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 | ABELL2811-OFF | 10.1781 | -28.7333 | 9.563743 | -29.007637 | 356.740152 | -30.181509 | 358.19144602 | -87.13859798 | 232.6526 | 53702.8821296296 | 2005-11-28 21:10:16 | 53703.731412037 | 2005-11-29 17:33:14 | 800006010 | 33.9494 | 25 | 33.9574 | 33.9654 | 33.9494 | 33.9498 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 30.9056 | 30.9056 | 73.3659 | 1 | PROCESSED | 57528.1125115741 | 2016-05-20 02:42:01 | 54247 | 2007-05-27 00:00:00 | 54038.6719560185 | 2006-10-30 16:07:37 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001025 | We propose to observe the central region of the Sculptor supercluster at z=0.11, in a search for the theoretically predicted Warm/Hot Intergalactic Medium (WHIM). The WHIM has been 'missing' observationally, until recent detection of the X-ray absorption due to the ionized light elements in the background quasar spectra. Still there is no confident detection of the expected soft X-ray emission. This is mainly because that the X-ray brightness is very low, compared to the Galactic diffuse emission in the soft X-ray band and/or the spectral sensitivity of previous experiments are limited. To separate the expected X-ray lines of the WHIM (mainly O VII) from the Galactic emission, we select an unique supercluster at z>0.1. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | TAKAYUKI TAMURA | JAP | 0 | SWG | THE SCULPTOR SUPERCLUSTER: SEARCH FOR THE WARM/HOT INTERGALACTIC MEDIUM | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800006010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '800006010'
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