Update spectra parameters

Select maser type: , , , ,

Actual statistics of known maser sources

Detected / Non-Detected
Number of observations (H2O): 10100/14105
Number of observations (OH): 16700/18523
Number of observations (SiO): 4040/5713
Number of observations (CH3OH I): 3361/7513
Number of observations (CH3OH II): 7823/10236
Number of observations (NH3):
Number of observations (H2CO):

Detected / Non-Detected
Number of objects (H2O): 2793/6514
Number of objects (OH): 4017/4428
Number of objects (SiO): 1971/2329
Number of objects (CH3OH I): 1430/1976
Number of objects (CH3OH II): 1367/5322
Number of objects (NH3):
Number of objects (H2CO):

Classification of objects with masers

	Total	IRAS (12-100 um)	HiGAL (70-500 um)	ATLASGAL (870 um)	Bolocam (1.1 mm)	THOR (1-2 GHz)	CORNISH (5 GHz)
Maser objects related to SFR+MIX category	98 (38.1%)	79 (38.0%)	31 (31.3%)	20 (31.7%)	17 (25.4%)	-1	2 (28.6%)
Young Stellar Objects	15 (22.4%)	11 (19.3%)	5 (15.2%)	4 (13.8%)	3 (12.5%)	-1	0 ( 0.0%)
Radio-emitting sources	12 (21.8%)	6 (13.6%)	5 (13.5%)	6 (17.6%)	3 ( 9.4%)	-1	0 ( 0.0%)
Dense cores	0 ( 0.0%)	0 ( 0.0%)	0 ( 0.0%)	0 ( 0.0%)	0 ( 0.0%)	-1	0 ( 0.0%)
HII regions	1 ( 3.2%)	1 ( 3.4%)	1 ( 4.8%)	1 ( 5.6%)	1 ( 5.6%)	-1	0 ( 0.0%)
Molecular clouds	9 (23.7%)	7 (21.2%)	2 (11.1%)	1 ( 7.1%)	2 (15.4%)	-1	0 ( 0.0%)
Outflow sources	0 ( 0.0%)	0	0	0	0 ( 0.0%)	-1	0
Other SFR sources	1 (100.0%)	1 (100.0%)	1 (100.0%)	1 (100.0%)	1 (100.0%)	-1	0
Maser objects related to EVOLVED category	1735 (57.5%)	1687 (58.4%)	58 (61.7%)	3 (50.0%)	11 (61.1%)	-1	3 (60.0%)
Stars	336 (45.5%)	327 (46.4%)	13 (40.6%)	1 (33.3%)	2 (40.0%)	-1	1 (50.0%)
Mira stars	765 (75.2%)	748 (75.7%)	2 (66.7%)	0	2 (50.0%)	-1	0
OH/IR stars	235 (76.1%)	231 (77.0%)	14 (77.8%)	2 (66.7%)	2 (66.7%)	-1	1 (100.0%)
AGB/Post-AGB stars	356 (67.0%)	348 (67.3%)	28 (70.0%)	2 (66.7%)	9 (75.0%)	-1	1 (50.0%)
Other stars	294 (35.2%)	271 (35.6%)	11 (50.0%)	1 (33.3%)	2 (28.6%)	-1	1 (50.0%)
Star clusters	2 (28.6%)	1 (33.3%)	1 (50.0%)	1 (50.0%)	1 (33.3%)	-1	1 (100.0%)
Planetary nebulas	3 (25.0%)	3 (25.0%)	0 ( 0.0%)	0	0	-1	1 (100.0%)
Supernova Remnats	1 (33.3%)	0 ( 0.0%)	0 ( 0.0%)	0	0	-1	0
Other sources	294 (46.7%)	211 (46.9%)	5 (17.2%)	1 (33.3%)	0 ( 0.0%)	-1	0 ( 0.0%)
Unknown source types	211 (45.1%)	197 (47.7%)	4 (21.1%)	0 ( 0.0%)	0 ( 0.0%)	-1	0 ( 0.0%)
Extragalactic sources	10 (50.0%)	8 (57.1%)	0	0	0	-1	0
No associated SIMBAD sources	73 (51.4%)	6 (26.1%)	1 (10.0%)	1 (100.0%)	0 ( 0.0%)	-1	0

\texttt{**, Symbiotic*, LPV*, Be*, Candidate\_LP*, },\texttt{RRLyr, C*, Candidate\_C*, Orion\_V*, },\texttt{SG*, Candidate\_SG*, V*, V*?, },\texttt{RedSG*, FUOr, Em*, Ae*, Candidate\_Ae*, },\texttt{brownD*, Candidate\_brownD*, S*, },\texttt{PulsV*RVTau, EB*, SB*, PM*, pMS*, },\texttt{HMXB, EB*Algol, BlueSG*, Candidate\_PulsV*WVi, },\texttt{Candidate\_RSG*, PulsV*delSct, },\texttt{TTau*}
\multicolumn{2}{l}{\textbf{}} & 98 (38.1\%) & 15 (46.9\%) & 20 (31.7\%) & 31 (31.3\%) & 17 (25.4\%) & 79 (38.0\%) & 2 (28.6\%) \\
Young Stellar Objects & \texttt{YSO, Candidate\_YSO} & 15 (22.4\%) & 0 & 4 (13.8\%) & 5 (15.2\%) & 3 (12.5\%) & 11 (19.3\%) & 0 ( 0.0\%) \\
Radio-emitting sources & \texttt{Radio, Radio(sub-mm), Radio(mm), } & 12 (21.8\%) & 0 & 6 (17.6\%) & 5 (13.5\%) & 3 ( 9.4\%) & 6 (13.6\%) & 0 ( 0.0\%) \\
& \texttt{Radio(cm)} & & & & \\
Dense cores & \texttt{denseCore} & 0 ( 0.0\%) & 0 & 0 ( 0.0\%) & 0 ( 0.0\%) & 0 ( 0.0\%) & 0 ( 0.0\%) & 0 ( 0.0\%) \\
HII regions & \texttt{HII, Bubble} & 1 ( 3.2\%) & 0 & 1 ( 5.6\%) & 1 ( 4.8\%) & 1 ( 5.6\%) & 1 ( 3.4\%) & 0 ( 0.0\%) \\
Molecular clouds & \texttt{MolCld, PartOfCloud, Cloud, DkNeb} & 9 (23.7\%) & 0 & 1 ( 7.1\%) & 2 (11.1\%) & 2 (15.4\%) & 7 (21.2\%) & 0 ( 0.0\%) \\
Outflow sources & \texttt{Outflow, outflow?} & 0 ( 0.0\%) & 0 & 0 & 0 & 0 ( 0.0\%) & 0 & 0 \\
Other SFR sources & \texttt{Region, SFregion, ISM, HH} & 1 (100.0\%) & 0 & 1 (100.0\%) & 1 (100.0\%) & 1 (100.0\%) & 1 (100.0\%) & 0 \\
\multicolumn{2}{l}{\textbf{}} & 1735 (57.5\%) & 709 (61.4\%) & 3 (50.0\%) & 58 (61.7\%) & 11 (61.1\%) & 1687 (58.4\%) & 3 (60.0\%) \\
Stars & \texttt{Star} & 336 (45.5\%) & 60 (61.2\%) & 1 (33.3\%) & 13 (40.6\%) & 2 (40.0\%) & 327 (46.4\%) & 1 (50.0\%) \\
Mira stars & \texttt{Mira, Candidate\_Mi*} & 765 (75.2\%) & 568 (74.6\%) & 0 & 2 (66.7\%) & 2 (50.0\%) & 748 (75.7\%) & 0 \\
OH/IR stars & \texttt{OH/IR} & 235 (76.1\%) & 51 (92.7\%) & 2 (66.7\%) & 14 (77.8\%) & 2 (66.7\%) & 231 (77.0\%) & 1 (100.0\%) \\
AGB/Post-AGB stars & \texttt{AGB*, Candidate\_AGB*, post-AGB*, } & 356 (67.0\%) & 20 (43.5\%) & 2 (66.7\%) & 28 (70.0\%) & 9 (75.0\%) & 348 (67.3\%) & 1 (50.0\%) \\
& \texttt{Candidate\_post-AGB*} & & & & \\
Other stars & \fnsymbol{footnote} & 294 (35.2\%) & 89 (27.3\%) & 1 (33.3\%) & 11 (50.0\%) & 2 (28.6\%) & 271 (35.6\%) & 1 (50.0\%) \\
Star clusters & \texttt{OpCl, Cl*, Cl*?} & 2 (28.6\%) & 1 (25.0\%) & 1 (50.0\%) & 1 (50.0\%) & 1 (33.3\%) & 1 (33.3\%) & 1 (100.0\%) \\
Planetary nebulas & \texttt{PN, PN?, RfNeb, BrNeb, *inNeb} & 3 (25.0\%) & 0 ( 0.0\%) & 0 & 0 ( 0.0\%) & 0 & 3 (25.0\%) & 1 (100.0\%) \\
Supernova Remnats & \texttt{SN, SNR, SNR?} & 1 (33.3\%) & 0 & 0 & 0 ( 0.0\%) & 0 & 0 ( 0.0\%) & 0 \\
\multicolumn{2}{l}{\textbf{Other sources}} & 294 (46.7\%) & 15 (37.5\%) & 1 (33.3\%) & 5 (17.2\%) & 0 ( 0.0\%) & 211 (46.9\%) & 0 ( 0.0\%) \\
& \texttt{Maser, X, Unknown, multiple\_object, } & 211 (45.1\%) & 10 (38.5\%) & 0 ( 0.0\%) & 4 (21.1\%) & 0 ( 0.0\%) & 197 (47.7\%) & 0 ( 0.0\%) \\
& \texttt{EmObj} & & & & \\
Extragalactic sources & \texttt{StarburstG, GinPair, Seyfert, } & 10 (50.0\%) & 5 (50.0\%) & 0 & 0 & 0 & 8 (57.1\%) & 0 \\
& \texttt{AGN, Galaxy, EmG, LSB\_G, HII\_G, } & & & & \\
& & 73 (51.4\%) & 0 ( 0.0\%) & 1 (100.0\%) & 1 (10.0\%) & 0 ( 0.0\%) & 6 (26.1\%) & 0

target type	Objects (total)	SFR	EVOLVED	MIXED	OTHER
targeted	-1/-1 (0)	-1/-1 (0)	-1/-1 (0)	-1/-1 (0)	-1/-1 (0)
blind	-1/-1 (0)	-1/-1 (0)	-1/-1 (0)	-1/-1 (0)	-1/-1 (0)

DSS colored	2MASS colored	WISE colored
PACS color (70-160 um)	SPIRE color (250-500 um)	GLIMPSE 360
SDSS color	IRAC color I1,I2,I4	NVSS (1.4GHz)
ATLASGAL 870 um	ATLASGAL 870 um + Planck	Bolocam 1.1 mm
UKIDSS K Download UKIDSS K FITS	2MASS K Download 2MASS K FITS