Inside the bubble: exploring the environments of reionisation-era Lyman-$α$ emitting galaxies with JADES and FRESCO

Fuente: arXiv
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Autori principali: Witstok, Joris, Smit, Renske, Saxena, Aayush, Jones, Gareth C., Helton, Jakob M., Sun, Fengwu, Maiolino, Roberto, Kumari, Nimisha, Stark, Daniel P., Bunker, Andrew J., Arribas, Santiago, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Cameron, Alex J., Carniani, Stefano, Charlot, Stephane, Chevallard, Jacopo, Curti, Mirko, Curtis-Lake, Emma, Eisenstein, Daniel J., Endsley, Ryan, Hainline, Kevin, Ji, Zhiyuan, Johnson, Benjamin D., Looser, Tobias J., Nelson, Erica, Perna, Michele, Rix, Hans-Walter, Robertson, Brant E., Sandles, Lester, Scholtz, Jan, Simmonds, Charlotte, Tacchella, Sandro, Übler, Hannah, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris
Natura: Preprint
Pubblicazione: 2023
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author Witstok, Joris
Smit, Renske
Saxena, Aayush
Jones, Gareth C.
Helton, Jakob M.
Sun, Fengwu
Maiolino, Roberto
Kumari, Nimisha
Stark, Daniel P.
Bunker, Andrew J.
Arribas, Santiago
Baker, William M.
Bhatawdekar, Rachana
Boyett, Kristan
Cameron, Alex J.
Carniani, Stefano
Charlot, Stephane
Chevallard, Jacopo
Curti, Mirko
Curtis-Lake, Emma
Eisenstein, Daniel J.
Endsley, Ryan
Hainline, Kevin
Ji, Zhiyuan
Johnson, Benjamin D.
Looser, Tobias J.
Nelson, Erica
Perna, Michele
Rix, Hans-Walter
Robertson, Brant E.
Sandles, Lester
Scholtz, Jan
Simmonds, Charlotte
Tacchella, Sandro
Übler, Hannah
Williams, Christina C.
Willmer, Christopher N. A.
Willott, Chris
author_facet Witstok, Joris
Smit, Renske
Saxena, Aayush
Jones, Gareth C.
Helton, Jakob M.
Sun, Fengwu
Maiolino, Roberto
Kumari, Nimisha
Stark, Daniel P.
Bunker, Andrew J.
Arribas, Santiago
Baker, William M.
Bhatawdekar, Rachana
Boyett, Kristan
Cameron, Alex J.
Carniani, Stefano
Charlot, Stephane
Chevallard, Jacopo
Curti, Mirko
Curtis-Lake, Emma
Eisenstein, Daniel J.
Endsley, Ryan
Hainline, Kevin
Ji, Zhiyuan
Johnson, Benjamin D.
Looser, Tobias J.
Nelson, Erica
Perna, Michele
Rix, Hans-Walter
Robertson, Brant E.
Sandles, Lester
Scholtz, Jan
Simmonds, Charlotte
Tacchella, Sandro
Übler, Hannah
Williams, Christina C.
Willmer, Christopher N. A.
Willott, Chris
contents We present a study of the environments of 17 Lyman-$α$ (Ly$α$) emitting galaxies (LAEs) in the reionisation era ($5.8 < z < 8$) identified by JWST/NIRSpec as part of the JWST Advanced Deep Extragalactic Survey (JADES). Unless situated in sufficiently (re)ionised regions, Ly$α$ emission from these galaxies would be strongly absorbed by neutral gas in the intergalactic medium (IGM). We conservatively estimate sizes of the ionised regions required to reconcile the relatively low Ly$α$ velocity offsets ($Δv_\text{Ly$α$}<300\,\mathrm{km\,s^{-1}}$) with moderately high Ly$α$ escape fractions ($f_\mathrm{esc,\,Lyα}>5\%$) observed in our sample of LAEs, suggesting the presence of ionised hydrogen along the line of sight towards at least eight out of 17 LAEs. We find minimum physical `bubble' sizes of the order of $R_\text{ion}\sim0.1$-$1\,\mathrm{pMpc}$ are required in a patchy reionisation scenario where ionised bubbles containing the LAEs are embedded in a fully neutral IGM. Around half of the LAEs in our sample are found to coincide with large-scale galaxy overdensities seen in FRESCO at $z \sim 5.8$-$5.9$ and $z\sim7.3$, suggesting Ly$α$ transmission is strongly enhanced in such overdense regions, and underlining the importance of LAEs as tracers of the first large-scale ionised bubbles. Considering only spectroscopically confirmed galaxies, we find our sample of UV-faint LAEs ($M_\text{UV}\gtrsim-20\,\mathrm{mag}$) and their direct neighbours are generally not able to produce the required ionised regions based on the Ly$α$ transmission properties, suggesting lower-luminosity sources likely play an important role in carving out these bubbles. These observations demonstrate the combined power of JWST multi-object and slitless spectroscopy in acquiring a unique view of the early Universe during cosmic reionisation via the most distant LAEs.
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id arxiv_https___arxiv_org_abs_2306_04627
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Inside the bubble: exploring the environments of reionisation-era Lyman-$α$ emitting galaxies with JADES and FRESCO
Witstok, Joris
Smit, Renske
Saxena, Aayush
Jones, Gareth C.
Helton, Jakob M.
Sun, Fengwu
Maiolino, Roberto
Kumari, Nimisha
Stark, Daniel P.
Bunker, Andrew J.
Arribas, Santiago
Baker, William M.
Bhatawdekar, Rachana
Boyett, Kristan
Cameron, Alex J.
Carniani, Stefano
Charlot, Stephane
Chevallard, Jacopo
Curti, Mirko
Curtis-Lake, Emma
Eisenstein, Daniel J.
Endsley, Ryan
Hainline, Kevin
Ji, Zhiyuan
Johnson, Benjamin D.
Looser, Tobias J.
Nelson, Erica
Perna, Michele
Rix, Hans-Walter
Robertson, Brant E.
Sandles, Lester
Scholtz, Jan
Simmonds, Charlotte
Tacchella, Sandro
Übler, Hannah
Williams, Christina C.
Willmer, Christopher N. A.
Willott, Chris
Astrophysics of Galaxies
We present a study of the environments of 17 Lyman-$α$ (Ly$α$) emitting galaxies (LAEs) in the reionisation era ($5.8 < z < 8$) identified by JWST/NIRSpec as part of the JWST Advanced Deep Extragalactic Survey (JADES). Unless situated in sufficiently (re)ionised regions, Ly$α$ emission from these galaxies would be strongly absorbed by neutral gas in the intergalactic medium (IGM). We conservatively estimate sizes of the ionised regions required to reconcile the relatively low Ly$α$ velocity offsets ($Δv_\text{Ly$α$}<300\,\mathrm{km\,s^{-1}}$) with moderately high Ly$α$ escape fractions ($f_\mathrm{esc,\,Lyα}>5\%$) observed in our sample of LAEs, suggesting the presence of ionised hydrogen along the line of sight towards at least eight out of 17 LAEs. We find minimum physical `bubble' sizes of the order of $R_\text{ion}\sim0.1$-$1\,\mathrm{pMpc}$ are required in a patchy reionisation scenario where ionised bubbles containing the LAEs are embedded in a fully neutral IGM. Around half of the LAEs in our sample are found to coincide with large-scale galaxy overdensities seen in FRESCO at $z \sim 5.8$-$5.9$ and $z\sim7.3$, suggesting Ly$α$ transmission is strongly enhanced in such overdense regions, and underlining the importance of LAEs as tracers of the first large-scale ionised bubbles. Considering only spectroscopically confirmed galaxies, we find our sample of UV-faint LAEs ($M_\text{UV}\gtrsim-20\,\mathrm{mag}$) and their direct neighbours are generally not able to produce the required ionised regions based on the Ly$α$ transmission properties, suggesting lower-luminosity sources likely play an important role in carving out these bubbles. These observations demonstrate the combined power of JWST multi-object and slitless spectroscopy in acquiring a unique view of the early Universe during cosmic reionisation via the most distant LAEs.
title Inside the bubble: exploring the environments of reionisation-era Lyman-$α$ emitting galaxies with JADES and FRESCO
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2306.04627