Details on Acronym: ALP | |
| ALP | (Anguita+Loyola+Pedreros) |
| ***** | Avoid the usage of ALP, prefer [ALP2000] |
| Origin | of the Acronym: L (2002AJ....123.1971P) |
Details on Acronym: [ALP2000] | |
| [ALP2000] | (Anguita+Loyola+Pedreros, 2000)= (ALP) |
| Write: | <<[ALP2000] JHHMM+DDMM>> <<[ALP2000] JHHMM+DDMM NN>> |
| N: | 2+23+52+16 |
| Object: | QSO + * (SIMBAD class: Star) |
| Stat: | is completely incorporated in Simbad |
| Note: | N=2 QSOs behind the LMC, from Maza, 1989, private communication. Tables 2-4: N=23 ref. stars in the field of QSO [VV98c] J055721.8-671338. N=52 ref. stars in the field of QSO [ALP2000] J0558-6707. N=16 ref. stars in the field of QSO [ALP2000] J0615-6615. See also [PAM2002]. |
| Ref: | =2000AJ....120..845A |
| by | ANGUITA C. , LOYOLA P., PEDREROS M.H. |
| Astron. J., 120, 845-854 (2000) | |
| Proper motion of the Large Magellanic Cloud using QSOs as an inertial reference system. | |
| o | Table 1: <[ALP2000] JHHMM+DDMM> N=2. Tables 2-4: <[ALP2000] JHHMM+DDMM NN> N=23+52+16. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |