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Letteratura scientifica selezionata sul tema "Photometric"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 25 luglio 2025

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Articoli di riviste sul tema "Photometric"

1

Sun, Mingxu, Bingqiu Chen, Helong Guo, He Zhao, Ming Yang, and Wenyuan Cui. "SPar: Estimating Stellar Parameters from Multiband Photometries with Empirical Stellar Libraries." Astronomical Journal 166, no. 3 (2023): 126. http://dx.doi.org/10.3847/1538-3881/ace5ab.

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Abstract Modern large-scale photometric surveys have provided us with multiband photometries of billions of stars. Determining the stellar atmospheric parameters, such as the effective temperature (T eff) and metallicities ([Fe/H]), absolute magnitudes (M G ), distances (d), and reddening values (E(G BP − G RP)) is fundamental to study the stellar populations, structure, kinematics, and chemistry of the Galaxy. This work constructed an empirical stellar library that maps the stellar parameters to multiband photometries from a data set with Gaia parallaxes, LAMOST atmospheric parameters, and op

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2

Evans, D. W., M. Riello, F. De Angeli, et al. "Gaia Photometric Catalogue: the calibration of the DR2 photometry." Proceedings of the International Astronomical Union 14, A30 (2018): 466–70. http://dx.doi.org/10.1017/s174392131900512x.

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AbstractGaia DR2 was released in April 2018 and contains a photometric catalogue of more than 1 billion sources. This release contains colour information in the form of integrated BP and RP photometry in addition to the latest G-band photometry. The level of uncertainty can be as good as 2 mmag with some residual systematics at the 10 mmag level. The addition of colour information greatly enhances the value of the photometric data for the scientific community. A high level overview of the photometric processing, with a focus on the improvements with respect to Gaia DR1, was given. The definiti

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3

Prokhorov, M. E., A. I. Zakharov, V. G. Moshkalev, N. L. Krusanova, and M. S. Tuchin. "Mass Computations of the Brightness of Stars in an Arbitrary Spectral Band." Астрономический журнал 100, no. 6 (2023): 500–511. http://dx.doi.org/10.31857/s0004629923050092.

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The problem of calculating the brightness of an array of stars in an arbitrary photometric band, which is not the standard band of astronomical photometry, is considered from their multicolor photometry in some other photometric system. A similar problem is to transfer photometric measurements of stars from one multicolor photometric system to another. This task includes methods for calculating and comparing magnitudes, as well as merging photometric catalogs. The questions of choice of various zero-points of photometry and reduction of measurements for the atmosphere are considered. The issue

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4

Fotopoulou, S., and S. Paltani. "CPz: Classification-aided photometric-redshift estimation." Astronomy & Astrophysics 619 (October 30, 2018): A14. http://dx.doi.org/10.1051/0004-6361/201730763.

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Broadband photometry offers a time and cost effective method to reconstruct the continuum emission of celestial objects. Thus, photometric redshift estimation has supported the scientific exploitation of extragalactic multiwavelength surveys for more than twenty years. Deep fields have been the backbone of galaxy evolution studies and have brought forward a collection of various approaches in determining photometric redshifts. In the era of precision cosmology, with the upcoming Euclid and LSST surveys, very tight constraints are put on the expected performance of photometric redshift estimati

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5

Li, Xiao Pan, Cheng Yang, Li Zhou, and Hai Tao Yang. "Photometric Data Procession of the Swift/UVOT Instrument." Advanced Materials Research 989-994 (July 2014): 3489–92. http://dx.doi.org/10.4028/www.scientific.net/amr.989-994.3489.

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The Ultraviolet/Optical Telescope (UVOT) which is one of three scientific instruments onboard the NASA-led Swift satellite provides simultaneous ultraviolet and optical photometric data. We present the installing procedures of HEASoft software and the detailed method for using the HEASoft in UVOT photometric data processions. We focus on the application of photometry processes, and present the photometry of Quasar PKS 0537-441. The analysis of the photometric data shows that this source has extreme variations in optical and ultraviolet bands and the shape of photometric flux curves in each ban

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6

Wittman, D., P. Riechers, and V. E. Margoniner. "Photometric Redshifts and Photometry Errors." Astrophysical Journal 671, no. 2 (2007): L109—L112. http://dx.doi.org/10.1086/525020.

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7

Walker, Alistair, Saul Adelman, Eugene Milone, et al. "DIVISION B COMMISSION 25: ASTRONOMICAL PHOTOMETRY AND POLARIMETRY." Proceedings of the International Astronomical Union 11, T29A (2015): 159–70. http://dx.doi.org/10.1017/s1743921316000727.

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Commission 25 (C25) deals with the techniques and issues involved with the measurement of optical and infrared radiation intensities and polarization from astronomical sources. As such, in recent years attention has focused on photometric standard stars, atmospheric extinction, photometric passbands, transformation between systems, nomenclature, and observing and reduction techniques. At the start of the trimester C25 changed its name from Stellar Photometry and Polarization to Astronomical Photometry and Polarization so as to explicitly include in its mandate particular issues arising from th

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8

Tatarnikov, A. M., та A. A. Tatarnikov. "Сolor transformation between photometric systems of 2MASS catalog and ASTRONIRCAM of SAI MSU 2.5-m telescope". Seriya 3: Fizika, Astronomiya, № 2_2023 (2 червня 2023): 2320801–1. http://dx.doi.org/10.55959/msu0579-9392.78.2320801.

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In this paper, we consider a method for determining the coefficients of the transformation equations between different photometric systems based on the photometry of all field stars recorded during observations of the primary standards of one of the photometric systems. Using this method, the coefficients of color transformation equations between the photometric system of ASTRONIRCAM of the 2.5-m telescope KGO SAI MSU and the 2MASS all-sky survey catalog photometric system are obtained.

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9

Toptun, Victoria A., Igor V. Chilingarian, Kirill A. Grishin, and Ivan Yu Katkov. "Color Transformations of Photometric Measurements of Galaxies in Optical and Near-infrared Wide-field Imaging Surveys*." Publications of the Astronomical Society of the Pacific 135, no. 1050 (2023): 084102. http://dx.doi.org/10.1088/1538-3873/aceca0.

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Abstract Over the past 2 decades, wide-field photometric surveys in optical and infrared domains reached a nearly all-sky coverage thanks to numerous observational facilities operating in both hemispheres. However, subtle differences among exact realizations of Johnson and SDSS photometric systems require one to convert photometric measurements into the same system prior to analysis of composite data sets originating from multiple surveys. It turns out that the published photometric transformations lead to substantial biases when applied to integrated photometry of galaxies from the correspond

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10

Pforr, Janine. "The Spitzer Extragalactic Representative Volume Survey - measuring photometric redshifts for ∼4 million galaxies - challenges and ways forward." Proceedings of the International Astronomical Union 15, S341 (2019): 157–61. http://dx.doi.org/10.1017/s1743921319002412.

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AbstractWe highlight the challenges as well as lessons learnt in the derivation of the photometric redshifts for ∼4 million galaxies at 0 < z ≲ 6 contained in the Spitzer Extragalactic Representative Volume Survey (SERVS) and summarise the photometric redshift results recently published in Pforr et al. (2019). The inhomogeneous nature of the ancillary photometry for SERVS presents a similar situation to the one future, large, extragalactic surveys with e.g. LSST and JWST will face. We employ template SED-fitting to determine photometric redshifts. Our comparison of photometric redshifts to

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Tesi sul tema "Photometric"

1

Halliday, Colin George. "Aspects of photometric titration." Thesis, Queen's University Belfast, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.329513.

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2

Powell, Christopher. "Mutual illumination photometric stereo." Thesis, University of East Anglia, 2018. https://ueaeprints.uea.ac.uk/67065/.

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Many techniques have been developed in computer vision to recover three-dimensional shape from two-dimensional images. These techniques impose various combinations of assumptions/restrictions of conditions to produce a representation of shape (e.g. surface normals or a height map). Although great progress has been made it is a problem which remains far from solved. In this thesis we propose a new approach to shape recovery - namely `mutual illumination photometric stereo'. We exploit the presence of colourful mutual illumination in an environment to recover the shape of objects from a single i

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3

Pocino, Yuste Andrea. "Cosmology with photometric redshift." Doctoral thesis, Universitat Autònoma de Barcelona, 2020. http://hdl.handle.net/10803/671733.

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Els cartografiats de galàxies fotomètrics actuals i futurs observaran un gran volum de l’univers que ens permetrà acotar amb precisió el model cosmològic. Tanmateix, la capacitat de delimitar el model que tenen aquests cartografiats a través de les sondes cosmològiques depèn de la precisió i certesa amb les que es determina el redshift de les galàxies. Per tant, la determinació del redshift fotomètric i els seus efectes en les anàlisis cosmològiques han de ser tractats i estudiats curosament. En la primera part de la tesi, transformem la fotometria de simulacions que ja existeixen per imitar

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4

Bezanson, Rachel, David A. Wake, Gabriel B. Brammer, et al. "LEVERAGING 3D-HST GRISM REDSHIFTS TO QUANTIFY PHOTOMETRIC REDSHIFT PERFORMANCE." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621218.

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We present a study of photometric redshift accuracy in the 3D-HST photometric catalogs, using 3D-HST grism redshifts to quantify and dissect trends in redshift accuracy for galaxies brighter than JH(IR) > 24 with an unprecedented and representative high-redshift galaxy sample. We find an average scatter of 0.0197 +/- 0.0003(1 + z) in the Skelton et al. photometric redshifts. Photometric redshift accuracy decreases with magnitude and redshift, but does not vary monotonically with color or stellar mass. The 1 sigma scatter lies between 0.01 and 0.03 (1 + z) for galaxies of all masses and colors

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5

Blake, R. Melvin. "Photometric decomposition of NGC 6166." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1997. http://www.collectionscanada.ca/obj/s4/f2/dsk2/ftp04/mq22790.pdf.

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6

Silva, Fernández Simón Yeco. "Photometric Redshifts in the HDFS." Tesis, Universidad de Chile, 2015. http://repositorio.uchile.cl/handle/2250/133104.

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Magíster en Ciencias, Mención Astronomía<br>Se presenta fotometría óptica en 11 bandas medias a partir de observaciones realizadas con el telescopio de 2.2m en LSO (WFI) sobre un campo de ~30'×30' deg extendido en el Hubble Deep Field-South (EHDF-S), el cual es uno de los campos que contiene información en multibandas como parte del Multiwavelength Survey by Yale-Chile (MUSYC). Este campo tiene una gran cantidad de datos públicos y datos auxiliares en bandas UV, óptico, infrarrojo cercano e infrarrojo lejano. Se determinaron aperturas óptimas para fotometría de alta precisión para diversas fue

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7

Campisi, Andrea. "Development of a photometric stereo system." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2018.

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Photometric stereo is a method of estimating surface geometry by using a fixed-position camera and multiple light sources. The idea of photometric stereo is to vary the direction of incident illumination between successive images, while the viewing direction is constant; in this way, the correspondence of image points is known beforehand, as the position of the object is not changed, and surface orientation is determined by using the radiance values recorded with the different images. Photometric stereo has several applications: it is used to detect small surface defects, imperceptible to the

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8

Samaddar, Debasmita. "Photometric variability of three brown dwarfs." Access to citation, abstract and download form provided by ProQuest Information and Learning Company; downloadable PDF file 2.24 Mb., 65 p, 2006. http://proquest.umi.com/pqdlink?did=1075713471&Fmt=7&clientId=8331&RQT=309&VName=PQD.

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9

Buyukatalay, Soner. "Photometric Stereo Considering Highlights And Shadows." Phd thesis, METU, 2011. http://etd.lib.metu.edu.tr/upload/12613749/index.pdf.

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Three dimensional (3D) shape reconstruction that aims to reconstruct 3D surface of objects using acquired images, is one of the main problems in computer vision. There are many applications of 3D shape reconstruction, from satellite imaging to material sciences, considering a continent on earth or microscopic surface properties of a material. One of these applications is the automated firearm identification that is an old, yet an unsolved problem in forensic science. Firearm evidence matching algorithms rely on the fact that a firearm creates characteristic marks on surfaces of the bullets and

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10

Botzler, Christine S. "Finding Structures in Photometric Redshift Surveys." Diss., lmu, 2004. http://nbn-resolving.de/urn:nbn:de:bvb:19-22187.

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Libri sul tema "Photometric"

1

Booker, Robert L. Photometric calibrations. U.S. Dept. of Commerce, National Bureau of Standards, 1992.

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2

Ohno, Yoshihiro. Photometric calibrations. U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1997.

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3

A, McSparron Donald, and United States. National Bureau of Standards, eds. Photometric calibrations. U.S. Dept. of Commerce, National Bureau of Standards, 1992.

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4

Ohno, Yoshihiro. Photometric calibrations. U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1997.

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5

Ohno, Yoshihiro. Photometric calibrations. U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1997.

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6

Ohno, Yoshihiro. Photometric calibrations. U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1997.

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7

A, McSparron Donald, and United States. National Bureau of Standards., eds. Photometric calibrations. U.S. Dept. of Commerce, National Bureau of Standards, 1987.

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8

-I, Lagerkvist C., ed. Asteroid photometric catalogue. Astronomiska Observatoriet Uppsala, 1992.

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9

-I, Lagerkvist C., ed. Asteroid photometric catalogue. Consiglio nazionale delle ricerche, 1987.

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10

-I, Lagerkvist C., and Istituto astrofisica spaziale (Italy), eds. Asteroid photometric catalogue. Consiglio nazionale delle ricerche, Istituto di astrofisica spaziale, 1988.

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Capitoli di libri sul tema "Photometric"

1

Gooch, Jan W. "Photometric." In Encyclopedic Dictionary of Polymers. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-6247-8_8682.

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2

Weik, Martin H. "photometric." In Computer Science and Communications Dictionary. Springer US, 2000. http://dx.doi.org/10.1007/1-4020-0613-6_14004.

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3

Sterken, Chr, and J. Manfroid. "Photometric systems." In Astrophysics and Space Science Library. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2476-8_16.

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4

Sterken, Chr, and J. Manfroid. "Photometric filters." In Astrophysics and Space Science Library. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2476-8_5.

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5

Ikeuchi, Katsushi, Yasuyuki Matsushita, Ryusuke Sagawa, et al. "Photometric Stereo." In Active Lighting and Its Application for Computer Vision. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-56577-0_5.

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6

Ikeuchi, Katsushi, Yasuyuki Matsushita, Ryusuke Sagawa, et al. "Photometric Estimation." In Active Lighting and Its Application for Computer Vision. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-56577-0_8.

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7

Robles-Kelly, Antonio, and Cong Phuoc Huynh. "Photometric Invariance." In Imaging Spectroscopy for Scene Analysis. Springer London, 2013. http://dx.doi.org/10.1007/978-1-4471-4652-0_6.

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8

Basri, Ronen. "Photometric Stereo." In Computer Vision. Springer US, 2014. http://dx.doi.org/10.1007/978-0-387-31439-6_254.

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9

Zickler, Todd. "Photometric Invariants." In Computer Vision. Springer US, 2014. http://dx.doi.org/10.1007/978-0-387-31439-6_544.

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Zickler, Todd. "Photometric Invariants." In Computer Vision. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-63416-2_544.

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Atti di convegni sul tema "Photometric"

1

Lee, Barry B. "Physiological basis of photometry." In OSA Annual Meeting. Optica Publishing Group, 1990. http://dx.doi.org/10.1364/oam.1990.thf3.

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The human photopic luminous efficiency function, the basis of photopic photometry for over 50 years, may be derived from several psychophysical tasks. These tasks are sometimes assumed to tap a "luminance channel" in the visual system, but the physiological identity of this channel has been controversial. The physiological basis of two photometric tasks will be discussed. For flicker photometry, there is strong evidence that cells of the phasic, magnocellular system of the primate visual pathway form the substrate. Not only can photometric properties, such as additivity and transitivity, be de

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2

Lutze, Margaret, Nancy J. Cox, Vivianne C. Smith, and Joel Pokorny. "Genetics of Rayleigh matches and photometric matches in normals." In OSA Annual Meeting. Optica Publishing Group, 1988. http://dx.doi.org/10.1364/oam.1988.mz3.

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At the 1988 ARVO meeting we presented Rayleigh match midpoint and photometric match data collected from a population of nonrelated males and from family members. Photometric matches between a 667- and 551-nm stimulus were obtained using heterochromatic modulation photometry (HMP). We employed statistical methods to determine whether the source of variation for each of these traits was due to allelic variation at a single gene locus, variation at multiple loci (polygenic), or environmental factors. Results indicated that variations in Rayleigh match midpoints and HMP photometric matches in obse

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3

Shitomi, H. "METROLOGICAL IMPACT OF INTRODUCING CONE FUNDAMENTAL-BASED PHOTOMETRY AS THE BASIS TO DERIVE PHOTOMETRIC UNITS." In CIE 2023 Conference. International Commission on Illumination, CIE, 2023. http://dx.doi.org/10.25039/x50.2023.op035.

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CIE cone-fundamental-based photometry has drawn close attention as a concept to derive scientifically more reliable data to quantify visual sensation. Recently argument has been stirred up about the possibility to adopt a revised spectral luminous efficiency function VF(λ) based on the CIE cone-fundamentals as a standard function to derive photometry quantities, instead of current V(λ) function. While adopting a scientifically more rigorous concept in the SI is quite important, there seems controversy on the idea to replace from V(λ) to VF(λ). Two ways of analysis, in terms of the potential ch

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4

Haefner, Bjoern, Yvain Queau, and Daniel Cremers. "Photometric Segmentation: Simultaneous Photometric Stereo and Masking." In 2019 International Conference on 3D Vision (3DV). IEEE, 2019. http://dx.doi.org/10.1109/3dv.2019.00033.

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Zwinkels, Joanne C. "Issues and Strategies for Improving Measurement Uncertainties for Solid-State Lighting." In NCSL International Workshop & Symposium. NCSL International, 2016. http://dx.doi.org/10.51843/wsproceedings.2016.23.

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The use of solid-state lighting (SSL), such as light-emitting-diode (LED) products for general lighting and display applications, has increased dramatically over the past decade. However, there are significant photometric and radiometric metrological challenges with this new lighting technology. The photometric procedures and standards that have been developed for traditional lighting products, such as incandescent and compact fluorescent (CFL) lamps, do not work well for LEDs because they exhibit significantly different characteristics. This paper will discuss these differences in the spectra

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6

Popescu, Nedelia A. "Photometric redshifts determinations for galaxies by means of multicolor photometry." In FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP, 2007. http://dx.doi.org/10.1063/1.2720449.

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Olczak, Paul, and Jack Tumblin. "Photometric camera calibration." In ACM SIGGRAPH 2014 Posters. ACM Press, 2014. http://dx.doi.org/10.1145/2614217.2614244.

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Hauagge, Daniel, Scott Wehrwein, Kavita Bala, and Noah Snavely. "Photometric Ambient Occlusion." In 2013 IEEE Conference on Computer Vision and Pattern Recognition (CVPR). IEEE, 2013. http://dx.doi.org/10.1109/cvpr.2013.325.

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Du, Hao, Dan Goldman, and Steven Seitz. "Binocular Photometric Stereo." In British Machine Vision Conference 2011. British Machine Vision Association, 2011. http://dx.doi.org/10.5244/c.25.84.

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Calef, Brandoch, John Africano, Brian Birge, Doyle Hall, and Paul Kervin. "Photometric signature inversion." In SPIE Optics + Photonics, edited by Victor L. Gamiz, Paul S. Idell, and Marija S. Strojnik. SPIE, 2006. http://dx.doi.org/10.1117/12.683015.

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Rapporti di organizzazioni sul tema "Photometric"

1

Ohno, Yoshihiro. Photometric calibrations. National Institute of Standards and Technology, 1997. http://dx.doi.org/10.6028/nist.sp.250-37.

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2

Booker, Robert L., and Donald A. McSparron. Photometric calibrations. National Bureau of Standards, 1987. http://dx.doi.org/10.6028/nbs.sp.250-15.

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3

Perrin, TE, CC Brown, ME Poplawski, and NJ Miller. Characterizing Photometric Flicker. Office of Scientific and Technical Information (OSTI), 2017. http://dx.doi.org/10.2172/1607663.

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4

Zong, Yuqin, Maria E. Nadal, Benjamin K. Tsai, and C. Cameron Miller. NIST measurement services: photometric calibrations. National Institute of Standards and Technology, 2018. http://dx.doi.org/10.6028/nist.sp.250-95.

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5

Leon, Felipe A., Joshua A. McIntosh, Addison J. Rutz, Naomi J. Miller, and Michael P. Royer. Characterizing Photometric Flicker - Handheld Meters. Office of Scientific and Technical Information (OSTI), 2019. http://dx.doi.org/10.2172/1567860.

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6

Landolt, Arlo. Faint Photoelectric Photometric Standard Star Sequences. Defense Technical Information Center, 1988. http://dx.doi.org/10.21236/ada201999.

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7

Kent, Stephen, Mary Elizabeth Kaiser, Susana E. Deustua, et al. Photometric calibrations for 21st century science. Office of Scientific and Technical Information (OSTI), 2009. http://dx.doi.org/10.2172/951353.

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8

May, M. J. Photometric Calibration of the SPRED at the FTU Tokamak. Office of Scientific and Technical Information (OSTI), 1999. http://dx.doi.org/10.2172/15004653.

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9

Carrasco Kind, Matias. Probabilistic Photometric Redshifts in the Era of Petascale Astronomy. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1172583.

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10

Ortiz, M. Growing Self-Organizing Maps as Predictors for Photometric Redshift. Office of Scientific and Technical Information (OSTI), 2019. http://dx.doi.org/10.2172/1557954.

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