My arXiv Library
A running log of papers I find relevant to my work, updated every few days. This is not a quality assessment — just a short note on what caught my attention. Inspired by M. Bustamante. Logging initiated on May 22, 2026.
September 2026
2 Sep
August 2026
28 Aug
21 Aug
19 Aug
11 Aug
7 Aug
5 Aug
July 2026
Note: I'm on vacation from July 1 until July 19 and won't be posting new papers in the meantime. I'll add them retroactively once I'm back.
30 Jul
Note: Interesting two papers; I am a bit confused about the framing of the headline result considering the fairly fragile tension (as described in the text). Need to read more carefully.
29 Jul
28 Jul
22 Jul
June 2026
25 Jun
16 Jun
15 Jun
12 Jun
10 Jun
5 Jun
Joint Multi-Period Fermi-LAT and LHAASO Constraints on Axion-Like Particles from Mrk 421 Using Profile Likelihood with Gaussian Copula Correlation
Why: Joint Fermi-LAT + LHAASO ALP constraints from Mrk 421---potentially methodologically interesting.
3 Jun
A New Record Census of Dwarf AGN and a Bimodal MBH–M★ Scaling Relation with DESI DR1
Why: Relevant for gamma-ray searches in dwarf AGN.
2 Jun
The Delta Resonance in the Neutrino Sky
Why: Proposes that the ~30 TeV break in IceCube's diffuse neutrino spectrum arises from the Δ-resonance in p–γ interactions, which would also lower the neutrino-source contribution to the isotropic gamma-ray background.
Possible High-Energy Neutrino Emission from Dark Matter Annihilation in the Disrupting Dwarf Galaxy Boötes III
Why: Candidate high-energy neutrino signal from dark matter annihilation in the disrupting dwarf Boötes III, with a post-trial significance of 3.1σ pointing to a ~26.5 TeV dark matter mass.
May 2026
29 May
Why: Fermi-LAT Collaboration 2017egm detection paper, following arXiv:2605.29897. My own work, arXiv:2604.16595, comes to similar conclusions on the engine parameters, though with a different approach to the time selection.
27 May
Why: LVK results / reference analysis / data products for the second part of the fourth observing run (O4b).
Strong Constraints on Millisecond Pulsar Injection Spectra from Fermi-LAT Observations of the Galactic Center
Why: The expected follow-up to arXiv:2605.22913 - with all the caveats from that paper.
Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey
Why: Keeping up with the state of evolving dark energy: full six-year DES combining SN + BAO + 3×2pt results in a 2.2σ deviation from ΛCDM from a single survey, rising to 3σ when combined with DESI DR2 BAO and CMB.
26 May
Electromagnetic Signatures From Primordial Black Holes in the Solar System
Why: Detection forecasts for signals from asteroid-mass PBH transits (AMEGO-X) and PBH explosions in the outer Solar System (HAWC, LHAASO, Fermi). Nice to see this mass window probed concretely --- have to read in more detail.
Legacy analysis of Milky Way dwarf spheroidal satellite galaxies: an update
Why: An update to McDaniel et al. (2024), stricter cuts, different source class, PS map modeling.
Why: An upgraded LAT analysis of the GCE across 9 IEMs that pushes residuals to ≲10% and finds a spherical gNFW (γ≈1.15) preferred over NB+BB bulge templates. At face value, interesting result.
I am curious about the iterative "find_sources" step, that (I think) is run with the NFW in place with extensions allowed up to 2 deg---these are comparable to the angular scales of the boxy bulge wings for example.
Why: A nice step toward 3D Galactic CR tomography beyond traditional ring analyses, though the physical interpretation of the 4–6 kpc enhancement remains assumption-dependent.