Table A.2.
Properties of each quasar and extended Lyα emission.
| ID | z (a) |
z (b) |
(c) |
(d) |
Area(e) | Δvgauss(f) | Δvm1(g) | FWHMgauss(h) | Δλm2(i) |
|---|---|---|---|---|---|---|---|---|---|
| 1042 erg s−1 Å−1 | 1042 erg s−1 | arcsec2 | km s−1 | km s−1 | km s−1 | km s−1 | |||
| 62 | 3.043 | 3.043 | 1.47±0.07 | 5.22±0.52 | 6±1 | 16±75 | 50±81 | 1421±176 | 587±63 |
| 63 | 3.137 | ... | 3.63±0.09 | ... | ... | ... | ... | ... | ... |
| 64 | 3.058 | 3.053 | 2.43±0.08 | 8.89±0.55 | 10±1 | -105±27 | -13±28 | 776±65 | 262±31 |
| 65 | 3.031 | 3.031 | 4.85±0.07 | 23.52±0.90 | 22±2 | 24±30 | 26±22 | 1044±73 | 415±16 |
| 66 | 3.143 | 3.145 | 6.96±0.09 | 44.31±1.13 | 45±5 | 32±24 | 85±16 | 1070±56 | 427±13 |
| 67 | 3.138 | 3.136 | 6.75±0.09 | 17.99±0.93 | 18±2 | 51±43 | 31±42 | 1424±100 | 565±34 |
| 68 | 3.059 | 3.059 | 12.05±0.07 | 58.92±0.96 | 42±4 | 147±11 | 175±8 | 828±28 | 344±6 |
| 69 | 3.148 | 3.146 | 4.37±0.09 | 23.07±1.06 | 20±2 | -50±60 | -81±44 | 1671±142 | 749±29 |
| 70 | 3.145 | 3.142 | 4.93±0.08 | 15.38±0.67 | 15±2 | 31±22 | 70±21 | 859±53 | 365±15 |
| 71 | 3.186 | 3.201 | 5.38±0.09 | 34.79±1.45 | 30±3 | 721±58 | 675±46 | 1937±137 | 800±36 |
| 72 | 3.105 | ... | 1.22±0.07 | ... | ... | ... | ... | ... | ... |
| 73 | 3.081 | 3.07 | 2.29±0.07 | 32.89±1.36 | 35±4 | -510±45 | -470±39 | 1637±106 | 628±32 |
| 74 | 3.182 | 3.184 | 3.41±0.08 | 23.87±1.13 | 26±3 | 156±46 | 213±40 | 1478±108 | 598±29 |
| 75 | 2.996 | 2.994 | 8.47±0.08 | 44.71±1.05 | 30±3 | 95±23 | 129±13 | 963±54 | 401±9 |
| 76 | 3.193 | 3.196 | 17.93±0.1 | 17.54±1.02 | 12±1 | 389±46 | 423±49 | 1588±116 | 655±36 |
| 77 | 3.113 | 3.111 | 3.93±0.08 | 33.50±0.93 | 27±3 | -60±18 | -83±16 | 1031±42 | 437±12 |
| 78 | 3.092 | 3.098 | 2.32±0.07 | 19.18±1.15 | 12±1 | 409±98 | 388±68 | 1984±232 | 858±46 |
| 79 | 3.156 | 3.149 | 8.87±0.08 | 23.38±0.75 | 20±2 | -232±16 | -286±15 | 849±38 | 359±10 |
| 80 | 3.028 | 3.023 | 24.28±0.1 | 74.65±1.29 | 49±5 | -235±11 | -210±7 | 765±27 | 306±5 |
| 81 | 3.026 | 3.027 | 2.93±0.07 | 16.61±0.48 | 16±2 | -262±7 | -272±7 | 395±17 | 154±6 |
| 82 | 3.042 | ... | 0.74±0.15 | ... | ... | ... | ... | ... | ... |
| 83 | 3.091 | 3.091 | 4.99±0.08 | 19.04±0.97 | 15±2 | 177±41 | 185±42 | 1460±97 | 630±30 |
| 84 | 3.046 | 3.045 | 3.83±0.08 | 23.46±0.90 | 22±2 | -64±26 | -62±23 | 1037±60 | 427±16 |
| 85 | 3.139 | ... | 2.58±0.08 | ... | ... | ... | ... | ... | ... |
| 86 | 3.189 | 3.191 | 7.46±0.09 | 38.1±1.46 | 37±4 | 154±52 | 152±35 | 1648±122 | 696±23 |
| 87 | 3.146 | 3.159 | 3.47±0.07 | 12.18±0.78 | 12±1 | 742±92 | 793±70 | 1956±216 | 788±52 |
| 88 | 3.035 | 3.029 | 2.46±0.07 | 12.85±0.77 | 16±2 | -374±52 | -416±44 | 1316±122 | 535±31 |
| 89 | 3.143 | 3.152 | 2.9±0.08 | 5.63±0.51 | 8±1 | 467±54 | 493±58 | 1101±129 | 420±51 |
| 90 | 3.043 | 3.044 | 8.64±0.09 | 34.51±1.18 | 33±3 | 105±21 | 125±19 | 946±49 | 418±12 |
| 91 | 3.045 | ... | 5.73±0.08 | ... | ... | ... | ... | ... | ... |
| 92 | 3.115 | 3.112 | 5.31±0.08 | 14.78±0.81 | 16±2 | -40±39 | -47±38 | 1246±93 | 556±25 |
| 93 | 3.046 | ... | 0.51±0.06 | ... | ... | ... | ... | ... | ... |
| 94 | 3.178 | 3.181 | 5.75±0.08 | 20.42±0.88 | 21±2 | 89±24 | 97±28 | 1113±57 | 449±20 |
| 95 | 3.024 | ... | 1.96±0.08 | ... | ... | ... | ... | ... | ... |
| 96 | 3.118 | 3.12 | 8.57±0.08 | 73.94±1.44 | 49±5 | -71±17 | -91±13 | 1203±41 | 477±10 |
| 97 | 3.092 | 3.096 | 7.41±0.08 | 14.47±0.77 | 17±2 | 221±32 | 275±31 | 1074±78 | 394±27 |
| 98 | 3.074 | 3.077 | 4.26±0.07 | 22.24±1.02 | 17±2 | 1±48 | 30±46 | 1762±113 | 749±30 |
| 99 | 3.105 | 3.106 | 3.95±0.08 | 11.72±0.76 | 10±1 | 203±67 | 215±61 | 1631±156 | 720±40 |
| 100 | 3.059 | 3.06 | 2.57±0.09 | 8.17±0.65 | 7±1 | 179±56 | 278±61 | 1310±132 | 507±55 |
| 101 | 3.084 | 3.078 | 7.25±0.08 | 26.66±1.24 | 25±3 | -233±54 | -287±50 | 1873±129 | 648±47 |
| 102 | 3.193 | 3.197 | 8.22±0.10 | 44.26±1.23 | 35±3 | 42±15 | 21±14 | 918±35 | 370±11 |
| 103 | 3.01 | 3.002 | 9.43±0.08 | 32.57±1.28 | 22±2 | -23±73 | 97±46 | 2028±172 | 756±37 |
| 104 | 3.14 | 3.143 | 12.58±0.09 | 43.01±1.27 | 28±3 | 36±29 | 3±23 | 1439±68 | 634±16 |
| 105 | 3.188 | 3.188 | 3.4±0.08 | 22.51±1.02 | 19±2 | 138±46 | 223±39 | 1500±108 | 623±30 |
| 106 | 3.181 | 3.18 | 2.99±0.07 | 5.38±0.47 | 8±1 | 111±57 | 145±57 | 1152±136 | 382±58 |
| 107 | 3.086 | 3.083 | 5.97±0.08 | 15.08±0.88 | 18±2 | -109±54 | -158±54 | 1617±129 | 623±45 |
| 108 | 3.092 | 3.092 | 5.77±0.09 | 30.23±1.23 | 26±3 | -141±43 | -157±37 | 1606±102 | 618±29 |
| 109 | 3.076 | 3.077 | 5.19±0.08 | 29.45±1.22 | 27±3 | 60±54 | 180±44 | 1805±127 | 751±32 |
| 110 | 3.098 | ... | 1.76±0.07 | ... | ... | ... | ... | ... | ... |
| 111 | 3.043 | 3.045 | 3.91±0.07 | 6.47±0.55 | 9±1 | 171±62 | 154±56 | 1151±146 | 372±65 |
| 112 | 3.101 | 3.103 | 4.35±0.08 | 38.03±1.20 | 41±4 | 212±24 | 217±19 | 1033±57 | 440±12 |
| 113 | 3.105 | 3.108 | 4.58±0.10 | 39.69±1.66 | 34±3 | 48±42 | 33±41 | 1719±99 | 699±31 |
| 114 | 3.148 | ... | 2.50±0.07 | ... | ... | ... | ... | ... | ... |
| 115 | 3.116 | 3.116 | 3.25±0.07 | 12.71±0.49 | 12±1 | -83±12 | -97±12 | 567±28 | 240±9 |
| 116 | 3.069 | 3.069 | 8.03±0.08 | 22.27±1.00 | 19±2 | 14±42 | -18±40 | 1591±100 | 650±30 |
| 117 | 3.186 | 3.186 | 2.40±0.08 | 30.33±1.19 | 34±3 | 67±37 | 60±33 | 1444±86 | 575±25 |
| 118 | 3.108 | ... | 2.18±0.08 | ... | ... | ... | ... | ... | ... |
| 119 | 3.176 | 3.175 | 2.87±0.08 | 19.03±0.82 | 22±2 | -11±23 | 2±22 | 874±53 | 356±17 |
| 120 | 3.407 | 3.406 | 2.81±0.08 | 3.56±0.31 | 4±0 | 94±26 | 113±32 | 648±63 | 255±27 |
Notes.
Redshift of the observed Lyα peak in a quasar spectrum integrated within an aperture of radius 1.5 arcsec centered at the quasar location. The intrinsic uncertainty on this value is Δz ∼ 0.001.
Redshift of the observed Lyα peak in the spectrum integrated within the 2σ isophote of the nebular emission.
Observed peak Lyα luminosity density of the integrated quasar spectrum.
Integrated Lyα luminosity within the nebular 2σ isophote.
Area within the nebular 2σ isophote.
Velocity shift between the quasar Lyα redshift and the Gaussian centroid of the nebular Lyα line.
Velocity shift between the quasar Lyα redshift and the flux weighted first moment of the nebular Lyα line.
FWHM of the Gaussian fit to the nebular Lyα line. The reported values are not corrected for instrumental broadening.
Flux weighted second moment of the nebular Lyα line.
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