A dataset provided by the European Space Agency

Name 12762
Title M51: Using the Kinematics of a Grand-Design Spiral to Understand the Physics of the Hot ISM, SNRs, and XRBs
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12762;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-zbniuv1
Author European Space Agency
Description This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=12762&mission=hst
Publication Discovery of an Intermediate-luminosity Red Transient in M51 and Its Likely Dust-obscured, Infrared-variable Progenitor, Jencson, J.,Adams, Scott M.,Bond, Howard E., The Astrophysical Journal, 880, 2019-08-01 00:00:00, 2019ApJ...880L..20J||Optical Identification and Spectroscopy of Supernova Remnants in the Galaxy M51, Winkler, P. Frank,Coffin, Sadie C.,Blair, William P., The Astrophysical Journal, 908, 2021-02-01 00:00:00, 2021ApJ...908...80W
Instrument WFC3, WFC3/UVIS
Temporal Coverage 2012-04-03T01:23:23Z/2012-04-12T07:32:17Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2013-04-13T11:53:13Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, M51: Using The Kinematics Of A Grand-Design Spiral To Understand The Physics Of The Hot Ism, Snrs, And Xrbs, 1.0, European Space Agency, https://doi.org/10.5270/esa-zbniuv1