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 |