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| [FB2003] J232719.475+061555.95 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST06:15:04 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2003GCN..1842....1F | 2 | 4 | GRB 020819: afterglow candidate. | FRAIL D.A. and BERGER E. | |||||
| 2005ApJ...629...45J | 27 | 42 | The radio afterglow and host galaxy of the dark GRB 020819. | JAKOBSSON P., FRAIL D.A., FOX D.B., et al. | |||||
| 2008ApJ...676.1151T | 3 | 18 | 120 | Spatially resolved properties of the GRB 060505 host: implications for the nature of the progenitor. | THONE C.C., FYNBO J.P.U., OSTLIN G., et al. | ||||
| 2009ApJ...691..182S | 92 | D | F | 80 | 394 | The galaxy population hosting gamma-ray bursts. | SAVAGLIO S., GLAZEBROOK K. and LE BORGNE D. | ||
| 2010MNRAS.409L..74S | 13 | 18 | Low radio-derived star formation rates in z < 0.5 gamma-ray burst host galaxies. | STANWAY E.R., DAVIES L.J.M. and LEVAN A.J. | |||||
| 2014PASP..126....1L | 170 | D | X C | 4 | 42 | 23 | The host galaxies of long-duration gamma-ray bursts. | LEVESQUE E.M. | |
| 2014A&A...565A.112H | Z | 33 | 60 | New light on gamma-ray burst host galaxies with Herschel. | HUNT L.K., PALAZZI E., MICHALOWSKI M.J., et al. | ||||
| 2014Natur.510..247H | 4 | 4 | 32 | Two γ-ray bursts from dusty regions with little molecular gas. | HATSUKADE B., OHTA K., ENDO A., et al. | ||||
| 2016A&A...593A..17G | 16 | D | 1 | 115 | 8 | Probing dust-obscured star formation in the most massive gamma-ray burst host galaxies. | GREINER J., MICHALOWSKI M.J., KLOSE S., et al. | ||
| 2016A&A...595A..72M | 39 | C * | 2 | 65 | 22 | GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow. | MICHALOWSKI M.J., CASTRO CERON J.M., WARDLOW J.L., et al. | ||
| 2017MNRAS.466.2787C | 159 | X | 4 | 25 | 5 | Metallicities in long gamma-ray burst host galaxies at z < 0.5 calculated by the detailed modelling of optical and infrared line ratios. | CONTINI M. |
