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BOW ACO 370 CC055 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST14:13:31 |
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 |
---|---|---|---|---|---|---|---|---|---|
1988A&AS...73..471S | 86 | 33 | Spectroscopic observations of the distant cluster of galaxies Abell 370 : a catalogue of 84 spectra. | SOUCAIL G., MELLIER Y., FORT B., et al. | |||||
1988MNRAS.230..249M | 135 | 63 | Spectral energy distributions of galaxies in high-redshift clusters. III. Abell 370 at z=0.37. | MacLAREN I., ELLIS R.S. and COUCH W.J. | |||||
1994ApJ...430..121C | 81 | 227 | Morphological studies of the galaxy populations in distant "Butcher-Oemler" clusters with HST. I. AC 114 at z = 0.31 and Abell 370 at z = 0.37. | COUCH W.J., ELLIS R.S., SHARPLES R.M., et al. | |||||
1995ApJ...450..512S | 324 | 130 | Evolution of infrared-selected galaxies in z about 0.4 clusters. | STANFORD S.A., EISENHARDT P.R.M. and DICKINSON M. | |||||
2016ApJ...833..178V | 16 | D | 1 | 172 | 15 | The Grism Lens-Amplified Survey from Space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3 <= z <= 0.7. | VULCANI B., TREU T., SCHMIDT K.B., et al. | ||
2019MNRAS.485.3738L | 17 | D | 1 | 565 | 57 | Probing 3D structure with a large MUSE mosaic: extending the mass model of Frontier Field Abell 370. | LAGATTUTA D.J., RICHARD J., BAUER F.E., et al. | ||
2021A&A...646A..83R | 17 | D | 1 | 3710 | 61 | An atlas of MUSE observations towards twelve massive lensing clusters. | RICHARD J., CLAEYSSENS A., LAGATTUTA D., et al. | ||
2022ApJ...925....4M | 376 | D | X C | 8 | 43 | 17 | Observing Ram Pressure at Work in Intermediate Redshift Clusters with MUSE: The Case of Abell 2744 and Abell 370. | MORETTI A., RADOVICH M., POGGIANTI B.M., et al. | |
2022ApJ...937...18B | 90 | F | 1 | 22 | 3 | Locations and Morphologies of Jellyfish Galaxies in A2744 and A370. | BELLHOUSE C., POGGIANTI B., MORETTI A., et al. |