{"arxiv_id":"1704.05556","incoming":{"papers":4,"sentences":7,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":2,"quotes":[{"arxiv_id":"1906.04274","title":"Lyman-alpha in the GJ 1132 System: Stellar Emission and Planetary Atmospheric Evolution","url":"/paper/1906.04274","section":"Spectrum Reconstruction","sentence":"By integrating the reconstructed emission profile, we find a Ly$α$ flux of 2.88$^+0.42_-0.31$x10$^-14$ erg s$^-1$ cm$^-2$ which gives f[Ly$α$]/f[bol] = 2.9$±$0.4x10$^-5$, where we have calculated the bolometric luminosity of GJ 1132b as: [equation] Where values for the T$_eff$ and R$_*$ were taken from [ref] and the distance to the star is taken from [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1906.04274","title":"Lyman-alpha in the GJ 1132 System: Stellar Emission and Planetary Atmospheric Evolution","url":"/paper/1906.04274","section":"Introduction","sentence":"The recent discoveries of terrestrial planets orbiting nearby M dwarfs [ref] provide us with the first opportunity to study small terrestrial planets outside our solar system, and observatories such as the Hubble Space Telescope allow us to analyze the atmospheres of these rocky exoplanets.","intent_p":0.9,"contests_p":null}]}],"unlabelled_sentences":4},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":{"arxiv_id":"1704.05556","kind":"model","paper_version":1,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T19:55:42+00:00","loaded_at":"2026-10-28T01:03:38.279680+00:00","evidence":"substantial","account":[],"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"entries":[{"p":0.89,"quote":null,"citing":[{"self":false,"year":2018,"title":"The independent discovery of planet candidates around low mass stars and astrophysical false positives from the first two TESS sectors","arxiv_id":"1812.08145"}],"verified":true,"paraphrase":"Followed this paper's use of GP regression modelling for radial velocity activity mitigation, initializing lnλ to ln3P_GP."}],"papers_all":2,"self_papers":0,"self_entries":[]},{"kind":"data_used","label":"Uses its data or values","papers":1,"entries":[],"papers_all":15,"self_papers":1,"self_entries":[{"p":1.0,"quote":null,"citing":[{"self":true,"year":2019,"title":"Lyman-alpha in the GJ 1132 System: Stellar Emission and Planetary Atmospheric Evolution","arxiv_id":"1906.04274"}],"verified":true,"paraphrase":"Took the distance to the star from this paper when calculating the bolometric luminosity of GJ 1132b."}]},{"kind":"comparison","label":"Compares with it","papers":1,"entries":[],"papers_all":4,"self_papers":1,"self_entries":[{"p":0.92,"quote":null,"citing":[{"self":true,"year":2018,"title":"A second terrestrial planet orbiting the nearby M dwarf LHS 1140","arxiv_id":"1808.00485"}],"verified":true,"paraphrase":"Noted that its own density for planet b decreased from the value reported by this paper, mostly due to a 21% increase in the planetary radius."}]}],"counts":{"by_kind":{"data_used":15,"comparison":4,"method_or_tool":2},"dropped":{"relied_on":0,"unknown_ids":0,"account_lines":0,"contest_vetoed":0,"below_threshold":0,"contest_drawback":0,"contest_without_basis":0,"contest_not_one_sentence":0,"contest_on_group_citation":0},"papers_read":12,"self_papers":23,"citing_papers":71,"sentences_read":17,"citing_sentences":106,"unambiguous_read":17,"typed_independent":14,"independent_papers":48,"by_kind_independent":{"data_used":11,"comparison":2,"method_or_tool":1}},"input_sha256":"22a8b3973f1871cce2ae3081697aad3b0bf02a5f9f16949a915d0c432a61f64e","method":"For a paper with five or more citing arXiv papers, Pith selected up to 40 citing sentences its citation classifier typed, read those whose citation markers point at this paper alone, and wrote one paraphrase for each later paper in each group, each resting on one sentence. A later paper is listed under a label only when the classifier gives one of its sentences that label at intent probability 0.8 or more (0.95 for support), Pith's reading of the sentence finds that the citing paper itself did it, and a second check of the paraphrase against the sentence passes. The section lists uses only: building on the paper, using its method, tool, data or values, comparing with it and citing it as support. It does not list criticism or disagreement, so their absence says nothing about how the paper has been received. Code counted the papers, wrote the summary from the listed entries, set the evidence level and linked each entry to its citing paper. Quotes are copied from the citing sentence and shown only when the citing paper's licence is CC BY, CC BY-SA or CC0; otherwise the paraphrase is shown. Papers that share an author with this one are listed apart. A paper with fewer citing papers gets a line counted by code, which names uses only: a later paper whose only label is a contest is counted as not described.","line":null,"summary":"1 later paper by other authors is listed below: 1 used its method or tool. 2 more papers by the same authors are listed: 1 used its data or values and 1 compared its own results with it."},"_links":{"html":"https://pith.science/paper/1704.05556"}}