PNV J17581670-2914490

Image:
Object: PNV J17581670-2914490
DATE-OBS: 2021-04-09T22:44:01.89
EXPTIME: 600.00 (seconds)
SUBFRMS: 20I/20R/20V
OBJCTRA: 17 58 16.70
OBJCTDEC: -29 14 49.00
Instrument:
Catalog: ATLAS
Bessell (B): +*.*, Bessell (V): +8.87*
Bessell (R): +7.92, Bessell (I): +7.07
CCD: ATIK-383L+
FILTERS: V/R/I
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora, K Arora
Remark:
Sky Clear.
End

VRI Image

Photometry: C/2021 R4 ATLAS

Image:
Object: C/2020 R4 ATLAS
DATE-OBS: 2021-04-02T22:59:39.4896
EXPTIME: 2040.00 (seconds)
SUBFRMS: 34
OBJCTRA: 19 42 07.77
OBJCTDEC: +00 00 51.90
Instrument:
Catalog: UCAC4
Bessell (B): +*.*, Bessell (V): +*.*
Bessell (R): +14.3, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear.
End

SN2021hiz/IC3322A

Image:
Object: SN2021hiz/IC3322A
DATE-OBS: 2021-04-04T17:28:28.060
EXPTIME: 4950.00 (seconds)
SUBFRMS: 55
OBJCTRA: 12 25 41.67
OBJCTDEC: +07 13 42.3
Instrument:
Catalog: ATLAS
Bessell (B): +*.*, Bessell (V): +*.*
Bessell (R): +14.0, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear, Star marked in blue box are ATLAS catalog data.
End

SN2021hpr/NGC3147

Image:
Object: SN2021hpr/NGC3147
DATE-OBS: 2021-04-04T16:44:14.22
EXPTIME: 1440.00 (seconds)
SUBFRMS: 16
OBJCTRA: 10 16 38.62
OBJCTDEC: +73 24 01.80
Instrument:
Catalog: ATLAS
Bessell (B): +*.*, Bessell (V): +*.*
Bessell (R): +15.7, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear, Star marked in blue box are ATLAS catalog data.
End

C/2020 R4 ATLAS

Image:
Object: C/2020 R4 ATLAS
DATE-OBS: 2021-04-02T22:59:39.4896
EXPTIME: 2040.00 (seconds)
SUBFRMS: 34
OBJCTRA: 19 42 07.77
OBJCTDEC: +00 00 51.90
Instrument:
Catalog: UCAC4
Bessell (B): +*.*, Bessell (V): +*.*
Bessell (R): +14.3, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear.
End

Video Link: https://www.youtube.com/watch?v=7_AREOFLgZo

C/2017 K2 (PANSTARRS)

Image:
Object: C/2017 K2 (PANSTARRS) 
DATE-OBS: 2021-04-02T22:02:41.0592
EXPTIME: 2460.00 (seconds)
SUBFRMS: 41
OBJCTRA: 18 28 03.73
OBJCTDEC: +39 34 45.90
Instrument:
Catalog: UCAC4
Bessell (B): +*.*, Bessell (V): +*.*
Bessell (R): +15.2, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Sky Clear.
End

Astrometry and Photometry of Globular Star Cluster M13

We examine the astrometry and photometry of globular star cluster M13 using Gaia EDR3 and ATLAS catalogs. The Gaia EDR3 catalog is for astrometry and ATLAS catalog is for high precession differential photometry. The software Tycho 8.0 supports both the catalogs upto +22.0 magnitudes. If stars are well resolved (imaged at higher focal length), the results will be promising.

Image:
Object: M13
DATE-OBS: 2021-03-27T20:56:25.69
EXPTIME: 1320.00 (seconds)
SUBFRMS: 22
OBJCTRA: 16 41 46.016
OBJCTDEC: +36 27 13.50
Instrument:
Catalog: Gaia EDR3 + ATLAS
Bessell (B): +*.*, Bessell (V): +*.*
Bessell (R): +*.*, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
High Moon, Sky Clear.
End

The offline variant, “GRAPPA”, was developed by Marc Serrau.
Please also include the following acknowledgements if using the catalog in a published paper:

Acknowledgements:

  • Marc Serrau
  • ESA GAIA Mission as GRAPPA3 has made use of data from the European Space Agency
    (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing
    and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium).

The acknowledgements for ALTAS catalog, to be used when publishing a paper, are as follows:
This work has made use of data from the Asteroid Terrestrial-impact Last Alert System (ATLAS) project.
ATLAS is primarily funded to search for near earth asteroids through NASA grants NN12AR55G, 80NSSC18K0284,
and 80NSSC18K1575; byproducts of the NEO search include images and catalogs from the survey area.
The ATLAS science products have been made possible through the contributions of the University of Hawaii
Institute for Astronomy, the Queen’s University Belfast, the Space Telescope Science Institute,
and the South African Astronomical Observatory.

References:
Tonry, J.L., Denneau, L., Flewelling, H., Heinze, A.N., Onken, C.A., Smartt, S.J., Stalder, B., Weiland,
H.J., Wolf, C. (2018). “The ATLAS All-Sky Stellar Reference Catalog.” Astrophys. J. 867, A105.
Kostov, A., Bonev, T. (2017). “Transformation of Pan-STARRS1 gri to Stetson BVRI magnitudes.
Photometry of small bodies observations.” Bulgarian Astron. J. 28, 3 (AriXiv:1706.06147v2).

Comet C/2020 T2 (Palomar)

Image:
Object: Comet C/2020 T2 (Palomar)
DATE-OBS: 2021-03-21T21:25:26
EXPTIME: 1800.00 (seconds)
SUBFRMS: 30
OBJCTRA: 14 06 59.539
OBJCTDEC: +33 32 45.144
Instrument:
Catalog: UCAC4
Bessell (B): +*.*, Bessell (V): +15.0
Bessell (R): +14.8, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: R
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho, Astrometrica
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Average Seeing, Sky Clear.
End

AT2021gmj/NGC3310

Image:
Object: AT2021gmj/NGC3310
DATE-OBS: 2021-03-21T16:06:19.9344
EXPTIME: 1800.00 (seconds)
SUBFRMS: 30
OBJCTRA: 10 38 52.764
OBJCTDEC: +53 29 32.96
Instrument:
Catalog: UCAC4
Bessell (B): +*.*, Bessell (V): +15.0
Bessell (R): +*.*, Bessell (I): +*.*
CCD: ATIK-383L+
FILTERS: V
TELESCOPE: C11, 1623.0mm
PRiSMv10, Tycho
Site:
ORIGIN: Cepheid Observatory, India, Vorion Scientific, India
SITELAT: +24:55:00:00
SITELONG:+75:33:58:99
Observers:
V.K.Agnihotri, B. Kumar, S. Mahawar, K.Vora
Remark:
Average Seeing, Sky Clear.
End

International Churyumov readings “CAMMAC-2020”

Our minimal contribution appeared here!. International Churyumov readings “CAMMAC-2020”.

THE DISINTEGRATIONS OF COMETATLAS BY OBSERVATIONS IN TAJIKISTAN AND INDIA:

G.I.Kokhirova1, О.V.Ivanova2,3,4, F.Dzh.Rakhmatullaeva1,S.Borysenko3, V.K.Agnihotri5, A.M. Buriev1.1. Institute of Astrophysics of the National Academy of Sciences of Tajikistan,2. Astronomical Institute of the Slovak Academy of Sciences,3. Main astronomical observatory of the National Academy of Sciences of Ukraine,4. Astronomical Observatory named after T. ShevchenkoKyiv National University5. Cepheid Observatory, Rawabhata Via Kota,Raj, India

E-mail:rahmat.firuza@gmail.com

Long-period comet C/2019Y4 (Atlas) discovered 28 on December 2019, has passed the perihelion on May 31, 2020.At the end of March 2020, observations by the Hubble Space Telescope were registered the disintegrations ofthe comet’s nucleus into several fragments. To study the nuclear fragmentation observations of comet C/2019Y4(Atlas)in the Cepheid Observatory of India, the International Astronomical Observatory Sanglokh (IAOS)and the Hissar Astronomical Observatory (HissAO) of the Institute of Astrophysics of the National Academy of Science of Tajikistanwere out carried in March-April 2020.Some physical properties of the main nucleus fragment were evaluated using the photometric measurements of comet images.These data confirm the disintegrations of the comet’s nucleus. The coordinates of the comet were determined, the orbit was calculated.and it was shown that the disintegration of the nucleus did not affect the stability of the orbit of the main.Key words: comet, photometry, light curve, astrometry, nucleus, coordinates, orbit. Page35/36 https://cammac.univ.kiev.ua/book-of-abstracts