The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old: I. Survey overview and case studies

Herrera-Camus, R, González-López, J, Förster Schreiber, N ORCID: 0000-0003-4264-3381, Aravena, M ORCID: 0000-0002-6290-3198, De Looze, I, Spilker, J, Tadaki, K, Barcos-Muñoz, L, Assef, RJ ORCID: 0000-0002-9508-3667, Birkin, JE ORCID: 0000-0002-3272-7568, Bolatto, AD, Bouwens, R, Bovino, S, Bowler, RAA ORCID: 0000-0003-3917-1678, Calistro Rivera, G, Da Cunha, E, Davies, RI ORCID: 0000-0002-3324-4824, Davies, RL ORCID: 0000-0002-3324-4824, Díaz-Santos, T, Ferrara, A et al (2025) The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old: I. Survey overview and case studies. Astronomy & Astrophysics, 699. ISSN 0004-6361

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Abstract

We present the ALMA-CRISTAL survey, an ALMA Cycle 8 Large Program designed to investigate the physical properties of star-forming galaxies at 4 ≤ z ≤ 6 through spatially resolved, multiwavelength observations. This survey targets 19 star-forming main-sequence galaxies selected from the ALPINE survey, using ALMA Band 7 observations to study [CII] 158 μm line emission and dust continuum, complemented by JWST/NIRCam and HST imaging to map stellar and UV emission. The CRISTAL sample expanded to 39 after including newly detected galaxies in the CRISTAL fields, archival data, and pilot study targets. The resulting dataset provides a detailed view of gas, dust, and stellar structures on kiloparsec scales at the end of the era of reionization. The survey reveals diverse morphologies and kinematics, including rotating disks, merging systems, [CII] emission tails from potential interactions, and clumpy star formation. Notably, the [CII] emission in many cases extends beyond the stellar light seen in HST and JWST imaging. Scientific highlights include CRISTAL-10, exhibiting an extreme [CII] deficit similar to Arp 220, and CRISTAL-13, where feedback from young star-forming clumps likely causes an offset between the stellar clumps and the peaks of [CII] emission. CRISTAL galaxies exhibit global [CII]/FIR ratios that decrease with increasing FIR luminosity, similar to trends seen in local galaxies but shifted to higher luminosities, likely due to their higher molecular gas content. CRISTAL galaxies also span a previously unexplored range of global FIR surface brightness at high-redshift, showing that high-redshift galaxies can have elevated [CII]/FIR ratios. These elevated ratios are likely influenced by factors such as lower-metallicity gas, the presence of significant extraplanar gas, and contributions from shock-excited gas.

Item Type:	Article
Uncontrolled Keywords:	5101 Astronomical Sciences; 51 Physical Sciences; 0201 Astronomical and Space Sciences; Astronomy & Astrophysics; 5101 Astronomical sciences; 5107 Particle and high energy physics; 5109 Space sciences
Subjects:	Q Science > QB Astronomy Q Science > QC Physics
Divisions:	Astrophysics Research Institute
Publisher:	EDP Sciences
Date of acceptance:	1 April 2025
Date of first compliant Open Access:	27 August 2025
Date Deposited:	27 Aug 2025 14:57
Last Modified:	27 Aug 2025 15:00
DOI or ID number:	10.1051/0004-6361/202553896
URI:	https://researchonline.ljmu.ac.uk/id/eprint/27002

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