2007/03/13 by M. Janson, Markus Janson, Wolfgang Brandner +24 · 4 citations
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/516632
published as Astron.J.133:2442-2456,2007 · 40 pages, 20 figures, accepted for publication in AJ
arxiv created 2007/03/13 · openalex publication_date 2007/04/11 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31
The active K2 V star Eri hosts the nearest known extrasolar planet. With an angular separation of about 1'' on average, and an age of a few to several hundred megayears, Eri b is one of the prime candidates for becoming the first definitive extrasolar planet imaged directly. We present a multiepoch deep differential imaging survey performed with NACO-SDI at the VLT with the aim of finding the planet. The results are combined with recent astrometry in an attempt to further constrain the detection limits. No convincing candidate is found among the many coherent structures that constitute the residual speckle noise, which is the dominant noise at small angular scales. We present our detection limits, compare them with the estimated brightness of Eri b, and analyze how the limits can be improved further. It is found that integration time remains a very important parameter for achieving good results, even in the speckle-dominated regimes. The results yield new, improved 3 σ upper limits on the absolute H -band (1.6 μm) brightness of the 1.55 M Jup companion of 19.1-19.5 mag, depending on the specific age of the system.