Details on Acronym: [SSR2017] | |
| [SSR2017] | (Satyapal+Secrest+Ricci+, 2017)= ([SSR2017a]) |
| Write: | <<[SSR2017] SDSS JHHMM+DDMM>> <<[SSR2017] SDSS JHHMM+DDMM Gal N>> |
| N: | 15+29 |
| Object: | Pair of G + G (SIMBAD class: Unknown = Object of Unknown Nature) |
| Note: | Chandra ACIS-S, XMM-Newton, and LBT LUCI NIR observations of N=6+9 pairs of galaxies and N=8+21 galaxies in galaxy mergers. |
| Ref: | =2017ApJ...848..126S |
| by | SATYAPAL S. , SECREST N.J., RICCI C., ELLISON S.L., ROTHBERG B., BLECHA L., CONSTANTIN A., GLIOZZI M., McNULTY P., FERGUSON J. |
| Astrophys. J., 848, 126-126 (2017) | |
| Buried AGNs in advanced mergers: mid-infrared color selection as a dual AGN candidate finder. | |
| o | Tables 3-6: <[SSR2017] SDSS JHHMM+DDMM> N=6, <[SSR2017] SDSS JHHMM+DDMM Gal N> N=8. |
| Ref: | =2019ApJ...875..117P |
| by | PFEIFLE R.W. , SATYAPAL S., SECREST N.J., GLIOZZI M., RICCI C., ELLISON S.L., ROTHBERG B., CANN J., BLECHA L., WILLIAMS J.K., CONSTANTIN A. |
| Astrophys. J., 875, 117-117 (2019) | |
| Buried black hole growth in ir-selected mergers: new results from Chandra. | |
| o | Fig. 2, Table 4: <[SSR2017] SDSS JHHMM+DDMM> N=9 added, <[SSR2017] SDSS JHHMM+DDMM Gal N> N=21 added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [SSR2017a] | |
| [SSR2017a] | (Satyapal+Secrest+Ricci+, 2017) |
| ***** | Avoid the usage of [SSR2017a], prefer [SSR2017] |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |