{ "id": "2112.10030", "version": "v2", "published": "2021-12-19T00:12:07.000Z", "updated": "2022-03-07T20:54:46.000Z", "title": "A Stacking Survey of Gamma-ray Pulsars", "authors": [ "Yuzhe Song", "Timothy A. D. Paglione", "Joshua Tan", "Charles Lee-Georgescu" ], "comment": "Submitted to ApJ. Second revision. 15 pages, 11 figures, and 2 tables", "categories": [ "astro-ph.HE" ], "abstract": "We report on a likelihood stacking search for gamma-ray pulsars at 525 high latitude locations that coincide with known radio pulsar positions. We significantly detect a stacked signal over the background. Stacking their likelihood profiles in spectral parameter space implies a pulsar-like spectral index and a characteristic flux one order of magnitude below the Fermi-LAT sensitivity. The same procedures performed on empty control fields imply a false detection rate as much as 50\\%, although the stacked spectra of the control fields are distinctly softer than those of the pulsars. This study also probes a unique region of parameter space populated by older, transitional, and recycled (millisecond) pulsars. Many of these sources have lower rotational energy loss rates implying that the empirical gamma-ray \"death line\" could be predominantly a sensitivity limit. These new stacking results sensitively probe an unexplored population of low luminosity and low spin-down power pulsars. The millisecond pulsar luminosity function measured for the stack of sub-threshold millisecond pulsars constrains their contribution to the Galactic center GeV excess.", "revisions": [ { "version": "v2", "updated": "2022-03-07T20:54:46.000Z" } ], "analyses": { "keywords": [ "gamma-ray pulsars", "stacking survey", "energy loss rates implying", "lower rotational energy loss rates", "spectral parameter space implies" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable" } } }