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<titleInfo><title>The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy</title></titleInfo>


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<name type="personal">
  <namePart type="given">Fuga</namePart>
  <namePart type="family">Komori</namePart>
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<name type="personal">
  <namePart type="given">Akio K</namePart>
  <namePart type="family">Inoue</namePart>
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  <namePart type="given">Ken</namePart>
  <namePart type="family">Mawatari</namePart>
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  <namePart type="given">Yuma</namePart>
  <namePart type="family">Sugahara</namePart>
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  <namePart type="given">Hideki</namePart>
  <namePart type="family">Umehata</namePart>
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<name type="personal">
  <namePart type="given">Rhythm</namePart>
  <namePart type="family">Shimakawa</namePart>
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  <namePart type="given">Satoshi</namePart>
  <namePart type="family">Yamanaka</namePart>
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<name type="personal">
  <namePart type="given">Takuya</namePart>
  <namePart type="family">Hashimoto</namePart>
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  <namePart type="given">Jorryt J</namePart>
  <namePart type="family">Matthee</namePart>
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  <namePart type="family">Misawa</namePart>
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<abstract lang="eng">The H i gas distribution in damped Lyman $\alpha$ absorbers (DLAs) has remained elusive due to the point-source nature of background quasar emission. Observing DLAs against spatially extended background galaxies provides a new method for constraining their size and structure. Using the Keck Cosmic Web Imager, we present the first ‘silhouette’ image of a DLA at $z=3.34$, identified in the spectrum of a background galaxy at $z=3.61$. Although the silhouette remains unresolved due to limited spatial resolution, this represents a successful proof-of-concept for studying DLA morphology using extended background sources. Possible residual emission in the DLA trough suggests an optical depth contrast exceeding $10^7$ in the internal structure, implying a sharp edge or patchy structure. A Lyman $\alpha$ emitter (LAE) at $z_{\rm LAE}=3.3433\pm 0.0005$, consistent with the DLA redshift, is detected at an angular separation of $1{{_{.}^{\prime\prime}} }73\pm 0{{_{.}^{\prime\prime}} }28$ ($12.9\pm 2.1$ kpc). The DLA is surrounded by three galaxies within 140 kpc in projected distance and 500 km s$^{-1}$ in line-of-sight velocity, indicating that it resides in the circumgalactic medium of the LAE or within a galaxy group/protocluster environment. An O i  $\lambda 1302$ absorption at $z_{\rm OI}=3.3288\pm 0.0004$ is also detected along the line of sight. This absorber may trace metal-enriched outflow from the LAE or a gas-rich galaxy exhibiting the highest star formation activity among the surrounding galaxies. Future large spectroscopic surveys of galaxies will expand such a DLA sample, and three-dimensional spectroscopy for it will shed new light on the role of intergalactic dense gas in galaxy formation and evolution.</abstract>

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<originInfo><publisher>Oxford University Press</publisher><dateIssued encoding="w3cdtf">2025</dateIssued>
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<relatedItem type="host"><titleInfo><title>Monthly Notices of the Royal Astronomical Society</title></titleInfo>
  <identifier type="issn">0035-8711</identifier>
  <identifier type="eIssn">1365-2966</identifier>
  <identifier type="ISI">001592326700001</identifier><identifier type="doi">10.1093/mnras/staf1622</identifier>
<part><detail type="volume"><number>543</number></detail><detail type="issue"><number>3</number></detail><extent unit="pages">2943-2957</extent>
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<chicago>Komori, Fuga, Akio K Inoue, Ken Mawatari, Yuma Sugahara, Hideki Umehata, Rhythm Shimakawa, Satoshi Yamanaka, Takuya Hashimoto, Jorryt J Matthee, and Toru Misawa. “The First Direct Imaging of the Silhouette of a Damped Lyman α System along the Line-of-Sight to a Background Galaxy.” &lt;i&gt;Monthly Notices of the Royal Astronomical Society&lt;/i&gt;. Oxford University Press, 2025. &lt;a href=&quot;https://doi.org/10.1093/mnras/staf1622&quot;&gt;https://doi.org/10.1093/mnras/staf1622&lt;/a&gt;.</chicago>
<short>F. Komori, A.K. Inoue, K. Mawatari, Y. Sugahara, H. Umehata, R. Shimakawa, S. Yamanaka, T. Hashimoto, J.J. Matthee, T. Misawa, Monthly Notices of the Royal Astronomical Society 543 (2025) 2943–2957.</short>
<apa>Komori, F., Inoue, A. K., Mawatari, K., Sugahara, Y., Umehata, H., Shimakawa, R., … Misawa, T. (2025). The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy. &lt;i&gt;Monthly Notices of the Royal Astronomical Society&lt;/i&gt;. Oxford University Press. &lt;a href=&quot;https://doi.org/10.1093/mnras/staf1622&quot;&gt;https://doi.org/10.1093/mnras/staf1622&lt;/a&gt;</apa>
<ista>Komori F, Inoue AK, Mawatari K, Sugahara Y, Umehata H, Shimakawa R, Yamanaka S, Hashimoto T, Matthee JJ, Misawa T. 2025. The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy. Monthly Notices of the Royal Astronomical Society. 543(3), 2943–2957.</ista>
<ama>Komori F, Inoue AK, Mawatari K, et al. The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy. &lt;i&gt;Monthly Notices of the Royal Astronomical Society&lt;/i&gt;. 2025;543(3):2943-2957. doi:&lt;a href=&quot;https://doi.org/10.1093/mnras/staf1622&quot;&gt;10.1093/mnras/staf1622&lt;/a&gt;</ama>
<ieee>F. Komori &lt;i&gt;et al.&lt;/i&gt;, “The first direct imaging of the silhouette of a damped Lyman α system along the line-of-sight to a background galaxy,” &lt;i&gt;Monthly Notices of the Royal Astronomical Society&lt;/i&gt;, vol. 543, no. 3. Oxford University Press, pp. 2943–2957, 2025.</ieee>
<mla>Komori, Fuga, et al. “The First Direct Imaging of the Silhouette of a Damped Lyman α System along the Line-of-Sight to a Background Galaxy.” &lt;i&gt;Monthly Notices of the Royal Astronomical Society&lt;/i&gt;, vol. 543, no. 3, Oxford University Press, 2025, pp. 2943–57, doi:&lt;a href=&quot;https://doi.org/10.1093/mnras/staf1622&quot;&gt;10.1093/mnras/staf1622&lt;/a&gt;.</mla>
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