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| TYC 4718-375-1 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:52:43 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
1979AJ.....84..783D |
608 | 26 | Spectral classifications for Landolt's celestial equatorial standard stars. | DRILLING J.S. and LANDOLT A.U. | |||||
|
1983AJ.....88..439L |
1 | 222 | 1507 | UBVRI Photometric standard stars around the celestial equator. | LANDOLT A.U. | ||||
| 1990PASP..102..131W | 84 | 44 | UBVRI CCD photometry of stars near SN 1987A. | WALKER A.R. and SUNTZEFF N.B. | |||||
| 1991MNRAS.248..642M | 210 | 103 | UBV(RI)c photometry of equatorial standard stars. A direct comparison between the northern and southern systems. | MENZIES J.W., MARANG F., LAING J.D., et al. | |||||
|
1992AJ....104..340L |
16 | D | 1 | 529 | 4449 | UBVRI photometric standard stars in the magnitude range 11.5 < V < 16.0 around the celestial equator. | LANDOLT A.U. | ||
| 1993RMxAA..25...91G | 21 | 2 | The atmospheric extinction at Estacion Astronomica "Dr Carlos Ulrrico Cesco". | GIL-HUTTON R. | |||||
| 1997PASP..109.1193S | 150 | 12 | The Mount Wilson halo mapping project 1975-1985. I. The UBV(RI)$MW$ photometric system compared with other standard systems: the adopted trigonometric HR diagram in (R-I)$MW$ and (V-I)$MW$. | SANDAGE A. | |||||
|
2003A&A...397..361Z |
3604 | 54 | 15 colour photometry of the Landolt SA 95 standard star field. | ZHOU X., JIANG Z., MA J., et al. | |||||
|
2005AN....326..321B |
310 | 29 | Absolute magnitudes for late-type dwarf stars for Sloan photometry. | BILIR S., KARAALI S. and TUNCEL S. | |||||
|
2009AJ....137.4186L |
15 | D | 1 | 597 | 289 | UBVRI photometric standard stars around the celestial equator: updates and additions. | LANDOLT A.U. | ||
|
2021ApJ...919..131H |
17 | D | 1 | 158508 | 22 | A "quick look" at all-sky Galactic archeology with TESS: 158,000 oscillating red giants from the MIT Quick-look Pipeline. | HON M., HUBER D., KUSZLEWICZ J.S., et al. |