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Related papers: Spectroscopic Classification of Extragalactic Tran…

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[Abridged] We present a search for fast optical transients (~0.5 hr-1 day) using repeated observations of the Pan-STARRS1 Medium-Deep Survey (PS1/MDS) fields. Our search takes advantage of the consecutive g/r-band observations (16.5 min in…

We present the Keck Infrared Transient Survey (KITS), a NASA Key Strategic Mission Support program to obtain near-infrared (NIR) spectra of astrophysical transients of all types, and its first data release, consisting of 105 NIR spectra of…

During 1990-92, the WATCH all-sky X-ray monitor on Granat discovered six short-duration X-ray transients. In this paper we discuss their possible relationship to peculiar stars. Only one of the fast (few hours) X-ray transients (GRS…

Astrophysics · Physics 2007-05-23 Alberto Castro-Tirado , Soeren Brandt , Niels Lund , Rashid Sunyaev

Although a multitude of studies have focused on targeted observations of Galactic X-ray transients, blind surveys and population studies have been limited. We have used the ROSAT, eROSITA and Gaia source catalogs to find Galactic X-ray…

High Energy Astrophysical Phenomena · Physics 2025-11-17 Vikash Maan , Aman Katira , Kunal. P. Mooley

Calcium-rich (Ca-rich) transients are a new class of supernovae (SNe) that are known for their comparatively rapid evolution, modest peak luminosities, and strong nebular calcium emission lines. Currently, the progenitor systems of Ca-rich…

High Energy Astrophysical Phenomena · Physics 2022-03-30 Y. Dong , D. Milisavljevic , J. Leja , S. K. Sarbadhicary , A. E. Nugent , R. Margutti , W. V. Jacobson-Galan , A. Polin , J. Banovetz , J. M. Reynolds , B. Subrayan

This work presents the observations and analysis of ATLAS19dqr/SN 2019bkc, an extraordinary rapidly evolving transient event located in an isolated environment, tens of kiloparsecs from any likely host. Its light curves rise to maximum…

Extragalactic fast X-ray transients (FXTs) are short flashes of X-ray photons of unknown origin that last a few minutes to hours. We extend the search for extragalactic FXTs from Quirola et al. 2022 (Paper I; based on sources in the Chandra…

High Energy Astrophysical Phenomena · Physics 2023-07-05 J. Quirola-Vásquez , F. E. Bauer , P. G. Jonker , W. N. Brandt , G. Yang , A. J. Levan , Y. Q. Xue , D. Eappachen , E. Camacho , M. E. Ravasio , X. C. Zheng , B. Luo

We present the discovery of two new X-ray transients in archival Chandra data. The first transient, XRT 110103, occurred in January 2011 and shows a sharp rise of at least three orders of magnitude in count rate in less than 10 s, a flat…

High Energy Astrophysical Phenomena · Physics 2015-05-27 A. Glennie , P. G. Jonker , R. P. Fender , T. Nagayama , M. L. Pretorius

We introduce Deep-HiTS, a rotation invariant convolutional neural network (CNN) model for classifying images of transients candidates into artifacts or real sources for the High cadence Transient Survey (HiTS). CNNs have the advantage of…

Instrumentation and Methods for Astrophysics · Physics 2017-02-22 Guillermo Cabrera-Vives , Ignacio Reyes , Francisco Förster , Pablo A. Estévez , Juan-Carlos Maureira

We report the spectral and temporal variability properties of 18 candidate transient and potential transient (TC and PTC) sources detected in deep multi-epoch Chandra observation of the nearby elliptical galaxies, NGC 3379, NGC 4278 and NGC…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 N. J. Brassington , G. Fabbiano , A. Zezas , A. Kundu , D. -W. Kim , T. Fragos , A. R. King , S. Pellegrini , G. Trinchieri , S. Zepf , N. J. Wright

For radio transients, an inverted spectrum (defined as $\alpha > 0$ for a power law spectrum $S_{\nu}\propto \nu^{\alpha}$) constrains physical properties, which in principle can be a useful criterion for selecting specific targets of…

High Energy Astrophysical Phenomena · Physics 2025-06-13 Yuyang Chen , B. M. Gaensler , Tracy Clarke , Wendy Peters , Emil Polisensky , Kovi Rose

We present a study of the properties of the host galaxies of unusual transient objects of two types, both being sub-luminous compared with the major classes of supernovae. Those of one type exhibit unusually strong calcium features, and…

Solar and Stellar Astrophysics · Physics 2015-06-16 Joseph Lyman , Phil James , Hagai B. Perets , Joseph P. Anderson , Avishay Gal-Yam , Paolo Mazzali , Sue Percival

A new class of core-collapse supernovae (SNe) has been discovered in recent years by optical/infrared surveys; these SNe suggest the presence of one or more extremely dense (~10^5-10^11 cm^-3) shells of circumstellar material (CSM) on…

High Energy Astrophysical Phenomena · Physics 2011-11-07 Kohta Murase , Todd A. Thompson , Brian C. Lacki , John F. Beacom

We present a search for an electromagnetic counterpart of the gravitational wave source GW151226. Using the Pan-STARRS1 telescope we mapped out 290 square degrees in the optical i_ps filter starting 11.5hr after the LIGO information release…

The progenitors of SN 2008S and the 2008 transient in NGC300 were dust-enshrouded, with extremely red mid-infrared (MIR) colors and relatively low luminosities. The transients were optically faint (-13 < M_V < -15) compared to normal…

We show that the spectrum of the unusual transient SCP06F6 is consistent with emission from a cool, optically thick and carbon-rich atmosphere if the transient is located at a redshift of z~0.14. The implied extragalactic nature of the…

Astrophysics · Physics 2010-01-15 B. T. Gaensicke , A. J. Levan , T. R. Marsh , P. J. Wheatley

We discuss 76 large amplitude transients (Delta-m>1.5) occurring in the nuclei of galaxies, nearly all with no previously known Active Galactic Nucleus (AGN). They have been discovered as part of the Pan-STARRS1 (PS1) 3pi survey, by…

The ANTARES telescope has the opportunity to detect transient neutrino sources, such as gamma-ray bursts, core-collapse supernovae, flares of active nuclei... To enhance the sensitivity to these sources, we have developed a new detection…

High Energy Astrophysical Phenomena · Physics 2019-08-15 D. Dornic , S. Basa , J. Brunner , I. Al Samarai , J. Busto , A. Klotz , S. Escoffier , V. Bertin , B. Vallage , B. Gendre , A. Mazure , M. Boer