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19952018
most citedIMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr

139 citations · 495 across the 11 of their papers we have counts for

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astro-ph2008★ 139 cited

IMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr

M. Puech, H. Flores, F. Hammer +22

Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z~0.6 for a representative sample of 65 galaxies with emission…

astro-ph2008★ 72 cited

IMAGES II. A surprisingly low fraction of undisturbed rotating spiral disks at z~0.6: The morpho-kinematical relation 6 Gyrs ago

B. Neichel, F. Hammer, M. Puech +21

We present a first combined analysis of the morphological and dynamical properties for the Intermediate MAss Galaxy Evolution Sequence (IMAGES) sample. It is a representative sampl…

astro-ph2006★ 136 cited

531 new spectroscopic redshifts from the CDFS and a test on the cosmological relevance of the GOODS-South field

C. D. Ravikumar, M. Puech, H. Flores +23

(Abbrev.) This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to z=1. Intermediate mass galaxies (MJ <=-20.3) are selected…

astro-ph2006★ 1 cited

The non-linear behavior of the black hole system GRS 1915+105

R. Misra, K. P. Harikrishnan, G. Ambika +1

Using non-linear time series analysis, along with surrogate data analysis, it is shown that the various types of long term variability exhibited by the black hole system GRS 1915+1…

astro-ph2004★ 40 cited

The chaotic behavior of the black hole system GRS 1915+105

R. Misra, K. P. Harikrishnan, B. Mukhopadhyay +2

A modified non-linear time series analysis technique, which computes the correlation dimension , is used to analyze the X-ray light curves of the black hole system GRS 1915+10…

astro-ph2003★ 8 cited

A Continuous Injection Plasma Model for the X-Ray/Radio Knots in Kpc-Scale Jets of AGN

S. Sahayanathan, R. Misra, A. K. Kembhavi +1

We consider the evolution of a spherically expanding plasma cloud, where there is continuous injection of non-thermal electrons. We compute the time dependent electron distribution…