| Name . | Hubble . | RA . | DEC . | AV . | R25 . | amax . | d . | m − M . | Distance . | Source . | |$M_{V_{0}}$| . | (B − V)0 . | Scale . | Source . | Proposal . | Number . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| . | Type . | (J2000) . | (J2000) . | (mag) . | (′) . | (′) . | (Mpc) . | (mag) . | method . | . | . | . | (pc) . | SSCs . | ID . | of fields . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . | (16) . | (17) . |
| M81 | Sab | 09:55:33.1 | 69:03:55 | 0.220 | 13.45 | 7.74 | 3.61 | 27.79 ± 0.06 | Cepheids | 1 | −21.10 | 0.91 | 0.87 | 1,2 | 11570 | 29 |
| M101 | Scd | 14:03:12.5 | 54:20:56 | 0.023 | 14.42 | 7.49 | 6.95 | 29.21 ± 0.06 | Cepheids | 2 | −21.37 | 0.44 | 1.68 | 4,6,7 | 9490,9492 | 12 |
| NGC 4258 | Sbc | 12:18:57.5 | 47:18:14 | 0.045 | 9.31 | 8.60 | 7.576 | 29.397 ± 0.032 | MASER | 3 | −21.03 | 0.67 | 1.84 | 3 | 1157 | 17 |
| M51 | Sbc | 13:29:56.2 | 47:13:50 | 0.095 | 5.61 | 3.40 | 8.43 | 29.67 ± 0.02 | SNII | 4 | −21.40 | 0.57 | 2.04 | 4,5 | 10452 | 6(4) |
| NGC 628 | Sc | 01:36:41.7 | 15:47:01 | 0.192 | 5.23 | 5.1 | 9.77 | 29.95 ± 0.04 | SNII | 5 | −20.75 | 0.50 | 2.36 | 4,8 | 10402 | 3 |
| Name . | Hubble . | RA . | DEC . | AV . | R25 . | amax . | d . | m − M . | Distance . | Source . | |$M_{V_{0}}$| . | (B − V)0 . | Scale . | Source . | Proposal . | Number . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| . | Type . | (J2000) . | (J2000) . | (mag) . | (′) . | (′) . | (Mpc) . | (mag) . | method . | . | . | . | (pc) . | SSCs . | ID . | of fields . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . | (16) . | (17) . |
| M81 | Sab | 09:55:33.1 | 69:03:55 | 0.220 | 13.45 | 7.74 | 3.61 | 27.79 ± 0.06 | Cepheids | 1 | −21.10 | 0.91 | 0.87 | 1,2 | 11570 | 29 |
| M101 | Scd | 14:03:12.5 | 54:20:56 | 0.023 | 14.42 | 7.49 | 6.95 | 29.21 ± 0.06 | Cepheids | 2 | −21.37 | 0.44 | 1.68 | 4,6,7 | 9490,9492 | 12 |
| NGC 4258 | Sbc | 12:18:57.5 | 47:18:14 | 0.045 | 9.31 | 8.60 | 7.576 | 29.397 ± 0.032 | MASER | 3 | −21.03 | 0.67 | 1.84 | 3 | 1157 | 17 |
| M51 | Sbc | 13:29:56.2 | 47:13:50 | 0.095 | 5.61 | 3.40 | 8.43 | 29.67 ± 0.02 | SNII | 4 | −21.40 | 0.57 | 2.04 | 4,5 | 10452 | 6(4) |
| NGC 628 | Sc | 01:36:41.7 | 15:47:01 | 0.192 | 5.23 | 5.1 | 9.77 | 29.95 ± 0.04 | SNII | 5 | −20.75 | 0.50 | 2.36 | 4,8 | 10402 | 3 |
Note. (1) Galaxy Name, (2) Hubble morphological type from RC3 (Corwin, Buta & de Vaucouleurs 1994), (3,4) Right ascension, Declination, in J2000, (5): Galactic extinction from Schlafly & Finkbeiner (2011), (6) R25 from RC3 (Corwin et al. 1994), (7) amax is the angular size along the semi-major axis covered by observations, (8) Distance used in this work, (9) Distance modulus, (10) Distance estimation method, (11) Source of distances: 1. Tully et al. (2013); 2. Riess et al. (2016). 3. Reid, Pesce & Riess (2019); 4. Rodríguez, Clocchiatti & Hamuy (2014); 5. Olivares E. et al. (2010), (12,13) Absolute magnitude in V band and (B − V)0 colour from RC3 (Corwin et al. 1994), (14) HST/ACS pixel scale in pc pixel−1, (15) References to previous studies of stellar clusters: 1. Santiago-Cortés, Mayya & Rosa-González (2010); 2. Nantais et al. (2010a); 3. González-Lópezlira et al. (2017); 4. Whitmore et al. (2014); 5. Hwang & Lee (2008); 6. Barmby et al. (2006); 7. Simanton, Chandar & Whitmore (2015); 8. Adamo et al. (2017), (16) HST proposal number, (17) Number of ACS fields of each galaxy used in this work.
| Name . | Hubble . | RA . | DEC . | AV . | R25 . | amax . | d . | m − M . | Distance . | Source . | |$M_{V_{0}}$| . | (B − V)0 . | Scale . | Source . | Proposal . | Number . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| . | Type . | (J2000) . | (J2000) . | (mag) . | (′) . | (′) . | (Mpc) . | (mag) . | method . | . | . | . | (pc) . | SSCs . | ID . | of fields . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . | (16) . | (17) . |
| M81 | Sab | 09:55:33.1 | 69:03:55 | 0.220 | 13.45 | 7.74 | 3.61 | 27.79 ± 0.06 | Cepheids | 1 | −21.10 | 0.91 | 0.87 | 1,2 | 11570 | 29 |
| M101 | Scd | 14:03:12.5 | 54:20:56 | 0.023 | 14.42 | 7.49 | 6.95 | 29.21 ± 0.06 | Cepheids | 2 | −21.37 | 0.44 | 1.68 | 4,6,7 | 9490,9492 | 12 |
| NGC 4258 | Sbc | 12:18:57.5 | 47:18:14 | 0.045 | 9.31 | 8.60 | 7.576 | 29.397 ± 0.032 | MASER | 3 | −21.03 | 0.67 | 1.84 | 3 | 1157 | 17 |
| M51 | Sbc | 13:29:56.2 | 47:13:50 | 0.095 | 5.61 | 3.40 | 8.43 | 29.67 ± 0.02 | SNII | 4 | −21.40 | 0.57 | 2.04 | 4,5 | 10452 | 6(4) |
| NGC 628 | Sc | 01:36:41.7 | 15:47:01 | 0.192 | 5.23 | 5.1 | 9.77 | 29.95 ± 0.04 | SNII | 5 | −20.75 | 0.50 | 2.36 | 4,8 | 10402 | 3 |
| Name . | Hubble . | RA . | DEC . | AV . | R25 . | amax . | d . | m − M . | Distance . | Source . | |$M_{V_{0}}$| . | (B − V)0 . | Scale . | Source . | Proposal . | Number . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| . | Type . | (J2000) . | (J2000) . | (mag) . | (′) . | (′) . | (Mpc) . | (mag) . | method . | . | . | . | (pc) . | SSCs . | ID . | of fields . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . | (16) . | (17) . |
| M81 | Sab | 09:55:33.1 | 69:03:55 | 0.220 | 13.45 | 7.74 | 3.61 | 27.79 ± 0.06 | Cepheids | 1 | −21.10 | 0.91 | 0.87 | 1,2 | 11570 | 29 |
| M101 | Scd | 14:03:12.5 | 54:20:56 | 0.023 | 14.42 | 7.49 | 6.95 | 29.21 ± 0.06 | Cepheids | 2 | −21.37 | 0.44 | 1.68 | 4,6,7 | 9490,9492 | 12 |
| NGC 4258 | Sbc | 12:18:57.5 | 47:18:14 | 0.045 | 9.31 | 8.60 | 7.576 | 29.397 ± 0.032 | MASER | 3 | −21.03 | 0.67 | 1.84 | 3 | 1157 | 17 |
| M51 | Sbc | 13:29:56.2 | 47:13:50 | 0.095 | 5.61 | 3.40 | 8.43 | 29.67 ± 0.02 | SNII | 4 | −21.40 | 0.57 | 2.04 | 4,5 | 10452 | 6(4) |
| NGC 628 | Sc | 01:36:41.7 | 15:47:01 | 0.192 | 5.23 | 5.1 | 9.77 | 29.95 ± 0.04 | SNII | 5 | −20.75 | 0.50 | 2.36 | 4,8 | 10402 | 3 |
Note. (1) Galaxy Name, (2) Hubble morphological type from RC3 (Corwin, Buta & de Vaucouleurs 1994), (3,4) Right ascension, Declination, in J2000, (5): Galactic extinction from Schlafly & Finkbeiner (2011), (6) R25 from RC3 (Corwin et al. 1994), (7) amax is the angular size along the semi-major axis covered by observations, (8) Distance used in this work, (9) Distance modulus, (10) Distance estimation method, (11) Source of distances: 1. Tully et al. (2013); 2. Riess et al. (2016). 3. Reid, Pesce & Riess (2019); 4. Rodríguez, Clocchiatti & Hamuy (2014); 5. Olivares E. et al. (2010), (12,13) Absolute magnitude in V band and (B − V)0 colour from RC3 (Corwin et al. 1994), (14) HST/ACS pixel scale in pc pixel−1, (15) References to previous studies of stellar clusters: 1. Santiago-Cortés, Mayya & Rosa-González (2010); 2. Nantais et al. (2010a); 3. González-Lópezlira et al. (2017); 4. Whitmore et al. (2014); 5. Hwang & Lee (2008); 6. Barmby et al. (2006); 7. Simanton, Chandar & Whitmore (2015); 8. Adamo et al. (2017), (16) HST proposal number, (17) Number of ACS fields of each galaxy used in this work.
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