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Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR. / Heesen, V.; E., Buie II; Huff, C. J.; Perez, L. A.; Woolsey, J. G.; Rafferty, D. A.; Basu, A.; Beck, R.; Brinks, E.; Horellou, C.; Scannapieco, E.; Brüggen, M.; Dettmar, R. -J.; Sendlinger, K.; Nikiel-Wroczyński, B.; Chyży, K. T.; Best, P.N.; Heald, George H.; Paladino, R.

In: Astronomy & Astrophysics, 15.10.2018.

Research output: Contribution to journalArticlepeer-review

Harvard

Heesen, V, E., BII, Huff, CJ, Perez, LA, Woolsey, JG, Rafferty, DA, Basu, A, Beck, R, Brinks, E, Horellou, C, Scannapieco, E, Brüggen, M, Dettmar, R-J, Sendlinger, K, Nikiel-Wroczyński, B, Chyży, KT, Best, PN, Heald, GH & Paladino, R 2018, 'Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR', Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201833905

APA

Heesen, V., E., B. II., Huff, C. J., Perez, L. A., Woolsey, J. G., Rafferty, D. A., Basu, A., Beck, R., Brinks, E., Horellou, C., Scannapieco, E., Brüggen, M., Dettmar, R. -J., Sendlinger, K., Nikiel-Wroczyński, B., Chyży, K. T., Best, P. N., Heald, G. H., & Paladino, R. (2018). Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201833905

Vancouver

Author

Heesen, V. ; E., Buie II ; Huff, C. J. ; Perez, L. A. ; Woolsey, J. G. ; Rafferty, D. A. ; Basu, A. ; Beck, R. ; Brinks, E. ; Horellou, C. ; Scannapieco, E. ; Brüggen, M. ; Dettmar, R. -J. ; Sendlinger, K. ; Nikiel-Wroczyński, B. ; Chyży, K. T. ; Best, P.N. ; Heald, George H. ; Paladino, R. / Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR. In: Astronomy & Astrophysics. 2018.

Bibtex

@article{a445c726789341c0bba9e27120195be0,
title = "Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR",
abstract = " Radio continuum (RC) emission in galaxies allows us to measure star formation rates (SFRs) unaffected by extinction due to dust, of which the low-frequency part is uncontaminated from thermal (free-free) emission. We calibrate the conversion from the spatially resolved 140 MHz RC emission to the SFR surface density ($\Sigma_{\rm SFR}$) at 1 kpc scale. We used recent observations of three galaxies (NGC 3184, 4736, and 5055) from the LOFAR Two-metre Sky Survey (LoTSS), and archival LOw-Frequency ARray (LOFAR) data of NGC 5194. Maps were created with the facet calibration technique and converted to radio $\Sigma_{\rm SFR}$ maps using the Condon relation. We compared these maps with hybrid $\Sigma_{\rm SFR}$ maps from a combination of GALEX far-ultraviolet and Spitzer 24 $\mu\rm m$ data using plots tracing the relation at $1.2\times 1.2$-kpc$^2$ resolution. The RC emission is smoothed with respect to the hybrid $\Sigma_{\rm SFR}$ owing to the transport of cosmic-ray electrons (CREs). This results in a sublinear relation $(\Sigma_{\rm SFR})_{\rm RC} \propto [(\Sigma_{\rm SFR})_{\rm hyb}]^{a}$, where $a=0.59\pm 0.13$ (140 MHz) and $a=0.75\pm 0.10$ (1365 MHz). Both relations have a scatter of $\sigma = 0.3~\rm dex$. If we restrict ourselves to areas of young CREs ($\alpha > -0.65$; $I_\nu \propto \nu^\alpha$), the relation becomes almost linear at both frequencies with $a\approx 0.9$ and a reduced scatter of $\sigma = 0.2~\rm dex$. We then simulate the effect of CRE transport by convolving the hybrid $\Sigma_{\rm SFR}$ maps with a Gaussian kernel until the RC-SFR relation is linearised; CRE transport lengths are $l=1$-5 kpc. Solving the CRE diffusion equation, we find diffusion coefficients of $D=(0.13$-$1.5) \times 10^{28} \rm cm^2\,s^{-1}$ at 1 GeV. A RC-SFR relation at $1.4$ GHz can be exploited to measure SFRs at redshift $z \approx 10$ using $140$ MHz observations. ",
keywords = "astro-ph.GA",
author = "V. Heesen and E., {Buie II} and Huff, {C. J.} and Perez, {L. A.} and Woolsey, {J. G.} and Rafferty, {D. A.} and A. Basu and R. Beck and E. Brinks and C. Horellou and E. Scannapieco and M. Br{\"u}ggen and Dettmar, {R. -J.} and K. Sendlinger and B. Nikiel-Wroczy{\'n}ski and Chy{\.z}y, {K. T.} and P.N. Best and Heald, {George H.} and R. Paladino",
note = "9 figures, 6 tables and 17 pages. This paper is part of the LOFAR surveys data release 1 and has been accepted for publication in a special edition of A&A that will appear in Feb 2019, volume 622. The catalogues and images from the data release will be publicly available on lofar-surveys.org upon publication of the journal. Reproduced with permission from Astronomy & Astrophysics. {\textcopyright} 2018 ESO.",
year = "2018",
month = oct,
day = "15",
doi = "10.1051/0004-6361/201833905",
language = "English",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR

AU - Heesen, V.

AU - E., Buie II

AU - Huff, C. J.

AU - Perez, L. A.

AU - Woolsey, J. G.

AU - Rafferty, D. A.

AU - Basu, A.

AU - Beck, R.

AU - Brinks, E.

AU - Horellou, C.

AU - Scannapieco, E.

AU - Brüggen, M.

AU - Dettmar, R. -J.

AU - Sendlinger, K.

AU - Nikiel-Wroczyński, B.

AU - Chyży, K. T.

AU - Best, P.N.

AU - Heald, George H.

AU - Paladino, R.

N1 - 9 figures, 6 tables and 17 pages. This paper is part of the LOFAR surveys data release 1 and has been accepted for publication in a special edition of A&A that will appear in Feb 2019, volume 622. The catalogues and images from the data release will be publicly available on lofar-surveys.org upon publication of the journal. Reproduced with permission from Astronomy & Astrophysics. © 2018 ESO.

PY - 2018/10/15

Y1 - 2018/10/15

N2 - Radio continuum (RC) emission in galaxies allows us to measure star formation rates (SFRs) unaffected by extinction due to dust, of which the low-frequency part is uncontaminated from thermal (free-free) emission. We calibrate the conversion from the spatially resolved 140 MHz RC emission to the SFR surface density ($\Sigma_{\rm SFR}$) at 1 kpc scale. We used recent observations of three galaxies (NGC 3184, 4736, and 5055) from the LOFAR Two-metre Sky Survey (LoTSS), and archival LOw-Frequency ARray (LOFAR) data of NGC 5194. Maps were created with the facet calibration technique and converted to radio $\Sigma_{\rm SFR}$ maps using the Condon relation. We compared these maps with hybrid $\Sigma_{\rm SFR}$ maps from a combination of GALEX far-ultraviolet and Spitzer 24 $\mu\rm m$ data using plots tracing the relation at $1.2\times 1.2$-kpc$^2$ resolution. The RC emission is smoothed with respect to the hybrid $\Sigma_{\rm SFR}$ owing to the transport of cosmic-ray electrons (CREs). This results in a sublinear relation $(\Sigma_{\rm SFR})_{\rm RC} \propto [(\Sigma_{\rm SFR})_{\rm hyb}]^{a}$, where $a=0.59\pm 0.13$ (140 MHz) and $a=0.75\pm 0.10$ (1365 MHz). Both relations have a scatter of $\sigma = 0.3~\rm dex$. If we restrict ourselves to areas of young CREs ($\alpha > -0.65$; $I_\nu \propto \nu^\alpha$), the relation becomes almost linear at both frequencies with $a\approx 0.9$ and a reduced scatter of $\sigma = 0.2~\rm dex$. We then simulate the effect of CRE transport by convolving the hybrid $\Sigma_{\rm SFR}$ maps with a Gaussian kernel until the RC-SFR relation is linearised; CRE transport lengths are $l=1$-5 kpc. Solving the CRE diffusion equation, we find diffusion coefficients of $D=(0.13$-$1.5) \times 10^{28} \rm cm^2\,s^{-1}$ at 1 GeV. A RC-SFR relation at $1.4$ GHz can be exploited to measure SFRs at redshift $z \approx 10$ using $140$ MHz observations.

AB - Radio continuum (RC) emission in galaxies allows us to measure star formation rates (SFRs) unaffected by extinction due to dust, of which the low-frequency part is uncontaminated from thermal (free-free) emission. We calibrate the conversion from the spatially resolved 140 MHz RC emission to the SFR surface density ($\Sigma_{\rm SFR}$) at 1 kpc scale. We used recent observations of three galaxies (NGC 3184, 4736, and 5055) from the LOFAR Two-metre Sky Survey (LoTSS), and archival LOw-Frequency ARray (LOFAR) data of NGC 5194. Maps were created with the facet calibration technique and converted to radio $\Sigma_{\rm SFR}$ maps using the Condon relation. We compared these maps with hybrid $\Sigma_{\rm SFR}$ maps from a combination of GALEX far-ultraviolet and Spitzer 24 $\mu\rm m$ data using plots tracing the relation at $1.2\times 1.2$-kpc$^2$ resolution. The RC emission is smoothed with respect to the hybrid $\Sigma_{\rm SFR}$ owing to the transport of cosmic-ray electrons (CREs). This results in a sublinear relation $(\Sigma_{\rm SFR})_{\rm RC} \propto [(\Sigma_{\rm SFR})_{\rm hyb}]^{a}$, where $a=0.59\pm 0.13$ (140 MHz) and $a=0.75\pm 0.10$ (1365 MHz). Both relations have a scatter of $\sigma = 0.3~\rm dex$. If we restrict ourselves to areas of young CREs ($\alpha > -0.65$; $I_\nu \propto \nu^\alpha$), the relation becomes almost linear at both frequencies with $a\approx 0.9$ and a reduced scatter of $\sigma = 0.2~\rm dex$. We then simulate the effect of CRE transport by convolving the hybrid $\Sigma_{\rm SFR}$ maps with a Gaussian kernel until the RC-SFR relation is linearised; CRE transport lengths are $l=1$-5 kpc. Solving the CRE diffusion equation, we find diffusion coefficients of $D=(0.13$-$1.5) \times 10^{28} \rm cm^2\,s^{-1}$ at 1 GeV. A RC-SFR relation at $1.4$ GHz can be exploited to measure SFRs at redshift $z \approx 10$ using $140$ MHz observations.

KW - astro-ph.GA

U2 - 10.1051/0004-6361/201833905

DO - 10.1051/0004-6361/201833905

M3 - Article

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

ER -