This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 9.54 10:39:58.06 -29:17:11.4
271.33223 25.39924 galactic Hya Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5455633043256165760 | 10:39:56.14 -29:17:46.6 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE SpType: A3V 1982MSS...C03....0H HD 92442
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:39:58.06 -29:17:11.4: 12.94 +/- 0.04 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:39:58.06 -29:17:11.4: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5455633043256165760,2461152.6431,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5455633043256165760 20260422.1431 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 9.73 10:52:50.43 -22:37:01.9
270.11326 32.58969 galactic Hya Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3549317993678159744 | 10:52:52.83 -22:36:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8/K1III: 1988MSS...C04....0H HD 94321
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:52:50.43 -22:37:01.9: 13.11 +/- 0.05 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:52:50.43 -22:37:01.9: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3549317993678159744,2461152.6431,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3549317993678159744 20260422.1431 9.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 9.80 10:39:43.70 -27:27:41.3
270.18776 26.90864 galactic Hya Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5468113908979890560 | 10:39:45.96 -27:27:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A9V 1982MSS...C03....0H HD 92417
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:39:43.70 -27:27:41.3: 12.58 +/- 0.03 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:39:43.70 -27:27:41.3: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5468113908979890560,2461152.6431,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5468113908979890560 20260422.1431 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.11 10:42:40.39 -28:05:17.1
271.18046 26.72953 galactic Hya Second-epoch detections are separated by 3.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5456012099889489024 | 10:42:39.94 -28:04:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:42:40.39 -28:05:17.1: 12.99 +/- 0.04 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:42:40.39 -28:05:17.1: 13.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5456012099889489024,2461152.6431,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5456012099889489024 20260422.1431 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.02 10:44:50.69 -24:23:13.7
269.39555 30.11645 galactic Hya Second-epoch detections are separated by 5.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J161.2136-24.3879 | 10:44:49.53 -24:23:24.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:44:50.69 -24:23:13.7: 13.34 +/- 0.05 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:44:50.69 -24:23:13.7: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J161.2136-24.3879,2461152.6431,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J161.2136-24.3879 20260422.1431 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.02 10:34:54.61 -22:16:48.5
265.83868 30.58432 galactic Hya Second-epoch detections are separated by 7.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5474818524727683840 | 10:34:54.34 -22:17:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:34:54.61 -22:16:48.5: 13.26 +/- 0.04 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:34:54.61 -22:16:48.5: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5474818524727683840,2461152.6431,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5474818524727683840 20260422.1431 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.97 10:46:19.53 -28:30:04.8
272.18989 26.79916 galactic Hya Second-epoch detections are separated by 8.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5455741138993168128 | 10:46:18.94 -28:29:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:46:19.53 -28:30:04.8: 13.38 +/- 0.05 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:46:19.53 -28:30:04.8: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5455741138993168128,2461152.6431,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5455741138993168128 20260422.1431 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.88 10:47:27.80 -27:30:45.0
271.85550 27.77515 galactic Hya Second-epoch detections are separated by 4.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5457359345229023488 | 10:47:26.46 -27:30:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:47:27.80 -27:30:45.0: 12.84 +/- 0.03 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:47:27.80 -27:30:45.0: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5457359345229023488,2461152.6431,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5457359345229023488 20260422.1431 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.11 10:23:35.76 -25:17:18.6
265.47596 26.62887 galactic Hya Second-epoch detections are separated by 7.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5472520785943821952 | 10:23:35.78 -25:16:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:23:35.76 -25:17:18.6: 14.23 +/- 0.11 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:23:35.76 -25:17:18.6: 13.93 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5472520785943821952,2461152.6431,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5472520785943821952 20260422.1431 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.99 10:21:50.96 -27:10:46.9
266.38109 24.87801 galactic Hya Second-epoch detections are separated by 8.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5468885147667381248 | 10:21:51.26 -27:10:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:21:50.96 -27:10:46.9: 12.99 +/- 0.04 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:21:50.96 -27:10:46.9: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5468885147667381248,2461152.6431,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5468885147667381248 20260422.1431 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.86 10:32:25.71 -28:43:57.2
269.47280 24.96086 galactic Hya Second-epoch detections are separated by 5.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5467543606042314880 | 10:32:24.20 -28:44:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:32:25.71 -28:43:57.2: 12.89 +/- 0.03 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:32:25.71 -28:43:57.2: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5467543606042314880,2461152.6431,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5467543606042314880 20260422.1431 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.71 10:27:34.53 -25:00:09.5
266.09892 27.39356 galactic Hya Second-epoch detections are separated by 6.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5472590639291739008 | 10:27:34.02 -24:59:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:27:34.53 -25:00:09.5: 13.04 +/- 0.04 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:27:34.53 -25:00:09.5: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5472590639291739008,2461152.6431,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5472590639291739008 20260422.1431 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.48 10:31:15.43 -25:02:00.5
266.88380 27.85509 galactic Hya Second-epoch detections are separated by 4.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469550691502527104 | 10:31:15.10 -25:01:41.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:31:15.43 -25:02:00.5: 12.54 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:31:15.43 -25:02:00.5: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469550691502527104,2461152.6431,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469550691502527104 20260422.1431 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.50 10:37:08.06 -25:36:47.8
268.49461 28.13252 galactic Hya Second-epoch detections are separated by 3.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5470032247532501760 | 10:37:07.49 -25:36:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:37:08.06 -25:36:47.8: 12.77 +/- 0.03 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:37:08.06 -25:36:47.8: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5470032247532501760,2461152.6431,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5470032247532501760 20260422.1431 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.85 10:30:17.35 -25:09:49.7
266.76723 27.62192 galactic Hya Second-epoch detections are separated by 6.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469589041267369984 | 10:30:17.65 -25:10:06.6 (Gaia DR3) | VAR (local) | A (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:30:17.35 -25:09:49.7: 11.83 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:30:17.35 -25:09:49.7: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469589041267369984,2461152.6431,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469589041267369984 20260422.1431 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.06 10:39:42.74 -27:27:37.2
270.18372 26.90767 galactic Hya Second-epoch detections are separated by 4.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5468113908979890560 | 10:39:45.96 -27:27:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A9V 1982MSS...C03....0H HD 92417
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:39:42.74 -27:27:37.2: 13.59 +/- 0.07 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:39:42.74 -27:27:37.2: 13.68 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5468113908979890560,2461152.6431,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5468113908979890560 20260422.1431 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.07 10:26:08.72 -29:08:40.8
268.48748 23.84087 galactic Hya Second-epoch detections are separated by 3.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5461664001973082368 | 10:26:10.19 -29:09:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:26:08.72 -29:08:40.8: 14.41 +/- 0.14 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:26:08.72 -29:08:40.8: 14.45 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5461664001973082368,2461152.6431,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5461664001973082368 20260422.1431 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.00 10:29:32.17 -21:51:58.8
264.38971 30.18563 galactic Hya Second-epoch detections are separated by 8.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5475819904942208256 | 10:29:31.21 -21:51:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:29:32.17 -21:51:58.8: 13.06 +/- 0.04 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:29:32.17 -21:51:58.8: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5475819904942208256,2461152.6431,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5475819904942208256 20260422.1431 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.84 10:33:06.00 -26:33:02.1
268.24407 26.84811 galactic Hya Second-epoch detections are separated by 5.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5468449500545187456 | 10:33:06.92 -26:33:26.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:33:06.00 -26:33:02.1: 13.58 +/- 0.06 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:33:06.00 -26:33:02.1: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5468449500545187456,2461152.6431,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5468449500545187456 20260422.1431 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.95 10:23:25.93 -23:41:35.6
264.36169 27.87993 galactic Hya Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5472983439820951936 | 10:23:26.13 -23:42:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:23:25.93 -23:41:35.6: 14.57 +/- 0.14 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:23:25.93 -23:41:35.6: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5472983439820951936,2461152.6431,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5472983439820951936 20260422.1431 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.92 10:30:01.25 -24:12:53.7
266.08495 28.35754 galactic Hya Second-epoch detections are separated by 3.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 5474152255041075584 | 10:30:01.60 -24:13:20.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:30:01.25 -24:12:53.7: 14.06 +/- 0.09 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:30:01.25 -24:12:53.7: 14.25 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5474152255041075584,2461152.6431,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 5474152255041075584 20260422.1431 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.04 10:47:00.98 -27:07:10.9
271.52855 28.05921 galactic Hya Second-epoch detections are separated by 3.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASAS J104701-2706.7 | 10:47:00.99 -27:06:39.8 (Gaia DR3) | MISC (local) | 2451964.30000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:47:00.98 -27:07:10.9: 14.86 +/- 0.21 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:47:00.98 -27:07:10.9: 14.71 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J104701-2706.7,2461152.6431,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J104701-2706.7 20260422.1431 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.98 10:46:13.17 -24:47:57.3
269.95556 29.93646 galactic Hya Second-epoch detections are separated by 4.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5470322415522994944 | 10:46:14.65 -24:48:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:46:13.17 -24:47:57.3: 13.33 +/- 0.05 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:46:13.17 -24:47:57.3: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5470322415522994944,2461152.6431,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5470322415522994944 20260422.1431 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.89 10:37:58.53 -22:29:39.6
266.65613 30.81653 galactic Hya Second-epoch detections are separated by 3.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5474834983042499840 | 10:37:57.89 -22:29:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:37:58.53 -22:29:39.6: 15.03 +/- 0.22 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:37:58.53 -22:29:39.6: 15.03 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5474834983042499840,2461152.6431,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5474834983042499840 20260422.1431 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.24 10:20:19.90 -24:50:25.6
264.51454 26.53943 galactic Hya Second-epoch detections are separated by 3.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5472790166292593664 | 10:20:18.48 -24:50:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:20:19.90 -24:50:25.6: 14.16 +/- 0.10 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:20:19.90 -24:50:25.6: 14.05 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5472790166292593664,2461152.6431,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5472790166292593664 20260422.1431 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 10.97 10:46:12.29 -24:48:04.5
269.95355 29.93299 galactic Hya Second-epoch detections are separated by 2.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5470322415522994944 | 10:46:14.65 -24:48:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:46:12.29 -24:48:04.5: 14.47 +/- 0.14 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:46:12.29 -24:48:04.5: 14.62 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5470322415522994944,2461152.6431,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5470322415522994944 20260422.1431 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.03 10:50:33.10 -26:44:00.1
272.06932 28.79681 galactic Hya Second-epoch detections are separated by 6.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5457888313403402112 | 10:50:33.44 -26:43:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:50:33.10 -26:44:00.1: 13.66 +/- 0.07 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:50:33.10 -26:44:00.1: 13.65 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5457888313403402112,2461152.6431,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5457888313403402112 20260422.1431 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.41 10:24:36.06 -25:24:58.4
265.76507 26.66194 galactic Hya Second-epoch detections are separated by 3.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J156.1526-25.4083 | 10:24:34.93 -25:24:36.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:24:36.06 -25:24:58.4: 13.75 +/- 0.07 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:24:36.06 -25:24:58.4: 13.94 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J156.1526-25.4083,2461152.6431,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J156.1526-25.4083 20260422.1431 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.46 10:20:17.73 -22:06:19.6
262.60735 28.69003 galactic Hya Second-epoch detections are separated by 8.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5475610551056312832 | 10:20:16.72 -22:05:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:20:17.73 -22:06:19.6: 13.56 +/- 0.06 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:20:17.73 -22:06:19.6: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5475610551056312832,2461152.6431,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5475610551056312832 20260422.1431 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.33 10:47:56.64 -29:40:07.7
273.19715 25.97825 galactic Hya Second-epoch detections are separated by 2.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5454855757254915840 | 10:47:57.95 -29:40:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:47:56.64 -29:40:07.7: 14.16 +/- 0.12 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:47:56.64 -29:40:07.7: 14.40 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5454855757254915840,2461152.6431,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5454855757254915840 20260422.1431 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.38 10:42:41.86 -27:05:31.7
270.58922 27.57521 galactic Hya Second-epoch detections are separated by 8.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5457621681833113344 | 10:42:39.20 -27:05:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:42:41.86 -27:05:31.7: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:42:41.86 -27:05:31.7: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5457621681833113344,2461152.6431,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5457621681833113344 20260422.1431 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.46 10:34:53.30 -30:04:14.0
270.77751 24.14298 galactic Ant Second-epoch detections are separated by 4.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5455312157660471552 | 10:34:56.55 -30:04:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:34:53.30 -30:04:14.0: 14.15 +/- 0.12 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:34:53.30 -30:04:14.0: 14.13 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 22.1431* 10 34 53.30 -30 04 14.0 11.5 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5455312157660471552,2461152.6431,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5455312157660471552 20260422.1431 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.25 10:46:12.50 -24:47:41.6
269.95041 29.93880 galactic Hya Second-epoch detections are separated by 2.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5470322415522994944 | 10:46:14.65 -24:48:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:46:12.50 -24:47:41.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:46:12.50 -24:47:41.6: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5470322415522994944,2461152.6431,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5470322415522994944 20260422.1431 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.18 10:53:12.58 -29:31:23.4
274.22221 26.67639 galactic Hya Second-epoch detections are separated by 8.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5456128201445829760 | 10:53:14.31 -29:31:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:53:12.58 -29:31:23.4: 13.78 +/- 0.09 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:53:12.58 -29:31:23.4: 13.73 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5456128201445829760,2461152.6431,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5456128201445829760 20260422.1431 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.36 10:36:02.65 -26:26:09.8
268.78370 27.31310 galactic Hya Second-epoch detections are separated by 6.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5468463759836254080 | 10:36:03.15 -26:26:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:36:02.65 -26:26:09.8: 13.42 +/- 0.05 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:36:02.65 -26:26:09.8: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5468463759836254080,2461152.6431,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5468463759836254080 20260422.1431 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.34 10:36:19.50 -25:54:28.5
268.50989 27.78635 galactic Hya Second-epoch detections are separated by 5.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469997887794113920 | 10:36:18.17 -25:54:44.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:36:19.50 -25:54:28.5: 13.51 +/- 0.06 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:36:19.50 -25:54:28.5: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469997887794113920,2461152.6431,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469997887794113920 20260422.1431 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.54 10:48:28.59 -28:37:37.2
272.71646 26.93411 galactic Hya Second-epoch detections are separated by 6.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5456477399466238080 | 10:48:26.51 -28:37:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:48:28.59 -28:37:37.2: 14.96 +/- 0.24 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:48:28.59 -28:37:37.2: 15.40 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.96 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5456477399466238080,2461152.6431,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5456477399466238080 20260422.1431 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.69 10:33:54.29 -29:19:28.5
270.13104 24.64842 galactic Hya Second-epoch detections are separated by 2.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5455497872045709696 | 10:33:54.20 -29:20:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:33:54.29 -29:19:28.5: 15.01 +/- 0.25 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:33:54.29 -29:19:28.5: 14.79 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5455497872045709696,2461152.6431,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5455497872045709696 20260422.1431 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.61 10:24:43.73 -26:15:56.7
266.35332 25.99519 galactic Hya Second-epoch detections are separated by 6.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469038460820018048 | 10:24:42.09 -26:16:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:24:43.73 -26:15:56.7: 13.49 +/- 0.06 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:24:43.73 -26:15:56.7: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469038460820018048,2461152.6431,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469038460820018048 20260422.1431 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.60 10:45:22.63 -27:38:08.2
271.48263 27.42918 galactic Hya Second-epoch detections are separated by 7.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5457342337160572288 | 10:45:24.83 -27:38:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:45:22.63 -27:38:08.2: 14.08 +/- 0.10 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:45:22.63 -27:38:08.2: 13.89 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5457342337160572288,2461152.6431,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5457342337160572288 20260422.1431 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.61 10:46:00.76 -26:53:05.8
271.17334 28.14233 galactic Hya Second-epoch detections are separated by 5.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5457683598081245952 | 10:46:01.56 -26:53:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:46:00.76 -26:53:05.8: 15.44 +/- 0.34 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:46:00.76 -26:53:05.8: 15.39 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.41 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5457683598081245952,2461152.6431,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5457683598081245952 20260422.1431 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.81 10:29:47.11 -25:52:00.5
267.12139 26.98310 galactic Hya Second-epoch detections are separated by 2.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469482216840811264 | 10:29:48.01 -25:52:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:29:47.11 -25:52:00.5: 14.70 +/- 0.17 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:29:47.11 -25:52:00.5: 14.46 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469482216840811264,2461152.6431,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469482216840811264 20260422.1431 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.84 10:31:13.82 -26:40:39.2
267.94020 26.50601 galactic Hya Second-epoch detections are separated by 7.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469101888897170304 | 10:31:16.64 -26:41:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:31:13.82 -26:40:39.2: 15.30 +/- 0.27 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:31:13.82 -26:40:39.2: 15.41 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.34 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469101888897170304,2461152.6431,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469101888897170304 20260422.1431 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.72 10:32:46.38 -23:55:03.1
266.47000 28.96497 galactic Hya Second-epoch detections are separated by 6.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5474266501171058560 | 10:32:48.07 -23:54:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:32:46.38 -23:55:03.1: 14.29 +/- 0.11 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:32:46.38 -23:55:03.1: 14.45 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5474266501171058560,2461152.6431,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5474266501171058560 20260422.1431 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 11.90 10:39:01.73 -22:45:48.9
267.06692 30.73287 galactic Hya Second-epoch detections are separated by 8.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5471822076367652096 | 10:39:02.21 -22:45:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:39:01.73 -22:45:48.9: 14.94 +/- 0.21 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:39:01.73 -22:45:48.9: 15.00 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5471822076367652096,2461152.6431,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5471822076367652096 20260422.1431 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.12 10:23:47.81 -27:15:24.8
266.81619 25.07258 galactic Hya Second-epoch detections are separated by 6.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5468825086844864896 | 10:23:47.30 -27:15:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:23:47.81 -27:15:24.8: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:23:47.81 -27:15:24.8: 15.24 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5468825086844864896,2461152.6431,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5468825086844864896 20260422.1431 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.13 10:35:02.35 -25:40:49.1
268.09466 27.81208 galactic Hya Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5470766274623495296 | 10:35:01.10 -25:40:29.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:35:02.35 -25:40:49.1: 14.04 +/- 0.09 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:35:02.35 -25:40:49.1: 14.16 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5470766274623495296,2461152.6431,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5470766274623495296 20260422.1431 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.21 10:36:22.64 -25:33:52.9
268.30341 28.07732 galactic Hya Second-epoch detections are separated by 3.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5470763457124706048 | 10:36:21.01 -25:33:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:36:22.64 -25:33:52.9: 14.46 +/- 0.13 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:36:22.64 -25:33:52.9: 14.61 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5470763457124706048,2461152.6431,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5470763457124706048 20260422.1431 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1431 2461152.6431 12.21 10:36:20.26 -26:02:36.0
268.59808 27.67566 galactic Hya Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5469991703041199232 | 10:36:19.87 -26:02:08.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:36:20.26 -26:02:36.0: 14.89 +/- 0.20 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:36:20.26 -26:02:36.0: 14.61 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5469991703041199232,2461152.6431,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5469991703041199232 20260422.1431 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5474102570858580096,2461152.6431,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5474102570858580096 20260422.1431 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5474633394457737216,2461152.6431,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5474633394457737216 20260422.1431 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5473158979427957888,2461152.6431,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5473158979427957888 20260422.1431 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461152.64340006 22.04.2026 03:26:19.765 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7374
Objects passed selection criteria: 7332
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 4371.5
Average stars matched: 4180 (95.6194 %)
Memory usage VmPeak: 113360 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 21 22:32:59 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461152.64340006 22.04.2026 03:26:19.765 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 191
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 42654
Objects passed selection criteria: 42545
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 25673
Average stars matched: 24017.8 (93.5526 %)
Memory usage VmPeak: 145812 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 21 22:35:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461152.64285059
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits'
wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits exists and is non-empty
Saving wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits to local_wcs_cache/
'wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits (1st reference image)
verification OK: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Image size: 941.2'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:33:35.280 -26:00:04.03 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits (1st new image)
verification OK: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Image size: 938.0'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:33:36.057 -26:00:00.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:36.057 -26:00:00.10
Angular distance between the image centers 0.0031 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits (2nd new image)
verification OK: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Image size: 938.0'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:33:36.744 -25:59:23.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:36.744 -25:59:23.35
Angular distance between the image centers 0.0126 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:33:36.057 -26:00:00.10
Second-epoch second image center 10:33:36.744 -25:59:23.35
Angular distance between the image centers 0.01053 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.qyGuzpVDgB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.6OE52JlVvS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits &> /tmp/tmp.guyjP3yj3b
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits &> /tmp/tmp.tiIRqwKjdf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat' -> 'wcsmag.cat'
Read 9188 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1995 to 167.3695 deg, Dec -31.3041 to -20.4278 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 149.1995 to 167.3695 deg, Dec -31.3041 to -20.4278 deg
Loaded 8646 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6476 out of 6648 total matches.
Matched with Tycho-2 6648 out of 9188 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.827572
a=0.000000 b=1.000000 c=22.827572
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.74
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.74
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9188 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1995 to 167.3695 deg, Dec -31.3041 to -20.4278 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 149.1995 to 167.3695 deg, Dec -31.3041 to -20.4278 deg
Loaded 8646 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6476 out of 6648 total matches.
Matched with Tycho-2 6648 out of 9188 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits -> calib.txt_param_ref_wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits (aperture=6.1)
Read 9186 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1992 to 167.3696 deg, Dec -31.3041 to -20.4319 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 149.1992 to 167.3696 deg, Dec -31.3041 to -20.4319 deg
Loaded 8646 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6464 out of 6641 total matches.
Matched with Tycho-2 6641 out of 9186 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
2.3 pix Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
9.4 pix fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
9.1 pix fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
2.3 pix wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
2.3 pix wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
14.7 mag. Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
14.8 mag. Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
12.5 mag. fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
12.5 mag. fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 10.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qyGuzpVDgB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=502, passed=9188
Got 9188 stars (including 8670 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 9188 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6OE52JlVvS (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, passed=9186
Got 9186 stars (including 8663 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 9186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.guyjP3yj3b (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=201, passed=2130
Got 2130 stars (including 1929 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 2130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 2111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.09"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.82"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.51"
Excluding outliers - 958 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tiIRqwKjdf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=219, passed=2192
Got 2192 stars (including 1973 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 2192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 2168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.06"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 2168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.80"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 2168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.51"
Excluding outliers - 959 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits'
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits'
Preparing the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20575.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20350_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 20350_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:19:32.94 -22:20:42.2: 10.06 +/- 0.00 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:19:32.94 -22:20:42.2: 10.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.06 +/- 0.00
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Considering the candidate 20351_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 20351_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:28:35.32 -22:48:14.7: 9.82 +/- 0.00 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:28:35.32 -22:48:14.7: 9.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.80 +/- 0.00
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Considering the candidate 20534_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 20534_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 20564_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 20564_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20575_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 20575_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 03583_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 03583_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:37:13.36 -27:24:39.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06739_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 06739_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:34:00.66 -23:44:47.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 21s
Prepared the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:39:58.06 -29:17:11.4
10:52:50.43 -22:37:01.9
10:39:43.70 -27:27:41.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits exists and is non-empty
wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits (1st reference image)
verification OK: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Image size: 941.2'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:33:35.280 -26:00:04.03 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits (1st new image)
verification OK: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Image size: 938.0'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:33:36.057 -26:00:00.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:36.057 -26:00:00.10
Angular distance between the image centers 0.0031 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits (2nd new image)
verification OK: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Image size: 938.0'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:33:36.744 -25:59:23.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:36.744 -25:59:23.35
Angular distance between the image centers 0.0126 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:33:36.057 -26:00:00.10
Second-epoch second image center 10:33:36.744 -25:59:23.35
Angular distance between the image centers 0.01053 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.pxU41iSAy2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.zVFP6Ftqlb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits &> /tmp/tmp.kyjVJbikDv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits &> /tmp/tmp.dV6An7oCtH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat' -> 'wcsmag.cat'
Read 52516 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1799 to 167.4334 deg, Dec -31.3047 to -20.4069 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 149.1799 to 167.4334 deg, Dec -31.3047 to -20.4069 deg
Loaded 8722 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6662 out of 7301 total matches.
Matched with Tycho-2 7301 out of 52516 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.700451
a=0.000000 b=1.000000 c=22.700451
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.85
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.85
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 52516 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1799 to 167.4334 deg, Dec -31.3047 to -20.4069 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 149.1799 to 167.4334 deg, Dec -31.3047 to -20.4069 deg
Loaded 8722 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6662 out of 7301 total matches.
Matched with Tycho-2 7301 out of 52516 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits -> calib.txt_param_ref_wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits (aperture=5.0)
Read 53237 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1798 to 167.4499 deg, Dec -31.3078 to -20.4068 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 149.1798 to 167.4499 deg, Dec -31.3078 to -20.4068 deg
Loaded 8731 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6679 out of 7298 total matches.
Matched with Tycho-2 7298 out of 53237 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 169 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
2.4 pix Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
7.4 pix fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
7.0 pix fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
2.4 pix wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
2.4 pix wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
14.8 mag. Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
14.9 mag. Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
12.9 mag. fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
13.0 mag. fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pxU41iSAy2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2425, passed=52512
Got 52512 stars (including 49995 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 52512 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 51223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 51223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 51224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zVFP6Ftqlb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=2429, passed=53236
Got 53236 stars (including 50714 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 53236 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 51985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 51984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 51983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kyjVJbikDv (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2936, passed=10689
Got 10689 stars (including 7753 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 10689 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 10580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.99"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 10578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.92"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 10578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.41"
Excluding outliers - 962 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dV6An7oCtH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=3157, passed=11075
Got 11075 stars (including 7916 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 11075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 10944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.96"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 10943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.91"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 10943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.35"
Excluding outliers - 963 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-25-32_20.00sec_-5.00C_LIGHT_0065.fits
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Hya-10-Q2b1x1_222707_TTUQ2b1x1_1963506_DsVw7QW7/wcs_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066.fits
Preparing the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out66312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out31598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68349.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 132s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 34s
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Considering the candidate 66250_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66250_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 66254_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66254_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:17:29.15 -23:32:10.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:17:29.15 -23:32:10.4: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
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Considering the candidate 66257_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66257_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66260_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66260_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66264_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66264_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:34:28.93 -29:29:14.8: 12.19 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:34:28.93 -29:29:14.8: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
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Considering the candidate 66266_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66266_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:18:55.92 -25:52:32.7: 12.88 +/- 0.03 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:18:55.92 -25:52:32.7: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
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Considering the candidate 66267_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66267_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66268_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66268_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 66270_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66270_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66273_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66273_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:23:30.78 -24:44:54.5: 12.09 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:23:30.78 -24:44:54.5: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
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Considering the candidate 66275_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66275_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:20:56.07 -28:40:34.8: 12.04 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:20:56.07 -28:40:34.8: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
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Considering the candidate 66280_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66280_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:31:39.92 -22:13:22.8: 12.14 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:31:39.92 -22:13:22.8: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
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Considering the candidate 66281_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66281_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 66298_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66298_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:26:11.29 -28:51:42.4: 12.22 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:26:11.29 -28:51:42.4: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
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Considering the candidate 66312_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66312_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:30:29.76 -27:28:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 4.079 5467926854564022528 157.62349608362 -27.47706998223 11.2500 10.7603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66313_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66313_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 66314_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66314_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66317_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66317_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:19:46.46 -21:54:50.9: 12.14 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:19:46.46 -21:54:50.9: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
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Considering the candidate 66319_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66319_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:38:52.51 -23:48:04.8: 12.17 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:38:52.51 -23:48:04.8: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
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Considering the candidate 66325_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66325_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 66326_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66326_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 66327_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66327_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:20:44.21 -26:02:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 2.832 5472094587747280768 155.18466238942 -26.04595027347 11.4415 11.0195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66329_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66329_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 66330_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66330_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:22:31.17 -24:11:14.4: 11.96 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:22:31.17 -24:11:14.4: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
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Considering the candidate 66331_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66331_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66334_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66334_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66341_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66341_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 66342_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66342_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:36:26.08 -28:55:01.5: 11.89 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:36:26.08 -28:55:01.5: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
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Considering the candidate 66344_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66344_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:31:46.00 -27:49:24.9: 12.01 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:31:46.00 -27:49:24.9: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
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Considering the candidate 66352_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66352_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 66353_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66353_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 66354_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66354_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 66360_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66360_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 66365_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66365_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:43:48.97 -28:20:07.7: 12.53 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:43:48.97 -28:20:07.7: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
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Considering the candidate 66366_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66366_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:35:06.15 -25:38:27.6: 11.90 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:35:06.15 -25:38:27.6: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
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Considering the candidate 66367_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66367_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:35:15.36 -25:40:55.0: 11.26 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:35:15.36 -25:40:55.0: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.00
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Considering the candidate 66370_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66370_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:50:27.43 -21:43:44.8: 11.72 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:50:27.43 -21:43:44.8: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
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Considering the candidate 66371_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66371_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:28:34.88 -27:30:03.0: 11.89 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:28:34.88 -27:30:03.0: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
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Considering the candidate 66375_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66375_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 66379_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66379_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:34:10.09 -24:34:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 1.630 5471091180309446016 158.54155060336 -24.56875819883 11.0711 10.4254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66381_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66381_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66382_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66382_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 66386_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66386_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:26:36.08 -23:49:36.3: 12.11 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:26:36.08 -23:49:36.3: 12.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
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Considering the candidate 66402_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66402_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:33:16.94 -24:19:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 5.344 5471148492352988928 158.32089725127 -24.32234899669 10.7090 9.9513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66403_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66403_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66406_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66406_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:24:25.88 -28:16:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 3.834 5468510523439906176 156.10662561474 -28.28075066627 11.1735 10.4777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66409_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66409_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 66410_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66410_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 66414_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66414_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:33:28.59 -25:21:55.1: 11.50 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:33:28.59 -25:21:55.1: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.01
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Considering the candidate 66424_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66424_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:35:04.85 -25:38:09.0: 11.26 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:35:04.85 -25:38:09.0: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
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Considering the candidate 66426_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66426_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 66427_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66427_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:33:27.92 -25:15:40.7: 11.35 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:33:27.92 -25:15:40.7: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.00
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Considering the candidate 66429_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66429_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:14:48.24 -29:51:37.0: 11.86 +/- 0.02 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:14:48.24 -29:51:37.0: 11.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
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Considering the candidate 66431_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66431_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:40:42.47 -25:29:21.3: 11.53 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:40:42.47 -25:29:21.3: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
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Considering the candidate 66437_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66437_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:33:59.81 -27:05:06.9: 11.18 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:33:59.81 -27:05:06.9: 11.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.00
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Considering the candidate 66439_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66439_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:28:52.37 -27:13:42.9: 12.03 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:28:52.37 -27:13:42.9: 12.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
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Considering the candidate 66442_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66442_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:24:06.61 -26:05:14.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)
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Considering the candidate 66444_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66444_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:33:30.75 -28:03:37.4: 11.45 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:33:30.75 -28:03:37.4: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
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Considering the candidate 66445_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66445_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 66447_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66447_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:18:19.33 -23:36:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.741 5473689665586689280 154.57956221681 -23.61145280034 11.0043 10.3050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66448_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66448_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 66449_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66449_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:37:08.25 -25:36:18.0: 11.52 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:37:08.25 -25:36:18.0: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
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Considering the candidate 66450_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66450_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:28:31.14 -27:06:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 1.621 5468703281572109056 157.12959166691 -27.11084441857 10.6330 9.8395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66452_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66452_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:30:57.93 -27:22:28.3: 11.34 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:30:57.93 -27:22:28.3: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.01
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Considering the candidate 66457_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66457_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:29:00.77 -25:00:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 2.352 5469608591958341632 157.25388123403 -25.01346021131 10.8971 10.1166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66458_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66458_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:24:34.63 -27:12:28.2: 11.47 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:24:34.63 -27:12:28.2: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
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Considering the candidate 66460_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66460_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:28:51.25 -29:23:11.8: 11.49 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:28:51.25 -29:23:11.8: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
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Considering the candidate 66462_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66462_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:28:36.09 -27:30:03.2: 11.58 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:28:36.09 -27:30:03.2: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
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Considering the candidate 66463_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66463_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:31:55.88 -25:39:09.9: 11.98 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:31:55.88 -25:39:09.9: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
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Considering the candidate 66464_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66464_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 66468_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66468_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 66473_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66473_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:25:36.22 -28:07:03.6: 11.96 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:25:36.22 -28:07:03.6: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
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Considering the candidate 66474_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66474_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 66476_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66476_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:25:20.58 -22:54:38.2: 11.07 +/- 0.01 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:25:20.58 -22:54:38.2: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.00
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Considering the candidate 66477_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66477_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66483_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66483_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66485_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66485_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 66489_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66489_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:39:21.99 -26:06:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 4.341 5469944114803754112 159.84244575197 -26.10453769313 10.9521 10.4505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66490_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66490_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 66497_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66497_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 66500_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66500_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 66502_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66502_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 66503_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66503_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits at 10:43:07.12 -26:15:30.3: 10.41 +/- 0.00 detection
Forced photometry on wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits at 10:43:07.12 -26:15:30.3: 10.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.00
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Considering the candidate 66704_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 66704_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:39:58.25 -29:17:09.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 66800_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 66800_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67129_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67129_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67132_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67132_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67135_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67135_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67137_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67137_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67161_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67161_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67173_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67173_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67184_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67184_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67188_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67188_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67227_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67227_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 67269_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67269_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 67288_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67288_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67302_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67302_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67333_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67333_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67419_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67419_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 67429_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67429_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67447_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67447_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 67459_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67459_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67479_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67479_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67500_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67500_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67521_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67521_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67527_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67527_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 67528_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67528_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67537_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67537_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 67578_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67578_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 67594_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67594_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67610_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67610_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67630_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67630_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 67644_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67644_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67648_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67648_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 67650_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67650_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67661_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67661_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 67663_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67663_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 67670_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67670_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 67675_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67675_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67708_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67708_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67726_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67726_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 67762_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67762_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 67767_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67767_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 67783_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67783_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 67801_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67801_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67817_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67817_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 67838_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67838_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67951_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 67951_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 67961_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 67961_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 68011_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68011_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68024_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68024_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68029_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68029_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 68068_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68068_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68076_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68076_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 68089_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68089_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 68111_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68111_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 68127_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68127_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 68171_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68171_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 68234_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68234_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 68240_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68240_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 68247_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68247_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 68256_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68256_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68263_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68263_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 68288_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68288_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 68294_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68294_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 68302_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68302_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 68323_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68323_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 68336_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68336_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68341_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68341_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68343_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68343_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 68349_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 68349_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 68363_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 68363_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 45531_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 45531_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:34:57.65 -23:10:32.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 48387_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 48387_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:34:00.69 -23:44:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29735_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 29735_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:21:21.51 -25:22:23.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 23375_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 23375_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:36:04.41 -26:40:32.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 24256_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 24256_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:30:51.30 -26:29:00.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41741_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 41741_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 42997_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 42997_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 31598_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
Preparing report for the candidate 31598_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
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Considering the candidate 18246_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 18246_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:36:42.62 -27:39:23.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 18850_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 18850_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:37:13.23 -27:24:41.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15203_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 15203_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:31:48.47 -28:14:13.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09960_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 09960_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:25:23.70 -29:11:36.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 48678_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 48678_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:21:28.55 -23:42:37.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06946_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 06946_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:29:28.92 -29:39:44.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 04952_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 04952_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:23:13.09 -30:09:44.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10623_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 10623_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:18:07.76 -28:59:27.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 49668_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066
The candidate 49668_fd_Hya-10-Q2b1x1_2026-04-21_22-26-19_20.00sec_-4.90C_LIGHT_0066 did not pass the final checks
**** FOUND 10:14:09.03 -23:48:50.5 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 170s
Prepared the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:39:58.06 -29:17:11.4
10:52:50.43 -22:37:01.9
10:39:43.70 -27:27:41.3
10:15:05.80 -25:02:43.4
10:19:33.73 -22:20:45.8
10:29:15.36 -22:39:19.2
10:42:40.39 -28:05:17.1
10:44:50.69 -24:23:13.7
10:34:54.61 -22:16:48.5
10:46:19.53 -28:30:04.8
10:47:27.80 -27:30:45.0
10:23:35.76 -25:17:18.6
10:21:50.96 -27:10:46.9
10:32:25.71 -28:43:57.2
10:27:34.53 -25:00:09.5
10:31:15.43 -25:02:00.5
10:37:08.06 -25:36:47.8
10:30:17.35 -25:09:49.7
10:39:42.74 -27:27:37.2
10:26:08.72 -29:08:40.8
10:29:32.17 -21:51:58.8
10:33:06.00 -26:33:02.1
10:23:25.93 -23:41:35.6
10:30:01.25 -24:12:53.7
10:47:00.98 -27:07:10.9
10:46:13.17 -24:47:57.3
10:37:58.53 -22:29:39.6
10:20:19.90 -24:50:25.6
10:46:12.29 -24:48:04.5
10:50:33.10 -26:44:00.1
10:24:36.06 -25:24:58.4
10:20:17.73 -22:06:19.6
10:47:56.64 -29:40:07.7
10:42:41.86 -27:05:31.7
10:34:53.30 -30:04:14.0
10:46:12.50 -24:47:41.6
10:53:12.58 -29:31:23.4
10:36:02.65 -26:26:09.8
10:36:19.50 -25:54:28.5
10:48:28.59 -28:37:37.2
10:33:54.29 -29:19:28.5
10:24:43.73 -26:15:56.7
10:45:22.63 -27:38:08.2
10:46:00.76 -26:53:05.8
10:29:47.11 -25:52:00.5
10:31:13.82 -26:40:39.2
10:32:46.38 -23:55:03.1
10:39:01.73 -22:45:48.9
10:23:47.81 -27:15:24.8
10:35:02.35 -25:40:49.1
10:36:22.64 -25:33:52.9
10:36:20.26 -26:02:36.0
########### Completed Hya-10-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
10:39:58.06 -29:17:11.4
10:52:50.43 -22:37:01.9
10:39:43.70 -27:27:41.3
10:42:40.39 -28:05:17.1
10:44:50.69 -24:23:13.7
10:34:54.61 -22:16:48.5
10:46:19.53 -28:30:04.8
10:47:27.80 -27:30:45.0
10:23:35.76 -25:17:18.6
10:21:50.96 -27:10:46.9
10:32:25.71 -28:43:57.2
10:27:34.53 -25:00:09.5
10:31:15.43 -25:02:00.5
10:37:08.06 -25:36:47.8
10:30:17.35 -25:09:49.7
10:39:42.74 -27:27:37.2
10:26:08.72 -29:08:40.8
10:29:32.17 -21:51:58.8
10:33:06.00 -26:33:02.1
10:23:25.93 -23:41:35.6
10:30:01.25 -24:12:53.7
10:47:00.98 -27:07:10.9
10:46:13.17 -24:47:57.3
10:37:58.53 -22:29:39.6
10:20:19.90 -24:50:25.6
10:46:12.29 -24:48:04.5
10:50:33.10 -26:44:00.1
10:24:36.06 -25:24:58.4
10:20:17.73 -22:06:19.6
10:47:56.64 -29:40:07.7
10:42:41.86 -27:05:31.7
10:34:53.30 -30:04:14.0
10:46:12.50 -24:47:41.6
10:53:12.58 -29:31:23.4
10:36:02.65 -26:26:09.8
10:36:19.50 -25:54:28.5
10:48:28.59 -28:37:37.2
10:33:54.29 -29:19:28.5
10:24:43.73 -26:15:56.7
10:45:22.63 -27:38:08.2
10:46:00.76 -26:53:05.8
10:29:47.11 -25:52:00.5
10:31:13.82 -26:40:39.2
10:32:46.38 -23:55:03.1
10:39:01.73 -22:45:48.9
10:23:47.81 -27:15:24.8
10:35:02.35 -25:40:49.1
10:36:22.64 -25:33:52.9
10:36:20.26 -26:02:36.0
10:19:33.73 -22:20:45.8
10:29:15.36 -22:39:19.2
10:15:05.80 -25:02:43.4
###################################################################################
10:39:58.06 -29:17:11.4 -- not an asteroid (will add it to exclusion list)
10:52:50.43 -22:37:01.9 -- not an asteroid (will add it to exclusion list)
10:39:43.70 -27:27:41.3 -- not an asteroid (will add it to exclusion list)
10:42:40.39 -28:05:17.1 -- not an asteroid (will add it to exclusion list)
10:44:50.69 -24:23:13.7 -- not an asteroid (will add it to exclusion list)
10:34:54.61 -22:16:48.5 -- not an asteroid (will add it to exclusion list)
10:46:19.53 -28:30:04.8 -- not an asteroid (will add it to exclusion list)
10:47:27.80 -27:30:45.0 -- not an asteroid (will add it to exclusion list)
10:23:35.76 -25:17:18.6 -- not an asteroid (will add it to exclusion list)
10:21:50.96 -27:10:46.9 -- not an asteroid (will add it to exclusion list)
10:32:25.71 -28:43:57.2 -- not an asteroid (will add it to exclusion list)
10:27:34.53 -25:00:09.5 -- not an asteroid (will add it to exclusion list)
10:31:15.43 -25:02:00.5 -- not an asteroid (will add it to exclusion list)
10:37:08.06 -25:36:47.8 -- not an asteroid (will add it to exclusion list)
10:30:17.35 -25:09:49.7 -- not an asteroid (will add it to exclusion list)
10:39:42.74 -27:27:37.2 -- not an asteroid (will add it to exclusion list)
10:26:08.72 -29:08:40.8 -- not an asteroid (will add it to exclusion list)
10:29:32.17 -21:51:58.8 -- not an asteroid (will add it to exclusion list)
10:33:06.00 -26:33:02.1 -- not an asteroid (will add it to exclusion list)
10:23:25.93 -23:41:35.6 -- not an asteroid (will add it to exclusion list)
10:30:01.25 -24:12:53.7 -- not an asteroid (will add it to exclusion list)
10:47:00.98 -27:07:10.9 -- not an asteroid (will add it to exclusion list)
10:46:13.17 -24:47:57.3 -- not an asteroid (will add it to exclusion list)
10:37:58.53 -22:29:39.6 -- not an asteroid (will add it to exclusion list)
10:20:19.90 -24:50:25.6 -- not an asteroid (will add it to exclusion list)
10:46:12.29 -24:48:04.5 -- not an asteroid (will add it to exclusion list)
10:50:33.10 -26:44:00.1 -- not an asteroid (will add it to exclusion list)
10:24:36.06 -25:24:58.4 -- not an asteroid (will add it to exclusion list)
10:20:17.73 -22:06:19.6 -- not an asteroid (will add it to exclusion list)
10:47:56.64 -29:40:07.7 -- not an asteroid (will add it to exclusion list)
10:42:41.86 -27:05:31.7 -- not an asteroid (will add it to exclusion list)
10:34:53.30 -30:04:14.0 -- not an asteroid (will add it to exclusion list)
10:46:12.50 -24:47:41.6 -- not an asteroid (will add it to exclusion list)
10:53:12.58 -29:31:23.4 -- not an asteroid (will add it to exclusion list)
10:36:02.65 -26:26:09.8 -- not an asteroid (will add it to exclusion list)
10:36:19.50 -25:54:28.5 -- not an asteroid (will add it to exclusion list)
10:48:28.59 -28:37:37.2 -- not an asteroid (will add it to exclusion list)
10:33:54.29 -29:19:28.5 -- not an asteroid (will add it to exclusion list)
10:24:43.73 -26:15:56.7 -- not an asteroid (will add it to exclusion list)
10:45:22.63 -27:38:08.2 -- not an asteroid (will add it to exclusion list)
10:46:00.76 -26:53:05.8 -- not an asteroid (will add it to exclusion list)
10:29:47.11 -25:52:00.5 -- not an asteroid (will add it to exclusion list)
10:31:13.82 -26:40:39.2 -- not an asteroid (will add it to exclusion list)
10:32:46.38 -23:55:03.1 -- not an asteroid (will add it to exclusion list)
10:39:01.73 -22:45:48.9 -- not an asteroid (will add it to exclusion list)
10:23:47.81 -27:15:24.8 -- not an asteroid (will add it to exclusion list)
10:35:02.35 -25:40:49.1 -- not an asteroid (will add it to exclusion list)
10:36:22.64 -25:33:52.9 -- not an asteroid (will add it to exclusion list)
10:36:20.26 -26:02:36.0 -- not an asteroid (will add it to exclusion list)
10:19:33.73 -22:20:45.8 -- not an asteroid (will add it to exclusion list)
10:29:15.36 -22:39:19.2 -- not an asteroid (will add it to exclusion list)
10:15:05.80 -25:02:43.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:15:05.80 -25:02:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:19:33.73 -22:20:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:20:17.73 -22:06:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:20:19.90 -24:50:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:50.96 -27:10:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:23:25.93 -23:41:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:23:35.76 -25:17:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:23:47.81 -27:15:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:24:36.06 -25:24:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:24:43.73 -26:15:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:08.72 -29:08:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:27:34.53 -25:00:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:15.36 -22:39:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:32.17 -21:51:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:47.11 -25:52:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:01.25 -24:12:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:17.35 -25:09:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:13.82 -26:40:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:15.43 -25:02:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:25.71 -28:43:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:46.38 -23:55:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:06.00 -26:33:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:54.29 -29:19:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:53.30 -30:04:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:54.61 -22:16:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:02.35 -25:40:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:02.65 -26:26:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:19.50 -25:54:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:20.26 -26:02:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:22.64 -25:33:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:08.06 -25:36:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:58.53 -22:29:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:01.73 -22:45:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:42.74 -27:27:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:43.70 -27:27:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:58.06 -29:17:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:42:40.39 -28:05:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:42:41.86 -27:05:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:50.69 -24:23:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:22.63 -27:38:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:00.76 -26:53:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:12.29 -24:48:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:12.50 -24:47:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:13.17 -24:47:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:19.53 -28:30:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:00.98 -27:07:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:27.80 -27:30:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:56.64 -29:40:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:28.59 -28:37:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:50:33.10 -26:44:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:52:50.43 -22:37:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:53:12.58 -29:31:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
10:15:05.80 -25:02:43.4 -- not a known variable star
10:19:33.73 -22:20:45.8 -- a known variable star
10:20:17.73 -22:06:19.6 -- not a known variable star
10:20:19.90 -24:50:25.6 -- not a known variable star
10:21:50.96 -27:10:46.9 -- not a known variable star
10:23:25.93 -23:41:35.6 -- not a known variable star
10:23:35.76 -25:17:18.6 -- not a known variable star
10:23:47.81 -27:15:24.8 -- not a known variable star
10:24:36.06 -25:24:58.4 -- not a known variable star
10:24:43.73 -26:15:56.7 -- not a known variable star
10:26:08.72 -29:08:40.8 -- not a known variable star
10:27:34.53 -25:00:09.5 -- not a known variable star
10:29:15.36 -22:39:19.2 -- not a known variable star
10:29:32.17 -21:51:58.8 -- not a known variable star
10:29:47.11 -25:52:00.5 -- not a known variable star
10:30:01.25 -24:12:53.7 -- not a known variable star
10:30:17.35 -25:09:49.7 -- not a known variable star
10:31:13.82 -26:40:39.2 -- not a known variable star
10:31:15.43 -25:02:00.5 -- not a known variable star
10:32:25.71 -28:43:57.2 -- not a known variable star
10:32:46.38 -23:55:03.1 -- not a known variable star
10:33:06.00 -26:33:02.1 -- not a known variable star
10:33:54.29 -29:19:28.5 -- not a known variable star
10:34:53.30 -30:04:14.0 -- not a known variable star
10:34:54.61 -22:16:48.5 -- not a known variable star
10:35:02.35 -25:40:49.1 -- not a known variable star
10:36:02.65 -26:26:09.8 -- not a known variable star
10:36:19.50 -25:54:28.5 -- not a known variable star
10:36:20.26 -26:02:36.0 -- not a known variable star
10:36:22.64 -25:33:52.9 -- not a known variable star
10:37:08.06 -25:36:47.8 -- not a known variable star
10:37:58.53 -22:29:39.6 -- not a known variable star
10:39:01.73 -22:45:48.9 -- not a known variable star
10:39:42.74 -27:27:37.2 -- not a known variable star
10:39:43.70 -27:27:41.3 -- not a known variable star
10:39:58.06 -29:17:11.4 -- not a known variable star
10:42:40.39 -28:05:17.1 -- not a known variable star
10:42:41.86 -27:05:31.7 -- not a known variable star
10:44:50.69 -24:23:13.7 -- not a known variable star
10:45:22.63 -27:38:08.2 -- not a known variable star
10:46:00.76 -26:53:05.8 -- not a known variable star
10:46:12.29 -24:48:04.5 -- not a known variable star
10:46:12.50 -24:47:41.6 -- not a known variable star
10:46:13.17 -24:47:57.3 -- not a known variable star
10:46:19.53 -28:30:04.8 -- not a known variable star
10:47:00.98 -27:07:10.9 -- not a known variable star
10:47:27.80 -27:30:45.0 -- not a known variable star
10:47:56.64 -29:40:07.7 -- not a known variable star
10:48:28.59 -28:37:37.2 -- not a known variable star
10:50:33.10 -26:44:00.1 -- not a known variable star
10:52:50.43 -22:37:01.9 -- not a known variable star
10:53:12.58 -29:31:23.4 -- not a known variable star
Found 51 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
52 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 52 (excluding asteroids and hot pixels, 51 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461152.64285059 -observatory V36
00:41:32.96 +01:40:45.6 Mercury (-0.2mag)
03:39:01.61 +20:00:28.2 Venus (-3.9mag)
00:35:15.84 +02:46:27.3 Mars (1.2mag)
07:15:37.11 +22:41:12.0 Jupiter (-2.1mag)
00:31:53.34 +01:05:46.5 Saturn (0.9mag)
03:49:01.32 +19:51:41.8 Uranus (5.8mag)
00:11:37.69 -00:10:25.5 Neptune (7.8mag)
20:33:59.16 -22:53:01.2 Pluto (14.5mag)
06:23:23.39 +27:29:02.6 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Apr 21 22:33 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461152.64285059:
07:15:40.76 +22:41:01.8 Io (5.8mag)
07:15:25.34 +22:41:38.1 Europa (5.9mag)
07:15:55.09 +22:40:36.1 Ganymede (5.4mag)
07:15:16.47 +22:41:48.1 Callisto (6.6mag)
07:18:40.06 +22:26:07.5 Himalia (15.4mag)
07:15:37.18 +22:41:09.6 Thebe (16.3mag)
07:18:58.63 +22:56:25.9 Elara (17.3mag)
07:14:55.00 +23:17:59.5 Pasiphae (17.4mag)
07:23:48.17 +22:39:46.7 Carme (18.6mag)
00:31:47.63 +01:05:45.4 Titan (8.8mag)
00:31:59.14 +01:05:48.3 Rhea (10.1mag)
00:31:25.43 +01:04:57.7 Iapetus (11.5mag)
00:31:42.56 +01:06:02.9 Hyperion (14.8mag)
00:33:25.17 +01:13:53.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 21 22:33 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461152.64285059:
16:03:02.92 -20:13:14.1 JWST
17:08:18.11 +43:46:00.5 Chandra
07:56:51.62 -37:03:48.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 21 22:33 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461152.64285059 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:30:05.12 +30:49:46.0 18.0mag P/2009 WX51 (Catalina)
18:54:06.15 -29:09:15.0 13.8mag P/2010 H2 (Vales)
05:11:18.40 -69:22:56.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:52.46 +31:28:54.2 17.3mag C/2017 K2 (PANSTARRS)
17:29:38.20 +11:15:48.0 17.6mag C/2021 G2 (ATLAS)
23:11:43.23 +29:28:58.1 17.1mag C/2022 E2 (ATLAS)
04:36:28.09 +26:12:00.1 16.1mag C/2022 N2 (PANSTARRS)
09:04:59.19 +32:01:52.7 16.3mag C/2022 QE78 (ATLAS)
08:32:12.34 +00:28:33.7 17.4mag C/2022 R6 (PANSTARRS)
18:52:03.54 +19:02:13.6 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:32.99 -11:25:51.5 17.5mag P/2023 B1 (PANSTARRS)
09:05:05.45 -10:55:37.2 17.7mag C/2023 F3 (ATLAS)
21:59:57.15 +63:16:55.8 17.6mag C/2023 H5 (Lemmon)
19:13:15.53 -03:51:18.8 14.1mag C/2023 R1 (PANSTARRS)
21:12:46.94 +86:46:27.9 17.8mag C/2023 X2 (Lemmon)
06:21:15.84 +63:30:00.0 17.2mag C/2024 A1 (ATLAS)
05:26:01.52 +20:10:18.9 11.4mag C/2024 E1 (Wierzchos)
16:15:07.46 +07:23:19.6 17.3mag C/2024 G6 (ATLAS)
20:22:16.11 +16:58:29.9 14.5mag C/2024 J3 (ATLAS)
03:31:58.22 -21:28:23.1 16.3mag C/2024 T5 (ATLAS)
05:22:02.55 +43:48:47.5 17.7mag C/2025 J1 (Borisov)
13:13:52.01 +48:48:29.1 15.5mag C/2025 L1 (ATLAS)
03:35:16.10 -27:12:27.0 17.9mag C/2025 Q3 (ATLAS)
01:04:08.38 +14:16:34.0 7.8mag C/2025 R3 (PANSTARRS)
12:51:30.40 +03:22:12.5 17.4mag C/2025 Y1 (ATLAS)
04:10:00.76 +02:07:46.5 14.9mag C/2026 A1 (MAPS)
00:16:33.10 +38:16:45.4 14.8mag C/2026 B2 (Sun-Gao)
18:54:51.56 -09:23:02.8 11.5mag 10P/Tempel
14:51:55.63 +02:30:49.1 14.5mag 24P/Schaumasse
11:01:20.52 -01:20:28.4 15.7mag 29P/Schwassmann-Wachmann
10:37:44.74 -03:39:00.6 17.0mag 43P/Wolf-Harrington
01:58:12.53 +18:31:23.9 17.3mag 47P/Ashbrook-Jackson
07:22:22.67 +35:40:14.8 17.0mag 63P/Wild
23:36:46.00 -10:43:40.0 15.7mag 65P/Gunn
04:19:58.31 +23:17:23.1 15.9mag 76P/West-Kohoutek-Ikemura
01:19:15.13 +09:25:26.3 14.3mag 78P/Gehrels
23:21:14.61 -07:34:29.0 14.7mag 88P/Howell
02:28:02.47 +22:13:57.7 15.1mag 93P/Lovas
05:06:39.98 +32:35:37.5 16.1mag 123P/West-Hartley
08:36:02.54 +35:32:03.2 16.2mag 124P/Mrkos
02:42:47.03 +15:02:37.2 16.4mag 128P/Shoemaker-Holt
02:59:38.21 +15:13:07.9 17.5mag 131P/Mueller
01:58:54.41 +15:12:28.6 10.5mag 141P/Machholz
02:06:50.48 +07:08:55.9 10.5mag 141P-A/Machholz
00:49:33.17 +02:54:11.1 12.1mag 141P-D/Machholz
02:37:28.00 +08:53:08.1 17.9mag 141P-I/Machholz
01:19:35.96 +01:34:34.7 15.0mag 162P/SidingSpring
14:40:38.87 +00:29:48.2 17.8mag 210P/Christensen
21:55:54.03 -09:59:03.5 17.8mag 218P/LINEAR
17:17:23.76 -13:10:58.6 16.1mag 235P/LINEAR
05:47:54.29 +35:06:56.0 16.8mag 240P/NEAT
07:41:45.19 -04:31:56.5 17.8mag 242P/Spahr
22:32:17.00 -19:16:55.9 17.7mag 260P/McNaught
02:10:56.34 +21:59:39.2 17.9mag 295P/LINEAR
15:40:01.99 +07:22:20.4 17.5mag 391P/Kowalski
07:36:46.80 +21:22:23.7 17.7mag 450P/LONEOS
05:44:59.22 +44:40:26.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 21 22:33 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
-rw-r--r-- 1 apache apache 5.8K Apr 21 22:32 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 21 22:32 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:06:16.602 -06:52:59.29 AT 2026jpa 2026-04-13.89 19.276
06:42:32.732 -34:30:04.15 AT 2026joz 2026-04-14.77 18.707
13:06:33.339 -08:24:24.46 AT 2026joy 2026-04-14.02 19.307
21:07:11.613 -12:36:56.09 AT 2026jox 2026-04-14.14 18.849
05:34:42.408 -28:21:31.62 AT 2026jow 2026-04-14.74 18.902
12:30:54.108 -14:11:53.07 AT 2026jov 2026-04-14.03 19.309
05:52:53.155 -34:43:22.49 AT 2026jou 2026-04-14.75 19.398
05:40:18.921 -24:52:33.50 AT 2026jot 2026-04-14.77 18.65
15:53:02.304 +04:30:53.21 AT 2026jos 2026-04-14.09 19.566
11:19:37.053 +36:36:59.54 AT 2026jor 2026-04-11.94 20.14
08:17:15.784 +16:04:01.41 AT 2026joq 2026-04-11.86 19.95
15:52:58.319 -17:01:02.93 AT 2026jop 2026-04-09.53 19.69
09:28:29.338 +17:46:10.46 AT 2026joo 2026-04-11.90 19.1
14:08:31.151 +20:01:29.32 AT 2026jon 2026-04-08.02 19.9
08:15:22.510 -21:29:08.39 AT 2026jom 2026-04-12.37 19.76
12:13:11.990 +05:30:27.70 AT 2026jol 2026-04-08.25 16.6
09:57:55.902 +03:33:01.27 AT 2026jok 2026-03-06.10 21.72
15:47:58.800 -16:07:43.45 AT 2026joj 2026-04-10.44 20.1583
09:57:44.859 +01:08:42.73 AT 2026joi 2026-04-06.02 22.85
14:40:55.647 +05:24:36.73 SN 2026joh 2026-04-14.03 17.708
-rw-r--r-- 1 apache apache 30K Apr 21 22:32 tns_transients_list.txt
