From owner-vsnet-campaign@kusastro.kyoto-u.ac.jp Tue Aug 8 03:01 JST 2000 To: vsnet-campaign cc: uemura Date: Tue, 08 Aug 2000 02:50:26 +0900 From: Makoto Uemura <uemura@kusastro.kyoto-u.ac.jp> X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24] Subject: [vsnet-campaign 414] VSNET Weekly Campaign Summary Content-Type: text Content-Length: 8967 VSNET Weekly Campaign Summary *** Last week news *** (new targets) V730 Sgr (RA = 19h23m00s.79, Dec = -28d29'29".2) As report by Williams in [vsnet-alert 5167], the suspected dwarf nova V730 Sgr was in outburst (13.6mag on August 4). The first outburst reported to VSNET was in 1998 May, by Stubbings (mv=13.8) (vsnet-campaign 409). The data observed by N. Butterworth can be seen in [vsnet-campaign-data 34] and T. Kato commented about the data that the data seems to indicate the absence of variations greater than 0.1 mag (vsnet-campaign 412). More time-series photometry is needed to clarify the sub-type of this object. SN 2000da (RA = 00h03m06s.52, Dec = -01d54'41".8) This supernova was discovered by the Lick Observatory team (IAUC 7474). H. Yamaoka reported that the recession velocity of UGC 5 (the host galaxy of SN 2000da) is 7271 km/s, from which the expected maximum of typical SN Ia is about 16.6 mag (vsnet-campaign-sn 38). Close monitorings are encouraged. (continuous targets) SY Vol (RA = 08h53m28s.9, Dec = -71d12'29".9) The outburst has faded since July 31 (vsnet-campaign-dn 74). Now it is at quiescent state. BR Lup (RA = 15h35m51s.61, Dec = -40d34'25".4) The superoutburst continues. The current magnitude is about 14.0mag (vsnet-campaign-dn 98). Time-series observations are strongly encouraged. V1008 Her (RA = 18h05m46s.4, Dec = +31d40'18") T. Vanmunster performed an unfiltered CCD photometry on July 30/31 and reported that the resulting light curve is flat, showing no periodic modulations. With his past run, he commented that this outbursting object seems to be an UGSS type dwarf nova (vsnet-campaign 406). The long outburst finally began fading from August 4 (13.7mag by M. Reszelski)(vsnet-campaign-dn 95). DH Aql (RA = 19h26m12s.05, Dec = -10d15'21".4) H. Iwamatsu and T. Kato performed CCD photometry on this SU UMa-type dwarf nova under superoutburst on August 2, and confirmed that the object was still bright (vsnet-campaign-dn 81). From the light curve obtained through August 3 observation at Ouda station by H. Iwamatsu and T. Kato, they revealed that there were fully grown superhumps with the amplitude of 0.30mag (vsnet-campaign-dn 92). They calculated the superhump period with the data on August 3, 4, and 5 to be 0.07991 d (vsnet-campaign-dn 99). It is still in superoutburst and the current magnitude is about 12.7mag. More observations are strongly encouraged. Delta Sco (RA = 16h00m19s.9, Dec = -22d37'17") E. Pollmann reported the equivalent width of H-alpha line on July 30 to be 1.9 and 1.6 A derived from the two spectra (vsnet-campaign-be 21). The object may show slightly fading (vsnet-campaign-be 31). V4641 Sgr (RA = 18h19m21s.6, Dec = -25d24'25") No prominent activity was reported (vsnet-campaign-xray 27,30,31). SN 2000cx (RA = 01h24m46s.15, Dec = +09o30'30".9) This supernova reached the maximum at about 13.1mag around the end of July (vsnet-campaign-sn 36), and then, started fading (vsnet-campaign-sn 39). The current magnitude is about 13.9mag. 1H 1933+510 (RA = 19h34m36s.08, Dec = +51d07'42".2) After this new likely dwarf nova (originally NL type) returned to low-state, another outburst was reported by S. O'Connor at 15.8mag on August 4 (vsnet-campaign 408). T. Vanmunster performed CCD photometry on August 04/05 and reported that the resulting light curve shows some small modulations, but clearly nothing related to superhumps (vsnet-campaign 411). G. Tovmassian and S. Zharikov got the spectrum which looks very similar to Dwarf Novae in outburst (vsnet-campaign 413). Time-series photometry is strongly urged to study this object and the outburst nature. CI Aql (RA = 18h52m03s.6, Dec = -01d28m38.9s) The data observed by S. Kiyota can be seen in [vsnet-campaign-data 25-33]. V803 Cen (RA = 13h23m44s.5, Dec = -41d44'30".1) The striking oscillation is ongoing. A brightening was reported on July 31 (13.6mag by R. Stubbings) (vsnet-campaign-dn 76). On August 1st, R. Stubbings reported the object was dimmer than 13.9mag, and then, showed another brightening on August 2 (vsnet-campaign-dn 82). S. Walker performed CCD photometry on August 1 and 2, and detected possible superhumps with their amplitude of 0.1mag (vsnet-campaign-dn 84, vsnet-campaign 407). A rapid fading from the bright outburst was reported on August 5 ( <14.8 by R. Stubbings)(vsnet-campaign-dn 96). Close monitorings and long-run with CCD are encouraged. BL Lac (RA = 22h02m42s.86, Dec = +42d16'37.6") The activity becomes mild (vsnet-campaign-blazer 50, 51). XTE J1118+480 (RA = 11h18m10s.9, Dec = +48d02'12".9) A dramatic fading from the long outburst was reported by M. Verdenet (14.3mag on July 31), and then, the light curve of Kyoto team confirmed the trend (vsnet-campaign-xray 28,29). The decline rate is about 0.07mag/d, which is faster than previously reported one (vsnet-campaign-xray 29,25,34). V. Simon sent the long-term light curve to M. Uemura and it can be seen in [vsnet-image 13] (vsnet-campaign-xray 33). A. Oksanen and M. Moilanen reported their CCD observation of 14.7mag on August 5, which confirmed the rapid decline (vsnet-campaign-xray 35). It is in rapid decline phase. Time-series observation will reveal the activity during this phase of X-ray nova. V1494 Aql The data observed by L. Cook on JD2451711 - 2451755 can be seen in [vsnet-campaign-nova 73]. V2051 Oph The object, which had faded on July 24, brightened again on July 31 (vsnet-campaign-dn 77). *** Future schedule *** V382 Vel, V1494 Aql, Nova in LMC 2000 campaign (August 7) (August 21) S. Starrfield and his collaborators will be obtaining CHANDRA observations of V382 Vel and V1494 Aql the week beginning August 7, 2000 and they will be obtaining HST/STIS observations of Nova LMC 2000 the week of August 21, 2000. Ground based observations are encouraged. Observers those who are interested in this campaign, should contact with Dr. Starrfield (sumner.starrfield@asu.edu). [vsnet-campaign-nova 71] BL Lac campaign (July 17 - August 11) Massimo Villata, Gino Tosti, and Enrico Massaro organize an optical campaign on BL Lac contemporaneous with the high-energy campaign involving X-ray and TeV observatories such as BeppoSAX, RXTE, STACEE, CAT, HEGRA. Their goal is high-density and high-precision coverage, possibly in two optical bands (B and R). Observers interested in participating to this optical campaign are invited to contact with M. Villata (villata@to.astro.it). [vsnet-campaign 204] NY Ser spectroscopic observations at the Calar Alto Observatory (July 08/09 and 09/10) D. Nogami noticed their schedule of spectroscopic observations of NY Ser and wrote: "Because it is quite important for us to know the state of NY Ser at our observations as accurately as possible, we would ask observers to make a close monitor of this star for ~1 month from now (this article was posted on June 29)." For more information, please see [vsnet-campaign 265], or contact with D. Nogami (daisaku@uni-sw.gwdg.de). [vsnet-campaign 265] V446 Her campaign (throughout this summer) Boris T. Gaensicke organize a campaign on the post nova V446 Her (V~18). Their aim is to obtain a *good* contiguous light curve of V446 Her that covers 2-3 dwarf nova-like outbursts of the system, in order to compare its outburst characteristics to those of ``normal'' dwarf novae. They invite those of you equipped with a CCD camera to obtain a couple of images of V446 Her per night throughout the next three months, say, until the end of September. For more information, please see [vsnet-campaign 325] or contact with Boris T. Gaensicke (boris@uni-sw.gwdg.de). In [vsnet-campaign 368]..... "The V446 Her campaign from July 7 was started (through the end of September). But we have received very few observations since then. Negative observations, for instance, <17.0, are also useful. We strongly encourage observers to contribute to this project. Let's clarify the physics of post novae!" *** General information *** V2051 Oph eclipse ephemeris, see [vsnet-campaign-dn 80] XTE J1118+480 long-term light curves http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-image/msg00013.html (by V. Simon) http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Xray/xtej1118-camp.html (by VSNET collaboration team) (This summary is reproduction free.) Regards, Makoto Uemura