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[LDM2003] GRB J065349.4+791619 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST16:35:09 |
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...400..499L | 2 | 38 | 257 | Are the hosts of gamma-ray bursts sub-luminous and blue galaxies? | LE FLOC'H E., DUC P.-A., MIRABEL I.F., et al. | ||||
2004ApJ...614...84B | 45 | 15 | The galaxy density environment of gamma-ray burst host galaxies. | BORNANCINI C.G., MARTINEZ H.J., LAMBAS D.G., et al. | |||||
2005ApJ...633...29C | 62 | 71 | Gamma-ray burst-selected high-redshift galaxies: comparison to field galaxy populations to z ∼ 3. | CONSELICE C.J., VREESWIJK P.M., FRUCHTER A.S., et al. | |||||
2005ApJ...634.1155X | 62 | 5 | Testing gamma-ray burst jet structure with the distribution of gamma-ray energy release. | XU L., WU X.F. and DAI Z.G. | |||||
2006ApJ...642..636L | 43 | 76 | Probing cosmic star formation using long gamma-ray bursts: new constraints from the Spitzer Space Telescope. | LE FLOC'H E., CHARMANDARIS V., FORREST W.J., et al. | |||||
2007ApJ...657..367W | 74 | 96 | A morphological study of gamma-ray burst host galaxies. | WAINWRIGHT C., BERGER E. and PENPRASE B.E. | |||||
2007ApJ...659.1431E | 42 | 8 | A revised estimate of the CO J=1-0 emission from the host galaxy of GRB 030329 using the Nobeyama Millimeter Array. | ENDO A., KOHNO K., HATSUKADE B., et al. | |||||
2008A&A...481..319W | 38 | X | 1 | 19 | 16 | Spectroscopy and multiband photometry of the afterglow of intermediate duration γ-rayburst GRB040924 and its host galaxy. | WIERSEMA K., VAN DER HORST A.J., KANN D.A., et al. | ||
2009ApJ...691..182S | 93 | D | F | 83 | 394 | The galaxy population hosting gamma-ray bursts. | SAVAGLIO S., GLAZEBROOK K. and LE BORGNE D. | ||
2016A&A...595A..72M | 161 | C F | 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. |