ALMA Lensing Cluster Survey (ALCS)A systematic search for lensed dusty galaxies in the early universe

ALMA data products and supporting resources

1) Hubble Frontier Fields (HFF): 5 fields

Cluster name ALCS field of view (ds9 region file) 1.2 mm continuum fits * continuum fits (tar.gz) continuum quick-look image ** cube fits catalog HST Spitzer Herschel Mass models calibrated visibilities (MS) Note
Abell2744    
MACSJ0416.1-2403    
MACSJ1149.5+2223    
AbellS1063    
Abell370    

* Typically you use "cont_all_clean_nat.fits" for 1.2 mm continuum image. A tapered image, cont_all_clean_tap2.0.fits, which may have better S/N for extended sources, is also available. See readme for details.

** For HFF clusters, Tune 1 (ALCS) and Tune 2 (HFF-ALMA, 2013.1.00999.S and 2015.1.01425.S) have different FoVs.

2) CLASH: 12 fields

Cluster name ALCS field of view (ds9 regioin file) 1.2 mm continuum fits * continuum fits (tar.gz) continuum quick-look image cube fits catalog HST Spitzer Herschel Mass moels calibrated visibilities (MS) Note
MACS0329.7-0211      
Abell383      
Abell209      
MACS1931.8-2635      
MACS2129.4-0741      
RXJ2129.7+0005      
RXJ_1347-1145      
MACS1423.8+2404      
MACS1311.0-0310      
MACS1206.2-0847      
MACS1115.9+0129      
MACS0429.6-0253      

* Typically you use "cont_all_clean_nat.fits" for 1.2 mm continuum . A tapered , cont_all_clean_tap2.0.fits, which may have better S/N for extended sources, is also available. See readme for details.

3) RELICS: 16 fields

Cluster name ALCS field of view (ds9 regioin file) 1.2 mm continuum fits * continuum fits (tar.gz) continuum quick-look cube fits catalog HST Spitzer Herschel Mass models calibrated visibilities (MS) Note
Abell2163      
SMACSJ0723.3-7327    
MACSJ0257.1-2325      
ACT-CLJ0102-49151      
MACSJ0417.5-1154      
RXCJ0600.1-2007      
PLCKG171.9-40.7      
RXCJ2211.7-0350      
MACSJ0553.4-3342      
RXCJ0949.8+1707      
RXCJ0032.1+1808    
Abell3192      
MACSJ0159.8-0849      
MACSJ0035.4-2015      
AbellS295      
Abell2537      

* Typically you use "cont_all_clean_nat.fits" for 1.2 mm continuum image. A tapered image, cont_all_clean_tap2.0.fits, which may have better S/N for extended sources, is also available. See readme for details.