Data Set of "Molecular inventory of a young eruptive star's environment - Case study of the classical FU Orionis star V1057 Cyg"

This is the full version of the fits files for each tuning in the "Molecular inventory of a young eruptive star's environment - Case study of the classical FU Orionis star V1057 Cyg” conducted using the IRAM 30-m and the APEX 12-m telescopes.

The paper is accepted for publication in Astronomy & Astrophysics, and can be found at: https://doi.org/10.1051/0004-6361/202245032

The units are in main beam temperature (T_MB) in all cases.

Notes:

IRAM 30-m files:

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v1057cyg_s_*

- v1057cyg_s_0 --> 73 GHz tuning

- v1057cyg_s_1 --> 80 GHz tuning

- v1057cyg_s_2 --> 94 GHz tuning

- v1057cyg_s_3 --> 141 GHz tuning

- v1057cyg_s_4 --> 133 GHz tuning

- v1057cyg_s_5-0806-otf --> 90 GHz tuning in the otf (on the fly) mode, spectra extracted from the source position

- v1057cyg_s_6 --> 202 GHz tuning

- v1057cyg_s_7 --> 210 GHz tuning

- v1057cyg_s_9 --> 242 GHz tuning

APEX 12-m files: 

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- with nFLASH

2021-july-20-tmb.fits

2021-july-21-tmb.fits

2021-july-31-tmb.fits --> otf mode

- with LAsMA --> both otf

v1057cyg-2021-11-19_tmb.fits

v1057cyg-2021-11-20_tmb.fits

- with SEPIA

v1057-cyg-sepia345-tmb.fits