The Evolutionary Map of the Universe pilot survey

Ray P. Norris; Joshua Marvil; J. D. Collier; Anna D. Kapinska; Andrew N. O’Brien; L. Rudnick; Heinz Andernach; Jacobo Asorey; Michael J. I. Brown; Marcus Brüggen; Evan Crawford; Jayanne English; Syed Faisal ur Rahman; Miroslav D. Filipovic; Yjan Gordon; Gülay Gürkan; Catherine Hale; Andrew M. Hopkins; Minh T. Huynh; Kim HyeongHan; M. James Jee; Bärbel S. Koribalski; Emil Lenc; Kieran Luken; David Parkinson; Isabella Prandoni; Wasim Raja; Thomas H. Reiprich; Christopher J. Riseley; Stanislav S. Shabala; Jaimie R. Sheil; Tessa Vernstrom; Matthew T. Whiting; James R. Allison; C. S. Anderson; Lewis Ball; Martin Bell; John Bunton; T. J. Galvin; Neeraj Gupta; Aidan Hotan; Colin Jacka; Peter J. Macgregor; Elizabeth K. Mahony; Umberto Maio; Vanessa Moss; M. Pandey-Pommier; Maxim A. Voronkov

doi:10.1017/pasa.2021.42

The Evolutionary Map of the Universe pilot survey

Ray P. Norris, Joshua Marvil, J. D. Collier, Anna D. Kapinska, Andrew N. O’Brien, L. Rudnick, Heinz Andernach, Jacobo Asorey, Michael J. I. Brown, Marcus Brüggen, Evan Crawford, Jayanne English, Syed Faisal ur Rahman, Miroslav D. Filipovic, Yjan Gordon, Gülay Gürkan, Catherine Hale, Andrew M. Hopkins, Minh T. Huynh, Kim HyeongHanM. James Jee, Bärbel S. Koribalski, Emil Lenc, Kieran Luken, David Parkinson, Isabella Prandoni, Wasim Raja, Thomas H. Reiprich, Christopher J. Riseley, Stanislav S. Shabala, Jaimie R. Sheil, Tessa Vernstrom, Matthew T. Whiting, James R. Allison, C. S. Anderson, Lewis Ball, Martin Bell, John Bunton, T. J. Galvin, Neeraj Gupta, Aidan Hotan, Colin Jacka, Peter J. Macgregor, Elizabeth K. Mahony, Umberto Maio, Vanessa Moss, M. Pandey-Pommier, Maxim A. Voronkov

Western Sydney University

Research output: Contribution to journal › Article › peer-review

115 Citations (Scopus)

Abstract

We present the data and initial results from the first pilot survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers 270 deg2 of an area covered by the Dark Energy Survey, reaching a depth of 25-30 Î¼Jy beamâˆ’1 rms at a spatial resolution of âˆ¼11-18 arcsec, resulting in a catalogue of âˆ¼220 000 sources, of which âˆ¼180 000 are single-component sources. Here we present the catalogue of single-component sources, together with (where available) optical and infrared cross-identifications, classifications, and redshifts. This survey explores a new region of parameter space compared to previous surveys. Specifically, the EMU Pilot Survey has a high density of sources, and also a high sensitivity to low surface brightness emission. These properties result in the detection of types of sources that were rarely seen in or absent from previous surveys. We present some of these new results here.

Original language	English
Article number	e046
Number of pages	26
Journal	Publications of the Astronomical Society of Australia
Volume	38
DOIs	https://doi.org/10.1017/pasa.2021.42
Publication status	Published - 2021

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10.1017/pasa.2021.42

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Norris, R. P., Marvil, J., Collier, J. D., Kapinska, A. D., O’Brien, A. N., Rudnick, L., Andernach, H., Asorey, J., Brown, M. J. I., Brüggen, M., Crawford, E., English, J., Rahman, S. F. U., Filipovic, M. D., Gordon, Y., Gürkan, G., Hale, C., Hopkins, A. M., Huynh, M. T., ... Voronkov, M. A. (2021). The Evolutionary Map of the Universe pilot survey. Publications of the Astronomical Society of Australia, 38, Article e046. https://doi.org/10.1017/pasa.2021.42

@article{e6194fdf3dbc413796935053605edaaa,

title = "The Evolutionary Map of the Universe pilot survey",

abstract = "We present the data and initial results from the first pilot survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers 270 deg2 of an area covered by the Dark Energy Survey, reaching a depth of 25-30 {\^I}¼Jy beam{\^a}ˆ{\textquoteright}1 rms at a spatial resolution of {\^a}ˆ¼11-18 arcsec, resulting in a catalogue of {\^a}ˆ¼220 000 sources, of which {\^a}ˆ¼180 000 are single-component sources. Here we present the catalogue of single-component sources, together with (where available) optical and infrared cross-identifications, classifications, and redshifts. This survey explores a new region of parameter space compared to previous surveys. Specifically, the EMU Pilot Survey has a high density of sources, and also a high sensitivity to low surface brightness emission. These properties result in the detection of types of sources that were rarely seen in or absent from previous surveys. We present some of these new results here.",

author = "Norris, {Ray P.} and Joshua Marvil and Collier, {J. D.} and Kapinska, {Anna D.} and O{\textquoteright}Brien, {Andrew N.} and L. Rudnick and Heinz Andernach and Jacobo Asorey and Brown, {Michael J. I.} and Marcus Br{\"u}ggen and Evan Crawford and Jayanne English and Rahman, {Syed Faisal ur} and Filipovic, {Miroslav D.} and Yjan Gordon and G{\"u}lay G{\"u}rkan and Catherine Hale and Hopkins, {Andrew M.} and Huynh, {Minh T.} and Kim HyeongHan and Jee, {M. James} and Koribalski, {B{\"a}rbel S.} and Emil Lenc and Kieran Luken and David Parkinson and Isabella Prandoni and Wasim Raja and Reiprich, {Thomas H.} and Riseley, {Christopher J.} and Shabala, {Stanislav S.} and Sheil, {Jaimie R.} and Tessa Vernstrom and Whiting, {Matthew T.} and Allison, {James R.} and Anderson, {C. S.} and Lewis Ball and Martin Bell and John Bunton and Galvin, {T. J.} and Neeraj Gupta and Aidan Hotan and Colin Jacka and Macgregor, {Peter J.} and Mahony, {Elizabeth K.} and Umberto Maio and Vanessa Moss and M. Pandey-Pommier and Voronkov, {Maxim A.}",

year = "2021",

doi = "10.1017/pasa.2021.42",

language = "English",

volume = "38",

journal = "Publications of the Astronomical Society of Australia",

issn = "1323-3580",

publisher = "CSIRO",

}

Norris, RP, Marvil, J, Collier, JD, Kapinska, AD, O’Brien, AN, Rudnick, L, Andernach, H, Asorey, J, Brown, MJI, Brüggen, M, Crawford, E, English, J, Rahman, SFU, Filipovic, MD, Gordon, Y, Gürkan, G, Hale, C, Hopkins, AM, Huynh, MT, HyeongHan, K, Jee, MJ, Koribalski, BS, Lenc, E, Luken, K, Parkinson, D, Prandoni, I, Raja, W, Reiprich, TH, Riseley, CJ, Shabala, SS, Sheil, JR, Vernstrom, T, Whiting, MT, Allison, JR, Anderson, CS, Ball, L, Bell, M, Bunton, J, Galvin, TJ, Gupta, N, Hotan, A, Jacka, C, Macgregor, PJ, Mahony, EK, Maio, U, Moss, V, Pandey-Pommier, M & Voronkov, MA 2021, 'The Evolutionary Map of the Universe pilot survey', Publications of the Astronomical Society of Australia, vol. 38, e046. https://doi.org/10.1017/pasa.2021.42

TY - JOUR

T1 - The Evolutionary Map of the Universe pilot survey

AU - Norris, Ray P.

AU - Marvil, Joshua

AU - Collier, J. D.

AU - Kapinska, Anna D.

AU - O’Brien, Andrew N.

AU - Rudnick, L.

AU - Andernach, Heinz

AU - Asorey, Jacobo

AU - Brown, Michael J. I.

AU - Brüggen, Marcus

AU - Crawford, Evan

AU - English, Jayanne

AU - Rahman, Syed Faisal ur

AU - Filipovic, Miroslav D.

AU - Gordon, Yjan

AU - Gürkan, Gülay

AU - Hale, Catherine

AU - Hopkins, Andrew M.

AU - Huynh, Minh T.

AU - HyeongHan, Kim

AU - Jee, M. James

AU - Koribalski, Bärbel S.

AU - Lenc, Emil

AU - Luken, Kieran

AU - Parkinson, David

AU - Prandoni, Isabella

AU - Raja, Wasim

AU - Reiprich, Thomas H.

AU - Riseley, Christopher J.

AU - Shabala, Stanislav S.

AU - Sheil, Jaimie R.

AU - Vernstrom, Tessa

AU - Whiting, Matthew T.

AU - Allison, James R.

AU - Anderson, C. S.

AU - Ball, Lewis

AU - Bell, Martin

AU - Bunton, John

AU - Galvin, T. J.

AU - Gupta, Neeraj

AU - Hotan, Aidan

AU - Jacka, Colin

AU - Macgregor, Peter J.

AU - Mahony, Elizabeth K.

AU - Maio, Umberto

AU - Moss, Vanessa

AU - Pandey-Pommier, M.

AU - Voronkov, Maxim A.

PY - 2021

Y1 - 2021

N2 - We present the data and initial results from the first pilot survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers 270 deg2 of an area covered by the Dark Energy Survey, reaching a depth of 25-30 Î¼Jy beamâˆ’1 rms at a spatial resolution of âˆ¼11-18 arcsec, resulting in a catalogue of âˆ¼220 000 sources, of which âˆ¼180 000 are single-component sources. Here we present the catalogue of single-component sources, together with (where available) optical and infrared cross-identifications, classifications, and redshifts. This survey explores a new region of parameter space compared to previous surveys. Specifically, the EMU Pilot Survey has a high density of sources, and also a high sensitivity to low surface brightness emission. These properties result in the detection of types of sources that were rarely seen in or absent from previous surveys. We present some of these new results here.

AB - We present the data and initial results from the first pilot survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers 270 deg2 of an area covered by the Dark Energy Survey, reaching a depth of 25-30 Î¼Jy beamâˆ’1 rms at a spatial resolution of âˆ¼11-18 arcsec, resulting in a catalogue of âˆ¼220 000 sources, of which âˆ¼180 000 are single-component sources. Here we present the catalogue of single-component sources, together with (where available) optical and infrared cross-identifications, classifications, and redshifts. This survey explores a new region of parameter space compared to previous surveys. Specifically, the EMU Pilot Survey has a high density of sources, and also a high sensitivity to low surface brightness emission. These properties result in the detection of types of sources that were rarely seen in or absent from previous surveys. We present some of these new results here.

UR - https://hdl.handle.net/1959.7/uws:62191

U2 - 10.1017/pasa.2021.42

DO - 10.1017/pasa.2021.42

M3 - Article

SN - 1323-3580

VL - 38

JO - Publications of the Astronomical Society of Australia

JF - Publications of the Astronomical Society of Australia

M1 - e046

ER -

The Evolutionary Map of the Universe pilot survey

Abstract

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