Relevant bibliographies by topics / Galaxy: general

Contents

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

Academic literature on the topic 'Galaxy: general'

Author: Grafiati
Published: 4 June 2021
Last updated: 26 July 2025

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Journal articles on the topic "Galaxy: general"

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Wang, Qingqing, Xin Ren, Bo Wang, Yi-Fu Cai, Wentao Luo, and Emmanuel N. Saridakis. "Galaxy–Galaxy Lensing Data: f(T) Gravity Challenges General Relativity." Astrophysical Journal 969, no. 2 (2024): 119. http://dx.doi.org/10.3847/1538-4357/ad47c0.

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Abstract We use galaxy–galaxy lensing data to test general relativity and f(T) gravity at galaxy scales. We consider an exact spherically symmetric solution of f(T) theory, which is obtained from an approximate quadratic correction, and thus it is expected to hold for every realistic deviation from general relativity. Quantifying the deviation by a single parameter Q, and following the post-Newtonian approximation, we obtain the corresponding deviation in the gravitational potential, shear component, and effective excess surface density profile. We used five stellar mass samples and divided th
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Martínez-González, E., and J. L. Sanz. "The General Galaxy Luminosity Function." Symposium - International Astronomical Union 130 (1988): 582. http://dx.doi.org/10.1017/s007418090013709x.

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The general luminosity function of galaxies is believed to be well represented by the Schechter function with exponent α ≃ −1 and L* ≃ 1010L⊙, but with a wide range of variation from one sample to another. This function decreases exponentially at high luminosities and has a power law behaviour increasing towards low luminosities with no present evidence of turn over or cut-off.
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Grimm, Nastassia, Fulvio Scaccabarozzi, Jaiyul Yoo, Sang Gyu Biern, and Jinn-Ouk Gong. "Galaxy power spectrum in general relativity." Journal of Cosmology and Astroparticle Physics 2020, no. 11 (2020): 064. http://dx.doi.org/10.1088/1475-7516/2020/11/064.

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Smith, Keith T. "Testing General Relativity on galaxy scales." Science 360, no. 6395 (2018): 1310.8–1311. http://dx.doi.org/10.1126/science.360.6395.1310-h.

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Yoo, Jaiyul. "Incompatibility of standard galaxy bias models in general relativity." Journal of Cosmology and Astroparticle Physics 2023, no. 10 (2023): 054. http://dx.doi.org/10.1088/1475-7516/2023/10/054.

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Abstract The standard model for galaxy bias is built in a Newtonian framework, and several attempts have been made in the past to put it in a relativistic framework. The focus of past works was, however, to use the same Newtonian formulation, but to provide its interpretation in a relativistic framework by either fixing a gauge condition or transforming to a local coordinate system. Here we demonstrate that these reverse-engineered approaches do not respect the diffeomorphism symmetry in general relativity, and we need to develop a covariant model of galaxy bias that is diffeomorphism compatib
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Andrianomena, Sambatra, Camille Bonvin, David Bacon, et al. "Testing general relativity with the Doppler magnification effect." Monthly Notices of the Royal Astronomical Society 488, no. 3 (2019): 3759–71. http://dx.doi.org/10.1093/mnras/stz1905.

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ABSTRACT The apparent sizes and brightnesses of galaxies are correlated in a dipolar pattern around matter overdensities in redshift space, appearing larger on their near side and smaller on their far side. The opposite effect occurs for galaxies around an underdense region. These patterns of apparent magnification induce dipole and higher multipole terms in the cross-correlation of galaxy number density fluctuations with galaxy size/brightness (which is sensitive to the convergence field). This provides a means of directly measuring peculiar velocity statistics at low and intermediate redshif
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Raccanelli, Alvise, Francesco Montanari, Daniele Bertacca, Olivier Doré, and Ruth Durrer. "Cosmological measurements with general relativistic galaxy correlations." Journal of Cosmology and Astroparticle Physics 2016, no. 05 (2016): 009. http://dx.doi.org/10.1088/1475-7516/2016/05/009.

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Anosova, J., S. Iyer, and R. K. Varma. "Clusters and Voids in General Galaxy Field." Symposium - International Astronomical Union 168 (1996): 523–24. http://dx.doi.org/10.1017/s0074180900110563.

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In our previous works (Anosova 1987, Anosova, Iyer, Varma 1994), we developed a new method for determination of the structure of a clustered distribution. In this work, we apply this method studying the observed distribution of galaxies in the Universe.
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Eyer, L. "Understanding the Galaxy." Proceedings of the International Astronomical Union 14, S339 (2017): 50–55. http://dx.doi.org/10.1017/s174392131800220x.

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AbstractThis general overview of our understanding of the Galaxy followed the lines of its main structures (halo, disc, bulge/bar) and emphasized some time-domain astronomy contributions. On the one hand the distance and tangential motions of the stars are essential to that understanding, and are obtained through multi-epoch surveys. On the other hand the chemistry of the stars and their radial velocities are also key elements for mapping the Galactic (sub-)structures, and unravelling their history and evolution. Contemporary surveys are revolutionizing our view of the Milky Way and of galaxie
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Zhdanov, V. I. "The General Relativistic Potential of Astrometric Studies at Microarcsecond Level." Symposium - International Astronomical Union 166 (1995): 295–300. http://dx.doi.org/10.1017/s0074180900228234.

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The relativistic effects in positioning of distant objects at microarcsecond level are studied. The main points are: statistics of random variations of the image position of a distant radiation source due to the gravitational field of moving stars, motion of the image due to individual invisible gravitators, and possibilities to obtain information on their masses and velocities. The gravitators shifting the object image may be stars of our Galaxy or of a lensing galaxy.
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Dissertations / Theses on the topic "Galaxy: general"

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Rosselli, Damiano. "Probing general relativity: new measures of gravitational redshifts in galaxy clusters." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2022. http://amslaurea.unibo.it/25349/.

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In this Thesis work we test the Einstein theory of General Relativity by measuring the gravitational redshift effect in galaxy clusters, within the ΛCDM cosmological framework. To perform the gravitational redshift measurements, we create two new cluster member galaxies by exploiting the galaxy coordinates and spectroscopic redshifts derived from the sixteenth data release of the Sloan Digital Sky Survey, and two cluster catalogs, namely the Wen-Han-Liu cluster catalog (WHL15) and the cluster catalog derived from the latest data release of the Dark Energy Survey Instrument (DESI). We accura
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Hood, Ross John. "Characterising the optical properties of galaxy clusters with GMPhoRCC." Thesis, University of Edinburgh, 2014. http://hdl.handle.net/1842/9638.

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The properties of galaxy clusters, such as abundance and mass to light ratios, have long been used to investigate and constrain cosmology. With vast numbers of newly detected clusters, such as from the Planck mission (Planck Collaboration et al., 2013), full determination of cluster properties, particularly mass, can be hugely expensive and time consuming. Optical characterisation o ers a cheap solution, using optical data alone to estimate cluster properties such as redshift. With the abundance of current optical data, such as from the Sloan Digital Sky Survey (SDSS), (Ahn et al., 2012) and u
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Rykoff, E. S., E. Rozo, D. Hollowood, et al. "THE REDMAPPER GALAXY CLUSTER CATALOG FROM DES SCIENCE VERIFICATION DATA." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621223.

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We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specifically designed for large photometric surveys. The updated algorithm is applied to 150 deg(2) of Science Verification (SV) data from the Dark Energy Survey (DES), and to the Sloan Digital Sky Survey (SDSS) DR8 photometric data set. The DES SV catalog is locally volume limited and contains 786 clusters with richness lambda > 20 (roughly equivalent to M500c greater than or similar to 10(14) h(70)(-1)M(circle dot)) and 0.2 < z < 0.9. The DR8 catalog consists of 26,311 clusters with 0.08 < z < 0.6, with
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Baxter, Eric, Chihway Chang, Bhuvnesh Jain, et al. "The Halo Boundary of Galaxy Clusters in the SDSS." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624484.

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Analytical models and simulations predict a rapid decline in the halo density profile associated with the transition from the "infalling" regime outside the halo to the "collapsed" regime within the halo. Using data from SDSS, we explore evidence for such a feature in the density profiles of galaxy clusters using several different approaches. We first estimate the steepening of the outer galaxy density profile around clusters, finding evidence for truncation of the halo profile. Next, we measure the galaxy density profile around clusters using two sets of galaxies selected on color. We find ev
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Farahi, Arya, August E. Evrard, Eduardo Rozo, Eli S. Rykoff, and Risa H. Wechsler. "Galaxy cluster mass estimation from stacked spectroscopic analysis." OXFORD UNIV PRESS, 2016. http://hdl.handle.net/10150/621426.

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We use simulated galaxy surveys to study: (i) how galaxy membership in redMaPPer clusters maps to the underlying halo population, and (ii) the accuracy of a mean dynamical cluster mass, M-sigma(lambda), derived from stacked pairwise spectroscopy of clusters with richness lambda. Using similar to 130 000 galaxy pairs patterned after the Sloan Digital Sky Survey (SDSS) redMaPPer cluster sample study of Rozo et al., we show that the pairwise velocity probability density function of central-satellite pairs with m(i) < 19 in the simulation matches the form seen in Rozo et al. Through joint membersh
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Zasowski, G., R. E. Cohen, S. D. Chojnowski, et al. "Target Selection for the SDSS-IV APOGEE-2 Survey." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626051.

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APOGEE-2 is a high-resolution, near-infrared spectroscopic survey observing similar to 3. x. 10(5) stars across the entire sky. It is the successor to APOGEE and is part of the Sloan Digital Sky Survey IV (SDSS-IV). APOGEE-2 is expanding on APOGEE's goals of addressing critical questions of stellar astrophysics, stellar populations, and Galactic chemodynamical evolution using (1) an enhanced set of target types and (2) a second spectrograph at Las Campanas Observatory in Chile. APOGEE-2 is targeting red giant branch and red clump stars, RR Lyrae, lowmass dwarf stars, young stellar objects, and
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Frusciante, Noemi. "Deviations from General Relativity in Cosmology and Astrophysics." Doctoral thesis, SISSA, 2014. http://hdl.handle.net/20.500.11767/3861.

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Two of the most prominent challenges of Modern Cosmology are the recent late-time accelerated expansion of the Universe and Dark Matter (DM). DM is of fundamental importance in the process of structure formation at galactic, extragalactic and cosmic scales. It seems to dominate down to small galactocentric radii, as highlighted by the galaxies rotation curves and on cosmic scale, it is well known that the spatial distribution of galaxies is biased with respect to the underlying DM distribution. This relation is called ``bias''. Part of this thesis is devoted to the investigation of the
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Rees, Bryan. "A study of planetary nebulae in and towards the Galactic Bulge." Thesis, University of Manchester, 2011. https://www.research.manchester.ac.uk/portal/en/theses/a-study-of-planetary-nebulae-in-and-towards-the-galactic-bulge(ff6c0373-e5a5-491f-b5fb-bda36acac8ba).html.

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A planetary nebula (PN) consists of material, mainly gas, that has been ejected from a star on the asymptotic giant branch of its life cycle. This material emits electromagnetic radiation due to photoionization and recombination, collisional and radiative excitation or free-free radiation. The envelope of material moves outwards from the central star and may take one of a variety of shapes. These shapes are believed to be sculpted by the stellar wind, magnetic fields and interactions with a binary companion. However, within a time scale of as little as 10 000 years the nebula fades from view a
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Hennig, C., J. J. Mohr, A. Zenteno, et al. "Galaxy Populations in Massive Galaxy Clusters to z = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/623801.

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We study the galaxy populations in 74 Sunyaev-Zeldovich effect selected clusters from the South Pole Telescope survey, which have been imaged in the science verification phase of the Dark Energy Survey. The sample extends up to z similar to 1.1 with 4 x 10(14)M(circle dot) <= M-200 <= 3 x 10(15)M(circle dot). Using the band containing the 4000 angstrom break and its redward neighbour, we study the colour-magnitude distributions of cluster galaxies to similar to m(*) + 2, finding that: (1) The intrinsic rest frame g - r colour width of the red sequence (RS) population is similar to 0.03 out to
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Dawson, William Anthony. "Constraining Dark Matter Through the Study of Merging Galaxy Clusters." Thesis, University of California, Davis, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3602041.

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<p> <b>Context:</b> The majority (~85%) of the matter in the universe is composed of dark matter, a mysterious particle that does not interact via the electromagnetic force yet does interact with all other matter via the gravitational force. Many direct detection experiments have been devoted to finding interactions of dark matter with baryonic matter via the weak force. It is still possible that dark matter interacts with itself via a strong scale force and has a self-scattering cross-section of ~0.5 cm<sup>2</sup>g<sup> -1</sup>. In fact such a strong scale scattering force could resolve s
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Books on the topic "Galaxy: general"

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Kaplan, Dean. Samsung Galaxy Tab Application Sketch Book. Apress, 2011.

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Carnell, John. The hitchhiker's guide to the galaxy. DC Comics, 1993.

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Antillean Galaxy. Caribbean Lion Publishing, 2023.

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Dean. Fiberglass Galaxy. DeAngelo, Brooke, 2019.

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Galaxy Unstable (Forgotten Galaxy, Book Two). Quirky Algorithms, 2024.

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Galaxy Undone (Forgotten Galaxy, Book Four). Quirky Algorithms, 2024.

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Galaxy Unknown (Forgotten Galaxy, Book One). Quirky Algorithms, 2024.

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Publishing, Love Planet. Savage Galaxy Rescue. Love Planet Publishing, 2022.

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Publishing, Love Planet. Savage Galaxy Rescue. Love Planet Publishing, 2022.

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Lord, Karen. Galaxy Game. Quercus, 2016.

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Book chapters on the topic "Galaxy: general"

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Barrow, John D. "General Discussion: Galaxy Clustering." In Statistical Challenges in Modern Astronomy. Springer New York, 1992. http://dx.doi.org/10.1007/978-1-4613-9290-3_18.

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Martínez-González, E., and J. L. Sanz. "The General Galaxy Luminosity Function." In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_134.

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Anosova, J., S. Iyer, and R. K. Varma. "Clusters and Voids in General Galaxy Field." In Examining the Big Bang and Diffuse Background Radiations. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0145-2_68.

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Høg, Erik. "General Discussion and Photometric System for GAIA." In Census of the Galaxy: Challenges for Photometry and Spectrometry with GAIA. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0361-2_28.

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Gupta, S. "“Multiple Bending of Light Ray” Can Create Many Images for One Galaxy: In Our Dynamic Universe — A Computer Simulation." In Recent Developments in General Relativity, Genoa 2000. Springer Milan, 2002. http://dx.doi.org/10.1007/978-88-470-2101-3_31.

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Jacquart, Melissa, and Regy-Null R. Arcadia. "Idealizations in Astrophysical Computer Simulations." In Synthese Library. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-26618-8_8.

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AbstractThis chapter examines some of the philosophical literature on idealizations in science and the epistemic challenges idealizations potentially pose for astrophysical methodology, particularly its use of computer simulations. We begin by surveying philosophical literature on idealization connected to (1) kinds of idealizations deployed in science, (2) the aims of idealization in science, and (3) various strategies for de-idealization. Using collisional ring galaxy simulations as a case study, we examine how these three themes play out in the context of astrophysical computer simulations.
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Saslaw, William C. "Galaxy distribution functions." In The Renaissance of General Relativity and Cosmology. Cambridge University Press, 1993. http://dx.doi.org/10.1017/cbo9780511622724.009.

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Jones, Bernard J. T. "Nonlinear galaxy clustering." In The Renaissance of General Relativity and Cosmology. Cambridge University Press, 1993. http://dx.doi.org/10.1017/cbo9780511622724.010.

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"Motion of the Stars in the Galaxy." In General Relativistic Dynamics. WORLD SCIENTIFIC, 2009. http://dx.doi.org/10.1142/9789814271172_0009.

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Weinberg, Steven. "General Theory of Small Fluctuations." In Cosmology. Oxford University PressOxford, 2008. http://dx.doi.org/10.1093/oso/9780198526827.003.0005.

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Abstract In most of the work described in the previous chapters, the universe has been treated as isotropic and homogeneous, with a gravitational field described by the Robertson–Walker metric. This is of course just an approximation, which ignores many of the most interesting things in the universe: galaxy clusters, galaxies, stars, us. We now turn to an analysis of these departures from homogeneity and isotropy.
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Conference papers on the topic "Galaxy: general"

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STARLING, RHAANA, RALPH WIJERS, and KLAAS WIERSEMA. "GAMMA-RAY BURST HOST GALAXY GAS AND DUST." In Proceedings of the MG11 Meeting on General Relativity. World Scientific Publishing Company, 2008. http://dx.doi.org/10.1142/9789812834300_0310.

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Schiavi, Riccardo, Roberto Capuzzo-Dolcetta, and Manuel Arca-Sedda. "The future Milky Way and Andromeda galaxy merger." In Proceedings of the MG15 Meeting on General Relativity. WORLD SCIENTIFIC, 2022. http://dx.doi.org/10.1142/9789811258251_0243.

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Hartnett, John G. "Spiral galaxy rotation curves described using cosmological general relativity." In FRONTIERS OF FUNDAMENTAL PHYSICS: Eighth International Symposium FFP8. AIP, 2007. http://dx.doi.org/10.1063/1.2736981.

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Battistelli, Elia S., Carlo Burigana, Paolo de Bernardis, et al. "Galaxy clusters as probes for cosmology and dark matter." In Proceedings of the MG14 Meeting on General Relativity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813226609_0032.

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Donnari, Martina, Marco Merafina, and Manuel Arca-Sedda. "The local effect of Dark Energy in galaxy clusters." In Proceedings of the MG14 Meeting on General Relativity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813226609_0251.

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ROSHAN, MAHMOOD. "VIRIAL MASSES OF GALAXY CLUSTERS IN THE POST-NEWTONIAN LIMIT." In Proceedings of the MG13 Meeting on General Relativity. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814623995_0056.

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Rieser, Hans-Martin, Björn M. Schäfer, and Frederic P. Schuller. "Area metric gravity: Confrontation with observations of galaxy rotation curves." In Proceedings of the MG15 Meeting on General Relativity. WORLD SCIENTIFIC, 2022. http://dx.doi.org/10.1142/9789811258251_0090.

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Carvalho, Ana, Alberto Krone-Martins, and Antonio da Silva. "Unsupervised photometric detection of galaxy cluster candidates in large surveys." In Proceedings of the MG16 Meeting on General Relativity. WORLD SCIENTIFIC, 2023. http://dx.doi.org/10.1142/9789811269776_0030.

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Giri, Sambit Kumar. "Imprints of early Universe galaxy formation on the 21-cm signal." In XXXVth URSI General Assembly and Scientific Symposium. URSI – International Union of Radio Science, 2023. http://dx.doi.org/10.46620/ursigass.2023.3549.xmne8933.

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Chen, Xi, Simon P. Ellingsen, Ye Xu, and Zhi-Qiang Shen. "Searches for class I methanol masers in the Galaxy." In 2014 XXXIth URSI General Assembly and Scientific Symposium (URSI GASS). IEEE, 2014. http://dx.doi.org/10.1109/ursigass.2014.6930058.

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Reports on the topic "Galaxy: general"

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Meyer, B. S., and D. N. Schramm. General constraints on the age and chemical evolution of the Galaxy. Office of Scientific and Technical Information (OSTI), 1986. http://dx.doi.org/10.2172/5797647.

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Ortiz, Verónica, Rosa Rodriguez, and Joaquin Tintoré. Lessons learnt from the EuroSea public engagement activities. EuroSea, 2023. http://dx.doi.org/10.3289/eurosea_d8.5.

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The overall goal of this report is to analyse the EuroSea itinerant exhibition as a case study of public engagement activity. Aimed at the general public, this modular and itinerant exhibition raises awareness about the EuroSea project while also promoting ocean literacy and highlighting the importance of ocean observing and forecasting. Public engagement plays a crucial role in Horizon 2020, the EU's research and innovation funding program. It aims to bridge the gap between researchers and society, ensuring that their work is aligned with societal needs and values. This involves bringing toge
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Agudelo Vanegas, Fernán Alonso, and María Camila Henao Hernández. Identificación de estrategias de promoción y fortalecimiento de la participación ciudadana y el control social en pro del control fiscal desde las Contralorías del Departamento de Antioquia. Contraloría General de Antioquia, 2023. http://dx.doi.org/10.58373/obscga.007.

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La organización política colombiana está fundada mentada en el estado social de derecho, el cual dispone de normas que les permiten a los ciudadanos incidir en los distintos momentos de la gestión pública, configurándose así la llamada democratización del Estado. En este sentido, la participación ciudadana es primordial en la medida que orienta el devenir general de la sociedad. Por esta razón, la participación ciudadana en torno al control fiscal en el país se ha ido consolidando desde la década de los años 90 con la habilitación de espacios en el órgano de control fiscal. No obstante, a la f
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Flaishman, Moshe, Herb Aldwinckle, Shulamit Manulis, and Mickael Malnoy. Efficient screening of antibacterial genes by juvenile phase free technology for developing resistance to fire blight in pear and apple trees. United States Department of Agriculture, 2008. http://dx.doi.org/10.32747/2008.7613881.bard.

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Objectives: The original objectives of this project were to: Produce juvenile-free pear and apple plants and examine their sensitivity to E. amylovora; Design novel vectors, for antibacterial proteins and promoters expression, combined with the antisense TFL1 gene, and transformation of Spadona pear in Israel and Galaxy apple in USA. The original objectives were revised from the development of novel vectors with antibacterial proteins combined with the TFL-1 due to the inefficiency of alternative markes initially evaluated in pear, phoshomannose-isomerase and 2-deoxyglucose-6-phosphate phospha
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Galili, Naftali, Roger P. Rohrbach, Itzhak Shmulevich, Yoram Fuchs, and Giora Zauberman. Non-Destructive Quality Sensing of High-Value Agricultural Commodities Through Response Analysis. United States Department of Agriculture, 1994. http://dx.doi.org/10.32747/1994.7570549.bard.

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The objectives of this project were to develop nondestructive methods for detection of internal properties and firmness of fruits and vegetables. One method was based on a soft piezoelectric film transducer developed in the Technion, for analysis of fruit response to low-energy excitation. The second method was a dot-matrix piezoelectric transducer of North Carolina State University, developed for contact-pressure analysis of fruit during impact. Two research teams, one in Israel and the other in North Carolina, coordinated their research effort according to the specific objectives of the proj
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