Interstellar silicate profile towards Galactic Center
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https://figshare.com/articles/dataset/Interstellar_silicate_profile_towards_Galactic_Center/5208829/1
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Data set from Kemper et al. 2004, Astrophys. J. 609, 826, doi:10.1086/421339, http://adsabs.harvard.edu/abs/2004ApJ...609..826K<br>sgr_wjv_tot.dat: observed spectrum towards Sgr A*. Columns are wavelength (micron), flux (Jy), error (Jy), according to Figure 20 of W.J. Vriend's thesis. <br>sgra_tau2_wjv.dat: Optical depth in the silicate feature, 8-13 micron. This spectrum represents the <b>interstellar silicate profile </b>and this is what you want to use in comparison with silicate features elsewhere, or directly with mass absorption coefficients or opacities.<br>GCS3_abs4.txt: Optical depth spectrum of GCS3, from 7-13 micron. GCS3_mgr.txt: Observed spectrum of GCS3<br>GCS4_abs4.txt: Optical depth spectrum of GCS4, from 7-13 micron. GCS4_mgr.txt: Observed spectrum of GCS4<br>Direct any questions to Ciska Kemper at ciska@asiaa.sinica.edu.tw
提供机构：
figshare
创建时间：
2017-07-14
