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| PSR J1844+0115 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST15:06:08 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012ApJ...757...90C | 496 | K A | D | X C | 13 | 17 | 16 | Four highly dispersed millisecond pulsars discovered in the Arecibo PALFA galactic plane survey. | CRAWFORD F., STOVALL K., 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. | ||
|
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. | ||
| 2017ApJ...834..137L | 16 | D | 1 | 75 | 11 | Timing of 29 pulsars discovered in the PALFA survey. | LYNE A.G., STAPPERS B.W., BOGDANOV S., et al. | ||
| 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. | ||
|
2019ApJ...879...10A |
16 | D | 1 | 225 | 87 | Searches for gravitational waves from known pulsars at two harmonics in 2015-2017 LIGO data. | ABBOTT B.P., ABBOTT R., ABBOTT T.D., 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. | ||
| 2022MNRAS.510.6011W | 17 | D | 1 | 53 | 15 | Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white dwarfs. | WANG B., LIU D. and CHEN H. | ||
|
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. | ||
| 2024MNRAS.532.2196W | 18 | D | 1 | 49 | ~ | Formation of millisecond pulsars with wide orbits. | WANG B., LIU D., GUO Y., 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. |