Matches in SemOpenAlex for { <https://semopenalex.org/work/W3149212074> ?p ?o ?g. }
- W3149212074 endingPage "1869" @default.
- W3149212074 startingPage "1853" @default.
- W3149212074 abstract "The mean free path of ionizing photons, $lambda_{rm mfp}$, is a key factor in the photoionization of the intergalactic medium (IGM). At $z gtrsim 5$, however, $lambda_{rm mfp}$ may be short enough that measurements towards QSOs are biased by the QSO proximity effect. We present new direct measurements of $lambda_{rm mfp}$ that address this bias and extend up to $z sim 6$ for the first time. Our measurements at $z sim 5$ are based on data from the Giant Gemini GMOS survey and new Keck LRIS observations of low-luminosity QSOs. At $z sim 6$ we use QSO spectra from Keck ESI and VLT X-Shooter. We measure $lambda_{rm mfp} = 9.09^{+1.62}_{-1.28}$ proper Mpc and $0.75^{+0.65}_{-0.45}$ proper Mpc (68% confidence) at $z = 5.1$ and 6.0, respectively. The results at $z = 5.1$ are consistent with existing measurements, suggesting that bias from the proximity effect is minor at this redshift. At $z = 6.0$, however, we find that neglecting the proximity effect biases the result high by a factor of two or more. Our measurement at $z = 6.0$ falls well below extrapolations from lower redshifts, indicating rapid evolution in $lambda_{rm mfp}$ over $5 < z < 6$. This evolution disfavors models in which reionization ended early enough that the IGM had time to fully relax hydrodynamically by $z = 6$, but is qualitatively consistent with models wherein reionization completed at $z = 6$ or even significantly later. Our mean free path results are most consistent with late reionization models wherein the IGM is still 20% neutral at $z=6$, although our measurement at $z = 6.0$ is even lower than these models prefer." @default.
- W3149212074 created "2021-04-13" @default.
- W3149212074 creator A5012920561 @default.
- W3149212074 creator A5016892258 @default.
- W3149212074 creator A5048295002 @default.
- W3149212074 creator A5059662714 @default.
- W3149212074 creator A5068565883 @default.
- W3149212074 creator A5082299044 @default.
- W3149212074 date "2021-09-21" @default.
- W3149212074 modified "2023-10-15" @default.
- W3149212074 title "The mean free path of ionizing photons at 5 < <i>z</i> < 6: evidence for rapid evolution near reionization" @default.
- W3149212074 cites W1848567999 @default.
- W3149212074 cites W1975627161 @default.
- W3149212074 cites W1983716874 @default.
- W3149212074 cites W1984797436 @default.
- W3149212074 cites W1985198043 @default.
- W3149212074 cites W1985328401 @default.
- W3149212074 cites W1993138845 @default.
- W3149212074 cites W1995453045 @default.
- W3149212074 cites W1996447018 @default.
- W3149212074 cites W2005411300 @default.
- W3149212074 cites W2006553744 @default.
- W3149212074 cites W2008204335 @default.
- W3149212074 cites W2015423217 @default.
- W3149212074 cites W2024914408 @default.
- W3149212074 cites W2025549670 @default.
- W3149212074 cites W2033911211 @default.
- W3149212074 cites W2042749826 @default.
- W3149212074 cites W2044093857 @default.
- W3149212074 cites W2054801391 @default.
- W3149212074 cites W2056718431 @default.
- W3149212074 cites W2062919088 @default.
- W3149212074 cites W2073762506 @default.
- W3149212074 cites W2078522449 @default.
- W3149212074 cites W2079716425 @default.
- W3149212074 cites W2102747712 @default.
- W3149212074 cites W2103453948 @default.
- W3149212074 cites W2106758945 @default.
- W3149212074 cites W2109614102 @default.
- W3149212074 cites W2112028701 @default.
- W3149212074 cites W2170086864 @default.
- W3149212074 cites W2171262111 @default.
- W3149212074 cites W2259243443 @default.
- W3149212074 cites W2325917856 @default.
- W3149212074 cites W2332784587 @default.
- W3149212074 cites W2370208167 @default.
- W3149212074 cites W2415069146 @default.
- W3149212074 cites W2507062171 @default.
- W3149212074 cites W2569199829 @default.
- W3149212074 cites W2610513321 @default.
- W3149212074 cites W2736471281 @default.
- W3149212074 cites W2750305088 @default.
- W3149212074 cites W2766974034 @default.
- W3149212074 cites W2774444386 @default.
- W3149212074 cites W2787977416 @default.
- W3149212074 cites W2801870339 @default.
- W3149212074 cites W2811351692 @default.
- W3149212074 cites W2890475738 @default.
- W3149212074 cites W2951178208 @default.
- W3149212074 cites W2955186154 @default.
- W3149212074 cites W2969413580 @default.
- W3149212074 cites W2979864507 @default.
- W3149212074 cites W2982243028 @default.
- W3149212074 cites W2989175718 @default.
- W3149212074 cites W2994716021 @default.
- W3149212074 cites W2997882247 @default.
- W3149212074 cites W3003722324 @default.
- W3149212074 cites W3088318530 @default.
- W3149212074 cites W3098519065 @default.
- W3149212074 cites W3098965552 @default.
- W3149212074 cites W3099532244 @default.
- W3149212074 cites W3100038651 @default.
- W3149212074 cites W3100048804 @default.
- W3149212074 cites W3100765228 @default.
- W3149212074 cites W3101667439 @default.
- W3149212074 cites W3102758673 @default.
- W3149212074 cites W3102834201 @default.
- W3149212074 cites W3103121943 @default.
- W3149212074 cites W3103442925 @default.
- W3149212074 cites W3103511866 @default.
- W3149212074 cites W3103732358 @default.
- W3149212074 cites W3104305918 @default.
- W3149212074 cites W3105127634 @default.
- W3149212074 cites W3105816966 @default.
- W3149212074 cites W3108004685 @default.
- W3149212074 cites W3109170567 @default.
- W3149212074 cites W3124389704 @default.
- W3149212074 cites W3124621509 @default.
- W3149212074 cites W3125688855 @default.
- W3149212074 cites W3125944961 @default.
- W3149212074 cites W3195413215 @default.
- W3149212074 cites W4288079944 @default.
- W3149212074 doi "https://doi.org/10.1093/mnras/stab2696" @default.
- W3149212074 hasPublicationYear "2021" @default.
- W3149212074 type Work @default.
- W3149212074 sameAs 3149212074 @default.
- W3149212074 citedByCount "59" @default.
- W3149212074 countsByYear W31492120742021 @default.