ALMA data of H2CO 3_21-2_11 and 5_15-4_14 emission lines in the TW HYA Disk

This data set consists of image cubes, images, radial profiles and spectra of two H2CO emission lines towards the protoplanetary disk TW Hya as presented in Öberg et al. (2017, ApJ 839:43 'H2CO Distribution and Formation in the TW HYA Disk'). The data was observed with the Atacama Large Millimeter/submillimeter Array (ALMA) in 2014 as a part of observing program 2013.1.00114.S. In particular the data set corresponds to the channel maps presented in Fig. 1, and the Moment 0 maps, radial profiles and spectra presented in Fig. 2. The image cubes from which all other data products were derived were produced using CASA following standard calibration and imaging procedures as outlined in the publication. The raw data is archived by the ALMA observatory and can be found here: 

http://almascience.nrao.edu/aq/

All publications making use of this data must include the following acknowledgement:

This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00114.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.