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| REBELS-P7 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:20:48 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2022ApJ...928...31S | 19 | D | 2 | 18 | 48 | Significant Dust-obscured Star Formation in Luminous Lyman-break Galaxies at z ∼ 7-8. | SCHOUWS S., STEFANON M., BOUWENS R., et al. | ||
2022MNRAS.515.3126I 
|
400 | D | X F | 9 | 55 | 45 | The ALMA REBELS Survey: dust continuum detections at z > 6.5. | INAMI H., ALGERA H.S.B., SCHOUWS S., et al. | |
| 2023MNRAS.518.6142A | 87 | F | 1 | 47 | 27 | The ALMA REBELS survey: the dust-obscured cosmic star formation rate density at redshift 7. | ALGERA H.S.B., INAMI H., OESCH P.A., et al. | ||
| 2023ApJ...954..103S | 409 | D | X C | 9 | 32 | ~ | ALMA as a Redshift Machine: Using [C II] to Efficiently Confirm Galaxies in the Epoch of Reionization. | SCHOUWS S., BOUWENS R., SMIT R., et al. | |
| 2024MNRAS.527...10V | 1496 | D | X C F | 32 | 8 | ~ | Spatially resolved Kennicutt-Schmidt relation at z ≈ 7 and its connection with the interstellar medium properties. | VALLINI L., WITSTOK J., SOMMOVIGO L., et al. | |
| 2024MNRAS.527.5808B | 18 | D | 1 | 63 | ~ | The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z= 4-8 revealed by the IRX-β and M⋆ relations. | BOWLER R.A.A., INAMI H., SOMMOVIGO L., et al. | ||
| 2024MNRAS.527.6867A | 18 | D | 1 | 21 | ~ | Cold dust and low [O III]/[C II] ratios: an evolved star-forming population at redshift 7. | ALGERA H.S.B., INAMI H., SOMMOVIGO L., et al. | ||
| 2024MNRAS.528..499L | 18 | D | 1 | 192 | ~ | [C II] 158 μm emission as an indicator of galaxy star formation rate. | LIANG L., FELDMANN R., MURRAY N., et al. | ||
| 2024ApJ...971..161M | 18 | D | 2 | 39 | ~ | SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution. | MITSUHASHI I., HARIKANE Y., BAUER F.E., et al. | ||
| 2025ApJ...980..138H | 19 | D | 1 | 68 | ~ | JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe. | HARIKANE Y., INOUE A.K., ELLIS R.S., et al. |
