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Table 1

ALMA Band 7 observations and detected molecular lines in the HD 97048 protoplanetary disk.

Observations Cycle 0 (2011.0.00863.S) Cycle 2 (2013.1.00658.S)
Date observed 14 December 2012 22 May 2015
Baselines (m) 15.1–402 21.4–555.5
On source integration time (min,sec) 23, 59 7, 10
Number of antenna 22 36
CLEAN image weighting Natural

Molecule CO H13CO+ HC15N CO HCO+
Transition J = 3−2 J = 4−3 J = 4−3 J = 3−2 J = 4−3
Frequency (GHz) 345.796 346.998 344.200 345.796 356.734
Einstein A coefficient (s−1) 2.497e-06 3.288e-03 1.879e-03 2.497e-06 3.627e-03
Eup(K) 33.19 41.63 41.30 33.19 42.80
Synthesised beam 0. ′′74 × 0. ′′51 0. ′′74 × 0. ′′51 0. ′′74 × 0. ′′52 0. ′′71 × 0. ′′44 0. ′′67 × 0. ′′42
Beam PA −26° − 26° − 27° −161° − 161°
Spectral resolution (km s−1) 0.21 0.21 0.21 0.10 0.10
σ (Jy beam−1 per channel (a)) 0.016 0.016 0.016 0.016 0.019

Notes. The values for the line frequencies, Einstein A coefficients, and upper energy levels (Eup) are from the Leiden Atomic and Molecular Database: http://home.strw.leidenuniv.nl/~moldata/ (LAMDA; Schöier et al. 2005). (a) At the stated spectral resolution.

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