GSC6412-408

Summary

GSC6412-408 is a star^[1].

Key Facts

• GSC6412-408's instance of is recorded as star^[2].
• GSC6412-408's instance of is recorded as infrared source^[3].
• GSC6412-408's constellation is recorded as Cetus^[4].
• GSC6412-408's spectral class is recorded as F0p^[5].
• GSC6412-408's catalog code is recorded as GSC 06412-00408^[6].
• GSC6412-408's catalog code is recorded as HIP 85^[7].
• GSC6412-408's catalog code is recorded as 2MASS J00010147-2442505^[8].
• GSC6412-408's catalog code is recorded as CD-25 16747^[9].
• GSC6412-408's catalog code is recorded as CPD-25 7607^[10].
• GSC6412-408's catalog code is recorded as GCRV 20390^[11].
• GSC6412-408's catalog code is recorded as HIC 85^[12].
• GSC6412-408's catalog code is recorded as PPM 242413^[13].
• GSC6412-408's catalog code is recorded as TYC 6412-408-1^[14].
• GSC6412-408's catalog code is recorded as UBV 20623^[15].
• GSC6412-408's catalog code is recorded as UBV M 5673^[16].
• GSC6412-408's catalog code is recorded as uvby98 -002516747^[17].
• GSC6412-408's catalog code is recorded as YZ 114 15948^[18].
• GSC6412-408's catalog code is recorded as Gaia DR1 2336600713129372416^[19].
• GSC6412-408's catalog code is recorded as Gaia DR2 2336600717425196544^[20].
• GSC6412-408's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.5035'}^[21].
• GSC6412-408's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.884'}^[22].
• GSC6412-408's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.697'}^[23].
• GSC6412-408's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.643'}^[24].
• GSC6412-408's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.91'}^[25].
• GSC6412-408's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.56'}^[26].

Body

Designation and Status

Recorded instance of include star^[2] and infrared source^[3].

History and Context

Catalog codes include GSC 06412-00408^[6], HIP 85^[7], 2MASS J00010147-2442505^[8], CD-25 16747^[9], CPD-25 7607^[10], and GCRV 20390^[11].