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Return-Path: <atel@astronomerstelegram.org> Delivered-To: stefano@bicar.it Received: by mail.planetcloud-host.com (Postfix, from userid 1016) id CF45714EB7; Fri, 11 Apr 2025 09:06:00 +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 D958814BEA for <stefano@bicar.it>; Fri, 11 Apr 2025 09:05:58 +0200 (CEST) Received: from server.astronomerstelegram.org (localhost [127.0.0.1]) by server.astronomerstelegram.org (Postfix) with ESMTP id 4E6E628807A6 for <stefano@bicar.it>; Fri, 11 Apr 2025 03:05:57 -0400 (EDT) To: stefano@bicar.it From: atel@astronomerstelegram.org Subject: ATel 17141 Message-Id: <20250411070557.4E6E628807A6@server.astronomerstelegram.org> Date: Fri, 11 Apr 2025 03:05:57 -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 #17141 ATEL #17141 Title: Continuing observations of KT Eri by Swift Author: K. L. Page (U. Leicester) Queries: kpa@star.le.ac.uk Posted: 10 Apr 2025; 15:10 UT Subjects:Ultra-Violet, X-ray, Nova Further observations of KT Eri (Nova Eri 2009) have been obtained by the Neil Gehrels Swift Observatory, following the increase in optical brightness announced in ATel #17125. As reported by Masetti & Munari in ATel #17140, an observation with the X-ray Telescope (XRT) on 2025 April 6 did not detect an X-ray source, to a 3σ upper limit of 5 x 10<sup>-3</sup> count s<sup>-1</sup> (0.3-10 keV). Observations on April 8 and 10, however, both revealed a faint X-ray source at > 3σ significance, with a mean count rate of (4.2 +1.1/-0.9) x 10<sup>-3</sup> count s<sup>-1</sup>. There is no evidence of variation in the count rate between the two observations. While there are too few counts to perform a detailed spectral fit, it is clear that the emission is not super-soft. Data collected by the UV/Optical Telescope show the UV emission to be increasing, rising from w2 = 13.05 +/- 0.02 to 12.75 +/- 0.03 mag (Vega system) between April 6 and 10. Continuing observations with Swift are planned until KT Eri enters the solar observing constraint on 22nd April. ------------------------------------------------------------------------------ Password Certification: Kim Page (kpa@star.le.ac.uk) https://www.astronomerstelegram.org/?read=17141 ============================================================================== ============================================================================== 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
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