Overlap Zoo Beta: A Catalogue of ~800 Occulting Pairs in the DESI Legacy Survey using Citizen Science
University of Louisville（路易斯维尔大学）；University of Alabama（阿拉巴马大学）；Northern Kentucky University（北肯塔基大学）
T. Butrum, B. Holwerda, W. C. Keel, C. Robertson, I. Castellano, S. Pandey, S. M. R. Adnan, L. C. Bills, D. Patel, K. Cook, T. Hardin, A. Palao, B. Connelly, M. Morton
备注：
15 pages, 7 figures, 8 tables, and a link to the catalogue included. Soon to be published in PASA
Overlapping galaxies, in which a foreground galaxy partially overlaps a background galaxy, offer a unique opportunity to measure dust attenuation, a key nuisance parameter in galaxy studies, empirically and in great detail by modelling the light of both the foreground and background galaxy and inferring the missing light in the overlapping region. However, the current catalogue of overlapping pairs is relatively limited in number compared to catalogues dedicated to individual galaxies. Expanding this catalogue is not only a necessity to facilitate further detailed dust studies beyond the few limited studies conducted thus far, but also to improve pair-to-pair variance and support automated identification through machine learning techniques. To achieve this, we utilise galaxies classified as "overlapping" from Galaxy Zoo DECaLS (GZD-1, -2, and -5), along with images from Data Release 10 (DR10) of the DESI Legacy Survey, in our individual citizen science project to classify these pairs directly using volunteers. This new catalogue will not only provide a wealth of targets for future dust studies but will also contribute to a deeper understanding of these pairs and dust as a whole.
Specific Star Formation Rate Enhancement across the Galaxy Merger Sequence: Insights from Citizen Science Classifications
Minnetonka High School（明尼通卡高中）；Minnesota Institute for Astrophysics, University of Minnesota（明尼苏达大学天体物理研究所）；Department of Physics & Astronomy, University of Missouri Kansas City（密苏里大学堪萨斯城分校物理与天文系）；Missouri Institute for Defense & Energy (MIDE)（密苏里国防与能源研究所）
Gems of the Galaxy Zoos -- a Wide-Ranging Hubble Space Telescope Gap-Filler Program
我们描述了银河系动物园的宝石（动物园宝石）项目，一个填补空白的项目，在哈勃太空望远镜的时间表中使用短窗口。与以前的快照计划一样，目标是根据位置从一个池中提取的;我们结合了志愿者在银河动物园和无线电银河动物园公民科学项目中选择的对象。Zoo Gems使用Advanced Camera for Surveys（ACS）的曝光来解决星系形态，星际介质内容，活动星系核的宿主星系和星系演化等广泛的主题。科学案例包括研究星系的相互作用，星系中的背光尘埃，星暴后系统，环和特殊的螺旋图案，通常的颜色-形态关系的异常值，绿豆紧凑的星暴系统，螺旋宿主星系的双射电源，以及活动星系核周围的扩展发射线区域。对于这些科学类别中的许多类别，从更大的列表中最终选择目标是通过投票过程使用公众输入。到目前为止的亮点包括在蓝色的，显然是早期类型的星系中紧密缠绕的螺旋结构的流行，一个几乎完整的爱因斯坦环从一个群透镜，在较低的表面亮度周围的紧凑的绿豌豆星爆的红色组件，以及螺旋星系托管大型双射电源的高概率例子。
Galaxy Zoo: Cosmic Dawn -- morphological classifications for over 41,000 galaxies in the Euclid Deep Field North from the Hawaii Two-0 Cosmic Dawn survey
The Open University（开放大学）；University of Toronto（多伦多大学）；University of Minnesota（明尼苏达大学）；European Space Agency (ESA)（欧洲航天局）；Haverford College（哈弗福德学院）；Lancaster University（兰卡斯特大学）；University of Oxford（牛津大学）
Citizen Science Research with the Square Kilometre Array Observatory (SKAO)
UM-DAE Centre for Excellence in Basic Sciences, University of Mumbai（孟买大学基础科学卓越中心）；Centre for Excellence in Theoretical and Computational Science, University of Mumbai（孟买大学理论与计算科学卓越中心）；Astrophysics Division, National Centre for Nuclear Research（国家核研究中心天体物理部）；School of Physical Sciences, The Open University（开放大学物理科学学院）；Department of Pure and Applied Sciences, Midnapore City College（金德尔布尔城市学院纯科学与应用科学系）；Space Radio-Diagnostics Research Centre, University of Warmia and Mazury（瓦尔米亚和马祖里大学空间无线电诊断研究中心）；Astronomical Observatory, Jagiellonian University（雅盖隆大学天文台）；Center for Astrophysics, Gravitation and Cosmology, Shri Ramasamy Memorial (SRM) University Sikkim（锡金斯里·拉玛萨米纪念大学天体物理、引力和宇宙学中心）；Department of Physics, Shri Ramasamy Memorial (SRM) University Sikkim（锡金斯里·拉玛萨米纪念大学物理系）
Deep Learning Segmentation of Spiral Arms and Bars for 600,000 Galaxies in DESI
University of Hertfordshire（赫特福德大学）；Dunlap Institute for Astronomy and Astrophysics, University of Toronto（多伦多大学邓普天体物理研究所）；Jodrell Bank Centre for Astrophysics, Department of Physics & Astronomy, University of Manchester（曼彻斯特大学物理与天文系乔德雷克天体物理学中心）；Department of Physics and Astronomy, Haverford College（哈弗福德学院物理与天文系）；Masaryk University（马萨里克大学）；Lancaster University（兰卡斯特大学）；The Open University（开放大学）
From Galaxy Zoo DECaLS to BASS/MzLS: detailed galaxy morphology classification with unsupervised domain adaption
Shanghai Astronomical Observatory, Chinese Academy of Sciences（中国科学院上海天文台）；School of Astronomy and Space Science, University of Chinese Academy of Sciences（中国科学院大学天文与空间科学学院）；Shanghai Key Lab for Astrophysics, Shanghai Normal University（上海师范大学上海市天体物理重点实验室）；Centre for Astrophysics Research, University of Hertfordshire（赫特福德大学天体物理研究中心）
Fishing for Jellyfish Galaxies: Exploring ram-pressure stripping with crowd science
INAF- Osservatorio astronomico di Padova（意大利国家天体物理研究所帕多瓦天文台）；University of Nottingham（诺丁汉大学）；Universidad Técnica Federico Santa María（费德里科·圣玛丽亚技术大学）；Millennium Nucleus for Galaxies (MINGAL)（银河系千年核）；University of Birmingham（伯明翰大学）
