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Are James Webb Space Telescope Observations Consistent with Warm Dark Matter?
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作者 Bruce Hoeneisen 《International Journal of Astronomy and Astrophysics》 2024年第1期45-60,共16页
We compare observed with predicted distributions of galaxy stellar masses M<sub>* </sub>and galaxy rest-frame ultra-violet luminosities per unit bandwidth L<sub>UV</sub>, in the redsh... We compare observed with predicted distributions of galaxy stellar masses M<sub>* </sub>and galaxy rest-frame ultra-violet luminosities per unit bandwidth L<sub>UV</sub>, in the redshift range z=2 to 13. The comparison is presented as a function of the comoving warm dark matter free-streaming cut-off wavenumber k<sub>fs</sub>. For this comparison the theory is a minimal extension of the Press-Schechter formalism with only two parameters: the star formation efficiency, and a proportionality factor between the star formation rate per galaxy and LUV</sub>. These two parameters are fixed to their values obtained prior to the James Webb Space Telescope (JWST) data. The purpose of this comparison is to identify if, and where, detailed astrophysical evolution is needed to account for the new JWST observations. 展开更多
关键词 James Webb space Telescope JWST Warm Dark Matter
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Two suggested configurations for the Chinese space telescope 被引量:2
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作者 Ding-Qiang Su Xiang-Qun Cui 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2014年第9期1055-1060,共6页
China will establish a 2-meter space-based astronomical telescope. Its main science goals are performing a sky survey for research about dark matter and dark energy, and high resolution observations. Some experts sugg... China will establish a 2-meter space-based astronomical telescope. Its main science goals are performing a sky survey for research about dark matter and dark energy, and high resolution observations. Some experts suggest that this space telescope should be installed inside the Chinese space station. In accord with this suggestion we put forward our first configuration, i.e., to adopt a coude system for this telescope. This coude system comes from the Chinese 2.16 m telescope's coude system, which includes a relay mirror so that excellent image quality can be obtained. In our second configuration, we suggest that the whole space telescope fly freely as an independent satellite outside the space station. When it needs servicing, for example, changing in- struments, refilling refrigerant or propellant, etc., this space telescope can fly near or even dock with the core space station. Although some space stations have had accom- panying satellites, the one we propose is a space telescope that will be much larger than other accompanying satellites in terms of weight and volume. On the basis of the second configuration, we also put forward the following idea: the space station can be composed of several large independent modules if necessary. 展开更多
关键词 instruments -- space telescope -- space station -- survey -- high angu- lar resolution
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Presentation on the Electronic Control System of Space Solar Telescope
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作者 Zhang Bin, Li Wei, Song Guofeng, Jin Shengzhen 1 (Beijing Astronomical Observatory, The Chinese Academy of Sciences, Beijing 100012, China) 2 (National Astronomical Observatories, Beijing 100012, China) 《天文研究与技术》 CSCD 1999年第S1期130-133,共4页
This paper gives the brief view of the electronic control system of SPACE SOLAR TELESCOPE (SST), especially the On Board Data Handling unit (OBDH) on the SST which control the operation of the instrument, acquire data... This paper gives the brief view of the electronic control system of SPACE SOLAR TELESCOPE (SST), especially the On Board Data Handling unit (OBDH) on the SST which control the operation of the instrument, acquire data and make data analysis and storage. In OBDH, the Scientific Data Unit (SDU) is a special unit that requires high speed computer. In this paper gives a brief comparison of two possible choices and discuss selection of electronic parts in the space environment. 展开更多
关键词 Presentation on the Electronic Control System of space Solar Telescope
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Korean Participation in the Galex Ultraviolet Space Telescope Project
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作者 Young Wook Lee (Center for Space Astrophysics, Yonsei University, Seoul 120-749, Korea) 《天文研究与技术》 CSCD 1999年第S1期8-10,共3页
The Center for Space Astrophysics at Yonsei university, Seoul, Korea, is actively participating in the development and operation of the Galaxy Evolution Explorer (GALEX), a NASA ultraviolet space telescope project to ... The Center for Space Astrophysics at Yonsei university, Seoul, Korea, is actively participating in the development and operation of the Galaxy Evolution Explorer (GALEX), a NASA ultraviolet space telescope project to be launched in late 2001. As the first official case of NASA Korea cooperation on major space science program, this project will greatly expand the capability of Korean astronomy into space based operations. 展开更多
关键词 Korean Participation in the Galex Ultraviolet space Telescope Project
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Photometric Calibration of the Lunar-based Ultraviolet Telescope for Its First Six Months of Operation on the Lunar Surface 被引量:3
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作者 Jing Wang Li Cao +10 位作者 Xian-Min Meng Hong-Bo Cai Jing-Song Deng Xu-Hui Han Yu-Lei Qiu Fang Wang Shen Wang Wei-Bin Wen Chao Wu Jian-Yan Wei Jing-Yao Hu 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2015年第7期1068-1076,共9页
We describe the photometric calibration of the Lunar-based Ultraviolet Telescope(LUT), the first robotic astronomical telescope working on the lunar surface, for its first six months of operation on the lunar surfac... We describe the photometric calibration of the Lunar-based Ultraviolet Telescope(LUT), the first robotic astronomical telescope working on the lunar surface, for its first six months of operation on the lunar surface. Two spectral datasets(set A and B) from near-ultraviolet(NUV) to the optical band were constructed with 44 International Ultraviolet Explorer(IUE) standards, because of the LUT's relatively wide wavelength coverage. Set A was obtained by extrapolating the IUE NUV spectra(λ 〈 3200 ) to the optical band based upon the theoretical spectra of stellar atmosphere models. Set B was composed of theoretical spectra from 2000 to 8000 extracted from the same model grid. In total, seven standards have been observed in15 observational runs until May 2014. The calibration results show that the photometric performance of LUT is highly stable in its first six months of operation. The magnitude zero points obtained from the two spectral datasets are also consistent with each other, i.e., zp = 17.54 ± 0.09 mag(set A) and zp = 17.52 ± 0.07 mag(set B). 展开更多
关键词 space vehicles: instruments -- telescopes -- techniques: photometric --ultraviolet: general
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JWST Discoveries—Confirmation of World-Universe Model Predictions
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2022年第4期1134-1154,共21页
In 1937, P. Dirac proposed the Large Number Hypothesis and Hypothesis of Variable Gravitational Constant [1], and later added notion of Continuous Creation of Matter in the World [2]. Developed Hypersphere World-Unive... In 1937, P. Dirac proposed the Large Number Hypothesis and Hypothesis of Variable Gravitational Constant [1], and later added notion of Continuous Creation of Matter in the World [2]. Developed Hypersphere World-Universe Model (WUM) follows these ideas, albeit introducing different mechanism of Matter creation. Most direct observational evidence of validity of WUM are: 1) Microwave Background Radiation and Intergalactic Plasma speak in favor of existence of Medium;2) Laniakea Supercluster with binding mass ~10<sup>17</sup>M<sub>&odot;</sub> is home to Milky Way (MW) galaxy and ~10<sup>5</sup> other nearby galaxies, which did not start their movement from Initial Singularity (see Figure 1);3) MW is gravitationally bounded with Virgo Supercluster (VSC) and has Orbital Angular Momentum calculated based on distance of 65 Mly from VSC and orbital speed of ~400 km·s<sup>-1</sup>, which far exceeds rotational angular momentum of MW;4) Mass-to-light ratio of VSC is ~300 times larger than that of Solar ratio. Similar ratios are obtained for other superclusters (see Figure 2). These ratios are main arguments in favor of the presence of tremendous amounts of Dark Matter (DM) in the World. JWST discoveries confirm the most important predictions of WUM in 2018: 1) Absolute Age of World is 14.22 Gyr;2) Dark Epoch (spanning for Laniakea Supercluster (LSC) from the Beginning of World for 0.45 Gyr) when only DM Macroobjects (MOs) form and evolve;3) Luminous Epoch (ever since, 13.77 Gyr for LSC) when Luminous MOs (superclusters, galaxies, extrasolar systems, etc.) emerge;4) Transition from Dark Epoch to Luminous Epoch is due to Explosive Rotational Fission of Overspinning (surface speed at equator exceeding escape velocity) DM Supercluster’s Cores and self-annihilation of DM Particles (DMPs);5) MOs of World form from top (Superclusters) down to Galaxies and Extrasolar systems in parallel around different Cores made up of different DMPs;6) 3D Finite Boundless World presents a Patchwork Quilt of different Luminous Superclusters, which emerged in different places of World at different Cosmological times. 展开更多
关键词 James Webb space Telescope World-Universe Model Medium Angular Momentum Dark Matter Dark Epoch Luminous Epoch Rotational Fission Patchwork Quilt Early-Galaxies Inter-Connectivity of Primary Cosmological Parameters
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The first comprehensive Milky Way stellar mock catalogue for the Chinese Space Station Telescope Survey Camera
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作者 Yang Chen Xiaoting Fu +9 位作者 Chao Liu Piero Dal Tio Léo Girardi Giada Pastorelli Alessandro Mazzi Michele Trabucchi Hao Tian Dongwei Fan Paola Marigo Alessandro Bressan 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2023年第11期206-220,共15页
The Chinese Space Station Telescope(CSST)is a cutting-edge two-meter astronomical space telescope currently under construction.Its primary Survey Camera(SC)is designed to conduct large-area imaging sky surveys using a... The Chinese Space Station Telescope(CSST)is a cutting-edge two-meter astronomical space telescope currently under construction.Its primary Survey Camera(SC)is designed to conduct large-area imaging sky surveys using a sophisticated seven-band photometric system.The resulting data will provide unprecedented data for studying the structure and stellar populations of the Milky Way.To support the CSST development and scientific projects related to its survey data,we generate the first comprehensive Milky Way stellar mock catalogue for the CSST SC photometric system using the TRILEGAL stellar population synthesis tool.The catalogue includes approximately 12.6 billion stars,covering a wide range of stellar parameters,photometry,astrometry,and kinematics,with magnitude reaching down to g=27.5 mag in the AB magnitude system.The catalogue represents our benchmark understanding of the stellar populations in the Milky Way,enabling a direct comparison with the future CSST survey data.Particularly,it sheds light on faint stars hidden from current sky surveys.Our crowding limit analysis based on this catalogue provides compelling evidence for the extension of the CSST Optical Survey(OS)to cover low Galactic latitude regions.The strategic extension of the CSST-OS coverage,combined with this comprehensive mock catalogue,will enable transformative science with the CSST. 展开更多
关键词 The Chinese space Station Telescope(CSST) stellar content and populations Milky Way sky surveys
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Black holes as the source of dark energy:A stringent test with high-redshift JWST AGNs
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作者 Lei Lei Lei Zu +12 位作者 Guan-Wen Yuan Zhao-Qiang Shen Yi-Ying Wang Yuan-Zhu Wang Zhen-Bo Su Wen-Ke Ren Shao-Peng Tang Hao Zhou Chi Zhang Zhi-Ping Jin Lei Feng Yi-Zhong Fan Da-Ming Wei 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2024年第2期181-188,共8页
Studies have proposed that there is evidence for cosmological coupling of black holes(BHs)with an index of k≈3;hence,BHs serve as the astrophysical source of dark energy.However,the data sample is limited for the red... Studies have proposed that there is evidence for cosmological coupling of black holes(BHs)with an index of k≈3;hence,BHs serve as the astrophysical source of dark energy.However,the data sample is limited for the redshifts of≤2.5.In recent years,the James Webb Space Telescope(JWST)has detected many high-redshift active galactic nuclei(AGNs)and quasars.Among the JWST NIRSpec-/NIRCam-resolved AGNs,three are determined to be in early-type host galaxies with a redshift of z~4.5-7.However,their M_(*)and MBH are in tension with the predicted cosmological coupling of black holes with k=3 at a confidence level of~2σ,which challenges the hypothesis that BHs serve as the origin of dark energy.Future work on high-redshift AGNs using the JWST will further assess such a hypothesis by identifying more early-type host galaxies in the higher mass range. 展开更多
关键词 dark energy supermassive black hole active galactic nuclei James Webb space Telescope
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Deployment dynamics for flexible deployable primary mirror of space telescope with paraboloidal and laminated structure by using absolute node coordinate method 被引量:4
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作者 Bindi YOU Dong LIANG +1 位作者 Xiangjie YU Xiaolei WEN 《Chinese Journal of Aeronautics》 SCIE EI CAS CSCD 2021年第4期306-319,共14页
A nonlinear dynamic modeling method for primary mirror of Flower-like Deployable Space Telescope(F-DST)undergoing large deployment motion is proposed in this paper.To ensure pointing accuracy and attitude stability of... A nonlinear dynamic modeling method for primary mirror of Flower-like Deployable Space Telescope(F-DST)undergoing large deployment motion is proposed in this paper.To ensure pointing accuracy and attitude stability of the paraboloidal primary mirror,the mirror is discretized into equal thickness shell elements by considering shell curvature.And the material nonlinear constitutive relation of flexible mirror is acquired using Absolute Nodal Coordinate Formulation(ANCF).Furthermore,the primary mirror of F-DST can be regarded as a clustered multi-body system,and its dynamic equations of elastic deformation and deployment motion are established by virtual work principle.Finally,the deployment motion of primary mirror by different driving conditions are simulated,the results show that the vibrations of mirrors that driven by elastic hinge device are more than that driven by servo motor.In addition,single sub-mirror deployment process will perturb the pointing accuracy of primary mirror,and the multiple sub-mirrors simultaneously deploying will seriously affect all the sub-mirrors surface accuracy because of the coupling effect.Thus,there are theoretical value and practical significance for the controlling surface accuracy and attitude accuracy of space telescope. 展开更多
关键词 Deployable space telescope Deployment dynamics Flexible deformation Laminated mirror Paraboloidal structure
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The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies 被引量:3
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作者 Ziwei Wang Lei Lei +2 位作者 Hao Jiao Lei Feng Yi-Zhong Fan 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2023年第12期11-19,共9页
Recently,pulsar timing array(PTA)experiments have provided compelling evidence for the existence of the nanohertz stochastic gravitational wave background(SGWB).In this work,we demonstrated that cosmic string loops ge... Recently,pulsar timing array(PTA)experiments have provided compelling evidence for the existence of the nanohertz stochastic gravitational wave background(SGWB).In this work,we demonstrated that cosmic string loops generated from cosmic global strings offer a viable explanation for the observed nanohertz SGWB data,requiring a cosmic string tension parameter of log(Gμ)~-12 and a loop number density of log N~4.Additionally,we revisited the impact of cosmic string loops on the abundance of massive galaxies at high redshifts.However,our analysis revealed challenges in identifying a consistent parameter space that can concurrently explain both the SGWB data and observations from the James Webb Space Telescope.This indicates the necessity for either extending the existing model employed in this research or acknowledging distinct physical origins for these two phenomena. 展开更多
关键词 nanohertz stochastic gravitational-wave background cosmic string loop JamesWebb space Telescope galaxy formation
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基于单向饱和绳索作动器的大型太空望远镜桁架的振动主动控制
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作者 唐颖卓 刘晓峰 +1 位作者 蔡国平 刘翔 《Acta Mechanica Sinica》 SCIE EI CAS CSCD 2022年第9期117-129,共13页
由于质量轻、易于折叠展开、光学成像精度高等显著优势,近年来大型薄膜衍射太空望远镜已经成为对地观测领域的研究热点之一.大型太空望远镜在太空中受到外界扰动或在进行姿态调整时,不可避免地会发生一定程度的振动,从而影响对地成像精... 由于质量轻、易于折叠展开、光学成像精度高等显著优势,近年来大型薄膜衍射太空望远镜已经成为对地观测领域的研究热点之一.大型太空望远镜在太空中受到外界扰动或在进行姿态调整时,不可避免地会发生一定程度的振动,从而影响对地成像精度.因此,为了满足成像精度要求,有必要采取合适的控制方法来快速抑制太空望远镜的有害振动.本文采用主动绳索作为作动器对大型太空望远镜进行振动主动控制研究.由于绳索存在可受拉不可受压且受拉能力有限的特性,本文在控制设计时考虑了绳索作动器的单向性和饱和性.首先,采用有限元方法建立了薄膜衍射太空望远镜的动力学模型.其次,结合二次线性调节器和bangbang调节器,构造了一个分段代价函数来设计结构的振动主动控制律.接着,采用可控性准则和遗传算法进行了绳索作动器的最优位置布置.最后,通过数值模拟验证了所提出的控制方法的有效性.模拟结果表明,采用本文设计的控制方法可有效抑制太空望远镜的振动,并且给出了满足望远镜成像要求的绳索作动器的最少数量及其位置分布. 展开更多
关键词 Membrane diffraction space telescope Cable actuator Position optimization Vibration control
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