AGC 332347 , the SIMBAD biblio

AGC 332347 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST14:13:34

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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
2003A&A...397..463U viz 52 21 The Hamburg/SAO Survey for low metallicity blue compact/HII galaxies (HSS-LM). I. The first list of 46 strong-lined galaxies. UGRYUMOV A.V., ENGELS D., PUSTILNIK S.A., et al.
2012MNRAS.423..197B viz 15       D               1 114 103 MIPS 24–160 µm photometry for the Herschel-SPIRE local galaxies guaranteed time programs. BENDO G.J., GALLIANO F. and MADDEN S.C.
2013A&A...557A..95R 16       D               4 54 127 Revealing the cold dust in low-metallicity environments. I. Photometry analysis of the Dwarf Galaxy Survey with Herschel. REMY-RUYER A., MADDEN S.C., GALLIANO F., et al.
2014A&A...563A..31R 78             C       1 126 472 Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range. REMY-RUYER A., MADDEN S.C., GALLIANO F., et al.
2014A&A...568A..62D 54       D     X         2 468 300 The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. DE LOOZE I., CORMIER D., LEBOUTEILLER V., et al.
2013PASP..125..600M 16       D               5 66 182 An overview of the Dwarf Galaxy Survey. MADDEN S.C., REMY-RUYER A., GALAMETZ M., et al.
2014PASP..126.1079M 15       D               1 49 7 An overview of the Dwarf Galaxy Survey (PASP, 125, 600, [2013])-Corrigendum. MADDEN S.C., REMY-RUYER A., GALAMETZ M., et al.
2015A&A...578A..53C viz 17       D               2 63 177 The Herschel Dwarf Galaxy Survey. I. Properties of the low-metallicity ISM from PACS spectroscopy. CORMIER D., MADDEN S.C., LEBOUTEILLER V., et al.
2015A&A...582A.121R viz 328       D     X         9 109 127 Linking dust emission to fundamental properties in galaxies: the low-metallicity picture. REMY-RUYER A., MADDEN S.C., GALLIANO F., et al.
2016ApJS..226...19F viz 16       D               1 242 63 Far-infrared line spectra of active galaxies from the Herschel/PACS spectrometer: the complete database. FERNANDEZ-ONTIVEROS J.A., SPINOGLIO L., PEREIRA-SANTAELLA M., et al.
2017ApJ...846...68Q 16       D               1 84 1 The dependence of the IR-radio correlation on the metallicity. QIU J., SHI Y., WANG J., et al.
2019AJ....157...81O viz 16       D               1 393 ~ The Arecibo Pisces-Perseus Supercluster Survey. I. Harvesting ALFALFA. O'DONOGHUE A.A., HAYNES M.P., KOOPMANN R.A., et al.
2019A&A...626A..23C viz 42           X         1 47 74 The Herschel Dwarf Galaxy Survey. II. Physical conditions, origin of [C II] emission, and porosity of the multiphase low-metallicity ISM. CORMIER D., ABEL N.P., HONY S., et al.
2020A&A...637A..32B 16       D               1 50 30 Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10. BURGARELLA D., NANNI A., HIRASHITA H., et al.
2020A&A...641A.168N viz 16       D   O           2 48 34 The gas, metal, and dust evolution in low-metallicity local and high-redshift galaxies. NANNI A., BURGARELLA D., THEULE P., et al.
2021A&A...649A..18G viz 17       D               1 834 42 A nearby galaxy perspective on dust evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples. GALLIANO F., NERSESIAN A., BIANCHI S., et al.
2022A&A...667A..35R 400       D     X C       9 48 11 Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies. RAMAMBASON L., LEBOUTEILLER V., BIK A., et al.
2023A&A...677A..44R 17       D               2 30 ~ Star-formation-driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel. ROMANO M., NANNI A., DONEVSKI D., et al.
2024A&A...683L...9R 18       D               1 29 ~ Evidence of extended [CII] and dust emission in local dwarf galaxies. ROMANO M., DONEVSKI D., JUNAIS, et al.

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