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| PSR J1835-0115 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:23:47 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2009MNRAS.395..410E | 128 | D | X F | 3 | 7 | 22 | An interference removal technique for radio pulsar searches. | EATOUGH R.P., KEANE E.F. and LYNE A.G. | |
| 2013MNRAS.431..292E | 323 | D | S X C | 7 | 26 | 14 | A coherent acceleration search of the Parkes multibeam pulsar survey - techniques and the discovery and timing of 16 pulsars. | EATOUGH R.P., KRAMER M., LYNE A.G., et al. | |
| 2014MNRAS.437.2217S | 15 | D | 1 | 84 | 15 | The nature of millisecond pulsars with helium white dwarf companions. | SMEDLEY S.L., TOUT C.A., FERRARIO L., et al. | ||
| 2014MNRAS.439.2033G | 15 | D | 1 | 77 | 17 | On the non-detection of γ-rays from energetic millisecond pulsars - dependence on viewing geometry. | GUILLEMOT L. and TAURIS T.M. | ||
| 2015MNRAS.450.2185L | 16 | D | 1 | 55 | 33 | The Parkes multibeam pulsar survey - VII. Timing of four millisecond pulsars and the underlying spin-period distribution of the Galactic millisecond pulsar population. | LORIMER D.R., ESPOSITO P., MANCHESTER R.N., et al. | ||
|
2015BaltA..24..395M |
16 | D | 1 | 619 | 2 | Binary star DataBase: binaries discovered in non-optical bands. | MALKOV O.Y., TESSEMA S.B. and KNIAZEV A.Y. | ||
| 2018ApJ...864...30H | 16 | D | 1 | 89 | 2 | On the orbital properties of millisecond pulsar binaries. | HUI C.Y., WU K., HAN Q., et al. | ||
|
2021ApJS..255....5A |
17 | D | 1 | 977 | ~ | The CHIME pulsar project: system overview. | AMIRI M., BANDURA K.M., BOYLE P.J., et al. | ||
|
2023RAA....23j4002W |
17 | D | 1 | 530 | ~ | FAST Pulsar Database. I. Polarization Profiles of 682 Pulsars. | WANG P.F., HAN J.L., XU J., et al. | ||
| 2025ApJ...992..116M | 19 | D | 1 | 181 | ~ | Irradiated Pulsar Planets and Companions as 511 keV Positron Annihilation Line Sources. | METZLER Z. and WADIASINGH Z. |