I describe the IR and X-ray observational campaign we have undertaken for the purpose of determining the nature of the faint discrete X-ray source population discovered by Chandra in the Galactic Center (GC). Data obtained for this project includes a deep Chandra survey of the Galactic Bulge; deep, high resolution IR imaging from VLT/ISAAC, CTIO/ISPI, and the UKIDSS Galactic Plane Survey (GPS); and IR spectroscopy from VLT/ISAAC and IRTF/SpeX. By cross-correlating the GC X-ray imaging from Chandra with our IR surveys, we identify candidate counterparts to the X-ray sources via astrometry. Using a detailed IR extinction map, we are deriving magnitudes and colors for all the candidates. Having thus established a target list, we will use the m...
The Chandra Galactic Bulge Survey (GBS) is a shallow but wide survey of two approximately 6x1 degree...
International audienceOver the last decade, X-ray observations of Sgr A* have revealed a black hole ...
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central...
I describe the IR and X-ray observational campaign we have undertaken for the purpose of determining...
I describe the IR and X-ray campaign we have undertaken to determine the nature of the faint discret...
We present early results from the first near-IR imaging of the weak X-ray sources discovered in the ...
We present results from the first near-IR imaging of the weak X-ray sources discovered in the Chandr...
I describe the IR and X‐ray campaign we have undertaken to determine the nature of the faint discret...
We present results of a multi-wavelength program to study the faint discrete X-ray source population...
We present results of a multi-wavelength program to study the faint discrete X-ray source population...
We present near-IR imaging of a sample of the faint, hard X-ray sources discovered in the 2001 Chand...
We present near-infrared imaging of a sample of the faint, hard X-ray sources discovered in the 2001...
We present results from the first near‐IR imaging of the weak X‐ray sources discovered in the Chandr...
We report on a campaign to identify the counterparts to the population of X-ray sources discovered a...
The Chandra X-ray Observatory has now discovered nearly 10,000 X-ray point sources in the 2 ◦ × 0.8...
The Chandra Galactic Bulge Survey (GBS) is a shallow but wide survey of two approximately 6x1 degree...
International audienceOver the last decade, X-ray observations of Sgr A* have revealed a black hole ...
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central...
I describe the IR and X-ray observational campaign we have undertaken for the purpose of determining...
I describe the IR and X-ray campaign we have undertaken to determine the nature of the faint discret...
We present early results from the first near-IR imaging of the weak X-ray sources discovered in the ...
We present results from the first near-IR imaging of the weak X-ray sources discovered in the Chandr...
I describe the IR and X‐ray campaign we have undertaken to determine the nature of the faint discret...
We present results of a multi-wavelength program to study the faint discrete X-ray source population...
We present results of a multi-wavelength program to study the faint discrete X-ray source population...
We present near-IR imaging of a sample of the faint, hard X-ray sources discovered in the 2001 Chand...
We present near-infrared imaging of a sample of the faint, hard X-ray sources discovered in the 2001...
We present results from the first near‐IR imaging of the weak X‐ray sources discovered in the Chandr...
We report on a campaign to identify the counterparts to the population of X-ray sources discovered a...
The Chandra X-ray Observatory has now discovered nearly 10,000 X-ray point sources in the 2 ◦ × 0.8...
The Chandra Galactic Bulge Survey (GBS) is a shallow but wide survey of two approximately 6x1 degree...
International audienceOver the last decade, X-ray observations of Sgr A* have revealed a black hole ...
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central...