\ 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 and the rebinned IRS fluxes for protostars in CrA \ eHOPS_ID \ ___ eHOPS ID of the protostar \ 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 \ ___ if , flux density is used as an upper limit \ s_*_flux \ ___ sky limit \ ___ if , 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) \ Rebinned IRS fluxes at wavelengths (in microns): \ I0540 (5.4), I0645 (6.45), I0750 (7.5), I0810 (8.1), I0860 (8.6), I0920 (9.2), I0980 (9.8), I1050 (10.5), \ I1250 (12.5), I1400 (14.0), I1650 (16.5), I1900 (19.0), I2300 (23.0), I2700 (27.0), I3100 (31.0), I3500 (35.0) \ Comments: Reason for the protostar identification (see section 4 in Pokhrel et al. 2023) \fixlen = T | eHOPS_ID| 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|I0540_flux|e_I0540_flux|I0645_flux|e_I0645_flux|I0750_flux|e_I0750_flux|I0810_flux|e_I0810_flux|I0860_flux|e_I0860_flux|I0920_flux|e_I0920_flux|I0980_flux|e_I0980_flux|I1050_flux|e_I1050_flux|I1250_flux|e_I1250_flux|I1400_flux|e_I1400_flux|I1650_flux|e_I1650_flux|I1900_flux|e_I1900_flux|I2300_flux|e_I2300_flux|I2700_flux|e_I2700_flux|I3100_flux|e_I3100_flux|I3500_flux|e_I3500_flux| Comments| | char| 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| 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| | | 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| 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| 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| eHOPS-cra-1 284.46925 -37.24452 null null null null null null 2.0 null 1.0 8.7 0.1 1.0 35.0 0.5 1.7 86.8 1.1 12.3 169.7 1.7 248.6 1.8 null 9.2 0.2 58.4 1.0 158.0 3.6 2380.0 131.9 56.8 null null null 1195.6 63.7 25.5 434.4 16.0 19.8 237.4 15.5 26.4 65.4 17.9 U 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 Step 3--- [3.6]-[4.5] > 0.65, alpha_{4.5,24} > -0.3 eHOPS-cra-2 285.42328 -36.975386 5.3 0.1 124.3 2.9 924.7 19.6 2175.3 29.6 166.8 3107.4 41.8 167.9 6364.0 83.2 298.5 7245.0 123.5 747.7 null null null 2766.4 451.0 10582.7 1832.5 19949.4 845.2 39809.6 110.0 70319.0 3833.2 1518.4 70914.8 3555.8 91.8 52268.3 2650.2 101.1 23442.1 1113.0 412.8 15280.8 1369.7 561.5 11625.3 1300.7 357.0 1675.8 22.7 1.7 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 Step 3--- [3.6]-[4.5] > 0.65, alpha_{4.5,24} > -0.3 eHOPS-cra-3 285.45023 -36.956182 null null 3.4 0.4 58.2 2.1 384.9 5.2 31.8 757.4 10.1 59.8 1278.4 16.8 222.5 1668.1 22.0 458.0 4851.4 59.0 1944.7 279.7 6.2 1125.6 27.0 2153.4 31.7 9212.7 152.7 27608.1 1423.5 348.8 21336.1 1067.6 20.5 null null 38.4 41022.5 5141.6 U 56321.6 136.4 U 43059.9 117.0 U 803.6 64.8 U 1180.9 32.9 1335.1 118.6 1617.4 99.5 1706.5 16.9 1369.6 25.0 962.8 23.0 934.1 61.9 1419.1 24.0 2361.4 50.5 3003.0 214.1 null null null null 8727.1 59.1 10902.5 70.7 12100.4 75.7 12916.6 120.5 Step 1--- [3.6]-[4.5] > 0.65, alpha_{4.5,24} > 0.3, IRS: Rising or Absorption eHOPS-cra-4 285.4521 -36.954322 null null 1.3 0.4 6.2 0.9 11.2 0.5 31.8 29.5 1.0 59.8 52.5 1.3 48.8 80.7 3.4 458.0 null null null null null null null null null null null null null 276.4 23770.7 1189.1 18.1 31834.7 1596.7 38.0 36975.7 4325.8 U 42368.2 5302.0 U 44133.3 4090.6 U 821.2 47.2 U 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 Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry eHOPS-cra-5 285.4606 -36.943586 null null null null null null 106.7 1.4 16.6 136.4 1.8 37.4 172.0 2.4 26.3 188.0 2.5 96.7 369.9 38.1 814.8 133.6 2.7 189.9 3.1 397.3 5.1 1104.6 40.7 8952.5 453.2 68.5 12557.8 628.1 8.1 11144.2 560.7 21.1 7277.9 3545.8 1332.2 38246.1 54.6 U 34634.0 75.3 U 981.8 43.6 U 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 Step 3--- [3.6]-[4.5] > 0.65, -0.5 < alpha_{4.5,24} < -0.3 eHOPS-cra-6 285.46126 -36.969444 0.7 0.1 34.6 0.9 556.2 21.5 3122.6 42.8 270.3 5279.1 72.6 498.2 null null 2888.7 null null 4839.9 null null null 3640.1 248.1 25386.2 8651.5 31183.9 5399.8 null null 107118.0 5747.3 2084.4 89274.2 4470.6 119.5 62165.1 3126.8 104.6 61428.4 233.7 U 53519.9 203.7 U 49788.4 230.0 U 1929.9 100.3 4.2 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 Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry eHOPS-cra-7 285.48072 -36.95613 null null null null null null 58.4 2.9 41.8 209.6 4.0 124.9 580.9 10.9 4322.1 976.7 23.0 687.9 null null null null null null null null null 90696.0 250.6 268319.0 13681.5 2674.9 161579.0 8085.7 140.6 202590.0 10144.4 179.1 261768.0 3957.6 U 154967.0 524.0 U 98240.3 356.9 U 3489.3 110.5 U 616.4 14.4 905.2 15.0 1671.0 30.4 1225.1 18.6 615.3 10.2 297.0 13.9 310.1 33.7 692.9 9.7 3529.3 161.1 null null null null null null null null null null null null null null Step 1--- [3.6]-[4.5] > 0.65, alpha_{4.5,24} > 0.3, IRS: Rising or Absorption eHOPS-cra-8 285.4851 -36.957954 null null null null null null 35.1 1.3 9.8 225.8 3.8 124.9 676.4 9.9 144.8 916.4 14.6 687.9 null null null null null null null null null null null 148388.0 7593.2 1711.3 102002.0 5104.1 91.4 115085.0 5789.8 183.2 217769.0 599.9 U 148899.0 581.2 U 122466.0 1864.9 U 5461.4 44.5 U 517.5 36.4 656.9 21.2 1046.6 90.0 806.1 54.3 299.9 7.8 81.8 9.6 null null 176.9 16.3 947.4 14.4 null null null null null null null null null null null null null null Step 4--- From alpha_{3.6,4.5} versus alpha_{5.8,8.0} plot eHOPS-cra-9 285.49418 -36.95242 null null null null null null 23.0 0.4 2.9 67.5 0.9 5.5 150.1 3.8 10.0 193.9 2.7 33.2 710.4 40.9 null 24.7 0.6 77.3 1.4 302.2 4.2 2218.1 47.0 12046.9 619.8 145.7 14714.0 736.5 15.4 31600.9 1586.2 42.0 39481.3 2709.7 990.3 51213.9 278.3 U 47874.3 226.7 U 1594.0 67.5 15.1 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 Step 3--- [3.6]-[4.5] > 0.65, alpha_{4.5,24} > -0.3 eHOPS-cra-10 285.74464 -37.126793 0.1 null 0.5 null 1.1 0.1 7.5 0.2 2.0 17.4 0.3 1.9 17.9 0.3 3.0 12.9 0.2 1.8 2414.5 22.7 488.5 6.6 0.1 28.9 0.5 47.6 0.7 2120.3 39.1 42596.8 2262.5 754.6 47689.8 2391.9 187.0 41512.6 2100.0 218.2 28623.6 596.7 249.0 19628.8 546.7 323.8 11705.0 419.2 248.2 957.5 22.2 4.1 31.2 1.5 17.1 1.9 20.1 1.9 16.1 1.0 5.9 0.7 null null 2.6 0.4 6.8 1.1 36.9 3.3 null null null null null null 2011.5 45.0 4775.3 26.5 7884.8 55.6 10931.9 55.9 Step 1--- [3.6]-[4.5] > 0.65, alpha_{4.5,24} > 0.3, IRS: Rising or Absorption eHOPS-cra-11 285.77898 -37.213852 182.0 4.6 732.3 25.6 2125.8 36.0 null null 260.1 null null 637.6 null null 3085.1 null null 5395.9 null null null 5489.3 1147.7 34913.9 null 31327.8 5078.5 48751.5 89.8 101662.0 5422.1 1877.8 74253.2 3719.1 218.4 51022.9 2574.5 179.6 26205.7 533.4 193.5 12254.7 295.6 254.7 5347.4 289.8 225.4 1109.1 13.5 0.9 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 Step 5--- Using completeness limits for one or more Spitzer or Herschel/PACS photometry