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This file contains: relevant columns from Gaia DR2 Pan-STARRS (PS1) photometry (grizy) de-reddened PS1 photometry (g0, r0, etc.) binary masks to apply to select out stars that pass our proper motion and color-magnitude diagram selection (pm_mask, gi_cmd_mask) a binary mask to apply to select out stars in the stream track defined in Price-Whelan & Bonaca (2018) (stream_track_mask) GD-1 positional coordinates (phi1, phi2) Proper motions in the GD-1 coordinate system (pm_phi1_cosphi2, pm_phi2) Proper motions in the GD-1 coordinate system, corrected for solar reflex motion (pm_phi1_cosphi2_no_reflex, pm_phi2_no_reflex) To select out probable members of the GD-1 stream in, e.g., Python, use: from astropy.table import Table tbl = Table.read('gd1-with-masks.fits') tbl = tbl[tbl['pm_mask'] & tbl['gi_cmd_mask']] To select out only stars within the stream track identified in Price-Whelan & Bonaca (2018), do: from astropy.table import Table tbl = Table.read('gd1-with-masks.fits') tbl = tbl[tbl['pm_mask'] & tbl['gi_cmd_mask'] & tbl['stream_track_mask']
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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