Discovery of a Rapid, Luminous Nova in NGC 300 by the KMTNet Supernova Program
Energy-dependent orbital phases in NGC 300 X-1
Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
Is NGC 300 a pure exponential disk galaxy?
Multiwavelength Study of the X-Ray Bright Supernova Remnant N300-S26 in NGC 300
New outburst from the luminous supersoft source SSS1 in NGC 300 with periodic modulation
Recurring X-ray outbursts in the supernova impostor SN 2010da in NGC 300
Soft extragalactic X-ray binaries at the Eddington Threshold
The impact of satellite trails on Hubble Space Telescope observations
The Intermediate Luminosity Optical Transient SN 2010da: The Progenitor, Eruption, and Aftermath of a Peculiar Supergiant High-mass X-Ray Binary
Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2014-05-09T14:24:59Z/2014-09-05T18:22:10Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Binder comma Breanna, 2015, 'The Effect of Intermediate-Luminosity Transients on the X-ray Luminosity Functions of Spiral Disks', 1.0, European Space Agency, https://doi.org/10.5270/esa-273z6p8