费米大面积望远镜伽马射线脉冲星第三星表
高能天体物理现象
2023-11-29 v1
摘要
我们给出了在费米伽马射线空间望远镜的大面积望远镜（LAT）的 GeV 数据中发现的两百九十四颗脉冲星。在针对 LAT 源的深场射电搜索中发现的另外 33 颗毫秒脉冲星（MSP）一旦获得相位连接的自转星历表，很可能显现出脉冲。还有十余个与 LAT 源共位的光学和/或 X 射线双星系统也可能藏有伽马射线 MSP。因此，本星表报告了约 340 颗伽马射线脉冲星及候选体，占所有已知脉冲星的 10%，而费米之前已知的不超过 11 颗。伽马射线脉冲星中半数为年轻脉冲星。其中，未在射电波段探测到的那些相比年轻射电亮脉冲星具有更宽的银纬分布。其余为 MSP，其中 6 颗未在射电波段探测到。总体而言，在 50 MeV 以上亮度足以拟合脉冲轮廓、能谱或两者的超过 235 颗。对于常见的双峰轮廓，最靠近磁极穿越的伽马射线峰通常具有较软的能谱。随着自转能损率 下降到其在 erg s 附近的观测最小值，谱能分布趋于变窄，接近单能电子同步辐射的形状。我们在有距离可用时计算了伽马射线光度。我们的全天伽马射线灵敏度图可用于星族综合。电子星表版本提供了伽马射线脉冲星星历表、性质和拟合结果，以指导并与建模结果进行比较。
引用
@article{arxiv.2307.11132,
title = {The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars},
author = {David A. Smith and Philippe Bruel and Colin J. Clark and Lucas Guillemot and Matthew T. Kerr and Paul Ray and Soheila Abdollahi and Marco Ajello and Luca Baldini and Jean Ballet and Matthew Baring and Cees Bassa and Josefa Becerra Gonzalez and Ronaldo Bellazzini and Alessandra Berretta and Bhaswati Bhattacharyya and Elisabetta Bissaldi and Raffaella Bonino and Eugenio Bottacini and Johan Bregeon and Marta Burgay and Toby Burnett and Rob Cameron and Fernando Camilo and Regina Caputo and Patrizia Caraveo and Elisabetta Cavazzuti and Graziano Chiaro and Stefano Ciprini and Ismael Cognard and Paolo Cristarella Orestano and Milena Crnogorcevic and Alessandro Cuoco and Sara Cutini and Filippo D'Ammando and Alessandro de Angelis and Salvatore De Gaetano and Raniere de Menezes and Francesco de Palma and Megan DeCesar and Julia Deneva and Niccola Di Lalla and Leonardo Di Venere and Feraol Fana Dirirsa and Alberto Dominguez and Denis Dumora and Stephen Fegan and Elizabeth Ferrara and Alessio Fiori and Henrike Fleischhack and Chris Flynn and Anna Franckowiak and Paulo Freire and Yasushi Fukazawa and Piergiorgio Fusco and Giorgio Galanti and Viviana Gammaldi and Fabio Gargano and Dario Gasparrini and Federica Giacchino and Nico Giglietto and Francesco Giordano and Marcello Giroletti and David Green and Isabelle Grenier and Sylvain Guiriec and Michael Gustafsson and Alice Harding and Liz Hays and John Hewitt and Deirdre Horan and Xian Hou and Fabian Jankowski and Tyrel Johnson and Robert Johnson and Simon Johnston and Jun Kataoka and Michael J. Keith and Michael Kramer and Michael Kuss and Luca Latronico and Shiu-Hang Lee and Di Li and Jian Li and Brent Limyansky and Francesco Longo and Francesco Loparco and Leonarda Lorusso and Michael Lovellette and Marcus Lower and Pasquale Lubrano and Andrew Lyne and Simone Maldera and Richard Manchester and Alberto Manfreda and Martino Marelli and Guillem Marta-Devesa and Mario Nicola Mazziotta and Julie McEnery and Isabella Mereu and Peter Michelson and Warit Mitthumsiri and Tsunefumi Mizuno and Alex Moiseev and Maria Elena Monzani and Aldo Morselli and Michela Negro and Rodrigo Nemmen and Lars Nieder and Eric Nuss and Nicola Omodei and Monica Orienti and Elena Orlando and Jonathan F. Ormes and Michele Palatiello and David Paneque and Giuliana Panzarini and Massimo Persic and Melissa Pesce-Rollins and Roberta Pillera and Helen Poon and Troy Porter and Giacomo Principe and Silvia Raino and Riccardo Rando and Scott Ransom and Massimiliano Razzano and Soebur Razzaque and Anita Reimer and Olaf Reimer and Nicolas Renault-Tinacci and Roger Romani and Miguel A. Sanchez-Conde and Pablo Saz Parkinson and Lorenzo Scotton and Davide Serini and Carmelo Sgro and Ryan Shannon and Vidushi Sharma and Eric J. Siskind and Gloria Spandre and Paolo Spinelli and Ben Stappers and Tom Stephens and Dan Suson and Hiro Tajima and Dongguen Tak and Gilles Theureau and David Thompson and Omar Tibolla and Diego F. Torres and Janeth Valverde and Christo Venter and Zorawar Wadiasingh and Nina Wang and Pei Wang and Patrick Weltevrede and Kent Wood and Gabrijela Zaharijas},
journal= {arXiv preprint arXiv:2307.11132},
year = {2023}
}
备注
142 pages. Accepted by the Astrophysical Journal Supplement