; List of sources to be observed by NIKA2 run 1 during the Oct 2015 run ; Planets can be observed: (Strong signal and Calibration) ; Not needed here. In IRAM catalog ; Coordinates in J2000 ; Radio sources from IRAM catalog ; ------------------------------- 3C84, 03h19m48.154s, +41d30'42.16", =0316+413, RNeriPdB, PdBM 3C111, 04h18m21.28s, +38d01'35.8", PdBM, 2Jy 1-2mm, z=0.0485 OJ287, 08h54m48.9s, +20d06'31", Highly Variable. S(3.3) = 2.9 - 8.3 Jy. 0923+392, 09h27m03.01s, +39d02'20.7", RNeri PdB standard, PdBM = 4C+39.25 S(3.3) = 1.3 - 3.2 Jy B0954+658, 09h58m47.26s, +65d33'54.70", F2mm~1Jy B1039+811, 10h44m23.10s, +80d54'39.30", F2mm~1Jy 3C273, 12h29m06.70s, +02d03'08.6", Variable. S(3.3) = 10 - 20 Jy., PdBM 3C279, 12h56m11.1s, -05d47'22", Variable. S(3.3) = 6.4 - 8.2 Jy. 3C286, 13h31m08.3s, +30d30'33", Polar Calibrator, 1.3mm:0.2-0.4Jy, 3mm:0.8-1Jy B1418+546, 14h19m46.600s, +54d23'14.80", NIKA run1 S(2)=1.2 Jy 3C345, 16h42m58.8s, +39d48'37", Variable. S(3.3) = 5.6 - 7.7 Jy., PdBM NRAO530, 17h33m02.7s, -13d04'50", Variable. S(3.3) = 5 - 7 Jy. 1749+096, 17h51m32.8s, +09d39'00.7", RNeris PdB standard ~3 Jy? B1800+440, 18h01m32.310s, +44d04'21.90", NIKA run1 S(2)=0.1Jy 3C380, 18h29m31.8s, +48d44'46", S(3.3) = 1.0 - 2.8 Jy. CygA, 19h59m28.35s, +40d44'02.1", 3C405 3 sources 3C454.3, 22h53m57.7s, +16d08'54", S(2)=S(1)=6Jy variable? RNeriPdB, PdBM ; ; Secondary calibrators from the report by Lisenfeld et al. 2000 ; created by CK, 14-Apr-2012 ; Add from this list to the already available list (CWLEO=IRC10216) ; W3OH is already in the iram-J2000.sou but leave it here for good measure W3OH, 02h27m03.8653s, +61d52'24.829" , secondary calibrator 1mm GL490, 03h27m38.8834s, +58d47'00.719" , secondary calibrator 1mm L1551IRS5, 04h31m34.1541s, +18d08'05.163" , secondary calibrator 1mm HLTAU, 04h31m38.4437s, +18d13'57.978" , secondary calibrator 1mm CRL618, 04h42m53.3448s, +36d06'52.750" , secondary calibrator 1mm ALFORI, 05h55m10.2737s, +07d24'25.393" , secondary calibrator 1mm G45.1, 19h13m22.0201s, +10d50'53.392" , secondary calibrator 1mm K3-50A, 20h01m45.70s, +33d32'43.518", MWC349, 20h32m45.44s, +40d39'36.8", S2mm=1.55 Jy (Secondary Calibrator) RNeriPdB CRL2688, 21h02m18.7458s, +36d41'37.780" , secondary calibrator 1mm NGC7027, 21h07m01.59s, +42d14'10.183", LKH234, 21h43m06.7208s, +66d06'54.618" , secondary calibrator 1mm CepA, 22h56m17.87s, +62d01'49.8", secondary calibrator (AGB star) NGC7538, 23h13m45.33s, +61d28'10.6", secondary calibrator (Uc HII) ;Galactic sources ; strong source, complex map. Test of mapping procedures. ;------------------ SN1181, 02h05m37.88s, +64d49'40.7", =3C58, SNR, 10x10 arcmin map, need 1sigma=4mJy/beam @2mm ie 100s per 2x2 map. See Haley Gomez (Herschel data) Changed coordinates NGC1333, 03h29m10.5s, +31d13'30.9", 5x5 arcmin map, centered on IRAS 4A in Perseus, expect 1Jy at 1mm Crab, 05h34m31.95s, +22d00'52.1", SNR, Map should be 450x450", 200Jy totalflux, look at index variations, Bandiera Horsehead, 05h41m00.0s, -02d27'00.0", 6x6 arcmin horsehead nebula PHBlant map with Mambo exists, Max Flux is low (50mJy/beam at 1mm) NGC2023, 05h41m26.73s, -02d18'18.5", (LBS 36 SM2) (SM1 is within 2 beams) Launhardt96, Peak1.3mm= 0.30 Jy, Total = 3.45 Jy (55x70) OrionLBS23SM, 05h46m08.81s, -00d10'39.9", Peak1.3mm=1.32 Jy, Total 4.80 (70x110") Launhardt96 NGC2071, 05h47m04.84s, +00d21'45.1", LBS 8SM Peak1.3mm=2.27Jy, Total 11.1Jy (70x80") Launhardt96 IRC10216, 09h47m57.41s, +13d16'43.6", F1.1mm=3.764 Jy SgrB2_FIR1, 17h47m19.93s, -28d22'18.3", galactic center (Gordon 1993) G34.262, 18h50m47.0s, +01d10'49", G34.3, 18h53m18.50s, +01d14'58.20", LSR 0.000 FL 12.50 G35.191, 18h59m14.5s, +01d08'46", W49, 19h08m11.4s, +09d03'32", 2200Jy at 100micron W51, 19h23m42.0s, +14d30'33.0", DR21, 20h39m01.1s, +42d19'43.0", strong 1mm source (Hii region extended) DR21_OH, 20h39m01.1s, +42d22'50.2", strong source too (extended) CasA, 23h23m27.85s, +58d48'42.8", SNR, 360x360" map, Look for contaminating dust, Dunne et al KL, 05h35m14.5s, -05d22'30.0", Orion center for maximum polarization (Tatematsu, PASJ, 2008, 60, 407) NGC7023NW, 21h01m36.0s, +68d11'28.0", ; NW cloud CDS gives: 21h01m36.9s, +68d09'48.0", Bright nebula center, Mambo Habart gives RA = 21h 01mn 46.964s DEC = 68d 08' 57.94'' map center ; Weak galactic sources (stars and shells and one molecular cloud) ;---------------------------------- CXTau, 04h14m47.865s, +26d28'11.01", Faint Galactic Sources S1.3mm=20-40mJy? Ph Mauskopf L1495AS, 04h18m39.9s, +28d23'16", Observed by SCUBA at 850 microns, ABacmann FTTau, 04h23m39.19s, +24d56'14.1", F2mm= 51mJy, Karl's expectation DHTau, 04h29m41.56s, +26d32'58.3", F2mm= 17mJy, Karl's expectation ZZTauIRS, 04h30m51.714s, +24d41'47.51", Should be quite strong S1.3mm=100mJy Ph Mauskopf B18, 04h31m55.7s, +24d32'33", Cold core done by Mambo 37mJy near peak 4hrs J. Kirk Cardiff TMC2, 04h32m48.7s, +24d25'12", F1.3mmPeak ~ 45 mJy/beam(11") 2peaks, ABacmann (Old pos was 04h32m45.5s, +24d25'08") GKTau, 04h33m34.56s, +24d21'05.9", F2mm= 6mJy, Karl's expectation AATau, 04h34m55.42s, +24d28'53.2", F2mm= 30mJy, Karl's expectation DOTau, 04h38m28.58s, +26d10'49.4", F2mm= 37mJy, Karl's expectation BullsTail, 04h41m30.0s, +25d45'00.0", Tau Filament, Nutter et al 2008, Scuba 850um map, Do 10x10 arcmin maps, 1h DRTau, 04h47m06.21s, +16d58'42.8", F2mm= 51mJy, Karl's expectation GMAur, 04h55m10.98s, +30d21'59.5", F2mm= 70mJy, Karl's expectation V836Tau, 05h03m06.60s, +25d23'19.7", F2mm= 15mJy, Karl's expectation NGC2268, 05h46m39.0s, +00d00'00", OrionB filament source at the Equator, 2 hrs 10x6 arcmin map (D. Nutter) Follow-up of Scuba2 RHOOPHSM1, 16h26m27.39s, -24d23'57.9", SM1 center of Rho Oph L1689B, 16h34m48.3s, -24d38'04", F1.3mmPeak ~ 65 mJy/beam(11") ABacmann IRC10420, 19h26m48.100s, +11d21'16.70", F1.1mm= 460.7 +-27.8mJy PCyg, 20h17m47.202s, +38d01'58.55", WR147, 20h36m43.640s, +40d21'07.60", Fomalhaut, 22h57m39.046s, -29d37'20.05", F1.0=100mJy, do a fine sampled map to get disk debris ;Nearby Galaxies (Test of mapping) ;--------------- M33, 01h34m11.80s, +30d50'23.40", 600"x500" map -> 3 mol clouds F1mm~11mJy/11" F2mm~7mJy/18", S(353Planck)=2.5+-0.26 Jy Extended NGC604, 01h34m32.8s, +30d47'00.6", Region in M33 mapped by Carsten with Herschel and Gismo, need at least 5x5, coord from Carsten NGC891, 02h22m33.4s, +42d20'57", Nice edge-on galaxy, need at least 5arcmin size map, 600 mJy in 90" (Chini...) +Guelin1993 NGC1068, 02h42m40.7s, -00d00'48", =M77, F1.3mm = 22mJy, rising to 36 at 3mm, S(217Planck)=0.720+-0.065 Jy !... M82, 09h55m52.7s, +69d40'46s, S(143Planck)=0.960+-0.053Jy, S(217Planck)=2.69+-0.050Jy , Coordinates OK. NGC3690, 11h28m32.200s, +58d33'44.00", Galaxy pair F1.2mm = 95+-11mJy on 30", Could be extended, S(353Planck)=0.644+-0.063Jy = Arp299 Arp244, 12h01m52.8s, -18d51'54", Antennae galaxies, S(353Planck)=0.861+-0.097 M87, 12h30m49.40s, +12d23'28.00", Easy to detect NIKA1 run, S(143Planck)=5.34+0.07Jy, S(217Planck)=4.04+0.09Jy Need a map. See radio maps. M51, 13h29m52.37s, +47d11'40.8", Too weak? ;Distant Galaxy or faint quasars (Test of point source flux noise) ; ------------------------------------------------ XMM_M5, 02h18m56.74s, -04d35'44.9", S(1.3mm)exp=10mJy, See Ismael XMM_17, 02h22m11.54s, -07d02'22.9", S(1.3mm)exp=25mJy, See Ismael, very red Spire source XMM_M6, 02h24m22.87s, -04d44'22.9", S(1.3mm)exp=11mJy, See Ismael XMM_M2, 02h25m15.10s, -02d47'09.2", S(1.3mm)exp=12mJy, See Ismael 4C05.19, 04h14m37.8s, +05d34'42", (lensed by MG J0414+0534), z=2.639, S1.2mm=40+-2mJy, nonthermal J07561, 07h56m18.14s, +41d04'08.6", J075618.14+410408.6, z= 5.09, F1.3 mm = 5.5 +- 0.5 mJy Wang et al 2008, ApJ, 135, 1201 APM08279, 08h31m41.7s, +52d45'17.4", z=3.91, S1.2mm=17.0+-0.5mJy (is APM08279+5255 = IRAS F08279+5255) (no + sign in name for Pako) HSO_ID017, 09h03m02.90s, -01d41'27.6", S1.2=15.3+-1.3 mJy, z=2.308 HSO_ID081, 09h03m11.60s, +00d39'06.3", S1.2=20.0+-0.7 mJy, z=3.042 HSO_ID009, 09h07m40.05s, -00d42'00.0", S1.2mm = 6.9+-1.2 mJy Mambo HSO_ID011, 09h10m43.06s, -00d03'22.4", S1.2=12.2+-1.2 mJy, z=1.786 HSO_ID130, 09h13m05.09s -00d53'42.8", S1.2=11.2+-1.2 mJy, z=2.626 HLS091828, 09h18m28.6s, +51d42'23.3", HLSJ091828.6+514223., z=5.243, F1.3sma= 55+-7mJy, F0.88mm= 125+-8mJy, F2mm= 15+-7mJy, Combes et aL. 2012 HAT091840, 09h18m40.8s, +02d30'47", J091840.8+023047, z=2.581, G09v2.343, F1.3mbo= 8.1+-1.2mJy J09272, 09h27m21.82s, +20d01'23.7", J092721.82+200123.7, z= 5.77, F1.3 mm = 5.0 +- 0.8 mJy, F3.5 mm = 0.12 +- 0.03 mJy F10214+4724, 10h24m34.56s, +47d09'09.5", SDSS J102434.56+470909.5, F1.3mm = 10 mJy, faint IRAS galaxy 2mJy expected at 2 mm HLSW01, 10h57m51.1s, +57d30'27", Conley+ 2011, ApJ, z=2.958, S1.3=12.0 +- 0.5 mJy CSO/Z-Spec, S3.4=0.61 +- 0.19 mJy CARMA BR1202-0725, 12h05m23.08s, -07d42'32", z=4.69 S1.2mm= 12.6+-2.3mJy HAT133008, 13h30m08.56s, +24d58'58.3", J133008.4+245900, z=3.111, NB.v1.78, F1.3= 36.9+-0.4mJy (240GHz PdBI) BRI1335-0417, 13h38m03.4s, -04d32'35", z=4.41, S1.2mm= 10.3+-1.0mJy SBS1408+567, 14h09m55.6s, +56d28'26", (other name: J1409+5628), z=2.56, S1.2mm=10.7+-0.6mJy H1413+517, 14h15m46.24s, +11d29'43.4", Cloverleaf z=2.558 F1.3mm 18+-2 mJy Arp220, 15h34m57.10s, +23d30'11.00", S1.3mm=106mJy, S2.6mm=25mJy (Downes, Eckart 2007 ), S(353Planck)=0.943+-0.080 Jy Dole80.2, 15h44m33.25s, +50d23'45.07", Planck Lensed source confirmed, Scuba2, Wise, PdB3mm (30mJy) z=2.6? HFLS3, 17h06m47.8s, +58d46'23", J170647.8+584623, z=6.337, Riechers, Nature, 2013, S240GHz=15+-0.2mJy, S140=3.2+0.12 PdBI MM18423, 18h42m22.5s, +59d38'30", MM18423+5938 z=3.93, S1.2mm=30mJy+-2mJy Lestrade 2010, serendipitous discovery see 2010 iram news GRB121123A, 20h29m16.29s, -11d51'35.9", ToO, BAT+NOT detection 20121123, no z., do OTF_faint maps 1h SMMJ2135, 21h35m11.6s, -01d02'52.0", z=2.326, S1.2mm=26+-4 mJy (SMA), S2.2=2.0+-0.3 (PdB), Swinbank Lensed galaxy PSS2322+1944, 23h22m07.2s, +19d44'23", z=4.12, S1.2mm=9.6+-0.5mJy ; HATLAS Lenses measured by Mambo (Dannerbauer, Omont et al. in preparation) SMam is flux at 1.2mm in mJy HATLENS07, +08h30m51.02s, +01d32'24.87", SMam= 34.6 was in previous runs :HAT083051, J083051.0+013224, z=x , G09v2.97 HATLENS16, +08h49m33.40s, +02d14'43.14", SMam= 13.4 was HAT084933 = J084933.4+021443, z=2.410, G09v2.114, F1.3mbo= 13.5+-3.0mJy HATLENS08, +08h53m58.94s, +01d55'37.21", SMam= 25.6 HATLENS23, +09h09m48.88s, +00d39'15.97", SMam= 2.6 HATLENS09, +11h35m26.36s, -01d46'06.08", SMam= 23.9 was HAT113526, J113526.3-014605, z=3.128, G12v2.43, F1.3mbo= 24+-2.5mJy HATLENS25, +11h38m33.77s, -01d46'56.41", SMam= 0.7 HATLENS03, +11h46m38.01s, -00d11'32.05", SMam= 37.7 was HAT114637, J114637.9-001132, z=3.259, G12v2.30, F1.3mbo= 38+-3.0mJy, Condensation of sources HATLENS12, +12h01m27.62s, -01d40'44.41", SMam= 16.7 HATLENS01, +12h51m35.43s, +26d14'57.42", SMam= 45.2 HATLENS15, +13h00m53.93s, +26d03'02.58", SMam= 13.6 HATLENS10, +13h01m18.06s, +25d37'08.36", SMam= 21.9 HATLENS18, +13h23m29.80s, +31d15'29.19", SMam= 10.2 HATLENS02, +13h26m30.17s, +33d44'08.76", SMam= 39.0 HATLENS04, +13h28m59.34s, +29d23'25.93", SMam= 36.6 HATLENS11, +13h36m49.93s, +29d17'59.49", SMam= 19.8 was HAT133649, J133649.9+291801, z=2.202, NA.v1.144, F1.3mbo= 20+-4.0mJy, 16.4+/-0.7 mJy at 230GHz PdBI HATLENS24, +13h36m59.56s, +32d18'02.45", SMam= 2.5 HATLENS22, +13h38m08.81s, +25d51'56.22", SMam= 4.3 HATLENS19, +13h43m42.37s, +26d39'20.92", SMam= 8.8 HATLENS06, +13h44m29.48s, +30d30'34.64", SMam= 36.0 was HAT134429, J134429.4+303036, z=2.301, NA.v1.56, F1.3mbo= 35+-3.0mJy HATLENS20, +13h48m55.68s, +24d07'45.79", SMam= 8.1 HATLENS17, +13h49m02.61s, +28d46'36.02", SMam= 10.5 HATLENS13, +14h13m51.99s, -00d00'26.83", SMam= 17.2 was HAT141351, J141351.9-000026, z=2.478, G15v2.235, F1.3mbo= 18.3+-1.7mJy HATLENS05, +14h24m13.98s, +02d23'03.62", SMam= 36.0 was HSO_ID141, Cox et al 2011, S1.2=36+-2 mJy Mambo, S2=9.7mJy PdB HATLENS14, +14h44m33.29s, +00d16'38.66", SMam= 13.6 HATLENS21, +14h46m08.65s, +02d19'27.44", SMam= 5.6 ; Deep survey around these sources ;--------------------------------- Subaru, 02h18m02.15s, -05d00'19", Subaru deep field (Scuba) SXDF, 02h18m30.6s, -05d31'30", Centered on Orochi Aztec source: 34mJy at 1.1mm, 15mJy 1.3mmCarma and 70 mJy SMA data 0.88mm. Aztec1, 09h59m42.86s, +02d29'38.2", z=4.65, S1.3mm= 9.4+-1.6 mJy, S850=16mJy, Smolcic 2011, ApJL 731, L27 GN20, 12h37m11.90s, +62d22'12.1", z=4.055, S850um=30mJy, 3.3mm=0.33mJy, Daddi et al 2009, ApJ, 694, 1517 ; Clusters of galaxies (mapping noise test) ; --------------------------------- CL0016+16, 00h18m33.3s, +16d26'36", rc=55", map 3x5', step 9", 20"/s, 5min, T=8keV, y~2E-4 (Hughes Birkinshaw 1998) MS0451, 04h54m11.0s, -03d00'53", z=0.55, y0=3E-4, rc=60" seen by ; Bolocam, ACT, CARMA A520, 04h54m19.0s, +02d56'49", z=0.199, Request by Angelo MACS0717, 07h17m33.8s, +37d45'20", MACS J0717.5+3745 z=0.545800 Bolocam data see M. De Petris, 11.6 keV XSize=5 arcmin, do 7 A665, 08h30m45.2s, +65d52'55", rc=17.7", coordinates OK A697, 08h42m58s, +36d21'56", z= 0.28, y0=3.1E-4, rc=98", bolocam +PlanckESZ RXJ1347-1145, 13h47m31.0s, -11d45'25", Beware of south extension. From Rémi, Coord of the X-ray center and not the south extension A1835, 14h01m02.0s, +02d51'32", yc=5e-4, 3rd brightest X-ray cluster z=0.253200 IDCSJ1426, 14h26m34.0s, +35d08'02.6", z=1.75 SZA detected position A2163, 16h15m45.91s, -06d08'53.5", Same map Thetac=1.2' A2204, 16h32m45.7s, +05d34'43", yc=2e-4 z=0.152158 M2228, 22h28m33.0s, +20d37'14.4", z=0.412, thetac=20", DeltaT0=-1.73mK, y0=3E-4, LaRoque et al 2006., = MACS J2228.5+2036