Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30250
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BONATO, MATTEO | en_US |
dc.contributor.author | Sajina, Anna | en_US |
dc.contributor.author | DE ZOTTI, Gianfranco | en_US |
dc.contributor.author | McKinney, Jed | en_US |
dc.contributor.author | BARONCHELLI, IVANO | en_US |
dc.contributor.author | Negrello, Mattia | en_US |
dc.contributor.author | Marchesini, Danilo | en_US |
dc.contributor.author | Roebuck, Eric | en_US |
dc.contributor.author | Shipley, Heath | en_US |
dc.contributor.author | Kurinsky, Noah | en_US |
dc.contributor.author | Pope, Alexandra | en_US |
dc.contributor.author | Noriega-Crespo, Alberto | en_US |
dc.contributor.author | Yan, Lin | en_US |
dc.contributor.author | Kirkpatrick, Allison | en_US |
dc.date.accessioned | 2021-02-09T07:53:57Z | - |
dc.date.available | 2021-02-09T07:53:57Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30250 | - |
dc.description.abstract | The James Webb Space Telescope’s Medium Resolution Spectrometer (MRS), will offer nearly two orders of magnitude improvement in sensitivity and >3× improvement in spectral resolution over our previous space-based mid-IR spectrometer, the Spitzer IRS. In this paper, we make predictions for spectroscopic pointed observations and serendipitous detections with the MRS. Specifically, pointed observations of Herschel sources require only a few minutes on source integration for detections of several star-forming and active galactic nucleus lines, out to z = 3 and beyond. But the same data will also include tens of serendipitous 0 ≲ z ≲ 4 galaxies per field with infrared luminosities ranging ∼10<SUP>6</SUP>-10<SUP>13</SUP> L <SUB>☉</SUB>. In particular, for the first time and for free we will be able to explore the L <SUB>IR</SUB> < 10<SUP>9</SUP> L <SUB>☉</SUB> regime out to z ∼ 3. We estimate that with ∼ 100 such fields, statistics of these detections will be sufficient to constrain the evolution of the low-L end of the infrared luminosity function, and hence the star formation rate function. The above conclusions hold for a wide range in the potential low-L end of the IR luminosity function, and account for the PAH deficit in low-L, low-metallicity galaxies. | en_US |
dc.language.iso | eng | en_US |
dc.title | Exploring the Evolution of Star Formation and Dwarf Galaxy Properties with JWST/MIRI Serendipitous Spectroscopic Surveys | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/aa5c85 | en_US |
dc.identifier.scopus | 2-s2.0-85014449961 | en_US |
dc.identifier.isi | 000395919500004 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/aa5c85 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 836 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 171 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017ApJ...836..171B | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0001-9139-2342 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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