Table 2
Candidate low surface rightness dwarfs in the Virgo cluster.
| ID | RAJ2000 | DecJ2000 | g | r | Rh | μV,h | DM87 |
| [deg] | [deg] | [mag] | [mag] | [arcsec] | [mag/arcsec2] | [deg] | |
|
|
|||||||
| SECCO-LSB-VC1 | 182.26566 | +4.62742 | 9.4 | ||||
| SECCO-LSB-VC2 | 182.26848 | +4.61088 | 9.4 | ||||
| SECCO-LSB-VD1 | 185.28652 | +13.59057 | ~ 19.5 | ~ 18.1 | ~ 13.2 | ~ 26.3 | 2.6 |
| SECCO-LSB-VD2 | 185.28589 | +13.57372 | ~ 23.2 a | ~22.6a | ~2.5a | ~26.8a | 2.6 |
| SECCO-LSB-VD3 | 185.34763 | +13.58349 | ~ 20.6 | ~ 19.8 | ~ 5.8 | ~ 25.9 | 2.6 |
| SECCO-LSB-U1c | 167.39125 | +5.31381 | 21.3 | ||||
| SECCO-LSB-VX1 | 188.48816 | +8.40119 | 4.1 | ||||
Notes. The last group of letters in the ID (after SECCO-LSB-, whose meaning is obvious) may contain a V, indicating the likely association with Virgo, the letter of the SECCO field where the galaxy has been found (in this case Field C, Field D and Field X; see Paper I), anda number to distinguish between dwarfs lying in the same SECCO field. DM87 is the angular distance from the M 87 galaxy, taken as a proxy for the centre of the Virgo cluster. Integrated magnitudes and surface brightness values were corrected for reddening assuming E(B−V) = 0.048 (Paper I).
Same coordinates, within 1.0″, of LSBVCC357 listed by Davies et al. (2016).
This galaxy lies ~4° beyond the zero velocity boundary of Virgo as estimated by Karachentsev & Nosonova (2010), between the Leo I and Leo II galaxy groups, both lying at a distance of about 10−12 Mpc from us, according to the NED database.
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