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Anton M. Koekemoer

Researcher at Space Telescope Science Institute

Publications -  1262
Citations -  116974

Anton M. Koekemoer is an academic researcher from Space Telescope Science Institute. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 168, co-authored 1127 publications receiving 106796 citations. Previous affiliations of Anton M. Koekemoer include University of Massachusetts Amherst & Max Planck Society.

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A Very Large (θ E ≳ 40″) Strong Gravitational Lens Selected with the Sunyaev-Zel’dovich Effect: PLCK G287.0+32.9 (z = 0.38)

TL;DR: In this article, strong-lensing analysis of the PLCK G287 cluster is presented, identifying 20 sets of multiply imaged galaxies and candidates in new Hubble Space Telescope (HST) data, including a long, l similar to 22 '' giant arc, as well as a quadruply imaged, apparently bright (magnified to J(F110W) = 25.3 AB), likely high redshift dropout galaxy at z(phot) = 6.90 [6.13-8.43] (95% C.I.).
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The ALMA Frontier Fields Survey III: 1.1 mm Emission Line Identifications in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370, and Abell S1063

TL;DR: In this paper, the authors perform a search for emission lines in the ALMA observations of five Frontier Fields clusters and assess the reliability of their detection by associating line candidates with detected galaxies in deep nearinfrared imaging.
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Radio observations of the CDF-South: a possible link between radio emission and star formation in X-ray selected AGN

TL;DR: In this paper, the authors explore the radio emission of X-ray selected AGN by combining deep radio (1.4GHz; 60micro-Jy) and Xray data with multi-wavelength (optical, mid-infrared) observations in the Extended Chandra Deep Field South (E-CDFS).
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COSMOS 5921+0638: characterization and analysis of a new strong gravitationally lensed AGN

TL;DR: In this paper, the authors investigated the nature of COSMOS 5921+0638 by studying its photometric, spectroscopic and physical properties and concluded that the observed flux ratio anomalies are probably due to microlensing by stars in the lensing galaxy and/or a combination of static phenomena.