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--- tests:streams:results [2015/09/03 05:52] – aspagna
+++ tests:streams:results [2022/10/24 12:26] (current) – external edit 127.0.0.1
@@ Line 22: / Line 22: @@
 We selected all the stream stellar particles within 3 kpc of the Sun from Robyn Sanderson's data set and applied the random errors expected for FGK dwarfs as estimated by [[http://adsabs.harvard.edu/abs/2015arXiv150803736R| Re Fiorentin et al. 2015]].
+{{ :tests:streams:spagna_figura10b.png?600 |}}
 Here, we present the resulting Lxy vs. Lz distribution of the "expected" local streams found using the "true" values (bottom panel),  the final Gaia catalog (middle panel), and the current ground based surveys (top panel).
@@ Line 53: / Line 55: @@
 {{:tests:streams:bothlt_n50_5e3_1e4_120min_line-triangle_two_params.png?200|}}
+The results for $(M/(10^{12}M_\odot), q_z, R_{Halo})$:
+A sample of 50 stars:
+{{:tests:streams:from0000_line-triangle_three_params.png?200|}}
+Another different sample of 50 stars and the histogram of acceleration at Pal5 for this sample:
+{{:tests:streams:from3000_line-triangle_three_params.png?200|}}
+{{:tests:streams:hist_acc_kohei.png?200|}}
@@ Line 185: / Line 196: @@
 ===Kohei Hattori===
 [Kohei2015]
-I use 50 randomly selected stars (without error) from a single stream (#41). I model the orbital energy distribution in the stream (without distinguishing leading and trailing streams) as a Gaussian distribution and run an emcee code to derive the posterior distribution of $(\log_{10} M/M_\odot, \log_{10} b/{\rm kpc})$.
+I use 50 randomly selected stars (without error) from a single stream. I model the orbital energy distribution in the stream (without distinguishing leading and trailing streams) as a Gaussian distribution and run an emcee code to derive the posterior distribution of $(\log_{10} M/M_\odot, \log_{10} b/{\rm kpc})$.
+Results for Stream #41
 {{:tests:streams:kohei_isochrone41_line-triangle_two_params.png?200|}}
 {{:tests:streams:isochrone41_posterior_kohei.png?200|}}
+Results for Stream #79
+{{:tests:streams:kohei_isochrone79_line-triangle_two_params.png?200|}}
+Results for Stream #111
+{{:tests:streams:kohei_isochrone111_line-triangle_two_params.png?200|}}
+Why b is overestimated in some cases? [e.g., #41]
+{{:tests:streams:sphericalisochrone_radius_energy.png?200|}}
 ====Finding streams in the halo challenge====