Table 6
Predicted differential quasar counts over 15.5 < g < 25 and 0 < z < 6 for a survey covering 10 000 deg2, based on our best-fit PLE or PLE+LEDE luminosity function model.
PLE model | |||||||
g \ z | 0.5 | 1.5 | 2.5 | 3.5 | 4.5 | 5.5 | Total |
|
|||||||
15.75 | 26 | 2 | 10 | 0 | 0 | 0 | 38 |
16.25 | 58 | 8 | 33 | 0 | 0 | 0 | 100 |
16.75 | 143 | 39 | 87 | 3 | 0 | 0 | 272 |
17.25 | 386 | 180 | 231 | 10 | 0 | 0 | 806 |
17.75 | 1134 | 813 | 626 | 26 | 0 | 0 | 2599 |
18.25 | 3396 | 3468 | 1727 | 68 | 0 | 0 | 8660 |
18.75 | 8930 | 12 525 | 4780 | 179 | 0 | 0 | 26 413 |
19.25 | 17 963 | 32 977 | 12 319 | 462 | 1 | 0 | 63 722 |
19.75 | 28 172 | 61 064 | 26 357 | 1170 | 3 | 0 | 11 3766 |
20.25 | 38 732 | 90 121 | 45 742 | 2827 | 7 | 0 | 177 430 |
20.75 | 50 756 | 121 402 | 68 898 | 6299 | 18 | 0 | 247 474 |
21.25 | 65 550 | 157 499 | 95 351 | 12 540 | 47 | 0 | 331 487 |
21.75 | 84 300 | 204 485 | 125 498 | 22 098 | 120 | 0 | 436 402 |
22.25 | 108 476 | 264 463 | 159 494 | 35 046 | 301 | 1 | 567 480 |
22.75 | 138 490 | 341 419 | 201 444 | 51 351 | 737 | 3 | 733 442 |
23.25 | 178 421 | 440 413 | 251 497 | 70 978 | 1722 | 7 | 943 438 |
23.75 | 228 412 | 570 415 | 314 473 | 93 793 | 3739 | 17 | 1 210 549 |
24.25 | 292 450 | 737 414 | 392 421 | 119 423 | 7357 | 42 | 1 250 506 |
24.75 | 374 472 | 954 440 | 491 472 | 149 432 | 13 010 | 106 | 1 282 533 |
|
|||||||
Total | 1 220 567 | 3 292 548 | 2 292 558 | 565 406 | 27 062 | 175 | 8 299 516 |
|
|||||||
PLE+LEDE model | |||||||
g \ z | 0.5 | 1.5 | 2.5 | 3.5 | 4.5 | 5.5 | Total |
|
|||||||
15.75 | 35 | 5 | 1 | 0 | 0 | 0 | 42 |
16.25 | 82 | 20 | 5 | 0 | 0 | 0 | 108 |
16.75 | 200 | 77 | 20 | 1 | 0 | 0 | 298 |
17.25 | 519 | 291 | 76 | 3 | 0 | 0 | 889 |
17.75 | 1402 | 1088 | 287 | 10 | 0 | 0 | 2787 |
18.25 | 3758 | 3887 | 1065 | 35 | 0 | 0 | 8745 |
18.75 | 9092 | 12 345 | 3737 | 117 | 0 | 0 | 25 291 |
19.25 | 17 972 | 31 289 | 11 415 | 382 | 1 | 0 | 61 059 |
19.75 | 28 629 | 59 594 | 27 445 | 1163 | 4 | 0 | 116 436 |
20.25 | 39 554 | 90 405 | 50 511 | 3077 | 13 | 0 | 183 460 |
20.75 | 51 163 | 121 409 | 76 197 | 6648 | 36 | 1 | 255 453 |
21.25 | 64 559 | 155 423 | 103 493 | 11 780 | 97 | 2 | 335 454 |
21.75 | 80 771 | 196 466 | 133 441 | 18 077 | 242 | 4 | 429 401 |
22.25 | 100 458 | 246 495 | 169 498 | 25 349 | 543 | 9 | 543 453 |
22.75 | 125 446 | 309 493 | 214 495 | 33 716 | 1063 | 21 | 684 434 |
23.25 | 156 421 | 387 478 | 271 421 | 43 594 | 1820 | 46 | 860 480 |
23.75 | 194 486 | 485 419 | 342 470 | 55 625 | 2799 | 93 | 1 281 592 |
24.25 | 241 494 | 609 419 | 433 445 | 70 598 | 3989 | 173 | 1 259 518 |
24.75 | 299 497 | 764 419 | 549 467 | 89 454 | 5393 | 291 | 1 208 521 |
|
|||||||
Total | 1 216 538 | 3 276 523 | 2 289 589 | 359 429 | 16 003 | 640 | 7 258 521 |
Notes. Bins are centered on the indicated magnitude and redshift values. The ranges in each bin are Δg = 0.5 and Δz = 1.
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