This fileset contains the raw and reduced data, as well as previews for all spectra in the Montreal Spectral Library (see link below). Please always cite the references in the "Reference" column when using these spectra. When you use parts or all of this spectral library in a publication, we would appreciate that you acknowledge it in the following way : "This research has benefitted from the Montreal Spectral Library, maintained by Jonathan Gagné at http://sites.google.com/site/mbderg/montreal-spectral-library".

These figures show the positions of J1207 and J1247 (red star symbols; see Gagné et al. 2014b; first link below) in 2MASS/WISE color-magnitude diagrams, compared to the field sequence (black line), its scatter (gray region) and all candidate members to young moving groups from the BASS sample (black dots or purple dots when youth is confirmed; see Gagné et al. 2013; second link below) Please cite the papers below (see related links) when using this figure.

These figures show the 2-dimensional posterior probability density functions associated with each hypothesis, as a function of radial velocity and distance for J1207-3900 and J1247-3816 (see Gagné et al. 2014b; first link). Please refer to Gagné et al. (2014a, second link) for more details on these types of figures, which are output from BANYAN II. Please cite both papers in the links below if you use these figures.

This figure shows the expected position of J1207-3900 (Thick green line; Gagné et al. 2014b, see first link below) and its uncertainty (dashed green line) in a spectral type-absolute magnitude diagram (from Liu et al. 2013, see second link below), using the statistical distance prediction from BANYAN II (Gagné et al. 2014a, see third link below). It can be seen that J1207-3900 is expected to be neither over- or under- luminous as compared to old, field L dwarfs. This is consistent with other young L1 dwarfs, which are inflated, but more dusty ; the two effects cancel out on their total luminosity. However, due to enhanced dust it has redder than normal NIR colors (see Gagné e tal. 2014b). Please cite all 3 references in the links below if you use this figure.

These figures compare J1207-3900 and J1247-3816 to various old and young spectroscopic templates. Please cite Gagné et al. 2014b as well as Cruz et al. 2009 and the poster link below if you use these figures.

This figure shows the complete near-infrared spectra of J1207-3900 and J1247-3816 (see Gagné et al. 2014b, link below), compared to other TW Hydrae candidates and members.

These IDL save files each contain a structure, grouping all spectral indices from several bibliographical references. There is one IDL savefile per spectrum. You can find all spectra in the Montreal Spectral Library (1st link below). The data can be restored into IDL with the following example command : IDL> restore, 'J1247-3816_SpeX_LowRes15_spectral_indices.sav', /verbose It is also possible to restore IDL save files in Python (see 2nd link below on how to do this) Please cite Gagné et al. 2014b (3rd link below) as well as corresponding references in the IDL structure tag names, when you use any of these informations.

This figure is an analog of Figure 4 in Gagné et al. (2014b; see first link below), but adding also all TWA candidates in the BASS survey (see Gagné et al. 2013; second link below). Please cite all papers in the links below if you use this figure.

These figures show the positions of J1207 and J1247 (red star symbols; see Gagné et al. 2014b; first link below) in 2MASS/WISE color-magnitude diagrams, compared to the field sequence (black line), its scatter (gray region) and all candidate members to young moving groups from the BASS sample (black dots or purple dots when youth is confirmed; see Gagné et al. 2013; second link below) Please cite the papers below (see related links) when using this figure.

This fileset contains the data and previews for all spectra in the Montreal Spectral Library (see link below).