Measuring the baryonic Tully-Fisher relation below the detection threshold
We present a novel 2D flux density model for observed H i emission lines combined with a Bayesian stacking technique to measure the baryonic Tully-Fisher relation below the nominal detection threshold. We simulate a galaxy catalogue, which includes H i lines described with either Gaussian or busy fu...
المؤلفون الرئيسيون: | Pan, H, Jarvis, MJ, Ponomareva, AA, Santos, MG, Allison, JR, Maddox, N, Frank, BS |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
Oxford University Press
2021
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مواد مشابهة
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