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We present photometry and spectroscopy of four hydrogen-poor luminous supernovae discovered during the two-month science commissioning and early operations of the Zwicky Transient Facility (ZTF) survey. Three of these objects, SN2018bym…

The end of the Cosmic Dark Age marked the onset of reionization, driven by extreme-UV photons from the first galaxies. Direct detection of such photons has remained challenging due to strong intergalactic attenuation. Here, we report the…

The Hubble Ultra Deep Field Survey has not only provided the deepest optical and near infrared views of universe, but has enabled a search for the most distant supernovae to z~2.2. We have found four supernovae by searching spans of…

天体物理学 · 物理学 2008-11-26 Louis-Gregory Strolger , Adam G. Riess

We introduce a pipeline that performs rapid image subtraction and source selection to detect transients, with a focus on identifying gravitational wave optical counterparts using the Dark Energy Camera (DECam). In this work, we present the…

天体物理仪器与方法 · 物理学 2024-08-27 Shenming Fu , Thomas Matheson , Aaron Meisner , Yuanyuan Zhang , Sebastián Vicencio , Destry Saul

We present the discovery of SN 2025mkn, a gravitationally lensed Type II supernova. First detected as a blue transient in ZTF, 0.83$^{\prime\prime}$ from a $z=0.42$ elliptical galaxy, follow-up SNIFS/UH2.2m and LRIS/Keck spectra revealed…

宇宙学与河外天体物理 · 物理学 2026-04-10 Cameron Lemon , Ariel Goobar , Joel Johansson , Edvard Mörtsell , Steve Schulze , Igor Andreoni , Aleksandra Bochenek , Seán J. Brennan , Malte Busmann , Michael Coughlin , Kaustav K. Das , Suhail Dhawan , Christoffer Fremling , Anjasha Gangopadhyay , Daniel Gruen , Xander J. Hall , Anna Y. Q. Ho , Mansi M. Kasliwal , Daniel A. Perley , Mickael Rigault , Genevieve Schroeder , Mathew Smith , Jesper Sollerman , Jean J. Somalwar , Robert Stein , Stephen Thorp , Alice Townsend , Jacob L. Wise , Lin Yan , Nikki Arendse , Eric C. Bellm , Tracy X. Chen , Andrew Drake , Frank J. Masci , Josiah Purdum , Roger Smith , Jason T. Hinkle , T. Emil Rivera-Thorsen , Benjamin J. Shappee , Michael A. Tucker , Jessica Aguilar , Steven Ahlen , Greg Aldering , Segev Benzvi , Davide Bianchi , David Brooks , Todd Claybaugh , Axel de la Macorra , John Della Costa , Arjun Dey , Peter Doel , Brenna Flaugher , Andreu Font-Ribera , Jaime E. Forero-Romero , Enrique Gaztañaga , Satya Gontcho A. Gontcho , Gaston Gutierrez , Dragan Huterer , Mustapha Ishak , Jorge Jimenez , Dick Joyce , Stephanie Juneau , Robert Kehoe , Alex G. Kim , David Kirkby , Theodore Kisner , Anthony Kremin , Ofer Lahav , Martin Landriau , Laurent Le Guillou , Michael E. Levi , Marc Manera , Aaron Meisner , Ramon Miquel , John Moustakas , Seshadri Nadathur , Brendan O'Connor , Nathalie Palanque-Delabrouille , Antonella Palmese , Will J. Percival , Ignasi Pérez-Ràfols , Claire Poppett , Francisco Prada , Graziano Rossi , Eusebio Sanchez , David Schlegel , Michael Schubnell , Arman Shafieloo , Joseph Silber , David Sprayberry , Gregory Tarlé , Benjamin A. Weaver , Hu Zou

We perform a detailed analysis and simulations on the transient detection capability in the near-ultraviolet (NUV) band by focusing on some major local transient events. These events include the tidal disruption event due to a supermassive…

天体物理仪器与方法 · 物理学 2019-07-31 J. Wang , E. W. Liang , J. Y. Wei

The Catalina Real-time Transient Survey (CRTS) carried out a public survey for optical transients between 2007 and 2019, discovering more than 16,000 transient candidates. Here we present the spectra and highlight the results of the…

高能天体物理现象 · 物理学 2025-10-27 A. J. Drake , S. G. Djorgovski , M. J. Graham , D. Stern , A. A. Mahabal , M. Catelan , J. L. Prieto , S. Larson

The Pan-STARRS1 (PS1) survey has obtained imaging in 5 bands (grizy_P1) over 10 Medium Deep Survey (MDS) fields covering a total of 70 square degrees. This paper describes the search for apparently hostless supernovae (SNe) within the first…

We present the first results of the High cadence Transient Survey (HiTS), a survey whose objective is to detect and follow up optical transients with characteristic timescales from hours to days, especially the earliest hours of supernova…

During the Zwicky Transient Facility (ZTF) Phase-I operation, 78 hydrogen-poor superluminous supernovae (SLSNe-I) were discovered in less than three years, making up the largest sample from a single survey. This paper (Paper I) presents the…

There are currently many large-field surveys operational and planned including the powerful Vera C. Rubin Observatory Legacy Survey of Space and Time. These surveys will increase the number and diversity of transients dramatically. However,…

The ongoing optical time-domain astronomy surveys are routinely reporting fifty transient candidates per night. Here, I investigate the demographics of astronomical transients and supernova classifications reported to the Transient Name…

天体物理仪器与方法 · 物理学 2020-04-14 S. R. Kulkarni

We identified a new X-ray transient CXOM31 004252.457+411631.17 (T13) in M31 during a 2013 June Chandra observation. This system is particularly exciting because it is located within 100" of M31*; it is thought that this region of the bulge…

高能天体物理现象 · 物理学 2015-06-18 R. Barnard , M. R. Garcia , F. Primini , S. S. Murray

We report on the detection of a remarkable new fast high-energy transient found in the Chandra Deep Field-South, robustly associated with a faint ($m_{\rm R}=27.5$ mag, $z_{\rm ph}$$\sim$2.2) host in the CANDELS survey. The X-ray event is…

We present rapidly rising transients discovered by a high-cadence transient survey with Subaru telescope and Hyper Suprime-Cam. We discovered five transients at z=0.384-0.821 showing the rising rate faster than 1 mag per 1 day in the…

We report the discovery of a bright X-ray transient, CXOU J132527.6-430023, in the nearby early-type galaxy NGC 5128. The source was first detected over the course of five Chandra observations in 2007, reaching an unabsorbed outburst…

We report the discovery by the Robotic Optical Transient Experiment (ROTSE-IIIb) telescope of SN 2008es, an overluminous supernova (SN) at z=0.205 with a peak visual magnitude of -22.2. We present multiwavelength follow-up observations with…