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Иш: EVOLUTION OF INTRINSIC SCATTER IN THE SFR–STELLAR MASS CORRELATION AT 0.5 < z < 3
The Dust Content and Opacity of Actively Star‐forming Galaxies
Daniela Calzetti, L. Armus, R. C. Bohlin +3
Мақола200018 иқтибосABIInference from Iterative Simulation Using Multiple Sequences
Andrew Gelman, Donald B. Rubin
Мақола199212 иқтибосABIThe Slope of the Black Hole Mass versus Velocity Dispersion Correlation
Scott Tremaine, Karl Gebhardt, R. Bender +12
Мақола20024 иқтибосABIUV Star Formation Rates in the Local Universe
Samir Salim, R. Michael Rich, Stephane Charlot +21
Мақола20073 иқтибосABI