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| IRAS 18487-0015 , the SIMBAD biblio (23 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST12:11:26 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
1988IRASP.C......0J |
14 | D | 1 | 245223 | ~ | Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 | JOINT IRAS SCIENCE WORKING GROUP | ||
|
1993A&AS..101..153P |
761 | 132 | Classification and statistical properties of galactic H2O masers. | PALAGI F., CESARONI R., COMORETTO G., et al. | |||||
|
1994ApJS...91..347B |
1608 | 236 | A 5GHz VLA survey of the galactic plane. | BECKER R.H., WHITE R.L., HELFAND D.J., et al. | |||||
|
1997A&A...325..255B |
203 | 64 | A survey of star-forming regions in the 5 cm lines of OH. | BAUDRY A., DESMURS J.F., WILSON T.L., et al. | |||||
|
2000A&AS..143..269S |
1601 | 191 | A survey of the 6.7 GHz methanol maser emission from IRAS sources. I. Data. | SZYMCZAK M., HRYNEK G. and KUS A.J. | |||||
| 2000MNRAS.312..211S | 70 | 19 | Observations of OH 4765-MHz maser emission from star-forming regions. | SZYMCZAK M., KUS A.J. and HRYNEK G. | |||||
| 2000MNRAS.315..316G | 134 | 4 | Infrared emission from 6.7-GHz methanol maser sources. | GOEDHART S., VAN DER WALT D.J. and SCHUTTE A.J. | |||||
| 2002A&A...383..244V | 62 | 19 | Long-term study of water maser emission associated with young stellar objects. I. The database. | VALDETTARO R., PALLA F., BRAND J., et al. | |||||
| 2002A&A...392..277S | 157 | 62 | 6.7 GHz methanol masers at sites of star formation. A blind survey of the Galactic plane between 20°≤l≤40° and |b|≤0.52°. | SZYMCZAK M., KUS A.J., HRYNEK G., et al. | |||||
| 2003A&A...407..573B | 34 | 34 | Long-term study of water masers associated with Young Stellar Objects. II. Analysis. | BRAND J., CESARONI R., COMORETTO G., et al. | |||||
|
2004A&A...413..233B |
100 | 24 | 12.2GHz survey towards 6.7GHz methanol masers. A comparison of 12.2GHz and 6.7GHz spectra. | BLASZKIEWICZ L. and KUS A.J. | |||||
|
2005A&A...432..737P |
942 | 204 | A general catalogue of 6.7-GHz methanol masers. I. Data. | PESTALOZZI M.R., MINIER V. and BOOTH R.S. | |||||
| 2005ApJS..156..179D | 93 | 48 | Observations of massive star-forming regions with water masers: mid-infrared imaging. | DE BUIZER J.M., RADOMSKI J.T., TELESCO C.M., et al. | |||||
| 2007A&A...476..373F | O | 47 | 27 | Water maser variability over 20 years in a large sample of star-forming regions: the complete database. | FELLI M., BRAND J., CESARONI R., et al. | ||||
| 2010A&A...510A..86C | 580 | D | X C | 15 | 24 | 12 | Looking for high-mass young stellar objects: H2O and OH masers in ammonia cores. | CODELLA C., CESARONI R., LOPEZ-SEPULCRE A., et al. | |
|
2010RAA....10...67L |
15 | D | 1 | 100 | 6 | A search for massive young stellar objects with 98 CH3OH maser sources. | LIU T., WU Y.-F. and WANG K. | ||
|
2014A&A...563A.130S |
39 | X | 1 | 16 | 7 | 6.7 GHz methanol maser survey toward GLIMPSE point sources and BGPS 1.1 mm dust clumps. | SUN Y., XU Y., CHEN X., et al. | ||
| 2017MNRAS.466.4364C | 175 | D | X | 5 | 8 | 2 | Detections of 2 cm formaldehyde emissions towards Galactic star-forming regions with 6 cm counterpart. | CHEN X., SHEN Z.-Q., LI X.-Q., et al. | |
| 2017ApJS..232...29A | 40 | X | 1 | 22 | 4 | Long-term variability of H2CO masers in star-forming regions. | ANDREEV N., ARAYA E.D., HOFFMAN I.M., et al. | ||
| 2017ApJ...851L...3C | 40 | X | 1 | 9 | 1 | The brightest known H2CO maser in the Milky Way: G339.88-1.26. | CHEN X., SHEN Z.-Q., ELLINGSEN S.P., et al. | ||
|
2023ApJS..268...56Z |
17 | D | 2 | 247 | ~ | A Systematic Observational Study on Galactic Interstellar Ratio 18O/17O. II. C18O and C17O J = 2-1 Data Analysis. | ZOU Y.P., ZHANG J.S., HENKEL C., et al. | ||
| 2025A&A...701A.275V | 47 | X | 1 | 25 | ~ | Notes on the formaldehyde masers. | VAN DER WALT D.J. | ||
| 2026ApJS..282...15L | 100 | X | 2 | 21 | ~ | A 6 cm Formaldehyde Line Survey toward WISE Point Sources. | LIU J.-T., CHEN X., OUYANG X.-J., et al. |