[BMP2010] 2049 , the SIMBAD biblio

[BMP2010] 2049 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:44:29


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Title First 3 Authors
2006A&A...452..119O viz 3542 8 ESO imaging survey: infrared observations of CDF-S and HDF-S. OLSEN L.F., MIRALLES J.-M., DA COSTA L., et al.
2010A&A...512A..12B viz 15       D               1 4352 228 The Great Observatories Origins Deep Survey. VLT/VIMOS spectroscopy in the GOODS-South field: part II. BALESTRA I., MAINIERI V., POPESSO P., et al.
2010ApJ...719..425F 15       D               1 53 47 Ultra-deep mid-infrared spectroscopy of luminous infrared galaxies at z ∼ 1 and z ∼ 2. FADDA D., YAN L., LAGACHE G., et al.
2012MNRAS.423.1909P 92       D         F     4 37 22 The AGN content in luminous infrared galaxies at z ∼ 2 from a global SED analysis including Herschel data. POZZI F., VIGNALI C., GRUPPIONI C., et al.
2012ApJ...759..139K viz 15       D               1 158 148 GOODS-Herschel: impact of active galactic nuclei and star formation activity on infrared spectral energy distributions at high redshift. KIRKPATRICK A., POPE A., ALEXANDER D.M., et al.
2013ApJ...762..108L 15       D               1 32 23 The complex physics of dusty star-forming galaxies at high redshifts as revealed by Herschel and Spitzer. LO FARO B., FRANCESCHINI A., VACCARI M., et al.
2015MNRAS.447.3442L 94       D         F     4 40 3 Combining physical galaxy models with radio observations to constrain the SFRs of high-z dusty star-forming galaxies. LO FARO B., SILVA L., FRANCESCHINI A., et al.
2017MNRAS.472.1372L 80               F     1 24 74 Characterizing the UV-to-NIR shape of the dust attenuation curve of IR luminous galaxies up to z ∼ 2. LO FARO B., BUAT V., ROEHLLY Y., et al.
2020ApJ...892..119M 222       D     X         6 10 ~ Measuring the heating and cooling of the interstellar medium at high redshift: PAH and [C II] observations of the same star-forming galaxies at z ∼ 2. McKINNEY J., POPE A., ARMUS L., et al.
2023ApJ...955..136M 148       D     X         4 18 ~ The IR Compactness of Dusty Galaxies Sets Star Formation and Dust Properties at z ∼ 0-2. McKINNEY J., POPE A., KIRKPATRICK A., et al.

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