This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb
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 07 16.1668 2461237.6668 12.37 00:01:30.02 +53:59:26.2
115.55514 -8.16435 galactic Cas Second-epoch detections are separated by 2.2" and 6.0 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 | target | 00:01:30.02 +53:59:26.2 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.038 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:30.02 +53:59:26.2: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:30.02 +53:59:26.2: 13.71 +/- 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!
TCP 2026 07 16.1668* 00 01 30.02 +53 59 26.2 12.4 U Cas 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
target,2461237.6668,12.37,0.05,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
target 20260716.1668 12.37CV 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 07 16.1668 2461237.6668 12.48 23:45:18.42 +55:48:27.4
113.68089 -5.87179 galactic Cas Second-epoch detections are separated by 1.6" 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 | target | 23:45:18.42 +55:48:27.4 (user input) | T | P | (position from user input) J-Ks=0.333+/-0.039 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:18.42 +55:48:27.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:18.42 +55:48:27.4: 13.59 +/- 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!
TCP 2026 07 16.1668* 23 45 18.42 +55 48 27.4 12.5 U Cas 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
target,2461237.6668,12.48,0.05,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
target 20260716.1668 12.48CV 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 07 16.1668 2461237.6668 12.25 00:23:01.27 +53:17:43.5
118.63578 -9.33913 galactic Cas 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 | target | 00:23:01.27 +53:17:43.5 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:01.27 +53:17:43.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:01.27 +53:17:43.5: 13.64 +/- 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!
TCP 2026 07 16.1668* 00 23 01.27 +53 17 43.5 12.2 U Cas 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
target,2461237.6668,12.25,0.05,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
target 20260716.1668 12.25CV 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 07 16.1668 2461237.6668 12.44 23:49:50.78 +54:41:26.6
114.03491 -7.11358 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J357.4575+54.6918 | 23:49:50.78 +54:41:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.839+/-0.058 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:50.78 +54:41:26.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:50.78 +54:41:26.6: 13.49 +/- 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!
TCP 2026 07 16.1668* 23 49 50.78 +54 41 26.6 12.4 U Cas 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
ATO J357.4575+54.6918,2461237.6668,12.44,0.05,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 J357.4575+54.6918 20260716.1668 12.44CV 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 07 16.1668 2461237.6668 12.18 00:18:37.75 +51:19:43.7
117.71772 -11.21048 galactic Cas Second-epoch detections are separated by 2.4" 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 394972201928561024 | 00:18:37.52 +51:20:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.233+/-0.042 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:37.75 +51:19:43.7: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:37.75 +51:19:43.7: 13.59 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.32
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!
TCP 2026 07 16.1668* 00 18 37.75 +51 19 43.7 12.2 U Cas 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 394972201928561024,2461237.6668,12.18,0.05,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 394972201928561024 20260716.1668 12.18CV 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 07 16.1668 2461237.6668 12.14 00:10:34.20 +49:54:02.1
116.21312 -12.43727 galactic Cas Second-epoch detections are separated by 0.5" and 6.4 pix
The object was found in VSX19" Gaia DR3 393709623281055744
Type: ROT
# Max. Min./Amp. JD0 Period
13.180 G 13.190 G 0.515320000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:34.20 +49:54:02.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:34.20 +49:54:02.1: 13.62 +/- 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!
TCP 2026 07 16.1668* 00 10 34.20 +49 54 02.1 12.1 U Cas 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 393709623281055744,2461237.6668,12.14,0.05,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 393709623281055744 20260716.1668 12.14CV 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 07 16.1668 2461237.6668 12.14 00:12:56.75 +55:53:17.1
117.51690 -6.57844 galactic Cas Second-epoch detections are separated by 1.9" and 6.0 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 420720844406907264 | 00:12:57.41 +55:52:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:56.75 +55:53:17.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:56.75 +55:53:17.1: 13.53 +/- 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!
TCP 2026 07 16.1668* 00 12 56.75 +55 53 17.1 12.1 U Cas 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 420720844406907264,2461237.6668,12.14,0.05,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 420720844406907264 20260716.1668 12.14CV 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 07 16.1668 2461237.6668 12.30 23:43:58.84 +55:38:50.0
113.45801 -5.97878 galactic Cas Second-epoch detections are separated by 2.5" 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 | target | 23:43:58.84 +55:38:50.0 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:58.84 +55:38:50.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:58.84 +55:38:50.0: 13.46 +/- 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!
TCP 2026 07 16.1668* 23 43 58.84 +55 38 50.0 12.3 U Cas 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
target,2461237.6668,12.30,0.05,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
target 20260716.1668 12.30CV 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 07 16.1668 2461237.6668 12.20 23:55:13.96 +53:46:20.4
114.59662 -8.18733 galactic Cas Second-epoch detections are separated by 0.5" 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 1945516418680563840 | 23:55:11.76 +53:46:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.394+/-0.046 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:13.96 +53:46:20.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:13.96 +53:46:20.4: 13.18 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.26
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!
TCP 2026 07 16.1668* 23 55 13.96 +53 46 20.4 12.2 U Cas 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 1945516418680563840,2461237.6668,12.20,0.05,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 1945516418680563840 20260716.1668 12.20CV 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 07 16.1668 2461237.6668 12.15 23:28:42.94 +51:00:33.2
109.90159 -9.75767 galactic Cas Second-epoch detections are separated by 0.9" 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 | ATO J352.1729+51.0017 | 23:28:42.94 +51:00:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.283+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:42.94 +51:00:33.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:42.94 +51:00:33.2: 13.52 +/- 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!
TCP 2026 07 16.1668* 23 28 42.94 +51 00 33.2 12.2 U Cas 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
ATO J352.1729+51.0017,2461237.6668,12.15,0.05,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 J352.1729+51.0017 20260716.1668 12.15CV 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 07 16.1668 2461237.6668 12.17 00:05:00.28 +52:55:22.2
115.87050 -9.31111 galactic Cas Second-epoch detections are separated by 0.9" 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 396098655893341312 | 00:04:57.64 +52:55:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:00.28 +52:55:22.2: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:00.28 +52:55:22.2: 13.64 +/- 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!
TCP 2026 07 16.1668* 00 05 00.28 +52 55 22.2 12.2 U Cas 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 396098655893341312,2461237.6668,12.17,0.05,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 396098655893341312 20260716.1668 12.17CV 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 07 16.1668 2461237.6668 11.85 00:31:04.43 +55:22:25.9
120.01750 -7.38261 galactic Cas Second-epoch detections are separated by 0.9" and 6.2 pix
The object was found in VSX 1" Gaia DR3 418234333222683648
Type: ROT
# Max. Min./Amp. JD0 Period
13.930 G 13.950 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:04.43 +55:22:25.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:04.43 +55:22:25.9: 13.42 +/- 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!
TCP 2026 07 16.1668* 00 31 04.43 +55 22 25.9 11.8 U Cas 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 418234333222683648,2461237.6668,11.85,0.05,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 418234333222683648 20260716.1668 11.85CV 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 07 16.1668 2461237.6668 12.21 23:59:36.07 +56:58:36.4
115.88297 -5.18384 galactic Cas Second-epoch detections are separated by 3.4" and 6.1 pix
The object was found in VSX16" ZTF J235934.26+565842.3
Type: VAR
# Max. Min./Amp. JD0 Period
17.218 r Y 0.143 r 2458256.98000 0.142362300000
ATTENTION: measured mag 12.21 is 4.9 mag brighter than the VSX record maximum brightness 17.07 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:36.07 +56:58:36.4: 13.52 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:36.07 +56:58:36.4: 12.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.09 +/- 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!
TCP 2026 07 16.1668* 23 59 36.07 +56 58 36.4 12.2 U Cas 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
ZTF J235934.26+565842.3,2461237.6668,12.21,0.05,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
ZTF J235934.26+565842.3 20260716.1668 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 07 16.1668 2461237.6668 11.96 00:19:34.11 +52:53:24.6
118.06527 -9.68018 galactic Cas Second-epoch detections are separated by 3.1" and 6.5 pix
The object was found in VSX 5" Gaia DR3 419178641912133120
Type: ROT
# Max. Min./Amp. JD0 Period
13.720 G 13.770 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:34.11 +52:53:24.6: 13.10 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:34.11 +52:53:24.6: 12.82 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.94 +/- 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!
TCP 2026 07 16.1668* 00 19 34.11 +52 53 24.6 12.0 U Cas 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 419178641912133120,2461237.6668,11.96,0.05,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 419178641912133120 20260716.1668 11.96CV 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 07 16.1668 2461237.6668 12.04 23:46:14.85 +52:45:10.9
113.03352 -8.86131 galactic Cas Second-epoch detections are separated by 1.5" 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 1945363281626831488 | 23:46:14.29 +52:44:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:14.85 +52:45:10.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:14.85 +52:45:10.9: 13.67 +/- 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!
TCP 2026 07 16.1668* 23 46 14.85 +52 45 10.9 12.0 U Cas 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 1945363281626831488,2461237.6668,12.04,0.05,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 1945363281626831488 20260716.1668 12.04CV 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 07 16.1668 2461237.6668 12.17 23:53:29.55 +54:54:32.3
114.60088 -7.02275 galactic Cas Second-epoch detections are separated by 1.6" 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 | target | 23:53:29.55 +54:54:32.3 (user input) | T | P | (position from user input) J-Ks=0.980+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:29.55 +54:54:32.3: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:29.55 +54:54:32.3: 13.64 +/- 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!
TCP 2026 07 16.1668* 23 53 29.55 +54 54 32.3 12.2 U Cas 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
target,2461237.6668,12.17,0.05,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
target 20260716.1668 12.17CV 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 07 16.1668 2461237.6668 11.88 23:53:11.05 +53:50:49.3
114.31556 -8.04732 galactic Cas Second-epoch detections are separated by 0.7" 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 1993564943675259776 | 23:53:07.33 +53:51:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.709+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:11.05 +53:50:49.3: 13.19 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:11.05 +53:50:49.3: 12.77 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.13
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!
TCP 2026 07 16.1668* 23 53 11.05 +53 50 49.3 11.9 U Cas 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 1993564943675259776,2461237.6668,11.88,0.05,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 1993564943675259776 20260716.1668 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 07 16.1668 2461237.6668 11.91 00:11:24.91 +55:00:14.9
117.16467 -7.41882 galactic Cas Second-epoch detections are separated by 1.9" 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 | ATO J002.8471+55.0015 | 00:11:24.91 +55:00:14.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.379+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:24.91 +55:00:14.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:24.91 +55:00:14.9: 13.65 +/- 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!
TCP 2026 07 16.1668* 00 11 24.91 +55 00 14.9 11.9 U Cas 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
ATO J002.8471+55.0015,2461237.6668,11.91,0.05,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 J002.8471+55.0015 20260716.1668 11.91CV 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 07 16.1668 2461237.6668 11.98 00:07:14.33 +56:13:57.4
116.78153 -6.11042 galactic Cas Second-epoch detections are separated by 0.8" 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 420957995321025152 | 00:07:11.30 +56:14:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:14.33 +56:13:57.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:14.33 +56:13:57.4: 13.60 +/- 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!
TCP 2026 07 16.1668* 00 07 14.33 +56 13 57.4 12.0 U Cas 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 420957995321025152,2461237.6668,11.98,0.05,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 420957995321025152 20260716.1668 11.98CV 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 07 16.1668 2461237.6668 12.07 23:45:47.64 +57:16:14.5
114.11835 -4.47347 galactic Cas Second-epoch detections are separated by 3.4" 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 | ATO J356.4612+57.2675 | 23:45:47.64 +57:16:14.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.058 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.64 +57:16:14.5: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:47.64 +57:16:14.5: 13.60 +/- 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!
TCP 2026 07 16.1668* 23 45 47.64 +57 16 14.5 12.1 U Cas 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
ATO J356.4612+57.2675,2461237.6668,12.07,0.05,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
ATO J356.4612+57.2675 20260716.1668 12.07CV 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 07 16.1668 2461237.6668 11.92 00:12:08.51 +52:31:38.4
116.88359 -9.88233 galactic Cas Second-epoch detections are separated by 1.7" and 6.5 pix
The object was found in VSX21" Gaia DR3 395921875037713920
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.950 G 12.980 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:08.51 +52:31:38.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:08.51 +52:31:38.4: 13.66 +/- 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!
TCP 2026 07 16.1668* 00 12 08.51 +52 31 38.4 11.9 U Cas 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 395921875037713920,2461237.6668,11.92,0.05,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
Gaia DR3 395921875037713920 20260716.1668 11.92CV 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 07 16.1668 2461237.6668 11.77 00:18:30.99 +50:48:52.0
117.63170 -11.71819 galactic Cas Second-epoch detections are separated by 0.7" 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 394929497072882176 | 00:18:33.93 +50:48:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:30.99 +50:48:52.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:30.99 +50:48:52.0: 13.58 +/- 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!
TCP 2026 07 16.1668* 00 18 30.99 +50 48 52.0 11.8 U Cas 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 394929497072882176,2461237.6668,11.77,0.05,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 394929497072882176 20260716.1668 11.77CV 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 07 16.1668 2461237.6668 11.76 00:15:49.08 +57:58:47.2
118.20901 -4.56496 galactic Cas Second-epoch detections are separated by 1.7" and 6.0 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 | target | 00:15:49.08 +57:58:47.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:49.08 +57:58:47.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:49.08 +57:58:47.2: 13.53 +/- 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!
TCP 2026 07 16.1668* 00 15 49.08 +57 58 47.2 11.8 U Cas 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
target,2461237.6668,11.76,0.05,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
target 20260716.1668 11.76CV 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 07 16.1668 2461237.6668 11.92 23:36:46.39 +53:03:07.6
111.72448 -8.18720 galactic Cas Second-epoch detections are separated by 3.2" 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 | target | 23:36:46.39 +53:03:07.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:46.39 +53:03:07.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:46.39 +53:03:07.6: 13.55 +/- 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!
TCP 2026 07 16.1668* 23 36 46.39 +53 03 07.6 11.9 U Cas 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
target,2461237.6668,11.92,0.05,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
target 20260716.1668 11.92CV 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 07 16.1668 2461237.6668 11.72 00:25:55.05 +55:20:53.6
119.27936 -7.34243 galactic Cas Second-epoch detections are separated by 1.1" and 6.0 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 | ATO J006.4750+55.3531 | 00:25:55.05 +55:20:53.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.631+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:55.05 +55:20:53.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:55.05 +55:20:53.6: 13.57 +/- 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!
TCP 2026 07 16.1668* 00 25 55.05 +55 20 53.6 11.7 U Cas 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
ATO J006.4750+55.3531,2461237.6668,11.72,0.05,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
ATO J006.4750+55.3531 20260716.1668 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 07 16.1668 2461237.6668 11.87 23:41:51.68 +54:39:57.7
112.90373 -6.84537 galactic Cas Second-epoch detections are separated by 0.7" 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 | ATO J355.4769+54.6722 | 23:41:51.68 +54:39:57.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:51.68 +54:39:57.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:51.68 +54:39:57.7: 13.60 +/- 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!
TCP 2026 07 16.1668* 23 41 51.68 +54 39 57.7 11.9 U Cas 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
ATO J355.4769+54.6722,2461237.6668,11.87,0.05,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 J355.4769+54.6722 20260716.1668 11.87CV 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 07 16.1668 2461237.6668 11.94 23:24:46.90 +55:53:57.1
110.94172 -4.94208 galactic Cas Second-epoch detections are separated by 3.2" 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 | ATO J351.2120+55.8960 | 23:24:46.90 +55:53:57.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:46.90 +55:53:57.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:46.90 +55:53:57.1: 13.15 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.15 +/- 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!
TCP 2026 07 16.1668* 23 24 46.90 +55 53 57.1 11.9 U Cas 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
ATO J351.2120+55.8960,2461237.6668,11.94,0.05,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 J351.2120+55.8960 20260716.1668 11.94CV 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 07 16.1668 2461237.6668 11.91 23:52:21.52 +51:55:19.5
113.74819 -9.89309 galactic Cas Second-epoch detections are separated by 1.8" 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 | target | 23:52:21.52 +51:55:19.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:21.52 +51:55:19.5: 12.93 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:21.52 +51:55:19.5: 12.76 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.84 +/- 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!
TCP 2026 07 16.1668* 23 52 21.52 +51 55 19.5 11.9 U Cas 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
target,2461237.6668,11.91,0.05,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
target 20260716.1668 11.91CV 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 07 16.1668 2461237.6668 11.68 23:39:32.20 +55:18:28.7
112.75659 -6.13692 galactic Cas Second-epoch detections are separated by 1.8" 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 | target | 23:39:32.20 +55:18:28.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:32.20 +55:18:28.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:32.20 +55:18:28.7: 13.52 +/- 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!
TCP 2026 07 16.1668* 23 39 32.20 +55 18 28.7 11.7 U Cas 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
target,2461237.6668,11.68,0.05,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
target 20260716.1668 11.68CV 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 07 16.1668 2461237.6668 11.67 00:20:58.69 +52:34:39.0
118.24137 -10.01662 galactic Cas Second-epoch detections are separated by 1.9" 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 419154727534462336 | 00:20:59.17 +52:34:19.4 (Gaia DR3) | ROT (local) | 4.454290000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:58.69 +52:34:39.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:58.69 +52:34:39.0: 13.56 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.33
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!
TCP 2026 07 16.1668* 00 20 58.69 +52 34 39.0 11.7 U Cas 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 419154727534462336,2461237.6668,11.67,0.05,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 419154727534462336 20260716.1668 11.67CV 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 07 16.1668 2461237.6668 11.62 00:23:03.30 +56:42:13.9
119.02246 -5.95229 galactic Cas Second-epoch detections are separated by 0.5" 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 | ATO J005.7746+56.7038 | 00:23:03.30 +56:42:13.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:03.30 +56:42:13.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:03.30 +56:42:13.9: 13.55 +/- 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!
TCP 2026 07 16.1668* 00 23 03.30 +56 42 13.9 11.6 U Cas 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
ATO J005.7746+56.7038,2461237.6668,11.62,0.05,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 J005.7746+56.7038 20260716.1668 11.62CV 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 07 16.1668 2461237.6668 11.81 00:15:45.59 +53:37:26.0
117.59163 -8.87751 galactic Cas Second-epoch detections are separated by 2.0" 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 | target | 00:15:45.59 +53:37:26.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:45.59 +53:37:26.0: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:45.59 +53:37:26.0: 13.64 +/- 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!
TCP 2026 07 16.1668* 00 15 45.59 +53 37 26.0 11.8 U Cas 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
target,2461237.6668,11.81,0.05,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
target 20260716.1668 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 07 16.1668 2461237.6668 11.55 00:09:36.34 +53:24:29.2
116.64324 -8.95209 galactic Cas Second-epoch detections are separated by 0.6" 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 420037223052857472 | 00:09:34.97 +53:24:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.637+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:36.34 +53:24:29.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:36.34 +53:24:29.2: 13.60 +/- 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!
TCP 2026 07 16.1668* 00 09 36.34 +53 24 29.2 11.6 U Cas 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 420037223052857472,2461237.6668,11.55,0.05,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 420037223052857472 20260716.1668 11.55CV 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 07 16.1668 2461237.6668 11.68 23:32:58.58 +56:46:21.5
112.29906 -4.47058 galactic Cas Second-epoch detections are separated by 0.4" and 6.6 pix
The object was found in VSX 7" Gaia DR3 1998580365968459136
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.790 G 13.810 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:58.58 +56:46:21.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:58.58 +56:46:21.5: 13.54 +/- 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!
TCP 2026 07 16.1668* 23 32 58.58 +56 46 21.5 11.7 U Cas 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 1998580365968459136,2461237.6668,11.68,0.05,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 1998580365968459136 20260716.1668 11.68CV 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 07 16.1668 2461237.6668 11.66 23:41:28.05 +52:04:55.1
112.14319 -9.31800 galactic Cas Second-epoch detections are separated by 0.9" 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 | ATO J355.3702+52.0801 | 23:41:28.05 +52:04:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:28.05 +52:04:55.1: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:28.05 +52:04:55.1: 13.70 +/- 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!
TCP 2026 07 16.1668* 23 41 28.05 +52 04 55.1 11.7 U Cas 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
ATO J355.3702+52.0801,2461237.6668,11.66,0.05,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 J355.3702+52.0801 20260716.1668 11.66CV 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 07 16.1668 2461237.6668 11.83 23:46:34.57 +51:28:31.2
112.75579 -10.11031 galactic Cas Second-epoch detections are separated by 2.4" 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 | ATO J356.6454+51.4778 | 23:46:34.57 +51:28:31.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.391+/-0.039 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:34.57 +51:28:31.2: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:34.57 +51:28:31.2: 13.71 +/- 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!
TCP 2026 07 16.1668* 23 46 34.57 +51 28 31.2 11.8 U Cas 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
ATO J356.6454+51.4778,2461237.6668,11.83,0.05,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 J356.6454+51.4778 20260716.1668 11.83CV 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 07 16.1668 2461237.6668 11.43 00:19:06.05 +56:05:25.3
118.40301 -6.49677 galactic Cas Second-epoch detections are separated by 1.2" and 6.0 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 | ATO J004.7658+56.1014 | 00:19:06.05 +56:05:25.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:06.05 +56:05:25.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:06.05 +56:05:25.3: 13.62 +/- 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!
TCP 2026 07 16.1668* 00 19 06.05 +56 05 25.3 11.4 U Cas 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
ATO J004.7658+56.1014,2461237.6668,11.43,0.05,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 J004.7658+56.1014 20260716.1668 11.43CV 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 07 16.1668 2461237.6668 11.51 00:31:00.10 +57:25:00.0
120.17113 -5.34549 galactic Cas Second-epoch detections are separated by 2.0" and 5.8 pix
The object was found in VSX 2" Gaia DR3 421839975445105536
Type: E
# Max. Min./Amp. JD0 Period
13.480 G 13.690 G 2.085110000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:00.10 +57:25:00.0: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:00.10 +57:25:00.0: 13.54 +/- 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!
TCP 2026 07 16.1668* 00 31 00.10 +57 25 00.0 11.5 U Cas 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 421839975445105536,2461237.6668,11.51,0.05,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 421839975445105536 20260716.1668 11.51CV 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 07 16.1668 2461237.6668 11.72 23:44:50.64 +54:41:18.1
113.32868 -6.93696 galactic Cas Second-epoch detections are separated by 4.3" and 7.1 pix
The object was found in VSX 2" Gaia DR3 1994179536316071424
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.760 G 13.800 G 0.027338400000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:50.64 +54:41:18.1: 13.40 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:50.64 +54:41:18.1: 13.06 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.18
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!
TCP 2026 07 16.1668* 23 44 50.64 +54 41 18.1 11.7 U Cas 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 1994179536316071424,2461237.6668,11.72,0.05,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 1994179536316071424 20260716.1668 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 07 16.1668 2461237.6668 11.54 00:06:34.80 +54:54:40.0
116.45890 -7.39587 galactic Cas Second-epoch detections are separated by 1.6" 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 | target | 00:06:34.80 +54:54:40.0 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.398+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:34.80 +54:54:40.0: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:34.80 +54:54:40.0: 13.70 +/- 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!
TCP 2026 07 16.1668* 00 06 34.80 +54 54 40.0 11.5 U Cas 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
target,2461237.6668,11.54,0.05,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
target 20260716.1668 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 07 16.1668 2461237.6668 11.70 23:50:03.46 +50:48:21.9
113.12655 -10.89337 galactic Cas Second-epoch detections are separated by 2.0" 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 1943993874253244032 | 23:50:02.21 +50:49:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1927AnHar.100...33C HD 236225 J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:03.46 +50:48:21.9: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:03.46 +50:48:21.9: 13.61 +/- 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!
TCP 2026 07 16.1668* 23 50 03.46 +50 48 21.9 11.7 U Cas 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 1943993874253244032,2461237.6668,11.70,0.05,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 1943993874253244032 20260716.1668 11.70CV 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 07 16.1668 2461237.6668 11.70 23:30:12.79 +52:40:51.0
110.65776 -8.24440 galactic Cas Second-epoch detections are separated by 1.1" and 6.5 pix
The object was found in VSX 8" ZTF J233013.50+524056.1
Type: EW
# Max. Min./Amp. JD0 Period
16.903 r Y 0.104 r 2458281.96660 0.306489800000
ATTENTION: measured mag 11.70 is 5.1 mag brighter than the VSX record maximum brightness 16.80 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:12.79 +52:40:51.0: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:12.79 +52:40:51.0: 13.65 +/- 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!
TCP 2026 07 16.1668* 23 30 12.79 +52 40 51.0 11.7 U Cas 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
ZTF J233013.50+524056.1,2461237.6668,11.70,0.05,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
ZTF J233013.50+524056.1 20260716.1668 11.70CV 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 07 16.1668 2461237.6668 11.60 23:36:52.97 +56:58:23.1
112.86979 -4.43502 galactic Cas Second-epoch detections are separated by 2.7" and 6.2 pix
The object was found in VSX 1" Gaia DR3 1998633211244654336
Type: ROT
# Max. Min./Amp. JD0 Period
13.210 G 13.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:52.97 +56:58:23.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:52.97 +56:58:23.1: 13.57 +/- 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!
TCP 2026 07 16.1668* 23 36 52.97 +56 58 23.1 11.6 U Cas 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 1998633211244654336,2461237.6668,11.60,0.05,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 1998633211244654336 20260716.1668 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 07 16.1668 2461237.6668 11.56 23:51:22.92 +53:52:58.6
114.06275 -7.95141 galactic Cas Second-epoch detections are separated by 0.4" 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 1993521817902507648 | 23:51:19.84 +53:53:07.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.460+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:22.92 +53:52:58.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:22.92 +53:52:58.6: 13.68 +/- 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!
TCP 2026 07 16.1668* 23 51 22.92 +53 52 58.6 11.6 U Cas 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 1993521817902507648,2461237.6668,11.56,0.05,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 1993521817902507648 20260716.1668 11.56CV 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 07 16.1668 2461237.6668 11.63 23:18:44.16 +55:58:25.8
110.16854 -4.58357 galactic Cas Second-epoch detections are separated by 0.3" and 6.6 pix
The object was found in VSX10" NSVS J2318429+555826
Type: SR
# Max. Min./Amp. JD0 Period
15.453 g Y 0.762 g 2458235.85240 249.075952100000 M5
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:44.16 +55:58:25.8: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:44.16 +55:58:25.8: 13.58 +/- 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!
TCP 2026 07 16.1668* 23 18 44.16 +55 58 25.8 11.6 U Cas 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
NSVS J2318429+555826,2461237.6668,11.63,0.05,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
NSVS J2318429+555826 20260716.1668 11.63CV 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 07 16.1668 2461237.6668 11.38 00:24:54.36 +53:26:45.9
118.93545 -9.21966 galactic Cas Second-epoch detections are separated by 1.0" 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 419472344650653312 | 00:24:52.91 +53:26:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.351+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:54.36 +53:26:45.9: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:54.36 +53:26:45.9: 13.54 +/- 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!
TCP 2026 07 16.1668* 00 24 54.36 +53 26 45.9 11.4 U Cas 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 419472344650653312,2461237.6668,11.38,0.05,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 419472344650653312 20260716.1668 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 07 16.1668 2461237.6668 11.36 00:24:30.09 +57:44:09.1
119.32958 -4.94736 galactic Cas Second-epoch detections are separated by 1.1" 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 422083031936705536 | 00:24:27.49 +57:43:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:30.09 +57:44:09.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:30.09 +57:44:09.1: 13.46 +/- 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!
TCP 2026 07 16.1668* 00 24 30.09 +57 44 09.1 11.4 U Cas 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 422083031936705536,2461237.6668,11.36,0.05,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 422083031936705536 20260716.1668 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 07 16.1668 2461237.6668 11.31 00:23:38.03 +50:04:08.1
118.36735 -12.55625 galactic Cas Second-epoch detections are separated by 2.3" 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 394275974847473024 | 00:23:39.41 +50:03:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:38.03 +50:04:08.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:38.03 +50:04:08.1: 13.53 +/- 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!
TCP 2026 07 16.1668* 00 23 38.03 +50 04 08.1 11.3 U Cas 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 394275974847473024,2461237.6668,11.31,0.05,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 394275974847473024 20260716.1668 11.31CV 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 07 16.1668 2461237.6668 11.39 00:27:36.32 +51:31:27.3
119.15732 -11.17275 galactic Cas Second-epoch detections are separated by 2.8" and 6.4 pix
The object was found in VSX 1" Gaia DR3 418844012415546240
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.140 G 13.160 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:36.32 +51:31:27.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:36.32 +51:31:27.3: 13.61 +/- 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!
TCP 2026 07 16.1668* 00 27 36.32 +51 31 27.3 11.4 U Cas 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 418844012415546240,2461237.6668,11.39,0.05,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 418844012415546240 20260716.1668 11.39CV 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 07 16.1668 2461237.6668 11.44 23:21:46.86 +54:35:20.2
110.09538 -6.03289 galactic Cas Second-epoch detections are separated by 1.2" 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 | Large-amplitude variable Gaia DR2 1996007405677510528 | 23:21:46.14 +54:35:02.9 (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) SpType: K1 (LAMOST DR5) J-Ks=0.682+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:46.86 +54:35:20.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:46.86 +54:35:20.2: 13.38 +/- 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!
TCP 2026 07 16.1668* 23 21 46.86 +54 35 20.2 11.4 U Cas 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
Large-amplitude variable Gaia DR2 1996007405677510528,2461237.6668,11.44,0.05,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 1996007405677510528 20260716.1668 11.44CV 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 07 16.1668 2461237.6668 11.10 23:58:38.56 +53:54:04.5
115.12089 -8.16789 galactic Cas Second-epoch detections are separated by 1.9" 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 | ATO J359.6649+53.9052 | 23:58:38.56 +53:54:04.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.56 +53:54:04.5: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.56 +53:54:04.5: 13.73 +/- 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!
TCP 2026 07 16.1668* 23 58 38.56 +53 54 04.5 11.1 U Cas 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
ATO J359.6649+53.9052,2461237.6668,11.10,0.05,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 J359.6649+53.9052 20260716.1668 11.10CV 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 07 16.1668 2461237.6668 11.54 23:15:12.39 +52:26:37.9
108.41056 -7.69356 galactic And Second-epoch detections are separated by 2.4" 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 | ATO J348.7960+52.4487 | 23:15:12.39 +52:26:37.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.719+/-0.052 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:12.39 +52:26:37.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:12.39 +52:26:37.9: 13.47 +/- 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!
TCP 2026 07 16.1668* 23 15 12.39 +52 26 37.9 11.5 U And 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
ATO J348.7960+52.4487,2461237.6668,11.54,0.05,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
ATO J348.7960+52.4487 20260716.1668 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 07 16.1668 2461237.6668 11.05 00:06:20.65 +54:44:21.4
116.39484 -7.55911 galactic Cas Second-epoch detections are separated by 0.7" 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 | ATO J001.5720+54.7461 | 00:06:20.66 +54:44:48.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:20.65 +54:44:21.4: 13.59 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:20.65 +54:44:21.4: 13.14 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.19
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!
TCP 2026 07 16.1668* 00 06 20.65 +54 44 21.4 11.1 U Cas 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
ATO J001.5720+54.7461,2461237.6668,11.05,0.05,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 J001.5720+54.7461 20260716.1668 11.05CV 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 07 16.1668 2461237.6668 11.13 23:29:28.33 +54:40:59.2
111.18400 -6.30825 galactic Cas Second-epoch detections are separated by 1.4" and 6.4 pix
The object was found in VSX10" Gaia DR3 1995868454895136896
Type: ROT
# Max. Min./Amp. JD0 Period
16.960 G 17.020 G K
ATTENTION: measured mag 11.13 is 5.8 mag brighter than the VSX record maximum brightness 16.96 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:28.33 +54:40:59.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:28.33 +54:40:59.2: 13.59 +/- 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!
TCP 2026 07 16.1668* 23 29 28.33 +54 40 59.2 11.1 U Cas 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 1995868454895136896,2461237.6668,11.13,0.05,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 1995868454895136896 20260716.1668 11.13CV 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 07 16.1668 2461237.6668 10.98 23:18:34.53 +54:31:30.9
109.63494 -5.93138 galactic Cas Second-epoch detections are separated by 3.9" 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 1996050389711552512 | 23:18:37.19 +54:31:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:34.53 +54:31:30.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:34.53 +54:31:30.9: 13.47 +/- 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!
TCP 2026 07 16.1668* 23 18 34.53 +54 31 30.9 11.0 U Cas 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 1996050389711552512,2461237.6668,10.98,0.05,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 1996050389711552512 20260716.1668 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 07 16.1668 2461237.6668 10.82 00:06:15.65 +55:15:12.0
116.47397 -7.05094 galactic Cas Second-epoch detections are separated by 1.9" and 6.6 pix
The object was found in VSX21" ASASSN-V J000613.81+551458.3
Type: L
# Max. Min./Amp. JD0 Period
11.300 V 11.410 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:15.65 +55:15:12.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:15.65 +55:15:12.0: 13.55 +/- 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!
TCP 2026 07 16.1668* 00 06 15.65 +55 15 12.0 10.8 U Cas 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
ASASSN-V J000613.81+551458.3,2461237.6668,10.82,0.05,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
ASASSN-V J000613.81+551458.3 20260716.1668 10.82CV 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 07 16.1668 2461237.6668 11.14 23:13:08.57 +53:45:17.3
108.60823 -6.36088 galactic Cas Second-epoch detections are separated by 4.1" and 6.9 pix
The object was found in VSX 3" ZTF J231308.58+534520.0
Type: M
# Max. Min./Amp. JD0 Period
19.454 g Y 4.908 g 2458360.34240 358.008827700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:08.57 +53:45:17.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:08.57 +53:45:17.3: 13.35 +/- 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!
TCP 2026 07 16.1668* 23 13 08.57 +53 45 17.3 11.1 U Cas 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
ZTF J231308.58+534520.0,2461237.6668,11.14,0.05,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
ZTF J231308.58+534520.0 20260716.1668 11.14CV 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 07 16.1668 2461237.6668 10.60 23:46:35.18 +51:42:26.9
112.81682 -9.88608 galactic Cas Second-epoch detections are separated by 0.5" 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 1945016110828646912 | 23:46:35.08 +51:42:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:35.18 +51:42:26.9: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:35.18 +51:42:26.9: 13.74 +/- 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!
TCP 2026 07 16.1668* 23 46 35.18 +51 42 26.9 10.6 U Cas 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 1945016110828646912,2461237.6668,10.60,0.05,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 1945016110828646912 20260716.1668 10.60CV 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 07 16.1668 2461237.6668 10.54 00:13:40.77 +56:53:47.7
117.76819 -5.59612 galactic Cas Second-epoch detections are separated by 0.5" 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 | ATO J003.4030+56.9099 | 00:13:37.40 +56:53:50.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.766+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:40.77 +56:53:47.7: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:40.77 +56:53:47.7: 13.37 +/- 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!
TCP 2026 07 16.1668* 00 13 40.77 +56 53 47.7 10.5 U Cas 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
ATO J003.4030+56.9099,2461237.6668,10.54,0.05,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
ATO J003.4030+56.9099 20260716.1668 10.54CV 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 07 16.1668 2461237.6668 10.64 23:15:49.25 +52:24:22.8
108.48473 -7.76268 galactic And Second-epoch detections are separated by 1.8" 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 1992259170540322432 | 23:15:47.60 +52:24:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.216+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:49.25 +52:24:22.8: 12.11 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:49.25 +52:24:22.8: 12.12 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.11 +/- 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!
TCP 2026 07 16.1668* 23 15 49.25 +52 24 22.8 10.6 U And 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 1992259170540322432,2461237.6668,10.64,0.05,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 1992259170540322432 20260716.1668 10.64CV 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 07 16.1668 2461237.6668 10.32 00:13:38.81 +51:49:34.7
117.00751 -10.61020 galactic Cas Second-epoch detections are separated by 0.8" and 6.2 pix
The object was found in VSX14" Gaia DR3 395791720350917888
Type: ROT
# Max. Min./Amp. JD0 Period
11.700 G 11.750 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:38.81 +51:49:34.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:38.81 +51:49:34.7: 13.56 +/- 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!
TCP 2026 07 16.1668* 00 13 38.81 +51 49 34.7 10.3 U Cas 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 395791720350917888,2461237.6668,10.32,0.05,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 395791720350917888 20260716.1668 10.32CV 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 07 16.1668 2461237.6668 9.97 23:50:25.89 +49:51:13.6
112.95297 -11.83225 galactic Cas Second-epoch detections are separated by 1.6" 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 1940880469640450304 | 23:50:26.96 +49:51:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.045+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:25.89 +49:51:13.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:25.89 +49:51:13.6: 13.59 +/- 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!
TCP 2026 07 16.1668* 23 50 25.89 +49 51 13.6 10.0 U Cas 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 1940880469640450304,2461237.6668,9.97,0.05,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 1940880469640450304 20260716.1668 9.97CV 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 07 16.1668 2461237.6668 9.63 00:15:19.60 +53:12:03.2
117.46669 -9.28724 galactic Cas Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX 1" Gaia DR3 419244578251557888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.410 G 11.480 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:19.60 +53:12:03.2: 13.26 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.60 +53:12:03.2: 13.15 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.21 +/- 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!
TCP 2026 07 16.1668* 00 15 19.60 +53 12 03.2 9.6 U Cas 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 419244578251557888,2461237.6668,9.63,0.05,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 419244578251557888 20260716.1668 9.63CV 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 07 16.1668 2461237.6668 10.79 00:14:30.57 +53:45:36.6
117.42583 -8.71632 galactic Cas Second-epoch detections are separated by 2.2" and 6.0 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 | ATO J003.6140+53.7732 | 00:14:31.08 +53:46:21.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1927AnHar.100...33C HD 232142 J-Ks=0.848+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:30.57 +53:45:36.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:30.57 +53:45:36.6: 13.57 +/- 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!
TCP 2026 07 16.1668* 00 14 30.57 +53 45 36.6 10.8 U Cas 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
ATO J003.6140+53.7732,2461237.6668,10.79,0.05,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 J003.6140+53.7732 20260716.1668 10.79CV 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 07 16.1668 2461237.6668 11.52 23:12:17.84 +57:05:07.9
109.74326 -3.22574 galactic Cas Second-epoch detections are separated by 0.6" 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 | ATO J348.0943+57.0885 | 23:12:22.53 +57:04:44.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4II 2018MNRAS.475.2003D IRAS 23101+5648
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.84 +57:05:07.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.84 +57:05:07.9: 13.40 +/- 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!
TCP 2026 07 16.1668* 23 12 17.84 +57 05 07.9 11.5 U Cas 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
ATO J348.0943+57.0885,2461237.6668,11.52,0.05,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 J348.0943+57.0885 20260716.1668 11.52CV 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 07 16.1668 2461237.6668 11.58 23:19:32.19 +55:36:23.6
110.14530 -4.96700 galactic Cas Second-epoch detections are separated by 0.9" 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 1996916972372159360 | 23:19:35.92 +55:36:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:32.19 +55:36:23.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:32.19 +55:36:23.6: 13.59 +/- 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!
TCP 2026 07 16.1668* 23 19 32.19 +55 36 23.6 11.6 U Cas 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 1996916972372159360,2461237.6668,11.58,0.05,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 1996916972372159360 20260716.1668 11.58CV 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 07 16.1668 2461237.6668 11.28 00:22:45.20 +50:51:08.7
118.31460 -11.76199 galactic Cas Second-epoch detections are separated by 0.4" and 6.3 pix
The object was found in VSX 2" WISE J002245.1+505109
Type: EW
# Max. Min./Amp. JD0 Period
13.633 g Y 0.402 g 2458358.92060 0.489835600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:45.20 +50:51:08.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:45.20 +50:51:08.7: 13.60 +/- 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!
TCP 2026 07 16.1668* 00 22 45.20 +50 51 08.7 11.3 U Cas 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
WISE J002245.1+505109,2461237.6668,11.28,0.05,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
WISE J002245.1+505109 20260716.1668 11.28CV 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 07 16.1668 2461237.6668 11.70 23:11:51.54 +55:18:28.8
109.01867 -4.85084 galactic Cas Second-epoch detections are separated by 3.1" and 7.2 pix
The object was found in VSX 4" Gaia DR3 1996757100812082688
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.560 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.54 +55:18:28.8: 13.61 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.54 +55:18:28.8: 13.27 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.22
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!
TCP 2026 07 16.1668* 23 11 51.54 +55 18 28.8 11.7 U Cas 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 1996757100812082688,2461237.6668,11.70,0.05,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 1996757100812082688 20260716.1668 11.70CV 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 07 16.1668 2461237.6668 11.69 23:29:24.32 +51:40:00.0
110.21668 -9.16840 galactic Cas Second-epoch detections are separated by 7.9" 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 | target | 23:29:24.32 +51:40:00.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.32 +51:40:00.0: 13.10 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:24.32 +51:40:00.0: 12.75 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.89 +/- 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!
TCP 2026 07 16.1668* 23 29 24.32 +51 40 00.0 11.7 U Cas 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
target,2461237.6668,11.69,0.05,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
target 20260716.1668 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 07 16.1668 2461237.6668 11.74 23:37:39.15 +55:12:19.8
112.46854 -6.16020 galactic Cas Second-epoch detections are separated by 1.0" 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 1997488104243041024 | 23:37:38.28 +55:12:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.184+/-0.039 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:39.15 +55:12:19.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:39.15 +55:12:19.8: 13.58 +/- 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!
TCP 2026 07 16.1668* 23 37 39.15 +55 12 19.8 11.7 U Cas 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 1997488104243041024,2461237.6668,11.74,0.05,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 1997488104243041024 20260716.1668 11.74CV 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 07 16.1668 2461237.6668 11.52 00:26:37.43 +54:30:45.2
119.29824 -8.18403 galactic Cas Second-epoch detections are separated by 1.5" and 5.9 pix
The object was found in VSX 2" Gaia DR3 419605596020621824
Type: ROT
# Max. Min./Amp. JD0 Period
13.590 G 13.610 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:37.43 +54:30:45.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:37.43 +54:30:45.2: 13.48 +/- 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!
TCP 2026 07 16.1668* 00 26 37.43 +54 30 45.2 11.5 U Cas 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 419605596020621824,2461237.6668,11.52,0.05,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 419605596020621824 20260716.1668 11.52CV 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 07 16.1668 2461237.6668 11.69 23:57:00.38 +53:44:34.8
114.84894 -8.27232 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J359.2312+53.7452 | 23:57:00.38 +53:44:34.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:00.38 +53:44:34.8: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:00.38 +53:44:34.8: 13.40 +/- 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!
TCP 2026 07 16.1668* 23 57 00.38 +53 44 34.8 11.7 U Cas 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
ATO J359.2312+53.7452,2461237.6668,11.69,0.05,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
ATO J359.2312+53.7452 20260716.1668 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 07 16.1668 2461237.6668 11.65 00:04:53.69 +51:59:43.9
115.68261 -10.21990 galactic Cas Second-epoch detections are separated by 0.7" 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 | ATO J001.2174+52.0011 | 00:04:53.69 +51:59:43.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.69 +51:59:43.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:53.69 +51:59:43.9: 13.62 +/- 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!
TCP 2026 07 16.1668* 00 04 53.69 +51 59 43.9 11.7 U Cas 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
ATO J001.2174+52.0011,2461237.6668,11.65,0.05,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 J001.2174+52.0011 20260716.1668 11.65CV 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 07 16.1668 2461237.6668 11.90 23:42:43.15 +51:24:46.3
112.14988 -10.01456 galactic Cas Second-epoch detections are separated by 2.2" 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 | ATO J355.6820+51.4157 | 23:42:43.15 +51:24:46.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.525+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:43.15 +51:24:46.3: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:43.15 +51:24:46.3: 13.71 +/- 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!
TCP 2026 07 16.1668* 23 42 43.15 +51 24 46.3 11.9 U Cas 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
ATO J355.6820+51.4157,2461237.6668,11.90,0.05,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
ATO J355.6820+51.4157 20260716.1668 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 07 16.1668 2461237.6668 11.79 23:34:08.27 +54:02:57.5
111.64088 -7.11916 galactic Cas Second-epoch detections are separated by 3.2" and 6.3 pix
The object was found in VSX 0" Gaia DR3 1994286807419596416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.630 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.27 +54:02:57.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.27 +54:02:57.5: 13.48 +/- 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!
TCP 2026 07 16.1668* 23 34 08.27 +54 02 57.5 11.8 U Cas 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 1994286807419596416,2461237.6668,11.79,0.05,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 1994286807419596416 20260716.1668 11.79CV 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 07 16.1668 2461237.6668 11.70 00:25:03.29 +52:04:19.4
118.81302 -10.58857 galactic Cas Second-epoch detections are separated by 2.9" and 6.7 pix
The object was found in VSX24" Gaia DR3 418893730956548864
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.770 G K
ATTENTION: measured mag 11.70 is 4.0 mag brighter than the VSX record maximum brightness 15.73 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:03.29 +52:04:19.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:03.29 +52:04:19.4: 13.21 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.25
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!
TCP 2026 07 16.1668* 00 25 03.29 +52 04 19.4 11.7 U Cas 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 418893730956548864,2461237.6668,11.70,0.05,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 418893730956548864 20260716.1668 11.70CV 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 07 16.1668 2461237.6668 12.11 23:46:00.50 +49:54:17.9
112.26083 -11.60625 galactic Cas Second-epoch detections are separated by 3.5" 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 1943509058346454656 | 23:46:00.08 +49:53:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:00.50 +49:54:17.9: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:00.50 +49:54:17.9: 13.68 +/- 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!
TCP 2026 07 16.1668* 23 46 00.50 +49 54 17.9 12.1 U Cas 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 1943509058346454656,2461237.6668,12.11,0.05,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 1943509058346454656 20260716.1668 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 07 16.1668 2461237.6668 12.13 23:55:27.56 +53:24:40.0
114.55022 -8.54719 galactic Cas Second-epoch detections are separated by 1.5" 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 | ATO J358.8870+53.4264 | 23:55:29.79 +53:25:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.038 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:27.56 +53:24:40.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:27.56 +53:24:40.0: 13.62 +/- 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!
TCP 2026 07 16.1668* 23 55 27.56 +53 24 40.0 12.1 U Cas 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
ATO J358.8870+53.4264,2461237.6668,12.13,0.05,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
ATO J358.8870+53.4264 20260716.1668 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 07 16.1668 2461237.6668 11.91 00:18:40.02 +52:56:35.1
117.93535 -9.61044 galactic Cas Second-epoch detections are separated by 1.4" 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 | target | 00:18:40.02 +52:56:35.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:40.02 +52:56:35.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:40.02 +52:56:35.1: 13.49 +/- 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!
TCP 2026 07 16.1668* 00 18 40.02 +52 56 35.1 11.9 U Cas 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
target,2461237.6668,11.91,0.05,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
target 20260716.1668 11.91CV 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 07 16.1668 2461237.6668 12.04 00:08:05.74 +52:31:35.1
116.26710 -9.78356 galactic Cas Second-epoch detections are separated by 2.2" 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 | ATO J002.0283+52.5431 | 00:08:08.06 +52:32:08.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.414+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:05.74 +52:31:35.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:05.74 +52:31:35.1: 13.57 +/- 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!
TCP 2026 07 16.1668* 00 08 05.74 +52 31 35.1 12.0 U Cas 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
ATO J002.0283+52.5431,2461237.6668,12.04,0.05,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
ATO J002.0283+52.5431 20260716.1668 12.04CV 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 07 16.1668 2461237.6668 12.19 00:11:51.24 +52:56:51.6
116.90584 -9.46031 galactic Cas Second-epoch detections are separated by 1.5" and 6.0 pix
The object was found in VSX 2" Gaia DR3 395958158922096768
Type: ROT
# Max. Min./Amp. JD0 Period
14.370 G 14.400 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:51.24 +52:56:51.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:51.24 +52:56:51.6: 13.59 +/- 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!
TCP 2026 07 16.1668* 00 11 51.24 +52 56 51.6 12.2 U Cas 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 395958158922096768,2461237.6668,12.19,0.05,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 395958158922096768 20260716.1668 12.19CV 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 07 16.1668 2461237.6668 12.24 00:24:13.88 +56:20:39.1
119.14547 -6.32740 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 00:24:13.88 +56:20:39.1 (user input) | T | P | (position from user input) J-Ks=0.139+/-0.051 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:13.88 +56:20:39.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:13.88 +56:20:39.1: 13.54 +/- 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!
TCP 2026 07 16.1668* 00 24 13.88 +56 20 39.1 12.2 U Cas 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
target,2461237.6668,12.24,0.05,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
target 20260716.1668 12.24CV 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 07 16.1668 2461237.6668 12.14 00:29:16.41 +53:37:28.2
119.60702 -9.10410 galactic Cas 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 419538663249899520 | 00:29:16.76 +53:36:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:29:16.41 +53:37:28.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:29:16.41 +53:37:28.2: 13.45 +/- 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!
TCP 2026 07 16.1668* 00 29 16.41 +53 37 28.2 12.1 U Cas 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 419538663249899520,2461237.6668,12.14,0.05,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 419538663249899520 20260716.1668 12.14CV 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 07 16.1668 2461237.6668 10.92 23:21:12.04 +50:00:11.9
108.41729 -10.30819 galactic And Second-epoch detections are separated by 0.8" and 6.8 pix
The object was found in VSX 4" AK And
Type: M
# Max. Min./Amp. JD0 Period
10.000 V < 15.000 V 2452930.00000 317.000000000000 S:
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:12.04 +50:00:11.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:12.04 +50:00:11.9: 13.47 +/- 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!
TCP 2026 07 16.1668* 23 21 12.04 +50 00 11.9 10.9 U And 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
AK And,2461237.6668,10.92,0.05,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
AK And 20260716.1668 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461237.66711568 16.07.2026 04:00:28.795 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 11 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): 21602
Objects passed selection criteria: 21551
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 18210
Average stars matched: 17259.5 (94.7803 %)
Memory usage VmPeak: 131332 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 15 23:07:50 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: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461237.66711568 16.07.2026 04:00:28.795 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 221
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 247 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): 162533
Objects passed selection criteria: 162162
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 145212
Average stars matched: 138353 (95.2767 %)
Memory usage VmPeak: 1938876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 15 23:16:22 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 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.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: 2461237.66652512
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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Image size: 939.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.716 +53:59:59.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.716 +53:59:59.05
Angular distance between the image centers 0.0228 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Image size: 939.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.159 +54:00:36.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.159 +54:00:36.86
Angular distance between the image centers 0.0141 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 00:00:02.716 +53:59:59.05
Second-epoch second image center 00:00:02.159 +54:00:36.86
Angular distance between the image centers 0.01059 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.yGsnaOUYDs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.1UxZwIDKrU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits &> /tmp/tmp.2f2pqILN6p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits &> /tmp/tmp.uioOzQId4I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 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 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
ERROR: only 52 of 28951 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.18%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.575300
a=0.000000 b=1.000000 c=22.575300
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 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 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
Read 32399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0011 to 359.9996 deg, Dec +48.2682 to +59.2618 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 0.0011 to 359.9996 deg, Dec 48.2682 to 59.2618 deg
Loaded 153285 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): 56 out of 62 total matches.
Matched with Tycho-2 62 out of 32399 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.0 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yGsnaOUYDs (6) ############
Parsing command line arguments...
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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0821 through 0 to 14.9840, gap 14.9840 to 345.0821
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 235 matched stars entering correct_measured_positions(), 5819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.02"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0724 through 0 to 15.0101, gap 15.0101 to 345.0724
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 401 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 345 matched stars entering correct_measured_positions(), 5883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.97"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.85"
Excluding outliers - 341 stars left (next iteration limit 258)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.000 sigma_q1_arcsec=26.458 sigma_q2_arcsec=26.280 sigma_q3_arcsec=7.321 sigma_q4_arcsec=8.000 n_q1=41 n_q2=24 n_q3=122 n_q4=154 worst_quadrant_to_overall_ratio=2.646
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1UxZwIDKrU (6) ############
Parsing command line arguments...
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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3204, bad_region=7312, passed=32399
Got 32399 stars (including 22421 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 32399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0823 through 0 to 14.9840, gap 14.9840 to 345.0823
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 320 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 234 matched stars entering correct_measured_positions(), 171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 6406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0732 through 0 to 15.0096, gap 15.0096 to 345.0732
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 399 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 343 matched stars entering correct_measured_positions(), 6467 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.48"
Accuracy estimation diagnostic: 340 matched stars entering correct_measured_positions(), 9572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.44"
Excluding outliers - 340 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=340 sigma_overall_arcsec=11.206 sigma_q1_arcsec=29.679 sigma_q2_arcsec=28.591 sigma_q3_arcsec=8.393 sigma_q4_arcsec=9.911 n_q1=41 n_q2=25 n_q3=115 n_q4=159 worst_quadrant_to_overall_ratio=2.649
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2f2pqILN6p (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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1253, bad_region=2987, passed=15978
Got 15978 stars (including 11924 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 15978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010441 (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
RA wraps around 0/360 boundary: field RA 344.8485 through 0 to 14.6560, gap 14.6560 to 344.8485
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8479 through 0 to 14.6562, gap 14.6562 to 344.8479
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits N_match=968 sigma_overall_arcsec=0.672 sigma_q1_arcsec=0.671 sigma_q2_arcsec=0.666 sigma_q3_arcsec=0.734 sigma_q4_arcsec=0.604 n_q1=319 n_q2=179 n_q3=284 n_q4=186 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uioOzQId4I (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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1238, bad_region=3012, passed=16126
Got 16126 stars (including 12049 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat
util/solve_plate_with_UCAC5 got 16126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010441 (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
RA wraps around 0/360 boundary: field RA 344.8484 through 0 to 14.6557, gap 14.6557 to 344.8484
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13466 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8480 through 0 to 14.6562, gap 14.6562 to 344.8480
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13466 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13466 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits N_match=973 sigma_overall_arcsec=0.670 sigma_q1_arcsec=0.663 sigma_q2_arcsec=0.627 sigma_q3_arcsec=0.775 sigma_q4_arcsec=0.627 n_q1=319 n_q2=179 n_q3=291 n_q4=184 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits sigma_overall=10.000 worst_q_ratio=2.646
ref2=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits sigma_overall=11.206 worst_q_ratio=2.649
new1=fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits sigma_overall=0.672 worst_q_ratio=1.091
new2=fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits sigma_overall=0.670 worst_q_ratio=1.157
reference average sigma_overall=10.603 worst_q_ratio=2.6475
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (341 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.98 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450_astrometric_residuals.png (340 matched stars from wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.94 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068_astrometric_residuals.png (968 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.61 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33557_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 33557_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:36:32.44 +52:37:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 21482_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:44:31.94 +56:34:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 07077_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:09:36.52 +51:34:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 06239_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:58:25.02 +51:23:24.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cas-04-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 ####
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 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Image size: 939.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.716 +53:59:59.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.716 +53:59:59.05
Angular distance between the image centers 0.0228 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Image size: 939.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.159 +54:00:36.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.159 +54:00:36.86
Angular distance between the image centers 0.0141 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 00:00:02.716 +53:59:59.05
Second-epoch second image center 00:00:02.159 +54:00:36.86
Angular distance between the image centers 0.01059 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.IzI7s8eQDK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.T0yhGmOc2m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits &> /tmp/tmp.LawRozjWiN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits &> /tmp/tmp.BDnUNWXobn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 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 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
ERROR: only 104 of 200953 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.05%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.521000
a=0.000000 b=1.000000 c=20.521000
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.21
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 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 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=4.7)
Read 213202 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9999 deg, Dec +48.2308 to +59.2649 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 0.0002 to 359.9999 deg, Dec 48.2308 to 59.2649 deg
Loaded 153847 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): 122 out of 166 total matches.
Matched with Tycho-2 166 out of 213202 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 184 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.0 pix fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
13.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
13.3 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
12.6 mag. fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
12.6 mag. fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.0 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.IzI7s8eQDK (6) ############
Parsing command line arguments...
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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=29230, bad_region=30798, passed=200893
Got 200893 stars (including 144443 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 200893 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0121 through 0 to 15.0290, gap 15.0290 to 345.0121
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 42039 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0161 through 0 to 15.0639, gap 15.0639 to 345.0161
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 402 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 42110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.32"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 65834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.71"
Excluding outliers - 341 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.173 sigma_q1_arcsec=28.653 sigma_q2_arcsec=29.926 sigma_q3_arcsec=7.272 sigma_q4_arcsec=10.943 n_q1=31 n_q2=26 n_q3=117 n_q4=167 worst_quadrant_to_overall_ratio=2.942
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.T0yhGmOc2m (6) ############
Parsing command line arguments...
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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=33709, bad_region=29431, passed=213150
Got 213150 stars (including 154424 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 213150 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0123 through 0 to 15.0317, gap 15.0317 to 345.0123
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 319 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 46390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0158 through 0 to 15.0663, gap 15.0663 to 345.0158
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 46448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.44"
Accuracy estimation diagnostic: 332 matched stars entering correct_measured_positions(), 66751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.69"
Excluding outliers - 332 stars left (next iteration limit 249)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=332 sigma_overall_arcsec=11.113 sigma_q1_arcsec=28.693 sigma_q2_arcsec=26.729 sigma_q3_arcsec=8.129 sigma_q4_arcsec=9.837 n_q1=36 n_q2=26 n_q3=118 n_q4=152 worst_quadrant_to_overall_ratio=2.582
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LawRozjWiN (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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=45, blended=13363, bad_region=20232, passed=135648
Got 135648 stars (including 103361 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 135648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010441 (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
RA wraps around 0/360 boundary: field RA 344.8485 through 0 to 14.7932, gap 14.7932 to 344.8485
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 118498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8478 through 0 to 14.7933, gap 14.7933 to 344.8478
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 118498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 118498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits N_match=976 sigma_overall_arcsec=0.672 sigma_q1_arcsec=0.666 sigma_q2_arcsec=0.613 sigma_q3_arcsec=0.731 sigma_q4_arcsec=0.605 n_q1=315 n_q2=199 n_q3=271 n_q4=191 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BDnUNWXobn (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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=52, blended=13582, bad_region=20004, passed=134711
Got 134711 stars (including 102414 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat
util/solve_plate_with_UCAC5 got 134711 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010441 (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
RA wraps around 0/360 boundary: field RA 344.7824 through 0 to 14.7929, gap 14.7929 to 344.7824
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 117892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.7820 through 0 to 14.7932, gap 14.7932 to 344.7820
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 117892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 117891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits N_match=976 sigma_overall_arcsec=0.651 sigma_q1_arcsec=0.637 sigma_q2_arcsec=0.603 sigma_q3_arcsec=0.756 sigma_q4_arcsec=0.607 n_q1=309 n_q2=196 n_q3=269 n_q4=202 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/wcs_fd_Cas-04-Q2b1x1_2026-07-15_22-59-37_20.00sec_4.90C_LIGHT_0068.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.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_2026-07-15_CI_Cas-04-Q2b1x1_230353_TTUQ2b1x1_3286505_dcYV1tFb/wcs_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:18.42 +55:48:27.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:30.02 +53:59:26.2: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:34.20 +49:54:02.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:50.78 +54:41:26.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:20.19 +55:33:16.2: 12.89 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:56.75 +55:53:17.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:58.84 +55:38:50.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:01.27 +53:17:43.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:37.75 +51:19:43.7: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:40.19 +56:02:28.1: 12.23 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:58.84 +55:38:50.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:50.78 +54:41:26.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:20.19 +55:33:16.2: 12.87 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:37.75 +51:19:43.7: 13.59 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:56.75 +55:53:17.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:18.42 +55:48:27.4: 13.59 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.88 +/- 0.12
Forced photometry reference-image weighted average: 13.59 +/- 0.32
Forced photometry filter REJECTED candidate at 00:12:20.19 +55:33:16.2: ref_mag=12.88 +/- 0.12 new_mean_mag=12.2417 delta=0.64 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:30.02 +53:59:26.2: 13.71 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 00:18:37.75 +51:19:43.7: ref_mag=13.59 +/- 0.32 new_mean_mag=12.1722 delta=1.41 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:40.19 +56:02:28.1: 12.37 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:34.20 +49:54:02.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:01.27 +53:17:43.5: 13.64 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.28 +/- 0.09
Forced photometry filter REJECTED candidate at 23:11:40.19 +56:02:28.1: ref_mag=12.28 +/- 0.09 new_mean_mag=12.4032 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:13.96 +53:46:20.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:41.64 +52:23:12.3: 13.23 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:13.96 +53:46:20.4: 13.18 +/- 0.26 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:41.64 +52:23:12.3: 12.80 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.26
Forced photometry reference-image weighted average: 12.96 +/- 0.13
Forced photometry filter KEPT candidate at 23:55:13.96 +53:46:20.4: ref_mag=13.18 +/- 0.26 new_mean_mag=12.1969 delta=0.98 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:45:41.64 +52:23:12.3: ref_mag=12.96 +/- 0.13 new_mean_mag=12.2093 delta=0.75 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:42.94 +51:00:33.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:42.94 +51:00:33.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:00.28 +52:55:22.2: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:00.28 +52:55:22.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:04.43 +55:22:25.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:04.43 +55:22:25.9: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:36.07 +56:58:36.4: 13.52 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:36.07 +56:58:36.4: 12.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.16
Forced photometry filter KEPT candidate at 23:59:36.07 +56:58:36.4: ref_mag=13.09 +/- 0.16 new_mean_mag=12.1773 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:34.11 +52:53:24.6: 13.10 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:14.85 +52:45:10.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:34.11 +52:53:24.6: 12.82 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.12
Forced photometry filter KEPT candidate at 00:19:34.11 +52:53:24.6: ref_mag=12.94 +/- 0.12 new_mean_mag=11.9617 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:29.55 +54:54:32.3: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:14.85 +52:45:10.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:29.55 +54:54:32.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:11.05 +53:50:49.3: 13.19 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:24.91 +55:00:14.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:11.05 +53:50:49.3: 12.77 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.13
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:24.91 +55:00:14.9: 13.65 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 23:53:11.05 +53:50:49.3: ref_mag=12.92 +/- 0.13 new_mean_mag=11.8386 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:14.33 +56:13:57.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:14.33 +56:13:57.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.64 +57:16:14.5: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:47.64 +57:16:14.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:30.58 +56:06:45.2: 12.61 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:30.58 +56:06:45.2: 12.23 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.09
Forced photometry filter REJECTED candidate at 00:31:30.58 +56:06:45.2: ref_mag=12.37 +/- 0.09 new_mean_mag=11.8179 delta=0.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:08.51 +52:31:38.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:08.51 +52:31:38.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:30.99 +50:48:52.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:26.77 +56:34:44.4: 12.50 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:30.99 +50:48:52.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:26.77 +56:34:44.4: 12.21 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.08
Forced photometry filter REJECTED candidate at 23:39:26.77 +56:34:44.4: ref_mag=12.34 +/- 0.08 new_mean_mag=11.9484 delta=0.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:49.08 +57:58:47.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:49.08 +57:58:47.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:46.39 +53:03:07.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:46.39 +53:03:07.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:55.05 +55:20:53.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:55.05 +55:20:53.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:51.68 +54:39:57.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:51.68 +54:39:57.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:46.90 +55:53:57.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:46.90 +55:53:57.1: 13.15 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.24
Forced photometry filter KEPT candidate at 23:24:46.90 +55:53:57.1: ref_mag=13.15 +/- 0.24 new_mean_mag=11.9399 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:21.52 +51:55:19.5: 12.93 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:21.52 +51:55:19.5: 12.76 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.11
Forced photometry filter KEPT candidate at 23:52:21.52 +51:55:19.5: ref_mag=12.84 +/- 0.11 new_mean_mag=11.9001 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:33.90 +56:38:57.1: 11.88 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:33.90 +56:38:57.1: 11.41 +/- 0.12 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.09
Forced photometry filter REJECTED candidate at 23:57:33.90 +56:38:57.1: ref_mag=11.60 +/- 0.09 new_mean_mag=11.7297 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:32.20 +55:18:28.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:58.69 +52:34:39.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:03.30 +56:42:13.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:32.20 +55:18:28.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:58.69 +52:34:39.0: 13.56 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.33
Forced photometry filter KEPT candidate at 00:20:58.69 +52:34:39.0: ref_mag=13.56 +/- 0.33 new_mean_mag=11.6660 delta=1.89 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:03.30 +56:42:13.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:45.59 +53:37:26.0: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:45.59 +53:37:26.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:36.34 +53:24:29.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:36.34 +53:24:29.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:58.58 +56:46:21.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:58.58 +56:46:21.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:04.42 +52:11:06.4: 9.88 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:04.42 +52:11:06.4: 9.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.67 +/- 0.01
Forced photometry filter REJECTED candidate at 23:36:04.42 +52:11:06.4: ref_mag=9.67 +/- 0.01 new_mean_mag=11.7604 delta=-2.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:28.05 +52:04:55.1: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:28.05 +52:04:55.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:34.57 +51:28:31.2: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:34.57 +51:28:31.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:06.05 +56:05:25.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:00.10 +57:25:00.0: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:06.05 +56:05:25.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:00.10 +57:25:00.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:50.64 +54:41:18.1: 13.40 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:50.64 +54:41:18.1: 13.06 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.18
Forced photometry filter KEPT candidate at 23:44:50.64 +54:41:18.1: ref_mag=13.20 +/- 0.18 new_mean_mag=11.7153 delta=1.49 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:56.79 +54:08:49.4: 12.49 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:56.79 +54:08:49.4: 12.54 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.09
Forced photometry filter REJECTED candidate at 23:12:56.79 +54:08:49.4: ref_mag=12.51 +/- 0.09 new_mean_mag=11.6382 delta=0.87 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:34.80 +54:54:40.0: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:14.64 +56:43:01.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:34.80 +54:54:40.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:14.64 +56:43:01.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:03.46 +50:48:21.9: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:12.79 +52:40:51.0: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:52.97 +56:58:23.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:03.46 +50:48:21.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:12.79 +52:40:51.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:52.97 +56:58:23.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:22.92 +53:52:58.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:44.16 +55:58:25.8: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:22.92 +53:52:58.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:44.16 +55:58:25.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:54.36 +53:26:45.9: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:54.36 +53:26:45.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:30.09 +57:44:09.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:30.09 +57:44:09.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:37.90 +57:55:02.8: 10.65 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:37.90 +57:55:02.8: 10.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.02
Forced photometry filter REJECTED candidate at 00:30:37.90 +57:55:02.8: ref_mag=10.53 +/- 0.02 new_mean_mag=11.2871 delta=-0.76 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:38.03 +50:04:08.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:36.32 +51:31:27.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:38.03 +50:04:08.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:36.32 +51:31:27.3: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:40.64 +56:24:48.5: 12.09 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:40.64 +56:24:48.5: 11.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.05
Forced photometry filter REJECTED candidate at 23:56:40.64 +56:24:48.5: ref_mag=11.97 +/- 0.05 new_mean_mag=11.3386 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:46.86 +54:35:20.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:46.86 +54:35:20.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:16.27 +56:06:05.2: 12.02 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:16.27 +56:06:05.2: 11.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.05
Forced photometry filter REJECTED candidate at 23:47:16.27 +56:06:05.2: ref_mag=11.98 +/- 0.05 new_mean_mag=11.1670 delta=0.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.56 +53:54:04.5: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:12.39 +52:26:37.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:28.18 +56:13:38.2: 10.54 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.56 +53:54:04.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:12.39 +52:26:37.9: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:28.18 +56:13:38.2: 10.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:28.18 +56:13:38.2: ref_mag=10.38 +/- 0.01 new_mean_mag=11.2454 delta=-0.87 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:20.65 +54:44:21.4: 13.59 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:20.65 +54:44:21.4: 13.14 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.19
Forced photometry filter KEPT candidate at 00:06:20.65 +54:44:21.4: ref_mag=13.30 +/- 0.19 new_mean_mag=11.0493 delta=2.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:28.33 +54:40:59.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:28.33 +54:40:59.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:34.53 +54:31:30.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:34.53 +54:31:30.9: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:21.97 +55:46:41.8: 8.44 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:21.97 +55:46:41.8: 8.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.27 +/- 0.00
Forced photometry filter REJECTED candidate at 00:26:21.97 +55:46:41.8: ref_mag=8.27 +/- 0.00 new_mean_mag=10.7802 delta=-2.51 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:15.65 +55:15:12.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:15.65 +55:15:12.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:08.57 +53:45:17.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:08.57 +53:45:17.3: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:35.18 +51:42:26.9: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:40.77 +56:53:47.7: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:35.18 +51:42:26.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:40.77 +56:53:47.7: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:49.25 +52:24:22.8: 12.11 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:38.81 +51:49:34.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:49.25 +52:24:22.8: 12.12 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.07
Forced photometry filter KEPT candidate at 23:15:49.25 +52:24:22.8: ref_mag=12.11 +/- 0.07 new_mean_mag=10.6378 delta=1.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:38.81 +51:49:34.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:25.89 +49:51:13.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:25.89 +49:51:13.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:19.60 +53:12:03.2: 13.26 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.60 +53:12:03.2: 13.15 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.16
Forced photometry filter KEPT candidate at 00:15:19.60 +53:12:03.2: ref_mag=13.21 +/- 0.16 new_mean_mag=9.6180 delta=3.59 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:30.57 +53:45:36.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:30.57 +53:45:36.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.84 +57:05:07.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:32.19 +55:36:23.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.84 +57:05:07.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:32.19 +55:36:23.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:45.20 +50:51:08.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:45.20 +50:51:08.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.54 +55:18:28.8: 13.61 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.54 +55:18:28.8: 13.27 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.22
Forced photometry filter KEPT candidate at 23:11:51.54 +55:18:28.8: ref_mag=13.40 +/- 0.22 new_mean_mag=11.6989 delta=1.71 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.32 +51:40:00.0: 13.10 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:24.32 +51:40:00.0: 12.75 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.12
Forced photometry filter KEPT candidate at 23:29:24.32 +51:40:00.0: ref_mag=12.89 +/- 0.12 new_mean_mag=11.6853 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:39.15 +55:12:19.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:39.15 +55:12:19.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:37.43 +54:30:45.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:37.43 +54:30:45.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:00.38 +53:44:34.8: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:00.38 +53:44:34.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.69 +51:59:43.9: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:53.69 +51:59:43.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:43.15 +51:24:46.3: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.27 +54:02:57.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:43.15 +51:24:46.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.27 +54:02:57.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:03.29 +52:04:19.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:03.29 +52:04:19.4: 13.21 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.25
Forced photometry filter KEPT candidate at 00:25:03.29 +52:04:19.4: ref_mag=13.21 +/- 0.25 new_mean_mag=11.6974 delta=1.51 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:00.50 +49:54:17.9: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:00.50 +49:54:17.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:27.56 +53:24:40.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:27.56 +53:24:40.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:40.02 +52:56:35.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:18:40.02 +52:56:35.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:05.74 +52:31:35.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:05.74 +52:31:35.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:35.50 +55:59:47.6: 11.06 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:35.50 +55:59:47.6: 10.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.02
Forced photometry filter REJECTED candidate at 00:12:35.50 +55:59:47.6: ref_mag=10.83 +/- 0.02 new_mean_mag=12.0842 delta=-1.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:51.24 +52:56:51.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:51.24 +52:56:51.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:22.88 +57:16:57.7: 7.22 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:22.88 +57:16:57.7: 7.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 7.10 +/- 0.00
Forced photometry filter REJECTED candidate at 00:05:22.88 +57:16:57.7: ref_mag=7.10 +/- 0.00 new_mean_mag=12.2320 delta=-5.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:13.88 +56:20:39.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:13.88 +56:20:39.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:29:16.41 +53:37:28.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:29:16.41 +53:37:28.2: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:12.04 +50:00:11.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:12.04 +50:00:11.9: 13.47 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out235717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out235432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25587.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 111s
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: 79s
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Considering the candidate 235432_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235432_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235447_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235447_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235454_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235454_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235464_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235464_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235471_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235471_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
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Considering the candidate 235477_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235477_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235481_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235481_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
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Considering the candidate 235501_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235501_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235507_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235507_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235509_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235509_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235510_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235510_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235529_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235529_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
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Considering the candidate 235532_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235532_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235534_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235534_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235535_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235535_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235547_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235547_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:43:41.88 +57:55:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235551_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235551_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:28:47.59 +54:01:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235556_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235556_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235561_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235561_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235563_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235563_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235567_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235567_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
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Considering the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235573_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235573_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:58:35.04 +54:07:52.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235579_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235579_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:11:34.27 +54:31:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235583_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235583_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235584_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235584_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235588_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235588_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235589_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235589_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235604_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235604_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:21:59.10 +57:17:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235606_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235606_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235613_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235613_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235618_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235618_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235627_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235627_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235630_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235630_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235637_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235637_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235641_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235641_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:15:34.32 +52:21:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235643_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235643_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235650_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235650_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235651_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235651_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235655_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235655_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235657_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235657_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235658_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235658_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235661_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235661_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235670_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235670_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235681_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:24:57.12 +54:22:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235682_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235682_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235688_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235688_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235694_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235694_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:29:32.03 +55:19:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235696_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235696_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235697_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235697_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235705_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 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 235711_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235711_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235714_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235714_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235716_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235716_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235717_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235717_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:21:14.64 +56:43:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 2.460 1997301496504605440 350.31089527865 +56.71762546693 12.1889 10.8057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 235718_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235718_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:27:46.34 +55:49:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235719_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235719_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235722_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235722_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235728_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235728_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235739_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235739_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235745_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235745_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235749_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235749_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:29:40.19 +57:40:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235750_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 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 235751_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235751_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235756_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:57:16.07 +56:30:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235759_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235759_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235763_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235763_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235769_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235769_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235774_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235774_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235775_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235775_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:08:45.58 +53:03:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235776_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235776_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235778_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235778_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:04:21.92 +51:49:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235780_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235780_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:45:59.07 +56:53:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235781_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235781_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:19:58.57 +52:48:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235788_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235788_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:08:01.92 +52:27:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235799_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235799_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:21:22.53 +54:40:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235801_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235801_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:01:36.30 +52:04:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235806_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235806_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235808_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235808_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235811_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235811_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235812_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235812_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:28:12.74 +50:35:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235815_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235815_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:25:16.13 +53:39:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235824_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235824_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:55:04.11 +54:11:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235827_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235827_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235829_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235829_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:06:20.92 +56:11:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235836_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235836_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235839_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235839_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235841_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235841_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235842_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235842_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235845_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235845_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235850_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235850_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:23:58.36 +52:05:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235852_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235852_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:51:56.60 +53:07:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235854_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235854_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235859_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235859_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235862_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235862_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235867_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235867_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235869_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235869_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:14:07.45 +51:33:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235872_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 235872_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235876_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235876_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:56:37.48 +54:36:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235877_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 235877_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:46:46.61 +51:02:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236258_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236258_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:13:11.49 +57:10:45.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236382_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236382_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:20:34.10 +52:06:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236435_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236435_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236516_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236516_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:22:51.05 +52:21:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236524_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236524_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:43:18.25 +50:54:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236547_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236547_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:57:58.37 +50:27:10.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236567_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236567_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:23:25.75 +55:49:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236576_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236576_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:11:16.68 +50:50:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236607_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236607_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:28:21.02 +54:48:22.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236611_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236611_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:27:19.43 +49:58:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236631_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236631_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:41:07.32 +51:33:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236634_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236634_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:59:00.17 +54:43:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236644_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236644_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:17:34.87 +49:43:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236658_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236658_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:18:03.78 +49:50:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236666_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236666_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236695_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236695_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236699_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236699_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:58:51.61 +54:42:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236700_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236700_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:31:40.46 +54:09:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236706_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236706_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:20:12.47 +50:06:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236719_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236719_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:24:57.66 +53:01:58.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236721_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236721_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:13:03.14 +49:56:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236723_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236723_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:59:00.37 +53:16:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236730_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236730_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:29:50.10 +54:38:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236733_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236733_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236742_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236742_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236761_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236761_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:47:42.16 +56:51:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236767_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236767_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:52:01.74 +50:05:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236774_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236774_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:11:49.40 +54:49:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236775_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236775_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:44:02.05 +51:36:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236793_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236793_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:37:53.18 +50:55:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236799_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236799_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236846_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236846_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:12:07.25 +53:36:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236874_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236874_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:31:37.41 +56:54:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236875_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236875_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:44:49.37 +50:34:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236883_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236883_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:20:15.40 +57:50:03.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236891_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236891_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:02:24.79 +55:25:33.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236906_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236906_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:31:16.72 +57:14:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236915_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236915_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:48:26.42 +54:40:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236924_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 236924_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236962_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236962_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:12:36.50 +57:12:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236972_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 236972_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:24:30.71 +56:57:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237001_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237001_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:36:14.96 +49:55:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237006_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237006_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237023_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237023_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:50:23.35 +54:12:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237050_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237050_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237060_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237060_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:55:33.17 +52:42:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237071_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237071_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:22:46.37 +56:26:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237073_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237073_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:19:49.05 +50:46:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237082_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237082_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237085_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237085_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:54:44.61 +53:43:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237102_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237102_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:55:54.10 +54:53:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237117_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237117_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:14:16.48 +56:52:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237138_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237138_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237142_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237142_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237147_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237147_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:51:04.21 +51:22:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237150_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237150_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:55:06.98 +56:11:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237162_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237162_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:02:26.94 +54:33:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237168_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237168_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237192_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237192_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:11:59.57 +54:08:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237201_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237201_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:51:27.98 +51:30:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237291_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237291_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:54:31.67 +54:58:35.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237305_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237305_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:06:05.05 +51:22:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237315_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237315_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237320_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237320_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237359_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237359_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237387_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237387_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237402_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237402_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237427_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237427_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:18:22.05 +54:10:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237445_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237445_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237472_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 237472_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237500_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237500_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237519_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 237519_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:09:36.50 +51:34:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 179100_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:15:50.79 +57:32:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17108_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 17108_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
Rejecting candidate due to large distance (39.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 23:44:31.92 +56:34:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64302_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069
The candidate 64302_fd_Cas-04-Q2b1x1_2026-07-15_23-00-28_20.00sec_5.00C_LIGHT_0069 did not pass the final checks
**** FOUND 00:02:27.13 +52:33:52.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 26s
make_report_in_HTML.sh TOTAL: 216s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:01:30.02 +53:59:26.2
23:45:18.42 +55:48:27.4
00:23:01.27 +53:17:43.5
23:49:50.78 +54:41:26.6
00:18:37.75 +51:19:43.7
00:10:34.20 +49:54:02.1
00:12:56.75 +55:53:17.1
23:43:58.84 +55:38:50.0
23:55:13.96 +53:46:20.4
23:28:42.94 +51:00:33.2
00:05:00.28 +52:55:22.2
00:31:04.43 +55:22:25.9
23:59:36.07 +56:58:36.4
00:19:34.11 +52:53:24.6
23:46:14.85 +52:45:10.9
23:53:29.55 +54:54:32.3
23:53:11.05 +53:50:49.3
00:11:24.91 +55:00:14.9
00:07:14.33 +56:13:57.4
23:45:47.64 +57:16:14.5
00:12:08.51 +52:31:38.4
00:18:30.99 +50:48:52.0
00:15:49.08 +57:58:47.2
23:36:46.39 +53:03:07.6
00:25:55.05 +55:20:53.6
23:41:51.68 +54:39:57.7
23:24:46.90 +55:53:57.1
23:52:21.52 +51:55:19.5
23:39:32.20 +55:18:28.7
00:20:58.69 +52:34:39.0
00:23:03.30 +56:42:13.9
00:15:45.59 +53:37:26.0
00:09:36.34 +53:24:29.2
23:32:58.58 +56:46:21.5
23:41:28.05 +52:04:55.1
23:46:34.57 +51:28:31.2
00:19:06.05 +56:05:25.3
00:31:00.10 +57:25:00.0
23:44:50.64 +54:41:18.1
00:06:34.80 +54:54:40.0
23:50:03.46 +50:48:21.9
23:30:12.79 +52:40:51.0
23:36:52.97 +56:58:23.1
23:51:22.92 +53:52:58.6
23:18:44.16 +55:58:25.8
00:24:54.36 +53:26:45.9
00:24:30.09 +57:44:09.1
00:23:38.03 +50:04:08.1
00:27:36.32 +51:31:27.3
23:21:46.86 +54:35:20.2
23:58:38.56 +53:54:04.5
23:15:12.39 +52:26:37.9
00:06:20.65 +54:44:21.4
23:29:28.33 +54:40:59.2
23:18:34.53 +54:31:30.9
00:06:15.65 +55:15:12.0
23:13:08.57 +53:45:17.3
23:46:35.18 +51:42:26.9
00:13:40.77 +56:53:47.7
23:15:49.25 +52:24:22.8
00:13:38.81 +51:49:34.7
23:50:25.89 +49:51:13.6
00:15:19.60 +53:12:03.2
00:14:30.57 +53:45:36.6
23:12:17.84 +57:05:07.9
23:19:32.19 +55:36:23.6
00:22:45.20 +50:51:08.7
23:11:51.54 +55:18:28.8
23:29:24.32 +51:40:00.0
23:37:39.15 +55:12:19.8
00:26:37.43 +54:30:45.2
23:57:00.38 +53:44:34.8
00:04:53.69 +51:59:43.9
23:42:43.15 +51:24:46.3
23:34:08.27 +54:02:57.5
00:25:03.29 +52:04:19.4
23:46:00.50 +49:54:17.9
23:55:27.56 +53:24:40.0
00:18:40.02 +52:56:35.1
00:08:05.74 +52:31:35.1
00:11:51.24 +52:56:51.6
00:24:13.88 +56:20:39.1
00:29:16.41 +53:37:28.2
23:21:12.04 +50:00:11.9
########### Completed Cas-04-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 ####
00:01:30.02 +53:59:26.2
23:45:18.42 +55:48:27.4
00:23:01.27 +53:17:43.5
23:49:50.78 +54:41:26.6
00:18:37.75 +51:19:43.7
00:10:34.20 +49:54:02.1
00:12:56.75 +55:53:17.1
23:43:58.84 +55:38:50.0
23:55:13.96 +53:46:20.4
23:28:42.94 +51:00:33.2
00:05:00.28 +52:55:22.2
00:31:04.43 +55:22:25.9
23:59:36.07 +56:58:36.4
00:19:34.11 +52:53:24.6
23:46:14.85 +52:45:10.9
23:53:29.55 +54:54:32.3
23:53:11.05 +53:50:49.3
00:11:24.91 +55:00:14.9
00:07:14.33 +56:13:57.4
23:45:47.64 +57:16:14.5
00:12:08.51 +52:31:38.4
00:18:30.99 +50:48:52.0
00:15:49.08 +57:58:47.2
23:36:46.39 +53:03:07.6
00:25:55.05 +55:20:53.6
23:41:51.68 +54:39:57.7
23:24:46.90 +55:53:57.1
23:52:21.52 +51:55:19.5
23:39:32.20 +55:18:28.7
00:20:58.69 +52:34:39.0
00:23:03.30 +56:42:13.9
00:15:45.59 +53:37:26.0
00:09:36.34 +53:24:29.2
23:32:58.58 +56:46:21.5
23:41:28.05 +52:04:55.1
23:46:34.57 +51:28:31.2
00:19:06.05 +56:05:25.3
00:31:00.10 +57:25:00.0
23:44:50.64 +54:41:18.1
00:06:34.80 +54:54:40.0
23:50:03.46 +50:48:21.9
23:30:12.79 +52:40:51.0
23:36:52.97 +56:58:23.1
23:51:22.92 +53:52:58.6
23:18:44.16 +55:58:25.8
00:24:54.36 +53:26:45.9
00:24:30.09 +57:44:09.1
00:23:38.03 +50:04:08.1
00:27:36.32 +51:31:27.3
23:21:46.86 +54:35:20.2
23:58:38.56 +53:54:04.5
23:15:12.39 +52:26:37.9
00:06:20.65 +54:44:21.4
23:29:28.33 +54:40:59.2
23:18:34.53 +54:31:30.9
00:06:15.65 +55:15:12.0
23:13:08.57 +53:45:17.3
23:46:35.18 +51:42:26.9
00:13:40.77 +56:53:47.7
23:15:49.25 +52:24:22.8
00:13:38.81 +51:49:34.7
23:50:25.89 +49:51:13.6
00:15:19.60 +53:12:03.2
00:14:30.57 +53:45:36.6
23:12:17.84 +57:05:07.9
23:19:32.19 +55:36:23.6
00:22:45.20 +50:51:08.7
23:11:51.54 +55:18:28.8
23:29:24.32 +51:40:00.0
23:37:39.15 +55:12:19.8
00:26:37.43 +54:30:45.2
23:57:00.38 +53:44:34.8
00:04:53.69 +51:59:43.9
23:42:43.15 +51:24:46.3
23:34:08.27 +54:02:57.5
00:25:03.29 +52:04:19.4
23:46:00.50 +49:54:17.9
23:55:27.56 +53:24:40.0
00:18:40.02 +52:56:35.1
00:08:05.74 +52:31:35.1
00:11:51.24 +52:56:51.6
00:24:13.88 +56:20:39.1
00:29:16.41 +53:37:28.2
23:21:12.04 +50:00:11.9
###################################################################################
00:01:30.02 +53:59:26.2 -- not an asteroid (will add it to exclusion list)
23:45:18.42 +55:48:27.4 -- not an asteroid (will add it to exclusion list)
00:23:01.27 +53:17:43.5 -- not an asteroid (will add it to exclusion list)
23:49:50.78 +54:41:26.6 -- not an asteroid (will add it to exclusion list)
00:18:37.75 +51:19:43.7 -- not an asteroid (will add it to exclusion list)
00:10:34.20 +49:54:02.1 -- not an asteroid (will add it to exclusion list)
00:12:56.75 +55:53:17.1 -- not an asteroid (will add it to exclusion list)
23:43:58.84 +55:38:50.0 -- not an asteroid (will add it to exclusion list)
23:55:13.96 +53:46:20.4 -- not an asteroid (will add it to exclusion list)
23:28:42.94 +51:00:33.2 -- not an asteroid (will add it to exclusion list)
00:05:00.28 +52:55:22.2 -- not an asteroid (will add it to exclusion list)
00:31:04.43 +55:22:25.9 -- not an asteroid (will add it to exclusion list)
23:59:36.07 +56:58:36.4 -- not an asteroid (will add it to exclusion list)
00:19:34.11 +52:53:24.6 -- not an asteroid (will add it to exclusion list)
23:46:14.85 +52:45:10.9 -- not an asteroid (will add it to exclusion list)
23:53:29.55 +54:54:32.3 -- not an asteroid (will add it to exclusion list)
23:53:11.05 +53:50:49.3 -- not an asteroid (will add it to exclusion list)
00:11:24.91 +55:00:14.9 -- not an asteroid (will add it to exclusion list)
00:07:14.33 +56:13:57.4 -- not an asteroid (will add it to exclusion list)
23:45:47.64 +57:16:14.5 -- not an asteroid (will add it to exclusion list)
00:12:08.51 +52:31:38.4 -- not an asteroid (will add it to exclusion list)
00:18:30.99 +50:48:52.0 -- not an asteroid (will add it to exclusion list)
00:15:49.08 +57:58:47.2 -- not an asteroid (will add it to exclusion list)
23:36:46.39 +53:03:07.6 -- not an asteroid (will add it to exclusion list)
00:25:55.05 +55:20:53.6 -- not an asteroid (will add it to exclusion list)
23:41:51.68 +54:39:57.7 -- not an asteroid (will add it to exclusion list)
23:24:46.90 +55:53:57.1 -- not an asteroid (will add it to exclusion list)
23:52:21.52 +51:55:19.5 -- not an asteroid (will add it to exclusion list)
23:39:32.20 +55:18:28.7 -- not an asteroid (will add it to exclusion list)
00:20:58.69 +52:34:39.0 -- not an asteroid (will add it to exclusion list)
00:23:03.30 +56:42:13.9 -- not an asteroid (will add it to exclusion list)
00:15:45.59 +53:37:26.0 -- not an asteroid (will add it to exclusion list)
00:09:36.34 +53:24:29.2 -- not an asteroid (will add it to exclusion list)
23:32:58.58 +56:46:21.5 -- not an asteroid (will add it to exclusion list)
23:41:28.05 +52:04:55.1 -- not an asteroid (will add it to exclusion list)
23:46:34.57 +51:28:31.2 -- not an asteroid (will add it to exclusion list)
00:19:06.05 +56:05:25.3 -- not an asteroid (will add it to exclusion list)
00:31:00.10 +57:25:00.0 -- not an asteroid (will add it to exclusion list)
23:44:50.64 +54:41:18.1 -- not an asteroid (will add it to exclusion list)
00:06:34.80 +54:54:40.0 -- not an asteroid (will add it to exclusion list)
23:50:03.46 +50:48:21.9 -- not an asteroid (will add it to exclusion list)
23:30:12.79 +52:40:51.0 -- not an asteroid (will add it to exclusion list)
23:36:52.97 +56:58:23.1 -- not an asteroid (will add it to exclusion list)
23:51:22.92 +53:52:58.6 -- not an asteroid (will add it to exclusion list)
23:18:44.16 +55:58:25.8 -- not an asteroid (will add it to exclusion list)
00:24:54.36 +53:26:45.9 -- not an asteroid (will add it to exclusion list)
00:24:30.09 +57:44:09.1 -- not an asteroid (will add it to exclusion list)
00:23:38.03 +50:04:08.1 -- not an asteroid (will add it to exclusion list)
00:27:36.32 +51:31:27.3 -- not an asteroid (will add it to exclusion list)
23:21:46.86 +54:35:20.2 -- not an asteroid (will add it to exclusion list)
23:58:38.56 +53:54:04.5 -- not an asteroid (will add it to exclusion list)
23:15:12.39 +52:26:37.9 -- not an asteroid (will add it to exclusion list)
00:06:20.65 +54:44:21.4 -- not an asteroid (will add it to exclusion list)
23:29:28.33 +54:40:59.2 -- not an asteroid (will add it to exclusion list)
23:18:34.53 +54:31:30.9 -- not an asteroid (will add it to exclusion list)
00:06:15.65 +55:15:12.0 -- not an asteroid (will add it to exclusion list)
23:13:08.57 +53:45:17.3 -- not an asteroid (will add it to exclusion list)
23:46:35.18 +51:42:26.9 -- not an asteroid (will add it to exclusion list)
00:13:40.77 +56:53:47.7 -- not an asteroid (will add it to exclusion list)
23:15:49.25 +52:24:22.8 -- not an asteroid (will add it to exclusion list)
00:13:38.81 +51:49:34.7 -- not an asteroid (will add it to exclusion list)
23:50:25.89 +49:51:13.6 -- not an asteroid (will add it to exclusion list)
00:15:19.60 +53:12:03.2 -- not an asteroid (will add it to exclusion list)
00:14:30.57 +53:45:36.6 -- not an asteroid (will add it to exclusion list)
23:12:17.84 +57:05:07.9 -- not an asteroid (will add it to exclusion list)
23:19:32.19 +55:36:23.6 -- not an asteroid (will add it to exclusion list)
00:22:45.20 +50:51:08.7 -- not an asteroid (will add it to exclusion list)
23:11:51.54 +55:18:28.8 -- not an asteroid (will add it to exclusion list)
23:29:24.32 +51:40:00.0 -- not an asteroid (will add it to exclusion list)
23:37:39.15 +55:12:19.8 -- not an asteroid (will add it to exclusion list)
00:26:37.43 +54:30:45.2 -- not an asteroid (will add it to exclusion list)
23:57:00.38 +53:44:34.8 -- not an asteroid (will add it to exclusion list)
00:04:53.69 +51:59:43.9 -- not an asteroid (will add it to exclusion list)
23:42:43.15 +51:24:46.3 -- not an asteroid (will add it to exclusion list)
23:34:08.27 +54:02:57.5 -- not an asteroid (will add it to exclusion list)
00:25:03.29 +52:04:19.4 -- not an asteroid (will add it to exclusion list)
23:46:00.50 +49:54:17.9 -- not an asteroid (will add it to exclusion list)
23:55:27.56 +53:24:40.0 -- not an asteroid (will add it to exclusion list)
00:18:40.02 +52:56:35.1 -- not an asteroid (will add it to exclusion list)
00:08:05.74 +52:31:35.1 -- not an asteroid (will add it to exclusion list)
00:11:51.24 +52:56:51.6 -- not an asteroid (will add it to exclusion list)
00:24:13.88 +56:20:39.1 -- not an asteroid (will add it to exclusion list)
00:29:16.41 +53:37:28.2 -- not an asteroid (will add it to exclusion list)
23:21:12.04 +50:00:11.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:30.02 +53:59:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:53.69 +51:59:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:00.28 +52:55:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:15.65 +55:15:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:20.65 +54:44:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:34.80 +54:54:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:14.33 +56:13:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:05.74 +52:31:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:36.34 +53:24:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:34.20 +49:54:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:24.91 +55:00:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:51.24 +52:56:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:08.51 +52:31:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:56.75 +55:53:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:38.81 +51:49:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:40.77 +56:53:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:30.57 +53:45:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:19.60 +53:12:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:45.59 +53:37:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:49.08 +57:58:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:30.99 +50:48:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:37.75 +51:19:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:40.02 +52:56:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:06.05 +56:05:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:34.11 +52:53:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:58.69 +52:34:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:45.20 +50:51:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:01.27 +53:17:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:03.30 +56:42:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:38.03 +50:04:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:13.88 +56:20:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:30.09 +57:44:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:54.36 +53:26:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:03.29 +52:04:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:55.05 +55:20:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:37.43 +54:30:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:36.32 +51:31:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:16.41 +53:37:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:00.10 +57:25:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:04.43 +55:22:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:51.54 +55:18:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:17.84 +57:05:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:08.57 +53:45:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:12.39 +52:26:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:49.25 +52:24:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:34.53 +54:31:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:44.16 +55:58:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:32.19 +55:36:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:12.04 +50:00:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:46.86 +54:35:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:46.90 +55:53:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:42.94 +51:00:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:24.32 +51:40:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:28.33 +54:40:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:12.79 +52:40:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:58.58 +56:46:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:08.27 +54:02:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:46.39 +53:03:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:52.97 +56:58:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:39.15 +55:12:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:32.20 +55:18:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:28.05 +52:04:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:51.68 +54:39:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:43.15 +51:24:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:58.84 +55:38:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:50.64 +54:41:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:18.42 +55:48:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:47.64 +57:16:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:00.50 +49:54:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:14.85 +52:45:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:34.57 +51:28:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:35.18 +51:42:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:50.78 +54:41:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:03.46 +50:48:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:25.89 +49:51:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:22.92 +53:52:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:21.52 +51:55:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:11.05 +53:50:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:29.55 +54:54:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:13.96 +53:46:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:27.56 +53:24:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:00.38 +53:44:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:38.56 +53:54:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:36.07 +56:58:36.4 -- 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)
00:01:30.02 +53:59:26.2 -- not a known variable star
00:04:53.69 +51:59:43.9 -- not a known variable star
00:05:00.28 +52:55:22.2 -- not a known variable star
00:06:15.65 +55:15:12.0 -- a known variable star
00:06:20.65 +54:44:21.4 -- not a known variable star
00:06:34.80 +54:54:40.0 -- not a known variable star
00:07:14.33 +56:13:57.4 -- not a known variable star
00:08:05.74 +52:31:35.1 -- not a known variable star
00:09:36.34 +53:24:29.2 -- not a known variable star
00:10:34.20 +49:54:02.1 -- a known variable star
00:11:24.91 +55:00:14.9 -- not a known variable star
00:11:51.24 +52:56:51.6 -- a known variable star
00:12:08.51 +52:31:38.4 -- a known variable star
00:12:56.75 +55:53:17.1 -- not a known variable star
00:13:38.81 +51:49:34.7 -- a known variable star
00:13:40.77 +56:53:47.7 -- not a known variable star
00:14:30.57 +53:45:36.6 -- not a known variable star
00:15:19.60 +53:12:03.2 -- a known variable star
00:15:45.59 +53:37:26.0 -- not a known variable star
00:15:49.08 +57:58:47.2 -- not a known variable star
00:18:30.99 +50:48:52.0 -- not a known variable star
00:18:37.75 +51:19:43.7 -- not a known variable star
00:18:40.02 +52:56:35.1 -- not a known variable star
00:19:06.05 +56:05:25.3 -- not a known variable star
00:19:34.11 +52:53:24.6 -- a known variable star
00:20:58.69 +52:34:39.0 -- not a known variable star
00:22:45.20 +50:51:08.7 -- a known variable star
00:23:01.27 +53:17:43.5 -- not a known variable star
00:23:03.30 +56:42:13.9 -- not a known variable star
00:23:38.03 +50:04:08.1 -- not a known variable star
00:24:13.88 +56:20:39.1 -- not a known variable star
00:24:30.09 +57:44:09.1 -- not a known variable star
00:24:54.36 +53:26:45.9 -- not a known variable star
00:25:03.29 +52:04:19.4 -- a known variable star
00:25:55.05 +55:20:53.6 -- not a known variable star
00:26:37.43 +54:30:45.2 -- a known variable star
00:27:36.32 +51:31:27.3 -- a known variable star
00:29:16.41 +53:37:28.2 -- not a known variable star
00:31:00.10 +57:25:00.0 -- a known variable star
00:31:04.43 +55:22:25.9 -- a known variable star
23:11:51.54 +55:18:28.8 -- a known variable star
23:12:17.84 +57:05:07.9 -- not a known variable star
23:13:08.57 +53:45:17.3 -- a known variable star
23:15:12.39 +52:26:37.9 -- not a known variable star
23:15:49.25 +52:24:22.8 -- not a known variable star
23:18:34.53 +54:31:30.9 -- not a known variable star
23:18:44.16 +55:58:25.8 -- a known variable star
23:19:32.19 +55:36:23.6 -- not a known variable star
23:21:12.04 +50:00:11.9 -- a known variable star
23:21:46.86 +54:35:20.2 -- not a known variable star
23:24:46.90 +55:53:57.1 -- not a known variable star
23:28:42.94 +51:00:33.2 -- not a known variable star
23:29:24.32 +51:40:00.0 -- not a known variable star
23:29:28.33 +54:40:59.2 -- a known variable star
23:30:12.79 +52:40:51.0 -- a known variable star
23:32:58.58 +56:46:21.5 -- a known variable star
23:34:08.27 +54:02:57.5 -- a known variable star
23:36:46.39 +53:03:07.6 -- not a known variable star
23:36:52.97 +56:58:23.1 -- a known variable star
23:37:39.15 +55:12:19.8 -- not a known variable star
23:39:32.20 +55:18:28.7 -- not a known variable star
23:41:28.05 +52:04:55.1 -- not a known variable star
23:41:51.68 +54:39:57.7 -- not a known variable star
23:42:43.15 +51:24:46.3 -- not a known variable star
23:43:58.84 +55:38:50.0 -- not a known variable star
23:44:50.64 +54:41:18.1 -- a known variable star
23:45:18.42 +55:48:27.4 -- not a known variable star
23:45:47.64 +57:16:14.5 -- not a known variable star
23:46:00.50 +49:54:17.9 -- not a known variable star
23:46:14.85 +52:45:10.9 -- not a known variable star
23:46:34.57 +51:28:31.2 -- not a known variable star
23:46:35.18 +51:42:26.9 -- not a known variable star
23:49:50.78 +54:41:26.6 -- not a known variable star
23:50:03.46 +50:48:21.9 -- not a known variable star
23:50:25.89 +49:51:13.6 -- not a known variable star
23:51:22.92 +53:52:58.6 -- not a known variable star
23:52:21.52 +51:55:19.5 -- not a known variable star
23:53:11.05 +53:50:49.3 -- not a known variable star
23:53:29.55 +54:54:32.3 -- not a known variable star
23:55:13.96 +53:46:20.4 -- not a known variable star
23:55:27.56 +53:24:40.0 -- not a known variable star
23:57:00.38 +53:44:34.8 -- not a known variable star
23:58:38.56 +53:54:04.5 -- not a known variable star
23:59:36.07 +56:58:36.4 -- a known variable star
Found 60 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
84 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 84 (excluding asteroids and hot pixels, 60 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)2461237.66652512 -observatory V36
07:17:00.13 +17:17:09.6 Mercury (4.8mag)
10:35:37.03 +10:04:07.5 Venus (-4.1mag)
04:41:24.65 +22:05:28.9 Mars (1.3mag)
08:21:58.16 +19:54:30.5 Jupiter (-1.8mag)
00:56:23.06 +03:22:04.8 Saturn (0.7mag)
04:08:18.67 +20:47:57.2 Uranus (5.8mag)
00:16:57.91 +00:19:58.1 Neptune (7.7mag)
20:30:22.37 -23:20:34.0 Pluto (14.4mag)
09:18:24.56 +16:00:00.1 Moon (-8.7mag)
-rw-r--r-- 1 apache apache 361 Jul 15 23:07 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461237.66652512:
08:22:01.87 +19:54:15.6 Io (6.1mag)
08:21:50.93 +19:54:58.4 Europa (6.3mag)
08:22:01.59 +19:54:21.8 Ganymede (5.6mag)
08:21:36.06 +19:55:51.7 Callisto (6.8mag)
08:20:14.15 +19:41:13.5 Himalia (15.7mag)
08:21:59.30 +19:54:26.9 Thebe (16.6mag)
08:19:34.90 +19:44:24.4 Elara (17.7mag)
08:25:40.62 +19:45:34.5 Pasiphae (17.9mag)
08:26:35.82 +20:00:27.4 Carme (19.0mag)
00:56:34.80 +03:21:48.6 Titan (8.5mag)
00:56:24.11 +03:21:49.8 Rhea (9.8mag)
00:55:48.30 +03:20:12.5 Iapetus (11.2mag)
00:56:09.97 +03:22:18.0 Hyperion (14.5mag)
00:56:16.02 +03:18:27.8 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 15 23:07 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.66652512:
17:55:31.48 -31:38:57.6 JWST
17:35:26.94 +39:31:39.3 Chandra
19:30:20.95 +06:06:13.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 15 23:07 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.66652512 -observatory V36
02:44:26.28 +15:06:19.0 17.8mag P/1996 R2 (Lagerkvist)
18:13:37.09 -34:30:16.5 13.8mag P/2010 H2 (Vales)
06:31:28.89 -68:14:30.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:48.18 +32:32:50.6 17.6mag C/2017 K2 (PANSTARRS)
02:18:22.99 +18:19:40.2 15.7mag P/2021 N1 (ZTF)
22:55:54.56 +32:15:08.0 17.3mag C/2022 E2 (ATLAS)
06:18:59.21 +26:52:13.0 16.7mag C/2022 N2 (PANSTARRS)
10:00:36.91 +29:31:10.4 16.9mag C/2022 QE78 (ATLAS)
09:13:30.58 +05:06:06.6 17.9mag C/2022 R6 (PANSTARRS)
18:03:44.95 +21:03:06.9 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.94 -11:31:44.0 17.7mag P/2023 B1 (PANSTARRS)
21:42:00.97 +67:32:27.7 17.8mag C/2023 H5 (Lemmon)
16:19:53.00 -10:40:54.7 14.0mag C/2023 R1 (PANSTARRS)
08:10:50.95 +66:01:42.7 17.9mag C/2024 A1 (ATLAS)
07:40:21.45 +30:17:37.4 14.8mag C/2024 E1 (Wierzchos)
15:13:40.21 +15:27:48.0 17.6mag C/2024 G6 (ATLAS)
19:33:47.25 +40:28:01.2 13.7mag C/2024 J3 (ATLAS)
21:41:19.00 +46:50:51.9 17.8mag C/2024 R4 (PANSTARRS)
04:55:05.11 -13:32:53.5 15.7mag C/2024 T5 (ATLAS)
06:39:19.89 +28:05:55.9 18.0mag C/2025 J1 (Borisov)
07:18:18.06 -13:25:34.7 16.8mag C/2025 R3 (PANSTARRS)
10:02:56.73 +22:10:41.3 17.6mag C/2025 V2 (Rankin)
12:46:41.51 +03:40:37.7 17.1mag C/2025 Y1 (ATLAS)
16:36:13.37 +79:09:38.2 17.2mag C/2026 A2 (Bok)
02:52:10.20 +45:28:59.3 16.8mag C/2026 B2 (Sun-Gao)
11:29:19.24 +05:32:04.3 17.0mag A/2026 E1
21:28:01.78 -17:15:39.2 7.1mag 10P/Tempel
11:16:15.06 -02:08:42.4 16.2mag 29P/Schwassmann-Wachmann
04:08:29.62 +30:10:39.3 17.9mag 47P/Ashbrook-Jackson
10:20:12.35 +12:09:03.9 17.1mag 63P/Wild
00:50:41.23 -05:02:52.9 15.5mag 65P/Gunn
04:41:26.15 +20:26:57.7 13.7mag 78P/Gehrels
02:31:30.91 +11:23:03.5 16.3mag 88P/Howell
06:52:41.82 +30:08:59.2 15.8mag 93P/Lovas
04:39:58.44 +31:18:17.8 16.7mag 114P/Wiseman-Skiff
08:22:54.04 +30:01:44.4 15.2mag 123P/West-Hartley
10:59:01.69 -01:10:19.1 16.9mag 124P/Mrkos
05:01:02.37 +20:57:54.4 16.2mag 128P/Shoemaker-Holt
05:47:10.44 +19:38:58.0 17.8mag 131P/Mueller
00:02:56.49 +03:08:34.8 17.9mag 139P/Vaisala-Oterma
07:34:29.70 +15:44:15.3 16.2mag 141P-D/Machholz
03:19:06.64 -20:38:27.3 15.2mag 161P/Hartley-IRAS
05:54:02.35 +35:07:23.7 15.4mag 162P/SidingSpring
18:47:16.49 +18:55:45.0 14.2mag 169P/NEAT
01:54:44.80 +08:12:46.5 17.6mag 220P/McNaught
16:35:30.41 -08:38:16.7 17.2mag 235P/LINEAR
08:57:28.81 +32:44:58.9 18.0mag 240P/NEAT
20:39:16.27 -50:46:00.9 17.8mag 259P/Garradd
02:15:39.33 +14:48:46.1 15.6mag 260P/McNaught
05:54:55.34 +37:15:51.0 17.4mag 295P/LINEAR
15:06:29.33 +05:31:33.2 17.6mag 391P/Kowalski
08:39:50.62 +19:26:11.1 17.9mag 450P/LONEOS
08:00:51.90 +38:43:48.9 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 15 23:07 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
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
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
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
-rw-r--r-- 1 apache apache 5.6K Jul 15 23:07 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 15 23:07 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:50:39.367 +12:02:04.48 AT 2026ssk 2026-06-23.30 21.04
21:28:51.588 -30:52:46.37 AT 2026ssj 2026-06-23.54 20.48
13:14:31.067 +38:32:01.92 AT 2026ssi 2026-06-11.32 19.048
00:23:13.025 -04:43:14.99 AT 2026ssh 2026-06-23.58 20.7
21:26:53.186 +04:17:24.51 AT 2026ssg 2026-06-23.48 20.92
22:34:24.397 -29:59:37.51 AT 2026ssf 2026-06-25.56 20.68
22:26:15.310 -27:42:10.55 AT 2026sse 2026-06-25.56 21.41
22:13:00.422 -28:48:04.48 AT 2026ssd 2026-06-25.55 21.47
22:13:31.243 -26:34:31.26 AT 2026ssc 2026-06-25.55 21.32
22:19:04.821 -24:39:28.70 AT 2026ssb 2026-06-25.56 20.53
12:00:29.299 +21:32:44.85 AT 2026ssa 2026-06-26.28 20.65
21:13:22.522 -05:45:33.06 AT 2026srz 2026-06-26.55 21.24
20:25:03.555 -06:07:40.73 AT 2026sry 2026-07-06.53 21.14
23:59:26.661 -08:45:47.98 AT 2026srx 2026-07-08.38 19.725
22:30:36.777 -00:06:36.54 AT 2026srw 2026-06-10.46 20.0846
22:24:20.174 +00:37:40.92 AT 2026srv 2026-07-08.42 19.8955
03:03:50.342 +03:47:14.56 AT 2026sru 2026-07-08.48 18.748
03:17:45.758 +01:39:35.34 AT 2026srt 2026-07-08.48 19.0953
22:40:48.893 -01:09:04.39 AT 2026srs 2026-07-08.39 19.4884
15:39:02.048 +07:51:43.65 AT 2026srr 2026-07-08.21 19.1495
-rw-r--r-- 1 apache apache 89K Jul 15 23:07 tns_transients_list.txt
