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Cited article:

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A colourful analysis: Probing the eclipse of the black hole and central engine in NGC 6814 using X-ray colour–colour grids

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Variable Magellanic HMXB Sources versus Variable ULX Sources: Nothing to Brag about the ULX Sources

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Color–color diagrams as tools for assessment of the variable absorption in high mass X-ray binaries

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Multiwavelength Study of the X-Ray Bright Supernova Remnant N300-S26 in NGC 300

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The Astrophysical Journal 877 (1) 15 (2019)
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Discovery of pulsations from NGC 300 ULX1 and its fast period evolution

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Recurring X-ray outbursts in the supernova impostor SN 2010da in NGC 300

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Discovery of a deep Seyfert-2 galaxy atz = 0.222 behind NGC 300

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XMM-Newtonobservation of the interacting galaxies NGC 1512 and NGC 1510

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Optical spectra of supernova remnant candidates in the Sculptor Group galaxy NGC 300

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Astrophysics and Space Science 332 (2) 221 (2011)
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EXTRAGALACTIC CHEMICAL ABUNDANCES: DO H II REGIONS AND YOUNG STARS TELL THE SAME STORY? THE CASE OF THE SPIRAL GALAXY NGC 300

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The Astrophysical Journal 700 (1) 309 (2009)
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A Wolf-Rayet/black-hole X-ray binary candidate in NGC 300

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Astronomy & Astrophysics 461 (1) L9 (2007)
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A 33 hour period for the Wolf-Rayet/black hole X-ray binary candidate NGC 300 X-1

S. Carpano, A. M. T. Pollock, A. Prestwich, et al.
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