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 NGC5548 214.4979 25.1264 213.930994 25.35658 201.999984 36.406639 31.92993093 70.49400067 281.7605 54317.0262268518 2007-08-05 00:37:46 54318.0211111111 2007-08-06 00:30:24 702042080 38.7757 210 38.7837 38.7917 0 38.7757 1 1 0 1 1 0 0 32.6497 32.6497 85.9519 0 PROCESSED 57539.4187037037 2016-05-31 10:02:56 54714 2008-09-05 00:00:00 54347.3528472222 2007-09-04 08:28:06 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021307 We propose a 2 month Suzaku monitoring program of 7 weekly 30ksec observations of the normal type 1 AGN, NGC5548. NGC5548 is uniquely well studied at all wavelengths, and will vary by a factor of 1.5, or more, at 97% probability. Variations of the Warm Absorber will determine its location in NGC5548, disciminating between models and determining the mass loss rate in the WA wind. This will provide a baseline data point for models of 'cosmological feedback' from AGN to galaxy formation. Simultaneously, the XIS and HXD spectra will study changes or lack thereof in the reflection components (narrow Fe-K, Compton Hump), again delimiting their location and choosing among models. The summed spectrum will determine the high energy continuum break, any broad Fe-K or high ionization edge. EXTRAGALACTIC COMPACT SOURCES 7 A MARTIN ELVIS USA 2 AO2 NGC5548 MONITORING: KEY TO AGN STRUCTURE AND COSMIC FEEDBACK XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702042080/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702042080'

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