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Reference: [ETO04B]

Non-detection table: Show non-detection table
Detection table: Show detection table (45 detection) Non-detection table: Show non-detection table (15 non-detection)
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Detection table from ETO04B

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ID	Obs. RA	Obs. Dec	l	b	Source name	Frequency	V_low	V_up	V_peak	V_peak(2)	F_peak	F_peak(2)	List	Ref.
	(J2000)	(J2000)	(deg.)	(deg.)		(MHz)	(km/s)	(km/s)	(km/s)	(km/s)	(Jy)	(Jy)
1	22 19 27.8	+59 51 22	104.908887	2.41315	IRAS 22177+5936	1667	-40.0	-10.8	-40.0	-10.8	0.420	0.06	ENG15	ETO04B
2	19 27 41.6	+16 37 22	51.802535	-0.223573	IRAS 19254+1631	1667	-17.1	20.0	-17.1	20.0	0.140	0.85	ENG15	ETO04B
3	18 51 25.7	-01 03 55	31.982718	-0.483594	IRAS 18488-0107	1667	55.2	96.8	55.2	96.8	0.160	0.98	ENG15	ETO04B
4	19 08 58.3	+08 37 47	42.603351	0.066875	IRAS 19065+0832	1667	36.0	70.3	36.0	70.3	0.470	1.63	ENG15	ETO04B
5	18 48 40.3	-02 50 35	30.086354	-0.68116	IRAS 18460-0254	1667	77.7	120.3	77.7	120.3	1.940	6.76	ENG15	ETO04B
6	18 45 52.7	-01 46 43	30.715212	0.425391	IRAS 18432-0149	1667	49.8	84.1	49.8	84.1	0.590	1.72	ENG15	ETO04B
7	18 28 28.5	-09 58 18	21.451054	0.499592	IRAS 18257-1000	1667	95.9	132.4	95.9	132.4	2.520	0.88	ENG15	ETO04B
8	18 22 42.2	-12 47 44	18.293382	0.432086	IRAS 18198-1249	1667	32.8	63.7	32.8	63.7	0.550	0.94	ENG15	ETO04B
9	18 16 26	-14 55 13	15.701684	0.769854	IRAS 18135-1456	1667	-13.4	15.3	-13.4	15.3	0.910	7.67	ENG15	ETO04B
10	17 58 4.1	-21 21 09	7.959122	1.447367	IRAS 17550-2120	1667	-34.9	-8.0	-34.9	-8.0	0.940	1.98	ENG15	ETO04B
11	17 44 58.6	-27 14 45	1.368317	1.002633	IRAS 17418-2713	1667	-29.3	3.9	-29.3	3.9	3.720	3.43	ENG15	ETO04B
12	17 42 31.7	-33 21 00	355.892743	-1.747771	IRAS 17392-3319	1667	-59.0	-30.4	-59.0	-30.4	0.270	0.44	ENG15	ETO04B
13	17 44 22.6	-31 55 39	357.308482	-1.332995	IRAS 17411-3154	1667	-41.1	-4.0	-41.1	-4.0	18.870	13.55	ENG15	ETO04B
14	17 35 2.1	-33 33 30	354.882477	-0.536978	IRAS 17317-3331	1667	-4.0	25.2	-4.0	25.2	0.810	2.99	ENG15	ETO04B
15	19 26 47.6	+11 21 15	47.063397	-2.539298	IRAS 19244+1115	1667	63.9	99.3	63.9	99.3	0.580	0.33	ENG15	ETO04B
16	19 18 14.5	+23 49 26	57.123973	5.116606	IRAS 19161+2343	1667	10.0	48.2	10.0	48.2	0.570	0.56	ENG15	ETO04B
17	19 09 57.1	+09 26 52	43.440782	0.229578	IRAS 19075+0921	1667	5.3	19.3	5.3	19.3	0.700	0.45	ENG15	ETO04B
18	17 53 46.5	-31 44 26	358.495592	-2.949245	IRAS 17505-3143	1667	-12.9	20.3	-12.9	20.3	0.380	0.48	ENG15	ETO04B
19	22 54 31.9	+60 49 38	109.160591	1.12026	IRAS 22525+6033	1667	-62.1	-43.0	-62.1	-43.0	0.170	0.27	ENG15	ETO04B
20	17 51 26.5	-28 25 36	1.095158	-0.831021	IRAS 17482-2824	1667	-10.8	31.9	-10.8	31.9	0.430	0.83	ENG15	ETO04B
21	20 42 18.7	-08 15 32	38.282328	-28.370069	IRAS 20396-0826	1667	-53.4	-47.2	-53.4	-47.2	0.070	0.12	ENG15	ETO04B
22	19 21 26.3	+11 33 54	46.629316	-1.283216	IRAS 19190+1128	1667	41.1	74.3	41.1	74.3	0.180	0.51	ENG15	ETO04B
23	18 37 32.2	-05 23 59	26.543049	0.618844	IRAS 18348-0526	1667	13.8	39.6	13.8	39.6	9.270	4.26	ENG15	ETO04B
24	15 28 43.7	+03 49 43	8.103521	45.839957	IRAS 15262+0400	1667	37.8	50.2	37.8	50.2	0.300	0.81	ENG15	ETO04B
25	22 19 27.8	+59 51 22	104.908887	2.41315	IRAS 22177+5936	1665	-41.2	-11.4	-41.2	-11.4	0.140	0.08	ENG15	ETO04B
26	19 37 23.5	+20 36 55	56.407962	-0.307135	IRAS 19352+2030	1665	-1.4		-1.4		0.470		ENG15	ETO04B
27	19 09 57.1	+09 26 52	43.440782	0.229578	IRAS 19075+0921	1665	5.2	21.0	5.2	21.0	0.460	0.94	ENG15	ETO04B
28	19 26 47.6	+11 21 15	47.063397	-2.539298	IRAS 19244+1115	1665	56.6	99.3	56.6	99.3	2.990	1.05	ENG15	ETO04B
29	17 35 2.1	-33 33 30	354.882477	-0.536978	IRAS 17317-3331	1665	-6.3	25.2	-6.3	25.2	0.160	0.71	ENG15	ETO04B
30	17 41 52	-33 33 40	355.640482	-1.741638	IRAS 17385-3332	1665	-258.2	-225.5	-258.2	-225.5	0.140	0.12	ENG15	ETO04B
31	17 42 31.7	-33 21 00	355.892743	-1.747771	IRAS 17392-3319	1665	-60.2	-22.5	-60.2	-22.5	0.080	0.07	ENG15	ETO04B
32	19 08 58.3	+08 37 47	42.603351	0.066875	IRAS 19065+0832	1665	34.9		34.9		0.140		ENG15	ETO04B
33	19 37 23.5	+20 36 55	56.407962	-0.307135	IRAS 19352+2030	1667	-1.4		-1.4		0.750		ENG15	ETO04B
34	18 48 40.3	-02 50 35	30.086354	-0.68116	IRAS 18460-0254	1665	81.0		81.0		0.100		ENG15	ETO04B
35	18 45 52.7	-01 46 43	30.715212	0.425391	IRAS 18432-0149	1665	48.7	83.0	48.7	83.0	0.140	0.13	ENG15	ETO04B
36	15 28 43.7	+03 49 43	8.103521	45.839957	IRAS 15262+0400	1665	38.4	49.1	38.4	49.1	0.190	0.22	ENG15	ETO04B
37	20 42 18.7	-08 15 32	38.282328	-28.370069	IRAS 20396-0826	1665	-51.1		-51.1		0.160		ENG15	ETO04B
38	18 37 32.2	-05 23 59	26.543049	0.618844	IRAS 18348-0526	1665	12.1	41.3	12.1	41.3	2.360	1.14	ENG15	ETO04B
39	18 16 26	-14 55 13	15.701684	0.769854	IRAS 18135-1456	1665	-16.2	13.1	-16.2	13.1	0.160	0.16	ENG15	ETO04B
40	17 44 58.6	-27 14 45	1.368317	1.002633	IRAS 17418-2713	1665	-21.4		-21.4		0.340		ENG15	ETO04B
41	17 58 4.1	-21 21 09	7.959122	1.447367	IRAS 17550-2120	1665	-34.9	-7.4	-34.9	-7.4	0.500	0.13	ENG15	ETO04B
42	17 44 22.6	-31 55 39	357.308482	-1.332995	IRAS 17411-3154	1665	-38.3	-14.1	-38.3	-14.1	0.320	0.51	ENG15	ETO04B
43	18 28 28.5	-09 58 18	21.451054	0.499592	IRAS 18257-1000	1665	95.9		95.9		0.170		ENG15	ETO04B
44	22 54 31.9	+60 49 38	109.160591	1.12026	IRAS 22525+6033	1665	-62.7	-41.9	-62.7	-41.9	0.410	0.25	ENG15	ETO04B
45	17 51 26.5	-28 25 36	1.095158	-0.831021	IRAS 17482-2824	1665	-10.8	30.8	-10.8	30.8	0.120	0.13	ENG15	ETO04B

Distribution of sources in all sky (l,b)

Distribution of sources in all sky using Aladin

Tip: Click on some source to get more informaiton

Distribution of sources in IRAS color-color diagram

Tip: Use "Box select" or "Lasso select" to display colour-selected sources in Aladin all-sky view

Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

Original color diagram is taken form van der Veen & Habing (1987)

Type	Description
I	Oxygen-rich non-variable stars without circumstellar shells
II	Variable stars with "young" O-rich circumstellar shells
IIIa	Variable stars with more evolved O-rich circumstellar shells
IIIb	Variable stars with thick O-rich circumstellar shells
IV	Variable stars with very thick O-rich circumstellar shells
V	Planetary nebulae and non- variable stars with very cool circumstellar shells
VIa	Variable stars with relatively cold dust at large distances; a significant part of the stars is carbon-rich
VIb	Variable stars with relatively hot dust close to the star and relatively cold dust at large distances; Some of the objects have proven to be O-rich
VII	Variable stars with more evolved C-rich circumstellar shells
VIII	Different sort of objects

Distribution of the detection velocities versus galactic longitude from ETO04B

Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

Distribution of sources from ETO04B in (l,b) histograms

Display associated data

Group name
Different Line detections
IRAS source	IRAS coordinates (RA, Dec)	IRAS source distance (arcsec)	IRAS flux density (F12,F25,F60,F100)
2MASS source	2MASS coordinates (RA, Dec)	2MASS source distance (arcsec)	2MASS magnituted (J,H,K)
GCVS source	GCVS coordinates (RA, Dec)	GCVS source distance (arcsec)	GCVS parameters
WISE source	WISE coordinates (RA, Dec)	WISE source distance (arcsec)	WISE magnitudes (w1, w2, w3, w4)
Akari IRC source	Akari IRC coordinates (RA, Dec)	Akari IRC source distance (arcsec)	Akari IRC fluxes (S09, S18)
Akari FIS source	Akari FIS coordinates (RA, Dec)	Akari FIS source distance (arcsec)	Akari FIS fluxes (S65, S90, S140, S160)
Continuum source	Continuum coordinates (RA, Dec)	Continuum source distance (arcsec)	Continuum parameters
Bolocam GPS	BGPS coordinates (RA, Dec)	BGPS source distance (arcsec)	BGPS parameters
EGO source	EGO coordinates (RA, Dec)	EGO source distance (arcsec)	EGO parameters
Select all	Select all	Select all	Select all

View images

DSS (optical)	SDSS (optical+NIR)	2MASS (JHK)	WISE (4-22 um)	IRAC (3-8 um)	GLIMPSE 360 (3.6-4.5 um)
AKARI color (60-160 um)	PACS color (70-160 um)	SPIRE color (250-500 um)	ATLASGAL (870 um)	ATLASGAL+Planck (870 um)	Bolocam (1.1 mm)
NVSS (1.4 GHz)	Image size: arcsec (default is 120 arcsec)
	Image size: arcsec (default is 120 arcsec)

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

select MAX(oh_data.ra_hms) as ra_hms,MAX(oh_data.dec_dms) as dec_dms,MAX(oh_data.source_name) as source_name,MAX(oh_data.ra) as ra,MAX(oh_data.dec) as dec,MAX(oh_data.l) as l,MAX(oh_data.b) as b,MAX(oh_data.vlow) as vlow,MAX(oh_data.vup) as vup,MAX(oh_data.vpeak) as vpeak,MAX(oh_data.vpeak_e) as vpeak_e,MAX(oh_data.vpeak2) as vpeak2,MAX(oh_data.vpeak2_e) as vpeak2_e,MAX(oh_data.dv) as dv,MAX(oh_data.other_name) as other_name,MAX(oh_data.peak) as peak,MAX(oh_data.peak_e) as peak_e,MAX(oh_data.peak2) as peak2,MAX(oh_data.peak2_e) as peak2_e,MAX(oh_data.int) as int,MAX(oh_data.int_e) as int_e,MAX(oh_data.rms) as rms,MAX(oh_data.date) as date,MAX(oh_data.date2) as date2,MAX(oh_data.telescope_ref) as telescope_ref,MAX(oh_data.units) as units,MAX(oh_data.beam) as beam,MAX(oh_data.ref) as ref,MAX(oh_data.list_ref) as list_ref,MAX(oh_data.ascii) as ascii,MAX(oh_data.image) as image,MAX(oh_data.id) as id,MAX(oh_data.date_txt) as date_txt,MAX(oh_data.freq) as freq FROM oh_data  WHERE ref ilike 'ETO04B' AND detected=true AND hide=false GROUP BY ref

select oh_data.ra_hms,oh_data.dec_dms,oh_data.source_name,oh_data.ra,oh_data.dec,oh_data.l,oh_data.b,oh_data.vlow,oh_data.vup,oh_data.vpeak,oh_data.vpeak_e,oh_data.vpeak2,oh_data.vpeak2_e,oh_data.dv,oh_data.other_name,oh_data.peak,oh_data.peak_e,oh_data.peak2,oh_data.peak2_e,oh_data.int,oh_data.int_e,oh_data.rms,oh_data.date,oh_data.date2,oh_data.telescope_ref,oh_data.units,oh_data.beam,oh_data.ref,oh_data.list_ref,oh_data.ascii,oh_data.image,oh_data.id,oh_data.date_txt,oh_data.freq FROM oh_data   WHERE ref ilike 'ETO04B' AND detected=true AND hide=false ORDER BY detected DESC,id