DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | RX J1712.6-2414 | 258.1492 | -24.2444 | 257.386071 | -24.185404 | 259.195725 | -1.246505 | 359.8664305 | 8.74215246 | 94.4586 | 54889.4875925926 | 2009-02-27 11:42:08 | 54892.2710532407 | 2009-03-02 06:30:19 | 403021010 | 110.4813 | 100 | 110.4893 | 110.4813 | 0 | 110.4893 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 89.4584 | 89.4584 | 240.4418 | 4 | PROCESSED | 57545.7503587963 | 2016-06-06 18:00:31 | 55330 | 2010-05-14 00:00:00 | 54908.5588310185 | 2009-03-18 13:24:43 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030106 | We propose to observe a peculiar Intermediate Polar, RX J1712.6-2414, which has no accretion disk around the white dwarf. This source shows the X-ray modulation only at the beat period and broad Fe-K emission lines in the phase-averaged spectrum. Our goal is to obtain a clear picture about the accretion flow geometry, which can explain the timing and spectral properties, utilizing the fine phase-resolved spectra. Furthermore, we examine the non-thermal emission from the source, since the magnetized white dwarf is a promising candidate of particle acceleration sites. | GALACTIC POINT SOURCES | 4 | B | HIDEYUKI MORI | JAP | 3 | AO3 | ACCRETION FLOW AND EMISSION MECHANISM OF A DISKLESS INTERMEDIATE POLAR, RX J1712.6-2414 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403021010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403021010'
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