other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
SWIRE J104704.97+592332.3 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST20:07:40 |
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 |
---|---|---|---|---|---|---|---|---|---|
2009A&A...508..117F | 15 | D | 2 | 43 | 19 | Multi-wavelength properties of Spitzer selected starbursts at z∼2. | FIOLET N., OMONT A., POLLETTA M., et al. | ||
2010ApJ...717...29K | 33 | 49 | Far-infrared properties of Spitzer-selected luminous starbursts. | KOVACS A., OMONT A., BEELEN A., et al. | |||||
2010ApJ...724..957S | 361 | D | X | 10 | 40 | 265 | A 158 µm [C II] line survey of galaxies at z ∼ 1-2: an indicator of star formation in the early universe. | STACEY G.J., HAILEY-DUNSHEATH S., FERKINHOFF C., et al. | |
2010A&A...524A..33F | 320 | D | X C | 8 | 20 | 22 | Mid-infrared spectroscopy of Spitzer-selected ultra-luminous starbursts at z ∼ 2. | FIOLET N., OMONT A., LAGACHE G., et al. | |
2014A&A...568A..62D | 16 | D | 1 | 467 | 300 | The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. | DE LOOZE I., CORMIER D., LEBOUTEILLER V., et al. | ||
2015MNRAS.449.2883G | 17 | D | 1 | 58 | 116 | The nature of the [CII] emission in dusty star-forming galaxies from the SPT survey. | GULLBERG B., DE BREUCK C., VIEIRA J.D., et al. | ||
2017ApJ...837...12W | 48 | 17 | The interstellar medium in high-redshift submillimeter galaxies as probed by infrared spectroscopy. | WARDLOW J.L., COORAY A., OSAGE W., et al. | |||||
2023A&A...679A.131R | 47 | O X | 1 | 138 | ~ | Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II], and [N III] up to z = 6. | RAMOS PADILLA A.F., WANG L., VAN DER TAK F.F.S., et al. |