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Merging sn_maf.sn_tools with sn_utils.
The result: sn_tools.
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Philippe Gris
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Mar 26, 2019
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/FilterWheel/1.3/Wed Jun 20 02:10:25 2012// | ||
/README/1.2/Wed Jun 20 02:10:25 2012// | ||
/instrument.cards/1.1.1.1/Wed Jun 20 02:10:25 2012// | ||
/sb_-41A.dat/1.1.1.1/Wed Jun 20 02:10:25 2012// | ||
/si_-25A.dat/1.1.1.1/Wed Jun 20 02:10:25 2012// | ||
/sr_-21A.dat/1.1.1.1/Wed Jun 20 02:10:25 2012// | ||
/sux_modified.dat/1.1/Wed Jun 20 02:10:25 2012// | ||
/sv_-27A.dat/1.1.1.1/Wed Jun 20 02:10:25 2012// | ||
D |
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snfit_data/Instruments/Landolt |
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:ext:[email protected]:/home/frogshome/cvsroot |
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U U_bessel sux_modified.dat | ||
B B_bessel sb_-41A.dat | ||
V V_bessel sv_-27A.dat | ||
R R_bessel sr_-21A.dat | ||
I I_bessel si_-25A.dat |
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Shifted Bessel transmissions to match Landolt magnitude system. | ||
(see calibration note, N. Reynault, 2005) | ||
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(*) We took Bessel transmissions (divided by lambda | ||
with respect to the Bessel (1990) original paper) | ||
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(*) The filters where shifted bluewards by the following amount | ||
in order to match the Landolt system well. (see the calib note | ||
in notes/calib for an explanation of the whole schmoll). | ||
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U shift: +76.8 dilatation of 0.93 (+) | ||
B shift: -41 A | ||
V shift: -27 A | ||
R shift: -21 A | ||
I shift: -25 A | ||
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(+) Using U-B B-V diagram of Landolt stars compared with synthetic ones. | ||
The filter obtained is thiner than the orginal one by a factor of 0.93 | ||
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sux_modified.dat | ||
sb_-41A.dat | ||
sv_-27A.dat | ||
sr_-21A.dat | ||
si_-25A.dat | ||
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