Relevant bibliographies by topics / Galaxies : à haute redshift

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Galaxies : à haute redshift'

Author: Grafiati
Published: 23 September 2022
Last updated: 31 July 2025

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Journal articles on the topic "Galaxies : à haute redshift"

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Mickaelian, A. M., S. K. Balayan, and S. A. Hakopian. "The Byurakan-IRAS Galaxy (BIG) Sample: The Redshift Survey." International Astronomical Union Colloquium 184 (2002): 217–19. http://dx.doi.org/10.1017/s0252921100030724.

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AbstractThe Byurakan-IRAS Galaxy (BIG) sample (1967 galaxies) is based on optical identifications of IRAS PSC sources at δ>+61° and |b| >15° (FBS area). A redshift survey for brighter objects (B<18m) is being carried out with the Byurakan Observatory 2.6m, Special Observatory 6m, and Observatoire de Haute-Provence 1.93m telescopes. 213 objects have been observed, and redshifts in the range 0.008-0.173 have been measured. For this subsample, 15% of the objects are AGNs, and 15% are LIGs and ULIGs.
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Mickaelian, A. M. "Investigation of the Local Universe by Means of IRAS Galaxies." Symposium - International Astronomical Union 204 (2001): 69. http://dx.doi.org/10.1017/s0074180900225904.

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The Byurakan-IRAS galaxy (BIG) sample is based on optical identifications of IRAS PSC sources (Beichman, C. A. et al., eds. 1988, Infrared Astronomical Satellite (IRAS) Catalogs and Atlases: The Point Source Catalog, NASA RP–1190, Washington, DC). It makes use of the IR colours, DSS images, and the First Byurakan Spectral Survey (Markarian, B. E. et al. 1989, Commun. Special Astrophys. Obs., 62, 5).All IRAS sources in the region +61° < δ < 90° at high galactic latitudes (|b| >15°) in an area of 1487 deg2 have been revealed up to the limit of the IRAS survey. The BIG sample (Mickaelian
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Mickaelian, Areg M. "Galaxy Evolution Traced by Multiple Galaxies from the BIG Sample." Proceedings of the International Astronomical Union 2, S235 (2006): 225. http://dx.doi.org/10.1017/s1743921306006314.

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AbstractOptical identifications of all IRAS PSC sources at high galactic latitudes by means of the First Byurakan Survey (FBS) in the area with +61° < δ < +90° at galactic latitudes |b|>15° have been carried out with a total surface of 1487 deg2. 1577 sources have been optically identified, 1178 sources corresponding to galaxies. The BIG sample (Byurakan-IRAS Galaxies) was constructed of 1178 newly identified galaxies and 789 other IRAS galaxies in the same area, known before, altogether 1967 galaxies. Studies of the BIG objects include: spectroscopic follow-up for the brighter (<1
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Barger, Amy. "High-Redshift Galaxies." Symposium - International Astronomical Union 216 (2005): 309–24. http://dx.doi.org/10.1017/s0074180900196743.

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Mapping the history of star formation requires combining observations at many wavelengths. The most dramatic episodes of star formation occurred in high-redshift (z > 1) galaxies obscured by dust. These galaxies can be seen at submillimeter wavelengths. While these episodes clearly constitute much of the star formation in the universe, we still do not know the redshift distribution. Although progess has been made in determining the nature of the brightest members of the submillimeter population, these galaxies comprise only a tiny fraction of the submillimeter extragalactic background light
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Bian, Fuyan, Lisa J. Kewley, Brent Groves, and Michael A. Dopita. "What drives the redshift evolution of strong emission line ratios?" Monthly Notices of the Royal Astronomical Society 493, no. 1 (2020): 580–85. http://dx.doi.org/10.1093/mnras/staa259.

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ABSTRACT We study the physical mechanisms that cause the offset between low-redshift and high-redshift galaxies on the [O iii] λ5007/H β versus [N ii] λ6584/H α ‘Baldwin, Phillips & Terlevich’ (BPT) diagram using a sample of local analogues of high-redshift galaxies. These high-redshift analogue galaxies are selected from the Sloan Digital Sky Survey. Located in the same region on the BPT diagram as the ultraviolet selected galaxies at z ∼ 2, these high-redshift analogue galaxies provide an ideal local benchmark to study the offset between the local and high-redshift galaxies on the BPT di
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Li, I. H., H. K. C. Yee, B. C. Hsieh, D. G. Gilbank, and M. D. Gladders. "The Evolution of Galaxies and Groups in Cluster Environments at 0.3 < z < 0.6." Proceedings of the International Astronomical Union 2, S235 (2006): 220. http://dx.doi.org/10.1017/s1743921306006260.

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We investigate the dependence of galaxy populations on environment. Our samples are selected from the follow-up of Red-Sequence Cluster Survey (RCS) catalogs using wide-field BVRz' imaging for 60 intermediate redshift (0.3 &lt; z &lt; 0.6) clusters. Galaxy redshifts are estimated using an empirical photometric redshift technique with a training set of 3996 galaxies to z 1.4. To obtain photometric redshift probability density for each galaxy, we bootstrap the training set galaxies to estimate the fitting uncertainties and apply Monte-Carlo method to simulate galaxy magnitudes errors. In order t
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Mahdi, Hareth Saad. "The Bimodal Color Distribution of Galaxies at Redshift of z=0-0.15 from the Sloan Digital Sky Survey (SDSS)." Al-Mustansiriyah Journal of Science 30, no. 2 (2019): 52. http://dx.doi.org/10.23851/mjs.v30i2.574.

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This work aims to use the color distribution of galaxies to differentiate between blue and red galaxies. The photometric data of 300000 galaxies at redshift of z = 0 – 0.15 were collected from the Sloan Digital Sky Survey (SDSS). Three redshift ranges were considered for the purpose of this work: 100000 galaxies at z = 0-0.05, 100000 galaxies at z = 0.05-0.1 and 100000 galaxies at z = 0.1-0.15. The color distributions for all redshift ranges were determined. The results have clearly shown that the color distributions for all redshift ranges are bimodal. One of the two peaks corresponds to the
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Jaskot, Anne, and Sally Oey. "The Green Peas: Searching for LyC Emitters at Low Redshift." Proceedings of the International Astronomical Union 11, S319 (2015): 126. http://dx.doi.org/10.1017/s1743921315010054.

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AbstractThe escape fraction of Lyman continuum (LyC) radiation from galaxies remains one of the primary uncertainties in studies of reionization. However, few LyC-emitting galaxies are known. The recently identified, low-redshift “Green Pea” (GP) galaxies exhibit a number of similarities with high-redshift galaxies, and their optical emission lines suggest they may be some of the elusive LyC emitters. Recent HST COS and ACS observations of four GPs suggest further evidence for LyC escape and give new insights into the origins of Lyα and low-ionization UV lines in high-redshift galaxies. The Ly
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Bian, Fuyan, Lisa J. Kewley, Brent Groves, and Michael A. Dopita. "Local analogs of high-redshift galaxies: Metallicity calibrations at high-redshift." Proceedings of the International Astronomical Union 15, S352 (2019): 309–13. http://dx.doi.org/10.1017/s1743921320000800.

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AbstractWe study the metallicity calibrations in high-redshift galaxies using a sample of local analogs of high-redshift galaxies selected from the SDSS survey. Located in the same region on the BPT diagram as star-forming galaxies at z ∼ 2, these high-redshift analogs share the same ionized ISM conditions as high-redshift galaxies. We establish empirical metallicity calibrations between the direct gas-phase oxygen abundances and varieties of metallicity indicators in our local analogs using direct Te method. These new metallicity calibrations are the best means to measure the metallicity in h
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Yuan, Qi-Rong, Qiang-Qiang Dang, Peng-Fei Yan, et al. "Correlation of morphological fraction with redshift in galaxy clusters." Proceedings of the International Astronomical Union 10, H16 (2012): 136. http://dx.doi.org/10.1017/s1743921314004979.

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AbstractBased on 187 galaxy clusters identified from the photometric redshifts of galaxies in the Cosmic Evolution Survey (COSMOS) field(Wen &amp; Han 2011), cluster galaxies brighter than MV = -20.5 are classified into four categories according to their best-fitting templates of the spectral energy distributions (SEDs) provided by Ilbert et al. (2009): early-type (including elliptical and lenticular) galaxies (E+S0), spiral galaxies (S), irregular galaxies (Irr), and starbursts (SB). The fractions of these four SED types are presented as the functions of redshift in Figure 1. Fraction of each
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Dissertations / Theses on the topic "Galaxies : à haute redshift"

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Pham, Tuan Anh. "Observations millimétriques-submillimétriques de galaxies lentillées gravitationellement à haut redshift." Toulouse 3, 2014. http://thesesups.ups-tlse.fr/2709/.

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Nous présentons une étude détaillée d'observations faites de la galaxie hôte d'un quasar lointain (z~2. 8), RX J0911. La détection de l'émission des molécules CO a été possible grâce au lentillage gravitationnel dû à la présence d'une galaxie plus proche sur la ligne de vue et à la qualité de l'interféromètre du Plateau de Bure. On a obtenu de très bonnes résolutions tant en fréquence, permettant une mesure précise de la largeur de raie, qu'en direction, permettant de résoudre la source aussi bien sur la raie que dans le continu, donc à la fois pour le gaz et pour la poussière. Nous avons disc
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Zanella, Anita. "Structural properties of clumpy galaxies and spheroids at high redshift." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC314/document.

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Cette thèse explore la question ouverte des mécanismes selon lesquels les galaxies lointaines évoluent au cours du temps. Elle se concentre sur l’étude des galaxies irrégulières et sur la cause de l’évolution en taille des galaxies passives et compactes. Bien que des régions de formation stellaire très lumineuses (clumps) soient observées dans les galaxies irrégulières depuis longtemps, leur nature et évolution sont encore débattues. Les instabilités gravitationnelles des disques ont été proposées comme la cause principale pour la formation in-situ des clumps, même si certains d’entre eux pour
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Salmi, Fadia. "Comprendre les modes de formation d’étoiles dans l’univers lointain." Thesis, Paris 11, 2012. http://www.theses.fr/2012PA112173/document.

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L'objectif de mon travail de thèse a consisté à tenter de comprendre quels sont les mécanismes principaux à l'origine de la formation d'étoiles dans les galaxies au cours des derniers dix milliards d'années. Alors qu'il avait été proposé dans le passé que le rôle des fusions de galaxies était dominant pour expliquer l'allumage de la formation d'étoiles dans les galaxies lointaines formant leurs étoiles à de très grands taux, des études plus récentes ont au contraire mis en évidence des lois d'échelles reliant le taux de formation d'étoiles des galaxies à leur masse stellaire ou masse de gaz. L
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Bieri, Rebekka. "The Role of AGN Feedback in Galaxy Formation." Thesis, Paris 6, 2016. http://www.theses.fr/2016PA066292/document.

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L’objectif de ma thèse porte sur les interactions entre les noyaux actifs de galaxies et le milieu interstellaire des galaxies. En particulier, je mets l’accent sur les deux mécanismes possibles responsables de la production des vents par les trous noirs : les jets et les vents produits par le rayonnement de ces trous noirs. Les simulations hydrodynamiques de haute résolution des galaxies comprenant la rétroac- tion d’un jet ont montré que l’activité des noyaux actifs peut conduire à une pression exces- sive sur les régions denses de formation stellaire dans les galaxies, et donc à au
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Villa, Vélez Jorge Andrés. "Spectrophotometric analysis around cosmic noon : emission-lines, dust attenuation, and star formation." Thesis, Aix-Marseille, 2021. http://www.theses.fr/2021AIXM0440.

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Les galaxies sont les éléments constitutifs de l'Univers. La compréhension de leur rôle dans le cosmos se fait grâce à l’étude de la lumière qu’elles émettent d'un point de vue multi-longueur d'onde car les processus physiques en leur sein sont responsables du rayonnement que nous observons. Dans ce travail, un échantillon de galaxies dans le champ COSMOS avec une photométrie de l'ultraviolet à l'infrarouge lointain et des flux Ha, Hb, [OIII]5007 est étudié à l'aide du logiciel CIGALE. La photométrie est ajustée avec les flux Ha pour obtenir des estimations robustes de la masse stellaire, du t
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Roos, Orianne. "Modelling feedback processes, star formation and outflows in high-redshift galaxies." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC148/document.

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Dans l’Univers, on observe des galaxies lointaines ne formant plus d’étoiles, mais les astrophysiciens n’ont pas encore identifié avec certitude les phénomènes physiques à l’origine de leur “mort”. Pour apporter des éléments de réponse, je me suis penchée sur l’étude de phénomènes qui pourraient y jouer un rôle : les processus de rétroaction des étoiles et des trous noirs supermassifs actifs, la formation stellaire, et les vents galactiques. Le Chapitre 1 présente toutes les notions nécessaires à la compréhension du problème : les caractéristiques des galaxies typiques de l’Univers proche et l
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Yang, Chentao. "Physical conditions of the interstellar medium in high-redshift submillimetre bright galaxies." Thesis, Université Paris-Saclay (ComUE), 2017. http://www.theses.fr/2017SACLS361/document.

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La découverte d'une population de galaxies submillimétrique (SMG) obscurcies par la poussière à grand décalage spectral, à l'aide de caméras submm, a révolutionné notre connaissance de l'évolution des galaxies et de la formation stellaire dans les conditions physiques extrêmes. Elles sont les flambées de formation stellaire les plus intenses dans l'Univers, approchant la limite d'Eddington et sont considérées comme les progéniteurs des galaxies actuelles les plus massives. Les modèles théoriques d'évolution de galaxies ont été remis en question par la découverte d'un grand nombre de SMGs à gra
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Fensch, Jérémy. "Star and stellar cluster formation in gas-dominated galaxies." Thesis, Sorbonne Paris Cité, 2017. http://www.theses.fr/2017USPCC207/document.

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Nous étudions la formation d’étoiles et d’amas d’étoiles dans les galaxies dominées par le gaz. Ce terme réfère en premier lieu aux galaxies de l’époque du pic de formation d’étoiles dans l’histoire de l’Univers, qui s’est déroulé vers z ~ 2, mais aussi à leurs analogues locaux, les galaxies naines de marées. En premier lieu, en utilisant des simulations numériques, nous montrons que les galaxies massives typiques de z=2, avec une fraction de gaz d’environ 50%, forment des structures gazeuses massives (10**7-8 masses solaires) et liées gravitationnellement, appelées grumeaux dans la suite. Ces
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Ribeiro, Bruno. "Morphology as a tracer of evolution in the early phases of galaxy assembly." Thesis, Aix-Marseille, 2016. http://www.theses.fr/2016AIXM4744/document.

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Les propriétés globales des galaxies montrent une forte évolution du taux de formation stellaire et de la densité de masse stellaire à l'époque de l'assemblage des galaxies précédent le pic de formation stellaire dans l'univers, produite par plusieurs processus physiques concurrents (fusion, accrétion, rétroaction, environnement, ...). Les propriétés morphologiques des galaxies ont aussi fortement évolué à la même époque. Dans cette thèse, j'étudie comment l'évolution des propriétés morphologique est reliée aux propriétés spectrophotométriques des galaxies depuis z ~ 6. Les données spectroscop
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Collet, Cédric. "Role of AGN feedback in galaxy evolution at high-redshift." Phd thesis, Université Paris Sud - Paris XI, 2014. http://tel.archives-ouvertes.fr/tel-01061155.

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There is growing evidence that supermassive black holes may play a crucial role for galaxy evolution, in particular during the formation of massive galaxies at high redshift (z ~ 2 - 3). Our work focuses on quantifying the effects of jets of radiogalaxies and of large bolometric luminosities of quasars on the interstellar gas in their host galaxies. To this end, we studied the kinematics of the ionized gas in 12 moderately powerful radio galaxies and 11 quasars (6 radio-loud and 5 radio-quiet) at high redshifts with rest-frame optical imaging spectroscopy obtained at the VLT with SINFONI. We s
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Books on the topic "Galaxies : à haute redshift"

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Appenzeller, Immo. High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2.

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IAP Workshop (3rd 1987 Paris, France). High redshift and primeval galaxies. Editions Frontières, 1987.

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Kron, Richard G., and Alvio Renzini, eds. Towards Understanding Galaxies at Large Redshift. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2919-7.

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G, Kron Richard, and United States. National Aeronautics and Space Administration., eds. A deep redshift survey of field galaxies. Space Telescope Science Institute, 1987.

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Arp, Halton C. Catalogue of discordant redshift associations. Apeiron, 2003.

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Ellis, Simon Charles. The evolution of high redshift clusters of galaxies. University of Birmingham, 2003.

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Bender, Ralf, and Alvio Renzini, eds. The Mass of Galaxies at Low and High Redshift. Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/b10204.

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Matthias, Steinmetz, and Rauch Michael, eds. Damped Lygas absorbers at high redshift - large disks or galactic building blocks? National Aeronautics and Space Administration, 1998.

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T, Stocke John, Penton Steve, and United States. National Aeronautics and Space Administration., eds. Intergalactic hydrogen clouds at low redshift: Connections to voids and dwarf galaxies. National Aeronautics and Space Administration, 1996.

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Law-Green, John Duncan Bradburn. The distant DRAGNS survey: A radio imaging survey of radio galaxies at high redshift. University of Manchester, 1996.

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Book chapters on the topic "Galaxies : à haute redshift"

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Bahcall, Neta A. "High-Redshift Galaxies." In Highlights of Astronomy. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2828-5_17.

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Chincarini, Guido, and Paolo Saracco. "High Redshift Galaxies." In Generation of Cosmological Large-Scale Structure. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-009-0053-0_1.

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Appenzeller, Immo. "Introduction." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_1.

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Appenzeller, Immo. "Implications." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_10.

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Appenzeller, Immo. "Ongoing Work." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_11.

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Appenzeller, Immo. "Future Facilities and their Opportunities." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_12.

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Appenzeller, Immo. "The Nearby Universe." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_2.

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Appenzeller, Immo. "The Past and the Future." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_3.

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Appenzeller, Immo. "Basic Techniques and their Limitations." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_4.

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Appenzeller, Immo. "Finding Very Distant Galaxies." In High-Redshift Galaxies. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-75824-2_5.

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Conference papers on the topic "Galaxies : à haute redshift"

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van Breugel, Willem J. "Highest redshift radio galaxies." In Astronomical Telescopes and Instrumentation, edited by Jacqueline Bergeron. SPIE, 2000. http://dx.doi.org/10.1117/12.390129.

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Fosbury, Robert A. E. "High redshift radio galaxies." In Astronomical Telescopes and Instrumentation, edited by Jacqueline Bergeron. SPIE, 2000. http://dx.doi.org/10.1117/12.390128.

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Woodgate, Bruce E., Paul J. Francis, and Anthony C. Danks. "High redshift galaxies already old?" In The ultraviolet universe at low and high redshift. AIP, 1997. http://dx.doi.org/10.1063/1.53801.

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Strazzullo, V., P. Rosati, C. Lidman, et al. "Cluster galaxies at redshift 1.4." In PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3141528.

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Heckman, Timothy M. "Starburst galaxies: implications at high-redshift." In AFTER THE DARK AGES. ASCE, 1999. http://dx.doi.org/10.1063/1.58617.

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Merrifield, Michael R. "A low redshift perspective on galaxies." In INTERNATIONAL CONFERENCE ON CONDENSED MATTER AND APPLIED PHYSICS (ICC 2015): Proceeding of International Conference on Condensed Matter and Applied Physics. Author(s), 2016. http://dx.doi.org/10.1063/1.4948804.

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ALEXANDER, D. M. "WHAT POWERS HIGH-REDSHIFT SCUBA GALAXIES?" In Proceedings of the Guillermo Haro Conference 2003. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702432_0033.

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Calzetti, Daniela. "UV opacity in nearby galaxies and application to distant galaxies." In The ultraviolet universe at low and high redshift. AIP, 1997. http://dx.doi.org/10.1063/1.53764.

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Gordon, Karl D., Daniela Calzetti, and Adolf N. Witt. "Dust in starburst galaxies." In The ultraviolet universe at low and high redshift. AIP, 1997. http://dx.doi.org/10.1063/1.53805.

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Gardner, Jonathan P., Sara R. Heap, Eliot M. Malumuth, Robert S. Hill, and Eric P. Smith. "Morphological evolution of galaxies." In The ultraviolet universe at low and high redshift. AIP, 1997. http://dx.doi.org/10.1063/1.53808.

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Reports on the topic "Galaxies : à haute redshift"

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Избрехт, А. Р. COSMOLOGICAL REDSHIFT OF GALAXIES’ SPECTRA. DOI СODE, 2015. http://dx.doi.org/10.18411/doicode-2023.162.

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Miley, G., C. Carilli, G. B. Taylor, C. de Breuck, and A. Cohen. High Redshift Radio Galaxies: Laboratories for Massive Galaxy and Cluster Formation in the Early Universe. Defense Technical Information Center, 2010. http://dx.doi.org/10.21236/ada520904.

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