COSMOS Spectroscopic Redshift Compilation (First Data Release): 488,000 Redshifts Encompassing Two Decades of Spectroscopy
| dc.contributor.author | Vaccari, Mattia | |
| dc.contributor.author | Khostovan, Ali Ahmad | |
| dc.contributor.author | Kartaltepe, Jeyhan S. | |
| dc.date.accessioned | 2026-05-14T12:54:10Z | |
| dc.date.available | 2026-05-14T12:54:10Z | |
| dc.date.issued | 2025 | |
| dc.description.abstract | We present the COSMOS Spectroscopic Redshift Compilation encompassing ∼20 yr of spectroscopic redshifts within a 10 deg2 area centered on the 2 deg2 COSMOS legacy field. This compilation contains 487,666 redshifts of 266,284 unique objects from 138 individual programs up to z ∼ 8 with median stellar mass ∼108.4–1010 M⊙ (redshift dependent). Rest-frame NUVrJ colors and star formation rate–stellar mass correlations show that the compilation primarily contains low-to-intermediate-mass star-forming and massive, quiescent galaxies at z < 1.25 and mostly low-mass bursty star-forming galaxies at z > 2. Sources in the compilation cover a diverse range of environments, including protoclusters such as “Hyperion.” The full compilation is 50% spectroscopically complete by i ∼ 23.4 mag and Ks ∼ 21.6 mag; however, this is redshift dependent. Spatially, the compilation is >50% (>30%) complete within the central (outer) region limited to i < 24 mag and Ks < 22.5 mag, separately. We demonstrate how the compilation can be used to validate photometric redshifts and investigate calibration metrics. By training self-organizing maps on COSMOS2020/Classic and projecting the compilation onto it, we find key subpopulations currently lacking spectroscopic coverage, including z < 1 intermediate-mass quiescent and low-/intermediate-mass bursty star-forming galaxies, z ∼ 2 massive quiescent galaxies, and z > 3 massive star-forming galaxies. This highlights how combining self-organizing maps with our compilation can provide guidance for future spectroscopic observations to get a complete spectroscopic view of galaxy populations. Lastly, the compilation will undergo periodic data releases incorporating new spectroscopic redshifts and providing a lasting legacy resource for the community. | |
| dc.identifier.citation | Khostovan, A.A., Kartaltepe, J.S., Salvato, M., Ilbert, O., Casey, C.M., Algera, H., Antwi-Danso, J., Battisti, A., Brinch, M., Brusa, M. and Calabrò, A., 2026. COSMOS Spectroscopic Redshift Compilation (First Data Release): 488,000 Redshifts Encompassing Two Decades of Spectroscopy. The Astrophysical Journal Supplement Series, 282(1), p.6. | |
| dc.identifier.uri | https://doi.org/10.3847/1538-4365/ae1cb9 | |
| dc.identifier.uri | https://hdl.handle.net/10566/22444 | |
| dc.language.iso | en | |
| dc.publisher | American Astronomical Society | |
| dc.subject | Spectroscopic redshifts | |
| dc.subject | COSMOS field | |
| dc.subject | Galaxy populations | |
| dc.subject | Photometric redshift calibration | |
| dc.subject | Self-organizing maps | |
| dc.title | COSMOS Spectroscopic Redshift Compilation (First Data Release): 488,000 Redshifts Encompassing Two Decades of Spectroscopy | |
| dc.type | Article |