"An atlas of color-selected quiescent galaxies at z>3 in public JWST fields" (Supplementary material)
收藏资源简介：
The files are organized as follows: 0) "<em>readme_atlas_jwst_paper.txt"</em><br> This file describes the content of the file "<em>supplementary_atlas_jwst_paper.tar</em>" containing supplementary figures and tables for the manuscript <em>"An atlas of color-selected quiescent galaxies at z>3 in public JWST fields" </em>by Valentino, Brammer, Gould et al. (2023, ApJ).<br> The information is also provided here below. 1) supplementary_figures/ 1.1) Depth in NIRCam/F150W, F200W, F277W, and F356W equivalent to Figure A.1 in Appendix A: f150w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png f200w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png f277w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png f356w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png These figures are also collected in a Figure Set available on the journal webpage. 1.2) Comoving number densities of <em>UVJ</em>-selected galaxies falling in the standard selection box by Williams+2009 and not accounting for the uncertainties on colors: uvj_number_densities_mass_bins_strict_nouncertainties.png The purple and green colors mark the <em>p(z)</em> of individual robust "standard" <em>UVJ</em> quiescent candidates with M* ≥ 10<sup>10.6</sup> M<sub>⊙</sub> and 10<sup>9.5</sup> ≤ M* < 10<sup>10.6</sup> M<sub>⊙</sub>, respectively. The <em>p(z) </em>are normalized by their area (∫<sub>z</sub> <em>p(z)</em> d<em>z</em> = 1). The sky coverage of each field is as labeled. We included the effect of gravitational lensing at these redshifts in the calculation of the areas around galaxy clusters (Sunrise, SMACS0723), for which the masses should be intended as observed (not delensed). The comoving number densities in units of 10<sup>-5</sup> Mpc<sup>-3</sup> obtained from the integration of <em>p(z)</em> within the 3 < <em>z</em> < 4, 4 < <em>z</em> < 5, and 5 < <em>z</em> < 6.5 bins marked by dotted lines are reported. The errors mark the 68% Poissonian confidence intervals. Estimates of the uncertainties from bootstrapping are within brackets. The first and second rows indicate <em>n</em> in the 10<sup>9.5</sup> ≤ M* < 10<sup>10.6 </sup>M<sub>⊙</sub> and M* ≥ 10<sup>10.6</sup> M⊙ bins, respectively. 2) uvj/ Folder containing the SEDs (seds/) and positions in the <em>UVJ</em> diagram (uvj_single/) of the UVJ-selected samples described in the manuscript. The latter include both the initial pool of candidates and the visually selected sample. Tables containing the basic properties of both samples described in the text are available in fits and html formats. By downloading the folder and clicking on the .html tables, the reader can visualize the content in a web browser. This feature allows to automatically visualize the properties, SEDs, position in the <em>UVJ</em> diagram, and generate RGB cutouts in the SW and LW NIRCam channels on-the-fly. The latter operation takes a few seconds. A .reg file compatible with DS9 is provided for the visually selected sample. The coordinates are aligned with GAIA DR3. 3) nuvuvj/ The content is similar to that of the uvj/ folder, but for the <em>NUVUVJ</em> selection in Gould, Brammer, Valentino et al. (2023, ApJ). Separate tables for "robust" and "probable" samples before and after the visual inspections are distributed in .fits and .html format. 4) carnall22_selection/ The content is similar to that of the nuvuvj/ folder, but for the sample selected by Carnall, McLeod, McLure et al. 2023 (2023MNRAS.tmp..383C, arXiv:2208.00986). The information is provided to allow for a rapid comparison with this work. <br> For further information or details, please write at: francesco.valentino@eso.org.
文件组织方式如下： 0) readme_atlas_jwst_paper.txt 该文件用于说明压缩包supplementary_atlas_jwst_paper.tar的内容，此包包含Valentino、Brammer、Gould等人于2023年发表在《天体物理学杂志》（Astrophysical Journal，ApJ）的论文《公共詹姆斯·韦布空间望远镜（James Webb Space Telescope，JWST）天区中z>3的颜色选择静止星系星表》的补充图表与表格。相关信息也将在下文呈现。 1) supplementary_figures/ 目录 1.1) 近红外相机（Near InfraRed Camera，NIRCam）F150W、F200W、F277W及F356W波段的深度信息，对应附录A中的图A.1，相关图像文件包括：f150w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png、f200w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png、f277w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png、f356w_flux_aper_1_observed_magnitude_sn_5.0_completeness_kde_allfields.png。上述图表也可在期刊官网的图表集中获取。 1.2) 落入Williams等人2009年提出的标准选择框内、未考虑颜色不确定性的UVJ色指数图（UVJ diagram，简称UVJ）选择星系的共动数密度，对应图像文件为uvj_number_densities_mass_bins_strict_nouncertainties.png。其中紫色与绿色分别标记恒星质量M* ≥ 10^10.6 M☉与10^9.5 ≤ M* < 10^10.6 M☉的单个稳健“标准”UVJ静止候选体的红移概率分布p(z)。所有p(z)均按其面积归一化（∫_z p(z) dz = 1）。每个天区的覆盖范围如标注所示。我们在星系团（Sunrise、SMACS0723）周边区域的面积计算中纳入了该红移处的引力透镜效应，此处的星系质量均为观测质量（未做透镜去偏置处理）。文中给出了在3<z<4、4<z<5及5<z<6.5红移区间内对p(z)积分得到的共动数密度，单位为10^-5 Mpc^-3，以虚线标注。误差棒代表68%泊松置信区间，自助法（bootstrapping）估算的不确定性以方括号标注。第一行与第二行分别对应10^9.5 ≤ M* < 10^10.6 M☉与M* ≥ 10^10.6 M☉的质量区间的数密度n。 2) uvj/ 目录 该目录包含论文中描述的UVJ选择样本的光谱能量分布（Spectral Energy Distribution，SED）文件（位于seds/子目录）以及UVJ色指数图中的位置信息（位于uvj_single/子目录），其中既包含初始候选体池，也包含目视选择的样本。文中提及的两类样本的基本属性表格以fits与html格式提供。下载该目录并点击html表格后，读者可在网页浏览器中查看表格内容，该功能可自动可视化天体的各项属性、SED、UVJ色指数图中的位置，并实时生成NIRCam短波段（SW）与长波段（LW）通道的RGB截图像，该操作耗时约数秒。针对目视选择的样本，还提供了兼容DS9天文图像查看软件的.reg文件，其坐标与盖亚第三版数据发布（GAIA Data Release 3，GAIA DR3）对齐。 3) nuvuvj/ 目录 该目录内容与uvj/类似，但对应Gould、Brammer、Valentino等人2023年发表在ApJ的论文中采用的NUVUVJ选择样本。针对目视检查前后的“稳健”与“疑似”样本，分别提供了.fits与.html格式的独立表格。 4) carnall22_selection/ 目录 该目录内容与nuvuvj/类似，但对应Carnall、McLeod、McLure等人2023年发表的样本（2023MNRAS.tmp..383C, arXiv:2208.00986）。提供该数据集旨在方便与本研究进行快速对比。 如需进一步咨询或获取详细信息，请致邮：francesco.valentino@eso.org。
