Research Investigates Extreme Blazar "2Whsp J073326.7+515354"
Arthur T Knackerbracket has found the following story:
In a new study published April 23 on arXiv.org, Spanish astronomers have reported on an extreme blazar known as 2WHSP J073326.7+515354. Results of the research reveal the distance to this source and provide essential information about the stellar population of its host galaxy.
Blazars are very compact quasars associated with supermassive black holes at the centers of active, giant elliptical galaxies. Based on their optical emission properties, astronomers divide blazars into two classes: flat-spectrum radio quasars (FSRQs) that feature broad, prominent optical emission lines, and BL Lacertae objects (BL Lacs), which do not.
One subclass of BL Lacs with the highest frequency of synchrotron peak (over 100 PHz) comprises extreme high-frequency peaked BL Lacs (EHBLs). 2WHSP J073326.7+515354 (also called PGC 2402248) is a gamma-ray emitter first reported in 2017, and one of the few EHBLs detected at TeV energies. Therefore, the object is of particular interest for astronomers studying very high energy (VHE) blazars.
A team of researchers led by Josefa Becerra Gonzalez of the University of La Laguna, Spain, have recently observed 2WHSP J073326.7+515354 using the 10.4-meter Gran Telescopio de Canarias (GTC) and the 2.5-meter Isaac Newton Telescope (INT). The observations allowed them to determine the blazar's redshift precisely and provided more hints about the properties of its host.
[...] The researchers found that 2WHSP J073326.7+515354 is at a redshift of approximately 0.0065. This is the first distance estimation for this source, and knowing the exact redshift could be important for gamma-ray studies. It could, for instance, be helpful to estimate the effect of the distortion imprinted by the interaction of gamma-rays with the extragalactic background light (EBL).
More information: Optical spectral characterization of the the TeV extreme blazar 2WHSP J073326.7+515354, arXiv:2004.11359 [astro-ph.GA] arxiv.org/abs/2004.11359
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