17-May-2023: Observations from 11 global telescopes lead to detection of the brightest flare of a century-old blazar

The brightness of BL Lacertae (BL Lac), a blazar located about 950 million light years from the Earth and discovered almost a century ago has been found to have reached its maxima.

Results published in the latest study, led by post-doctoral fellow Aditi Agarwal from the Raman Research Institute, an autonomous institute funded by the Department of Science and Technology (DST), stated that the flare emanated from BL Lac had reached the maxima on August 21, 2020, which is a novel finding about this source.

For several decades now, BL Lacertae (commonly referred as BL Lac), an Active Galactic Nucleus (AGN) source, has remained of significant interest for study among the global astronomy community.

Usually located in the core of the galaxy, AGNs are compact structures showing anomalous luminosity from time-to-time. The deviation in their brightness levels can vary and last either for a few hours, days, weeks or even some months. This luminosity variance, when seen with naked human eye, is nothing but the electromagnetic emissions that are visible across the radio, microwave, infrared, optical, ultra-violet, X-ray and gamma wavelengths. 

The flaring up and its decay of the emissions from BL Lac was detected using the continuous observations made by an ensemble of eleven optical telescopes located in across the world. One among them was the Himalayan Chandra Telescope located in Ladakh’s Hanle.

In early July 2020, astronomers suspected that BL Lac was beginning to flare up. All the eleven telescopes were instantly deployed and focused observations continued for 84 days starting July 13, 2020 till – September 14, 2020.

“As time progressed, it was observed that the flare was becoming brighter gradually, indicating that BL Lac was turning more active. For the first time on August 21, 2020, BL Lac’s brightness reached its maxima. This was captured well by the Modified Dall–Kirkham telescope located in Kraków, Poland,” said Agarwal, lead author of the paper titled ‘Analysis of the intra-night variability of BL Lacertae during its August 2020 flare’ published in the Astrophysical Journal Supplements Series.

Results showed that BL Lac’s magnitude (brightness) increased from 14 to 11.8 (astronomically used) whereas its flux value rose from 13.37 milli Jansky (mJy) to peak at 109.88 mJy, another maiden observation for this source. Additionally, this international collaboration of researchers calculated the source’s magnetic field, which was found to range from 7.5 Gauss to 76.3 Gauss during the flare.

These significant calculations, never possible before, was solely performed because of the availability of Terabytes of datasets obtained from the battery of telescopes.

“These new parameters shall form the basis for future multispectral studies of BL Lac,” Agarwal highlighted.

Furthermore, the researchers were also able to estimate the flare emitting region size of this source, which was calculated to be 1/8th on the actual jet radius.

Agarwal’s team continues to carry on with more observations of this BL Lac and attempt to understand its characteristics in the X-Ray and gamma wavelengths are currently underway.

17-May-2023: Observations from 11 global telescopes lead to detection of the brightest flare of a century-old blazar

The brightness of BL Lacertae (BL Lac), a blazar located about 950 million light years from the Earth and discovered almost a century ago has been found to have reached its maxima.

Results published in the latest study, led by post-doctoral fellow Aditi Agarwal from the Raman Research Institute, an autonomous institute funded by the Department of Science and Technology (DST), stated that the flare emanated from BL Lac had reached the maxima on August 21, 2020, which is a novel finding about this source.

For several decades now, BL Lacertae (commonly referred as BL Lac), an Active Galactic Nucleus (AGN) source, has remained of significant interest for study among the global astronomy community.

Usually located in the core of the galaxy, AGNs are compact structures showing anomalous luminosity from time-to-time. The deviation in their brightness levels can vary and last either for a few hours, days, weeks or even some months. This luminosity variance, when seen with naked human eye, is nothing but the electromagnetic emissions that are visible across the radio, microwave, infrared, optical, ultra-violet, X-ray and gamma wavelengths. 

The flaring up and its decay of the emissions from BL Lac was detected using the continuous observations made by an ensemble of eleven optical telescopes located in across the world. One among them was the Himalayan Chandra Telescope located in Ladakh’s Hanle.

In early July 2020, astronomers suspected that BL Lac was beginning to flare up. All the eleven telescopes were instantly deployed and focused observations continued for 84 days starting July 13, 2020 till – September 14, 2020.

“As time progressed, it was observed that the flare was becoming brighter gradually, indicating that BL Lac was turning more active. For the first time on August 21, 2020, BL Lac’s brightness reached its maxima. This was captured well by the Modified Dall–Kirkham telescope located in Kraków, Poland,” said Agarwal, lead author of the paper titled ‘Analysis of the intra-night variability of BL Lacertae during its August 2020 flare’ published in the Astrophysical Journal Supplements Series.

Results showed that BL Lac’s magnitude (brightness) increased from 14 to 11.8 (astronomically used) whereas its flux value rose from 13.37 milli Jansky (mJy) to peak at 109.88 mJy, another maiden observation for this source. Additionally, this international collaboration of researchers calculated the source’s magnetic field, which was found to range from 7.5 Gauss to 76.3 Gauss during the flare.

These significant calculations, never possible before, was solely performed because of the availability of Terabytes of datasets obtained from the battery of telescopes.

“These new parameters shall form the basis for future multispectral studies of BL Lac,” Agarwal highlighted.

Furthermore, the researchers were also able to estimate the flare emitting region size of this source, which was calculated to be 1/8th on the actual jet radius.

Agarwal’s team continues to carry on with more observations of this BL Lac and attempt to understand its characteristics in the X-Ray and gamma wavelengths are currently underway.

2021

13-Feb-2021: Indian astronomers detect huge optical flare in one of the oldest astronomic objects

Indian Astronomers have reported one of the strongest flares from a feeding supermassive black hole or blazar called BL Lacertae. Analysis of the flare from this blazar, one of the oldest astronomical objects, can help trace the mass of the black hole and the source of this emission. Such analysis can provide a lead to probe into mysteries and trace events at different stages of evolution of the Universe.

Blazars or feeding supermassive black holes in the heart of distant galaxies receive a lot of attention from the astronomical community because of their complicated emission mechanism. They emit jets of charged particles traveling nearly at the speed of light and are one of the most luminous and energetic objects in the Universe.

BL Lacertae blazar is 10 million light-years away and is among the 50 most prominent blazars that can be observed with the help of a relatively small telescope. It was among the 3 to 4 blazars that was predicted to be experiencing flares by the Whole Earth Blazar Telescope (WEBT), an international consortium of astronomers. 

A team of astronomers led by Dr. Alok Chandra Gupta from Aryabhatta Research Institute of Observational Sciences (ARIES), an autonomous institute of the Department of Science & Technology, Government of India who had been following the blazar since October 2020 as part of an international observational campaign detected the exceptionally high flare on January 16, 2021, with the help of Sampurnanand Telescope (ST) and 1.3m Devasthal Fast Optical Telescopes located in Nainital.

The data collected from the flare observed will help calculation of the black hole mass, size of emission region, and mechanism of the emission from one of the oldest astronomical objects known, hence opening a door to the origin and evolution of the Universe.