论文标题

安魂曲2D:HST 2D Grism光谱法的空间分辨出恒星种群

REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy

论文作者

Akhshik, Mohammad, Whitaker, Katherine E., Brammer, Gabriel, Mahler, Guillaume, Sharon, Keren, Leja, Joel, Bayliss, Matthew B., Bezanson, Rachel, Gladders, Michael D., Man, Allison, Nelson, Erica J., Rigby, Jane R., Rizzo, Francesca, Toft, Sune, Wellons, Sarah, Williams, Christina C.

论文摘要

我们提出了一种新型的贝叶斯方法,以共同模拟高红移星系的光度法和深哈勃太空望远镜(HST)2D Grism光谱。我们的Rembiem2D代码衡量了尚未解决和分辨的恒星种群,年龄和恒星形成历史(SFHS),以实现持续的重新QIUEM(解决静态放大)星系调查,该测量针对Z〜2处的强烈重力镜头的Quiescent Galaxies。我们使用Illustris宇宙学模拟中的Z〜2大型星系样本来测试\ texttt {requiem2d}的准确性,发现我们恢复了SFH和中位数恒星年龄的一般趋势。我们进一步介绍了一项针对Requiem Galaxies调查的试点研究:MRG-S0851,一项典范,大规模($ \ log m_* / m_* / m_* / m_ \ odot = 11.02 \ pm 0.04 $)$ z = 1.883 \ pm 0.001 $。估计的重力放大倍数为$μ= 5.7^{+0.4} _ { - 0.2} $,我们在0.6 kpc物理尺寸箱上采样了恒星种群。全球大规模加权的中位年龄约为$ 1.8 _ { - 0.2}^{+0.3} $ gyr,我们的空间解决分析表明,MRG-S0851在内部3 kpc的核心中具有统一的统一梯度,并考虑到对年龄和金属对年龄测量的微妙效果,对年龄的测量效果,有利于早期的形式,有利于早期形式的表现。完整的Requiem-2D样本的分析将在即将发表的论文中介绍,并释放Anceem2D代码的Beta-Release。

We present a novel Bayesian methodology to jointly model photometry and deep Hubble Space Telescope (HST) 2d grism spectroscopy of high-redshift galaxies. Our requiem2d code measures both unresolved and resolved stellar populations, ages, and star-formation histories (SFHs) for the ongoing REQIUEM (REsolving QUIEscent Magnified) Galaxies Survey, which targets strong gravitationally lensed quiescent galaxies at z~2. We test the accuracy of \texttt{requiem2d} using a simulated sample of massive galaxies at z~2 from the Illustris cosmological simulation and find we recover the general trends in SFH and median stellar ages. We further present a pilot study for the REQUIEM Galaxies Survey: MRG-S0851, a quintuply-imaged, massive ($\log M_* / M_\odot = 11.02 \pm 0.04$) red galaxy at $z=1.883\pm 0.001$. With an estimated gravitational magnification of $μ= 5.7^{+0.4}_{-0.2}$, we sample the stellar populations on 0.6 kpc physical size bins. The global mass-weighted median age is constrained to be $1.8_{-0.2}^{+0.3}$ Gyr, and our spatially resolved analysis reveals that MRG-S0851 has a flat age gradient in the inner 3 kpc core after taking into account the subtle effects of dust and metallicity on age measurements, favoring an early formation scenario. The analysis for the full REQUIEM-2D sample will be presented in a forthcoming paper with a beta-release of the requiem2d code.

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