| s selected by MSX colors. The survey covers the full Galactic plane, utilizing both the Karl G. Jansky Very Large Array (VLA) at 43 GHz and the Atacama Large Millimeter/submillimeter Array (ALMA) at 86 GHz. For more information, visit: http://www.phys.unm.edu/~baade/ | |
| in source: | NAME Galactic Bulge |
| Ref: | =2018ApJ...862..153S |
| by | STROH M.C. , PIHLSTROM Y.M., SJOUWERMAN L.O., CLAUSSEN M.J., MORRIS M.R., RICH M.R. |
| Astrophys. J., 862, 153-153 (2018) | |
| Quasi-simultaneous 43 and 86 GHz SiO maser observations and potential bias in the BAaDE survey are resolved. | |
| o | Tables 2-3: <BAaDE aa3a-NNNNN> N=86. |
| Ref: | =2019ApJS..244...25S |
| by | STROH M.C. , PIHLSTROM Y.M., SJOUWERMAN L.O., LEWIS M.O., CLAUSSEN M.J., MORRIS M.R., RICH R.M. |
| Astrophys. J., Suppl. Ser., 244, 25-25 (2019) | |
| The Bulge Asymmetries and Dynamical Evolution (BAaDE) SiO maser survey at 86 GHz with ALMA. | |
| o | Tables 2+5: <BAaDE aa3a-NNNNN> N=1427+4. |
| Ref: | =2020ApJ...892...52L |
| by | LEWIS M.O. , PIHLSTROM Y.M., SJOUWERMAN L.O., STROH M.C., MORRIS M.R., (The BAaDE Collaboration) |
| Astrophys. J., 892, 52-52 (2020) | |
| Carbon- and Oxygen-rich Asymptotic Giant Branch (AGB) stars in the Bulge Asymmetries and Dynamical Evolution (BAaDE) survey. | |
| o | Tables 1-3: <BAaDE aa3a-NNNNN> N=6+23+33. |
| Ref: | =2020ApJ...901...98L |
| by | LEWIS M.O. , PIHLSTROM Y.M., SJOUWERMAN L.O., QUIROGA-NUNEZ L.H. |
| Astrophys. J., 901, 98-98 (2020) | |
| Infrared color separation between thin-shelled oxygen-rich and carbon-rich AGB stars. | |
| o | Tables 1-2: <BAaDE aa3a-NNNNN> N=7+44. |
| Ref: | =2021AJ....161..111D |
| by | DIKE V. , MORRIS M.R., RICH R.M., LEWIS M.O., QUIROGA-NUNEZ L.H., STROH M.C., TRAPP A.C., CLAUSSEN M.J. |
| Astron. J., 161, 111-111 (2021) | |
| Ground vibrational state SiO emission in the VLA BAaDE survey. | |
| o | Table 1: <BAaDE aa3a-NNNNN> N=90. |
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