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XROM and RCOM: Two New OGLE-III Real Time Data Analysis Systems

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arxiv 0810.2244 v1 pith:GGCX7UL2 submitted 2008-10-13 astro-ph

classification astro-ph
keywords realtimeogle-iiircomsystemsxromanalysisdata
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We describe two new OGLE-III real time data analysis systems: XROM and RCOM. The XROM system has been designed to provide continuous real time photometric monitoring of the optical counterparts of X-ray sources while RCOM system provides real time photometry of R Coronae Borealis variable stars located in the OGLE-III fields. Both systems can be used for triggering follow-up observations in crucial phases of variability episodes of monitored objects.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Comprehensive Study of the Dust Declines in R Coronae Borealis Stars

    astro-ph.SR 2024-12 conditional novelty 6.0 of 10

    Using 1536 dust declines across 162 RCB stars, the study finds cooler stars decline more often and presents evidence that R CrB and SU Tau fade randomly while RY Sgr's fades cluster near pulsation periods.

  2. Broadband study of the Be X-ray binary RX J0520.5-6932 during its outburst in 2024

    astro-ph.HE 2024-12 conditional novelty 5.0 of 10

    The 2024 outburst of RX J0520.5-6932 shows a cyclotron line at 32.2 keV, a revised orbital period of 24.39 days, and a pulsed-fraction decrease at 15 keV, a first for an extragalactic source.

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