Multiwavelength Analysis of Six Luminous Fast Blue Optical Transients
Open Access
- 4 August 2026
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 1007 (1)
Abstract
We present early (≲1 yr) multiwavelength observations and analysis of six luminous fast blue optical transients (LFBOTs). We identified these LFBOTs in Zwicky Transient Facility survey data from their fast light-curve evolution ( t 1/2 ≤ 12 days), blue colors at peak brightness ( g − r ≤ −0.2 mag), a visible host galaxy, high optical luminosity ( M g < −20 mag), and an X-ray and/or radio detection. With the exception of AT2024aehp (ZTF24abygbss), these transients exhibit peaks in their 10 GHz radio light curves at t rest ≈ 50–100 days, with peak radio luminosities ranging from 10 38 to 10 40 erg s −1 . Modeling the radio emission as synchrotron radiation indicates a fast ( v = 0.1–0.3 c ) shock in a dense ( n e ≈ 10 3 –10 4 cm −3 ) medium. The X-ray emission varies by ≈2 orders of magnitude in luminosity (10 42 –10 44 erg s −1 ) at t rest ∼ 20 days. Analysis of the host-galaxy photometry and spectroscopy for each transient shows that LFBOTs are predominantly nonnuclear (a few kiloparsecs offset) with star-forming host galaxies of stellar masses = 10 9 –10 11 M ⊙ . Unlike all other LFBOTs to date, AT2024aehp exhibited a luminous ( M < −19 mag) plateau in the optical light curve and its 6–15 GHz radio emission brightened by over an order of magnitude from t rest ≈ 70 to 130 days. The mostly consistent radio behavior between these LFBOTs implies a similar circumburst medium, leading us to prefer a progenitor scenario in which mass is lost in a consistent way shortly prior to the terminal event.Keywords
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Funding Information
- National Aeronautics and Space Administration (80NSSC24K0377)
- Space Telescope Science Institute (HST-GO-17477.006-A)
- National Science Foundation (PHY-2409481)
- National Science Foundation (PHY-2308862)
- National Science Foundation (PHY-2117997)
- U.S. Department of Energy (DE-SC0025599)
- National Science Foundation (AST-2508620)
- National Science Foundation (PHY-2019786)
- National Science Foundation (AST-1440341)
- National Science Foundation (AST-203443)
- National Science Foundation (2407588)
- National Science Foundation (AST-1005313)
- National Science Foundation (AST-1238877)
- Chinese Academy of Sciences (XDB09000000)
- Chinese Academy of Sciences (114A11KYSB20160057)
- MOST ∣ National Natural Science Foundation of China (12120101003)
- National Aeronautics and Space Administration (NAS 5-2655)
- NASA ∣ SMD ∣ Planetary Science Division (NNX08AR22G)
- National Science Foundation (1106171)
- MOST ∣ National Natural Science Foundation of China (11433005)
- U.S. Department of Energy (DE-AC02-05CH1123)
- NSF ∣ MPS ∣ Division of Astronomical Sciences (AST-0950945)
- Alfred P. Sloan Foundation (FG-2024-21320)
This publication has 145 references indexed in Scilit:
- The Host Galaxies of Tidal Disruption EventsSpace Science Reviews, 2020
- Birth of a relativistic outflow in the unusual γ-ray transient Swift J164449.3+573451Nature, 2011
- The Nordic Optical Telescope2010
- A relativistic type Ibc supernova without a detected γ-ray burstNature, 2010
- Relativistic ejecta from X-ray flash XRF 060218 and the rate of cosmic explosionsNature, 2006
- The association of GRB 060218 with a supernova and the evolution of the shock waveNature, 2006
- The Swift X-Ray TelescopeSpace Science Reviews, 2005
- The Swift Ultra-Violet/Optical TelescopeSpace Science Reviews, 2005
- A common origin for cosmic explosions inferred from calorimetry of GRB030329Nature, 2003
- Radio emission from the unusual supernova 1998bw and its association with the γ-ray burst of 25 April 1998Nature, 1998