CSST Simulations
Milky Way stellar catalogue, PHAT stellar catalogue simulations for the China Space Station Telescope.
If you have any question or comment, please send an email to "cy-at-ahu.edu.cn".
Alternative mirror site: www.sec.center
Added Gaia EDR3 filters.
Added CSST main Survey Camera filters.
The paper is available at https://doi.org/10.1051/0004-6361/201936612 .
The paper is available at arXiv:1910.09037. It is accepted for publication in A&A.
Now you can supply different extinction value for different stars in your catalogue, by specifying the column number in section 4.
Instead of using polynominal coefficients as in the last update, we now compute grids with Av=[0., 0.5, 1., 2., 5., 10., 20] and interpolate among them. Correct an error for AB+Vega mixed photometric systems.
Every spectrum used has been convlved with the extinction curve (Cardelli et al. (1989) + O'Donnell (1994) with RV=3.1.), therefore the spectral variation effect hass been considered. The non-lineararity as a function of Av amount has been also taken into account until the third order of the polynomial: Ai = a1*Av + a2*Av^2 + a3*Av^3.
Now website is changed from Python/Flask to PHP. Latest BC tables and interpolation code used now.
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This website is now on public domain.
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The first time this website is on-line for internal test. It provides you the bolometric corrections given the stellar parameters.
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Milky Way stellar catalogue, PHAT stellar catalogue simulations for the China Space Station Telescope.
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