Table 4.
Compilation of key parameters of LAE LF studies from the literature in the redshift range probed by MW.
| Reference | Method* |
 |
z | Area | Volume | logLLyα, lim |
 |
 |
|---|---|---|---|---|---|---|---|---|
| (Å) | (deg2) | (Mpc3) | log (erg s−1) | |||||
| Ouchi et al. (2008) | SC/NB503 | 64 | 3.1 ± 0.03 | 0.983 | 7 × 105 | 42.0 | 356 | 41 |
| … | SC/NB570 | 44 | 3.7 ± 0.03 | 0.965 | 6.1 × 105 | 42.6 | 101 | 26 |
| … | SC/NB816 | 27 | 5.7 ± 0.05 | 1.033 | 9.2 × 105 | 42.5 | 401 | 17 |
| Grove et al. (2009) | FORS2/3NB | 25 | 2.85/3.15/3.25 | 0.037 | 1.4 × 104 | 41.5 | 83 | 59 |
| Cassata et al. (2011) | VIMOS | – | 2 − 6.6 | 0.62/0.16† | – | 41.0 | 84†† | 153†† |
| Matthee et al. (2017) | INT/NB501 | 12 | 3.06 ≤ z ≤ 3.17 | 0.7 | 7.2 × 105 | 43.0 | 32 | 5 |
| Sobral et al. (2018a) | SC/IA464-527♯ | 50 | 3.1 ± 0.4 | ≈2 | 17.3 × 106 | 42.5 | 2146 | ?‡ |
| … | SC/IA574,624 | 50 | 3.9 ± 0.3 | ≈2 | 10.1 × 106 | 42.95 | 240 | ?‡ |
| … | SC/IA679,709 | 50 | 4.7 ± 0.2 | ≈2 | 10.6 × 106 | 43.1 | 160 | ?‡ |
| … | SC/IA738-827♮ | 50 | 5.4 ± 0.5 | ≈2 | 15.5 × 106 | 43.3 | 147 | ?‡ |
| … | SC4K/global | 50 | ∼2.5 − 6 | ≈2 | ∼108 | 42.5 | 3434 | 112‡ |
| Drake et al. (2017b) | MUSE/HUDF | – | 3.5 ± 0.5 | 7 × 10−7 | 3.1 × 104 | 41.0 | – | 193 |
| … | … | – | 4.5 ± 0.5 | 7 × 10−7 | 2.6 × 104 | 41.0 | – | 144 |
| … | … | – | 5.8 ± 0.8 | 7 × 10−7 | 3.6 × 104 | 41.0 | – | 50 |
| … | … | – | 2.91 − 6.64 | 7 × 10−7 | 9.3 × 104 | 41.0 | – | 387 |
| Drake et al. (2017a) | MUSE/HDFS | – | 2.91 − 6.64 | 8 × 10−8 | 1 × 104 | 41.4 | – | 59 |
| Dawson et al. (2007) | 4m/5NB | 15 | 4.4 ± 0.1 | 2 × 10−4 | 1.5 × 104 | 42.0 | 97 | 79 |
| Shioya et al. (2009) | SC/NB711 | 12 | 4.86 ± 0.03 | 1.83 | 1.1 × 106 | 42.8 | 79 | 0 |
| Konno et al. (2018) | HSC/NB816 | 10 | 5.73 ± 0.05 | 13.8 | 1.2 × 107 | 42.9 | 1077 | 49 |
| Shimasaku et al. (2006) | SC/NB816 | 10 | 5.7 ± 0.05 | 0.2 | 1.8 × 105 | 42.5 | 89 | 39 |
| Santos et al. (2016) | SC/NB816 | 25 | 5.7 ± 0.05 | 7 | 6 × 106 | 42.4 | 514 | 46 |
| Henry et al. (2012) | IMACS/NB+slits | – | 5.7 ± 0.1 | 0.015 | 1.5 × 104 | 42.1 | 105‡‡ | 6 |
| Bina et al. (2016) | MUSE/Abell1689 | – | 2.91 − 6.64 | 8 × 10−8 | 900♭ | 40.5 | – | 17 |
Notes.( * )Legend for abbreviations: SC/X=Subaru Suprime-Cam with filter X; HSC/NB816=Subaru Hyper Suprime-Cam with NB816 filter; FORS2/3NB=ESO VLT/FORS2 – 3 fields, with three different narrow-band filters; VIMOS=ESO VLT/VIMOS multi-slit spectroscopic survey; INT/NB501= Wide-Field Camera with NB501 filter at Isaac Newton 2.5 m Telescope; MUSE/HUDF=MUSE Hubble Ultra Deep Field; MUSE/HDFS=MUSE Hubble Deep Field South; 4m/5NB=5 overlapping narrow-band filters on two 4m class telescopes; IMACS/NB+slits=Multi-slit narrow-band spectroscopic search with IMACS on the Baade telescope (see also Martin et al. 2008); MUSE/Abel1689=MUSE observations of the lensing cluster Abell 1689. ( * *)Number of photometrically selected LAE candidates (Nphot) and number of spectroscopic confirmations (Nspec). ( † )Area of the imaging campaign (VIMOS Deep Survey/VIMOS Ultra Deep Survey) from which targets were pre-selected for VIMOS multi-slit spectroscopy. ( † †)Here Nphot refers to the number of photometrically pre-selected LAEs, while Nspec indicates the number of serendipitously detected sources. ( ‡ )Spectroscopic confirmations only reported for the combined SC4K sample. ( ‡ ‡)Single unresolved emission line objects without continuum detections (see also Martin et al. 2008). (♯)IA464, IA484, IA505, and IA527 medium-band filters. (♮)IA738, IA767, and IA827 medium-band filters. (♭)Effective comoving volume from lensing magnification.
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