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| BD-04 376 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:54:44 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2012ApJ...756...27L |
15 | D | 1 | 4347 | 64 | Classification of X-ray sources in the XMM-Newton serendipitous source catalog. | LIN D., WEBB N.A. and BARRET D. | ||
|
2013A&A...557A..81M |
15 | D | 1 | 4209 | 16 | Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field. | MELNYK O., PLIONIS M., ELYIV A., et al. | ||
|
2016MNRAS.457..110M |
16 | D | 1 | 5299 | 75 | A spectroscopic survey of X-ray-selected AGNs in the northern XMM-XXL field. | MENZEL M.-L., MERLONI A., GEORGAKAKIS A., et al. | ||
|
2017MNRAS.472..675A |
16 | D | 1 | 13582 | 89 | Wide binaries in Tycho-Gaia: search method and the distribution of orbital separations. | ANDREWS J.J., CHANAME J. and AGUEROS M.A. | ||
|
2019A&A...622L..13M |
16 | D | 1 | 264 | 78 | Extended stellar systems in the solar neighborhood. II. Discovery of a nearby 120° stellar stream in Gaia DR2. | MEINGAST S., ALVES J. and FURNKRANZ V. | ||
|
2019AJ....158...77C |
16 | D | 2 | 156 | 65 | TESS reveals that the nearby Pisces-Eridanus stellar stream is only 120 Myr old. | CURTIS J.L., AGUEROS M.A., MAMAJEK E.E., et al. | ||
|
2020ApJ...893...67M |
16 | D | 1 | 533 | 31 | A relationship between stellar age and spot coverage. | MORRIS B.M. | ||
|
2020A&A...638A...9R |
16 | D | 1 | 2642 | ~ | A census of the nearby Pisces-Eridanus stellar stream. Commonalities with and disparities from the Pleiades. | ROSER S. and SCHILBACH E. | ||
|
2020A&A...639A..64R |
16 | D | 1 | 4276 | 26 | Extended stellar systems in the solar neighborhood. IV. Meingast 1: the most massive stellar stream in the solar neighborhood. | RATZENBOCK S., MEINGAST S., ALVES J., et al. | ||
|
2024AJ....167..210V |
18 | D | 1 | 7289 | ~ | The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. | VACH S., ZHOU G., HUANG C.X., et al. |