316
Seeing Red Redshifts Cosmology and Academic Science (1998)(en)(306s)-[Arp H C ].pdf
Seeing Red Redshifts Cosmology and Academic Science (1998)(en)(306s)-[Arp H C ]
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aztec half square degree survey of the shades fields - ii. identifications, redshifts, and evidence for large-scale structure.pdf
arXiv:1205.2370v2[astro-ph.CO] 30 Jul 2012Mon. Not. R. Astron. Soc. 000, 1–53 (2012) Printed 31 July
131
properties of qso metal line absorption systems at high redshifts nature and evolution of the absorbers and new evidence on escape of ionizing radiation from galaxies.pdf
QSOMETAL LINE ABSORPTIONSYSTEMS HIGHREDSHIFTS: NATURE ANDEVOLUTION NEWEVIDENCEON ESCAPE IONIZINGRADI
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Star Formation in Emission-Line Galaxies between Redshifts of 0.8 and 1.6(0.8至1.6的红移之间的发射线星系中的恒星形成).pdf
Star Formation in Emission‐Line Galaxies between Redshifts of 0.8 and 1.6(0.8至1.6的红移之间的发射线星系中的恒星形成)
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The effect of a relative infinity on cosmological redshifts.pdf
The effect of a relative infinity on cosmological redshifts
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DIRECT GAS-PHASE METALLICITIES, STELLAR PROPERTIES, AND LOCAL ENVIRONMENTS OF EMISSION-LINE GALAXIES AT REDSHIFTS BELOW 0.90.pdf
DIRECT GAS-PHASE METALLICITIES, STELLAR PROPERTIES, AND LOCAL ENVIRONMENTS OF EMISSION-LINE GALAXIES AT REDSHIFTS BELOW 0.90
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substructure in clusters containing wide-angle tailed radio galaxies. i. new redshifts.pdf
substructure in clusters containing wide-angle tailed radio galaxies. i. new redshifts
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CAIRNS: The Cluster And Infall Region Nearby Survey I. Redshifts and Mass Profiles.pdf
The CAIRNS (Cluster And Infall Region Nearby Survey) project is a nspectroscopic survey of the infall regions surrounding eight nearby, rich, nX-ray luminous clusters of galaxies. We collect 15665 redshifts (3471 new or nremeasured) within sim 5-10 Mpc of the centers of the clusters, making it the nlargest study of the infall regions of clusters. We determine cluster nmembership and the ma..
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the micro-arcsecond scintillation-induced variability (masiv) survey iii. optical identifications and new redshifts(335.78kb).pdf
the micro-arcsecond scintillation-induced variability (masiv) survey iii. optical identifications and new redshifts(335.78kb)

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