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| ACO 535 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:28:57 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1971ApJS...23..371S | 2711 | 51 | Rectangular coordinates of rich clusters of galaxies on the Palomar Sky Survey charts. | SASTRY G.N. and ROOD H.J. | |||||
|
1987ApJS...63..555S |
2712 | 116 | A catalog of morphological properties of the 2712 Abell clusters. | STRUBLE M.F. and ROOD H.J. | |||||
|
1989ApJS...70....1A |
5256 | 1561 | A catalog of rich clusters of galaxies. | ABELL G.O., CORWIN H.G.Jr and OLOWIN R.P. | |||||
|
2004A&A...425..367B |
15 | D | 1 | 461 | 528 | The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy cluster survey. V. The cluster catalogue. | BOEHRINGER H., SCHUECKER P., GUZZO L., et al. | ||
| 2010ApJ...708..403M | 16 | D | 1 | 6 | 12 | Absolute timing of the Crab pulsar with the INTEGRAL/SPI telescope. | MOLKOV S., JOURDAIN E. and ROQUES J.P. | ||
| 2010MNRAS.406.1773M | 76 | C | 1 | 137 | 300 | The observed growth of massive galaxy clusters - II. X-ray scaling relations. | MANTZ A., ALLEN S.W., EBELING H., et al. | ||
|
2011A&A...534A.109P |
15 | D | 1 | 1770 | 422 | The MCXC: a meta-catalogue of X-ray detected clusters of galaxies. | PIFFARETTI R., ARNAUD M., PRATT G.W., et al. | ||
|
2012MNRAS.425..477N |
15 | D | 1 | 1762 | 27 | γ-rays from annihilating dark matter in galaxy clusters: stacking versus single source analysis. | NEZRI E., WHITE R., COMBET C., et al. | ||
|
2017MNRAS.468.3322S |
16 | D | 1 | 28164 | 37 | CoMaLit - V. Mass forecasting with proxies: method and application to weak lensing calibrated samples. | SERENO M. and ETTORI S. | ||
|
2022A&A...658A..59X |
17 | D | 1 | 852 | 3 | Catalog of X-ray-selected extended galaxy clusters from the ROSAT All-Sky Survey (RXGCC). | XU W., RAMOS-CEJA M.E., PACAUD F., et al. | ||
| 2023MNRAS.526.2506L | 87 | F | 1 | 26 | ~ | Ultraluminous X-ray sources are beamed. | LASOTA J.-P. and KING A. |