年会上三场嘉宾论坛分别围绕三个主题来进行，即“云计算和大数据给我们带来哪些变化”、“天文学研究和科普教育对云计算、大数据有哪些需求”、“如何实现产学研的合作互赢”。
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工作组创始成员16人，其中很多是国际天文科普教育界的大咖，比如IAU天文学教育与发展委员会主席Beatriz Garcia博士、IAU天文学公众沟通委员会主席Pedro Russo博士、IAU天文普及办公室主任 ...
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该文章利用相互作用模型解释II型超新星多样性起源，是研究II型超新星爆发机制以及宇宙学应用的重要一环。论文链接：点击这里。根据光变曲线轮廓，传统上II型超新星分成光变曲线呈现出平台特征的IIP型以及光变曲线在星等尺度上线性下降的IIL型。然而，这两种II型超新星的起源尚存争议。该工作认为II型超新星爆炸极早期普遍存在相互作用，其强弱以及持续时间的长短是导致II型超新星观测多样性的主要因素。进一步提出早期相互作用是造成II型超新星光度-速度关系弥散的主要来源，指出了提高II型超新星宇宙学测距精度的方向。由于观测不够及时，以前往往没有捕捉到爆炸初始时刻的关键信息，从而对II型超新星分类产生误解。
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A new stellar database of the Ca II Triplet, which serves as an indicator for characterizing the chromospheric ...It includes R, R^+ index for Ca II IRT, stellar parameters and other valuable information, the uncertainties ...
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A new stellar database of the Ca II Triplet, which serves as an indicator for characterizing the chromospheric ...It includes R, R^+ index for Ca II IRT, stellar parameters and other valuable information, the uncertainties ...
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A new stellar database of the Ca II Triplet, which serves as an indicator for characterizing the chromospheric ...It includes R, R+ index for Ca II IRT, stellar parameters and other valuable information, the uncertainties ...
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A new stellar database of the Ca II Triplet, which serves as an indicator for characterizing the chromospheric ...It includes R, R+ index for Ca II IRT, stellar parameters and other valuable information, the uncertainties ...
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“Type II” flares are typical confined flares associated with the failed eruptions of the filaments/flux ...A total of 59 flares are “Type I” flares (about 40%) and 93 events are “Type II” flares (about 60%).the two types of confined flares, with “Type I” confined flares from ARs with a larger ΦAR than “Type II ...About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...reconnection flux ΦRIB and the flare duration τFWHM both give larger values for “Type I” than “Type II ...
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“Type II” flares are typical confined flares associated with the failed eruptions of the filaments/flux ...A total of 59 flares are “Type I” flares (about 40%) and 93 events are “Type II” flares (about 60%).the two types of confined flares, with “Type I” confined flares from ARs with a larger ΦAR than “Type II ...About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...reconnection flux ΦRIB and the flare duration τFWHM both give larger values for “Type I” than “Type II ...
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“Type II” flares are typical confined flares associated with the failed eruptions of the filaments/flux ...A total of 59 flares are “Type I” flares (about 40%) and 93 events are “Type II” flares (about 60%).the two types of confined flares, with “Type I” confined flares from ARs with a larger ΦAR than “Type II ...About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...reconnection flux ΦRIB and the flare duration τFWHM both give larger values for “Type I” than “Type II ...
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“Type II” flares are typical confined flares associated with the failed eruptions of the filaments/flux ...A total of 59 flares are “Type I” flares (about 40%) and 93 events are “Type II” flares (about 60%).the two types of confined flares, with “Type I” confined flares from ARs with a larger ΦAR than “Type II ...About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...reconnection flux ΦRIB and the flare duration τFWHM both give larger values for “Type I” than “Type II ...
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Properties of emission lines of type 1 AGNs derived from fitting to their spectra.Title: The Black Hole Masses and Eddington Ratios of Type 2 Quasars Authors: Kong M., Ho L.C. Table: Sample Properties ...
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A new stellar database of the Ca II Triplet, which serves as an indicator for characterizing the chromospheric ...It includes R, R+ index for Ca II IRT, stellar parameters and other valuable information, the uncertainties ...
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LAMOST大型光谱巡天项目为测量恒星色球层的Ca II线发射活动指标提供了大量数据，同时Kepler任务提供的高精度测光数据可以用来测量恒星光球层亮度变化。当转动周期超过几天后，Ca II线发射强度和光球亮度变化都会随着转动周期的增加而逐渐减弱，呈现出指数衰减关系。图1：不同光谱类型的恒星色球 Ca II 线发射强度指标（上）和光球亮度变化指标（下）分别与恒星转动周期的关系 ...
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3小时后，他将结果上传到TNS，把该候选体分类为II型超新星，红移为0.01，其编号随即变更为超新星编号SN 2024vs。管理员高兴使用宁波市教育局-新疆天文台望远镜（NEXT）上的Alpy 600光谱仪也获得了这颗超新星的光谱，16日上午，管理员赵经远对光谱数据进行了处理，并使用GELATO进行分类，结果显示这条光谱与一些II ...型超新星相似，例如爆炸后5.0天的II-P型超新星SN 1999em。图4 GELATO给出的分类及拟合结果（黑色：星明天文台获取的光谱；蓝色：II-P型超新星SN 1999em的光谱模板） 图5 Claudio Balcon（下）和星明天文台（上）的光谱分类报告 ...
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光谱显示出巴尔末发射线(Hα,Hβ,Hγ)，还有Fe II(42多重线)和Na I(D)和Si II(6347/6371Å)。S/N相对较差，但Na I D和Si II谱线显示出清晰的天鹅座P型星谱线轮廓。我们测量Hα线的半高全宽为2100km/s左右。这一光谱证实 AT 2020lye是M31中的新星，是Fe II类光谱的一员。 图4：ATel#13795原文 这是PSP项目2020年获得的第二颗发现。
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read=13337 ），证认该候选体为有着闪电离特征（flash-ionized signatures）的早期II型超新星；在TNS网页，该候选体被详细分类为II-pec型超新星，此候选体获得超新星正式编号 ...网页超新星分类及光谱等 以下为ATel #13337公报全文翻译（翻译：赵经远）： 丽江望远镜光谱将PSP19F（AT 2019wep）分类为有着闪电离特征的早期II ...蓝色连续谱与沃尔夫-拉叶星的突出狭窄发射线（例如He II，H I，C IV和N V）的光谱特征与有着相互作用特征的早期II型超新星一致。
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Properties of host galaxies of type II AGNs derived from 2D decomposition to their HST images using galfit ...
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5个小时后，他们将光谱数据及分类上传至TNS，证认这是一颗II型超新星，它的编号也变更为SN 2022yyz。几位老师在附注中写道：“基于丽江望远镜获得的红色无特征光谱，这可能是一颗相对早期的II型超新星，它被宿主星系强烈消光。红移由狭窄的Hα发射线得出。” 光谱及分类 SN 2022yyz所在的宿主星系UGC 11404曾在2012年11月也爆发过另一颗II型超新星，由徐智坚和高兴通过PSP的前身超新星与小行星搜寻项目（SASP .../followups/J19070073+2900166.html XM54ZX，星明天文台官网，http://xjltp.china-vo.org/徐智坚-xm54zx-sn2012gj-超新星-ii.html ...