Hα3: an Hα imaging survey of HI selected galaxies from ALFALFA - III. Nurture builds up the Hubble sequence in the Great Wall

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Table B.1

Linear regression coefficients of the relations in Figs. B.1a through d (only for Def_HI < 0.2) obtained using the bisector method (mean coefficients of the direct and the inverse relation). C = Coma, V = Virgo (Paper II).

Linear regression	r	Sample	Fig. B.1

log M_HI = 0.34 × log M_∗ + 6.25	0.76	C	a
log M_HI = 0.47 × log M_∗ + 4.71	0.85	V	a
log M_HI = 0.52 × log M_∗ + 4.54	0.84	V+C	a
log M_HI/M_∗ = −0.68 × log M_∗ + 6.50	–0.92	C	b
log M_HI/M_∗ = −0.69 × log M_∗ + 6.12	–0.90	V	b
log M_HI/M_∗ = −0.71 × log M_∗ + 6.58	–0.86	V+C	b
log SFR = 0.33 × log M_∗ − 3.71	0.52	C	c
log SFR = 0.80 × log M_∗ − 8.04	0.88	V	c
log SFR = 0.64 × log M_∗ − 6.75	0.85	V+C	c
log SSFR = −0.70 × log M_∗ − 3.43	–0.79	C	d
log SSFR = −0.26 × log M_∗ − 7.53	–0.53	V	d
log SSFR = −0.41 × log M_∗ − 6.23	–0.72	V+C	d

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