文件操作 - 1749452784.M642428P18276.mail.planetcloud-host.com,S=5113,W=5197:2,
返回文件管理
返回主菜单
删除本文件
文件: /var/vmail/bicar.it/stefano/cur/1749452784.M642428P18276.mail.planetcloud-host.com,S=5113,W=5197:2,
编辑文件内容
Return-Path: <atel@astronomerstelegram.org> Delivered-To: stefano@bicar.it Received: by mail.planetcloud-host.com (Postfix, from userid 1016) id 9056014EA9; Mon, 9 Jun 2025 09:06:24 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.4.0 (2014-02-07) on mail.planetcloud-host.com X-Spam-Level: X-Spam-Status: No, score=-0.0 required=7.0 tests=RCVD_IN_DNSWL_BLOCKED, RCVD_IN_VALIDITY_RPBL_BLOCKED,RCVD_IN_VALIDITY_SAFE_BLOCKED,SPF_HELO_NONE, SPF_PASS,URIBL_BLOCKED autolearn=disabled version=3.4.0 Received-SPF: Pass (sender SPF authorized) identity=mailfrom; client-ip=174.142.199.243; helo=server.astronomerstelegram.org; envelope-from=atel@astronomerstelegram.org; receiver=stefano@bicar.it Received: from server.astronomerstelegram.org (astronomerstelegram.org [174.142.199.243]) by mail.planetcloud-host.com (Postfix) with ESMTP id A365F14603 for <stefano@bicar.it>; Mon, 9 Jun 2025 09:06:22 +0200 (CEST) Received: from server.astronomerstelegram.org (localhost [127.0.0.1]) by server.astronomerstelegram.org (Postfix) with ESMTP id EF9B02880847 for <stefano@bicar.it>; Mon, 9 Jun 2025 03:06:20 -0400 (EDT) To: stefano@bicar.it From: atel@astronomerstelegram.org Subject: ATel 17226 Message-Id: <20250609070620.EF9B02880847@server.astronomerstelegram.org> Date: Mon, 9 Jun 2025 03:06:20 -0400 (EDT) ------------------------------------------------------------------------------ The Astronomer's Telegram is free to read, free to publish, free to use. Thanks to the support of our patrons, we can continue to keep it free. https://www.patreon.com/astronomerstel ------------------------------------------------------------------------------ The Astronomer's Telegram http://www.astronomerstelegram.org ------------------------------------------------------------------------------ Posted: Within the last 24 hours ============================================================================== ATEL #17226 ATEL #17226 Title: Fermi-LAT detection of renewed gamma-ray activity from the FSRQ Ton 599 (4C +29.45) Author: S. Wagner (University of Wuerzburg) and Pietro Monti-Guarnieri (University of Trieste and INFN Trieste) on behalf of the Fermi Large Area Telescope Collaboration Queries: sarah.wagner@physik.uni-wuerzburg.de Posted: 8 Jun 2025; 19:59 UT Subjects:Gamma Ray, >GeV, AGN, Blazar The Large Area Telescope (LAT), one of the two instruments on the Fermi Gamma-ray Space Telescope, has observed renewed gamma-ray activity from a source positionally consistent with the flat-spectrum radio quasar Ton 599, also known as 4FGL J1159.5+2914 (Abdollahi et al. 2022, ApJS, 260, 53), with coordinates RA = 179.88264 deg, Decl. = 29.24551 deg, (J2000; Johnston et al. 1995 AJ 110, 880) at z = 0.72449 (Adelman-McCarthy et al. 2008, ApJS, 175, 297). Preliminary analysis indicates that this source was in an elevated gamma-ray emission state on June 7, 2025 , with a daily averaged gamma-ray flux (E>100MeV) of (1.8 +/- 0.2) x 10^-6 photons cm^-2 s^-1 (statistical uncertainty only). This corresponds to a flux increase of a factor of 10 relative to the average flux reported in the fourth data release of the fourth Fermi-LAT catalog (4FGL-DR4, Ballet et al. 2023, arXiv:2307.12546). The corresponding photon index is 2.2 +/- 0.1, and is consistent with the 4FGL-DR4 value of 2.155 +/- 0.006 within the uncertainties. Gamma-ray flaring of Ton 599 has previously been reported in ATels #15859, #14897, #14722, #10931, #8319, and #2795. Because Fermi normally operates in an all-sky scanning mode, regular gamma-ray monitoring of this source will continue. A preliminary light curve for Ton 599 can be accessed via the <a href="https://fermi.gsfc.nasa.gov/ssc/data/access/lat/LightCurveRepository/source.html?source_name=4FGL_J1159.5+2914">Fermi-LAT Light-Curve Repository</a> and the <a href="https://fermi.gsfc.nasa.gov/ssc/data/access/lat/msl_lc/source/Ton_599">Monitored Source List</a>. We encourage multifrequency observations of this source. For this source, the Fermi-LAT contact persons are S. Ciprini (stefano.ciprini@ssdc.asi.it) and D. J. Thompson (David.J.Thompson@nasa.gov). The Fermi-LAT is a pair conversion telescope designed to cover the energy band from 20 MeV to greater than 300 GeV. It is the product of an international collaboration between NASA and DOE in the U.S. and many scientific institutions across France, Italy, Japan and Sweden. ------------------------------------------------------------------------------ Password Certification: Sarah Wagner (sarah.wagner@physik.uni-wuerzburg.de) https://www.astronomerstelegram.org/?read=17226 ============================================================================== ============================================================================== This is an automatically-generated notice. You can remove yourself permanently from receiving both the Daily Email Digest and Instant Email Notices from The Astronomer's Telegram by following this link: https://www.astronomerstelegram.org?unsubscribe&confirmation=a803d34e7ea924f9a4142bac00763549&address=stefano@bicar.it
修改文件时间
将文件时间修改为当前时间的前一年
删除文件