ALMA survey of a massive node of the Cosmic Web at z~3. I. Discovery of a large overdensity of CO emitters
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| Main Authors: | , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866910292826390528 |
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| author | Pensabene, A. Cantalupo, S. Cicone, C. Decarli, R. Galbiati, M. Ginolfi, M. de Beer, S. Fossati, M. Fumagalli, M. Lazeyras, T. Pezzulli, G. Travascio, A. Wang, W. Matthee, J. Maseda, M. V. |
| author_facet | Pensabene, A. Cantalupo, S. Cicone, C. Decarli, R. Galbiati, M. Ginolfi, M. de Beer, S. Fossati, M. Fumagalli, M. Lazeyras, T. Pezzulli, G. Travascio, A. Wang, W. Matthee, J. Maseda, M. V. |
| contents | Sub-mm surveys toward overdense regions in the early Universe are essential to uncover the obscured star-formation and the cold gas content of assembling galaxies within massive dark matter halos. In this work, we present deep ALMA mosaic observations covering an area of $\sim 2'\times2'$ around MQN01 (MUSE Quasar Nebula 01), one of the largest and brightest Ly-$α$ emitting nebulae discovered thus far surrounding a radio-quiet quasar at $z\simeq3.25$. Our observations target the 1.2- and the 3-mm dust continuum, as well as the carbon monoxide CO(4-3) transition in galaxies in the vicinity of the quasar. We identify a robust sample of eleven CO line-emitting galaxies (including a closely-separated quasar companion) which lie within $\pm 4000\,{\rm km\,s^{-1}}$ relatively to the quasar systemic redshift. A fraction of these objects are missed in previous deep rest-frame optical/UV surveys thus highlighting the critical role of (sub-)mm imaging. We also detect a total of eleven sources revealed in their 1.2-mm dust continuum with six of them having either high-fidelity spectroscopic redshift information from rest-frame UV metal absorptions, or CO line which place them in the same narrow redshift range. A comparison of the CO luminosity function (LF) and 1.2-mm number count density with that of the general fields points to a galaxy overdensity of $δ> 10$. We find evidence of a systematic flattening at the bright-end of the CO LF with respect to the trend measured in blank fields. Our findings reveal that galaxies in dense regions at $z\sim3$ are more massive and significantly richer in molecular gas than galaxies in fields, hence enabling a faster and accelerated assembly. This is the first of a series of studies to characterize one of the densest regions of the Universe found so far at $z > 3$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_04765 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | ALMA survey of a massive node of the Cosmic Web at z~3. I. Discovery of a large overdensity of CO emitters Pensabene, A. Cantalupo, S. Cicone, C. Decarli, R. Galbiati, M. Ginolfi, M. de Beer, S. Fossati, M. Fumagalli, M. Lazeyras, T. Pezzulli, G. Travascio, A. Wang, W. Matthee, J. Maseda, M. V. Astrophysics of Galaxies Sub-mm surveys toward overdense regions in the early Universe are essential to uncover the obscured star-formation and the cold gas content of assembling galaxies within massive dark matter halos. In this work, we present deep ALMA mosaic observations covering an area of $\sim 2'\times2'$ around MQN01 (MUSE Quasar Nebula 01), one of the largest and brightest Ly-$α$ emitting nebulae discovered thus far surrounding a radio-quiet quasar at $z\simeq3.25$. Our observations target the 1.2- and the 3-mm dust continuum, as well as the carbon monoxide CO(4-3) transition in galaxies in the vicinity of the quasar. We identify a robust sample of eleven CO line-emitting galaxies (including a closely-separated quasar companion) which lie within $\pm 4000\,{\rm km\,s^{-1}}$ relatively to the quasar systemic redshift. A fraction of these objects are missed in previous deep rest-frame optical/UV surveys thus highlighting the critical role of (sub-)mm imaging. We also detect a total of eleven sources revealed in their 1.2-mm dust continuum with six of them having either high-fidelity spectroscopic redshift information from rest-frame UV metal absorptions, or CO line which place them in the same narrow redshift range. A comparison of the CO luminosity function (LF) and 1.2-mm number count density with that of the general fields points to a galaxy overdensity of $δ> 10$. We find evidence of a systematic flattening at the bright-end of the CO LF with respect to the trend measured in blank fields. Our findings reveal that galaxies in dense regions at $z\sim3$ are more massive and significantly richer in molecular gas than galaxies in fields, hence enabling a faster and accelerated assembly. This is the first of a series of studies to characterize one of the densest regions of the Universe found so far at $z > 3$. |
| title | ALMA survey of a massive node of the Cosmic Web at z~3. I. Discovery of a large overdensity of CO emitters |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2401.04765 |