GREEN PEA GALAXIES AND COHORTS: LUMINOUS COMPACT EMISSION-LINE GALAXIES IN THE SLOAN DIGITAL SKY SURVEY

By Y. Izotov, N. Guseva, T. Thuan. 2011

134 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/042d25a8a2c344326c7151fdc02e950fe23d466e

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. P. V. van Dokkum
2. M. Franx
3. I. Labbé
4. P. Hopkins
5. R. Dav'e
6. A. Dekel
7. G. Brammer
8. L. Hernquist

In Instrumentation

1. P. V. van Dokkum
2. M. Franx
3. I. Labbé
4. G. Brammer
5. K. Whitaker
6. A. Dekel
7. E. Nelson
8. Ivelina G. Momcheva

In Statistical and Nonlinear Physics

1. M. Franx
2. I. Labbé
3. P. V. van Dokkum
4. K. Whitaker
5. M. Oey
6. A. Jaskot
7. Ivelina G. Momcheva
8. E. Nelson

Citations in the corpus

• THE ORIGIN AND OPTICAL DEPTH OF IONIZING RADIATION IN THE “GREEN PEA” GALAXIES (2013, methodology): “Using the Peas’ total stellar masses from Izotov et al. (2011) and the 3 Myr ages, the bursts account for 2-26% of the total stellar mass of the Peas.”
• Star formation sustained by gas accretion (2014, background): “We note that GPs are not special but just extreme cases in the continuous sequence of local star-forming galaxies (e.g., Izotov et al. 2011).”
• Lyα EMISSION FROM GREEN PEAS: THE ROLE OF CIRCUMGALACTIC GAS DENSITY, COVERING, AND KINEMATICS (2015, methodology): “Oxygen abundances are also taken from Izotov et al. (2011), where they were derived from [O III] electron temperature ([O III] λ4363).”
• CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 < z < 2.5 (2014, background): “This effect is only significant where the fraction of nebular gas relative to stars is high, or WHα 300 (e.g., Izotov et al. 2011).”
• Lyman-α spectral properties of five newly discovered Lyman continuum emitters (2016, background): “…Å emission, reaching equivalent widths as high as 1000 Å. Cardamone et al. (2009) identified a sample of ∼ 250 GPs in SDSS DR7, at z = 0.11 − 0.36, while Izotov et al. (2011) extended the number to ∼ 800 over a larger redshift range z = 0.02 − 0.63 (the colour changes with redshift, but their…”
• Detection of high Lyman continuum leakage from four low-redshift compact star-forming galaxies (2016, methodology): “Izotov et al. (2011) instead used not only images but SDSS spectra as well to produce a larger sample of Luminous Compact Galaxies (LCGs) with properties similar to GPs.”
• Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies (2014, background): “The extreme emission lines are thought to originate in starbursts at an early stage of their evolution (Östlin et al. 2001; Izotov et al. 2011; Jaskot & Oey 2013; Amorı́n et al. 2014a).”
• Using Lyman-α to detect galaxies that leak Lyman continuum (2014, background): “…sight, aligned by chance with an outflow axis, or peculiar objects, with extremely high ionisation parameters (e.g. blue compact galaxies, green peas, extremely strong emission line galaxies; Cardamone et al. 2009; Izotov et al. 2011; Jaskot & Oey 2013), may present these characteristics, however.”