\ Project: extension of HOPS out to 500 ParSecs (eHOPS) \ PI: S. T. Megeath \ Citation: Pokhrel et al. (2023b) \ Table info: Photometry in the 1-850 micron wavelengths for candidate protostars (CPs) \ Index \ ___ Arbitrary running index \ ra (degrees) \ ___ Right Ascension (J2000) \ dec (degrees) \ ___ Declination (J2000) \ *_flux (Jy) \ ___ flux density \ e_*_flux (Jy) \ ___ flux density uncertainty \ c_*_flux \ ___ completeness limit on the flux density (underestimated if the source is not detected due to saturation) \ ___ if "U", flux density is used as an upper limit \ s_*_flux \ ___ sky limit (underestimated if the source is not detected due to saturation) \ ___ if "U", flux density is used as an upper limit \ photometric bands: \ 2MASS: J (1.25 micron), H (1.65 micron), Ks (2.17 micron) \ Spitzer/IRAC: I1 (3.6 micron), I2 (4.5 micron), I3 (5.8 micron), I4 (8.0 micron) \ Spitzer/MIPS: M1 (24 micron) \ WISE: W1 (3.4 micron), W2 (4.6 micron), W3 (12 micron), W4 (22 micron) \ Herschel/PACS: P1 (70 micron), P2 (100 micron), P3 (160 micron) \ Herschel/SPIRE: SP1 (250 micron), SP2 (350 micron), SP3 (500 micron) \ JCMT/SCUBA2: SC (850 micron) \ Comments: Reason for classifying the source as a CP \fixlen = T | Index| ra| dec|J_flux|e_J_flux|H_flux|e_H_flux|Ks_flux|e_Ks_flux|I1_flux|e_I1_flux|c_I1_flux|I2_flux|e_I2_flux|c_I2_flux|I3_flux|e_I3_flux|c_I3_flux|I4_flux|e_I4_flux|c_I4_flux|M1_flux|e_M1_flux|c_M1_flux|W1_flux|e_W1_flux|W2_flux|e_W2_flux|W3_flux|e_W3_flux|W4_flux|e_W4_flux|P1_flux|e_P1_flux|s_P1_flux|P2_flux|e_P2_flux|s_P2_flux|P3_flux|e_P3_flux|s_P3_flux|SP1_flux|e_SP1_flux|s_SP1_flux|SP2_flux|e_SP2_flux|s_SP2_flux|SP3_flux|e_SP3_flux|s_SP3_flux|SC_flux|e_SC_flux|s_SC_flux| Comments| | long| double| double|double| double|double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| double| char| double| double| char| double| double| char| double| double| char| char| | | degrees| degrees| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| mJy| | | null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| null| 118120 247.02383 -24.88204 null null null null null null 0.2 null 0.1 0.2 null 0.1 null null 0.1 0.4 null 0.3 null null 3.5 null null null null null null null null null null 17.5 null null 5.2 97.9 6.9 6.1 100.8 73.5 109.8 2839.6 80.9 U 2506.5 80.9 U 52.4 6.4 U Step 5--- Using completeness limits for one or more IRAC photometry 129308 248.38645 -24.87127 null null null null null null null null null 0.1 null 0.1 null null null 0.3 null 0.3 null null 3.4 0.2 null 0.1 null 2.8 0.3 8.5 1.7 null null 15.5 144.1 9.4 6.0 null null 11.7 177.9 null 93.7 149.0 null 132.1 2121.7 91.1 U null 7.5 null Step 3--- [3.6]-[4.5] < 0.65, alpha_{4.5,24} > 0.3 152715 246.99755 -24.73606 null null null null null null 0.3 null null 0.3 null 0.1 0.1 null 0.2 null null 0.2 19.1 0.4 28.5 0.3 null 0.2 null 0.7 null 18.8 2.5 null null 16.4 151.5 9.6 5.9 174.5 10.1 6.4 8743.9 123.4 U 523.7 384.6 471.7 8270.3 76.8 U null 4.0 null Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry 229804 246.0102 -24.57684 null null null null null null 0.1 null 0.2 0.1 null 0.1 0.2 null 0.2 0.3 null 0.4 3.9 0.2 6.4 null null null null null null null null null null 14.2 152.7 9.4 5.5 139.9 8.6 6.4 146.3 119.6 123.8 2997.3 89.7 U 2510.8 76.7 U null 6.1 null Step 3--- [3.6]-[4.5] < 0.65, alpha_{4.5,24} > 0.3 235605 246.87482 -24.46072 null null 0.5 0.1 3.0 0.4 null null 39.0 null null 59.0 null null 302.5 null null 484.0 null null 3328.0 null null null null null null null null null null 55.5 13747.3 687.8 24.4 null null 48.0 35612.9 10753.8 1197.9 51260.8 3245.0 U 43998.9 1952.8 U 1491.2 3.5 U Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry 238470 247.37322 -24.56018 null null null null null null 0.1 null 0.1 0.1 null 0.1 null null 0.2 null null 0.2 null null 1.9 null null null null null null null null null null 17.5 116.8 8.3 5.9 138.6 8.6 6.2 46.6 110.0 70.6 2002.3 93.9 U 1820.6 81.0 U null 4.5 null Step 5--- Using completeness limits for one or more IRAC photometry 244790 248.08672 -24.508 3.1 0.1 13.1 0.5 25.8 1.1 40.7 0.5 22.3 44.2 0.5 7.9 50.8 0.6 54.0 54.0 0.7 14.6 null null 2544.0 null null null null null null null null null null 47.3 980.9 49.6 8.0 null null 17.5 13659.6 578.8 U 13281.1 312.3 U 12523.0 296.4 U 34.8 6.8 6.8 Step 5--- Using completeness limits for one or more IRAC photometry 247059 248.27602 -24.502 null null null null null null 0.1 null 0.2 0.1 null 0.1 null null 0.2 0.4 null 0.3 3.1 0.1 5.2 null null null null null null null null null null 15.7 127.3 8.6 5.8 null null 10.7 6754.8 1262.3 U 6478.3 549.9 U 5939.5 646.0 U null 3.6 null Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry 263365 250.10411 -24.49637 null null null null null null null null null 0.1 null 0.1 null null null 0.2 null 0.2 1.7 0.2 3.2 null null null null null null null null null null 19.5 100.2 7.4 5.4 null null 11.2 1628.0 153.0 U 1528.6 92.2 U 1350.9 82.7 U null 47.5 null Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry 280815 246.99624 -24.37398 null null null null null null null null 2.0 null null 1.2 null null 0.6 2.4 0.1 1.7 null null 5.6 null null null null null null null null null null 14.3 127.4 8.2 5.2 null null 6.4 716.1 175.8 216.6 817.6 142.9 300.9 5210.9 92.9 U 31.3 3.9 U Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry 281259 247.01979 -24.43867 null null null null null null 0.3 null 0.3 0.2 null 0.6 null null 1.2 null null 0.9 null null 3.2 null null null null null null null null null null 17.2 72.8 6.9 5.8 null null 6.4 4687.8 193.4 U 4458.9 100.3 U 4149.7 105.1 U null 4.2 null Step 5--- Using completeness limits for one or more IRAC photometry 283718 247.45109 -24.41919 null null null null null null 0.1 null 0.1 0.1 null 0.1 null null 0.2 null null 0.2 null null 1.9 null null null null null null null null null null 19.6 null null 5.8 80.2 6.7 6.6 87.0 62.4 54.8 1568.4 94.1 U 1369.2 74.3 U 46.6 4.7 U Step 5--- Using completeness limits for one or more IRAC photometry 485318 245.70923 -23.777 null null null null null null 0.1 null null 0.1 null 0.1 null null 0.2 null null 0.5 null null 1.3 null null null null null null null null null null 15.9 69.3 6.1 5.0 null null 11.2 46.7 63.6 129.0 35.5 21.4 168.7 2516.2 46.3 U null null null Step 5--- Using completeness limits for one or more IRAC photometry 651853 245.77268 -23.04914 2.0 0.1 2.8 0.1 3.0 0.1 2.3 null 0.1 2.5 null 0.1 3.3 null 0.2 5.1 0.1 0.7 91.5 0.9 113.6 2.1 0.1 2.1 null 8.2 0.5 99.0 2.7 328.4 24.6 18.4 null null null null null 20.3 4657.8 171.6 U 3709.9 103.6 U 3005.2 77.9 U null null null Step 3--- [3.6]-[4.5] < 0.65, alpha_{4.5,24} > 0.3 666140 245.50667 -22.90364 null null null null null null 0.2 null 0.1 0.1 null 0.1 null null 0.2 0.3 null 0.3 1.9 0.2 1.2 0.3 null 0.2 null 2.2 0.5 4.4 1.6 null null 16.5 null null null 161.1 19.0 21.5 88.8 122.1 90.3 2275.7 87.2 U 1917.5 77.8 U null null null Step 3--- [3.6]-[4.5] < 0.65, alpha_{4.5,24} > 0.3 696986 247.88064 -24.44131 5.2 0.2 6.7 0.2 5.5 0.1 3.1 null 0.4 2.3 null 0.3 2.0 null 0.3 2.1 0.1 0.7 44.5 0.6 84.5 null null null null null null null null 528.1 33.8 21.0 null null 6.5 671.8 38.0 12.6 824.8 794.6 77.6 501.3 268.0 117.6 258.1 262.2 92.2 110.3 5.7 -1.9 Step 3--- [3.6]-[4.5] < 0.65, alpha_{4.5,24} > 0.3 697461 247.8909 -24.07984 16.3 0.4 39.0 0.9 59.3 1.1 52.8 0.5 2.1 51.6 0.5 2.1 66.5 0.6 4.9 126.5 1.2 19.4 750.4 7.0 1227.0 118.2 2.5 160.9 3.0 324.1 4.5 735.8 17.6 null null 22.0 null null 6.4 628.2 33.6 10.8 4083.1 302.1 U 4437.8 247.6 U 4253.5 229.3 U 69.9 4.1 U Step 3--- [3.6]-[4.5] < 0.65, alpha_{4.5,24} > 0.3