Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies
We have worked outty predictions for the radio counts of star-forming galaxies down to nJy levels, along with redshift distributions down to the detection limits of the phase 1 Square Kilometer Array MID telescope (SKA1-MID) and of its precursors. Such predictions were obtained by coupling epoch-dep...
Published in: | The Astrophysical Journal |
---|---|
Main Authors: | , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | unknown |
Published: |
IOP Publishing
2015
|
Subjects: | |
Online Access: | https://orca.cardiff.ac.uk/id/eprint/83992/ https://doi.org/10.1088/0004-637X/810/1/72 |
id |
ftunivcardiff:oai:https://orca.cardiff.ac.uk:83992 |
---|---|
record_format |
openpolar |
spelling |
ftunivcardiff:oai:https://orca.cardiff.ac.uk:83992 2023-05-15T18:22:53+02:00 Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies Mancuso, C. Lapi, A. Cai, Z. Negrello, Mattia De Zotti, G. Bressan, A. Bonato, M. Perrotta, F. Danese, L. 2015-09-01 https://orca.cardiff.ac.uk/id/eprint/83992/ https://doi.org/10.1088/0004-637X/810/1/72 unknown IOP Publishing Mancuso, C., Lapi, A., Cai, Z., Negrello, Mattia https://orca.cardiff.ac.uk/view/cardiffauthors/A21919605.html orcid:0000-0002-7925-7663 orcid:0000-0002-7925-7663, De Zotti, G., Bressan, A., Bonato, M., Perrotta, F. and Danese, L. 2015. Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies. The Astrophysical Journal 810 (1) , p. 72. 10.1088/0004-637X/810/1/72 https://doi.org/10.1088/0004-637X%2F810%2F1%2F72 doi:10.1088/0004-637X/810/1/72 QC Physics Article PeerReviewed 2015 ftunivcardiff https://doi.org/10.1088/0004-637X/810/1/72 2022-11-03T23:36:45Z We have worked outty predictions for the radio counts of star-forming galaxies down to nJy levels, along with redshift distributions down to the detection limits of the phase 1 Square Kilometer Array MID telescope (SKA1-MID) and of its precursors. Such predictions were obtained by coupling epoch-dependent star formation rate (SFR) functions with relations between SFR and radio (synchrotron and free–free) emission. The SFR functions were derived taking into account both the dust-obscured and the unobscured star formation, by combining far-infrared, ultraviolet, and Hα luminosity functions up to high redshifts. We have also revisited the South Pole Telescope counts of dusty galaxies at 95 GHz, performing a detailed analysis of the Spectral Energy Distributions. Our results show that the deepest SKA1-MID surveys will detect high-z galaxies with SFRs two orders of magnitude lower compared to Herschel surveys. The highest redshift tails of the distributions at the detection limits of planned SKA1-MID surveys comprise a substantial fraction of strongly lensed galaxies. We predict that a survey down to 0.25 μJy at 1.4 GHz will detect about 1200 strongly lensed galaxies per square degree, at redshifts of up to 10. For about 30% of them the SKA1-MID will detect at least 2 images. The SKA1-MID will thus provide a comprehensive view of the star formation history throughout the re-ionization epoch, unaffected by dust extinction. We have also provided specific predictions for the EMU/ASKAP and MIGHTEE/MeerKAT surveys. Article in Journal/Newspaper South pole Cardiff University: ORCA (Online Research @ Cardiff) South Pole The Astrophysical Journal 810 1 72 |
institution |
Open Polar |
collection |
Cardiff University: ORCA (Online Research @ Cardiff) |
op_collection_id |
ftunivcardiff |
language |
unknown |
topic |
QC Physics |
spellingShingle |
QC Physics Mancuso, C. Lapi, A. Cai, Z. Negrello, Mattia De Zotti, G. Bressan, A. Bonato, M. Perrotta, F. Danese, L. Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies |
topic_facet |
QC Physics |
description |
We have worked outty predictions for the radio counts of star-forming galaxies down to nJy levels, along with redshift distributions down to the detection limits of the phase 1 Square Kilometer Array MID telescope (SKA1-MID) and of its precursors. Such predictions were obtained by coupling epoch-dependent star formation rate (SFR) functions with relations between SFR and radio (synchrotron and free–free) emission. The SFR functions were derived taking into account both the dust-obscured and the unobscured star formation, by combining far-infrared, ultraviolet, and Hα luminosity functions up to high redshifts. We have also revisited the South Pole Telescope counts of dusty galaxies at 95 GHz, performing a detailed analysis of the Spectral Energy Distributions. Our results show that the deepest SKA1-MID surveys will detect high-z galaxies with SFRs two orders of magnitude lower compared to Herschel surveys. The highest redshift tails of the distributions at the detection limits of planned SKA1-MID surveys comprise a substantial fraction of strongly lensed galaxies. We predict that a survey down to 0.25 μJy at 1.4 GHz will detect about 1200 strongly lensed galaxies per square degree, at redshifts of up to 10. For about 30% of them the SKA1-MID will detect at least 2 images. The SKA1-MID will thus provide a comprehensive view of the star formation history throughout the re-ionization epoch, unaffected by dust extinction. We have also provided specific predictions for the EMU/ASKAP and MIGHTEE/MeerKAT surveys. |
format |
Article in Journal/Newspaper |
author |
Mancuso, C. Lapi, A. Cai, Z. Negrello, Mattia De Zotti, G. Bressan, A. Bonato, M. Perrotta, F. Danese, L. |
author_facet |
Mancuso, C. Lapi, A. Cai, Z. Negrello, Mattia De Zotti, G. Bressan, A. Bonato, M. Perrotta, F. Danese, L. |
author_sort |
Mancuso, C. |
title |
Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies |
title_short |
Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies |
title_full |
Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies |
title_fullStr |
Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies |
title_full_unstemmed |
Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies |
title_sort |
predictions for ultra-deep radio counts of star-forming galaxies |
publisher |
IOP Publishing |
publishDate |
2015 |
url |
https://orca.cardiff.ac.uk/id/eprint/83992/ https://doi.org/10.1088/0004-637X/810/1/72 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
Mancuso, C., Lapi, A., Cai, Z., Negrello, Mattia https://orca.cardiff.ac.uk/view/cardiffauthors/A21919605.html orcid:0000-0002-7925-7663 orcid:0000-0002-7925-7663, De Zotti, G., Bressan, A., Bonato, M., Perrotta, F. and Danese, L. 2015. Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies. The Astrophysical Journal 810 (1) , p. 72. 10.1088/0004-637X/810/1/72 https://doi.org/10.1088/0004-637X%2F810%2F1%2F72 doi:10.1088/0004-637X/810/1/72 |
op_doi |
https://doi.org/10.1088/0004-637X/810/1/72 |
container_title |
The Astrophysical Journal |
container_volume |
810 |
container_issue |
1 |
container_start_page |
72 |
_version_ |
1766202299761295360 |