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| COSMOS2015 776817 , the SIMBAD biblio (13 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:33:13 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2021MNRAS.502.6044E | 18 | D | 3 | 36 | 52 | MMT spectroscopy of Lyman-alpha at z ≃ 7: evidence for accelerated reionization around massive galaxies. | ENDSLEY R., STARK D.P., CHARLOT S., et al. | ||
| 2022MNRAS.511.6042E | 189 | D | X | 5 | 12 | 27 | Strong Lyman-α emission in an overdense region at z = 6.8: a very large (R ∼ 3 physical Mpc) ionized bubble in COSMOS? | ENDSLEY R. and STARK D.P. | |
| 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.515.1751W | 1040 | D | X C F | 23 | 13 | 25 | Dual constraints with ALMA: new [O III] 88-μm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z ∼ 7. | WITSTOK J., SMIT R., MAIOLINO R., et al. | |
|
2022MNRAS.515.3126I |
17 | D | 3 | 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 | 453 | D | X C | 10 | 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 | 1138 | D | X C F | 24 | 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.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. | ||
| 2025ApJ...989..147G | 47 | X | 1 | 9 | ~ | Metallicity Gradients in Modern Cosmological Simulations. I. Tension between Smooth Stellar Feedback Models and Observations. | GARCIA A.M., TORREY P., BHAGWAT A., et al. |