A dataset provided by the European Space Agency

Name 13942
Title Does the IMF vary with galaxy mass? The X-ray binary population of a key galaxy, NGC7457
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13942;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ndx6sc3
Author Peacock, Mark B.
Description This is a scientific proposal for HST mission. For specific information please visit https:archive.stsci.eduproposal_search.php?id=13942&mission=hst
Publication Deep Chandra observations of NGC 7457, the X-ray point source populations of a low-mass early-type galaxy, Peacock, Mark B.,Zepf, Stephen E.,Kundu, Arunav, Monthly Notices of the Royal Astronomical Society, 466, 2017-04-01 00:00:00, 2017MNRAS.466.4021P||Further Constraints on Variations in the Initial Mass Function from Low-mass X-ray Binary Populations, Peacock, Mark B.,Zepf, Stephen E.,Kundu, Arunav, The Astrophysical Journal, 841, 2017-05-01 00:00:00, 2017ApJ...841...28P||Testing the Universality of the Stellar IMF with Chandra and HST, Coulter, D. A.,Lehmer, B. D.,Eufrasio, R. T., The Astrophysical Journal, 835, 2017-02-01 00:00:00, 2017ApJ...835..183C
Instrument ACS, ACS/WFC
Temporal Coverage 2014-12-11T08:01:30Z/2014-12-11T10:22:04Z
Version V1.0
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 2015-12-11 15:20:43
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015, 13942, V1.0. https://doi.org/10.5270/esa-ndx6sc3