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AGN number-density tests #178
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subclass_name: AGN_NumberDensities.AGN_NumberDensity | ||
band: g | ||
rest_frame_band: i | ||
Mag_lim: -22.5 | ||
z_lim: [0.3, 2.2] | ||
observation: 'SDSS' | ||
validation_range: [15.5, 19.] | ||
agn_flux_fraction: 0. | ||
duty_cycle_on: true | ||
no_agn_extinction: true | ||
included_by_default: true | ||
description: 'Plot N and N(<mag) distributions for selected magnitude bound and redshift range in specified band and compare with SDSS data from Richards 2006' |
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subclass_name: AGN_NumberDensities.AGN_NumberDensity | ||
band: g | ||
rest_frame_band: i | ||
Mag_lim: -22.5 | ||
z_lim: [0.3, 2.2] | ||
observation: 'SDSS' | ||
validation_range: [15.5, 19.] | ||
agn_flux_fraction: 0. | ||
duty_cycle_on: true | ||
no_agn_extinction: true | ||
cumulative_only: true | ||
truncate_cat_name: true | ||
included_by_default: false | ||
no_legend_title: true | ||
description: 'Plot N and N(<mag) distributions for selected magnitude bound and redshift range in specified band and compare with SDSS data from Richards 2006' |
Original file line number | Diff line number | Diff line change |
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subclass_name: AGN_NumberDensities.AGN_NumberDensity | ||
band: g | ||
rest_frame_band: i | ||
Mag_lim: -22.5 | ||
z_lim: [0.3, 2.2] | ||
observation: 'SDSS' | ||
validation_range: [15.5, 19.] | ||
agn_flux_fraction: 0.5 | ||
There was a problem hiding this comment. Choose a reason for hiding this commentThe reason will be displayed to describe this comment to others. Learn more. What motivated the minimum flux fraction of 0.5 here (and also in |
||
no_agn_extinction: true | ||
duty_cycle_on: false | ||
included_by_default: false | ||
description: 'Plot N and N(<mag) distributions for selected magnitude bound and redshift range in specified band and compare with SDSS data from Richards 2006' |
Original file line number | Diff line number | Diff line change |
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@@ -0,0 +1,12 @@ | ||
subclass_name: AGN_NumberDensities.AGN_NumberDensity | ||
band: i | ||
rest_frame_band: i | ||
Mag_lim: -22.5 | ||
z_lim: [0.3, 2.2] | ||
observation: 'SDSS' | ||
validation_range: [16., 19.5] | ||
agn_flux_fraction: 0. | ||
duty_cycle_on: true | ||
no_agn_extinction: true | ||
included_by_default: true | ||
description: 'Plot N and N(<mag) distributions for selected magnitude bound and redshift range in specified band and compare with SDSS data from Richards 2006' |
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -0,0 +1,15 @@ | ||
subclass_name: AGN_NumberDensities.AGN_NumberDensity | ||
band: i | ||
rest_frame_band: i | ||
Mag_lim: -22.5 | ||
z_lim: [0.3, 2.2] | ||
observation: 'SDSS' | ||
validation_range: [16., 19.5] | ||
agn_flux_fraction: 0. | ||
duty_cycle_on: true | ||
no_agn_extinction: true | ||
cumulative_only: true | ||
truncate_cat_name: true | ||
no_legend_title: true | ||
included_by_default: false | ||
description: 'Plot N and N(<mag) distributions for selected magnitude bound and redshift range in specified band and compare with SDSS data from Richards 2006' |
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -0,0 +1,12 @@ | ||
subclass_name: AGN_NumberDensities.AGN_NumberDensity | ||
band: i | ||
rest_frame_band: i | ||
Mag_lim: -22.5 | ||
z_lim: [0.3, 2.2] | ||
observation: 'SDSS' | ||
validation_range: [15.5, 19.] | ||
agn_flux_fraction: 0.5 | ||
no_agn_extinction: true | ||
duty_cycle_on: false | ||
included_by_default: false | ||
description: 'Plot N and N(<mag) distributions for selected magnitude bound and redshift range in specified band and compare with SDSS data from Richards 2006' |
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# RICHARDS ET AL. 2006_AJ_131_2766 | ||
# Differential counts for g band with 0.4 < z < 2.2, M_g < 22.5, N per 0.25 mag deg^-2 | ||
# Differential counts for i band with 0.3 < z < 2.2, M_i < 22.5, N per 0.25 mag deg^-2 | ||
# Cumulative number counts N(<x) in units of deg^-2 for 0.3 < z < 2.2 | ||
# Table differs from published version; i-band columns moved up by 1 row as instructed by Gordon Richards | ||
M N_g dN_g N(<g) dN(<g) N_Q N_i dN_i N(<i) dN(<i) N_Q | ||
15.475 0.00 0.00 0.00 0.00 2 0.00 0.00 0.00 0.00 3 | ||
15.725 0.00 0.00 0.00 0.00 3 0.00 0.00 0.00 0.00 2 | ||
15.975 0.00 0.00 0.01 0.00 4 0.01 0.00 0.02 0.00 10 | ||
16.225 0.01 0.00 0.01 0.00 11 0.01 0.00 0.02 0.00 12 | ||
16.475 0.01 0.00 0.02 0.00 10 0.01 0.00 0.03 0.00 23 | ||
16.725 0.02 0.00 0.04 0.00 32 0.04 0.01 0.08 0.01 67 | ||
16.975 0.06 0.01 0.10 0.01 85 0.07 0.01 0.15 0.01 107 | ||
17.225 0.08 0.01 0.17 0.01 117 0.11 0.01 0.26 0.01 174 | ||
17.475 0.12 0.01 0.29 0.01 190 0.21 0.01 0.47 0.01 327 | ||
17.725 0.23 0.01 0.53 0.01 357 0.33 0.01 0.80 0.01 511 | ||
17.975 0.31 0.01 0.83 0.01 472 0.55 0.02 1.35 0.02 849 | ||
18.225 0.56 0.02 1.40 0.02 868 0.82 0.02 2.17 0.02 1257 | ||
18.475 0.78 0.02 2.18 0.02 1202 1.25 0.03 3.42 0.03 1923 | ||
18.725 1.19 0.03 3.37 0.03 1839 1.86 0.04 5.28 0.03 2870 | ||
18.975 1.70 0.03 5.07 0.03 2620 2.62 0.04 7.90 0.04 4028 | ||
19.225 1.61 0.03 6.68 0.03 2484 ... ... ... ... 900 | ||
19.475 0.56 0.02 7.24 0.02 855 ... ... ... ... 216 | ||
19.725 0.13 0.01 7.37 0.01 206 ... ... ... ... 55 | ||
19.975 0.03 0.01 7.41 0.00 53 ... ... ... ... 20 | ||
20.225 0.01 0.00 7.42 0.00 19 ... ... ... ... ... |
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# RICHARDS ET AL. 2006_AJ_131_2766 | ||
There was a problem hiding this comment. Choose a reason for hiding this commentThe reason will be displayed to describe this comment to others. Learn more. Is it okay if the extension of this file goes like |
||
# Differential counts for g band with 0.4 < z < 2.2, M_g < 22.5, N per 0.25 mag deg^-2 | ||
# Differential counts for i band with 0.3 < z < 2.2, M_i < 22.5, N per 0.25 mag deg^-2 | ||
# Cumulative number counts N(<x) in units of deg^-2 for 0.3 < z < 2.2 | ||
M N_g dN_g N(<g) dN(<g) N_Q N_i dN_i N(<i) dN(<i) N_Q | ||
15.475 0.00 0.00 0.00 0.00 2 0.00 0.00 0.00 0.00 1 | ||
15.725 0.00 0.00 0.00 0.00 3 0.00 0.00 0.00 0.00 3 | ||
15.975 0.00 0.00 0.01 0.00 4 0.00 0.00 0.00 0.00 2 | ||
16.225 0.01 0.00 0.01 0.00 11 0.01 0.00 0.01 0.00 10 | ||
16.475 0.01 0.00 0.02 0.00 10 0.01 0.00 0.02 0.00 12 | ||
16.725 0.02 0.00 0.04 0.00 32 0.01 0.00 0.03 0.00 23 | ||
16.975 0.06 0.01 0.10 0.01 85 0.04 0.01 0.08 0.01 67 | ||
17.225 0.08 0.01 0.17 0.01 117 0.07 0.01 0.15 0.01 107 | ||
17.475 0.12 0.01 0.29 0.01 190 0.11 0.01 0.26 0.01 174 | ||
17.725 0.23 0.01 0.53 0.01 357 0.21 0.01 0.47 0.01 327 | ||
17.975 0.31 0.01 0.83 0.01 472 0.33 0.01 0.80 0.01 511 | ||
18.225 0.56 0.02 1.40 0.02 868 0.55 0.02 1.35 0.02 849 | ||
18.475 0.78 0.02 2.18 0.02 1202 0.82 0.02 2.17 0.02 1257 | ||
18.725 1.19 0.03 3.37 0.03 1839 1.25 0.03 3.42 0.03 1923 | ||
18.975 1.70 0.03 5.07 0.03 2620 1.86 0.04 5.28 0.03 2870 | ||
19.225 1.61 0.03 6.68 0.03 2484 2.62 0.04 7.90 0.04 4028 | ||
19.475 0.56 0.02 7.24 0.02 855 ... ... ... ... 900 | ||
19.725 0.13 0.01 7.37 0.01 206 ... ... ... ... 216 | ||
19.975 0.03 0.01 7.41 0.00 53 ... ... ... ... 55 | ||
20.225 0.01 0.00 7.42 0.00 19 ... ... ... ... 20 |
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# RICHARDS ET AL. 2006_AJ_131_2766 | ||
There was a problem hiding this comment. Choose a reason for hiding this commentThe reason will be displayed to describe this comment to others. Learn more. Is the QLF validation using Table 6 also planned? Maybe it'll go in a different PR? Please let me know if I'm missing something! |
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#phi in units of Mpc^-3 mag^-1 | ||
#Fill indicates how well column is covered by data | ||
z M_i(z=2) log_phi dlog_phi Fill zbar N_Q N_Q^corr | ||
0.49 -26.25 -7.74 5.48 1 0.59 11 11.6 | ||
0.49 -25.95 -7.46 7.55 1 0.58 21 22.2 | ||
0.49 -25.65 -7.26 9.47 1 0.58 33 34.8 | ||
0.49 -25.35 -7.07 11.90 1 0.55 52 54.9 | ||
0.49 -25.05 -6.81 16.01 1 0.56 94 99.3 | ||
0.49 -24.75 -6.59 20.52 1 0.58 154 163.0 | ||
0.49 -24.45 -6.42 24.94 1 0.57 228 241.0 | ||
0.49 -24.15 -6.23 35.98 0 0.54 337 358.2 | ||
0.49 -23.85 -6.08 43.96 0 0.51 358 377.2 | ||
0.49 -23.55 -5.97 75.48 0 0.45 311 331.3 | ||
0.49 -23.25 -5.81 102.81 0 0.41 290 307.2 | ||
0.49 -22.95 -6.35 174.24 0 0.41 39 46.9 | ||
0.87 -27.45 -8.39 1.81 1 0.95 5 5.3 | ||
0.87 -27.15 -7.81 3.53 1 0.95 19 20.0 | ||
0.87 -26.85 -7.63 4.36 1 0.95 29 30.5 | ||
0.87 -26.55 -7.29 6.48 1 0.94 64 67.4 | ||
0.87 -26.25 -6.96 9.38 1 0.91 134 141.2 | ||
0.87 -25.95 -6.84 10.84 1 0.92 179 188.5 | ||
0.87 -25.65 -6.62 13.87 1 0.92 293 308.6 | ||
0.87 -25.35 -6.42 17.57 1 0.93 470 495.1 | ||
0.87 -25.05 -6.30 24.49 0 0.89 492 520.0 | ||
0.87 -24.75 -6.23 51.36 0 0.78 284 307.6 | ||
0.87 -24.45 -6.13 100.79 0 0.73 122 133.7 | ||
0.87 -24.15 -5.86 1446.59 0 0.74 9 13.8 | ||
1.25 -28.05 -8.15 2.06 1 1.31 12 12.6 | ||
1.25 -27.75 -7.86 2.85 1 1.32 23 24.2 | ||
1.25 -27.45 -7.76 3.20 1 1.27 29 30.5 | ||
1.25 -27.15 -7.36 5.07 1 1.30 73 76.8 | ||
1.25 -26.85 -7.08 7.00 1 1.30 139 146.3 | ||
1.25 -26.55 -6.83 9.37 1 1.29 249 262.1 | ||
1.25 -26.25 -6.58 12.44 1 1.29 439 462.1 | ||
1.25 -25.95 -6.33 16.62 1 1.28 783 824.2 | ||
1.25 -25.65 -6.24 22.56 0 1.23 733 773.5 | ||
1.25 -25.35 -6.12 48.01 0 1.13 360 382.8 | ||
1.25 -25.05 -5.74 1332.39 0 1.09 12 14.6 | ||
1.63 -28.65 -8.25 1.70 1 1.66 11 11.6 | ||
1.63 -28.35 -8.08 2.06 1 1.67 16 16.8 | ||
1.63 -28.05 -7.78 2.91 1 1.68 32 33.7 | ||
1.63 -27.75 -7.39 4.57 1 1.66 79 83.2 | ||
1.63 -27.45 -7.12 6.23 1 1.67 147 154.7 | ||
1.63 -27.15 -6.86 8.43 1 1.66 269 283.2 | ||
1.63 -26.85 -6.63 10.94 1 1.65 453 476.8 | ||
1.63 -26.55 -6.40 14.35 1 1.66 779 820.0 | ||
1.63 -26.25 -6.26 19.09 0 1.62 892 940.9 | ||
1.63 -25.95 -6.14 38.86 0 1.52 477 506.0 | ||
2.01 -28.95 -8.41 1.37 1 1.99 8 8.4 | ||
2.01 -28.65 -7.94 2.37 1 2.02 24 25.3 | ||
2.01 -28.35 -7.75 2.94 1 2.02 37 39.0 | ||
2.01 -28.05 -7.37 4.53 1 2.01 88 92.7 | ||
2.01 -27.75 -7.15 5.86 1 2.03 147 155.0 | ||
2.01 -27.45 -6.87 8.03 1 2.02 276 291.0 | ||
2.01 -27.15 -6.67 10.22 1 2.01 447 471.1 | ||
2.01 -26.85 -6.45 13.97 0 1.99 648 682.7 | ||
2.01 -26.55 -6.24 40.12 0 1.90 430 464.3 | ||
2.01 -26.25 -6.03 495.10 0 1.87 30 39.4 | ||
2.40 -28.95 -8.12 2.07 1 2.44 14 17.9 | ||
2.40 -28.65 -8.03 2.30 1 2.41 17 21.8 | ||
2.40 -28.35 -7.59 3.71 1 2.37 48 59.7 | ||
2.40 -28.05 -7.29 5.28 1 2.37 98 121.2 | ||
2.40 -27.75 -7.05 7.01 1 2.37 164 208.1 | ||
2.40 -27.45 -6.82 9.50 0 2.38 265 356.0 | ||
2.40 -27.15 -6.61 22.11 0 2.30 246 309.0 | ||
2.40 -26.85 -6.24 249.51 0 2.25 37 48.8 | ||
2.80 -29.55 -8.57 1.76 1 2.70 3 6.2 | ||
2.80 -29.25 -8.34 1.84 1 2.82 7 10.6 | ||
2.80 -28.95 -8.08 6.51 1 2.82 10 19.2 | ||
2.80 -28.65 -7.95 3.68 1 2.80 12 25.9 | ||
2.80 -28.35 -7.65 11.94 1 2.83 24 51.5 | ||
2.80 -28.05 -7.33 15.75 1 2.81 50 107.9 | ||
2.80 -27.75 -7.11 20.63 1 2.82 75 180.9 | ||
2.80 -27.45 -7.07 24.17 1 2.79 73 199.8 | ||
3.25 -29.55 -8.54 1.10 1 3.35 7 8.2 | ||
3.25 -29.25 -8.30 1.45 1 3.25 12 14.2 | ||
3.25 -28.95 -8.33 1.40 1 3.20 11 13.1 | ||
3.25 -28.65 -7.94 2.18 1 3.25 28 32.5 | ||
3.25 -28.35 -7.64 3.12 1 3.23 54 64.6 | ||
3.25 -28.05 -7.47 3.89 1 3.25 77 95.9 | ||
3.25 -27.75 -7.32 4.72 1 3.24 103 134.3 | ||
3.25 -27.45 -7.09 6.47 1 3.21 161 228.8 | ||
3.25 -27.15 -6.99 7.48 1 3.22 191 287.9 | ||
3.25 -26.85 -6.80 10.40 0 3.20 234 377.5 | ||
3.25 -26.55 -6.63 39.58 0 3.11 52 103.7 | ||
3.75 -28.95 -8.24 1.56 1 3.69 14 15.7 | ||
3.75 -28.65 -8.02 2.03 1 3.67 22 25.7 | ||
3.75 -28.35 -7.65 3.06 1 3.77 54 60.5 | ||
3.75 -28.05 -7.64 3.11 1 3.76 55 62.1 | ||
3.75 -27.75 -7.44 4.07 1 3.74 83 99.3 | ||
3.75 -27.45 -7.27 4.96 1 3.76 119 144.2 | ||
3.75 -27.15 -7.16 6.59 0 3.72 117 158.4 | ||
3.75 -26.85 -6.89 25.48 0 3.59 27 54.6 | ||
4.25 -29.25 -8.48 1.16 1 4.25 8 8.4 | ||
4.25 -28.65 -8.18 1.64 1 4.22 16 16.9 | ||
4.25 -28.35 -8.11 1.79 1 4.19 19 20.0 | ||
4.25 -28.05 -7.91 2.26 1 4.21 30 31.8 | ||
4.25 -27.75 -7.81 2.53 1 4.24 38 40.2 | ||
4.25 -27.45 -7.59 3.84 0 4.16 44 47.1 | ||
4.75 -28.65 -8.52 1.14 1 4.66 7 7.4 | ||
4.75 -28.35 -8.46 1.22 1 4.71 8 8.4 | ||
4.75 -28.05 -8.00 2.07 1 4.66 23 24.2 | ||
4.75 -27.75 -8.06 1.94 0 4.66 20 21.1 | ||
4.75 -27.45 -7.78 20.57 0 4.62 6 8.3 |
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Why is the number density agreement for the three
for the
SDSS_g*
tests so poor? I'm looking at plots likeSDSS_g
test on thecosmoDC2_v1.1.4_small_combined_agn
catalog. I'll try running it for a bigger catalog; maybe the small one is missing the brightest quasars? Also, is there a list of catalogs this test is meant to run for and does DESCQA let you specify it anywhere?