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    Chapter and Conference Paper

    Observations of Supernova Remnants in the Large Magellanic Cloud with the Einstein Observatory

    As the nearest extragalactic system, the Large Magellanic Cloud (LMC) is destined to play a major role in understanding the X-ray emission from all normal galaxies including our own. Classed as a prototype Sb(...

    David J. Helfand, Knox S. Long in X-Ray Astronomy (1980)

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    Chapter and Conference Paper

    A Soft X-Ray Study of the Large Magellanic Cloud

    A survey of the Large Magellanic Cloud (LMC) has been carried out with the imaging X-ray telescope aboard the Einstein Observatory. Ninety-seven sources were detected. On statistical grounds, we estimate that les...

    David J. Helfand, Knox S. Long in X-Ray Astronomy (1981)

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    Chapter and Conference Paper

    An X-Ray Survey of Supernova Remnants in the Large Magellanic Cloud

    The last supernova (SN) observed in the Galaxy occurred ~375 years ago and it is clear that progress in SN research would be glacial at best if we were limited to the study of galactic events. Although the fir...

    David J. Helfand, Knox S. Long in Supernovae: A Survey of Current Research (1982)

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    Chapter and Conference Paper

    Extragalactic Supernova Remnants

    Because the supernova remnants (SNRs) in other galaxies are at well-defined distances and because in many cases the reddening within extragalactic samples is more uniform than is the case for the Galactic SNR ...

    Knox S. Long in X-Ray Astronomy in the Exosat Era (1985)

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    Chapter and Conference Paper

    A Comment on the Seyfert Environment

    The study on the Seyfert environment has been of considerable interest lately, since it is believed that the tidal force of a close companian may drive gas into the inner region and either fuel nuclear activit...

    Zou Zhen-long, Chen Jian-shen in Observational Cosmology (1987)

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    Chapter and Conference Paper

    The Two-Point Correlation Function of Groups in CFA Survey

    The power law form of the two-point spatial correlation function of groups of galaxies is observed among a statistically homogeneous group sample based on the CfA redshift survey. The correlation range is from...

    Zou Zhen-long, Liu Da-qing in High Energy Astrophysics (1988)

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    Chapter and Conference Paper

    Supernova Remnants and Candidates in M33

    Supernova remnants (SNRs) provide fundamental information about stellar evolution and the properties of the interstellar medium. The galactic sample of optical SNRs is large, but severely limited by obscuratio...

    R. Chris Smith, Robert P. Kirshner, P. Frank Winkler, Knox S. Long in Supernovae (1991)

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    Chapter and Conference Paper

    EUVE Observations of U Gem

    We have observed U Gem during the peak and declining phases of a wide outburst in 1993 December with EUVE. At peak, U Gem was one of the brightest EUV sources in the sky. The spectrum of the source is complex. Fi...

    Knox S. Long, Christopher W. Mauche, Paula Szkody, Janet A. Mattei in Cataclysmic Variables (1995)

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    Chapter and Conference Paper

    Far Ultraviolet Observations of Dwarf Novae made with the Hopkins Ultraviolet Telescope

    Observations with the Hopkins Ultraviolet Telescope on the Astro-1 and Astro-2 space shuttle missions have provided the first set of moderate (3 Å) resolution far ultraviolet (FUV) spectra of dwarf novae to in...

    Knox S. Long in Cataclysmic Variables and Related Objects (1996)

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    Chapter and Conference Paper

    Spectrally Resolved Maps of Optically Thick Accretion Disks

    We report first results of the HST/FOS time-resolved, low-resolution spectroscopy of the eclipsing cataclysmic variable UX UMa, including multi-wavelength map** of its accretion disk in the ultraviolet region.

    R. Baptista, K. Horne, I. Hubeny, K. Long in Cataclysmic Variables and Related Objects (1996)

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    Chapter and Conference Paper

    The EUVE Observations of Dwarf Novae

    In the standard theory of dwarf novae in outburst, the boundary layer region between the inner edge of the accretion disk and the white dwarf surface radiates primarily in the extreme ultraviolet. Using EUVE, obs...

    Knox S. Long in Astrophysics in the Extreme Ultraviolet (1996)

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    Chapter and Conference Paper

    Measuring the Galaxy Power Spectrum with Multiresolution Decomposition

    Yaoquan Chu, **aoHu Yang, Long-Long Feng in Statistical Challenges in Astronomy (2003)

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    Chapter and Conference Paper

    An Automatic Precise Registration Method Based on the Relative Geometric Calibration Between Bands for Satellite Multi-spectral Image

    A registration method for satellite multi-spectral image is proposed, which is based on the relative geometric calibration between bands. This method precisely calibrate the relative geometric distortion of re...

    He Wei, Long **aoxiang, Yu **g, Zhang Chi in 3rd International Symposium of Space Optic… (2017)

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    Chapter and Conference Paper

    Overview of High-Precision Spectral Payload On-Orbit Radiometric Calibration

    High-precision spectral payload during the track performance changes occur, and there for need to be calibrated by on-orbit radiation calibration technology. This paper describes several types of on-orbit radi...

    Shaofan Tang, Long Chen, Huan Li, Zhi Jun Lu in 4th International Symposium of Space Optic… (2018)

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    Chapter and Conference Paper

    Micro-Vibration Environment Parameters Measurement and Analysis of a Novel Satellite in Orbit

    The in-orbit remote sensing results of optical payloads on a novel kind of satellite are affected obviously by the micro-vibration environment in the satellite platform, and it is needed to suppress and compen...

    Pan-feng Wu, Zhen-long Xu, **ao-yu Wang in 5th International Symposium of Space Optic… (2020)

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    Chapter and Conference Paper

    Design of Lobster-Eye Focusing System for Dark Matter Detection

    Dark matter and dark energy are recognized as “Two dark clouds shrouded in the clear sky of physics in the twenty-first century.” Experimental and theoretical exploration of dark matter and dark energy will gr...

    Yun Su, **anmin Wu, Long Dong, Hong Lv in 5th International Symposium of Space Optic… (2020)

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    Chapter and Conference Paper

    Analysis of Straylight for the Green House Gas Instrument

    The Green House Gas Instrument (GHGI) is an imaging spectrometer, which has four spectrum bands within 0.75 ~ 2.38 μm. This paper discussed the stray light performance of GHGI. Because the straylight requireme...

    Long Ma in 6th International Symposium of Space Optical Instruments and Applications (2021)