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 | V1082 SGR | 286.8363 | -20.7721 | 286.094048 | -20.85102 | 285.710494 | 1.754645 | 15.88147607 | -12.67535412 | 81.3818 | 56009.1848148148 | 2012-03-23 04:26:08 | 56010.4459375 | 2012-03-24 10:42:09 | 406042010 | 39.4605 | 40 | 39.4605 | 39.4605 | 0 | 39.4605 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 36.0171 | 36.0171 | 108.924 | 2 | PROCESSED | 57605.0088541667 | 2016-08-05 00:12:45 | 56399 | 2013-04-17 00:00:00 | 56023.1564236111 | 2012-04-06 03:45:15 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061217 | V1082 Sgr is a BAT-detected cataclysmic variable with a 20 hr orbital period that exhibits high and low states. The high X-ray luminosity and the presence of the HeII 4686 lines in its optical spectrum have led to the suggestion that this is an intermediate polar (IP). We propose an exploratory 40 ks Suzaku observation with the aim of establishing if it is indeed an IP. If it is, then this system may provide a unique opportunity to study an IP in a low state, which has not been possible with other IPs. | GALACTIC POINT SOURCES | 4 | C | KOJI MUKAI | USA | 6 | AO6 | AN UNUSUAL BAT-DETECTED CATACLYSMIC VARIABLE, V1082 SGR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406042010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '406042010'
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