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Table D.1

Description of the columns available for the SPP catalog.

Column Label Units Description
1 ID - ID number
2 RAdeg deg Right ascension J2000.0
3 DEdeg deg Declination J2000.0
4 Vmag mag Magnitude transformed into the standard Johnson V magnitude
5 e_Vmag mag Error of Vmag
6 (b − y) mag Strömgren (b − y) color index
7 e_(b − y) mag Error of (b − y)
8 c1 mag Strömgren c1 index
9 e_c1 mag Error of c1
10 m1 mag Strömgren m1 index
11 e_m1 mag Error of m1
12 Hbeta mag New values for the Strömgren Hβ index
13 e_Hbeta mag Error of Hbeta
14 r_MB pc MB distance
15 e_r_MB pc Error of r_MB
16 (b − y)0_MB mag MB intrinsic color (b − y)0
17 e_(b − y)0_MB mag Error of (b − y)0_MB
18 Mv_MB mag MB absolute magnitude
19 e_Mv_MB mag Error of Mv_MB
20 Av_MB mag MB visual absorption
21 e_Av_MB mag Error of Av_MB
22 Teff K MB effective temperature
23 e_Teff K Error of Teff
24 logg – MB surface gravity
25 e_logg – Error of log g
26 lum L ⊙ MB luminosity
27 e_lum L ⊙ Error of lum
28 logAge – MB log (Age)
29 e_logAge – Error of logAge
30 Mass M ⊙ MB stellar mass
31 e_Mass M ⊙ Error of Mass
32 BC mag MB bolometric correction
33 e_BC mag Error of BC
34 DSE – Dse: 3D fitting parameter providing the distance between the star and the ellipsoid of errors in the [m1] − [c1] − Hβ space
35 DSG – Dsg: 3D fitting parameter providing the distance between the star and the point if the grid in the [m1] − [c1] − Hβ space
36 Pmax – Pmax parameter indicating the probability for the star to belong to the most probable point of the grid
37 PmaxB – parameter indicating the probability for the star to belong to the corresponding point of the grid at the other side of the gap
38 Nside – Nside: % of simulated stars located at the corresponding side of the gap1
39 r_EC pc EC distance
40 e_r_EC pc Error of r_EC
41 (b − y)0_EC mag EC intrinsic color (b − y)0
42 e_(b − y)0_EC mag Error of (b − y)0_EC
43 Mv_EC mag EC absolute magnitude
44 e_Mv_EC mag Error of Mv_EC
45 Av_EC mag EC visual absorption
46 e_Av_EC mag Error of Av_EC
47 regNC – Photometric region assigned to the star by the NC method
48 Nreg1 – % of simulated stars located in the early region (up to B9)
49 Nreg2 – % of simulated stars located in the intermediate region (A0-A3)
50 Nreg3 – % of simulated stars located in the late region (up to A9)
51 Nreg4 – % of simulated stars located in the late region (F0-G2)
52 Nreg5 – % of simulated stars located in the late region (later than G2)
53 rB pc MB (B) distance
54 (b − y)0B mag MB (B) (b − y)0 intrinsic color
55 MvB mag MB (B) absolute magnitude
56 AvB mag MB (B) visual absorption
57 TeffB K MB (B) effective temperature
58 loggB – MB (B) surface gravity
59 lumB L ⊙ MB (B) luminosity
60 logAgeB – MB (B) log (Age)
61 MassB M ⊙ MB (B) stellar mass
62 BCB mag MB (B) bolometric correction
63 EMLS – Flag indicating emission line stars according to IPHAS data2
64 DJKmin mag Minimum distance between the location of the star in the (J − K)0 vs. (b − y)0 plot and the main sequence relation (MB method)
65 DKHin mag Minimum distance between the location of the star in the (J − H)0 vs. (b − y)0 plot and the main sequence relation (MB method)
66 FlagJK – FlagJK = DJK,B,min − DJK,min comparing both assignations with 2MASS data
67 FlagJH – FlagJH = DJH,B,min − DJH,min comparing both assignations with 2MASS data

Notes. (B) indicates second option parameters forced to be at the other side of the [c1] − [m1] gap.

(1)

The limit between sides is empirically set at 10 000 K.

(2)

0: if it is not an emission line star, 1: if it is an emission line star, 2: when IPHAS information is not available.

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