The selection function of the RAVE survey
We characterize the selection function of RAVE using 2MASS as our underlying population, which we assume represents all stars which could have potentially been observed. We evaluate the completeness fraction as a function of position, magnitude, and color in two ways: first, on a field-by-field basi...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
2017
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1611.00733
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| Author Notes: | Jennifer Wojno, Georges Kordopatis, Tilmann Piffl, James Binney, Matthias Steinmetz, Gal Matijevič, Joss Bland-Hawthorn, Sanjib Sharma, Paul McMillan, Fred Watson, Warren Reid, Andrea Kunder, Harry Enke, Eva K. Grebel, George Seabroke, Rosemary F.G. Wyse, Tomaž Zwitter, Olivier Bienaymé, Kenneth C. Freeman, Brad K. Gibson, Gerry Gilmore, Amina Helmi, Ulisse Munari, Julio F. Navarro, Quentin A. Parker, Arnaud Siebert |
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