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Dissertations / Theses on the topic 'Photometric study'

Author: Grafiati

Published: 4 June 2021

Last updated: 26 July 2025

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1

Patel, Parimal. "A Photometric Study of Brightest Cluster Galaxies and Intracluster Light." Thesis, University of Nottingham, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.489891.

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Using deep Band r imaging of a sample of 26 clusters, we model the surface brightness of the central cD galaxies in each cluster using two-dimensional analytical fits. We find strong evidence, using X2 tests and an analysis of Petrosian profiles, for two components in the surface brightness profile and identify the outer component as being produced by unbound stars orbiting in the global cluster potential. We measure the structural properties of this intracluster light (ICL), as well as its luminosity, colour and spatial distribution and compare these with cluster masses and radii derived from

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Watson, Lyndon. "A photometric and spectroscopic study of selected southern, chromospherically active stars." Thesis, University of Canterbury. Astronomy, 1999. http://hdl.handle.net/10092/5718.

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The results of a combined photometric and high-resolution spectroscopic study of southern active-chromosphere stars selected from the ROSAT Bright Source Catalogue are presented. The star CS Ceti (HD 6628) is shown to be a single-lined spectroscopic binary and an orbital solution derived from radial-velocity measurements is presented. Evidence that one of the stars is an F-type dwarf and the other a highly active G-type subgiant is presented, together with information on the apparently asynchronous rotation of the latter and the spatial origin of its Hα emission. The system BB Sculptoris (HD

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Mazur, Brian. "A Photometric And Spectroscopic Study of Orion: From OB1b to Binaries." University of Toledo / OhioLINK, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=toledo1547208240532891.

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Carroll, Carla June. "A Feasibility Study of Photometric Reverberation Mapping with Meter-Class Telescopes." BYU ScholarsArchive, 2015. https://scholarsarchive.byu.edu/etd/5469.

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For the past several decades, mass estimates for supermassive black holes hosted by active galactic nuclei (AGN) have been made with the reverberation mapping (RM) technique. This methodology has produced consistent results and has been used to establish several relations that link the characteristics of the host galaxy to the mass of the central black hole. Despite this success, there are less than 50 AGN with black hole masses derived from RM. This low number is generally attributed to the difficulties in coordinating large blocks of telescope time for making simultaneous photometric and spe

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5

Cocozza, Gabriele <1974&gt. "A spectroscopic and photometric study of MSP companions in Galactic Globular Clusters." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2008. http://amsdottorato.unibo.it/631/1/Tesi_Cocozza_Gabriele.pdf.

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This Thesis is devoted to the study of the optical companions of Millisecond Pulsars in Galactic Globular Clusters (GCs) as a part of a large project started at the Department of Astronomy of the Bologna University, in collaboration with other institutions (Astronomical Observatory of Cagliari and Bologna, University of Virginia), specifically dedicated to the study of the environmental effects on passive stellar evolution in galactic GCs. Globular Clusters are very efficient “Kilns” for generating exotic object, such as Millisecond Pulsars (MSP), low mass X-ray binaries(LMXB) or Blue S

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Cocozza, Gabriele <1974&gt. "A spectroscopic and photometric study of MSP companions in Galactic Globular Clusters." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2008. http://amsdottorato.unibo.it/631/.

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This Thesis is devoted to the study of the optical companions of Millisecond Pulsars in Galactic Globular Clusters (GCs) as a part of a large project started at the Department of Astronomy of the Bologna University, in collaboration with other institutions (Astronomical Observatory of Cagliari and Bologna, University of Virginia), specifically dedicated to the study of the environmental effects on passive stellar evolution in galactic GCs. Globular Clusters are very efficient “Kilns” for generating exotic object, such as Millisecond Pulsars (MSP), low mass X-ray binaries(LMXB) or Blue S

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Pohlen, Michael. "The radial structure of galactic stellar disks surface photometric study on disk galaxies /." [S.l.] : [s.n.], 2001. http://deposit.ddb.de/cgi-bin/dokserv?idn=964128535.

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Kindl, Enrico. "A photometric and morphological study of compact groups of galaxies and their environments." Thesis, University of British Columbia, 1987. http://hdl.handle.net/2429/30722.

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This thesis examines properties of galaxies in and around compact groups. Astrometry, photometry and morphological classifications are derived from CCD images for all 463 galaxies in Hickson's sample of 100 compact groups. Some minor revisions to the membership of the original catalog are made. At high galactic latitude (b > 30°), the catalog is estimated to be 90% complete for groups with total B[formula omitted] magnitude 13.0 or less. 49% of all the catalogued galaxies, and 48% of first-ranked galaxies are spiral. No significant difference is found between the distribution of morphological

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9

Cluver, Michelle E. "Probing distant clusters : a pre-SALT photometric study of intermediate redshift galaxy cluster." Master's thesis, University of Cape Town, 2005. http://hdl.handle.net/11427/4415.

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tundo, elena. "Supermassive Black Holes: a spectroscopic and photometric study on the connection with their host galaxies." Doctoral thesis, Università degli studi di Padova, 2010. http://hdl.handle.net/11577/3426936.

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One of the main themes in extragalactic astronomy for the next decade will be the evolution of galaxies over cosmic time. It has, however, become clear that the properties and the evolution of galaxies are intimately linked to the growth of their Supermassive Black Holes (SMBH). Understanding the formation of galaxies, and their subsequent evolution, will therefore be incomplete without clearifing the connection between the SMBHs and their host galaxies. The formation, assembly history, and environmental impact of the SMBHs that are ubiquitous in the nuclei of luminous galaxy rema

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11

Mitchison, S. M. "A near-infrared photometric study of Rho Ophiunchus, Cygnus OB7, and five galactic plane molecular clouds." Thesis, University of Kent, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.594168.

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In this study, two nearby, low-mass star-forming regions (Ll688 in Rho Ophiuchus and L1003 in Cygnus OB7) were compared with a relatively unbiased sample of Galactic Plane molecular clouds < 2 kpc from the Sun. The study was motivated by a relative lack of unbiased surveys of this kind; most regions are surveyed following the discovery of significant st.ar formation. The photometric data here was obtained from the Wide Field Camera of the United Kingdom Infrared Telescope. Candid.te populations of young stellar objects were identified using near-infrared colour-colour diagrams and analysed sys

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Eriksson, Simon. "A Photometric Variability Study Using Brown Dwarfs As Giant Planet Analogues : Investigating rotation periods and cloud structure." Thesis, Stockholms universitet, Institutionen för astronomi, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-152174.

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Mucciarelli, Alessio <1980&gt. "A spectroscopic and photometric study of stellar populations in a sample of clusters in the Magellanic Clouds." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2008. http://amsdottorato.unibo.it/632/1/Tesi_Mucciarelli_Alessio.pdf.

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This Ph.D. Thesis has been carried out in the framework of a long-term and large project devoted to describe the main photometric, chemical, evolutionary and integrated properties of a representative sample of Large and Small Magellanic Cloud (LMC and SMC respectively) clusters. The globular clusters system of these two Irregular galaxies provides a rich resource for investigating stellar and chemical evolution and to obtain a detailed view of the star formation history and chemical enrichment of the Clouds. The results discussed here are based on the analysis of high-resolution photomet

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Mucciarelli, Alessio <1980&gt. "A spectroscopic and photometric study of stellar populations in a sample of clusters in the Magellanic Clouds." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2008. http://amsdottorato.unibo.it/632/.

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This Ph.D. Thesis has been carried out in the framework of a long-term and large project devoted to describe the main photometric, chemical, evolutionary and integrated properties of a representative sample of Large and Small Magellanic Cloud (LMC and SMC respectively) clusters. The globular clusters system of these two Irregular galaxies provides a rich resource for investigating stellar and chemical evolution and to obtain a detailed view of the star formation history and chemical enrichment of the Clouds. The results discussed here are based on the analysis of high-resolution photomet

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15

Önehag, Anna. "Solar Type Stars as Calibrators : A Photometric and Spectroscopic Study on the Atmospheric Properties of Late-type Stars." Doctoral thesis, Uppsala universitet, Institutionen för fysik och astronomi, 2011. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-158709.

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Detailed knowledge of solar-type stars is essential in the understanding of the evolutionary past, presence and future of the Sun as well as the formation of its planetary system. Moreover, solar-type stars are of key significance for the study of the evolution of the Galaxy. The ages of solar-type stars map the full galactic evolution. Their surface layers are well mixed and just little affected by the interior nuclear processes. They may therefore be used as samples of the gas from which the stars were once formed. Models of stellar atmospheres are used to derive fundamental stellar quantiti

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Kotze, J. P. "A deep photometric survey of the Abell cluster SO423 : a pilot study for the UCT SALT supercluster survey." Master's thesis, University of Cape Town, 2007. http://hdl.handle.net/11427/4422.

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Flateau, Davin C. "Weather on Other Worlds IV: In-Depth Study of Photometric Variability and Radiative Timescales for Atmospheric Evolution in Four L Dwarfs." Thesis, The University of Arizona, 2015. http://hdl.handle.net/10150/594630.

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Rotational phase mapping of brown dwarfs allows exploration of different cloud and photospheric properties within the same atmospheres, allowing a separation of these parameters from global parameters, such as composition, surface gravity, and age. This work presents an in-depth characterization of high SNR light curves from the Spitzer Space Telescope with up to 13 hours of continuous monitoring of four dwarfs spanning the L3 to L8 spectral type. An exhaustive exploration of currently available state-of-the-art models explains the observed color changes for two of these dwarfs with a linear c

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Kosyra, Ralf [Verfasser], and Ralf [Akademischer Betreuer] Bender. "Environmental selection effects of Sunyaev Zel'dovich selected clusters of galaxies and instrumentation dedicated to the photometric study of large scale structure / Ralf Kosyra. Betreuer: Ralf Bender." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2016. http://d-nb.info/1111505209/34.

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Kosyra, Ralf Verfasser], and Ralf [Akademischer Betreuer] [Bender. "Environmental selection effects of Sunyaev Zel'dovich selected clusters of galaxies and instrumentation dedicated to the photometric study of large scale structure / Ralf Kosyra. Betreuer: Ralf Bender." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2016. http://d-nb.info/1111505209/34.

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Hsu, Li-Ting [Verfasser], and Kirpal [Akademischer Betreuer] Nandra. "Photometric redshifts of faint X-ray sources : paving the way towards the study of AGN/galaxy co-evolution over cosmic time / Li-Ting Hsu. Betreuer: Kirpal Nandra." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2015. http://d-nb.info/1082504769/34.

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Wu, Tai-Pang. "A study on photometry in computer vision : shadow, stereo and separation /." View abstract or full-text, 2005. http://library.ust.hk/cgi/db/thesis.pl?COMP%202005%20WU.

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Bowens-Rubin, Rachel (Rachel A. ). "Feasibility-study for space-based transit photometry using mid-sized nanosatellites." Thesis, Massachusetts Institute of Technology, 2012. http://hdl.handle.net/1721.1/77872.

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Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2012.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (p. 85-88).<br>The photometric precision needed to measure a transit of small planets cannot be achieved by taking observations from the ground, so observations must be made from space. Mid-sized nanosatellites can provide a low-cost option for building an optical system to take these observations. The potential of using nanosatellites of varying sizes to perform transit measurements was evaluated using

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Ferreira, João Pedro de Jesus. "A broad-band study of the evolving emission-line properties of galaxies." Thesis, University of Edinburgh, 2018. http://hdl.handle.net/1842/28717.

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This thesis describes a new approach to the study of high-redshift star-formation and its environments that can be applied to large high-redshift surveys. Instead of relying on spectroscopy or narrow-band photometry to study galaxy line emission in detail, the properties of large emission line galaxy (ELG)populations are estimated from broadband photometry by measuring colour-residuals against colours drawn from a set of line-free stochastic burst models-based on (Bruzual & Charlot, 2003). Simulated star-formation histories drawn from semi-analytic and adaptive-mesh-refinement codes were conve

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Wall, Wilson. "A study of variation in human chromosomes shown by photometry, G, C, replication banding and in situ hybridisation." Thesis, Open University, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.314792.

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Hjort, Adam. "Future directions in the study of Asymptotic Giant Branch Stars with the James Webb Space Telescope." Thesis, Uppsala universitet, Observationell astrofysik, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-303344.

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In this study we present photometric predictions for C-type Asymptotic Giant Branch Stars (AGB) stars from Eriksson et al. (2014) for the James Webb Space Telescope (JWST) and the Wide-field Infrared Survey Explorer (WISE) instruments. The photometric predictions we have done are for JWST’s general purpose wide-band filters on NIRCam and MIRI covering wavelengths of 0.7 — 21 microns. AGB stars contribute substantially to the integrated light of intermediate-age stellar popula- tions and is a substantial source of the metals (especially carbon) in galaxies. Studies of AGB stars are (among other

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Czanik, Robert Johann. "An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik." Thesis, North-West University, 2013. http://hdl.handle.net/10394/9102.

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This study consisted of an optical photometric and spectroscopic analysis on a 7′ 7′ field around the Southern high mass star forming region RCW 34. A previous study on RCW 34 in the NIR discov- ered many deeply embedded young stellar objects which were suspected to be T Tauri stars and which justified further investigation. The data used in this study consisted of three sets, the first two are photometric and spectroscopic data sets which were obtained during the first two weeks of February 2002. A third data set of spectroscopic observations was obtained by the author during the second wee

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Caballero, García María Dolores. "Integral spectroscopy of black hole transients and multi-wavelengh study of a new accreting binary system." Doctoral thesis, Universitat de Barcelona, 2008. http://hdl.handle.net/10803/663215.

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En esta tesis utilizamos los instrumentos de altas energías del satélite INTEGRAL para hacer espectroscopía y la cámara OMC para hacer fotometría de dos tipos diferentes de objetos celestes emisores de rayos X. INTEGRAL permite obtener la espectroscop´ıa en rayos X y γ (cubriendo un rango espectral de 3–8000 keV) y OMC es una cámara CCD que opera en el ﬁltro V de Johnson, capaz de proporcionar una monitorización continua de las fuentes cientíﬁcas incluídas en el OMC Input Catalogue. La capacidad de hacer espectroscopía nos p

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Aljassim, Mohammad A. "A 6-Year Study of Long Period Variable Stars in the Globular Cluster NGC 6388." Bowling Green State University / OhioLINK, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1499442952467274.

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Chen, An-Chen, and 陳安貞. "Photometric Study of AGN Host Galaxies." Thesis, 2004. http://ndltd.ncl.edu.tw/handle/70407381680745346029.

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碩士<br>國立中央大學<br>天文研究所<br>92<br>We have obtained multi-band (BVR) photometry of a sample of 41 active galaxies, including type 1 Seyfert, type 2 Seyfert galaxies, and low ionization nuclear emission region (LINER). In order to study the physical properties of AGN host galaxies. the intensity pro les in each band are obtained. We calculate the colors of the nuclei and the e ective radii using average B-V, and V-R value. We nd that the Seyfert 1 galaxies have bluer nucleus color. We also caculate the nucleus-to-galaxy ratio, and find that the Seyfert 1 galaxies have higher ratio.

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PENNINGTON, ROBERT LEE. "A SURFACE PHOTOMETRIC STUDY OF NGC 5128." Thesis, 1985. http://hdl.handle.net/1911/15928.

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Calibrated digital surface photometry in the standard UBV pass- bands has been used to prepare two dimensional maps to examine the structure and stellar populations in NGC 5128 (Cen A). The main body of the galaxy exhibits colors and stellar populations slightly bluer than those of an old elliptical galaxy out to r (TURN) 176". Beyond this radius, excess emission in the inner halo contributes significantly to the U passband only, probably due to line emission from material swept into the halo from the dust lane. A gradient in B-V of (TURN)0('m)01/ 1.5 (D/3) kpc is evident along the major axis

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Huang, Jen-Chao, and 黃仁昭. "Photometric Study of Morphologically Identified Merging Galaxies." Thesis, 2011. http://ndltd.ncl.edu.tw/handle/69920293984525526041.

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碩士<br>國立中央大學<br>天文研究所<br>99<br>We investigate the photometric properties of the merging galaxies that were identified morphologically in the Red Sequence Cluster Survey 2 (RCS2) in 381 square degrees. We develop and apply an adaptive aperture photometry technique to retrieve all the available passband photometry from the RCS2 images. We also develop a color-color classification method by referring a set of empirical galaxy SED templates to study the color properties of these merging galaxies. We find that we have observed more red ellipticall-like mergers at relative high redshifts. Our res

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Kane, Stephen Robert. "A spectroscopic and photometric study of gravitational microlensing events." Thesis, 2000. https://eprints.utas.edu.au/20476/1/whole_KaneStephenRobert2000_thesis.pdf.

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Gravitational microlensing has generated a great deal of scientific interest over recent years. This has been largely due to the realization of its wide-reaching applications, such as the search for dark matter, the detection of planets, and the study of Galactic structure. A significant observational advance has been that most microlensing events can be identified in real-time while the source is still being lensed. More than 400 microlensing events have now been detected towards the Galactic bulge and Magellanic Clouds by the microlensing survey teams EROS, MACHO, OGLE, DUO, and MOA.

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Hsiang-Yao, Hsiao. "The Photometric Study of Eight Open Clusters with Different Ages." 2006. http://www.cetd.com.tw/ec/thesisdetail.aspx?etdun=U0021-2304200715042703.

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Hsiao, Hsiang-Yao, and 蕭翔耀. "The Photometric Study of Eight Open Clusters with Different Ages." Thesis, 2007. http://ndltd.ncl.edu.tw/handle/90160609746079824570.

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碩士<br>國立臺灣師範大學<br>地球科學系<br>95<br>The (U)BV CCD photometry of eight open clusters with different ages and distance are study. Five open clusters (IC348, NGC 2244, NGC 2301, NGC 5385, and Czernik 10) were observed with U, B, and V photometry, and the other three open clusters (NGC 2395, King 6 and NGC 663) only with B and V photometry. For IC348, the reddening E(B-V) is about 0.8, and its distance and age are 320 pc and 4.0-6.3 M yrs, respectively; The reddening of NGC 2244 is about 0.45, and its distance and age are 1320 pc and 4-13 Myrs, respectively. The reddening of NGC 2301 is about 0.08, a

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Chatelain, Joseph. "De Ilii Coloribus: A Photometric Study of the Largest Jupiter Trojan Asteroids." 2017. http://scholarworks.gsu.edu/phy_astr_diss/95.

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The Jupiter Trojan asteroids are minor bodies that orbit 60 degrees before and 60 degrees behind Jupiter. Because these orbits are stable over the lifetime of the Solar System, the properties of these objects may inform us about the conditions under which the Solar System formed. We present BVRI photometry for 110 of the intrinsically brightest and presumably largest members of the L4 and L5 Jupiter Trojans. We use a new principal color component derived by Chatelain et al. (2016) that is indicative of taxonomic types relevant to the Jupiter Trojan asteroids. We find that 83% of the largest Ju

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Nikolov, Krasimirov Nikolay [Verfasser]. "A photometric study of transiting extrasolar planets / put forward by Nikolay Krasimirov Nikolov." 2011. http://d-nb.info/1013226879/34.

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Cheng, Ping-Han, and 鄭秉漢. "Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225." Thesis, 2011. http://ndltd.ncl.edu.tw/handle/82040872684550253495.

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碩士<br>國立中央大學<br>天文研究所<br>99<br>Time-series photometric observations were carried over sixty nights in 2009 using the 81-cm Tenagra telescope in Arizona within the framework of a multi-year survey program of variable stars in open clusters. The analysis of NGC 1513 and NGC 225 was a pilot study of this effort, we also developed the basic algorithms of the eclipsing binary to compute the data points from our observations to understand the characteristics of eclipsing binary stars in NGC 1513 and NGC 225. About the model, we create some invented observation data to prove the accuracy of its. Tota

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Pohlen, Michael [Verfasser]. "The radial structure of galactic stellar disks : surface photometric study on disk galaxies / von Michael Pohlen." 2001. http://d-nb.info/964128535/34.

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Cheng, Yu-Chi, and 鄭宇棋. "Photometric Analysis and Dynamic Study of Short Period Comets with Distant Coma Activities from Pan-STARRS 1 Survey." Thesis, 2016. http://ndltd.ncl.edu.tw/handle/10162605464341276066.

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博士<br>國立中央大學<br>天文研究所<br>104<br>I developed a systematic method to analyze the snapshot images from sky survey projects such as the Pan-STARRS 1 (PS1) and Palomar Transient Factory (PTF) on all the numbered Jupiter Family Comets (JFCs). There are three objectives for my image processing pipeline to handling the five years survey data: to find out images that contains target of interest; to identify the signature of coma activity; and to measure the level of outgassing activity. Given that cometary activities are generally triggered by the sublimation of water ice, I introduce the water ice sno

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Jeffery, Elizabeth Jane. "White dwarfs and the ages of open clusters." 2009. http://hdl.handle.net/2152/10652.

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Open clusters have long been objects of interest in astronomy. As a good approximation of essentially pure stellar populations, they have proved very useful for studies in a wide range of astrophysically interesting questions, including stellar evolution and atmosphere, the chemical and dynamical evolution of our Galaxy, and the structure of our Galaxy. Of fundamental importance to our understanding of open clusters, as well as many other questions in astrophysics, is the accurate determination of ages. Currently there are two main techniques for independently determining the ages of stella

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Choudhury, Samyaday. "Study of Evolved Stellar Populations in the Magellanic Clouds." Thesis, 2015. http://etd.iisc.ac.in/handle/2005/3662.

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The Magellanic Clouds (MCs) consist of a pair of galaxies, the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC), which are located at a distance of 50 kpc and 60 kpc, with stellar masses of 1010 M and 109 M , respectively. Morphologically they are categorized as irregular type galaxies. The MCs are gas rich and metal poor (Z=0.008 for LMC, and 0.004 for SMC) as compared to the Milky Way (MW), and have active star-forming regions. Their proximity and location at high galactic latitude enable us to resolve their individual populations as well as detect faint stellar populations.

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Choudhury, Samyaday. "Study of Evolved Stellar Populations in the Magellanic Clouds." Thesis, 2015. http://etd.iisc.ernet.in/2005/3662.

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The Magellanic Clouds (MCs) consist of a pair of galaxies, the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC), which are located at a distance of 50 kpc and 60 kpc, with stellar masses of 1010 M and 109 M , respectively. Morphologically they are categorized as irregular type galaxies. The MCs are gas rich and metal poor (Z=0.008 for LMC, and 0.004 for SMC) as compared to the Milky Way (MW), and have active star-forming regions. Their proximity and location at high galactic latitude enable us to resolve their individual populations as well as detect faint stellar populations.

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Gupta, Prashansa. "Reflected Light of Exoplanets : a case study of WASP-43b using the Hubble Space Telescope." Thèse, 2019. http://hdl.handle.net/1866/23814.

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Avec près de 4000 exoplanètes connues, le domaine est passé de simplement détecter des exoplanètes à étudier leurs propriétés atmosphériques. Cependant, les spectres en lumières réfléchies de ces objets sont encore mal compris. Les exoplanètes réfléchissent une partie de la lumière qu’elles reçoivent de leur étoile, selon les propriétés de l’atmosphère, ce qui affecte le budget énergétique de la planète. Les Jupiters chaudes, c’est-à-dire des planètes de types Jupiter avec des périodes orbitales très courtes, sont les cibles les plus faciles à observer par spectroscopie des éclipses. L’albédo

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Chen, Chang-Hui, and 陳昌慧. "Photometry Study of NGC288 on uvby Bandpass." Thesis, 1996. http://ndltd.ncl.edu.tw/handle/99493105612966218669.

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蔡文旭. "Multiband Photometry Study of NGC288 on BATC Filter System." Thesis, 1999. http://ndltd.ncl.edu.tw/handle/12565537472450976417.

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46

Wainscoat, Richard James. "An infrared and optical study of edge-on galaxies." Phd thesis, 1986. http://hdl.handle.net/1885/138692.

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黃晟庭. "A study of reddening and extinction with UBV photometry of open clusters." Thesis, 2007. http://ndltd.ncl.edu.tw/handle/27158030447771003520.

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碩士<br>國立臺灣師範大學<br>地球科學系<br>95<br>For estimating accurately the distance and age of an open cluster with UBV photometry, the photometry of each member should be corrected by means of reddening and extinction. But the correction of reddening and extinction is usually done for the OB type stars only, the distribution on the TCD is looks likely linear. In this work, the correction of reddening and extinction is tried to G6V-K3V stars using the corrective processes as same as that for OB stars with the value of constants of equations for reddening and extinction taken from literature. The total fi

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Themeẞl, Nathalie. "Asteroseismic inferences from red-giant stars." Doctoral thesis, 2018. http://hdl.handle.net/11858/00-1735-0000-002E-E5F1-E.

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