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 NGC 4051 180.4686 44.1146 179.828661 44.392934 159.283243 39.862026 150.13143213 70.30340869 109.3717 55184.3459606482 2009-12-19 08:18:11 55186.5140509259 2009-12-21 12:20:14 504062010 89.6305 80 89.6385 89.6465 0 89.6305 3 2 0 2 1 0 0 37.0758 37.0758 187.2819 2 PROCESSED 57549.977337963 2016-06-10 23:27:22 55581 2011-01-20 00:00:00 55209.4570833333 2010-01-13 10:58:12 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040120 The highly ionized absorption lines of OVII and OVII at z = 0 have been unambiguously detected toward the bright AGN NGC 4051 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 and OVIII 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 C TOSHISHIGE HAGIHARA JAP 4 AO4 STUDY OF WARM-HOT GAS TOWARD NGC 4051 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504062010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504062010'

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