Name . | This work . | R17 . | O15 . | P16 . |
---|---|---|---|---|
NGC 6822 | 10.47 ± 0.10 | 10.30|$^{+0.04}_{-0.07}$| | – | – |
WLM | 9.95 ± 0.14 | 9.92|$^{+0.09}_{-0.12}$| | 10.09 | – |
Pegasus | 8.50 ± 0.55 | 8.83|$^{+0.23}_{-0.21}$| | 9.02 | – |
Aquarius | 8.82 ± 0.80 | 8.83|$^{+0.46}_{-0.38}$| | 8.80 | – |
NGC 247 | 11.39 ± 0.12 | – | – | 11.10 |
Name . | This work . | R17 . | O15 . | P16 . |
---|---|---|---|---|
NGC 6822 | 10.47 ± 0.10 | 10.30|$^{+0.04}_{-0.07}$| | – | – |
WLM | 9.95 ± 0.14 | 9.92|$^{+0.09}_{-0.12}$| | 10.09 | – |
Pegasus | 8.50 ± 0.55 | 8.83|$^{+0.23}_{-0.21}$| | 9.02 | – |
Aquarius | 8.82 ± 0.80 | 8.83|$^{+0.46}_{-0.38}$| | 8.80 | – |
NGC 247 | 11.39 ± 0.12 | – | – | 11.10 |
Note. The table lists the halo mass from this work compared to literature works that fit the H i data to a dark matter profile. R17 – Read et al. (2017); O15 – Oh et al. (2015); and P16 – Pace (2016).
Name . | This work . | R17 . | O15 . | P16 . |
---|---|---|---|---|
NGC 6822 | 10.47 ± 0.10 | 10.30|$^{+0.04}_{-0.07}$| | – | – |
WLM | 9.95 ± 0.14 | 9.92|$^{+0.09}_{-0.12}$| | 10.09 | – |
Pegasus | 8.50 ± 0.55 | 8.83|$^{+0.23}_{-0.21}$| | 9.02 | – |
Aquarius | 8.82 ± 0.80 | 8.83|$^{+0.46}_{-0.38}$| | 8.80 | – |
NGC 247 | 11.39 ± 0.12 | – | – | 11.10 |
Name . | This work . | R17 . | O15 . | P16 . |
---|---|---|---|---|
NGC 6822 | 10.47 ± 0.10 | 10.30|$^{+0.04}_{-0.07}$| | – | – |
WLM | 9.95 ± 0.14 | 9.92|$^{+0.09}_{-0.12}$| | 10.09 | – |
Pegasus | 8.50 ± 0.55 | 8.83|$^{+0.23}_{-0.21}$| | 9.02 | – |
Aquarius | 8.82 ± 0.80 | 8.83|$^{+0.46}_{-0.38}$| | 8.80 | – |
NGC 247 | 11.39 ± 0.12 | – | – | 11.10 |
Note. The table lists the halo mass from this work compared to literature works that fit the H i data to a dark matter profile. R17 – Read et al. (2017); O15 – Oh et al. (2015); and P16 – Pace (2016).
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