ALMA OBSERVATIONS OF THE HOST GALAXY OF GRB 090423 AT z = 8.23: DEEP LIMITS ON OBSCURED STAR FORMATION 630 MILLION YEARS AFTER THE BIG BANG

E. Berger, B. A. Zauderer, R.-r. Chary, T. Laskar, R. Chornock, N. R. Tanvir, E. R. Stanway, A. J. Levan, E. M. Levesque, J. E. Davies

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Abstract

We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F ν(222 GHz) lesssim 33 μJy and F ν(3.6 μm) lesssim 81 nJy. The FIR limit is about 20 times fainter than the luminosity of the local ULIRG Arp 220 and comparable to the local starburst M 82. Comparing this with model spectral energy distributions, we place a limit on the infrared (IR) luminosity of L IR(8-1000 μm) lesssim 3 × 1010 L ☉, corresponding to a limit on the obscured star formation rate of ${\rm SFR_{\rm IR}} \lesssim 5$ M ☉ yr–1. For comparison, the limit on the unobscured star formation rate from Hubble Space Telescope rest-frame ultraviolet (UV) observations is SFRUV lesssim 1 M ☉ yr–1. We also place a limit on the host galaxy stellar mass of M * lesssim 5 × 107 M ☉ (for a stellar population age of 100 Myr and constant star formation rate). Finally, we compare our millimeter observations to those of field galaxies at z gsim 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z gsim 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.
Original languageEnglish
JournalAstrophysical Journal
Volume796
Issue number2
DOIs
Publication statusPublished - 12 Nov 2014

Cite this

ALMA OBSERVATIONS OF THE HOST GALAXY OF GRB 090423 AT z = 8.23: DEEP LIMITS ON OBSCURED STAR FORMATION 630 MILLION YEARS AFTER THE BIG BANG. / Berger, E.; Zauderer, B. A.; Chary, R.-r.; Laskar, T.; Chornock, R.; Tanvir, N. R.; Stanway, E. R.; Levan, A. J.; Levesque, E. M.; Davies, J. E.

In: Astrophysical Journal, Vol. 796, No. 2, 12.11.2014.

Research output: Contribution to journalArticle

Berger, E. ; Zauderer, B. A. ; Chary, R.-r. ; Laskar, T. ; Chornock, R. ; Tanvir, N. R. ; Stanway, E. R. ; Levan, A. J. ; Levesque, E. M. ; Davies, J. E. / ALMA OBSERVATIONS OF THE HOST GALAXY OF GRB 090423 AT z = 8.23: DEEP LIMITS ON OBSCURED STAR FORMATION 630 MILLION YEARS AFTER THE BIG BANG. In: Astrophysical Journal. 2014 ; Vol. 796, No. 2.
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title = "ALMA OBSERVATIONS OF THE HOST GALAXY OF GRB 090423 AT z = 8.23: DEEP LIMITS ON OBSCURED STAR FORMATION 630 MILLION YEARS AFTER THE BIG BANG",
abstract = "We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F ν(222 GHz) lesssim 33 μJy and F ν(3.6 μm) lesssim 81 nJy. The FIR limit is about 20 times fainter than the luminosity of the local ULIRG Arp 220 and comparable to the local starburst M 82. Comparing this with model spectral energy distributions, we place a limit on the infrared (IR) luminosity of L IR(8-1000 μm) lesssim 3 × 1010 L ☉, corresponding to a limit on the obscured star formation rate of ${\rm SFR_{\rm IR}} \lesssim 5$ M ☉ yr–1. For comparison, the limit on the unobscured star formation rate from Hubble Space Telescope rest-frame ultraviolet (UV) observations is SFRUV lesssim 1 M ☉ yr–1. We also place a limit on the host galaxy stellar mass of M * lesssim 5 × 107 M ☉ (for a stellar population age of 100 Myr and constant star formation rate). Finally, we compare our millimeter observations to those of field galaxies at z gsim 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z gsim 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.",
author = "E. Berger and Zauderer, {B. A.} and R.-r. Chary and T. Laskar and R. Chornock and Tanvir, {N. R.} and Stanway, {E. R.} and Levan, {A. J.} and Levesque, {E. M.} and Davies, {J. E.}",
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T1 - ALMA OBSERVATIONS OF THE HOST GALAXY OF GRB 090423 AT z = 8.23: DEEP LIMITS ON OBSCURED STAR FORMATION 630 MILLION YEARS AFTER THE BIG BANG

AU - Berger, E.

AU - Zauderer, B. A.

AU - Chary, R.-r.

AU - Laskar, T.

AU - Chornock, R.

AU - Tanvir, N. R.

AU - Stanway, E. R.

AU - Levan, A. J.

AU - Levesque, E. M.

AU - Davies, J. E.

PY - 2014/11/12

Y1 - 2014/11/12

N2 - We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F ν(222 GHz) lesssim 33 μJy and F ν(3.6 μm) lesssim 81 nJy. The FIR limit is about 20 times fainter than the luminosity of the local ULIRG Arp 220 and comparable to the local starburst M 82. Comparing this with model spectral energy distributions, we place a limit on the infrared (IR) luminosity of L IR(8-1000 μm) lesssim 3 × 1010 L ☉, corresponding to a limit on the obscured star formation rate of ${\rm SFR_{\rm IR}} \lesssim 5$ M ☉ yr–1. For comparison, the limit on the unobscured star formation rate from Hubble Space Telescope rest-frame ultraviolet (UV) observations is SFRUV lesssim 1 M ☉ yr–1. We also place a limit on the host galaxy stellar mass of M * lesssim 5 × 107 M ☉ (for a stellar population age of 100 Myr and constant star formation rate). Finally, we compare our millimeter observations to those of field galaxies at z gsim 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z gsim 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.

AB - We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F ν(222 GHz) lesssim 33 μJy and F ν(3.6 μm) lesssim 81 nJy. The FIR limit is about 20 times fainter than the luminosity of the local ULIRG Arp 220 and comparable to the local starburst M 82. Comparing this with model spectral energy distributions, we place a limit on the infrared (IR) luminosity of L IR(8-1000 μm) lesssim 3 × 1010 L ☉, corresponding to a limit on the obscured star formation rate of ${\rm SFR_{\rm IR}} \lesssim 5$ M ☉ yr–1. For comparison, the limit on the unobscured star formation rate from Hubble Space Telescope rest-frame ultraviolet (UV) observations is SFRUV lesssim 1 M ☉ yr–1. We also place a limit on the host galaxy stellar mass of M * lesssim 5 × 107 M ☉ (for a stellar population age of 100 Myr and constant star formation rate). Finally, we compare our millimeter observations to those of field galaxies at z gsim 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z gsim 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.

U2 - 10.1088/0004-637X/796/2/96

DO - 10.1088/0004-637X/796/2/96

M3 - Article

VL - 796

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

ER -