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Adaptive optics deep imaging of QSO UM402 field: the host galaxy of a radio quiet QSO at z~3

, , , , and . (2013)cite arxiv:1301.1129Comment: 17 pages, 7 figures, submitted to PASJ on July 12, 2012.

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The reaction of OH with acetone and acetone-d(6) from 298 to 832 K: Rate coefficients and mechanism, , , and . Journal of Chemical Physics, 119 (20): 10600--10606 (November 2003)743CH Times Cited:20 Cited References Count:36.Discovery of a Damped Lya Absorber at z = 3.3 along a galaxy sight-line in the SSA22 field, , , , , , , and . (2015)cite arxiv:1512.04625Comment: 6 pages, 5 figures, submitted to ApJ.Herschel protocluster survey: A search for dusty star-forming galaxies in protoclusters at z=2-3, , , , , , , , , and 8 other author(s). (2016)cite arxiv:1605.07370Comment: 15 pages, 5 figures, 12 tables, Accepted for publication in MNRAS.ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1608.02941Comment: Accepted for publication in ApJ.Spatiotemporal chaos induced by a multiplicative noise process, , and . Physica A: Statistical and Theoretical Physics, 204 (1-4): 755--769 (Mar 1, 1994)Extending the Application of a Neural Network for Failure Analysis of Electronic Circuit Boards., , , , , , and . IIA/SOCO, ICSC Academic Press, Rochester, NY, USA, (1999)Silicon Photonics Coherent Optical Subassembly with EO and OE Bandwidths of over 50 GHz., , , , , , , , , and 5 other author(s). OFC, page 1-3. IEEE, (2020)Rate coefficients and mechanistic analysis for reaction of OH with vinyl chloride between 293 and 730 K, , , , , and . Journal of Physical Chemistry A, 105 (41): 9436--9444 (January 2001)Profiles of Lyman\alpha\ Emission Lines, , , , , and . (2012)cite arxiv:1203.3633Comment: 15 pages, Accepted for publication in Astrophysical Journal.Two complementary representations of a scale-free network, , , , and . Physica A: Statistical Mechanics and its Applications, 349 (1-2): 349--363 (Apr 1, 2005)