Table 1.

Description of our sample and the ALMA observations.|$^*$|

J1208−0200J2228+0152J2239+0207
RA (J2000.0)|${12^\rm h}{08^\rm m}{59^{\rm s}_{.}}22$||${22^\rm h}{28^\rm m}{47^{\rm s}_{.}}71$||${22^\rm h}{39^\rm m}{47^{\rm s}_{.}}48$|
Dec (J2000.0)|${-02{^{\circ}}00^{\prime}34^{\prime\prime}_{.}9}$||${+01{^{\circ}}52^{\prime}40^{\prime\prime}_{.}4}$||${+02{^{\circ}}07^{\prime}47^{\prime\prime}_{.}4}$|
|$z_{\rm Ly\alpha }$|6.26.086.26
|$M_{\rm 1450}$| (mag)|$-$|24.3|$-$|24.0|$-$|24.6
Number of antennas44–4644–4746–47
Baseline (m)15.1–783.515.1–783.515.1–783.5
On-source time (minutes)878765
Bandpass calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
Complex gain calibratorJ1218|$-$|0119J2226|$+$|0052J2226|$+$|0052
Flux calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
[C ii] cube
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}39}$||${0{^{\prime \prime}_{.}}44}$|  |$\times$|  |${0{^{\prime \prime}_{.}}40}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-59.^{\!\!\!\circ }6$||$-74.^{\!\!\!\circ }2$||$-83.^{\!\!\!\circ }2$|
rms noise per 100 km s|$^{-1}$|0.100.100.11
(mJy beam|$^{-1}$|⁠)
rms noise per 100 km s|$^{-1}$|0.150.150.17
(mJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
Continuum map
Observed continuum frequency (GHz)266.0260.1261.4
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}41}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-60.^{\!\!\!\circ }7$||$-81.^{\!\!\!\circ }1$||$-82.^{\!\!\!\circ }4$|
rms noise16.311.219.1
(μJy beam|$^{-1}$|⁠)
rms noise19.515.726.0
(μJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
J1208−0200J2228+0152J2239+0207
RA (J2000.0)|${12^\rm h}{08^\rm m}{59^{\rm s}_{.}}22$||${22^\rm h}{28^\rm m}{47^{\rm s}_{.}}71$||${22^\rm h}{39^\rm m}{47^{\rm s}_{.}}48$|
Dec (J2000.0)|${-02{^{\circ}}00^{\prime}34^{\prime\prime}_{.}9}$||${+01{^{\circ}}52^{\prime}40^{\prime\prime}_{.}4}$||${+02{^{\circ}}07^{\prime}47^{\prime\prime}_{.}4}$|
|$z_{\rm Ly\alpha }$|6.26.086.26
|$M_{\rm 1450}$| (mag)|$-$|24.3|$-$|24.0|$-$|24.6
Number of antennas44–4644–4746–47
Baseline (m)15.1–783.515.1–783.515.1–783.5
On-source time (minutes)878765
Bandpass calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
Complex gain calibratorJ1218|$-$|0119J2226|$+$|0052J2226|$+$|0052
Flux calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
[C ii] cube
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}39}$||${0{^{\prime \prime}_{.}}44}$|  |$\times$|  |${0{^{\prime \prime}_{.}}40}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-59.^{\!\!\!\circ }6$||$-74.^{\!\!\!\circ }2$||$-83.^{\!\!\!\circ }2$|
rms noise per 100 km s|$^{-1}$|0.100.100.11
(mJy beam|$^{-1}$|⁠)
rms noise per 100 km s|$^{-1}$|0.150.150.17
(mJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
Continuum map
Observed continuum frequency (GHz)266.0260.1261.4
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}41}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-60.^{\!\!\!\circ }7$||$-81.^{\!\!\!\circ }1$||$-82.^{\!\!\!\circ }4$|
rms noise16.311.219.1
(μJy beam|$^{-1}$|⁠)
rms noise19.515.726.0
(μJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
*

Rest-frame UV properties are quoted from Matsuoka et al. (2018c) and Onoue et al. (2019). The coordinates are updated after tying astrometric calibrations to the Gaia database.

The Mg ii redshifts are 6.148 (J1208|$-$|0200) and 6.246 (J2239|$+$|0207), respectively (Onoue et al. 2019). We did not obtain these Mg  ii measurements in hand at the time of our ALMA observations.

Table 1.

Description of our sample and the ALMA observations.|$^*$|

J1208−0200J2228+0152J2239+0207
RA (J2000.0)|${12^\rm h}{08^\rm m}{59^{\rm s}_{.}}22$||${22^\rm h}{28^\rm m}{47^{\rm s}_{.}}71$||${22^\rm h}{39^\rm m}{47^{\rm s}_{.}}48$|
Dec (J2000.0)|${-02{^{\circ}}00^{\prime}34^{\prime\prime}_{.}9}$||${+01{^{\circ}}52^{\prime}40^{\prime\prime}_{.}4}$||${+02{^{\circ}}07^{\prime}47^{\prime\prime}_{.}4}$|
|$z_{\rm Ly\alpha }$|6.26.086.26
|$M_{\rm 1450}$| (mag)|$-$|24.3|$-$|24.0|$-$|24.6
Number of antennas44–4644–4746–47
Baseline (m)15.1–783.515.1–783.515.1–783.5
On-source time (minutes)878765
Bandpass calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
Complex gain calibratorJ1218|$-$|0119J2226|$+$|0052J2226|$+$|0052
Flux calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
[C ii] cube
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}39}$||${0{^{\prime \prime}_{.}}44}$|  |$\times$|  |${0{^{\prime \prime}_{.}}40}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-59.^{\!\!\!\circ }6$||$-74.^{\!\!\!\circ }2$||$-83.^{\!\!\!\circ }2$|
rms noise per 100 km s|$^{-1}$|0.100.100.11
(mJy beam|$^{-1}$|⁠)
rms noise per 100 km s|$^{-1}$|0.150.150.17
(mJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
Continuum map
Observed continuum frequency (GHz)266.0260.1261.4
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}41}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-60.^{\!\!\!\circ }7$||$-81.^{\!\!\!\circ }1$||$-82.^{\!\!\!\circ }4$|
rms noise16.311.219.1
(μJy beam|$^{-1}$|⁠)
rms noise19.515.726.0
(μJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
J1208−0200J2228+0152J2239+0207
RA (J2000.0)|${12^\rm h}{08^\rm m}{59^{\rm s}_{.}}22$||${22^\rm h}{28^\rm m}{47^{\rm s}_{.}}71$||${22^\rm h}{39^\rm m}{47^{\rm s}_{.}}48$|
Dec (J2000.0)|${-02{^{\circ}}00^{\prime}34^{\prime\prime}_{.}9}$||${+01{^{\circ}}52^{\prime}40^{\prime\prime}_{.}4}$||${+02{^{\circ}}07^{\prime}47^{\prime\prime}_{.}4}$|
|$z_{\rm Ly\alpha }$|6.26.086.26
|$M_{\rm 1450}$| (mag)|$-$|24.3|$-$|24.0|$-$|24.6
Number of antennas44–4644–4746–47
Baseline (m)15.1–783.515.1–783.515.1–783.5
On-source time (minutes)878765
Bandpass calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
Complex gain calibratorJ1218|$-$|0119J2226|$+$|0052J2226|$+$|0052
Flux calibratorJ1229|$+$|0203J2148|$+$|0657J2148|$+$|0657
[C ii] cube
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}39}$||${0{^{\prime \prime}_{.}}44}$|  |$\times$|  |${0{^{\prime \prime}_{.}}40}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-59.^{\!\!\!\circ }6$||$-74.^{\!\!\!\circ }2$||$-83.^{\!\!\!\circ }2$|
rms noise per 100 km s|$^{-1}$|0.100.100.11
(mJy beam|$^{-1}$|⁠)
rms noise per 100 km s|$^{-1}$|0.150.150.17
(mJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
Continuum map
Observed continuum frequency (GHz)266.0260.1261.4
Beam size|${0{^{\prime \prime}_{.}}48}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}41}$||${0{^{\prime \prime}_{.}}45}$|  |$\times$|  |${0{^{\prime \prime}_{.}}38}$|
Position angle (east of north)|$-60.^{\!\!\!\circ }7$||$-81.^{\!\!\!\circ }1$||$-82.^{\!\!\!\circ }4$|
rms noise16.311.219.1
(μJy beam|$^{-1}$|⁠)
rms noise19.515.726.0
(μJy; |${1{^{\prime \prime}_{.}}0}$| aperture)
*

Rest-frame UV properties are quoted from Matsuoka et al. (2018c) and Onoue et al. (2019). The coordinates are updated after tying astrometric calibrations to the Gaia database.

The Mg ii redshifts are 6.148 (J1208|$-$|0200) and 6.246 (J2239|$+$|0207), respectively (Onoue et al. 2019). We did not obtain these Mg  ii measurements in hand at the time of our ALMA observations.

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