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20052022
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 5k across the 34 of their papers we have counts for

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Showing astro-ph.COShow all

15 papers · 1 filter

astro-ph.CO2013★ 2 cited

Revisiting the Dichotomy of Early-type Galaxies

Yan-Qin He, Cai-Na Hao, Xiao-Yang Xia

We study the relationship among isophotal shapes, central light profiles and kinematic properties of early-type galaxies (ETGs) based on a compiled sample of 184 ETGs. These sample…

astro-ph.CO2013★ 33 cited

Photometric properties and luminosity function of nearby massive early-type galaxies

Y. Q. He, X. Y. Xia, C. N. Hao +3

We perform photometric analyses for a bright early-type galaxy (ETG) sample with 2949 galaxies ( mag) in the redshift range of 0.05 to 0.15, drawn from the SDSS DR…

astro-ph.CO2013★ 25 cited

Star Formation Rates in Resolved Galaxies: Calibrations with Near and Far Infrared Data for NGC5055 and NGC6946

Yiming Li, Alison F. Crocker, Daniela Calzetti +21

We use the near--infrared Brγhydrogen recombination line as a reference star formation rate (SFR) indicator to test the validity and establish the calibration of the {\it Herschel}…

astro-ph.CO2012★ 18 cited

Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. I. Influences of Dust Attenuation and Stellar Population Age

Ye-Wei Mao, Robert C. Kennicutt, Cai-Na Hao +2

The correlation between infrared-to-ultraviolet luminosity ratio and ultraviolet color, i.e. the IRX-UV relation, was regarded as a prevalent recipe for correcting extragalactic du…

astro-ph.CO2012★ 56 cited

Molecular Gas in Infrared Ultraluminous QSO Hosts

X. Y. Xia, Y. Gao, C. -N. Hao +6

We report CO detections in 17 out of 19 infrared ultraluminous QSO (IR QSO) hosts observed with the IRAM 30m telescope. The cold molecular gas reservoir in these objects is in a ra…

astro-ph.CO2012★ 104 cited

Resolving the Far-IR Line Deficit: Photoelectric Heating and Far-IR Line Cooling in NGC 1097 and NGC 4559

Kevin V. Croxall, J. D. Smith, M. G. Wolfire +30

The physical state of interstellar gas and dust is dependent on the processes which heat and cool this medium. To probe heating and cooling of the ISM over a large range of infrare…