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
1 VICINITY_OF_PKS_2155-2 330.1861 -29.9649 329.464287 -30.205624 321.680429 -16.673826 18.22929909 -52.62033555 55.8323 54588.3553356482 2008-05-02 08:31:41 54590.7293865741 2008-05-04 17:30:19 503083010 87.3274 80 87.3274 87.3274 0 87.3274 2 2 0 2 1 0 0 75.8451 75.8451 205.1059 3 PROCESSED 57542.4726736111 2016-06-03 11:20:39 54975 2009-05-24 00:00:00 54608.2608912037 2008-05-22 06:15:41 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030135 The highly ionized absorption lines of OVII, OVIII, and NeIX at z = 0 have been unambiguously detected toward the bright AGN PKS 2155-304 by the high-resolution spectrometers onboard Chandra and XMM-Newton. However, the spatial extent and thus the nature of the absorbing warm-hot gas are yet unknown; it can be from 1 Mpc scale WHIM (Warm-hot intergalactic medium) to a few kpc scale galactic wind. We propose to observe the very vicinity of the AGN to determine the OVII, OVIII and NeIX emission line intensities and the temperature of the warm-hot gas. Joint analysis of absorption and emission lines will unambiguously constrain the spatial extent of the warm-hot gas. GALACTIC DIFFUSE EMISSION 5 A TOSHISHIGE HAGIHARA JAP 3 AO3 STUDY OF WARM-HOT GAS TOWARD PKS 2155-304 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503083010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503083010'

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