Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting – II. The case with unknown redshift. Pforr, J., Maraston, C., & Tonini, C. Monthly Notices of the Royal Astronomical Society, 435(2):1389–1425, October, 2013. Publisher: Oxford AcademicPaper doi abstract bibtex Abstract. In a recent work (Paper I), we explored the dependence of galaxy stellar population properties derived from broad-band spectral energy distribution f
@article{pforr_recovering_2013,
title = {Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting – {II}. {The} case with unknown redshift},
volume = {435},
issn = {0035-8711},
url = {https://academic.oup.com/mnras/article/435/2/1389/1039166},
doi = {10.1093/mnras/stt1382},
abstract = {Abstract. In a recent work (Paper I), we explored the dependence of galaxy stellar population properties derived from broad-band spectral energy distribution f},
language = {en},
number = {2},
urldate = {2020-03-24},
journal = {Monthly Notices of the Royal Astronomical Society},
author = {Pforr, Janine and Maraston, Claudia and Tonini, Chiara},
month = oct,
year = {2013},
note = {Publisher: Oxford Academic},
pages = {1389--1425},
}
Downloads: 0
{"_id":"fBhxfMDntHXu6sAoo","bibbaseid":"pforr-maraston-tonini-recoveringgalaxystellarpopulationpropertiesfrombroadbandspectralenergydistributionfittingiithecasewithunknownredshift-2013","author_short":["Pforr, J.","Maraston, C.","Tonini, C."],"bibdata":{"bibtype":"article","type":"article","title":"Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting – II. The case with unknown redshift","volume":"435","issn":"0035-8711","url":"https://academic.oup.com/mnras/article/435/2/1389/1039166","doi":"10.1093/mnras/stt1382","abstract":"Abstract. In a recent work (Paper I), we explored the dependence of galaxy stellar population properties derived from broad-band spectral energy distribution f","language":"en","number":"2","urldate":"2020-03-24","journal":"Monthly Notices of the Royal Astronomical Society","author":[{"propositions":[],"lastnames":["Pforr"],"firstnames":["Janine"],"suffixes":[]},{"propositions":[],"lastnames":["Maraston"],"firstnames":["Claudia"],"suffixes":[]},{"propositions":[],"lastnames":["Tonini"],"firstnames":["Chiara"],"suffixes":[]}],"month":"October","year":"2013","note":"Publisher: Oxford Academic","pages":"1389–1425","bibtex":"@article{pforr_recovering_2013,\n\ttitle = {Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting – {II}. {The} case with unknown redshift},\n\tvolume = {435},\n\tissn = {0035-8711},\n\turl = {https://academic.oup.com/mnras/article/435/2/1389/1039166},\n\tdoi = {10.1093/mnras/stt1382},\n\tabstract = {Abstract. In a recent work (Paper I), we explored the dependence of galaxy stellar population properties derived from broad-band spectral energy distribution f},\n\tlanguage = {en},\n\tnumber = {2},\n\turldate = {2020-03-24},\n\tjournal = {Monthly Notices of the Royal Astronomical Society},\n\tauthor = {Pforr, Janine and Maraston, Claudia and Tonini, Chiara},\n\tmonth = oct,\n\tyear = {2013},\n\tnote = {Publisher: Oxford Academic},\n\tpages = {1389--1425},\n}\n\n","author_short":["Pforr, J.","Maraston, C.","Tonini, C."],"key":"pforr_recovering_2013","id":"pforr_recovering_2013","bibbaseid":"pforr-maraston-tonini-recoveringgalaxystellarpopulationpropertiesfrombroadbandspectralenergydistributionfittingiithecasewithunknownredshift-2013","role":"author","urls":{"Paper":"https://academic.oup.com/mnras/article/435/2/1389/1039166"},"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":[],"search_terms":["recovering","galaxy","stellar","population","properties","broad","band","spectral","energy","distribution","fitting","case","unknown","redshift","pforr","maraston","tonini"],"title":"Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting – II. The case with unknown redshift","year":2013}