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A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy

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A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy. / Fu, Hai; Jullo, E.; Cooray, A.; Bussmann, R. S.; Ivison, R. J.; Pérez-Fournon, I.; Djorgovski, S. G.; Scoville, N.; Yan, L.; Riechers, D. A.; Aguirre, J.; Auld, R.; Baes, M.; Baker, A. J.; Bradford, M.; Cava, A.; Clements, D. L.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; Dole, H.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D.; Gavazzi, R.; Gurwell, M.; Harris, A. I.; Herranz, D.; Hopwood, R.; Hoyos, C.; Ibar, E.; Jarvis, M. J.; Kim, S.; Leeuw, L.; Lupu, R.; Maddox, S.; Martínez-Navajas, P.; Michałowski, M. J.; Negrello, M.; Omont, A.; Rosenman, M.; Scott, D.; Serjeant, S.; Smail, I.; Swinbank, A. M.; Valiante, E.; Verma, A.; Vieira, J.; Wardlow, J. L.; van der Werf, P.

In: The Astrophysical Journal, Vol. 753, No. 2, 01.07.2012, p. 134.

Research output: Contribution to journalJournal articlepeer-review

Harvard

Fu, H, Jullo, E, Cooray, A, Bussmann, RS, Ivison, RJ, Pérez-Fournon, I, Djorgovski, SG, Scoville, N, Yan, L, Riechers, DA, Aguirre, J, Auld, R, Baes, M, Baker, AJ, Bradford, M, Cava, A, Clements, DL, Dannerbauer, H, Dariush, A, De Zotti, G, Dole, H, Dunne, L, Dye, S, Eales, S, Frayer, D, Gavazzi, R, Gurwell, M, Harris, AI, Herranz, D, Hopwood, R, Hoyos, C, Ibar, E, Jarvis, MJ, Kim, S, Leeuw, L, Lupu, R, Maddox, S, Martínez-Navajas, P, Michałowski, MJ, Negrello, M, Omont, A, Rosenman, M, Scott, D, Serjeant, S, Smail, I, Swinbank, AM, Valiante, E, Verma, A, Vieira, J, Wardlow, JL & van der Werf, P 2012, 'A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy', The Astrophysical Journal, vol. 753, no. 2, pp. 134. https://doi.org/10.1088/0004-637X/753/2/134

APA

Fu, H., Jullo, E., Cooray, A., Bussmann, R. S., Ivison, R. J., Pérez-Fournon, I., Djorgovski, S. G., Scoville, N., Yan, L., Riechers, D. A., Aguirre, J., Auld, R., Baes, M., Baker, A. J., Bradford, M., Cava, A., Clements, D. L., Dannerbauer, H., Dariush, A., ... van der Werf, P. (2012). A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy. The Astrophysical Journal, 753(2), 134. https://doi.org/10.1088/0004-637X/753/2/134

Vancouver

Fu H, Jullo E, Cooray A, Bussmann RS, Ivison RJ, Pérez-Fournon I et al. A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy. The Astrophysical Journal. 2012 Jul 1;753(2):134. https://doi.org/10.1088/0004-637X/753/2/134

Author

Fu, Hai ; Jullo, E. ; Cooray, A. ; Bussmann, R. S. ; Ivison, R. J. ; Pérez-Fournon, I. ; Djorgovski, S. G. ; Scoville, N. ; Yan, L. ; Riechers, D. A. ; Aguirre, J. ; Auld, R. ; Baes, M. ; Baker, A. J. ; Bradford, M. ; Cava, A. ; Clements, D. L. ; Dannerbauer, H. ; Dariush, A. ; De Zotti, G. ; Dole, H. ; Dunne, L. ; Dye, S. ; Eales, S. ; Frayer, D. ; Gavazzi, R. ; Gurwell, M. ; Harris, A. I. ; Herranz, D. ; Hopwood, R. ; Hoyos, C. ; Ibar, E. ; Jarvis, M. J. ; Kim, S. ; Leeuw, L. ; Lupu, R. ; Maddox, S. ; Martínez-Navajas, P. ; Michałowski, M. J. ; Negrello, M. ; Omont, A. ; Rosenman, M. ; Scott, D. ; Serjeant, S. ; Smail, I. ; Swinbank, A. M. ; Valiante, E. ; Verma, A. ; Vieira, J. ; Wardlow, J. L. ; van der Werf, P. / A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy. In: The Astrophysical Journal. 2012 ; Vol. 753, No. 2. pp. 134.

Bibtex

@article{0597f2cddea84b939add804238aaba9c,
title = "A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy",
abstract = "We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 μm flux density (~300 mJy). It is the only high-redshift Planck detection in the 130 deg2 H-ATLAS Phase-I area. Keck Adaptive Optics images reveal a quadruply imaged galaxy in the K band while the Submillimeter Array and the Jansky Very Large Array show doubly imaged 880 μm and CO(1→0) sources, indicating differentiated distributions of the various components in the galaxy. In the source plane, the stars reside in three major kpc-scale clumps extended over ~1.6 kpc, the dust in a compact (~1 kpc) region ~3 kpc north of the stars, and the cold molecular gas in an extended (~7 kpc) disk ~5 kpc northeast of the stars. The emissions from the stars, dust, and gas are magnified by ~17, ~8, and ~7 times, respectively, by four lensing galaxies at z ~ 1. Intrinsically, the lensed galaxy is a warm (T dust ~ 40-65 K), hyper-luminous (L IR ~ 1.7 × 1013 L ⊙ star formation rate (SFR) ~2000 M ⊙ yr-1), gas-rich (M gas/M baryon ~ 70%), young (M stellar/SFR ~ 20 Myr), and short-lived (M gas/SFR ~ 40 Myr) starburst. With physical properties similar to unlensed z > 2 SMGs, HATLAS J114637.9-001132 offers a detailed view of a typical SMG through a powerful cosmic microscope.",
keywords = "galaxies: formation, galaxies: individual: HATLAS J114637.9–001132, galaxies: interactions",
author = "Hai Fu and E. Jullo and A. Cooray and Bussmann, {R. S.} and Ivison, {R. J.} and I. P{\'e}rez-Fournon and Djorgovski, {S. G.} and N. Scoville and L. Yan and Riechers, {D. A.} and J. Aguirre and R. Auld and M. Baes and Baker, {A. J.} and M. Bradford and A. Cava and Clements, {D. L.} and H. Dannerbauer and A. Dariush and {De Zotti}, G. and H. Dole and L. Dunne and S. Dye and S. Eales and D. Frayer and R. Gavazzi and M. Gurwell and Harris, {A. I.} and D. Herranz and R. Hopwood and C. Hoyos and E. Ibar and Jarvis, {M. J.} and S. Kim and L. Leeuw and R. Lupu and S. Maddox and P. Mart{\'i}nez-Navajas and Micha{\l}owski, {M. J.} and M. Negrello and A. Omont and M. Rosenman and D. Scott and S. Serjeant and I. Smail and Swinbank, {A. M.} and E. Valiante and A. Verma and J. Vieira and Wardlow, {J. L.} and {van der Werf}, P.",
year = "2012",
month = jul,
day = "1",
doi = "10.1088/0004-637X/753/2/134",
language = "English",
volume = "753",
pages = "134",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy

AU - Fu, Hai

AU - Jullo, E.

AU - Cooray, A.

AU - Bussmann, R. S.

AU - Ivison, R. J.

AU - Pérez-Fournon, I.

AU - Djorgovski, S. G.

AU - Scoville, N.

AU - Yan, L.

AU - Riechers, D. A.

AU - Aguirre, J.

AU - Auld, R.

AU - Baes, M.

AU - Baker, A. J.

AU - Bradford, M.

AU - Cava, A.

AU - Clements, D. L.

AU - Dannerbauer, H.

AU - Dariush, A.

AU - De Zotti, G.

AU - Dole, H.

AU - Dunne, L.

AU - Dye, S.

AU - Eales, S.

AU - Frayer, D.

AU - Gavazzi, R.

AU - Gurwell, M.

AU - Harris, A. I.

AU - Herranz, D.

AU - Hopwood, R.

AU - Hoyos, C.

AU - Ibar, E.

AU - Jarvis, M. J.

AU - Kim, S.

AU - Leeuw, L.

AU - Lupu, R.

AU - Maddox, S.

AU - Martínez-Navajas, P.

AU - Michałowski, M. J.

AU - Negrello, M.

AU - Omont, A.

AU - Rosenman, M.

AU - Scott, D.

AU - Serjeant, S.

AU - Smail, I.

AU - Swinbank, A. M.

AU - Valiante, E.

AU - Verma, A.

AU - Vieira, J.

AU - Wardlow, J. L.

AU - van der Werf, P.

PY - 2012/7/1

Y1 - 2012/7/1

N2 - We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 μm flux density (~300 mJy). It is the only high-redshift Planck detection in the 130 deg2 H-ATLAS Phase-I area. Keck Adaptive Optics images reveal a quadruply imaged galaxy in the K band while the Submillimeter Array and the Jansky Very Large Array show doubly imaged 880 μm and CO(1→0) sources, indicating differentiated distributions of the various components in the galaxy. In the source plane, the stars reside in three major kpc-scale clumps extended over ~1.6 kpc, the dust in a compact (~1 kpc) region ~3 kpc north of the stars, and the cold molecular gas in an extended (~7 kpc) disk ~5 kpc northeast of the stars. The emissions from the stars, dust, and gas are magnified by ~17, ~8, and ~7 times, respectively, by four lensing galaxies at z ~ 1. Intrinsically, the lensed galaxy is a warm (T dust ~ 40-65 K), hyper-luminous (L IR ~ 1.7 × 1013 L ⊙ star formation rate (SFR) ~2000 M ⊙ yr-1), gas-rich (M gas/M baryon ~ 70%), young (M stellar/SFR ~ 20 Myr), and short-lived (M gas/SFR ~ 40 Myr) starburst. With physical properties similar to unlensed z > 2 SMGs, HATLAS J114637.9-001132 offers a detailed view of a typical SMG through a powerful cosmic microscope.

AB - We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 μm flux density (~300 mJy). It is the only high-redshift Planck detection in the 130 deg2 H-ATLAS Phase-I area. Keck Adaptive Optics images reveal a quadruply imaged galaxy in the K band while the Submillimeter Array and the Jansky Very Large Array show doubly imaged 880 μm and CO(1→0) sources, indicating differentiated distributions of the various components in the galaxy. In the source plane, the stars reside in three major kpc-scale clumps extended over ~1.6 kpc, the dust in a compact (~1 kpc) region ~3 kpc north of the stars, and the cold molecular gas in an extended (~7 kpc) disk ~5 kpc northeast of the stars. The emissions from the stars, dust, and gas are magnified by ~17, ~8, and ~7 times, respectively, by four lensing galaxies at z ~ 1. Intrinsically, the lensed galaxy is a warm (T dust ~ 40-65 K), hyper-luminous (L IR ~ 1.7 × 1013 L ⊙ star formation rate (SFR) ~2000 M ⊙ yr-1), gas-rich (M gas/M baryon ~ 70%), young (M stellar/SFR ~ 20 Myr), and short-lived (M gas/SFR ~ 40 Myr) starburst. With physical properties similar to unlensed z > 2 SMGs, HATLAS J114637.9-001132 offers a detailed view of a typical SMG through a powerful cosmic microscope.

KW - galaxies: formation

KW - galaxies: individual: HATLAS J114637.9–001132

KW - galaxies: interactions

U2 - 10.1088/0004-637X/753/2/134

DO - 10.1088/0004-637X/753/2/134

M3 - Journal article

VL - 753

SP - 134

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

ER -