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 NGC 526A 20.9794 -35.0729 20.408158 -35.333404 3.010528 -40.076485 263.77547728 -79.45131683 257.0195 55578.7592939815 2011-01-17 18:13:23 55580.6404050926 2011-01-19 15:22:11 705044010 72.9346 70 72.9346 72.9346 0 72.9346 2 2 0 2 1 0 0 63.1372 63.1372 162.4977 2 PROCESSED 57600.6980324074 2016-07-31 16:45:10 55961 2012-02-04 00:00:00 55595.4905671296 2011-02-03 11:46:25 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051434 The Compton-thin NELG NGC 526a has large hard X-ray variability and likely an abnormally flat photon index, Gamma near 1.6. We request two observations of 70 ks each, spaced six months apart, to accurately constrain Compton reflection and obtain geometrical constraints on the accreting material to test Seyfert unification schemes, as well as constrain coronal power law parameters. Importantly, we will track long-term spectral variability to constrain the location and nature of the reflecting material. We also will resolve the moderately broad Fe K alpha line, which may indicate the presence of a truncated accretion disk, and thus constrain the amount of reflection off an accretion disk versus that from a torus. EXTRAGALACTIC COMPACT SOURCES 7 C ALEX MARKOWITZ USA 5 AO5 COMPTON REFLECTION AND LONG-TERM SPECTRAL VARIABILITY IN THE SEYFERT AGN NGC 526A XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705044010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705044010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏