procedure.

The learning curve for this procedure is relatively short, however, and endoscopists can usually become proficient in the technique quickly. Currently, the greatest body of literature exists concerning the use of methylene blue for diagnosing BE. At the present time, chromoendoscopy and magnification endoscopy appear to be most beneficial in detecting IM in short segments of esophageal columnar.

Contrast-to-noise ratio in magnification mammography: a Monte Carlo study. Magnification views are a common way to perform a secondary examination when suspicious abnormalities are found in a screening mammogram.

The visibility of microcalcifications and breast lesions is restricted by the compromise between the image quality and the absorbed dose. In this study, image quality characteristics in magnification mammography were evaluated based on Monte Carlo techniques. A breast phantom was utilized, simulating a homogeneous mixture of adipose and glandular tissue in various percentages of glandularity, containing inhomogeneities of various sizes and compositions.

Results demonstrate that CNR is improved with the degree of magnification and degraded as the breast glandularity is increased. Degree of magnification 1. Under magnification conditions, the role of dose is demoted against the image quality, as magnification views are secondary, diagnostic examinations and not screening procedures oriented to non-symptomatic women. An innovative solution for high- magnification microscopy, based on attaching afocal optics for focal length reduction, is proposed.

The solution, consisting of three spherical mirrors, allows one to enhance a magnification of a laboratory based soft x-ray microscope over x, where movies with diffraction-limited resolution can be observed with an x-ray CCD.

The design example, having a numerical aperture of 0. In this paper the effect of weak lensing magnification on galaxy number counts is studied by cross-correlating the positions of two galaxy samples, separated by redshift, using data from the Dark Energy Survey Science Verification dataset. After an extensive analysis, it cannot be attributed to any known systematic effect.

The detection of the magnification signal is robust to estimated uncertainties in the outlier rate of the pho- tometric redshifts, but this will be an important issue for use of photometric redshifts in magnification mesurements from larger samples. In addition to the detection of the magnification signal, a method to select the sample with the maximum signal-to-noise is proposed and validated with data.

Annular ring zoom system using two positive axicons. The production of an annular ring of light with a variable diameter has applications in laser material processing and machining, particle manipulation, and corneal surgery. This can readily be accomplished using a positive and negative axicon pair. However, negative axicons are very expensive and difficult to obtain with small diameters. In this paper, we present a design of an annular ring zoom system using two positive axicons.

One axicon is placed a distance before a primary lens that is greater than some prescribed minimum, and the second axicon is placed after the primary lens. The position of the second axicon determines the ring diameter. The ring diameter can be zoomed from some maximum design size to a zero diameter ring spot.

Experimental results from a developmental system will be presented. Estimation of cortical magnification from positional error in normally sighted and amblyopic subjects.

We describe a method for deriving the linear cortical magnification factor from positional error across the visual field. We compared magnification obtained from this method between normally sighted individuals and amblyopic individuals, who receive atypical visual input during development.

The cortical magnification factor was derived for each subject from positional error at 32 locations in the visual field, using an established model of conformal mapping between retinal and cortical coordinates. Magnification of the normally sighted group matched estimates from previous physiological and neuroimaging studies in humans, confirming the validity of the approach.

The estimate of magnification for the amblyopic group was significantly lower than the normal group: by 4. These estimates, if correct, suggest a role for early visual experience in establishing retinotopic mapping in cortex. We discuss the implications of altered cortical magnification for cortical size, and consider other neural changes that may account for the amblyopic results.

Due to the overwhelming amount of detail available in whole-slide images, analytic procedures-whether computational or visual-often operate at magnifications lower than the magnification at which the image was acquired. As a result, a corresponding reduction in image resolution occurs. It is unclear how much information is lost when magnification is reduced, and whether the rich color attributes of histologic slides can aid in reconstructing some of that information. By harnessing measured histologic features and the intrinsic spatial relationships between histologic structures, we developed a predictive model to estimate the histologic composition of tissue in a manner that exceeds the resolution of the image.

By utilizing pixel color, this ability was improved at all magnifications. Our findings suggest that some of these limitations may be overcome with computational modeling. The media regularly present negative news articles about teachers and teaching.

This paper focuses particularly on one such news article. Using reflective analytic practices, first we zoom in to conduct a detailed analysis of the text. We find that complex and contradictory moral categories of teachers are assembled within and through the text. This short word report presents a series of research needs for improving the measurement and understanding of trophic magnification factors TMFs.

TMFs are useful measures of trophic magnification and represent the diet-weighted average biomagnification factor BMF of che Research on the relation between the contact angle and the interface curvature radius of electrowetting liquid zoom lens. Therefore, a liquid lens was put forward to solve the problems. The liquid zoom lens has the merits of lower cost, smaller volume, quicker response, lower energy consumption, continuous zoom and higher accuracy.

In liquid zoom lens the precise focal length is obtained by the contact angle changing to affect the curvature radius of interface. In our works, the relations of the exerted voltage, the contact angle, the curvature radius and the focal length were researched and accurately calculated. The calculation of the focal length provides an important theoretical basis for instructing the design of liquid zoom lens. Experimental Demonstration of Longitudinal Magnification.

We describe an experiment which enables the observation of longitudinal magnification for the real image of a three-dimensional 3D object formed by a converging lens. The experiment also shows the absence of longitudinal inversion. Possible reasons for misconceptions with respect to real images and longitudinal inversions are discussed and a…. Dipolar modulation in the size of galaxies: the effect of Doppler magnification. Objects falling into an overdensity appear larger on its near side and smaller on its far side than other objects at the same redshift.

This produces a dipolar pattern of magnification , primarily as a consequence of the Doppler effect. At low redshift, this Doppler magnification completely dominates the usual integrated gravitational lensing contribution to the lensing magnification. We show that one can optimally observe this pattern by extracting the dipole in the cross-correlation of number counts and galaxy sizes.

Doppler magnification should be easily detectable in current and upcoming optical and radio surveys; by forecasting for telescopes such as the SKA, we show that this technique is competitive with using peculiar velocities via redshift-space distortions to constrain dark energy. It produces similar yet complementary constraints on the cosmological model to those found using measurements of the cosmic shear. Newly described features resulting from high- magnification dermoscopy of tinea capitis.

Five children 2 boys and 3 girls; aged years with multiple scaly patches of alopecia underwent scalp dermoscopy, direct microscopic examinations, and mycological cultures of skin scrapings. These horizontal white bands are usually multiple and may cause the hair to bend and break.

We also identified a new dermoscopic feature consisting of translucent, easily deformable hairs that look weakened and transparent and show unusual bends; they are likely the result of a massive fungal invasion involving the whole hair shaft.

Direct microscopic examination showed fungal infection and results of mycological culture were positive for Microsporum canis in all cases. The identification of new findings using higher- magnification dermoscopy may enhance the diagnosis of tinea capitis and be of help to better understand some pathogenetic mechanisms. Geographic Data Display Implementation.

The result is a change of extent around the cursor as seen in Products printer and a card- per-minute card reader with the Interdata 4 The with its 64K of core is the applications machine connected Anisotropic magnification distortion of the 3D galaxy correlation.

Real space. It has long been known that gravitational lensing, primarily via magnification bias, modifies the observed galaxy or quasar clustering. Such discussions have largely focused on the 2D angular correlation function. Here and in paper II [L. Hui, E. Gaztanaga, and M. LoVerde, arXiv The interesting point is that the distortion is anisotropic. Magnification bias in general preferentially enhances the observed correlation in the line-of-sight LOS orientation, especially on large scales.

This effect presents an interesting opportunity as well as a challenge. The opportunity: this lensing anisotropy is distinctive, making it possible to separately measure the galaxy-galaxy, galaxy- magnification , and magnification-magnification correlations, without measuring galaxy shapes.

The anisotropy is distinguishable from the well-known distortion due to peculiar motions, as will be discussed in paper II. The challenge: the magnification distortion of the galaxy correlation must be accounted for in interpreting data as precision improves.

The corresponding shifts in the inferred Hubble parameter and angular diameter distance, if ignored, could significantly bias measurements of the dark energy equation of state.

Lastly, magnification distortion offers a plausible explanation for the well-known excess correlations. We describe a new method for measuring galaxy magnification due to weak gravitational lensing.

Our method makes use of a tight scaling relation between galaxy properties that are modified by gravitational lensing, such as apparent size, and other properties that are not, such as surface brightness. In particular, we use a version of the well-known fundamental plane relation for early-type galaxies. This modified ''photometric fundamental plane'' uses only photometric galaxy properties, eliminating the need for spectroscopic data.

We present the first detection of magnification using this method by applying it to photometric catalogs from the Sloan Digital Sky Survey. Thismore » analysis shows that the derived magnification signal is within a factor of three of that available from conventional methods using gravitational shear. We suppress the dominant sources of systematic error and discuss modest improvements that may further enhance the lensing signal-to-noise available with this method.

Moreover, some of the dominant sources of systematic error are substantially different from those of shear-based techniques. With this new technique, magnification becomes a useful measurement tool for the coming era of large ground-based surveys intending to measure gravitational lensing.

Current microlensing follow-up observations focus on high- magnification events because of the high efficiency of planet detection. However, central perturbations of high- magnification events caused by a planet can also be produced by a very close or a very wide binary companion, and the two kinds of central perturbations are not generally distinguished without time consuming detailed modeling a planet-binary degeneracy.

Hence, it is important to resolve the planet-binary degeneracy that occurs in high- magnification events. In this paper, we investigate caustic-crossing high- magnification events caused by a planet and a wide binary companion.

From this investigation, we find that because of the differentmore » magnification excess patterns inside the central caustics induced by the planet and the binary companion, the light curves of the caustic-crossing planetary-lensing events exhibit a feature that is discriminated from those of the caustic-crossing binary-lensing events, and the feature can be used to immediately distinguish between the planetary and binary companions. The planetary-lensing feature appears in the interpeak region between the two peaks of the caustic-crossings.

The structure of the interpeak region for the planetary-lensing events is smooth and convex or boxy, whereas the structure for the binary-lensing events is smooth and concave. We also investigate the effect of a finite background source star on the planetary-lensing feature in the caustic-crossing high- magnification events.

From this, we find that the convex-shaped interpeak structure appears in a certain range that changes with the mass ratio of the planet to the planet-hosting star. Zhao, Yang; Williams, Daniel J. With the advancement in sensors, hyperspectral imaging in short wave infrared SWIR 0.

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