PSR J2129+1210G , the SIMBAD biblio

PSR J2129+1210G , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST18:36:07


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Title First 3 Authors
1993ApJS...88..529T viz 547 865 Catalog of 558 pulsars. TAYLOR J.H., MANCHESTER R.N. and LYNE A.G.
1996MmSAI..67..239Z 113 0 X-ray binaries. ZIOLKOWSKI J.
1996ARep...40..390M 41 0 The angle between the magnetic moment and rotation axis in millisecond pulsars. MALOV I.F.
1997PAZh...23..725A 53 ~ Are the pulsars actually born rarely or have low luminosities? ALLAKHVERDIEV A.O., GUSEINOV O.K. and TAGIEVA S.O.
1997ARep...41...56M viz 236 3 Cluster analysis of pulsar parameters. MALOV I.F. and MALOV O.I.
1998ApJ...508...74A 2 28 171 The COBE diffuse infrared background experiment search for the cosmic infrared background. III. Separation of galactic emission from the infrared sky brightness. ARENDT R.G., ODEGARD N., WEILAND J.L., et al.
2002ARep...46..451K viz 542 2 A comparative analysis of the integrated radio luminosities of normal and millisecond pulsars. KUZ'MIN A.D.
2007ApJ...670..363H 15       D               1 73 87 A 1.4 GHz Arecibo survey for pulsars in globular clusters. HESSELS J.W.T., RANSOM S.M., STAIRS I.H., et al.
2011MNRAS.417.1444M 77             C       1 202 13 On the pulse-width statistics in radio pulsars – II. Importance of the core profile components. MACIESIAK K. and GIL J.
2011MNRAS.418..477B 15       D               1 132 31 Luminosities of recycled radio pulsars in globular clusters. BAGCHI M., LORIMER D.R. and CHENNAMANGALAM J.
2014A&A...565A..43K 18 5 Precision astrometry of pulsars and other compact radio sources in the globular cluster M15. KIRSTEN F., VLEMMINGS W., FREIRE P., et al.
2021ApJS..255....5A viz 17       D               1 977 ~ The CHIME pulsar project: system overview. AMIRI M., BANDURA K.M., BOYLE P.J., et al.
2021RAA....21..185Q 174           X         4 16 ~ Spatial modulation search applied to the search and confirmation of highly scintillated pulsars at FAST with a pulsar discovered in M3. QIAN L. and PAN Z.-C.

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