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arXiv 2608.17242astro-ph.HEastro-ph.CO

AT 2020afjz(TSS2020a):TESS发现的首个河外快速暂现源

AT 2020afjz (TSS2020a): The First Fast Extragalactic Transient Discovered by TESS

Ryan Ridden-Harper, Hugh Roxburgh, Clarinda Montilla, Lancia Hubley, James Freeburn, Brayden Leicester, Andrew Moore, Zachary G. Lane, Jaime Luisi, Koji Shukawa… 展开作者

Ryan Ridden-Harper, Hugh Roxburgh, Clarinda Montilla, Lancia Hubley, James Freeburn, Brayden Leicester, Andrew Moore, Zachary G. Lane, Jaime Luisi, Koji Shukawa, Armin Rest, Jeff Cooke, Michele T. Bannister, Lilly Fox, Tait Keller, Qinan Wang

AI总结:

本研究发现了TESS首个小时级河外快速暂现源AT 2020afjz,经建模其或为轴上“脏火球”或轴外孤儿余烬,展现了TESS发现此类暂现源的潜力。

AI中文摘要:

我们报告AT 2020afjz(TSS2020a)的发现:这是首个在光学波段发现的时标为小时级的河外暂现源,其从爆发起始到衰减的完整演化过程在时间上被完整解析,也是首个由TESS发现的此类暂现源。AT 2020afjz是在TESSELLATE巡天框架下开展的HiLaTS预研项目中被识别的,其显著性大于10σ,该项目通过TESSELLATE pipeline盲搜TESS数据中的暂现现象。通过与 legacy成像数据交叉匹配,我们将其与DES J042144.37$-$383311.3相关联,该天体是一个相互作用星系对的成员,其测光红移为$z_{\rm phot}=0.67^{+0.07}_{-0.10}$。AT 2020afjz的持续时间和亮度与伽马射线暴(GRB)余烬类似,但它的上升时标约为1小时,在半峰值亮度以上仅持续2.4小时;使用VegasAfterglow对TESS光变曲线建模发现,它最适合被归类为轴上“脏火球”或轴外孤儿余烬。这两种罕见分类均依赖于伽马射线能量的非探测,但由于费米伽马射线暴监测器(Fermi-GBM)在爆发时处于地球掩蔽状态,无法明确确认AT 2020afjz的伽马射线宁静特性。无论如何,AT 2020afjz证明了TESS发现河外快速暂现源的能力,并预示着将有新的暂现源群有待通过TESSELLATE项目发现。

英文摘要:

We report the discovery of AT 2020afjz (TSS2020a): the first hour-scale extragalactic transient discovered in optical wavelengths whose complete evolution -- from explosion onset to decay -- is temporally resolved, and the first such transient discovered by TESS. AT 2020afjz was identified as a $>10σ$ detection in the pilot HiLaTS program run within the TESSELLATE Sky Survey, which blindly searches for transient phenomena in TESS data with the TESSELLATE pipeline. Through cross-matching with legacy imaging, we associate it with DES J042144.37$-$383311.3, a member of an interacting galaxy pair at $z_{\rm phot}=0.67^{+0.07}_{-0.10}$. While AT 2020afjz is similar in duration and brightness to GRB afterglows, it exhibits a slow rise time of $\sim1$ hr and lasts for only 2.4 hr above the half-max brightness; modeling the TESS light curve with VegasAfterglow finds that it is best described as either an on-axis "dirty-fireball" or off-axis orphan afterglow. Each of these rare classifications hinge upon a non-detection at gamma-ray energies, but as Fermi-GBM was Earth-occulted at the time of explosion, AT 2020afjz's gamma-quiet nature cannot be definitively confirmed. Regardless, AT 2020afjz demonstrates TESS's power to discover fast extragalactic transients, and heralds a new population awaiting discovery with TESSELLATE.

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