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| Query : 2024ApJ...960...98Y |
2024ApJ...960...98Y - Astrophys. J., 960, 98 (2024/January-2)
Indirect Detection of Decaying Dark Matter with High Angular Resolution: The Case for Axion Search by IRCS on the Subaru Telescope.
YIN W. and HAYASHI K.
Abstract (from CDS):
Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.
Journal keyword(s): Cold dark matter - Dark matter distribution - Infrared spectroscopy
Simbad objects: 19
| Number of rows : 19 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | NAME Tuc IV | G | 00 02.9 | -60 51 | ~ | 90 | 0 | |||||
| 2 | NAME Tri II | G | 02 13 17.40 | +36 10 42.4 | ~ | 164 | 0 | |||||
| 3 | NAME Hor I | G | 02 55 31.7 | -54 07 08 | ~ | 169 | 0 | |||||
| 4 | NAME Reticulum II | G | 03 35 42.1 | -54 02 57 | ~ | 375 | 0 | |||||
| 5 | NAME Eridanus II | G | 03 44 21.1 | -43 32 00 | ~ | 216 | 0 | |||||
| 6 | SN 1987A | SN* | 05 35 27.98840 | -69 16 11.1134 | SNIIpec | 5203 | 2 | |||||
| 7 | NAME UMa II Galaxy | G | 08 51 30.0 | +63 07 48 | 13.3 | ~ | 410 | 0 | ||||
| 8 | NAME Leo T | G | 09 34 53.4 | +17 03 05 | 15.1 | ~ | 434 | 0 | ||||
| 9 | NAME Antlia II Dwarf Galaxy | G | 09 35 32.8 | -36 46 02 | ~ | 109 | 0 | |||||
| 10 | NAME Crater II Dwarf Galaxy | G | 11 49 14 | -18 24.8 | ~ | 176 | 0 | |||||
| 11 | NAME Hydra II | G | 12 21 42.1 | -31 59 07 | ~ | 118 | 0 | |||||
| 12 | NAME Draco II | Gl? | 15 52 47.6 | +64 33 55 | ~ | 138 | 0 | |||||
| 13 | Z 300-12 | G | 17 20 14.335 | +57 55 16.39 | 12.40 | 10.6 | ~ | 1428 | 1 | |||
| 14 | ACO 2390 | ClG | 21 53 37.4 | +17 41 46 | ~ | 732 | 2 | |||||
| 15 | NAME Gru II | G | 22 04.1 | -46 26 | ~ | 110 | 0 | |||||
| 16 | NAME Tuc II | G | 22 51 55.1 | -58 34 08 | ~ | 192 | 0 | |||||
| 17 | NAME Grus I | G | 22 56 42.4 | -50 09 48 | ~ | 126 | 0 | |||||
| 18 | ACO 2667 | ClG | 23 51 39.37 | -26 05 02.7 | ~ | 190 | 0 | |||||
| 19 | NAME Tuc III | G | 23 56.6 | -59 36 | ~ | 229 | 0 |
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