Teses / dissertações sobre o tema "Chandrian"
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Bhowmik, Shefali. "Bangla Upanyase Prem o Bibaha:Bankim Chandra-Rabindra Nath-Sharat Chandra বাংলা উপন্যাসে প্রেম ও বিবাহ : বঙ্কিমচন্দ্র - রবীন্দ্রনাথ -শরৎচন্দ্র". Thesis, University of North Bengal, 1998. http://hdl.handle.net/123456789/1652.
Texto completo da fonteKakati, Jogesh. "Subhas Chandra Bose and the British Raj". Thesis, University of North Bengal, 2005. http://hdl.handle.net/123456789/1249.
Texto completo da fonteOtto, Tobias [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra, Gerd [Gutachter] Wanielik e Martin [Gutachter] Hagen. "Propagation effects influencing polarimetric weather radar measurements / Tobias Otto ; Gutachter: Madhukar Chandra, Gerd Wanielik, Martin Hagen ; Betreuer: Madhukar Chandra". Chemnitz : Universitätsbibliothek Chemnitz, 2011. http://d-nb.info/1213904889/34.
Texto completo da fonteMaurya, Devalāla. "Hindī sāhitya kā itihāsa-darśana aura Rāmacandra Śukla /". Ilāhābāda : Eksīlensa pabliśarsa, 1993. http://catalogue.bnf.fr/ark:/12148/cb36190705w.
Texto completo da fonteDalla, Mura Maria Elisabetta. "Ricerca di AGN oscurati nei Chandra Deep Fields". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/9893/.
Texto completo da fontePhruksahiran, Narathep [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra e Gerd [Gutachter] Wanielik. "Polarimetrische Streuungseigenschaften und Fokussierungsmethoden zur quantitativen Auswertung der polarimetrischen SAR-Daten / Narathep Phruksahiran ; Gutachter: Madhukar Chandra, Gerd Wanielik ; Betreuer: Madhukar Chandra". Chemnitz : Universitätsbibliothek Chemnitz, 2013. http://d-nb.info/121424520X/34.
Texto completo da fonteAqbi, Sadiq [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra e Ian Andrew [Gutachter] Glover. "Improving the Performance of Dual Linear Polarization Antennas with Metamaterial Structures / Sadiq Aqbi ; Gutachter: Madhukar Chandra, Ian Andrew Glover ; Betreuer: Madhukar Chandra". Chemnitz : Universitätsbibliothek Chemnitz, 2018. http://d-nb.info/121464984X/34.
Texto completo da fonteIbba, Tiziana. "Chandra investigation of 3CRR radio sources at high redshift". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/20023/.
Texto completo da fonteRutherford, John (John Morton). "Imaging X-ray spectroscopy with micro-X and Chandra". Thesis, Massachusetts Institute of Technology, 2013. http://hdl.handle.net/1721.1/84183.
Texto completo da fonteThis electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
Cataloged from student-submitted PDF version of thesis.
Includes bibliographical references (pages 245-258).
High spectral resolution observations of X-ray phenomena have the potential to uncover new physics. Currently, only point sources can be probed with high resolution spectra, using gratings. Extended objects like supernova remnants cannot be dispersed, leaving the dense forest of emission lines blended by the moderate resolution of modern instruments. In the first half of this thesis, I undertake two investigations of the supernova remnant Cassiopeia A using the flagship X-ray observatory, Chandra. The first study combines the spatial resolution of the ACIS instrument with the spectral resolution of the dispersive HETG to investigate the evolution of ejecta knots. The second improves on statistical limits of radioactive ejecta, and simulates what higher resolution instruments may observe. Micro-X, a new high resolution X-ray telescope, is the focus of the second half. I detail the commissioning of this novel sounding rocket payload, which uses a focal plane of micro-calorimeters to achieve high spectral resolution in each pixel. The flight hardware is in a final state of testing and integration before the launch, which is anticipated in 2014.
by John Rutherford.
Ph.D.
Rosignoli, Luca. "Analisi dettagliata di nuove osservazioni Chandra di Abell 2495". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2022. http://amslaurea.unibo.it/25297/.
Texto completo da fonteSom, Sarkar Dipika. "Iswar Chandra Gupter kabya bhasha ঈশ্বরচন্দ্র গুপ্তের কাব্য-ভাষা". Thesis, University of North Bengal, 1991. http://hdl.handle.net/123456789/1776.
Texto completo da fonteEckmiller, Helen [Verfasser]. "Testing X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups and Detailed Analysis of A2244 with Chandra and Suzaku / Helen Eckmiller". Bonn : Universitäts- und Landesbibliothek Bonn, 2012. http://d-nb.info/1044081880/34.
Texto completo da fonteVollbracht, Dennis [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra e Dirk [Gutachter] Fischer. "Design and development of phased-array antennas for dual-polarized weather radar applications / Dennis Vollbracht ; Gutachter: Madhukar Chandra, Dirk Fischer ; Betreuer: Madhukar Chandra". Chemnitz : Universitätsverlag Chemnitz, 2019. http://d-nb.info/1219664766/34.
Texto completo da fonteZichner, Ralf [Verfasser], Madhukar [Akademischer Betreuer] Chandra, Madhukar [Gutachter] Chandra, Reinhard R. [Akademischer Betreuer] Baumann e Reinhard R. [Gutachter] Baumann. "Hochfrequenz‐Kommunikation gedruckter Antennen in herausfordernden dielektrischen oder metallischen Umgebungen / Ralf Zichner ; Gutachter: Madhukar Chandra, Reinhard R. Baumann ; Madhukar Chandra, Reinhard R. Baumann". Chemnitz : Universitätsbibliothek Chemnitz, 2013. http://d-nb.info/1214245935/34.
Texto completo da fonteDebnath, Sailen. "Netaji Subhas Chandra Bose and secularism : his ideas and activities". Thesis, University of North Bengal, 1986. http://hdl.handle.net/123456789/1221.
Texto completo da fonteBhattacharya, Rama. "A critical approach to the short stories of Jagadish Chandra Gupta". Thesis, University of North Bengal, 1989. http://hdl.handle.net/123456789/1199.
Texto completo da fonteBertola, Elena. "The Chandra and XMM-Newton views of the Einstein Cross". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2019. http://amslaurea.unibo.it/17624/.
Texto completo da fonteHollowood, Devon. "Cosmological Studies through Large-Scale Distributed Analysis of Chandra Observations". Thesis, University of California, Santa Cruz, 2019. http://pqdtopen.proquest.com/#viewpdf?dispub=10973254.
Texto completo da fonteThe formation history of galaxy clusters is a powerful probe of cosmology. In particular, one may place strong constraints on the dark energy equation of state by examining the evolution across redshift of the number density of galaxy clusters as a function of mass. In this thesis, I describe my contributions to cluster cosmology, in particular to the development of the richness optical observable mass proxy.
I introduce redMaPPer, an optical cluster finder which represents an important upstream input for my thesis work. I next introduce the Mass Analysis Tool for Cha ndra (MATCha), a pipeline which uses a parallelized algorithm to analyze archival Chandra data. MATCha simultaneously calculates X-ray temperatures and luminosities and performs centering measurements for hundreds of potential galaxy clusters using archival X-ray exposures. I run MATCha on the redMaPPer SDSS DR8 cluster catalog and use MATCha's output X-ray temperatures and luminosities to analyze the galaxy cluster temperature-richness, luminosity-richness, luminosity-temperature, and temperature-luminosity scaling relations. I investigate the distribution of offsets between the X-ray center and redMaPPer center within 0.1 < z < 0.35 and explore some of the causes of redMaPPer miscentering. I collaborate with members of the Dark Energy Survey in order to repeat this analysis on Dark Energy Survey Year 1 data. I outline the various ways in which MATCha constitutes an important upstream work for a variety of astrophysical applications. These include the calibrations of two separate mass proxies, the study of the AGN fraction of galaxy clusters, and cosmology from cluster number densities and stacked weak lensing masses. Finally, I outline future upgrades and applications for MATCha throughout the lifespan of the Dark Energy Survey and the Large Synoptic Survey Telescope.
Bartolini, Chiara. "Proprietà termiche della galassia Jellyfish JO194 derivate da un'osservazione Chandra". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/24939/.
Texto completo da fontePAPALEXIOU, NIKOLAOS. "Sur la methode des orbites et l'homomorphisme de harish-chandra". Paris 7, 1998. http://www.theses.fr/1998PA077119.
Texto completo da fonteHanisch, Christoph. "Why the Law matters to you: Citizenship, Agency, and Public Identity". Bowling Green State University / OhioLINK, 2012. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1339933456.
Texto completo da fonteKhan, Akbar Ali. "Netaji Subash Chandra Bose and the provisional government of Azad Hind-an analytical construction". Thesis, University of North Bengal, 2003. http://hdl.handle.net/123456789/1200.
Texto completo da fonteHui, Chung Yue. "X-Ray Observations of Neutron Stars with XMM-Newton & Chandra". Diss., lmu, 2007. http://nbn-resolving.de/urn:nbn:de:bvb:19-89872.
Texto completo da fonteGonzalez, Edgar Raul 1977. "Results from five Chandra observations of the normal galaxy NGC 3877". Thesis, Massachusetts Institute of Technology, 2004. http://hdl.handle.net/1721.1/32740.
Texto completo da fonteIncludes bibliographical references (p. 67-72).
We present the results of five Chandra observations of the normal galaxy NGC 3877. A total of 27 X-ray sources are detected, including SN 1998S. We find 15 sources to be variable during the 646-day period covered by the observations. We use two methods to determine source color and find no apparent correlation between color and brightness in our population sample. We provide flux and luminosity estimates for every source and construct cumulative X-ray luminosity functions (XLFs) for each observation. We find a higher density of luminous ([approximately] 10³⁷ erg s⁻¹) sources in NGC 3877 than we see in two other galaxies. We tentatively identify some sources as X-ray binaries.
by Edgar Raul Gonzalez.
S.B.
Stevens, J. A. "Colonial subjectivity : Keshab Chandra Sen in London and Calcutta, 1870-1884". Thesis, University College London (University of London), 2011. http://discovery.ucl.ac.uk/1333989/.
Texto completo da fonteChandrasekharan, Nair Vinod Chandran [Verfasser], e Martin [Akademischer Betreuer] Jansen. "Heteronuclear spin decoupling sequences with frequency sweep in solid-state NMR spectroscopy / Vinod Chandran Chandrasekharan Nair. Betreuer: Martin Jansen". Stuttgart : Universitätsbibliothek der Universität Stuttgart, 2012. http://d-nb.info/1021343560/34.
Texto completo da fonteIgnesti, Alessandro. "A combined JVLA and Chandra study of the Abell 2626 galaxy cluster". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2017. http://amslaurea.unibo.it/12817/.
Texto completo da fonteGuerra, Raffaella. "Studio della variabilità dal centro galattico in 14 anni di osservazioni Chandra". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2017. http://amslaurea.unibo.it/12935/.
Texto completo da fontePekon, Yakup. "Analysis Of Chandra Data Of The Old Classical Nova Rr Pic (1925)". Master's thesis, METU, 2007. http://etd.lib.metu.edu.tr/upload/12608716/index.pdf.
Texto completo da fonteand observations with better spectral resolution are needed to determine the exact transitions. The source spectrum is better explained with photoionized plasma model rather than the cooling flow model. It has also been found that the neutral Hydrogen column density differs for orbital minimum and orbital maximum spectra with values 0.25 (+0.23 -0:18)*10^22 atoms/cm2 and 0.64 (+0.13 -0.14)*10^22 atoms/cm2 respectively at 3 sigma confidence level. The difference of neutral Hydrogen column density between the maximum and minimum phase spectra indicates existence of a warm absorbing region on the disc at the location of the impact zone.
Shrestha, Jyoti Chandra [Verfasser]. "Theoretical and experimental study of intracavity laser absorption spectroscopy / Jyoti Chandra Shrestha". Kassel : Universitätsbibliothek Kassel, 2015. http://d-nb.info/1069569550/34.
Texto completo da fonteThakur, Harish Chandra [Verfasser]. "Biochemical and biophysical characterization of the centrosomal protein TACC3 / Harish Chandra Thakur". Düsseldorf : Universitäts- und Landesbibliothek der Heinrich-Heine-Universität Düsseldorf, 2013. http://d-nb.info/1036727491/34.
Texto completo da fonteKraev, Urmila Mitra. "Flares on active M-type stars observed with XMM-Newton and Chandra". Thesis, University College London (University of London), 2007. http://discovery.ucl.ac.uk/1444852/.
Texto completo da fonteBonzini, Margherita. "The sub-mJy radio population in the Extended Chandra Deep Field South". Diss., Ludwig-Maximilians-Universität München, 2014. http://nbn-resolving.de/urn:nbn:de:bvb:19-173655.
Texto completo da fonteTiefe Beobachtungen im Radiobereich ermöglichen einen Blick auf aktive schwarze Löcher (”black holes“, BH) und auch Gebiete aktiver Sternentstehung (”star formation“, SF), ohne dass die Beobachtungen durch den Staub in Galaxien beeinflusst werden. Daher sind Radiobeobachtungen ideal, um deren Entwicklung und eine mögliche gegenseitige Beeinflussung von BH und SF Aktivit¨at über kosmische Zeiten hinweg zu untersuchen. Radioastronomie gewinnt darum für die Erforschung von Galaxienentwicklung zunehmend an Bedeutung. Dies ist auch bedingt durch die zahlreichen neuen Radioanlagen, die im Bau oder in Planung sind. Um das Potential dieser neuen Instrumente zu maximieren, ist es essentiell Vorhersagen dar¨uber zu machen, was wir beobachten werden und zu erfahren, wie wir die Radiodaten am besten mit Multiwellenl¨angendaten ergänzen. Das ist die Motivation meiner Doktorarbeit, in der ich eine Auswahl von 900 Radioquellen untersucht habe, die in einer der tiefsten jemals durchgef¨uhrten Radiodurchmusterungen detektiert wurden. Die Beobachtungen wurden bei 1.4GHz mit dem Very Large Array auf dem ”Extended Chandra Deep Field South“durchgeführt. Ich habe eine Multiwellenl¨angenmethode entwickelt, um die optischen und infraroten Pendants dieser Radioquellen zu identifizieren und sie als radiolaute (”radio loud“, RL) aktive galaktische Kerne (”active galactic nuclei“, AGNs), radioleise (”radio quiet“, RQ) AGNs und Galaxien mit aktiver Sternentstehung (”star forming galaxies“,SFGs) zu klassifizieren. Als erste war es mir möglich, die jeweiligen Anteile dieser verschiedenen Klassen an Quellen bis zu einer Flussdichte von nur ∼30 μJy zu bestimmen. Ich charakterisierte die Galaxieneigenschaften (Sternmasse, optische Farben, Morphologie) der Radioquellen; RQ AGN Galaxien und SFGs sind ¨ahnlich bezüglich der Scheibenmorphologie und der blauen Farben, w¨ahrend RL AGN Galaxien massiver, röter und meist elliptisch sind. Dies legt nahe, dass RQ und RL Aktivität auf zwei verschiedenen Entwicklungsstufen der BH − Galaxien Koevolution stattfindet. Die RQ Phase findet früher statt, wenn die Galaxie noch gasreich ist und aktiv Sterne bildet, während BHs erst als Radioquelle aktiv werden, wenn die Galaxie bereits den Groteil ihrer Sternpopulation gebildet hat, der Gasvorrat gesunken ist und die SF erheblich zurückgegangen ist. Ich quantifizierte die Sternentstehungsrate (”star formation rate“, SFR) der Radioquellen durch zwei unabh¨angige Indikatoren, die Radio- und die Ferninfrarotleuchtkraft. Ich habe Belege gefunden, dass der Hauptanteil der Radioemission von RQ AGNs durch die SF Aktivität der Galaxie entsteht. Dieses Ergebnis eröffnet die bemerkenswerte Möglichkeit, den Radiobereich des Spektrums zu benutzen um die SFR auch in Galaxien mit hellen,RQ AGNs abzuschätzen, bei denen die optische bis mittlere Infrarot Emission vom AGN dominiert sein kann. Ich habe gezeigt, dass tiefe Radiodurchmusterungen benutzt werden können um die kosmische Sternentstehungsgeschichte zu erforschen; Ich habe den Anteil des sogenannten ”Starburst“-Modus an der gesamten SFR-Dichte abgeschätzt und das Vorkommen von AGNs in Galaxien mit verschiedenem Grad an SF quantifiziert.
Samji, Isaac Chandra Annie Shalom [Verfasser]. "Intelligent Freeform Deformation for LED Illumination Optics / Annie Shalom Samji Isaac Chandra". Karlsruhe : KIT Scientific Publishing, 2018. http://www.ksp.kit.edu.
Texto completo da fonteHunziker, Markus. "Harish-Chandra systems on a reductive Lie algebra and the Zuckerman functor /". Diss., Connect to a 24 p. preview or request complete full text in PDF format. Access restricted to UC campuses, 1997. http://wwwlib.umi.com/cr/ucsd/fullcit?p9804516.
Texto completo da fonteHuenemoerder, David P., K. G. Gayley, Wolf-Rainer Hamann, Richard Ignace, J. S. Nichols, Lidia M. Oskinova, A. M. T. Pollock, Nobert S. Schulz e Tomer Shenar. "Probing Wolf–Rayet Winds: Chandra/HETG X-Ray Spectra of WR 6". Digital Commons @ East Tennessee State University, 2015. https://dc.etsu.edu/etsu-works/2692.
Texto completo da fonteRoy, Chowdhury Arpita. "Saratchandrer upanyaser bhashashilpo শরৎচন্দ্রের উপন্যাসের ভাষাশিল্প". Thesis, University of North Bengal, 2012. http://hdl.handle.net/123456789/1671.
Texto completo da fonteJoshi, Chandra P. [Verfasser]. "Kinetics and mechanism of the photocycle of photoactive yellow protein / Chandra P. Joshi". Berlin : Freie Universität Berlin, 2008. http://d-nb.info/1023049279/34.
Texto completo da fonteBernhardt, Karen 1977. "The generalized Harish-Chandra homomorphism for Hecke algebras of real reductive Lie groups". Thesis, Massachusetts Institute of Technology, 2005. http://hdl.handle.net/1721.1/28922.
Texto completo da fonteIncludes bibliographical references (p. 73-74).
For complex reductive Lie algebras g, the classical Harish-Chandra homomorphism allows to link irreducible finite dimensional representations of g to those of certain subalgebras l. The Casselman-Osborne theorem establishes an extension of this link to infinite dimensional irreducible representations. In this paper we present a generalized Harish-Chandra homomorphism construction for Hecke algebras, and establish the corresponding generalized Casselman-Osborne theorem. This homomorphism can be used to link representations of (g, L n K)-pairs to those of (g, L n K)-pairs, where is a certain subalgebra of g as in the classical case. Since representations of such pairs are closely related to those of the underlying Lie group G, this construction is a good first approximation to lifting the Harish-Chandra homomorphism from the Lie algebra to the Lie group level.
by Karen Bernhardt.
S.M.
Ai, Yanli, Liming Dou, Xiaohui Fan, Feige Wang, Xue-Bing Wu e Fuyan Bian. "EXPLORATORY CHANDRA OBSERVATION OF THE ULTRALUMINOUS QUASAR SDSS J010013.02+280225.8 AT REDSHIFT 6.30". IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621217.
Texto completo da fonteMarchesi, Stefano <1988>. "Black Hole and Galaxy Growth over Cosmic Time: the Chandra COSMOS Legacy Survey". Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amsdottorato.unibo.it/7240/1/marchesi_stefano_tesi.pdf.
Texto completo da fonteMarchesi, Stefano <1988>. "Black Hole and Galaxy Growth over Cosmic Time: the Chandra COSMOS Legacy Survey". Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amsdottorato.unibo.it/7240/.
Texto completo da fonteSaha, Dipak. "Uponyasik Ramesh Chandra Sen samaj bhabna o shilposiddhi উপন্যাসিক রমেশ চন্দ্র সেন : সমাজ ভাবনা ও শিল্পসিদ্ধি". Thesis, University of North Bengal, 2006. http://hdl.handle.net/123456789/2127.
Texto completo da fonteBulbul, Gul Esra. "Rxte And Chandra Observations Of Galctic Microquasars Grs 1915+105 And Gro J1655-40". Master's thesis, METU, 2006. http://etd.lib.metu.edu.tr/upload/12607392/index.pdf.
Texto completo da fontePammi, Sathish Chandra [Verfasser], e Hans [Akademischer Betreuer] Uszkoreit. "Synthesis of listener vocalizations : towards interactive speech synthesis / Sathish Chandra Pammi. Betreuer: Hans Uszkoreit". Saarbrücken : Saarländische Universitäts- und Landesbibliothek, 2012. http://d-nb.info/1051586569/34.
Texto completo da fonteLaird, Elise Sarah. "Chandra observations of ultra-violet selected star forming galaxies at redshift one and three". Thesis, Imperial College London, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.428592.
Texto completo da fonteGarnica-Vigil, Eugenio. "On the classification of tempered representations for a group in the Harish-Chandra class". Thesis, Massachusetts Institute of Technology, 1992. http://hdl.handle.net/1721.1/13244.
Texto completo da fonteTalluri, Bharath Chandra [Verfasser]. "Mechanistic and neural basis of choice-induced biases in decision-making / Bharath Chandra Talluri". Hamburg : Staats- und Universitätsbibliothek Hamburg Carl von Ossietzky, 2020. http://d-nb.info/1232407801/34.
Texto completo da fonteColzani, Alice. "Analisi di osservazioni Chandra dell'ammasso PLCK G287.0+32.9: connessione tra proprietà termiche e non termiche". Master's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/17080/.
Texto completo da fonteBernon, Florent. "Propriétés de l'intégrale de Cauchy Harish-Chandra pour les paires duales d'algèbres de Lie réductives". Poitiers, 2001. http://www.theses.fr/2001POIT2298.
Texto completo da fonte