NOVA Sco 2024 , the SIMBAD biblio

NOVA Sco 2024 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:09:54


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Title First 3 Authors
2024ATel16439....1C 179 T         X         3 1 ~ Fermi-LAT Gamma-ray Detection of the probable nova
PNV
J17261813-3809354
.
CHEUNG C.C. (The Fermi Large Area Telescope Collaboration)
2024ATel16440....1A 179 T         X         3 1 ~ SOAR spectroscopic classification of
PNV J17261813-3809354 as a nova near visible peak.
AYDI E., STRADER J., MOLINA I., et al.
2024ATel16441....1C 134 T         X         2 1 ~ Further Fermi-LAT gamma-ray observations of
Nova Sco 2024 (
PNV J17261813-3809354).
CHEUNG C.C., JEAN P. (The Fermi Large Area Telescope Collaboration)
2024ATel16442....1S 134 T         X         2 1 ~ Optical echelle spectroscopy of the classical nova
PNVJ17261813-133809354.
SHORE S., SHORE S., CHARBONNEL S., et al.
2024ATel16444....1S 448 T         X         9 3 ~ NuSTAR and Swift upper limits on the early X-ray emission from
Nova Scorpii 2024 (
V1723 Sco,
PNV J17261813-3809354).
SOKOLOVSKY K., LUNA G.J.M., AYDI E., et al.
2024ATel16454....1H 269 T         X         5 2 ~ Optical Photometry and Spectroscopy of
Nova Sco 2024 (
V1723 Sco).
HABTIE G.R. and DAS R.
2024ATel16484....1S 403 T         X         8 1 ~ Swift X-ray detection of
Nova Scorpii 2024 (
V1723 Sco).
SOKOLOVSKY K., LUNA G.J.M., KUIN P., et al.
2024ATel16492....1M 403 T         X         8 1 ~ VLA radio detection of
Nova Scorpii 2024 (
V1723 Sco).
MOLINA I., SOKOLOVSKY K., AYDI E., et al.
2025ApJ...980..129B 47           X         1 42 ~ Discovery and Detailed Study of the M31 Classical Nova AT 2023tkw: Evidence for Internal Shocks. BASU J., KUMAR R., ANUPAMA G.C., et al.
2025ApJ...993..232S 112       D       C       2 411 ~ Comprehensive Listing of 208 Nova White Dwarf Masses as the Primary Determinant of Spectral Class and Light-curve Class. SCHAEFER B.E.
2026A&A...705A..19F 2300 T   A D S   X C       44 8 ~ Fermi-LAT detections of the classical novae
V1723 Sco and V6598 Sgr in a multi-wavelength context.
FAUVERGE P., JEAN P., SOKOLOVSKY K., et al.

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