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20132026
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 6.9k across the 45 of their papers we have counts for

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18 papers · 1 filter

astro-ph.SR2026

Late-Time Evolution of the Massive Stellar Merger M101 OT2015-1

Marco A. Gómez-Muñoz, Nadejda Blagorodnova, Tomasz Kamiński +6

Luminous red novae (LRNe) are astronomical transients arising from unstable mass transfer and common envelope phases in close binary systems, culminating in stellar mergers. Their…

astro-ph.SR2026

Exploring stellar evolution with Luminous Red Novae and Interacting Gap Transients

Nadejda Blagorodnova

Interacting gap transients encompass several families of astrophysical phenomena where eruptive mass loss and interaction play an important role in shaping the observational proper…

astro-ph.SR2026

Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves

Chunliang Mu, Orsola De Marco, Luis C. Bermúdez-Bustamante +6

Luminous red novae are transient events thought to arise from common envelope binary interactions. In this paper, we perform post-processing light-curve calculations for two, 3D hy…

astro-ph.SR2026

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation

M. Wavasseur, N. Blagorodnova, M. A. Gómez-Muñoz +1

Luminous red novae are astrophysical transients associated with unstable mass transfer in interacting binaries and are commonly interpreted as outcomes of common-envelope evolution…

astro-ph.SR2026

XP-TEAL: Gaia XP Tool for Emission and Absorption Lines II. Gaia-HELIX catalogue of H emitters in Gaia BP/RP spectra

S. Malhotra, M. Weiler, F. Anders +8

Context: With Gaia's third Data Release (DR3), low-resolution BP/RP (XP) spectra became available for more than 219 million sources. In previous work, we developed a fast method fo…

astro-ph.SR2026

Red novae, their progenitors, and remnants

Tomasz Kaminski, Nadejda Blagorodnova

Red novae or luminous red novae are a class of optical transients that have emerged over the past two decades. They occupy an intermediate luminosity regime between classical novae…

astro-ph.SR2025★ 1 cited

Hot springs and dust reservoirs: JWST reveals the dusty, molecular aftermath of extragalactic stellar mergers

Viraj Karambelkar, Mansi Kasliwal, Ryan M. Lau +7

We present James Webb Space Telescope (JWST) observations of four Luminous Red Novae (LRNe): dusty, extragalactic transients from stellar mergers following common-envelope evolutio…

astro-ph.SR2025

The slow brightening of WNTR23bzdiq / WTP19aalzlk : Possible onset of common-envelope evolution in an asymptotic giant branch star?

Viraj Karambelkar, Mansi Kasliwal, Kishalay De +6

We present WNTR23bzdiq/WTP19aalzlk, a slow eruption of an early-asymptotic giant branch (AGB) star in M31 identified by the Wide-field Infrared Transient Explorer (WINTER) near-inf…

astro-ph.SR2024★ 2 cited

Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors

Hugo Tranin, Nadejda Blagorodnova, Viraj Karambelkar +5

After the main sequence phase, stars more massive than 2.5 M rapidly evolve through the Hertzsprung gap as yellow giants and supergiants (YSG), before settling into the red…

astro-ph.SR2022★ 12 cited

Searching for the Next Galactic Luminous Red Nova

Harry Addison, Nadejda Blagorodnova, Paul J. Groot +3

Luminous red novae (LRNe) are astrophysical transients believed to be caused by the partial ejection of a binary star's common envelope (CE) and the merger of its components. The f…

astro-ph.SR2021

AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary

Jacob E. Jencson, Jennifer E. Andrews, Howard E. Bond +39

Nova eruptions, thermonuclear explosions on the surfaces of white dwarfs (WDs), are now recognized to be among the most common shock-powered astrophysical transients. We present th…

astro-ph.SR2021★ 5 cited

The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor

Nadejda Blagorodnova, Jakub Klencki, Ondrej Pejcha +12

Luminous Red Novae (LRNe) are astrophysical transients associated with the partial ejection of a binary system's common envelope (CE) shortly before its merger. Here we present the…

astro-ph.SR2020★ 42 cited

Progenitor, Precursor and Evolution of the Dusty Remnant of the Stellar Merger M31-LRN-2015

Nadejda Blagorodnova, Viraj Karambelkar, Scott M. Adams +12

M31-2015-LRN is a likely stellar merger discovered in the Andromeda Galaxy in 2015. We present new optical to mid-infrared photometry and optical spectroscopy for this event. Archi…

astro-ph.SR2019★ 31 cited

Discovery of an intermediate-luminosity red transient in M51 and its likely dust-obscured, infrared-variable progenitor

Jacob E. Jencson, Scott M. Adams, Howard E. Bond +49

We present the discovery of an optical transient (OT) in Messier 51, designated M51 OT2019-1 (also ZTF19aadyppr, AT 2019abn, ATLAS19bzl), by the Zwicky Transient Facility (ZTF). Th…

astro-ph.SR2019★ 33 cited

Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye

Łukasz Wyrzykowski, P. Mróz, K. A. Rybicki +182

Gaia16aye was a binary microlensing event discovered in the direction towards the northern Galactic disc and was one of the first microlensing events detected and alerted to by the…

astro-ph.SR2015★ 45 cited

Total eclipse of the heart: The AM CVn Gaia14aae / ASSASN-14cn

H. C. Campbell, T. R. Marsh, M. Fraser +82

We report the discovery and characterisation of a deeply eclipsing AM CVn-system, Gaia14aae (= ASSASN-14cn). Gaia14aae was identified independently by the All-Sky Automated Survey…

astro-ph.SR2014★ 37 cited

OGLE-2013-SN-079: a lonely supernova consistent with a helium shell detonation

C. Inserra, S. A. Sim, L. Wyrzykowski +31

We present observational data for a peculiar supernova discovered by the OGLE-IV survey and followed by the Public ESO Spectroscopic Survey for Transient Objects. The inferred reds…

astro-ph.SR2013★ 118 cited

A statistical analysis of circumstellar material in Type Ia supernovae

Kate Maguire, Mark Sullivan, Ferdinando Patat +42

A key tracer of the elusive progenitor systems of Type Ia supernovae (SNe Ia) is the detection of narrow blueshifted time-varying Na I D absorption lines, interpreted as evidence o…