论文标题
Pan-Starrs调查(EGIPS)中的边缘星系
The Edge-on Galaxies in the Pan-STARRS survey (EGIPS)
论文作者
论文摘要
我们提出了使用Pan-Starrs调查的公共DR2数据创建的16551个边缘星系的目录。目录覆盖了DEC上方的天空的四分之三= -30度。使用卷积神经网络选择了星系,该网络对SDSS调查前面确定的边缘星系样本进行了训练。这种方法使我们能够在合理的时间内显着提高候选人选择的质量并进行彻底的视觉检查。该目录提供了有关星体的星体测量值和非参数形态统计的同质信息。对于13.8-17.4 R波段幅度范围内的物体,光度法是可靠的。根据HyperLeDA数据库,红移以目录中约63%的星系而闻名。我们的样本已很好地分为红色序列和蓝色云星系种群。红色序列的边缘星系系统地是Delta(G-I)〜0.1 MAG红色,而与观察者的任意角度相比,标准的星系相比。我们发现了星系颜色的星系厚度变化。红色序列星系比蓝色云的星系厚。在蓝云中,平均而言,较薄的星系变成了蓝色。将来,基于此目录,它旨在探索不同形态的星系的三维结构,并研究圆盘和凸起的缩放关系。
We present a catalogue of 16551 edge-on galaxies created using the public DR2 data of the Pan-STARRS survey. The catalogue covers the three quarters of the sky above Dec.=-30 degrees. The galaxies were selected using a convolutional neural network, trained on a sample of edge-on galaxies identified earlier in the SDSS survey. This approach allows us to dramatically improve the quality of the candidate selection and perform a thorough visual inspection in a reasonable amount of time. The catalogue provides homogeneous information on astrometry, SExtractor photometry, and non-parametric morphological statistics of the galaxies. The photometry is reliably for objects in the 13.8-17.4 r-band magnitude range. According to the HyperLeda database, redshifts are known for about 63 percent of the galaxies in the catalogue. Our sample is well separated into the red sequence and blue cloud galaxy populations. The edge-on galaxies of the red sequence are systematically Delta(g-i)~0.1 mag redder than galaxies oriented at an arbitrary angle to the observer. We found a variation of the galaxy thickness with the galaxy colour. The red sequence galaxies are thicker than the galaxies of the blue cloud. In the blue cloud, on average, thinner galaxies turn out to be bluer. In the future, based on this catalogue it is intended to explore the three-dimensional structure of galaxies of different morphologies, as well as to study the scaling relations for discs and bulges.