Table 1.
Summary of star-forming and quenched galaxies and diffuse gas per square degree in the simulated light cones (constructed up to z = 0.356).
| Type | Number of galaxies | Total stellar mass | Total gas mass | |
|---|---|---|---|---|
| (M⊙) | (M⊙) | |||
| LC0 | Star-forming galaxies | 1174 | 3.299 × 1013 | 1.114 × 1014 |
| Quenched galaxies | 459 | 3.847 × 1013 | 1.332 × 1014 | |
| Diffuse gas | ... | ... | 1.324 × 1015 | |
| LC1 | Star-forming galaxies | 1217 | 3.426 × 1013 | 1.283 × 1014 |
| Quenched galaxies | 669 | 5.376 × 1013 | 2.290 × 1014 | |
| Diffuse gas | ... | ... | 1.418 × 1015 | |
| LC2 | Star-forming galaxies | 1306 | 3.830 × 1013 | 1.450 × 1014 |
| Quenched galaxies | 675 | 5.395 × 1013 | 2.448 × 1014 | |
| Diffuse gas | ... | ... | 1.410 × 1015 | |
| LC3 | Star-forming galaxies | 1683 | 5.236 × 1013 | 2.004 × 1014 |
| Quenched galaxies | 868 | 6.501 × 1013 | 2.369 × 1014 | |
| Diffuse gas | ... | ... | 1.711 × 1015 | |
| LC4 | Star-forming galaxies | 1272 | 3.852 × 1013 | 1.641 × 1014 |
| Quenched galaxies | 577 | 4.175 × 1013 | 1.317 × 1014 | |
| Diffuse gas | ... | ... | 1.421 × 1015 | |
| LC5 | Star-forming galaxies | 1222 | 3.539 × 1013 | 1.418 × 1014 |
| Quenched galaxies | 518 | 4.242 × 1013 | 1.559 × 1014 | |
| Diffuse gas | ... | ... | 1.343 × 1015 | |
| LC6 | Star-forming galaxies | 1300 | 3.412 × 1013 | 1.241 × 1014 |
| Quenched galaxies | 554 | 4.419 × 1013 | 1.599 × 1014 | |
| Diffuse gas | ... | ... | 1.411 × 1015 | |
| LC7 | Star-forming galaxies | 1389 | 4.320 × 1013 | 1.684 × 1014 |
| Quenched galaxies | 666 | 5.162 × 1013 | 1.852 × 1014 | |
| Diffuse gas | ... | ... | 1.481 × 1015 | |
| LC8 | Star-forming galaxies | 1427 | 4.227 × 1013 | 1.657 × 1014 |
| Quenched galaxies | 665 | 5.142 × 1013 | 1.598 × 1014 | |
| Diffuse gas | ... | ... | 1.490 × 1015 | |
Notes. For the diffuse gas in the third line in each light-cone row, the last column (total gas mass) is calculated as the sum of masses of all the fuzz gas particles in the light cone. For either star-formation galaxies or quenched galaxies in the first or second line in each light-cone row, the total gas mass and the total stellar mass, respectively, are calculated as sums of all gas masses and stellar masses of subhalos located in a given light cone. Counting particles (belonging to subhalos) instead yields slightly lower values due to the boundary cut-off of the light cone.
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