Results 121 to 130 of about 48,593 (219)
We present follow-up imaging and spectroscopy and pre-explosion imaging of SN 2025pht located in NGC 1637 at 12 Mpc. Our spectroscopy shows that SN 2025pht is a Type II supernova (SN) with broad lines of hydrogen and with minimal line-of-sight extinction
Charles D. Kilpatrick +9 more
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We present and analyze panchromatic (0.35–14 μ m) spectroscopy of the Type II supernova 2023ixf, including near- and mid-infrared spectra obtained 33.6 days after explosion during the plateau phase, with the James Webb Space Telescope (JWST). This is the
J. M. DerKacy +48 more
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NEOWISE-R Caught the Luminous SN 2023ixf in Messier 101
During routine survey imaging, the reactivated Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE-R) serendipitously caught the Type II supernova SN 2023ixf in Messier 101 on the rise, starting day 3.6 through day 10.9, and again on the ...
Schuyler D. Van Dyk +18 more
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Discovery of a Likely Type II Supernova at z = 3.6 with JWST
Transient astronomy of the early, high-redshift ( z > 3) Universe is an unexplored regime that offers the possibility of probing the first stars and the epoch of reionization.
D. A. Coulter +32 more
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Late formation of silicon carbide in type II supernovae. [PDF]
Liu N +3 more
europepmc +1 more source
Early-phase Simultaneous Multiband Observations of the Type II Supernova SN 2024ggi with Mephisto
We present early-phase good-cadence (hour-to-day) simultaneous multiband ( ugi and vrz bands) imaging of the nearby supernova SN 2024ggi, which exploded in the nearby galaxy NGC 3621.
Xinlei Chen +26 more
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We present a comprehensive analysis of 32 type II supernovae (SNe II) with plateau phase photometry and late phase ( nebular ) spectroscopy available, aiming to bridge the gap between the surface and core of their red supergiant (RSG) progenitors.
Qiliang Fang +4 more
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Analysis of 14 Years of X-Ray Emission from SN 2011DH
Ejecta from core-collapse supernovae interact with the circumstellar medium shed by the progenitor star, producing X-ray emission. Previous studies analyzed the X-ray spectrum of the Type IIb supernova SN 2011dh up to ∼500 days after explosion. Long-term
Elisa J. Gao, Vikram V. Dwarkadas
doaj +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
In an effort to search for faint sources of emission over arbitrary timescales, we present a novel method for analyzing forced photometry light curves in difference imaging from optical surveys. Our method “ATLAS Clean,” or ATClean, utilizes the reported
S. Rest +18 more
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