<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"><channel><title>DPR Institute: research notes</title><description>Independent research in physics, electronics, chemistry, astronomy, and sustainability. Questions, methods, data, code, and results from DPR Institute, a working name for Derifield Physical Sciences Research.</description><link>https://dprinstitute.org/</link><language>en-gb</language><item><title>Two real single-transit fits, and why they are not a timing result</title><link>https://dprinstitute.org/notes/2026/two-real-single-transit-fits/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/two-real-single-transit-fits/</guid><description>KELT-11 b and HD 209458 b fits with the published period fixed, plus the full-sector cross-check that disagrees at the formal precision.</description><pubDate>Sun, 25 Oct 2026 00:00:00 GMT</pubDate><category>exoplanets</category><category>transit-timing</category><category>light-curves</category><category>astronomy-methods</category></item><item><title>Aperture diagnostics on the real sector 56 product set</title><link>https://dprinstitute.org/notes/2026/aperture-diagnostics/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/aperture-diagnostics/</guid><description>A threshold aperture run on the HD 209458 b target pixel file, compared with the mission SAP and PDCSAP columns on one common quality mask.</description><pubDate>Sat, 24 Oct 2026 00:00:00 GMT</pubDate><category>light-curves</category><category>astronomy-methods</category><category>open-science</category></item><item><title>The archive selection rule, and how 598 rows became 304 docket rows</title><link>https://dprinstitute.org/notes/2026/archive-selection-rule/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/archive-selection-rule/</guid><description>A fixed four-gate rule applied to a public confirmed-planet table, with the counts, the one-sided docket flag, and the limits recorded.</description><pubDate>Sat, 24 Oct 2026 00:00:00 GMT</pubDate><category>exoplanets</category><category>transit-timing</category><category>astronomy-methods</category></item><item><title>One real product set: HD 209458 b, sector 56</title><link>https://dprinstitute.org/notes/2026/hd-209458b-sector-56/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/hd-209458b-sector-56/</guid><description>The SPOC 120 s light curve and target pixel file for HD 209458 b, with archive URLs, byte counts, and SHA-256 digests. Acquisition record only.</description><pubDate>Sat, 24 Oct 2026 00:00:00 GMT</pubDate><category>exoplanets</category><category>light-curves</category><category>open-science</category></item><item><title>Injection-recovery: what twelve synthetic transits can and cannot show</title><link>https://dprinstitute.org/notes/2026/injection-recovery/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/injection-recovery/</guid><description>Twelve injected mid-transit times recovered on synthetic light curves. The timing bias is small against the pre-declared gate, but the sample is too small to calibrate a real pipeline.</description><pubDate>Sat, 24 Oct 2026 00:00:00 GMT</pubDate><category>transit-timing</category><category>astronomy-methods</category><category>reproducibility</category></item><item><title>A toy transit fit: what the trapezoid recovers on synthetic data</title><link>https://dprinstitute.org/notes/2026/synthetic-transit-fit/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/synthetic-transit-fit/</guid><description>A seeded synthetic light curve fitted with a trapezoid model. The recovered parameters agree with the injected values within about two reported sigma.</description><pubDate>Sat, 24 Oct 2026 00:00:00 GMT</pubDate><category>exoplanets</category><category>transit-timing</category><category>scientific-computing</category></item><item><title>Window QC on the sector 56 light curve</title><link>https://dprinstitute.org/notes/2026/window-qc/</link><guid isPermaLink="true">https://dprinstitute.org/notes/2026/window-qc/</guid><description>Cadence coverage, background, and centroid summaries for eight predicted transit windows in the HD 209458 b sector 56 light curve. Descriptive only.</description><pubDate>Sat, 24 Oct 2026 00:00:00 GMT</pubDate><category>light-curves</category><category>astronomy-methods</category><category>reproducibility</category></item></channel></rss>