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Journal articles on the topic 'Optical and near-Infrared'

Author: Grafiati

Published: 8 June 2024

Last updated: 31 July 2025

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1

Hielscher, A. H., A. Y. Bluestone, G. S. Abdoulaev, et al. "Near-Infrared Diffuse Optical Tomography." Disease Markers 18, no. 5-6 (2002): 313–37. http://dx.doi.org/10.1155/2002/164252.

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Diffuse optical tomography (DOT) is emerging as a viable new biomedical imaging modality. Using near-infrared (NIR) light, this technique probes absorption as well as scattering properties of biological tissues. First commercial instruments are now available that allow users to obtain cross-sectional and volumetric views of various body parts. Currently, the main applications are brain, breast, limb, joint, and fluorescence/bioluminescence imaging. Although the spatial resolution is limited when compared with other imaging modalities, such as magnetic resonance imaging (MRI) or X-ray computeri

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2

Murray, J. T., N. Peyghambarian, and R. C. Powell. "Near infrared optical parametric oscillators." Optical Materials 4, no. 1 (1994): 55–60. http://dx.doi.org/10.1016/0925-3467(94)90056-6.

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3

Liu, Xiaofei, Ruohui Chen, Yilin Lu, et al. "Optical performances of near-infrared metalenses with process-induced defects." Chinese Optics Letters 23, no. 6 (2025): 063602. https://doi.org/10.3788/col202523.063602.

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4

Kim, Sung-Man, and Hanbit Park. "Optimization of optical wireless power transfer using near-infrared laser diodes." Chinese Optics Letters 18, no. 4 (2020): 042603. http://dx.doi.org/10.3788/col202018.042603.

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5

Lingling, Wu, Zhang Huan, and Chen Jing. "Design of near infrared optical system." Journal of Applied Optics 36, no. 2 (2015): 183–87. http://dx.doi.org/10.5768/jao201536.0201004.

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6

Zhu, Banghe, and Anuradha Godavarty. "Near-Infrared Fluorescence-Enhanced Optical Tomography." BioMed Research International 2016 (2016): 1–10. http://dx.doi.org/10.1155/2016/5040814.

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Fluorescence-enhanced optical imaging using near-infrared (NIR) light developed forin vivomolecular targeting and reporting of cancer provides promising opportunities for diagnostic imaging. The current state of the art of NIR fluorescence-enhanced optical tomography is reviewed in the context of the principle of fluorescence, the different measurement schemes employed, and the mathematical tools established to tomographically reconstruct the fluorescence optical properties in various tissue domains. Finally, we discuss the recent advances in forward modeling and distributed memory parallel co

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7

Nafie, Laurence A., Bruce E. Brinson, Xiaolin Cao, et al. "Near-Infrared Excited Raman Optical Activity." Applied Spectroscopy 61, no. 10 (2007): 1103–6. http://dx.doi.org/10.1366/000370207782217752.

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Measurements of near-infrared scattered circular polarization Raman optical activity (SCP-ROA) are presented using laser excitation at 780 nm for samples of S-(—)-α-pinene and L-alanyl-L-alanine. These are the first measurements of ROA outside the blue-to-green visible region between 488 and 532 nm. Comparison of Raman and ROA intensities measured with excitation at 532 and 780 nm demonstrate that the expected frequency to the fourth-power dependence for Raman scattering and the corresponding fifth-power dependence for ROA are observed. It can be concluded that, to within this frequency depend

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8

Hai, Pengfei, Junjie Yao, Konstantin I. Maslov, Yong Zhou, and Lihong V. Wang. "Near-infrared optical-resolution photoacoustic microscopy." Optics Letters 39, no. 17 (2014): 5192. http://dx.doi.org/10.1364/ol.39.005192.

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9

Piao, Daqing, Hao Xie, Weili Zhang, et al. "Endoscopic, rapid near-infrared optical tomography." Optics Letters 31, no. 19 (2006): 2876. http://dx.doi.org/10.1364/ol.31.002876.

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10

Kim, Sung-Tae, Ji-Seon Yoo, Min-Woo Lee, Ji-Won Jung, and Jae-Hyung Jang. "CuInSe2-Based Near-Infrared Photodetector." Applied Sciences 12, no. 1 (2021): 92. http://dx.doi.org/10.3390/app12010092.

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Near-infrared (NIR) photodetectors have interesting roles in optical fiber communications and biomedical applications. Conventional NIR photodetectors have been realized using InGaAs and Ge, of which the cut-off wavelengths exceed 1500 nm. Si-based photodetectors exhibit limited external quantum efficiency at wavelengths longer than 1000 nm. By synthesizing a CuInSe2 compound on a glass substrate, photodetectors that can detect optical wavelengths longer than 1100 nm have been realized in this study. The bandgap energies of the CuInSe2 thin films were tuned by varying the Cu/In ratio from 1.02

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11

Fu, Tairan, Jiaqi Tang, Kai Chen, and Fan Zhang. "Visible, near-infrared and infrared optical properties of silica aerogels." Infrared Physics & Technology 71 (July 2015): 121–26. http://dx.doi.org/10.1016/j.infrared.2015.03.004.

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12

Walmsley, Thayer S., Kraig Andrews, Tianjiao Wang, et al. "Near-infrared optical transitions in PdSe2 phototransistors." Nanoscale 11, no. 30 (2019): 14410–16. http://dx.doi.org/10.1039/c9nr03505b.

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13

Kaino, Toshikuni. "Plastic optical fibers for near‐infrared transmission." Applied Physics Letters 48, no. 12 (1986): 757–58. http://dx.doi.org/10.1063/1.96711.

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14

Gurfinkel, Michael, Shi Ke, Xiaoxia Wen, Chun Li, and Eva M. Sevick-Muraca. "Near-Infrared Fluorescence Optical Imaging and Tomography." Disease Markers 19, no. 2-3 (2004): 107–21. http://dx.doi.org/10.1155/2004/474818.

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The advent of recent advances in near-infrared laser diodes and fast electro-optic detection has spawned a new research field of diagnostic spectroscopy and imaging based on targeting and reporting exogenous fluorescent agents. This review seeks to concisely address the physics, instrumentation, advancements in tomography, and near-infrared fluorescent contrast agent development that promises selective and specific molecular targeting of diseased tissues. As an example of one area of the field, recent work focusing on pharmacokinetic analysis of fluorophores targeting the epidermal growth fact

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15

GRATTON, GABRIELE, JOHN S. MAIER, MONICA FABIANI, WILLIAM W. MANTULIN, and ENRICO GRATTON. "Feasibility of intracranial near-infrared optical scanning." Psychophysiology 31, no. 2 (1994): 211–15. http://dx.doi.org/10.1111/j.1469-8986.1994.tb01043.x.

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16

Wright, Edward L. "Comparing Optical and Near-Infrared Luminosity Functions." Astrophysical Journal 556, no. 1 (2001): L17—L19. http://dx.doi.org/10.1086/322861.

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17

Debnath, Sisir, Jean-Francois Bergamini, Franck Artzner, Cristelle Mériadec, Franck Camerel, and Marc Fourmigué. "Near-infrared chiro-optical effects in metallogels." Chem. Commun. 48, no. 17 (2012): 2283–85. http://dx.doi.org/10.1039/c2cc16549j.

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18

Piao, Daqing, Guolong Zhang, Sreenivas Vemulapalli, Hamid Dehghani, and Brian W. Pogue. "Near-Infrared Optical Tomography in Endoscopy-Geometry." Optics and Photonics News 17, no. 12 (2006): 31. http://dx.doi.org/10.1364/opn.17.12.000031.

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19

Xie, Hanhan, Jundong Shao, Jiahong Wang, Zhengbo Sun, Xue-Feng Yu, and Qu-Quan Wang. "Near-infrared optical performances of two Bi2Se3nanosheets." RSC Adv. 7, no. 79 (2017): 50234–38. http://dx.doi.org/10.1039/c7ra09872c.

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20

Mahmood, U. "Near infrared optical applications in molecular imaging." IEEE Engineering in Medicine and Biology Magazine 23, no. 4 (2004): 58–66. http://dx.doi.org/10.1109/memb.2004.1337950.

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21

Hughes, D. H., E. I. Robson, and M. J. Ward. "Optical & Near Infrared Imaging of NGC1275." Symposium - International Astronomical Union 134 (1989): 376–78. http://dx.doi.org/10.1017/s0074180900141373.

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We are currently studying a selection of active galaxies using the new IR array camera IRCAM on UKIRT. Our aim is to seperate the underlying stellar emission from that of the active galactic nucleus. Although the optical is the best wavelength region to discriminate between the different populations in the underlying spiral and elliptical galaxies, it is in the infrared that the contrast between the non-thermal central core and the surrounding galaxy is increased. We present reduced data from infrared images taken at 1.25, 1.65 and 2.2 μm with an image scale of 0.6 arcsec/pixel together with o

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22

Duboz, J. Y., P. A. Badoz, J. Henz, and H. von Känel. "Near‐infrared optical properties of CoSi2thin films." Journal of Applied Physics 68, no. 5 (1990): 2346–50. http://dx.doi.org/10.1063/1.346542.

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23

Oliva, E., S. Gennari, L. Vanzi, A. Caruso, and M. Ciofini. "Optical materials for near infrared Wollaston prisms." Astronomy and Astrophysics Supplement Series 123, no. 1 (1997): 179–82. http://dx.doi.org/10.1051/aas:1997311.

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24

Wang, Chenyu, Jinman Kim, Craig T. Jin, Philip H. W. Leong, and Alistair McEwan. "Near Infrared Spectroscopy in Optical Coherence Tomography." Journal of Near Infrared Spectroscopy 20, no. 1 (2012): 237–47. http://dx.doi.org/10.1255/jnirs.975.

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25

Rangel-Rojo, R., T. Kosa, E. Hajto, et al. "Near-infrared optical nonlinearities in amorphous chalcogenides." Optics Communications 109, no. 1-2 (1994): 145–50. http://dx.doi.org/10.1016/0030-4018(94)90752-8.

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26

Lee, Seung-Young, Seulki Lee, In-Chan Youn, et al. "A Near-Infrared Fluorescence-Based Optical Thermosensor." Chemistry - A European Journal 15, no. 25 (2009): 6103–6. http://dx.doi.org/10.1002/chem.200900683.

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27

Takezawa, Yoshitaka, and Shuichi Ohara. "Polymer optical fiber for near infrared use." Journal of Applied Polymer Science 49, no. 1 (1993): 169–73. http://dx.doi.org/10.1002/app.1993.070490120.

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28

Hurt, R. L., J. L. Turner, D. Levine, K. M. Merrill, and I. Gatley. "Tracing Molecular Emission in Spiral Galaxies: The Near Infrared Correspondence." International Astronomical Union Colloquium 140 (1994): 370–71. http://dx.doi.org/10.1017/s0252921100020042.

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Near infrared imaging can be a powerful tool in tracing the densest molecular structures in galaxies. The observable molecular emission originates in large molecular cloud complexes which are also subject to significant extinctions caused by the associated dust. It can be difficult to distinguish between regions of moderate and large molecular density with optical observations as both will appear optically thick. Since extinction in the near infrared is only about a tenth of the corresponding visual extinction, multi-band near infrared imaging will trace the regions of the highest optical dept

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29

Surace, Jason A., D. B. Sanders, and A. S. Evans. "High‐Resolution Optical/Near‐Infrared Imaging of Cool Ultraluminous Infrared Galaxies." Astrophysical Journal 529, no. 1 (2000): 170–88. http://dx.doi.org/10.1086/308247.

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30

Surace, Jason A., D. B. Sanders, and A. S. Evans. "Optical and Near-Infrared Imaging of Infrared-Excess Palomar-Green Quasars." Astronomical Journal 122, no. 6 (2001): 2791–809. http://dx.doi.org/10.1086/324462.

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31

Cross, Nicholas J. G., and S. G. Djorgovski. "Optical & NIR Transient Surveys." Proceedings of the International Astronomical Union 7, S285 (2011): 185–90. http://dx.doi.org/10.1017/s1743921312000580.

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AbstractA workshop on Optical & Near Infrared Transients took place during the first afternoon of the Symposium. It ran for two sessions. The first was given over to talks about various current optical and near-infrared transient surveys, focussing on the Vista surveys, the Catalina Real-Time Transient Survey, Pan-STARRS, Gaia, TAOS and TAOS2. The second session was a panel-led discussion about coordinating multi-wavelength surveys and associated follow-ups.

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32

Ichikawa, T., N. Itoh, and K. Yanagisawa. "Multi-Color Surface Photometry of Nearby Galaxies." Symposium - International Astronomical Union 179 (1998): 285–86. http://dx.doi.org/10.1017/s0074180900128797.

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Near-infrared (NIR) emission in galaxies is mainly radiated by old population low temperature stars, which construct the basic stellar structure and keep the trails of past galaxy evolution. On the other hand, optical observations show recent star formation activity, especially in spiral galaxies. Therefore multi-color observations from optical to near-infrared wavelengths are very important to understand the past and recent star-formation history. Nearby large galaxies are well studied not only in optical but also in mid- and far-infrared by IRAS, CO and HI radio observations. However, the st

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33

HOSHI, Yoko. "Near-Infrared Optical Imaging by Time-Resolved Spectroscopy." Review of Laser Engineering 30, no. 11 (2002): 642–47. http://dx.doi.org/10.2184/lsj.30.642.

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34

Spyromilio, J., R. Gilmozzi, J. Sollerman, B. Leibundgut, C. Fransson, and J. G. Cuby. "Optical and near infrared observations of SN 1998bu." Astronomy & Astrophysics 426, no. 2 (2004): 547–53. http://dx.doi.org/10.1051/0004-6361:20040570.

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35

Spezzi, L., B. Merín, I. Oliveira, E. F. van Dishoeck, and J. M. Brown. "A deep optical/near-infrared catalogue of Serpens." Astronomy and Astrophysics 513 (April 2010): A38. http://dx.doi.org/10.1051/0004-6361/200913956.

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36

Brand, Kate, Michael J. I. Brown, Arjun Dey, et al. "TheChandraXBootes Survey. III. Optical and Near‐Infrared Counterparts." Astrophysical Journal 641, no. 1 (2006): 140–57. http://dx.doi.org/10.1086/500312.

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37

Sampath, Lakshmi, Wei Wang, and Eva M. Sevick-Muraca. "Near infrared fluorescent optical imaging for nodal staging." Journal of Biomedical Optics 13, no. 4 (2008): 041312. http://dx.doi.org/10.1117/1.2953498.

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38

Hall, Patrick Brian. "An Optical/Near‐Infrared Study of Quasar Environments." Publications of the Astronomical Society of the Pacific 110, no. 749 (1998): 880. http://dx.doi.org/10.1086/316195.

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39

Thornton, Jr., Robert J., Alan Stockton, and Susan E. Ridgway. "Optical and Near-Infrared Spectroscopy of Cygnus A." Astronomical Journal 118, no. 4 (1999): 1461–67. http://dx.doi.org/10.1086/301035.

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40

Eiroa, C., R. Lenzen, L. F. Miranda, J. M. Torrelles, G. Anglada, and R. Estalella. "Optical and near-infrared observations of S 140N." Astronomical Journal 106 (August 1993): 613. http://dx.doi.org/10.1086/116665.

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41

Cole, D. M., D. E. Vanden Berk, S. A. Severson, et al. "Optical/Near‐Infrared Observations of GRO J1744−28." Astrophysical Journal 480, no. 1 (1997): 377–82. http://dx.doi.org/10.1086/303973.

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42

Norman, Thaddeus J., Christian D. Grant, Donny Magana, et al. "Near Infrared Optical Absorption of Gold Nanoparticle Aggregates." Journal of Physical Chemistry B 106, no. 28 (2002): 7005–12. http://dx.doi.org/10.1021/jp0204197.

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43

Dhar Dwivedi, Shyam Murli Manohar, Avijit Dalal, Anupam Ghosh, et al. "InN Nanowires Based Near-Infrared Broadband Optical Detector." IEEE Photonics Technology Letters 31, no. 18 (2019): 1526–29. http://dx.doi.org/10.1109/lpt.2019.2936272.

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44

Dai, Zhifei, Xiuli Yue, Bixian Peng, Qiguang Yang, Xuchun Liu, and Peixian Ye. "Third-order optical nonlinearities of near-infrared dyes." Chemical Physics Letters 317, no. 1-2 (2000): 9–12. http://dx.doi.org/10.1016/s0009-2614(99)01372-x.

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45

Piednoir, A., and F. Creuzet. "Near-field optical microscopy in the infrared range." Micron 27, no. 5 (1996): 335–39. http://dx.doi.org/10.1016/s0968-4328(96)00026-1.

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46

Krühler, Thomas. "Optical and near-infrared flares in GRB afterglows." Proceedings of the International Astronomical Union 7, S279 (2011): 46–53. http://dx.doi.org/10.1017/s1743921312012677.

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AbstractAmong the diversities in the very early evolution of GRB afterglows are bright optical/near-infrared flares before or superimposed onto an otherwise smoothly decaying afterglow light curve. A lot has been learned about GRBs by using an optical flare or lack thereof as a diagnostic of the emission mechanisms and outflow conditions. In this contribution I will review the observational properties of rising and decaying light-curves in GRB afterglows, discuss their possible physical origins, and highlight in which way they help in understanding GRB and afterglows physics.

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47

Spyromilio, Jason. "Optical and Near-infrared Observations of Supernova 1987A." Publications of the Astronomical Society of Australia 9, no. 1 (1991): 8–12. http://dx.doi.org/10.1017/s1323358000024760.

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AbstractWe present observational results obtained during the first three years following the explosion of Supernova 1987 A. We discuss aspects of the optical and near infrared spectra as well as results from spectropolarimetric observations. The observations of the circumstellar and interstellar medium are also briefly discussed.

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48

Rao, K. Prahlad, S. Radhakrishnan, and M. Ramasubba Reddy. "Brain tissue phantoms for optical near infrared imaging." Experimental Brain Research 170, no. 4 (2005): 433–37. http://dx.doi.org/10.1007/s00221-005-0242-4.

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49

Mendeleyev, V. Ya, S. N. Skovorodko, E. N. Lubnin, and V. M. Prosvirikov. "Optical constants of silicon in near infrared region." Applied Physics Letters 93, no. 13 (2008): 131916. http://dx.doi.org/10.1063/1.2994669.

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50

Jagannath, Ravi Prasad K., and Phaneendra K. Yalavarthy. "Nonquadratic penalization improves near-infrared diffuse optical tomography." Journal of the Optical Society of America A 30, no. 8 (2013): 1516. http://dx.doi.org/10.1364/josaa.30.001516.

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