Astronomers measure record brightness of radio galaxy AI illustrationhow this picture was madeRadio galaxy NGC 1275 reached measured optical magnitudes of 12.629 in the R band and 13.137 in the V band on 19 September 2026, astronomers reported. [4]
The readings carry error margins of ±0.003 for the R band and ±0.004 for the V band. They were captured using the 0.30 m telescope at the Astronomical Observatory of the University of Siena. [5]
Spectroscopic follow up observations were obtained with the Kast spectrograph on the Shane telescope at Lick Observatory on 21 September 2026. [1]
Observations from the LCO 1-m telescope at Teide Observatory placed the start of the outburst around MJD 61302. [2] The BHTOM collaboration ran an observing campaign for the event using five separate ground telescope facilities. [3]La galaxia de radio NGC 1275 alcanzó magnitudes ópticas medidas de 12.629 en la banda R y 13.137 en la banda V el 19 de septiembre de 2026, informaron astrónomos. [4]
Estas lecturas presentan márgenes de error de ±0.003 para la banda R y ±0.004 para la banda V. Fueron registradas utilizando el telescopio de 0.30 m del Observatorio Astronómico de la Universidad de Siena. [5]
Se obtuvieron observaciones de seguimiento espectroscópicas con el espectrógrafo Kast en el telescopio Shane del Observatorio Lick el 21 de septiembre de 2026. [1]
Observaciones realizadas con el telescopio LCO 1-m del Observatorio del Teide situaron el inicio del estallido alrededor del MJD 61302. [2] La colaboración BHTOM ejecutó una campaña de observación para este evento utilizando cinco instalaciones terrestres de telescopios independientes. [3]
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The spectroscopic observations were obtained using the Kast spectrograph on the Shane telescope at the Lick Observatory on September 21, 2026. · The Astronomer's Telegram
Observations obtained with the LCO 1-m telescope at Teide Observatory showed the new outburst began around MJD 61302. · The Astronomer's Telegram
The BHTOM collaboration utilized five facilities including the 0.41-m telescope at the School Astronomical Observatory Bolecina and the 0.6-m f/6.5 ADYU60 reflector at the Observatory of Adiyaman University for the observing campaign. · The Astronomer's Telegram
On 2026-09-20, astronomers Alessandro Marchini, Leonardo Stiaccini, Gaia Verna, and Giacomo Bonnoli (University of Siena, Italy, and INAF - Brera) reported that the radio galaxy NGC 1275 reached an extreme optical magnitude of 12.629 ± 0.003 in the R band and 13.137 ± 0.004 in the V band in observations made on 2026-09-19 with the 0.30 m telescope at the Astronomical Observatory of the University of Siena (IAU MPC code K54). · The Astronomer's Telegram
The optical observations of NGC 1275 were conducted with a 0.30 m telescope at the Astronomical Observatory of the University of Siena, which has IAU MPC observatory code K54. · The Astronomer's Telegram
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