Constraining the coevolution of galaxies and black holes at low mass
Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. I. A Reverberation-based Measurement of the Black Hole Mass
Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. III. Optical Variability and X-Ray/UV/Optical Correlations
Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. II. X-Ray and Ultraviolet Continuum Variability
Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. IV. The Variable UV Absorption Lines
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2004-04-10T03:19:40Z/2004-07-03T19:14:44Z
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, Laor comma Ari, 2007, 'Reverberation Mapping of the Least Luminous Seyfert 1 Galaxy NGC 4395', 1.0, European Space Agency, https://doi.org/10.5270/esa-q4r7bbw