\ 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|   long|   long|  long|    long|  long|    long|   long|     long|   long|     long|     long|   long|     long|     long|   long|     long|     long|   long|     long|     long|   long|     long|     long|   long|     long|   long|     long|   long|     long|   long|     long|   long|     long|     long|   long|     long|     long|   long|     long|     long|    long|      long|      long|    long|      long|      long|    long|      long|      long|   long|     long|     long|    long|
|     |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|