Fig. 2 from Rossi X‐Ray Timing Explorer Absolute Timing Results for the Pulsars B1821−24 and B1509−58

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Rossi X‐Ray Timing Explorer Absolute Timing Results for the Pulsars B1821−24 and B1509−58

Authors: A. H. Rots, K. Jahoda, D. J. Macomb, N. Kawai, Y. Saito, V. M. Kaspi, A. G. Lyne, R. N. Manchester, D. C. Backer, A. L. Somer, D. Marsden, and R. E. Rothschild

Rots et al. 1998 The Astrophysical Journal 501 749.

Provider: AAS Journals

Caption: Fig. 2.

PSR B1821−24. Light curves based on (a) RXTE PCA (2–16 keV), and (b) Green Bank radio (800 MHz) observations, using timing ephemeris B1821−24G. The RXTE light curve is labeled in counts per second per bin (at 100 bins per period) with 1 σ errors indicated. The radio pulse components are identified by means of the same numbering as Backer & Sallmen (1997).

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