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 | 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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