IRAS F08390+0204 , the SIMBAD biblio

IRAS F08390+0204 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.13CEST06:10:24


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Title First 3 Authors
2009MNRAS.398..109W viz 15       D               1 50356 37 The imperial IRAS-FSC redshift catalogue. WANG L. and ROWAN-ROBINSON M.
2011MNRAS.413..971D viz 15       D               1 41769 860 Galaxy and mass assembly (GAMA): survey diagnostics and core data release. DRIVER S.P., HILL D.T., KELVIN L.S., et al.
2015MNRAS.449.2498I 16       D               4 37 12 A multiwavelength exploration of the [CII]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2. IBAR E., LARA-LOPEZ M.A., HERRERA-CAMUS R., et al.
2015MNRAS.452.2087L viz 16       D               1 71486 449 Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. LISKE J., BALDRY I.K., DRIVER S.P., et al.
2016MNRAS.456.2221D viz 16       D               1 117 13 H-ATLAS/GAMA: the nature and characteristics of optically red galaxies detected at submillimetre wavelengths. DARIUSH A., DIB S., HONY S., et al.
2017A&A...602A..49H 16       D               40 8 VALES. II. The physical conditions of interstellar gas in normal star-forming galaxies up to z = 0.2 revealed by ALMA. HUGHES T.M., IBAR E., VILLANUEVA V., et al.
2017MNRAS.470.3775V 97       D         F     2 68 26 VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35. VILLANUEVA V., IBAR E., HUGHES T.M., et al.
2018MNRAS.474.3875B viz 16       D               1 133171 163 Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3. BALDRY I.K., LISKE J., BROWN M.J.I., et al.
2020MNRAS.497.2771M 102       D     X         3 34 ~ VALES VI: ISM enrichment in star-forming galaxies up to z ∼ 0.2 using 12CO(1-0), 13CO(1-0), and C18O(1-0) line luminosity ratios. MENDEZ-HERNANDEZ H., IBAR E., KNUDSEN K.K., et al.
2022MNRAS.517..962D viz 18       D               1 385 17 Dust, CO, and [C I]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time. DUNNE L., MADDOX S.J., PAPADOPOULOS P.P., et al.

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