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 | V4641 SGR | 274.8371 | -25.4052 | 274.064433 | -25.426808 | 274.361493 | -2.037678 | 6.77442002 | -4.78571714 | 84.0004 | 56741.9737152778 | 2014-03-25 23:22:09 | 56744.8959722222 | 2014-03-28 21:30:12 | 408002010 | 49.2237 | 100 | 49.2237 | 49.2706 | 0 | 49.2242 | 3 | 3 | 0 | 3 | 1 | 0 | 0 | 89.7439 | 89.7439 | 252.4556 | 1 | PROCESSED | 57614.1632291667 | 2016-08-14 03:55:03 | 57190 | 2015-06-17 00:00:00 | 56821.8685532407 | 2014-06-13 20:50:43 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 080009 | We propose a 100 ksec Suzaku observation of the Galactic microquasar V4641 Sgr in an outburst. V4641 Sgr has many unique charactersitics: 1)giant X-ray outbursts with fast rise and decay times, 2)violent variability in X-ray and optical bands, and 3)remarkable iron-K disk-line profiles in the X-ray spectrum. However, it is hardly understood due to the poor X-ray coverage which results from its short outburst duration and rapid intensity variations. Hence, we collaborate closely with VSNET, MAXI/GSC, Swift/XRT and Swift/BAT team for a rapid trigger. The moderate energy resolution and wideband energy coverage of Suzaku enable us to clarify the radiation mechanisms of V4641 Sgr. This observation is now planned simultaneously with Swift, many radio and optical/NIR observatories. | GALACTIC POINT SOURCES | 4 | A | KAZUTAKA YAMAOKA | JAP | 8 | AO8-TOO | THE LARGEST-EVER CAMPAIGN OF THE GALACTIC MICROQUASAR V4641 SGR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408002010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '408002010'
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