SDSS J113722.14+352426.6 , the SIMBAD biblio

SDSS J113722.14+352426.6 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.09.26CEST17:10:49


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2021ApJ...906..104C 420       D     X C       8 12 ~ The effects of biconical outflows on Lyα escape from Green peas. CARR C., SCARLATA C., HENRY A., et al.
2021ApJ...914....2K 20       D               1 43 ~ The compact UV size of Green Pea galaxies as local analogs of high-redshift Lyα-emitters. KIM K.J., MALHOTRA S., RHOADS J.E., et al.
2020ApJ...892...48R 19       D               1 38 ~ The Lyman Alpha Reference Sample. X. Predicting Lyα output from star-forming galaxies using multivariate regression. RUNNHOLM A., HAYES M., MELINDER J., et al.
2020ApJ...893..134K 19       D               1 50 ~ The importance of star formation intensity in Lyα escape from Green Pea galaxies and Lyman Break Galaxy Analogs. KIM K., MALHOTRA S., RHOADS J.E., et al.
2020ApJ...896..170R 345       D     X C       7 14 ~ The semiforbidden C III] λ1909 emission in the rest-ultraviolet spectra of green pea galaxies. RAVINDRANATH S., MONROE T., JASKOT A., et al.
2020MNRAS.498.3043M 93             C       1 12 ~ The nature of CR7 revealed with MUSE: a young starburst powering extended Ly α emission at z = 6.6. MATTHEE J., PEZZULLI G., MACKENZIE R., et al.
2019ApJ...872..146J 18       D               1 39 ~ Correlation between SFR surface density and thermal pressure of ionized gas in local analogs of high-redshift galaxies. JIANG T., MALHOTRA S., YANG H., et al.
2018A&A...616A..60O 496       D     X C       11 12 3 Puzzling Lyman-alpha line profiles in green pea galaxies. ORLITOVA I., VERHAMME A., HENRY A., et al.
2018ApJ...855...96H 17       D               3 13 2 A close relationship between Lyα and Mg II in Green Pea galaxies. HENRY A., BERG D.A., SCARLATA C., et al.
2018ApJ...866...33L viz 17       D               1 341 ~ The COS CGM compendium. I. Survey design and initial results. LEHNER N., WOTTA C.B., HOWK J.C., et al.
2017A&A...599A..71D viz 17       D               1 209276 10 Aperture-free star formation rate of SDSS star-forming galaxies. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2017ApJ...838....4Y 17       D               1 31 9 Lyα and UV sizes of Green Pea galaxies. YANG H., MALHOTRA S., RHOADS J.E., et al.
2017ApJ...844..171Y viz 17       D               1 43 28 Lyα profile, dust, and prediction of Lyα escape fraction in Green Pea galaxies. YANG H., MALHOTRA S., GRONKE M., et al.
2017ApJ...851L...9J 17       D               1 33 3 Kinematics and optical depth in the Green Peas: suppressed superwinds in candidate LyC emitters. JASKOT A.E., OEY M.S., SCARLATA C., et al.
2016ApJ...820..130Y 19       D               1 12 33 Green pea galaxies reveal secrets of Lyα escape. YANG H., MALHOTRA S., GRONKE M., et al.
2016ApJ...828...49H 17       D               1 30 8 O VI emission imaging of a galaxy with the Hubble Space Telescope: a warm gas halo surrounding the intense starburst SDSS J115630.63+500822.1. HAYES M., MELINDER J., OSTLIN G., et al.
2015ApJ...809...19H 476       D     X C       11 11 82 Lyα emission from Green Peas: the role of circumgalactic gas density, covering, and kinematics. HENRY A., SCARLATA C., MARTIN C.L., et al.
2013ApJ...765...26S viz 16       D               1 301 11 Dissection of Hα emitters: low-z analogs of z > 4 star-forming galaxies. SHIM H. and CHARY R.-R.
2011ApJ...728..161I 77 99 Green pea galaxies and cohorts: luminous compact emission-line galaxies in the Sloan Digital Sky Survey. IZOTOV Yu.I., GUSEVA N.G. and THUAN T.X.
2009MNRAS.399.1191C 15       D               1 90 112 Galaxy Zoo green peas: discovery of a class of compact extremely star-forming galaxies. CARDAMONE C., SCHAWINSKI K., SARZI M., et al.

goto View the references in ADS


2021.09.26-17:10:49

© Université de Strasbourg/CNRS

    • Contact