AAVSO Alert Notice 530 8,10. 2015 Nova Aql

  • Im Adler ist eine Nova gemeldet worden.


    AAVSO Alert Notice 530


    October 8, 2015


    Nova Aquilae 2015 = ASASSN 15-qd = PNV J19215012+1509248


    Event: Nova Aquilae 2015 = ASASSN 15-qd = PNV J19215012+1509248


    Independent discovery by:
    - Koichi Itagaki (Teppo-cho, Yamagata, Japan), reported by S. Nakano
    (Sumoto, Japan)
    - All-Sky Automated Survey for Supernovae (ASAS-SN,
    http://www.astronomy.ohio-state.edu/~assassin/index.shtml),
    reported by B. J. Shappee (Hubble Fellow, Carnegie Observatories) et al.


    Discovery magnitude:
    - Itagaki: 12.4 unfiltered, using a 0.21-m f/3.0 reflector
    - ASAS-SN: 15.2 V


    Discovery date:
    - Itagaki: 2015 October 5.548 UT
    - ASAS-SN: 2015 October 01.29 UT


    Coordinates (2000.0): R.A. 19 21 50.15 Dec. +15 09 24.8 (from VSX)


    Spectra: Originally reported as a U Gem-type dwarf nova, ASASSN-15qd
    was reclassified as a highly reddened classical nova based on
    spectroscopic observations obtained by M. Fujii (Okayama, Japan) on
    2015 October 5.598 UT and reported by H. Maehara (Okayama
    Astrophysical Observatory, NAOJ). Fujii's spectrum is posted at:
    http://tinyurl.com/qbllf74. Colin Littlefield (LCO, Middletown, CT)
    also confirmed the nature of ASASSN-15qd with his spectrum taken
    2015 October 6.06 UT (vsnet-alert 19121, vsnet-alert 19127). His
    spectrum is posted at:
    https://wesfiles.wesleyan.edu/…/…/_xy-e13874214_1-t_bcWE8JkG.


    Observing recommendations: This nova is faint, but observations of
    all types (visual, CCD, DSLR, spectroscopy) as instrumentation
    permits are strongly encouraged as this nova evolves.


    Charts: Charts for Nova Aql 2015 may be created using the AAVSO
    Variable Star Plotter (VSP) at http://www.aavso.org/vsp. Be sure to
    include spaces in the name as shown.


    Observations reported to the AAVSO (observations are via CBET 4147
    unless otherwise noted):
    2015 Sep. 05.37 UT, <17.5 V (Shappee et al., ASAS-SN, via ATel #8126,
    http://www.astronomerstelegram.org/?read=8126);
    09.28, <17.6 V (Shappee et al., ASAS-SN, via ATel #8126);
    12.35 UT, <17.2 V (Shappee et al., ASAS-SN);
    21.452, [12: (H. Maehara, Kamogata-Kiso-Kyoto Wide-field Survey (KWS);
    27.409, 10.5 Ic (T. Kojima, Gunma, Japan, prediscovery);
    29.31, 14.7 V (Shappee et al., ASAS-SN);
    29.451, 10.2 Ic (Maehara, KWS);
    29.451, <13.1 V (Maehara, KWS);
    Oct. 01.29, 15.2 V ±0.1 (Shappee et al., ASAS-SN);
    02.435, 10.5 Ic (Maehara);
    05.428, 10.9 Ic (Maehara);
    06.4145, 15.7: V (K. Hirosawa, Aichi, Japan; via Maehara, via CBET 4147);
    06.4155, 13.15 Rc (Hirosawa);
    06.4162, 10.97 Ic (Hirosawa);
    06.452 13.5 U (T. Noguchi, Chiba-ken, Japan);


    Submit observations: Please submit observations to the AAVSO
    International Database using the name NOVA AQL 2015. Be sure
    to include spaces in name as shown. Once a GCVS name has been
    assigned, please use that name.


    Notes:
    a. Announced in IAU Central Bureau for Astronomical Telegrams
    Central Bureau Electronic Telegram 4147 (Daniel W. E. Green, ed.).
    Assigned the name PNV J19215012+1509248 when posted to the IAU
    CBAT Transient Object Confirmation Page (TOCP) at
    http://www.cbat.eps.harvard.edu/unconf/tocp.html


    b. Although the ASAS-SN discovery image was obtained earlier,
    Itagaki's report was received at the Central Bureau for Astronomical
    Telegrams over half a day prior to Shappee et al.'s announcement in
    ATel #8126.


    c. Itagaki reports nothing visible at this location on his earlier
    images. Shappee et al. (ATel #8126) report nothing was seen at this
    location on ASAS-SN images taken 2015 September 12.35 UT and before,
    and that no previous outbursts are detected in the previous 52
    epochs of ASAS-SN data at this location since ASAS-SN started
    observing the Galactic plane in February 2015.


    d. Maehara et al. (ATel #8127, http://www.astronomerstelegram.org/?read=8127)
    report the nova was not detected on KWS (see above) Ic-band archival
    images 2013 May 12.777 - 2015 Sep 21.452 UT (typical limiting mag
    about Ic=12).


    e. T. Maccarone (Texas Tech University, ATel #8136,
    http://www.astronomerstelegram.org/?read=8136) reports that a
    search of the UKIDSS Galactic Plane Survey database yields an
    infrared counterpart at the position of the nova with K=17.1+-0.1.
    The source is UGPS J192150.15+150924.8 (Lucas et al. 2008, MNRAS,
    391, 136).


    f. Position end figures:
    - K. Itagaki (Teppo-cho, Yamagata, Japan), Oct. 5.557, 50.12s, 24.8"
    - T. Noguchi (Chiba-ken, Japan), 2015 Oct. 6.452 UT, 50.13s, 25.3"


    g. Images:
    - K. Itagaki (Teppo-cho, Yamagata, Japan), 2015 Oct. 5.548 UT,
    discovery image at http://tinyurl.com/pwrm9k2.
    - T. Noguchi (Chiba-ken, Japan), 2015 Oct. 6.452 UT:
    http://park8.wakwak.com/~ngc/images/ASASSN-15qd.jpg.


    This AAVSO Alert Notice was compiled by Elizabeth O. Waagen.

  • Hallo Frank,
    habe mir eine Karte der AAVSO ausgedruct (x 15407 AL), Helligk. 14.7 bis (22.0 V.
    Ich glaube, das kann ich mir "abschminken". Da müßte man hier mit bl. Auge schon 6mag sehen, damit ich im Dobson bei 304fach noch einigermaßen schätzen kann.
    Lassen wir uns überraschen....


    Gruß
    Guenther

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