C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: We propose a ToO program in response to an ongoing Swift/XRT Deep Galactic Plane Survey. Phase-I is ~73% complete and has detected 150 sources, of which 110 are new or unclassified transients; 25% of Phase-II is approved. The surveys are aimed at mapping X-ray sources with good depth and coverage to enable source identification and multi-wavelength followups. The latter studies crucially depend on the Chandra subarcsec localization, which leads to source identification, especially in the crowded Galactic Plane. We propose 5 CXO ACIS-I (or HRC-I) SLOW ToO observations, at 2.5 ks each (total of 12.5ks), of bright sources found in the remaining part of Phase-I and/or Phase-II, which will be provided to us through private consultation. |
Remarks: In the rare exception of extremely bright sources, we will request an HRC-I observation to avoid ACIS-I saturation. We will communicate the ToO duration, details on the source brightness. |
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