queue: file paper from #50

Author: github-actions[bot]

bibliography/pyautomemory.bib

@@ -16126,3 +16126,16 @@ @unpublished{Vincken2026
   year = {2026},
   note = {In preparation; arXiv ID, DOI and full author list TODO once public}
 }
+
+@article{Morgan2026,
+  archivePrefix = {arXiv},
+  arxivId = {2608.17041},
+  author = {Morgan, Christopher W. and Margeson, James B. and Garcia, Gilberto and Dai, Xinyu and Goicoechea, Luis J. and Shalyapin, Vyacheslav N. and Chartas, George},
+  doi = {10.48550/arXiv.2608.17041},
+  eprint = {2608.17041},
+  journal = {ApJ},
+  note = {Accepted for publication},
+  title = {{The X-Ray Continuum Emission Region in the Lensed Quasar SDSS J133907.23+131038.6 is Much Smaller than the Accretion Disk}},
+  url = {https://arxiv.org/abs/2608.17041},
+  year = {2026}
+}

reading-queue.md

@@ -17,7 +17,7 @@ PyAutoPaper, now PyAutoMemory — became the unified knowledge repo.)
 ---
 
 ## Strong Lensing
-The X-Ray Continuum Emission Region in the Lensed Quasar SDSS J133907.23+131038.6 is Much Smaller than the Accretion Disk
+DONE 2026-08-21 — The X-Ray Continuum Emission Region in the Lensed Quasar SDSS J133907.23+131038.6 is Much Smaller than the Accretion Disk
 Confirmation of the Finch Flatter-Fainter Relation for the Quadruple Images of Lensed Point Sources
 The Koi Pond: A Strongly Lensed Protocluster Core hosting a Diverse Population of DSFGs
 Addressing position anomalies in the Strong Gravitational Lensing System HS~0810+2554 through Dark Matter Subhalos

wiki/lensing/sources/microlensing-imf.md

@@ -24,6 +24,16 @@ status: drafted
 **Do not use for:**
 - The IMF of an individual lens galaxy or an IMF constraint independent of external priors.
 
+## Morgan et al. 2026 — SDSS J1339+1310 X-ray continuum size
+
+**Canonical BibTeX key:** `Morgan2026`
+**Reference:** arXiv:2608.17041; accepted ApJ
+
+Microlensing of the lensed quasar SDSS J133907.23+131038.6 gives a
+half-light size for the X-ray continuum emission region consistent with
+the ISCO in Schwarzschild geometry, and smaller than the far-UV
+(193 nm) accretion-disk size measured from the same monitoring.
+
 ## See also
 
 - [[microlensing-imf]]