J/MNRAS/380/1497  JHKs & GLIMPSE photometry towards G305.2+0.2 (Longmore+, 2007)

Embedded stellar populations towards young massive star formation regions. I. G305.2+0.2. Longmore S.N., Maercker M., Ramstedt S., Burton M.G. <Mon. Not. R. Astron. Soc., 380, 1497-1510 (2007)> =2007MNRAS.380.1497L 2007MNRAS.380.1497L
ADC_Keywords: H II regions ; Photometry, infrared Keywords: stars: early-type - stars: evolution - stars: formation - stars: pre-main-sequence - open clusters and associations: general - infrared: stars Abstract: We present deep, wide field J, H and Ks images taken with Infrared Imager and Spectrometer 2 (IRIS2) on the Anglo-Australian Telescope, towards the massive star formation region G305.2+0.2. Combined with 3.6, 4.5, 5.8 and 8.0um data from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) survey on the Spitzer Space Telescope, we investigate the properties of the embedded stellar populations. After removing contamination from foreground stars, we separate the sources based on their infrared (IR) colour. Strong extended emission in the GLIMPSE images hampers investigation of the most embedded sources towards the known sites of massive star formation. However, we find a sizeable population of IR excess sources in the surrounding region free from these completeness effects. Investigation reveals the recent star formation activity in the region is more widespread than previously known. Description: The J-, H- and Ks-band (1.2, 1.6 and 2.2um) images were observed using IRIS2 (Infrared Imager and Spectrometer 2) on the 3.9-m Anglo-Australian Telescope (AAT) at Siding Spring Observatory. The Ks-band observations were taken on 2002 July 25 and the J/H band observations were carried out on 2006 May 16-17 with seeing of 1-1.2arcsec. For each source, a 3x3 image grid was created with ∼1arcmin offsets from the pointing centre. The integration time at each of the nine grid points was around 1min with 3x20s, 6x10s and 9x6s exposures at J, H and Ks, respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 136 7282 *IRIS2-GLIMPSE catalog of sources in G305.2+0.2 -------------------------------------------------------------------------------- Note on table1.dat: Sources identified as [LMR2007] DDD.dddd+DD.dddd in Simbad. -------------------------------------------------------------------------------- See also: http://www.astro.wisc.edu/glimpse/glimpsedata.html : GLIMPSE Home Page Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.4 deg RAdeg Right Ascension (J2000) 10- 17 F8.4 deg DEdeg Declination (J2000) 20- 25 F6.3 mag Jmag ?=- J magnitude from IRIS-2 27- 31 F5.3 mag e_Jmag ?=- J magnitude error 33- 37 I5 --- JID ?=- ID number of the IRIS-2 source 40- 45 F6.3 mag Hmag ?=- H magnitude from IRIS-2 47- 51 F5.3 mag e_Hmag ?=- H magnitude error 53- 57 I5 --- HID ?=- ID number of the IRIS-2 source 60- 65 F6.3 mag Ksmag ?=- Ks magnitude from IRIS-2 67- 71 F5.3 mag e_Ksmag ?=- Ks magnitude error 73- 77 I5 --- KsID ?=- ID number of the IRIS-2 source 80- 85 F6.3 mag 3.6mag ?=- GLIMPSE magnitude at 3.6µm 87- 91 F5.3 mag e_3.6mag ?=- Mean error on 3.6mag 93- 98 F6.3 mag 4.5mag ?=- GLIMPSE magnitude at 4.5µm 100-104 F5.3 mag e_4.5mag ?=- Mean error on 4.5mag 106-111 F6.3 mag 5.8mag ?=- GLIMPSE magnitude at 5.8µm 113-117 F5.3 mag e_5.8mag ?=- Mean error on 5.8mag 119-124 F6.3 mag 8.0mag ?=- GLIMPSE magnitude at 8.0µm 126-130 F5.3 mag e_8.0mag ?=- Mean error on 8.0mag 133-136 I4 --- GLIMPSE Glimpse identification -------------------------------------------------------------------------------- Acknowledgements: Steve Longmore, slongmore(at)cfa.harvard.edu
(End) Patricia Vannier [CDS] 21-Jan-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line