las & gcs sv2 reports

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LAS & GCS SV2 reports “UKIDSS SV meeting”, Edinburgh, 15 December 2005 Nicolas Lodieu

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LAS & GCS SV2 reports. Nicolas Lodieu. “UKIDSS SV meeting”, Edinburgh, 15 December 2005. LAS report. Photometry of known L/T dwarfs. LAS diagrams (1). WFCAM tile @ RA=10h46 dec=04 ° 24'. No constraint on the Class. Separation Stars & Galaxies. LAS diagrams (2). (J-H,Y-J) diagram. - PowerPoint PPT Presentation

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Page 1: LAS & GCS SV2 reports

LAS & GCS SV2 reports

“UKIDSS SV meeting”, Edinburgh, 15 December 2005

Nicolas Lodieu

Page 2: LAS & GCS SV2 reports

LAS report

Page 3: LAS & GCS SV2 reports

Photometry of known L/T dwarfs

Page 4: LAS & GCS SV2 reports

No constraint on the Class

LAS diagrams (1)

Separation Stars & Galaxies

WFCAM tile @ RA=10h46 dec=04°24'

Page 5: LAS & GCS SV2 reports

LAS diagrams (2)

(J-H,Y-J) diagram (J-K,Y-J) diagram

Page 6: LAS & GCS SV2 reports

LAS vs SDSSWFCAM tile @ RA=09h40 dec=45°WFCAM tile @ RA=10h46 dec=04°24'

(J-K,z-J) diagram(J-K,z-J) diagram

Page 7: LAS & GCS SV2 reports

Finding charts

Page 8: LAS & GCS SV2 reports

GCS report

Page 9: LAS & GCS SV2 reports

IC4665: completeness limits

Page 10: LAS & GCS SV2 reports

IC4665: errors on the magnitudes

Z

K

J

Y

H

J zoom

0.1 mag @ Z=19.0

0.1 mag @ J=18.5

0.1 mag @ K=17.0

0.1 mag @ Y=19.0

0.1 mag @ H=18.0

Page 11: LAS & GCS SV2 reports

IC4665: CMD (1)

(Y-J,Y) CMD from SV1

Page 12: LAS & GCS SV2 reports

IC4665: CMD (2)(Y-J,Y) CMD from SV2

Page 13: LAS & GCS SV2 reports

IC4665: Finding charts

Page 14: LAS & GCS SV2 reports

Coma Ber: (Y-J,Y) CMD

Page 15: LAS & GCS SV2 reports

Coma Ber: Finding charts

Page 16: LAS & GCS SV2 reports

Upper Sco: (Z-J,Z) CMD

Page 17: LAS & GCS SV2 reports

IC4665: colour-colour diagram

Page 18: LAS & GCS SV2 reports

Conclusions

1) Pipeline

2) Suggestions for WSA

Main concern: photometry in LAS and GCS

1) Pipeline seems to detect objects with nothing at their nominal positions

2) Photometry seems unreliable when two stars are close to each other

1) Coordinates in sexagesimal format when an image is output (currently only coordinates in degrees are output)

2) Possibility to input a list of objects to get their UKIDSS photometry