2MASX J14254352+3345275 , the SIMBAD biblio

2MASX J14254352+3345275 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST02:49:41

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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
2004MNRAS.351.1290R viz 15       D               3768 122 The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue. ROWAN-ROBINSON M., LARI C., PEREZ-FOURNON I., et al.
2005AJ....130.2571J viz 412 12 The KPNO International Spectroscopic Survey. V. Hα-selected survey list 3. JANGREN A., SALZER J.J., SARAJEDINI V.L., et al.
2005AJ....130.2584S viz 613 20 Spectroscopy of KISS emission-line galaxy candidates. IV. KPNO and WIYN observations. SALZER J.J., JANGREN A., GRONWALL C., et al.
2007ApJ...671..323H viz 15       D               2 54 29 Spitzer spectra of a 10 mJy galaxy sample and the star formation rate in the Local universe. HOUCK J.R., WEEDMAN D.W., LE FLOC'H E., et al.
2008ApJ...686..127W viz 15       D               1 247 29 The most luminous starbursts in the Universe. WEEDMAN D.W. and HOUCK J.R.
2009ApJ...693..370W viz 15       D               1 61 15 Average infrared galaxy spectra from Spitzer flux-limited samples. WEEDMAN D.W. and HOUCK J.R.
2009ApJ...701.1398S viz 15       D               1 367 16 Star formation rates for starburst galaxies from ultraviolet, infrared, and radio luminosities. SARGSYAN L.A. and WEEDMAN D.W.
2012ApJS..200....8K viz 15       D               1 21798 154 AGES: the AGN and Galaxy Evolution Survey. KOCHANEK C.S., EISENSTEIN D.J., COOL R.J., et al.
2014ApJ...788...45T viz 16       D               1 224162 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2014MNRAS.443.2711Y 16       D               1 94 2 Comparing infrared star formation rate indicators with optically derived quantities. YOUNG J.E., GRONWALL C., SALZER J.J., et al.

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