{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.revision/1","content_sha256":"60ac5ce695aaf8979d0a211b98e380e21388aa0cf32b36b7eec3a80047a6d980","created":"2026-10-03T07:17:56Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":["5475cf5dc5b1a72283d26dc95dc6e00d7ea4e00096a7c6492e409a1816eeb011"],"salt":"a291e131afb79ab0c246beb1cb896bf0008cb9cfe24189f63e2844853a3cd40b","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"revision"},"content":{"answer_type":"value","assisted_by":[],"external_id":"astro.system-architectures.super-earth-cold-jupiter","kind":"well-posed","literature_status":"contested","n":"1","parents":[],"plain":"Whether stars with close-in super-Earths are more or less likely to also have a Jupiter-like planet far out tells whether giant planets help or block the formation of inner small planets. Different surveys disagree.","posed_since":"2018","precise":"Measure $P(\\mathrm{CJ}\\mid \\mathrm{SE})$, the occurrence of cold Jupiters (M sin i ~ 0.3-13 M_Jup, a ~ 1-10 AU) around hosts of inner super-Earths ($R = 1-4\\,R_{\\mathrm{earth}}, P < 100\\,\\mathrm{d}$), versus the field rate of about 10 percent. Zhu and Wu 2018 and Bryan et al. 2019 ($39 \\pm 7\\,\\mathrm{percent}$) report an excess of about three times, while Bonomo et al. 2023 (A&A 677, A33) find $9.3(+7.7,-2.9)\\,\\mathrm{percent}$ and no excess. The answer is $P(\\mathrm{CJ}\\mid \\mathrm{SE})$ with metallicity dependence and uncertainty sufficient to decide the excess.","problem_ref":null,"references":"","settled_by":"Long-baseline radial-velocity follow-up of a large, homogeneously selected sample of super-Earth hosts with metallicities matched to a control sample.","status_note":"Bonomo et al. 2023 found no excess, contradicting the 2018-2019 results; the difference may reflect sample metallicity or selection.","title":"Do inner super-Earths and outer cold Jupiters tend to occur together?","topic_ref":"705ebcb3477b591f7d0888a668b37821e2d427d0c8c498a50e19534d5adf0f6f"},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"03c9004886ff9250e10ade4a407fa1c24ffc5d131250344ef66c8da48c738132","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"abb1312efcdf526adaeccb299fe61cb042bec16f4b6e22e6d2c516d1fadec9b3","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"uSJNvCuytfNaIwgpxgDC5wFbtqXNzgskqRG3gCTq-9IznLPp-nsp9CUHuo_Whq1ffcgYJyyORc7x03eBB_WHCA"},"schema":"pubphys.envelope/1"},"record_hash":"03c9004886ff9250e10ade4a407fa1c24ffc5d131250344ef66c8da48c738132","leaf_index":635}