Absence of nebular He II l4686 constrains the UV emission from the ultraluminous X-ray pulsar NGC 1313 X-2
A New Sample of Transient Ultraluminous X-Ray Sources Serendipitously Discovered by Swift/XRT
An Optical Study of Stellar and Interstellar Environments of Seven Luminous and Ultraluminous X-Ray Sources
Characteristics of Spiral Arms in Late-type Galaxies
Compact Optical Counterparts of Ultraluminous X-Ray Sources
Constraints for the Progenitor Masses of 17 Historic Core-collapse Supernovae
FEAST: Feedback in Emerging extragAlactic Star ClusTers: JWST Spots Polycyclic Aromatic Hydrocarbon Destruction in NGC 628 during the Emerging Phase of Star Formation
Feedback in Emerging Extragalactic Star Clusters, FEAST: The Relation between 3.3 mm Polycyclic Aromatic Hydrocarbon Emission and Star Formation Rate Traced by Ionized Gas in NGC 628
Investigating the Drivers of Electron Temperature Variations in H II Regions with Keck-KCWI and VLT-MUSE
JWST-FEAST: Feedback in Emerging extrAgalactic Star clusTers: Calibration of Star Formation Rates in the Mid-infrared with NGC 628
Legacy ExtraGalactic UV Survey with The Hubble Space Telescope: Stellar Cluster Catalogs and First Insights Into Cluster Formation and Evolution in NGC 628
Looking for Obscured Young Star Clusters in NGC 1313
Modeling Type II-P/II-L Supernovae Interacting with Recent Episodic Mass Ejections from Their Presupernova Stars with MESA and SNEC
MUSE spectroscopy of the ULX NGC 1313 X-1: A shock-ionised bubble, an X-ray photoionised nebula, and two supernova remnants
On the progenitor of the Type IIP SN 2013ej in M74.
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Optical Properties of the Ultraluminous X-Ray Source Holmberg IX X-1 and Its Stellar Environment
Optical Studies of the Ultraluminous X-Ray Source NGC 1313 X-2
PHANGS-HST: new methods for star cluster identification in nearby galaxies
Roche-lobe Overflow Systems Powered by Black Holes in Young Star Clusters: The Importance of Dynamical Exchanges
SN 2016X: a type II-P supernova with a signature of shock breakout from explosion of a massive red supergiant
Spitzer IRAC Observations of IR Excess in Holmberg IX X-1: A Circumbinary Disk or a Variable Jet?
Stellar subsystems of the galaxy NGC 1313
The Blue Supergiant Progenitor of the Supernova Imposter AT 2019krl
The impact of satellite trails on Hubble Space Telescope observations
The Optical Counterpart of NGC 1313 X-1
The resolved stellar populations around 12 Type IIP supernovae
The Spitzer Local Volume Legacy: Survey Description and Infrared Photometry
The Tip of the Red Giant Branch Distance to the Perfect Spiral Galaxy M74 Hosting Three Core-collapse Supernovae
The ultraluminous X-ray source NGC 1313 X-2. Its optical counterpart and environment
Type IIP Supernova Progenitors. II. Stellar Mass and Obscuration by the Dust in the Circumstellar Medium
Very Large Telescope MUSE Observations of the Bubble Nebula around NGC 1313 X-2 and Evidence for Additional Photoionization
X-Ray and Optical Variability of the Ultraluminous X-Ray Source NGC 1313 X-2
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2003-11-17T05:52:14Z/2004-03-25T11:20:36Z
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, Miller comma Jon Matthew, 2005, 'Observations of Intermediate Mass Black Hole Candidate Ultra-Luminous X-ray Sources', 1.0, European Space Agency, https://doi.org/10.5270/esa-qhqyxsu
